text: Eclipses only occur in the eclipse season, when the Sun is close to either the ascending or descending node of the Moon. Each eclipse is separated by one, five or six lunations (synodic months), and the midpoint of each season is separated by 173.3 days, which is the mean time for the Sun to travel from one node to the next. The period is a little less than half a calendar year because the lunar nodes slowly regress. Because 223 synodic months is roughly equal to 239 anomalistic months and 242 draconic months, eclipses with similar geometry recur 223 synodic months (about 6,585.3 days) apart. This period (18 years 11.3 days) is a saros. Because 223 synodic months is not identical to 239 anomalistic months or 242 draconic months, saros cycles do not endlessly repeat. Each cycle begins with the Moon's shadow crossing the earth near the north or south pole, and subsequent events progress toward the other pole until the Moon's shadow misses the earth and the series ends. Saros cycles are numbered; currently, cycles 117 to 156 are active.

text: Eclipses only occur in the

entity_name: Eclipse season

text: eclipse season

text: , when the Sun is close to either the ascending or descending

entity_name: Lunar node

text: node of the Moon

text: . Each eclipse is separated by one, five or six

entity_name: New moon

text: lunation

text: s (

entity_name: Lunar month

text: synodic month

text: s), and the midpoint of each season is separated by 173.3 days, which is the mean time for the Sun to travel from one node to the next. The period is a little less than half a calendar year because the lunar nodes slowly regress. Because 223 synodic months is roughly equal to 239

text: anomalistic month

text: s and 242

text: draconic month

text: s, eclipses with similar geometry recur 223 synodic months (about 6,585.3 days) apart. This period (18 years 11.3 days) is a

entity_name: Saros (astronomy)

text: saros

text: . Because 223 synodic months is not identical to 239 anomalistic months or 242 draconic months, saros cycles do not endlessly repeat. Each cycle begins with the Moon's shadow crossing the earth near the north or south pole, and subsequent events progress toward the other pole until the Moon's shadow misses the earth and the series ends. Saros cycles are numbered; currently, cycles 117 to 156 are active.

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text: People in eastern and southern Serbia believed that ale, in their voracity, attacked the Sun and the Moon. They gradually ate more and more of those celestial bodies, thereby causing an eclipse. During an eclipse, the Sun turned red because it was covered with its own blood as a result of the ale’s bites; when it shone brightly again, that meant it had defeated the ale. The spots on the Moon were seen as scars from the ale’s bites. While ale devoured the Sun or the Moon, many elderly people became depressed and even wept in fear. If ale succeeded in devouring the Sun, the world would end. To prevent that, men shot their guns toward the eclipse or rang bells, and women cast spells incessantly. There was a notion in the Homolje region that, if ale succeeded in devouring the Moon, the Sun would die from sorrow, and darkness would overwhelm the world.

text: People in eastern and southern Serbia believed that ale, in their voracity, attacked the

entity_name: Sun

text: Sun

text: and the

entity_name: Moon

text: Moon

text: . They gradually ate more and more of those celestial bodies, thereby causing an

entity_name: Eclipse

text: eclipse

text: . During an eclipse, the Sun turned red because it was covered with its own blood as a result of the ale’s bites; when it shone brightly again, that meant it had defeated the ale. The spots on the Moon were seen as scars from the ale’s bites. While ale devoured the Sun or the Moon, many elderly people became

entity_name: Depression (mood)

text: depressed

text: and even wept in fear. If ale succeeded in devouring the Sun, the world would end. To prevent that, men shot their guns toward the eclipse or rang bells, and women cast spells incessantly. There was a notion in the Homolje region that, if ale succeeded in devouring the Moon, the Sun would die from sorrow, and darkness would overwhelm the world.

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text: There were 12 solar eclipses observed from 2137 BC to 424 BC. all have a historical basis, because some old historical scriptures provide us details of these solar eclipses. Firstly, in writing sources of ancient China, we found a solar eclipse of 22 October, 2137 BC, but mostly Chinese ancient records shows details about comets, constellations, and fixed stars.

text: There were 12 solar eclipses observed from 2137 BC to 424 BC. all have a historical basis, because some old historical scriptures provide us details of these

entity_name: Solar eclipse

text: solar eclipses

text: . Firstly, in writing sources of

entity_name: History of China

entity_section: Ancient China

text: ancient China

text: , we found a solar eclipse of 22 October, 2137 BC, but mostly Chinese ancient records shows details about

entity_name: Comet

text: comets

entity_name: Constellation

text: constellations

text: , and

entity_name: Fixed stars

text: fixed stars

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answers: NDQ_002327

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answers: Earth that is having daytime

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answers: 2137 BC

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answers: There were 12 solar eclipses observed

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: It is impossible to say

answers: NDQ_002357

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answers: The first quarter phase of the moon

answers: NDQ_002359

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answers: 22 October, 2137 BC

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answers: 424 BC

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answers: one month

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answers: lunar eclipse

text: A partial solar eclipse occurred on June 10, 1964. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on June 10, 1964. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

entity_name: Earth

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: NDQ_002325

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answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

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answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

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answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on June 10, 1964

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: It's impossible to say

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

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answers: the 28th

answers: NDQ_002360

answers: The Sun

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answers: NDQ_002362

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answers: Earth

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answers: NDQ_002366

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answers: 1

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answers: partial solar eclipse

text: The drag from the solar atmosphere may cause the orbit of the Moon to decay. Once the orbit of the Moon closes to a distance of , it will cross the Earth's Roche limit. This means that tidal interaction with the Earth would break apart the Moon, turning it into a ring system. Most of the orbiting ring will then begin to decay, and the debris will impact the Earth. Hence, even if the Earth is not swallowed up by the Sun, the planet may be left moonless. The ablation and vaporization caused by its fall on a decaying trajectory towards the Sun may remove Earth's crust and mantle, then finally destroy it after at most 200 years. Following this event, Earth's sole legacy will be a very slight increase (0.01%) of the solar metallicity.

text: The drag from the solar atmosphere may cause the orbit of the Moon to decay. Once the orbit of the Moon closes to a distance of , it will cross the Earth's

entity_name: Roche limit

text: Roche limit

text: . This means that tidal interaction with the Earth would break apart the Moon, turning it into a ring system. Most of the orbiting ring will then begin to decay, and the debris will impact the Earth. Hence, even if the Earth is not swallowed up by the Sun, the planet may be left moonless. The

entity_name: Ablation

text: ablation

text: and

entity_name: Vaporization

text: vaporization

text: caused by its fall on a decaying trajectory towards the Sun may remove Earth's

entity_name: Crust (geology)

text: crust

text: and mantle, then finally destroy it after at most 200 years. Following this event, Earth's sole legacy will be a very slight increase (0.01%) of the solar

entity_name: Metallicity

text: metallicity

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answers: The Earth's Roche limit

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answers: It will cross the Earth's Roche limit

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answers: at most 200 years

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answers: 200 years

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text: In this system the revolution of the earth around fire "at the centre" or "the fire of the hearth" (Central Fire) was not yearly but daily, while the moon's revolution was monthly, and the sun's yearly. It was the earth's speedy travel past the slower moving sun that resulted in the appearance on earth of the sun rising and setting.  Further from the Central Fire, the planets' revolution was slower still and the outermost "sky" (i.e. stars) probably fixed.

text: In this system the revolution of the earth around fire "at the centre" or "the fire of the hearth" (Central Fire) was not yearly but daily, while the moon's revolution was monthly, and the sun's yearly. It was the earth's speedy travel past the slower moving sun that resulted in the appearance on earth of the sun rising and setting.  Further from the Central Fire, the planets' revolution was slower still and the outermost "sky" (i.e. stars) probably fixed.

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answers: NDQ_002326

answers: monthly

answers: NDQ_002327

answers: sun rising and setting

answers: NDQ_002328

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answers: NDQ_002329

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answers: NDQ_002330

answers: the sun

answers: NDQ_002331

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answers: NDQ_002334

answers: the outermost "sky

answers: NDQ_002335

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answers: lunar eclipse

answers: NDQ_002345

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answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: sun rising and setting

answers: NDQ_002351

answers: monthly

answers: NDQ_002352

answers: penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The appearance on earth of the sun rising and setting

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: monthly

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

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answers: the moon's

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

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answers: the sun rising and setting

answers: NDQ_002363

answers: planets'

answers: NDQ_002364

answers: earth's speedy travel past the slower moving sun

answers: NDQ_002365

answers: daily

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: monthly

answers: NDQ_002368

answers: monthly

text: A partial lunar eclipse took place on June 4, 2012. It was the first of two lunar eclipses occurring in 2012, the second eclipse set to happen on November 28. The moon was about one third covered by the Earth's northern umbral shadow at maximum eclipse. The portion of the moon inside the umbral shadow was illuminated by sunlight refracted through the Earth's atmosphere, thus much dimmer, and having a reddish hue.

text: A partial

entity_name: Lunar eclipse

text: lunar eclipse

text: took place on June 4, 2012. It was the first of two lunar eclipses occurring in 2012, the second eclipse set to happen on November 28. The moon was about one third covered by the Earth's northern umbral shadow at maximum eclipse. The portion of the moon inside the umbral shadow was illuminated by sunlight refracted through the Earth's atmosphere, thus much dimmer, and having a reddish hue.

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answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: northern umbral shadow

answers: NDQ_002325

answers: partial lunar eclipse

answers: NDQ_002326

answers: partial

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: partial lunar eclipse

answers: NDQ_002329

answers: one third

answers: NDQ_002330

answers: umbral shadow

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: maximum eclipse

answers: NDQ_002334

answers: umbral shadow

answers: NDQ_002335

answers: maximum eclipse

answers: NDQ_002343

answers: at maximum eclipse

answers: NDQ_002345

answers: It was the first of two lunar eclipses occurring in 2012

answers: NDQ_002348

answers: The moon was about one third covered

answers: NDQ_002350

answers: It was the first of two lunar eclipses

answers: NDQ_002351

answers: It was the first of two lunar eclipses

answers: NDQ_002352

answers: umbral

answers: NDQ_002353

answers: The moon was about one third covered

answers: NDQ_002354

answers: solar eclipses are rare

answers: NDQ_002355

answers: The moon was about one third covered

answers: NDQ_002356

answers: November 28

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answers: NDQ_002358

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answers: Earth's northern umbral shadow

answers: NDQ_002361

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answers: partial lunar eclipse

text: The appearance, or phase, of the Moon is due to its motion with respect to the Sun.  It varies in a period of  time called a lunation, also called synodic month; its duration is about 2 days longer than an anomalistic month.  The age is the number of days since new moon.

text: The appearance, or

entity_name: Lunar phase

text: phase

text: , of the Moon is due to its motion with respect to the Sun.  It varies in a period of  time called a lunation, also called

text: synodic month

text: ; its duration is about 2 days longer than an anomalistic month.  The age is the number of days since

text: new moon

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answers: the Moon

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answers: new moon

answers: NDQ_002326

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answers: NDQ_002327

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answers: NDQ_002328

answers: appearance

answers: NDQ_002329

answers: 2 days longer than an anomalistic month

answers: NDQ_002330

answers: the Sun

answers: NDQ_002331

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answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002343

answers: duration

answers: NDQ_002345

answers: The appearance, or phase, of the Moon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

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answers: NDQ_002352

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answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The appearance, or phase, of the Moon

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: lunation

answers: NDQ_002357

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answers: NDQ_002358

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answers: NDQ_002359

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answers: NDQ_002360

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answers: NDQ_002361

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answers: NDQ_002363

answers: motion with respect to the Sun

answers: NDQ_002364

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answers: NDQ_002365

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answers: NDQ_002366

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answers: new moon

text: For terrestrial observations, "Sun–object–Earth" is often nearly the same thing as "Sun–object–observer", since the difference depends on the parallax, which in the case of observations of the Moon can be as much as 1°, or two full Moon diameters. With the development of space travel, as well as in hypothetical observations from other points in space, the notion of phase angle became independent of Sun and Earth.

text: For terrestrial observations, "Sun–object–Earth" is often nearly the same thing as "Sun–object–observer", since the difference depends on the

entity_name: Parallax

text: parallax

text: , which in the case of observations of the

text: Moon

text: can be as much as 1°, or two full Moon diameters. With the development of

entity_name: Spaceflight

text: space travel

text: , as well as in hypothetical observations from other points in space, the notion of phase angle became independent of Sun and Earth.

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answers: as much as 1°

answers: NDQ_002327

answers: terrestrial observations

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answers: parallax

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answers: NDQ_002353

answers: The difference depends on the parallax

answers: NDQ_002354

answers: Solar eclipses are rare events

answers: NDQ_002355

answers: Partial lunar eclipse

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answers: It can be as much as 1°

answers: NDQ_002357

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answers: Parallax

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answers: NDQ_002361

answers: Parallax

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answers: Sun–object–Earth

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answers: NDQ_002366

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answers: NDQ_002367

answers: two full Moon diameters

answers: NDQ_002368

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text: There were two other eclipses that year. The first was a partial lunar eclipse, during which the shadow of the earth can be seen on the moon, and another solar eclipse that took place on December 3 over South America. The other solar eclipse however was an annular eclipse which occurs when the moon has a smaller apparent diameter and therefore never fully obscures the sun.

text: There were two other eclipses that year. The first was a partial lunar eclipse, during which the shadow of the earth can be seen on the moon, and another solar eclipse that took place on

entity_name: Solar eclipse of December 3, 1918

text: December 3 over South America

text: . The other solar eclipse however was an annular eclipse which occurs when the moon has a smaller apparent diameter and therefore never fully obscures the sun.

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answers: NDQ_002359

answers: December 3

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answers: NDQ_002361

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answers: NDQ_002365

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answers: NDQ_002366

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answers: NDQ_002368

answers: partial lunar eclipse

text: A partial solar eclipse occurred on November 10, 1920. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on November 10, 1920. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: partial

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answers: NDQ_002325

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answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: part of the Moon

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: It does not say.

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on November 10, 1920

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: on November 10, 1920

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: A crescent phase

answers: NDQ_002359

answers: November

answers: NDQ_002360

answers: The Sun

answers: NDQ_002361

answers: totally or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: one month

answers: NDQ_002368

answers: partial solar eclipse

text: An annular solar eclipse will occur on June 21, 2039. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.This eclipse will start only a few hours after the northern solstice and most of the path will go across areas with midnight sun.  For mainland Norway and Sweden it will be the first central solar eclipse since June 1954.

text: An annular

text: solar eclipse

text: will occur on June 21, 2039. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

entity_name: Angular diameter

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

entity_name: Annulus (mathematics)

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.This eclipse will start only a few hours after the

entity_name: June solstice

text: northern solstice

text: and most of the path will go across areas with

entity_name: Midnight sun

text: midnight sun

text: .  For mainland

entity_name: Norway

text: Norway

text: and

entity_name: Sweden

text: Sweden

text: it will be the first central solar eclipse since

entity_name: Solar eclipse of June 30, 1954

text: June 1954

method: UNH-qee

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answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: annular solar eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: an annular solar eclipse

answers: NDQ_002330

answers: the Sun

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: It will be the first central solar eclipse since June 1954

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly obscuring

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: For mainland Norway and Sweden it will be the first central solar eclipse since June 1954

answers: NDQ_002355

answers: An annular solar eclipse

answers: NDQ_002356

answers: June 21, 2039

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: when the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: a few hours

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: crescent

text: Photographing the Moon's phase every day for a month, starting in the evening after sunset, and repeating approximately fifty minutes later each successive day, ending in the morning before sunrise, would create a composite image like the example calendar from May 8, 2005, to June 6, 2005 here in the left. There is no picture on May 20 since a picture would be taken before midnight on May 19, and after midnight on May 21. Similarly, on a calendar listing moon rise or set times, some days will appear to be skipped. When the Moon rises just before midnight one night it will rise just after midnight the next (so too with setting). The 'skipped day' is just a feature of the moon's eastward movement in relation to the sun, which at most latitudes causes the moon to rise later each day. The moon has a predictable orbit every month.

text: Photographing the Moon's phase every day for a month, starting in the evening after sunset, and repeating approximately fifty minutes later each successive day, ending in the morning before sunrise, would create a composite image like the example calendar from May 8, 2005, to June 6, 2005 here in the left. There is no picture on May 20 since a picture would be taken before midnight on May 19, and after midnight on May 21. Similarly, on a calendar listing moon rise or set times, some days will appear to be skipped. When the Moon rises just before midnight one night it will rise just after midnight the next (so too with setting). The 'skipped day' is just a feature of the moon's eastward movement in relation to the sun, which at most latitudes causes the moon to rise later each day. The moon has a predictable orbit every month.

method: Bert-DRMMTKS

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answers: 4

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answers: 0

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answers: 2

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answers: 0

answers: NDQ_002323

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answers: NDQ_002324

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answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 4

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 0

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 4

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: setting

answers: NDQ_002324

answers: the evening after sunset

answers: NDQ_002325

answers: setting

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: sunset

answers: NDQ_002328

answers: The'skipped day'

answers: NDQ_002329

answers: phase every day for a month

answers: NDQ_002330

answers: the evening after sunset

answers: NDQ_002331

answers: sunset

answers: NDQ_002332

answers: Moon's phase

answers: NDQ_002334

answers: the sun

answers: NDQ_002335

answers: setting

answers: NDQ_002343

answers: approximately fifty minutes later each successive day

answers: NDQ_002345

answers: When the Moon rises just before midnight one night it will rise just after midnight the next (so too with setting)

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: When the Moon rises just before midnight one night it will rise just after midnight the next

answers: NDQ_002352

answers: When the Moon rises just before midnight one night it will rise just after midnight the next

answers: NDQ_002353

answers: Shadows are partly blocked in the umbra part.

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: The moon has a predictable orbit every month

answers: NDQ_002357

answers: When the Moon rises just before midnight one night it will rise just after midnight the next

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: When the Moon rises just before midnight one night it will rise just after midnight the next

answers: NDQ_002360

answers: Moon's eastward movement

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: eastward movement in relation to the sun

answers: NDQ_002363

answers: sun

answers: NDQ_002364

answers: the sun is obscured by clouds

answers: NDQ_002365

answers: a month

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: approximately fifty minutes

answers: NDQ_002368

answers: rise

text: Section D: MOON contains detailed positional information on the Moon including phases, mean elements of the orbit and rotation, lengths of mean months, ecliptic and equatorial coordinates, librations, and physical ephemerides.

text: Section D: MOON contains detailed positional information on the Moon including phases, mean elements of the orbit and rotation, lengths of mean months, ecliptic and equatorial coordinates, librations, and physical ephemerides.

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answers: NDQ_002348

answers: 5

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 5

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answers: 4

answers: NDQ_002367

answers: 0

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answers: NDQ_002323

answers: phases

answers: NDQ_002324

answers: equator and ecliptic

answers: NDQ_002325

answers: phases

answers: NDQ_002326

answers: Moon

answers: NDQ_002327

answers: orbit

answers: NDQ_002328

answers: phases

answers: NDQ_002329

answers: months

answers: NDQ_002330

answers: equatorial

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: phases

answers: NDQ_002334

answers: ecliptic

answers: NDQ_002335

answers: phases

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: MOON

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Daytime

answers: NDQ_002351

answers: months

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Moon

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: months

answers: NDQ_002357

answers: equator

answers: NDQ_002358

answers: Quarter phase

answers: NDQ_002359

answers: months

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: physical ephemerides

answers: NDQ_002363

answers: ecliptic

answers: NDQ_002364

answers: ecliptic

answers: NDQ_002365

answers: months

answers: NDQ_002366

answers: months

answers: NDQ_002367

answers: months

answers: NDQ_002368

answers: phases

text: A synodic month is longer than a sidereal month because the Earth-Moon system is orbiting the Sun in the same direction as the Moon is orbiting the Earth.   The Sun moves eastward with respect to the stars (as does the Moon) and it takes about 2.2 days longer for the Moon to return to the same apparent position with respect to the Sun.

text: A synodic month is longer than a sidereal month because the Earth-Moon system is orbiting the Sun in the same direction as the Moon is orbiting the Earth.   The Sun moves eastward with respect to the stars (as does the Moon) and it takes about 2.2 days longer for the Moon to return to the same apparent position with respect to the Sun.

method: UvABottomUpChangeOrder

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text: The main characters of the series are Jab get the back to the moon and Skills Vertigo, Montana, Emo, Jummpa, Panzer, Bommba, Juanito, Mole, Bubble, Missile, Tornado, Sharky and Quaka. They can’t live without each other but they also can’t help being selfish and playing pranks on each other constantly. The different phases of the moon change their personality for better or worse. These three friends don’t speak but they can communicate through noises, gestures and actions.

text: The main characters of the series are Jab get the back to the moon and Skills Vertigo, Montana, Emo, Jummpa, Panzer, Bommba, Juanito, Mole, Bubble, Missile, Tornado, Sharky and Quaka. They can’t live without each other but they also can’t help being selfish and playing pranks on each other constantly. The different phases of the moon change their personality for better or worse. These three friends don’t speak but they can communicate through noises, gestures and actions.

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text: Also many moons, even those that do not orbit the Sun directly, often exhibit features in common with true planets. There are 19 moons in the Solar System that have achieved hydrostatic equilibrium and would be considered planets if only the physical parameters are considered.  Both Jupiter's moon Ganymede and Saturn's moon Titan are larger than Mercury, and Titan even has a substantial atmosphere, thicker than the Earth's. Moons such as Io and Triton demonstrate obvious and ongoing geological activity, and Ganymede has a magnetic field. Just as stars in orbit around other stars are still referred to as stars, some astronomers argue that objects in orbit around planets that share all their characteristics could also be called planets. Indeed, Mike Brown makes just such a claim in his dissection of the issue, saying:

text: Also many moons, even those that do not orbit the Sun directly, often exhibit features in common with true planets. There are 19 moons in the Solar System that have achieved hydrostatic equilibrium and would be considered planets if only the physical parameters are considered.  Both Jupiter's moon

entity_name: Ganymede (moon)

text: Ganymede

text: and Saturn's moon

entity_name: Titan (moon)

text: Titan

text: are larger than Mercury, and Titan even has a substantial atmosphere, thicker than the Earth's. Moons such as

entity_name: Io (moon)

text: Io

text: and

text: Triton

text: demonstrate obvious and ongoing geological activity, and Ganymede has a

text: magnetic field

text: . Just as

text: star

text: s in orbit around other stars are still referred to as stars, some astronomers argue that objects in orbit around planets that share all their characteristics could also be called planets. Indeed, Mike Brown makes just such a claim in his dissection of the issue, saying:

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answers: Earth's

answers: NDQ_002324

answers: Moon and Earth's shadow

answers: NDQ_002325

answers: Ganymede

answers: NDQ_002326

answers: Earth-like

answers: NDQ_002327

answers: Earth's shadow

answers: NDQ_002328

answers: a magnetic field

answers: NDQ_002329

answers: smaller than the Earth's

answers: NDQ_002330

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answers: NDQ_002331

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answers: planets

answers: NDQ_002334

answers: Earth's shadow

answers: NDQ_002335

answers: Earth's

answers: NDQ_002343

answers: Moons in orbit around other planets are still referred to as stars

answers: NDQ_002345

answers: Moons in orbit around other planets are still referred to as stars

answers: NDQ_002348

answers: Moons in orbit around other planets are still referred to as stars

answers: NDQ_002350

answers: Earth's atmosphere is thicker than Titan's.

answers: NDQ_002351

answers: Ganymede has a full moon every 29.5 days.

answers: NDQ_002352

answers: Ganymede has a magnetic field

answers: NDQ_002353

answers: Earth's shadow is only partly blocked in the umbra.

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Moons in orbit around other planets are still referred to as stars

answers: NDQ_002356

answers: Moons in orbit around other planets that share all their characteristics

answers: NDQ_002357

answers: Moons in orbit around other planets are still referred to as stars

answers: NDQ_002358

answers: Moons in orbit around planets that share all their characteristics could also be called planets.

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month.

answers: NDQ_002360

answers: Moons in orbit around other planets are still referred to as stars

answers: NDQ_002361

answers: Moons in orbit around planets are still referred to as stars

answers: NDQ_002362

answers: Earth has a magnetic field

answers: NDQ_002363

answers: Earth's orbit around the Sun.

answers: NDQ_002364

answers: Earth's atmosphere is thinner than the Sun's

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answers: a few minutes

answers: NDQ_002366

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answers: one month

answers: NDQ_002368

answers: nebula

text: An eclipse can only occur when the Moon is close to the plane of the orbit of the Earth, i.e. when its ecliptic latitude is small.  This happens when the Moon is near one of the two nodes of its orbit on the ecliptic at the time of the syzygy.  Of course, to produce an eclipse, the Sun must also be near a node at that time: the same node for a solar eclipse, or the opposite node for a lunar eclipse.

text: An eclipse can only occur when the Moon is close to the plane of the orbit of the Earth, i.e. when its

text: ecliptic latitude

text: is small.  This happens when the Moon is near one of the two

text: node

text: s of its orbit on the ecliptic at the time of the

text: syzygy

text: .  Of course, to produce an eclipse, the Sun must also be near a node at that time: the same node for a solar eclipse, or the opposite node for a lunar eclipse.

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answers: lunar eclipse

answers: NDQ_002324

answers: the same node

answers: NDQ_002325

answers: lunar eclipse

answers: NDQ_002326

answers: right side

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: An eclipse

answers: NDQ_002329

answers: its ecliptic latitude is small

answers: NDQ_002330

answers: the ecliptic

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: lunar

answers: NDQ_002334

answers: the Earth

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: It can only occur when the Moon is close to the plane of the orbit of the Earth

answers: NDQ_002345

answers: An eclipse can only occur when the Moon is close to the plane of the orbit of the Earth

answers: NDQ_002348

answers: The Sun must also be near a node

answers: NDQ_002350

answers: The same node

answers: NDQ_002351

answers: Moon is near one of the two nodes

answers: NDQ_002352

answers: the opposite node for a lunar eclipse

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: An eclipse can only occur when the Moon is close to the plane of the orbit of the Earth

answers: NDQ_002355

answers: Moon is near one of the two nodes of its orbit

answers: NDQ_002356

answers: It can only occur when the Moon is close to the plane of the orbit of the Earth

answers: NDQ_002357

answers: opposite node

answers: NDQ_002358

answers: The first quarter phase of the moon

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: the opposite node

answers: NDQ_002361

answers: the same node

answers: NDQ_002362

answers: to produce an eclipse

answers: NDQ_002363

answers: orbit of the Earth

answers: NDQ_002364

answers: the Sun must also be near a node at that time

answers: NDQ_002365

answers: the same node

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: One of her experiments to study a lunar eclipse included placing a round table in a garden pavilion, acting as a globe; she hung a crystal lamp on a cord from the ceiling beams, representing the sun. Then on one side of the table she had a round mirror as the moon. She moved these three objects as if they were the sun, earth, and moon according to astronomical principles. Her findings and observations were very accurate and recorded in her article, "The Explanation of a Solar Eclipse."

text: One of her experiments to study a lunar eclipse included placing a round table in a garden pavilion, acting as a globe; she hung a crystal lamp on a cord from the ceiling beams, representing the sun. Then on one side of the table she had a round mirror as the moon. She moved these three objects as if they were the sun, earth, and moon according to astronomical principles. Her findings and observations were very accurate and recorded in her article, "The Explanation of a Solar Eclipse."

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answers: NDQ_002327

answers: lunar eclipse

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answers: lunar eclipse

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answers: a lunar eclipse

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: lunar

answers: NDQ_002334

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answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: Lunar eclipse

answers: NDQ_002345

answers: hung a crystal lamp

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answers: total lunar eclipse

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answers: solar eclipse

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: penumbra

answers: NDQ_002353

answers: the umbra

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answers: Solar eclipses are rare events

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answers: Earths umbra

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answers: a Solar Eclipse

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answers: quarter moon

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answers: lunar eclipse

text: A total solar eclipse took place on 13–15 November 2012 (UTC). Because it crossed the International Date Line it began in local time on November 14 west of the  date line over northern Australia, and ended in local time on November 13 east of the date line near the west coast of South America. Its greatest magnitude was 1.0500, occurring only 12 hours before perigee, with greatest eclipse totality lasting just over four minutes. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

text: A total

text: solar eclipse

text: took place on 13–15 November 2012 (

text: UTC

text: ). Because it crossed the

text: International Date Line

text: it began in

text: local time

text: on November 14 west of the  date line over northern

text: Australia

text: , and ended in local time on November 13 east of the date line near the west coast of

text: South America

text: . Its greatest

text: magnitude

text: was 1.0500, occurring only 12 hours before

text: perigee

text: , with greatest eclipse totality lasting just over four minutes. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's

text: apparent diameter

text: is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

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answers: perigee

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answers: total solar eclipse

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answers: partial solar eclipse

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: total solar eclipse

answers: NDQ_002329

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answers: totality

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answers: partial solar eclipse

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answers: totality

answers: NDQ_002335

answers: total solar eclipse

answers: NDQ_002343

answers: totality lasting just over four minutes

answers: NDQ_002345

answers: The Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness

answers: NDQ_002348

answers: The Moon's apparent diameter is larger than the Sun's

answers: NDQ_002350

answers: total solar eclipse

answers: NDQ_002351

answers: Its greatest magnitude was 1.0500

answers: NDQ_002352

answers: The Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight

answers: NDQ_002353

answers: total solar eclipse

answers: NDQ_002354

answers: Totality occurs in a narrow path across Earth's surface

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: Its greatest magnitude was 1.0500

answers: NDQ_002357

answers: total solar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

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answers: NDQ_002360

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002361

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answers: total solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: when the Moon's apparent diameter is larger than the Sun's

answers: NDQ_002365

answers: four minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 12 hours

answers: NDQ_002368

answers: perigee

text: The moon's orbit isn't in the same plane as the Earth's orbit around the sun, but crosses it in two places. The moon crosses the ecliptic plane twice a month, once when it goes up above the plane, and again 15 or so days later when it goes back down below the ecliptic. These two locations are the ascending and descending lunar nodes. Solar and lunar eclipses will occur only when the moon is positioned near one of these nodes, because at other times the moon is either too high or too low for an eclipse to be noticed from earth. Some astronomical clocks keep track of the position of the lunar nodes with a long pointer that crosses the dial. This so-called dragon hand makes one complete rotation around the ecliptic dial every 19 years. When the dragon hand and the new moon coincide, the moon is on the same plane as the earth and sun, and so there is every chance that an eclipse will be visible from somewhere on earth.

text: The moon's orbit isn't in the same plane as the Earth's orbit around the sun, but crosses it in two places. The moon crosses the ecliptic plane twice a month, once when it goes up above the plane, and again 15 or so days later when it goes back down below the ecliptic. These two locations are the ascending and descending

text: lunar nodes

text: . Solar and lunar eclipses will occur only when the moon is positioned near one of these nodes, because at other times the moon is either too high or too low for an eclipse to be noticed from earth. Some astronomical clocks keep track of the position of the lunar nodes with a long pointer that crosses the dial. This so-called dragon hand makes one complete rotation around the ecliptic dial every 19 years. When the dragon hand and the new moon coincide, the moon is on the same plane as the earth and sun, and so there is every chance that an eclipse will be visible from somewhere on earth.

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answers: new moon

answers: NDQ_002324

answers: rising and descending lunar nodes

answers: NDQ_002325

answers: new moon

answers: NDQ_002326

answers: eclipse

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: eclipses

answers: NDQ_002329

answers: 15 or so days later

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: new moon

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: new moon

answers: NDQ_002343

answers: When the dragon hand and the new moon coincide

answers: NDQ_002345

answers: The moon crosses the ecliptic plane twice a month

answers: NDQ_002348

answers: when the moon is positioned near one of these nodes

answers: NDQ_002350

answers: At other times the moon is either too high or too low

answers: NDQ_002351

answers: The moon crosses the ecliptic plane

answers: NDQ_002352

answers: The moon crosses the ecliptic plane

answers: NDQ_002353

answers: The umbra part of a shadow

answers: NDQ_002354

answers: when the moon is positioned near one of these nodes

answers: NDQ_002355

answers: The moon crosses the ecliptic plane twice a month

answers: NDQ_002356

answers: The moon crosses the ecliptic plane twice a month

answers: NDQ_002357

answers: When the dragon hand and the new moon coincide

answers: NDQ_002358

answers: When the dragon hand and the new moon coincide

answers: NDQ_002359

answers: 15 or so days later

answers: NDQ_002360

answers: at other times the moon is either too high or too low

answers: NDQ_002361

answers: at other times the moon is either too high or too low

answers: NDQ_002362

answers: solar and lunar eclipses

answers: NDQ_002363

answers: plane

answers: NDQ_002364

answers: the moon is on the same plane as the earth and sun

answers: NDQ_002365

answers: 15 or so days

answers: NDQ_002366

answers: 19 years

answers: NDQ_002367

answers: 15 or so days

answers: NDQ_002368

answers: new moon

text: The gravitational attraction between Earth and the Moon causes tides on Earth. The same effect on the Moon has led to its tidal locking: its rotation period is the same as the time it takes to orbit Earth. As a result, it always presents the same face to the planet. As the Moon orbits Earth, different parts of its face are illuminated by the Sun, leading to the lunar phases; the dark part of the face is separated from the light part by the solar terminator.

text: The gravitational attraction between Earth and the Moon causes

text: tide

text: s on Earth. The same effect on the Moon has led to its

text: tidal locking

text: : its rotation period is the same as the time it takes to orbit Earth. As a result, it always presents the same face to the planet. As the Moon orbits Earth, different parts of its face are illuminated by the Sun, leading to the

text: lunar phase

text: s; the dark part of the face is separated from the light part by the

text: solar terminator

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answers: NDQ_002361

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answers: NDQ_002362

answers: 4

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answers: NDQ_002364

answers: 5

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: solar terminator

answers: NDQ_002324

answers: dark part of the face

answers: NDQ_002325

answers: solar terminator

answers: NDQ_002326

answers: the solar terminator

answers: NDQ_002327

answers: tides

answers: NDQ_002328

answers: tides

answers: NDQ_002329

answers: lunar phases

answers: NDQ_002330

answers: the solar terminator

answers: NDQ_002331

answers: tides

answers: NDQ_002332

answers: solar terminator

answers: NDQ_002334

answers: the solar terminator

answers: NDQ_002335

answers: solar terminator

answers: NDQ_002343

answers: The dark part of the face is separated from the light part by the solar terminator

answers: NDQ_002345

answers: different parts of its face are illuminated by the Sun

answers: NDQ_002348

answers: different parts of its face are illuminated by the Sun

answers: NDQ_002350

answers: different parts of its face are illuminated by the Sun

answers: NDQ_002351

answers: the time it takes to orbit Earth

answers: NDQ_002352

answers: the solar terminator

answers: NDQ_002353

answers: the dark part of the face

answers: NDQ_002354

answers: different parts of its face are illuminated by the Sun

answers: NDQ_002355

answers: As the Moon orbits Earth, different parts of its face are illuminated by the Sun

answers: NDQ_002356

answers: It always presents the same face to the planet

answers: NDQ_002357

answers: The dark part of the face is separated from the light part by the solar terminator

answers: NDQ_002358

answers: As the Moon orbits Earth

answers: NDQ_002359

answers: lunar phases

answers: NDQ_002360

answers: different parts of its face are illuminated

answers: NDQ_002361

answers: different parts of its face are illuminated

answers: NDQ_002362

answers: as the Moon orbits Earth

answers: NDQ_002363

answers: solar terminator

answers: NDQ_002364

answers: the Sun is illuminated by the Moon

answers: NDQ_002365

answers: time

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: lunar phases

answers: NDQ_002368

answers: lunar phases

text: At the beginning of day three, the spacecraft was about  away from the Earth. The velocity of the craft steadily decreased, as it had not yet reached the lunar sphere of gravitational influence. The early part of day three was largely housekeeping, spacecraft maintenance and exchanging status reports with Mission Control in Houston. The crew performed the Apollo light flash experiment, or ALFMED, to investigate "light flashes" that were seen by the astronauts when the spacecraft was dark, regardless of whether or not their eyes were open, on Apollo lunar flights. This was thought to be caused by the penetration of the eye by cosmic ray particles. During the second half of the day, Young and Duke again entered the Lunar Module to power it up and check its systems, and perform housekeeping tasks in preparation for lunar landing. The systems were found to be functioning as expected. Following this, the crew donned their space suits and rehearsed procedures that would be used on landing day. Just before the end of flight day three at 59 hours, 19 minutes, 45 seconds after liftoff, while  from the Earth and  from the Moon, the spacecraft's velocity began increasing as it accelerated towards the Moon after entering the lunar sphere of influence.

text: At the beginning of day three, the spacecraft was about  away from the Earth. The velocity of the craft steadily decreased, as it had not yet reached the lunar sphere of gravitational influence. The early part of day three was largely housekeeping, spacecraft maintenance and exchanging status reports with Mission Control in Houston. The crew performed the Apollo light flash experiment, or ALFMED, to investigate "light flashes" that were seen by the astronauts when the spacecraft was dark, regardless of whether or not their eyes were open, on Apollo lunar flights. This was thought to be caused by the penetration of the

text: eye

text: by

text: cosmic ray

text: particles. During the second half of the day, Young and Duke again entered the Lunar Module to power it up and check its systems, and perform housekeeping tasks in preparation for lunar landing. The systems were found to be functioning as expected. Following this, the crew donned their space suits and rehearsed procedures that would be used on landing day. Just before the end of flight day three at 59 hours, 19 minutes, 45 seconds after liftoff, while  from the Earth and  from the Moon, the spacecraft's velocity began increasing as it accelerated towards the Moon after entering the lunar sphere of influence.

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answers: NDQ_002323

answers: lunar

answers: NDQ_002324

answers: Earth and from the Moon

answers: NDQ_002325

answers: lunar sphere

answers: NDQ_002326

answers: ALFMED

answers: NDQ_002327

answers: lunar sphere of influence

answers: NDQ_002328

answers: light flashes

answers: NDQ_002329

answers: the lunar sphere

answers: NDQ_002330

answers: sphere of influence

answers: NDQ_002331

answers: day three

answers: NDQ_002332

answers: lunar sphere

answers: NDQ_002334

answers: sphere of influence

answers: NDQ_002335

answers: Earth

answers: NDQ_002343

answers: It accelerated towards the Moon

answers: NDQ_002345

answers: The crew performed the Apollo light flash experiment, or ALFMED

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The crew performed the Apollo light flash experiment

answers: NDQ_002351

answers: 59 hours, 19 minutes

answers: NDQ_002352

answers: The lunar sphere of influence

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The crew performed the Apollo light flash experiment

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: It accelerated towards the Moon

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: gravitational influence

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: when the Earth is dark

answers: NDQ_002365

answers: 19 minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 19 minutes

answers: NDQ_002368

answers: dark

text: Zhang applied his extensive knowledge of mechanics and gears in several of his inventions. He invented the world's first water-powered armillary sphere to assist astronomical observation; improved the inflow water clock by adding another tank; and invented the world's first seismoscope, which discerned the cardinal direction of an earthquake  away. He improved previous Chinese calculations for pi. In addition to documenting about 2,500 stars in his extensive star catalog, Zhang also posited theories about the Moon and its relationship to the Sun: specifically, he discussed the Moon's sphericity, its illumination by reflected sunlight on one side and the hidden nature of the other, and the nature of solar and lunar eclipses. His fu (rhapsody) and shi poetry were renowned in his time and studied and analyzed by later Chinese writers. Zhang received many posthumous honors for his scholarship and ingenuity; some modern scholars have compared his work in astronomy to that of the Greco-Roman Ptolemy (AD 86–161).

text: Zhang applied his extensive knowledge of mechanics and gears in several of his inventions. He invented the world's first

text: water-powered

text: armillary sphere

text: to assist astronomical observation; improved the inflow

text: water clock

text: by adding another tank; and invented the world's first seismoscope, which discerned the

text: cardinal direction

text: of an

text: earthquake

text: away. He improved previous Chinese calculations for

text: pi

text: . In addition to documenting about 2,500 stars in his extensive

text: star catalog

text: , Zhang also posited theories about the

text: Moon

text: and its relationship to the

text: Sun

text: : specifically, he discussed the Moon's sphericity, its illumination by reflected sunlight on one side and the

text: hidden nature

text: of the other, and the nature of

text: solar

text: and

text: lunar

text: eclipse

text: s. His

text: fu

text: (rhapsody) and

text: shi

text: poetry were renowned in his time and studied and analyzed by later Chinese writers. Zhang received many posthumous honors for his scholarship and ingenuity; some modern scholars have compared his work in astronomy to that of the Greco-Roman

text: Ptolemy

text: (AD 86–161).

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text: A separate category of solar eclipses is that of the Sun being occluded by a body other than the Earth's moon, as can be observed at points in space away from the Earth's surface. Two examples are when the crew of Apollo 12 observed the Earth eclipse the Sun in 1969 and when the Cassini probe observed Saturn eclipsing the Sun in 2006.

text: A separate category of solar eclipses is that of the Sun being occluded by a body other than the Earth's moon, as can be observed at points in space away from the Earth's surface. Two examples are when the crew of

text: Apollo 12

text: observed the

text: Earth eclipse the Sun

text: in 1969 and when the

text: Cassini

text: probe

text: observed

text: Saturn eclipsing the Sun

text: in 2006.

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answers: Lunar eclipses generally last between 5-10 minutes.

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text: In 1918, Butler's association with Carnegie led to him being invited to witness and record the 1918 Solar eclipse that was observed from Baker City in Oregon. The expedition was organised by the U.S. Naval Observatory and included Samuel Alfred Mitchell as its expert on eclipses. Butler noted later that he used a system of taking notes of the colours using skills he had learnt for transient effects. Usually a sitting for a portrait took two hours but an eclipse would take just over 112 seconds. It has been noted that he had painted Carnegie thirteen times and like the eclipse he could never keep still to allow Butler to make considered notes. His revived interest in physics led to his 1923 book of Painter and Space which coincided with his second visit to a solar eclipse. He also created pictures of planets that were as seen from one of their moons. His last known eclipse visit was in 1932.

text: In 1918, Butler's association with Carnegie led to him being invited to witness and record the

text: 1918 Solar eclipse

text: that was observed from

text: Baker City

text: in

text: Oregon

text: . The expedition was organised by the

text: U.S. Naval Observatory

text: and included

text: Samuel Alfred Mitchell

text: as its expert on eclipses. Butler noted later that he used a system of taking notes of the colours using skills he had learnt for transient effects. Usually a sitting for a portrait took two hours but an eclipse would take just over 112 seconds. It has been noted that he had painted Carnegie thirteen times and like the eclipse he could never keep still to allow Butler to make considered notes. His revived interest in physics led to his 1923 book of Painter and Space which coincided with his second visit to a solar eclipse. He also created pictures of planets that were as seen from one of their moons. His last known eclipse visit was in 1932.

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answers: 112 seconds

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answers: Solar eclipse would take just over 112 seconds

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text: A partial solar eclipse will occur on March 29, 2025. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: will occur on March 29, 2025. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

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answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: March 29, 2025

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: March 29, 2025

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

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answers: NDQ_002360

answers: Moon passes between Earth and the Sun

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answers: Moon passes between Earth and the Sun

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answers: total or partly

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answers: partial

text: This is a list of solar eclipses in the 20th century BC. During the period 2000 to 1901 BC there were 239 solar eclipses of which 84 were partial, 71 were annular (one non-central), 62 were total, and 22 were hybrids. The greatest number of eclipses in one year was four, occurring in 10 different years: 1998 BC, 1983 BC, 1980 BC, 1958 BC, 1940 BC, 1926 BC, 1922 BC, 1918 BC, 1911 BC, and 1904 BC. One month, March 1958 BC, had two eclipses.

text: This is a list of

text: solar eclipse

text: s in the

text: 20th century BC

text: . During the period 2000 to 1901 BC there were 239 solar eclipses of which 84 were partial, 71 were annular (one

text: non-central

text: ), 62 were total, and 22 were hybrids. The greatest number of eclipses in one year was four, occurring in 10 different years: 1998 BC, 1983 BC, 1980 BC, 1958 BC, 1940 BC, 1926 BC, 1922 BC, 1918 BC, 1911 BC, and 1904 BC. One month, March 1958 BC, had two eclipses.

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answers: NDQ_002331

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answers: NDQ_002332

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answers: NDQ_002335

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answers: NDQ_002343

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answers: NDQ_002345

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answers: NDQ_002351

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answers: NDQ_002352

answers: annular

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answers: There were 239 solar eclipses

answers: NDQ_002355

answers: partial

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answers: March 1958 BC

answers: NDQ_002357

answers: solar eclipses

answers: NDQ_002358

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text: A related problem is that of centrifugal forces for the Earth-Moon-Sun system, where three rotations appear: the daily rotation of the Earth about its axis, the lunar-month rotation of the Earth-Moon system about their center of mass, and the annual revolution of the Earth-Moon system about the Sun. These three motions influence the tides.

text: A related problem is that of centrifugal forces for the Earth-Moon-Sun system, where three rotations appear: the daily rotation of the Earth about its axis, the lunar-month rotation of the Earth-Moon system about their center of mass, and the annual revolution of the Earth-Moon system about the Sun. These three motions influence the

text: tides

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answers: NDQ_002331

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text: However, if two celestial bodies attain the same declination at the time of a conjunction in right ascension (or the same ecliptic latitude at a conjunction in ecliptic longitude), the one that is closer to the Earth will pass in front of the other. In such a case, a syzygy takes place. If one object moves into the shadow of another, the event is an eclipse. For example, if the Moon passes into the shadow of Earth and disappears from view, this event is called a lunar eclipse. If the visible disk of the nearer object is considerably smaller than that of the farther object, the event is called a transit. When Mercury passes in front of the Sun, it is a transit of Mercury, and when Venus passes in front of the Sun, it is a transit of Venus. When the nearer object appears larger than the farther one, it will completely obscure its smaller companion; this is called an occultation. An example of an occultation is when the Moon passes between Earth and the Sun, causing the Sun to disappear either entirely or partially. This phenomenon is commonly known as a solar eclipse. Occultations in which the larger body is neither the Sun nor the Moon are very rare. More frequent, however, is an occultation of a planet by the Moon. Several such events are visible every year from various places on Earth.

text: However, if two celestial bodies attain the same

text: declination

text: at the time of a conjunction in

text: right ascension

text: (or the same ecliptic latitude at a conjunction in ecliptic longitude), the one that is closer to the Earth will pass in front of the other. In such a case, a

text: syzygy

text: takes place. If one object moves into the shadow of another, the event is an

text: eclipse

text: . For example, if the Moon passes into the shadow of Earth and disappears from view, this event is called a

text: lunar eclipse

text: . If the visible disk of the nearer object is considerably smaller than that of the farther object, the event is called a

text: transit

text: . When Mercury passes in front of the Sun, it is a

text: transit of Mercury

text: , and when Venus passes in front of the Sun, it is a

text: transit of Venus

text: . When the nearer object appears larger than the farther one, it will completely obscure its smaller companion; this is called an

text: occultation

text: . An example of an occultation is when the Moon passes between Earth and the Sun, causing the Sun to disappear either entirely or partially. This phenomenon is commonly known as a

text: solar eclipse

text: . Occultations in which the larger body is neither the Sun nor the Moon are very rare. More frequent, however, is an occultation of a planet by the

text: Moon

text: . Several such events are visible every year from various places on Earth.

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answers: NDQ_002335

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answers: Moon passes into the shadow of Earth

answers: NDQ_002345

answers: When the Moon passes between Earth and the Sun, causing the Sun to disappear either entirely or partially

answers: NDQ_002348

answers: Moon passes into the shadow of Earth and disappears from view

answers: NDQ_002350

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answers: NDQ_002351

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answers: Moon passes into the shadow of Earth

answers: NDQ_002353

answers: When the nearer object appears larger than the farther one

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answers: Occultations in which the larger body is neither the Sun nor the Moon are very rare

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text: A straight line connecting the pericenter and apocenter is the line of apsides. This is the major axis of the ellipse, its greatest diameter.  For a two-body system the center of mass of the system lies on this line at one of the two foci of the ellipse. When one body is sufficiently larger than the other it may be taken to be at this focus.  However whether or not this is the case, both bodies are in similar elliptical orbits each having one focus at the system's center of mass, with their respective lines of apsides being of length inversely proportional to their masses.  Historically, in geocentric systems, apsides were measured from the center of the Earth. However, in the case of the Moon, the center of mass of the Earth–Moon system, or Earth–Moon barycenter, as the common focus of both the Moon's and Earth's orbits about each other, is about 74% of the way from Earth's center to its surface.

text: A straight line connecting the pericenter and apocenter is the line of apsides. This is the major axis of the

text: ellipse

text: , its greatest diameter.  For a two-body system the

text: center of mass

text: of the system lies on this line at one of the two

text: foci

text: of the ellipse. When one body is sufficiently larger than the other it may be taken to be at this focus.  However whether or not this is the case, both bodies are in

text: similar

text: elliptical orbits each having one focus at the system's center of mass, with their respective lines of apsides being of length inversely proportional to their masses.  Historically, in

text: geocentric systems

text: , apsides were measured from the center of the Earth. However, in the case of the Moon, the center of mass of the Earth–Moon system, or

text: Earth–Moon barycenter

text: , as the common focus of both the Moon's and Earth's orbits about each other, is about 74% of the way from Earth's center to its surface.

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answers: 0

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answers: 0

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answers: 0

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 3

answers: NDQ_002356

answers: 0

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answers: 0

answers: NDQ_002358

answers: 0

answers: NDQ_002359

answers: 3

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

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answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 0

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: apogee

answers: NDQ_002324

answers: pericenter and apocenter

answers: NDQ_002325

answers: apocenter

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: Earth–Moon system

answers: NDQ_002328

answers: Earth–Moon barycenter

answers: NDQ_002329

answers: 74%

answers: NDQ_002330

answers: apsides

answers: NDQ_002331

answers: apsides

answers: NDQ_002332

answers: Moon barycenter

answers: NDQ_002334

answers: apsides

answers: NDQ_002335

answers: apollo

answers: NDQ_002343

answers: Earth–Moon system

answers: NDQ_002345

answers: When one body is sufficiently larger than the other it may be taken to be at this focus

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth–Moon system

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: apsides

answers: NDQ_002353

answers: umbra

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: about 74%

answers: NDQ_002357

answers: apocenter

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: Moon's and Earth's orbits about each other

answers: NDQ_002363

answers: ellipse

answers: NDQ_002364

answers: one body is sufficiently larger than the other

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth–Moon system

answers: NDQ_002367

answers: about 74%

answers: NDQ_002368

answers: apollo

text: Aryabhata described a geocentric model of the solar system, in which theSun and Moon are each carried by epicycles. They in turn revolve aroundthe Earth. In this model, which is also found in the Paitāmahasiddhānta (c. CE 425), the motions of the planets are each governed by two epicycles, a smaller manda (slow) and a larger śīghra (fast). The order of the planets in terms of distance from earth is taken as: the Moon, Mercury, Venus, the Sun, Mars, Jupiter, Saturn, and the asterisms."

text: Aryabhata described a

text: geocentric

text: model of the solar system, in which theSun and Moon are each carried by

text: epicycle

text: s. They in turn revolve aroundthe Earth. In this model, which is also found in the Paitāmahasiddhānta (c. CE 425), the motions of the planets are each governed by two epicycles, a smaller manda (slow) and a larger śīghra (fast). The order of the planets in terms of distance from earth is taken as: the

text: Moon

text: Mercury

text: Venus

text: , the

text: Sun

text: Mars

text: Jupiter

text: Saturn

text: , and the

text: asterisms

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answers: 0

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answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

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answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 4

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

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answers: 0

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 3

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answers: 3

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

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answers: 0

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answers: 0

answers: NDQ_002366

answers: 0

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: Earth

answers: NDQ_002324

answers: manda (slow) and a larger  ghra (fast)

answers: NDQ_002325

answers: manda

answers: NDQ_002326

answers: manda

answers: NDQ_002327

answers: They in turn revolve around the Earth

answers: NDQ_002328

answers: asterisms

answers: NDQ_002329

answers: smaller manda

answers: NDQ_002330

answers: the Sun

answers: NDQ_002331

answers: asterisms

answers: NDQ_002332

answers: ghra

answers: NDQ_002334

answers: Sun

answers: NDQ_002335

answers: manda

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: Earth

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The Sun and Moon are each carried by epicycles

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: Moon

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: Moon

answers: NDQ_002359

answers: Moon

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: Moon are each carried by epicycles

answers: NDQ_002362

answers: They in turn revolve around the Earth

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: Earth

answers: NDQ_002365

answers: Earth

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 425

answers: NDQ_002368

answers: manda

text: Fred Espanak of NASA lists 50 phases of the moon within year 0, showing that it is a full year, not an instant in time. Jean Meeus gives the following explanation:

text: Fred Espanak of

text: NASA

text: lists 50 phases of the moon within year 0, showing that it is a full year, not an instant in time. Jean Meeus gives the following explanation:

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answers: 0

answers: tqa2:L_0056/T_0550/028c40b7b41e40ba09d2487346bb8d7f

answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: Lunar eclipses last between 5-10 minutes.

answers: NDQ_002345

answers: Solar eclipses are caused by a partial eclipse of the Sun.

answers: NDQ_002348

answers: A total lunar eclipse occurs when the moon is completely covered by the sun's light.

answers: NDQ_002350

answers: A solar eclipse is seen on all of the Earth that is having daytime.

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: The cone-shaped part of the moons shadow is the penumbra.

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow

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answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Partially occludes the Earths umbra.

answers: NDQ_002356

answers: Lunar eclipses occur once every month.

answers: NDQ_002357

answers: Full moon phase occurs when the moon is on the opposite side of Earth from the sun

answers: NDQ_002358

answers: The first quarter phase of the moon is the first stage of the lunar cycle.

answers: NDQ_002359

answers: If the new moon occurs on the 1st of the month, the full moon will occur on the 28th of the month

answers: NDQ_002360

answers: Lunar eclipses occur when the Moon passes directly overhead of the Sun.

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answers: When a solar eclipse occurs, the moon cannot be seen from Earth.

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answers: a full moon passes directly overhead

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answers: 365 days

answers: NDQ_002367

answers: a full year

answers: NDQ_002368

answers: phase 1

text: There were 240 lunar eclipse events between -199 and -100 (200 BCE to 101 BCE)

text: There were 240 lunar eclipse events between -199 and -100 (200 BCE to 101 BCE)

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answers: total lunar eclipse

answers: NDQ_002350

answers: A solar eclipse is seen on all of the Earth

answers: NDQ_002351

answers: 29.5 days

answers: NDQ_002352

answers: lunar eclipse

answers: NDQ_002353

answers: Umbra

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answers: -100

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answers: 200 BCE

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answers: quarter moon

answers: NDQ_002368

answers: eclipse

text: Saturn's rings would be seen from an angle of only 0.019° and be almost invisible, but their shadow on Saturn's disk would be clearly distinguishable. Like our own Moon from Earth, Saturn itself would show regular phases. From Enceladus, the Sun would have a diameter of only 3.5 minutes of arc, one-ninth that of the Moon as seen from Earth.

text: Saturn's rings would be seen from an angle of only 0.019° and be almost invisible, but their shadow on Saturn's disk would be clearly distinguishable. Like our own Moon from Earth, Saturn itself would show regular

text: phase

text: s. From Enceladus, the Sun would have a diameter of only 3.5 minutes of arc, one-ninth that of the Moon as seen from Earth.

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answers: NDQ_002334

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answers: NDQ_002345

answers: their shadow on Saturn's disk

answers: NDQ_002348

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answers: NDQ_002350

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answers: NDQ_002352

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answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

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answers: NDQ_002355

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answers: NDQ_002356

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answers: NDQ_002357

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answers: NDQ_002358

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answers: NDQ_002360

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answers: NDQ_002363

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answers: NDQ_002364

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answers: NDQ_002365

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answers: NDQ_002366

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answers: NDQ_002368

answers: phases

text: It is a narrow path for the moon to pass within the penumbra and outside the umbra. It can happen on the Earth's northern or southern penumbral edges. In addition, the size of the penumbra is sometimes too small where the moon enters it to contain the moon. The width of the Earth's penumbra is determined by the sun's angular diameter at the time of the eclipse, and the moon's angular diameter is larger than the sun over part of its elliptical orbit, depending on whether the eclipse occurs at its nearest (perigee) or farthest point (apogee) in its orbit around the earth.  The majority of the time, the size of the moon and the size of the Earth's penumbra where the moon crosses it mean that most eclipses will not be total penumbral in nature.

text: It is a narrow path for the moon to pass within the penumbra and outside the umbra. It can happen on the Earth's northern or southern penumbral edges. In addition, the size of the penumbra is sometimes too small where the moon enters it to contain the moon. The width of the Earth's penumbra is determined by the sun's

text: angular diameter

text: at the time of the eclipse, and the moon's angular diameter is larger than the sun over part of its

text: elliptical orbit

text: , depending on whether the eclipse occurs at its nearest (

text: perigee

text: ) or farthest point (apogee) in its orbit around the earth.  The majority of the time, the size of the moon and the size of the Earth's penumbra where the moon crosses it mean that most eclipses will not be total penumbral in nature.

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answers: NDQ_002327

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answers: NDQ_002328

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answers: NDQ_002329

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answers: NDQ_002330

answers: 4

answers: NDQ_002331

answers: 4

answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002343

answers: 4

answers: NDQ_002345

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answers: NDQ_002348

answers: 5

answers: NDQ_002350

answers: 0

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answers: 4

answers: NDQ_002352

answers: 4

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 3

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 3

answers: NDQ_002360

answers: 4

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: umbra

answers: NDQ_002324

answers: umbra

answers: NDQ_002325

answers: penumbral

answers: NDQ_002326

answers: penumbra

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: eclipse

answers: NDQ_002329

answers: most eclipses will not be total penumbral in nature

answers: NDQ_002330

answers: penumbra

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: penumbra

answers: NDQ_002334

answers: umbra

answers: NDQ_002335

answers: umbra

answers: NDQ_002343

answers: It is a narrow path for the moon to pass within the penumbra and outside the umbra

answers: NDQ_002345

answers: penumbra and outside the umbra

answers: NDQ_002348

answers: The width of the Earth's penumbra

answers: NDQ_002350

answers: The majority of the time

answers: NDQ_002351

answers: It is a narrow path for the moon

answers: NDQ_002352

answers: umbra

answers: NDQ_002353

answers: penumbra

answers: NDQ_002354

answers: most eclipses will not be total penumbral in nature

answers: NDQ_002355

answers: It is a narrow path

answers: NDQ_002356

answers: most eclipses will not be total penumbral in nature

answers: NDQ_002357

answers: Earth's northern or southern penumbral edges

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The width of the Earth's penumbra

answers: NDQ_002360

answers: The width of the Earth's penumbra

answers: NDQ_002361

answers: penumbra and outside the umbra

answers: NDQ_002362

answers: the size of the moon and the size of the Earth's penumbra where the moon crosses it

answers: NDQ_002363

answers: Earth's penumbra

answers: NDQ_002364

answers: the sun's angular diameter is larger than the moon

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth's

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: penumbra

text: The word is often used in reference to the Sun, Earth, and either the Moon or a planet, where the latter is in conjunction or opposition. Solar and lunar eclipses occur at times of syzygy, as do transits and occultations. The term is often applied when the Sun and Moon are in conjunction (new moon) or opposition (full moon).

text: The word is often used in reference to the

text: Sun

text: Earth

text: , and either the

text: Moon

text: or a

text: planet

text: , where the latter is in

text: conjunction

text: or

text: opposition

text: Solar

text: and

text: lunar

text: eclipse

text: s occur at times of syzygy, as do

text: transits

text: and

text: occultation

text: s. The term is often applied when the Sun and Moon are in conjunction (

text: new moon

text: ) or opposition (

text: full moon

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answers: NDQ_002323

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answers: 4

answers: NDQ_002327

answers: 4

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answers: 4

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 4

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 4

answers: NDQ_002343

answers: 4

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 5

answers: NDQ_002350

answers: 0

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answers: 4

answers: NDQ_002352

answers: 0

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answers: 0

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

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answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 3

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answers: 4

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answers: 4

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

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answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 4

answers: NDQ_002323

answers: opposition

answers: NDQ_002324

answers: Moon or a planet

answers: NDQ_002325

answers: opposition

answers: NDQ_002326

answers: opposition

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: opposition

answers: NDQ_002329

answers: opposition

answers: NDQ_002330

answers: full moon

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: full moon

answers: NDQ_002334

answers: opposition

answers: NDQ_002335

answers: opposition

answers: NDQ_002343

answers: When the Sun and Moon are in conjunction (new moon) or opposition (full moon)

answers: NDQ_002345

answers: the Sun, Earth, and either the Moon or a planet

answers: NDQ_002348

answers: full moon

answers: NDQ_002350

answers: The term is often applied when the Sun and Moon are in conjunction

answers: NDQ_002351

answers: opposition

answers: NDQ_002352

answers: The term is often applied when the Sun and Moon are in conjunction

answers: NDQ_002353

answers: Eclipses occur at times of syzygy

answers: NDQ_002354

answers: Solar and lunar eclipses occur

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: full moon

answers: NDQ_002357

answers: opposition

answers: NDQ_002358

answers: full moon

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: opposition

answers: NDQ_002361

answers: opposition

answers: NDQ_002362

answers: Solar and lunar eclipses

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Sun and Moon are in opposition

answers: NDQ_002365

answers: full moon

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: full moon

answers: NDQ_002368

answers: new moon

text: In the future, a near feudal colony has risen up around the industrialisation of the Moon, and though technology keeps the deadly natural environment at bay, the four basic essentials of life—air, water, carbon and data—come at a price. Tiny "chibs" placed in the eye to meter usage of these Four Elementals serve as a constant reminder of this. Everyone also has a "familiar": a personalized, holographic avatar that hovers over one shoulder and serves as an interface with the Moon's network, other familiars and even one's physical surroundings. The Moon is controlled by five families, dubbed the Five Dragons: the Australian Mackenzies dominate mineral extraction, the Asamoahs of Ghana control a vast underground agricultural industry, the Russian Vorontsovs run the transportation systems, the Suns of China are masters of technology and the upstart Brazilian Cortas mine helium-3 to power Earth's fusion reactors. These families, and all citizens of the Moon, operate under contracts granted by the Lunar Development Corporation (LDC), the Moon's governing body. The Mackenzies and the Cortas—the oldest and the newest lunar families, respectively—are bitter rivals, and as the novel begins, the long-simmering animosity between them seems reignited.

text: In the future, a near feudal colony has risen up around the industrialisation of the Moon, and though technology keeps the deadly natural environment at bay, the four basic essentials of life—air, water, carbon and data—come at a price. Tiny "chibs" placed in the eye to meter usage of these Four Elementals serve as a constant reminder of this. Everyone also has a "familiar": a personalized, holographic

text: avatar

text: that hovers over one shoulder and serves as an interface with the Moon's network, other familiars and even one's physical surroundings. The Moon is controlled by five families, dubbed the Five Dragons: the Australian Mackenzies dominate mineral extraction, the Asamoahs of Ghana control a vast underground agricultural industry, the Russian Vorontsovs run the transportation systems, the Suns of China are masters of technology and the upstart Brazilian Cortas mine

text: to power Earth's

text: fusion reactor

text: s. These families, and all citizens of the Moon, operate under contracts granted by the Lunar Development Corporation (LDC), the Moon's governing body. The Mackenzies and the Cortas—the oldest and the newest lunar families, respectively—are bitter rivals, and as the novel begins, the long-simmering animosity between them seems reignited.

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text: The Moon and Earth orbit a common barycenter every 27.32 days relative to the background stars. When combined with the Earth–Moon system's common orbit around the Sun, the period of the synodic month, from new moon to new moon, is 29.53 days. Viewed from the celestial north pole, the motion of Earth, the Moon, and their axial rotations are all counterclockwise. Viewed from a vantage point above the north poles of both the Sun and Earth, Earth orbits in a counterclockwise direction about the Sun. The orbital and axial planes are not precisely aligned: Earth's axis is tilted some 23.44 degrees from the perpendicular to the Earth–Sun plane (the ecliptic), and the Earth–Moon plane is tilted up to ±5.1 degrees against the Earth–Sun plane. Without this tilt, there would be an eclipse every two weeks, alternating between lunar eclipses and solar eclipses.

text: The Moon and Earth orbit a common

text: barycenter

text: every 27.32 days relative to the background stars. When combined with the Earth–Moon system's common orbit around the Sun, the period of the

text: synodic month

text: , from new moon to new moon, is 29.53 days. Viewed from the

text: celestial north pole

text: , the motion of Earth, the Moon, and their axial rotations are all

text: counterclockwise

text: . Viewed from a vantage point above the north poles of both the Sun and Earth, Earth orbits in a counterclockwise direction about the Sun. The orbital and axial planes are not precisely aligned: Earth's

text: axis is tilted

text: some 23.44 degrees from the perpendicular to the Earth–Sun plane (the

text: ecliptic

text: ), and the Earth–Moon plane is tilted up to ±5.1 degrees against the Earth–Sun plane. Without this tilt, there would be an eclipse every two weeks, alternating between

text: lunar eclipse

text: s and

text: solar eclipse

text: s.

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text: While tidal forces from the primary are common on satellites, most satellite systems remain stable.  Perturbation between satellites can occur, particularly in the early formation, as the gravity of satellites affect each other, and can result in ejection from the system or collisions between satellites or with the primary.  Simulations show that such interactions cause the orbits of the inner moons of the Uranus system to be chaotic and possibly unstable.  Some of Io's active can be explained by perturbation from Europa's gravity as their orbits resonate.Perturbation has been suggested as a reason that Neptune does not follow the 10,000:1 ratio of mass between the parent planet and collective moons as seen in all other known giant planets. One theory of the Earth-Moon system suggest that a second companion which formed at the same time as the Moon, was perturbed by the Moon early in the system's history, causing it to impact with the Moon.

text: While tidal forces from the primary are common on satellites, most satellite systems remain stable.

text: Perturbation

text: between satellites can occur, particularly in the early formation, as the gravity of satellites affect each other, and can result in ejection from the system or collisions between satellites or with the primary.  Simulations show that such interactions cause the orbits of the inner moons of the Uranus system to be chaotic and possibly unstable.  Some of Io's active can be explained by perturbation from Europa's gravity as their orbits resonate.Perturbation has been suggested as a reason that Neptune does not follow the 10,000:1 ratio of mass between the parent planet and collective moons as seen in all other known giant planets. One theory of the Earth-Moon system suggest that a second companion which formed at the same time as the Moon, was perturbed by the Moon early in the system's history, causing it to impact with the Moon.

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answers: Moon

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answers: Umbra

answers: NDQ_002354

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answers: NDQ_002356

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answers: a few minutes

answers: NDQ_002366

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answers: quarter moon

answers: NDQ_002368

answers: active

text: The saros, a period of 6585.3211 days (14 common years + 4 leap years + 11.321 days, or 13 common years + 5 leap years + 10.321 days), is useful for predicting the times at which nearly identical eclipses will occur. Three periodicities related to lunar orbit, the synodic month, the draconic month, and the anomalistic month coincide almost perfectly each saros cycle. For an eclipse to occur, either the Moon must be located between the Earth and Sun (for a solar eclipse) or the Earth must be located between the Sun and Moon (for a lunar eclipse). This can happen only when the Moon is new or full, respectively, and repeat occurrences of these lunar phases result from solar and lunar orbits producing the Moon's synodic period of 29.53059 days. During most full and new moons, however, the shadow of the Earth or Moon falls to the north or south of the other body. Eclipses occur when the three bodies form a nearly straight line.  Because the plane of the lunar orbit is inclined to that of the earth, this condition occurs only when a full or new Moon is near or in the ecliptic plane, that is when the moon is at one of the two nodes (the ascending or descending node). The period of time for two successive lunar passes through the ecliptic plane (returning to the same node) is termed the draconic month, a 27.21222 day period.  The three-dimensional geometry of an eclipse, when the new or full moon is near one of the nodes, occurs every 5 or 6 months when the Sun is in conjunction or opposition to the Moon and coincidentally also near a node of the Moon's orbit at that time, or twice per eclipse year. Two Saros eclipses have the same appearance and duration due to the distance between the Earth and Moon being nearly the same for each event because the Saros eclipse cycle is also an integer of the anomalistic month, the period of the eccentricity of lunar orbit, 27.5545 days.

text: The saros, a period of 6585.3211 days (14 common years + 4 leap years + 11.321 days, or 13 common years + 5 leap years + 10.321 days), is useful for predicting the times at which nearly identical eclipses will occur. Three periodicities related to lunar orbit, the

text: synodic month

text: , the

text: draconic month

text: , and the

text: anomalistic month

text: coincide almost perfectly each saros cycle. For an eclipse to occur, either the Moon must be located between the Earth and Sun (for a

text: solar eclipse

text: ) or the Earth must be located between the Sun and Moon (for a

text: lunar eclipse

text: ). This can happen only when the Moon is

text: new

text: or

text: full

text: , respectively, and repeat occurrences of these

text: lunar phase

text: s result from solar and lunar orbits producing the Moon's synodic period of 29.53059 days. During most full and new moons, however, the shadow of the Earth or Moon falls to the north or south of the other body. Eclipses occur when the three bodies form a nearly straight line.  Because the plane of the lunar orbit is inclined to that of the earth, this condition occurs only when a full or new Moon is near or in the

text: ecliptic plane

text: , that is when the moon is at one of the two

text: nodes

text: (the ascending or descending node). The period of time for two successive lunar passes through the ecliptic plane (returning to the same node) is termed the draconic month, a 27.21222 day period.  The three-dimensional geometry of an eclipse, when the new or full moon is near one of the nodes, occurs every 5 or 6 months when the Sun is in conjunction or opposition to the Moon and coincidentally also near a node of the Moon's orbit at that time, or twice per

text: eclipse year

text: . Two Saros eclipses have the same appearance and duration due to the distance between the Earth and Moon being nearly the same for each event because the Saros eclipse cycle is also an integer of the anomalistic month, the period of the eccentricity of lunar orbit, 27.5545 days.

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answers: the ecliptic plane

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answers: lunar eclipse

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answers: Earth or Moon falls to the north or south

answers: NDQ_002335

answers: new

answers: NDQ_002343

answers: Earth must be located between the Sun and Moon

answers: NDQ_002345

answers: For an eclipse to occur, either the Moon must be located between the Earth and Sun

answers: NDQ_002348

answers: Earth must be located between the Sun and Moon

answers: NDQ_002350

answers: For an eclipse to occur, the Moon must be located between the Earth and Sun

answers: NDQ_002351

answers: Moon's synodic period of 29.53059 days

answers: NDQ_002352

answers: The three-dimensional geometry of an eclipse

answers: NDQ_002353

answers: the shadow of the Earth or Moon

answers: NDQ_002354

answers: It can happen only when the Moon is new or full

answers: NDQ_002355

answers: full or new Moon is near or in the ecliptic plane

answers: NDQ_002356

answers: The three-dimensional geometry of an eclipse

answers: NDQ_002357

answers: opposition

answers: NDQ_002358

answers: full

answers: NDQ_002359

answers: The synodic month

answers: NDQ_002360

answers: Earth must be located between the Sun and Moon

answers: NDQ_002361

answers: the Moon must be located between the Earth and Sun

answers: NDQ_002362

answers: Eclipses

answers: NDQ_002363

answers: plane

answers: NDQ_002364

answers: the Sun is in conjunction or opposition to the Moon

answers: NDQ_002365

answers: 11.321 days

answers: NDQ_002366

answers: saros

answers: NDQ_002367

answers: 29.53059 days

answers: NDQ_002368

answers: new

text: An annular solar eclipse will occur on June 22, 2085. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on June 22, 2085. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: June 22, 2085

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: on June 22, 2085

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: The Moon passes between Earth and the Sun

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: June 22, 2085

answers: NDQ_002367

answers: 2085

answers: NDQ_002368

answers: crescent

text: An eclipse involving the Sun, Earth, and Moon can occur only when they are nearly in a straight line, allowing one to be hidden behind another, viewed from the third. Because the orbital plane of the Moon is tilted with respect to the orbital plane of the Earth (the ecliptic), eclipses can occur only when the Moon is close to the intersection of these two planes (the nodes). The Sun, Earth and nodes are aligned twice a year (during an eclipse season), and eclipses can occur during a period of about two months around these times. There can be from four to seven eclipses in a calendar year, which repeat according to various eclipse cycles, such as a saros.

text: An eclipse involving the Sun, Earth, and Moon can occur only when they are nearly in a straight line, allowing one to be hidden behind another, viewed from the third. Because the

text: orbital plane of the Moon

text: is tilted with respect to the orbital plane of the Earth (the

text: ecliptic

text: ), eclipses can occur only when the Moon is close to the intersection of these two planes (the

text: node

text: s). The Sun, Earth and nodes are aligned twice a year (during an

text: eclipse season

text: ), and eclipses can occur during a period of about two months around these times. There can be from four to seven eclipses in a calendar year, which repeat according to various

text: eclipse cycle

text: s, such as a

text: saros

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answers: eclipse

answers: NDQ_002324

answers: the nodes

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: An eclipse

answers: NDQ_002329

answers: about two months

answers: NDQ_002330

answers: the nodes

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: the nodes

answers: NDQ_002335

answers: eclipse

answers: NDQ_002343

answers: It can last between 5-10 minutes.

answers: NDQ_002345

answers: Because the orbital plane of the Moon is tilted with respect to the orbital plane of the Earth

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: An eclipse involving the Sun, Earth, and Moon

answers: NDQ_002351

answers: about two months

answers: NDQ_002352

answers: the ecliptic

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: There can be from four to seven eclipses in a calendar year

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: about two months

answers: NDQ_002357

answers: The Sun, Earth and nodes are aligned twice a year

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: two months around these times

answers: NDQ_002360

answers: Moon is tilted with respect to the orbital plane of the Earth

answers: NDQ_002361

answers: The Moon is tilted with respect to the orbital plane of the Earth

answers: NDQ_002362

answers: An eclipse

answers: NDQ_002363

answers: orbital plane

answers: NDQ_002364

answers: they are nearly in a straight line, allowing one to be hidden behind another

answers: NDQ_002365

answers: two months

answers: NDQ_002366

answers: calendar year

answers: NDQ_002367

answers: two months

answers: NDQ_002368

answers: crescent

text: In the climax of the story, several of Earth's heroes were possessed by Eclipso and transported to the moon during an eclipse. He then absorbed these heroes into his own body, gaining their mass and also their inherent powers. Gordon led a group of heroes armed with solar weapons to the moon in an attempt to defeat Eclipso once and for all. The absorbed heroes were freed in the end, but only after Will Payton destroyed Eclipso's moon base by detonating his own solar-powered body. Eclipso's diamond shards remained on Earth.

text: In the climax of the story, several of Earth's heroes were possessed by Eclipso and transported to the moon during an eclipse. He then absorbed these heroes into his own body, gaining their mass and also their inherent powers. Gordon led a group of heroes armed with solar weapons to the moon in an attempt to defeat Eclipso once and for all. The absorbed heroes were freed in the end, but only after

text: Will Payton

text: destroyed Eclipso's moon base by detonating his own solar-powered body. Eclipso's diamond shards remained on Earth.

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answers: NDQ_002323

answers: eclipse

answers: NDQ_002324

answers: moon

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: an eclipse

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: an eclipse

answers: NDQ_002329

answers: an eclipse

answers: NDQ_002330

answers: Earth's heroes

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: an eclipse

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: eclipse

answers: NDQ_002343

answers: It generally lasts between 5-10 minutes

answers: NDQ_002345

answers: an eclipse

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: an eclipse

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Solar eclipses

answers: NDQ_002355

answers: Partially

answers: NDQ_002356

answers: It does not say.

answers: NDQ_002357

answers: an eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: an eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: during an eclipse

answers: NDQ_002363

answers: moon

answers: NDQ_002364

answers: Earth's

answers: NDQ_002365

answers: Earth's

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: one

answers: NDQ_002368

answers: eclipse

text: It appears that Johannes Werner inspired by Amerigo Vespucci's letter written in 1502 where he wrote: "...I maintain that I learned [my longitude] ... by the eclipses and conjunctions of the Moon with the planets; and I have lost many nights of sleep in reconciling my calculations with the precepts of those sages who have devised the manuals and written of the movements, conjunctions, aspects, and eclipses of the two luminaries and of the wandering stars, such as the wise King Don Alfonso in his Tables, Johannes Regiomontanus in his Almanac, and Blanchinus, and the Rabbi Zacuto in his almanac, which is perpetual; and these were composed in different meridians: King Don Alfonso's book in the meridian of Toledo, and Johannes Regiomontanus's in that of Ferrara, and the other two in that of Salamanca."2 The best "clock" to use for reference, is the stars. In the roughly 27.3 solar days of a lunar orbit, the Moon moves a full 360 degrees around the sky, returning to its old position among the stars. This is 13 degrees per day, or just over 0.5 degree per hour. So, while the rotation of the Earth causes the stars and the Moon to appear to move from east to west across the night sky, the Moon, because of its own orbit around the Earth, fights back against this apparent motion, and seems to move eastward (or retrograde) by about 0.5 degree per hour. In other words, the Moon "moves" west only 11.5 degrees per hour."

text: It appears that Johannes Werner inspired by Amerigo Vespucci's letter written in 1502 where he wrote: "...I maintain that I learned [my longitude] ... by the eclipses and conjunctions of the Moon with the planets; and I have lost many nights of sleep in reconciling my calculations with the precepts of those sages who have devised the manuals and written of the movements, conjunctions, aspects, and eclipses of the two luminaries and of the wandering stars, such as the wise King Don Alfonso in his Tables, Johannes Regiomontanus in his Almanac, and Blanchinus, and the

text: Rabbi Zacuto

text: in his almanac, which is perpetual; and these were composed in different meridians: King Don Alfonso's book in the meridian of Toledo, and Johannes Regiomontanus's in that of Ferrara, and the other two in that of Salamanca."2 The best "clock" to use for reference, is the stars. In the roughly 27.3 solar days of a lunar orbit, the Moon moves a full 360 degrees around the sky, returning to its old position among the stars. This is 13 degrees per day, or just over 0.5 degree per hour. So, while the rotation of the Earth causes the stars and the Moon to appear to move from east to west across the night sky, the Moon, because of its own orbit around the Earth, fights back against this apparent motion, and seems to move eastward (or retrograde) by about 0.5 degree per hour. In other words, the Moon "moves" west only 11.5 degrees per hour."

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answers: NDQ_002351

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answers: NDQ_002352

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answers: NDQ_002354

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answers: The Moon moves a full 360 degrees around the sky

answers: NDQ_002356

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answers: NDQ_002360

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answers: the Moon moves a full 360 degrees around the sky

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answers: 27.3 solar days

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answers: 27.3 solar days

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text: The phases of the moon are shown in the oculus of the upper part of the dial. It completes a full rotation in 29 days. The week days are shown in an opening at the base of the dial with allegorical subjects for each day of the week.

text: The phases of the moon are shown in the

text: oculus

text: of the upper part of the dial. It completes a full rotation in 29 days. The week days are shown in an opening at the base of the dial with allegorical subjects for each day of the week.

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text: The Principia deals primarily with massive bodies in motion, initially under a variety of conditions and hypothetical laws of force in both non-resisting and resisting media, thus offering criteria to decide, by observations, which laws of force are operating in phenomena that may be observed. It attempts to cover hypothetical or possible motions both of celestial bodies and of terrestrial projectiles. It explores difficult problems of motions perturbed by multiple attractive forces. Its third and final book deals with the interpretation of observations about the movements of planets and their satellites. It shows how astronomical observations prove the inverse square law of gravitation (to an accuracy that was high by the standards of Newton's time); offers estimates of relative masses for the known giant planets and for the Earth and the Sun; defines the very slow motion of the Sun relative to the solar-system barycenter; shows how the theory of gravity can account for irregularities in the motion of the Moon; identifies the oblateness of the figure of the Earth; accounts approximately for marine tides including phenomena of spring and neap tides by the perturbing (and varying) gravitational attractions of the Sun and Moon on the Earth's waters; explains the precession of the equinoxes as an effect of the gravitational attraction of the Moon on the Earth's equatorial bulge; and gives theoretical basis for numerous phenomena about comets and their elongated, near-parabolic orbits.

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answers: spring

answers: NDQ_002324

answers: equatorial bulge

answers: NDQ_002325

answers: Neap

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: marine tides

answers: NDQ_002328

answers: marine tides

answers: NDQ_002329

answers: neap

answers: NDQ_002330

answers: equatorial bulge

answers: NDQ_002331

answers: spring and neap tides

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: The Principia

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: the Sun and Moon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Principia

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: The Principia

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The Principia

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: total lunar eclipse

answers: NDQ_002357

answers: The Principia

answers: NDQ_002358

answers: the first quarter phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

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answers: spring and neap tides

answers: NDQ_002363

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answers: NDQ_002364

answers: Earth and the Sun

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answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: approximately

answers: NDQ_002368

answers: crescent

text: On the horizon refraction is slightly greater than the apparent diameter of the Sun, so when the bottom of the sun's disc appears to touch the horizon, the sun's true altitude is negative. If the atmosphere suddenly vanished, the sun would too. By convention, sunrise and sunset refer to times at which the Sun’s upper limb appears on or disappears from the horizon and the standard value for the Sun’s true altitude is −50′: −34′ for the refraction and −16′ for the Sun’s semi-diameter. The altitude of a celestial body is normally given for the center of the body’s disc. In the case of the Moon, additional corrections are needed for the Moon’s horizontal parallax and its apparent semi-diameter; both vary with the Earth–Moon distance.

text: On the horizon refraction is slightly greater than the apparent diameter of the Sun, so when the bottom of the sun's disc appears to touch the horizon, the sun's true altitude is negative. If the atmosphere suddenly vanished, the sun would too. By convention,

text: sunrise

text: and

text: sunset

text: refer to times at which the Sun’s upper limb appears on or disappears from the horizon and the standard value for the Sun’s true altitude is −50′: −34′ for the refraction and −16′ for the Sun’s

text: semi-diameter

text: . The altitude of a celestial body is normally given for the center of the body’s disc. In the case of the

text: Moon

text: , additional corrections are needed for the Moon’s

text: horizontal parallax

text: and its apparent semi-diameter; both vary with the Earth–Moon distance.

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answers: sunset

answers: NDQ_002324

answers: upper limb appears on or disappears from the horizon

answers: NDQ_002325

answers: sunset

answers: NDQ_002326

answers: positive

answers: NDQ_002327

answers: sunset

answers: NDQ_002328

answers: the Sun’s true altitude is  50′

answers: NDQ_002329

answers: the Sun’s upper limb appears on or disappears from the horizon

answers: NDQ_002330

answers: the Sun’s true altitude is negative

answers: NDQ_002331

answers: sunset

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: the bottom of the sun's disc appears to touch the horizon

answers: NDQ_002335

answers: Sunrise

answers: NDQ_002343

answers: It depends on the distance between the Earth and the Moon.

answers: NDQ_002345

answers: When the bottom of the sun's disc appears to touch the horizon, the sun's true altitude is negative

answers: NDQ_002348

answers: The bottom of the sun's disc appears to touch the horizon

answers: NDQ_002350

answers: The bottom of the sun's disc appears to touch the horizon

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: The altitude of a celestial body is normally given for the center of the body’s disc

answers: NDQ_002353

answers: the bottom of the sun's disc appears to touch the horizon

answers: NDQ_002354

answers: The Sun’s true altitude is  50′:  34′ for the refraction and  16′ for the Sun’s semi-diameter

answers: NDQ_002355

answers: Earth–Moon distance

answers: NDQ_002356

answers: Moon

answers: NDQ_002357

answers: Earth–Moon distance

answers: NDQ_002358

answers: Moon’s horizontal parallax and its apparent semi-diameter

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Earth–Moon distance

answers: NDQ_002361

answers: Earth–Moon distance

answers: NDQ_002362

answers: the Earth–Moon distance

answers: NDQ_002363

answers: celestial body

answers: NDQ_002364

answers: the bottom of the sun's disc appears to touch the horizon

answers: NDQ_002365

answers: 50′

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: crescent

text: Earth's Moon is a gray disc in the sky with cratering visible to the naked eye.  It spans, depending on its exact location, 29-33 arcminutes - which is about the size of a thumbnail at arm's length, and is readily identified.  Over 28 days, the moon goes through a full cycle of lunar phases.  People can generally identify phases within a few days by looking at the moon.  Unlike stars and most planets, the light reflected from the moon is bright enough to be seen during the day. (Venus can sometimes be seen even after sunrise.)

text: Earth's

text: Moon

text: is a gray disc in the sky with cratering visible to the naked eye.  It spans, depending on its exact location, 29-33

text: arcminutes

text: - which is about the size of a thumbnail at arm's length, and is readily identified.  Over 28 days, the moon goes through a full cycle of

text: lunar phase

text: s.  People can generally identify phases within a few days by looking at the moon.  Unlike stars and most planets, the light reflected from the moon is bright enough to be seen during the day. (Venus can sometimes be seen even after sunrise.)

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text: There are two reasons why the north pole and south pole of the Moon might be attractive locations for a human colony. First, there is evidence that water may be present in some continuously shaded areas near the poles. Second, the Moon's axis of rotation is sufficiently close to being perpendicular to the ecliptic plane that the radius of the Moon's polar circles is less than 50 km. Power collection stations could therefore be plausibly located so that at least one is exposed to sunlight at all times, thus making it possible to power polar colonies almost exclusively with solar energy. Solar power would be unavailable only during a lunar eclipse, but these events are relatively brief and absolutely predictable. Any such colony would therefore require a reserve energy supply that could temporarily sustain a colony during lunar eclipses or in the event of any incident or malfunction affecting solar power collection. Hydrogen fuel cells would be ideal for this purpose, since the hydrogen needed could be sourced locally using the Moon's polar water and surplus solar power. Moreover, due to the Moon's uneven surface some sites have nearly continuous sunlight. For example, Malapert mountain, located near the Shackleton crater at the Lunar south pole, offers several advantages as a site:

text: There are two reasons why the

text: north pole

text: and

text: south pole

text: of the Moon might be attractive locations for a human colony. First, there is evidence that water may be present in some continuously shaded areas near the poles. Second, the Moon's

text: axis of rotation

text: is sufficiently close to being perpendicular to the

text: ecliptic plane

text: that the radius of the Moon's

text: polar circle

text: s is less than 50 km. Power collection stations could therefore be plausibly located so that at least one is exposed to sunlight at all times, thus making it possible to power polar colonies almost exclusively with solar energy. Solar power would be unavailable only during a

text: lunar eclipse

text: , but these events are relatively brief and absolutely predictable. Any such colony would therefore require a reserve energy supply that could temporarily sustain a colony during lunar eclipses or in the event of any incident or malfunction affecting solar power collection. Hydrogen

text: fuel cells

text: would be ideal for this purpose, since the hydrogen needed could be sourced locally using the Moon's polar water and surplus solar power. Moreover, due to the Moon's uneven surface some sites have nearly continuous sunlight. For example,

text: Malapert mountain

text: , located near the

text: Shackleton crater

text: at the Lunar south pole, offers several advantages as a site:

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text: In the Babylon 5 universe, Minbar is a planet in the system of Chi Draconis — a binary star system just over 26 light years from Earth.  It is the seventh planet in orbit around the local suns and has two moons. Its day is shorter than Earth's, at 20 hours and 47 minutes, and its year is about 1.5 Earth years.  Like Earth, Minbar has an oxygen—nitrogen atmosphere.  The polar caps are larger than those on Earth; the northern cap covers 23% of the planet's surface and, on the whole, Minbar's climate is colder than that of Earth - more like the climate on Earth during the last Ice Age. The planet is noted for vast crystalline structures; many cities are carved directly from crystal. The population of the planet is about 4 billion, and the capital city is located at Yedor.

text: In the Babylon 5 universe, Minbar is a planet in the system of

text: Chi Draconis

text: — a binary

text: star system

text: just over 26 light years from Earth.  It is the seventh planet in orbit around the local suns and has two moons. Its day is shorter than Earth's, at 20 hours and 47 minutes, and its year is about 1.5 Earth years.  Like Earth, Minbar has an oxygen—nitrogen atmosphere.  The polar caps are larger than those on Earth; the northern cap covers 23% of the planet's surface and, on the whole, Minbar's climate is colder than that of Earth - more like the climate on Earth during the last Ice Age. The planet is noted for vast crystalline structures; many cities are carved directly from crystal. The population of the planet is about 4 billion, and the capital city is located at Yedor.

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text: Partial melting within the mantle of the Moon gave rise to the eruption of mare basalts on the lunar surface. Analyses of these basalts indicate that the mantle is composed predominantly of the minerals olivine, orthopyroxene and clinopyroxene, and that the lunar mantle is more iron rich than that of the Earth. Some lunar basalts contain high abundances of titanium (present in the mineral ilmenite), suggesting that the mantle is highly heterogeneous in composition. Moonquakes have been found to occur deep within the mantle of the Moon about 1,000 km below the surface. These occur with monthly periodicities and are related to tidal stresses caused by the eccentric orbit of the Moon about the Earth. A few shallow moonquakes with hypocenters located about 100 km below the surface have also been detected, but these occur more infrequently and appear to be unrelated to the lunar tides.

text: Partial melting within the mantle of the Moon gave rise to the eruption of mare basalts on the lunar surface. Analyses of these basalts indicate that the mantle is composed predominantly of the minerals

text: olivine

text: orthopyroxene

text: and

text: clinopyroxene

text: , and that the lunar mantle is more iron rich than that of the Earth. Some lunar basalts contain high abundances of titanium (present in the mineral

text: ilmenite

text: ), suggesting that the mantle is highly heterogeneous in composition.

text: Moonquake

text: s have been found to occur deep within the mantle of the Moon about 1,000 km below the surface. These occur with monthly periodicities and are related to tidal stresses caused by the eccentric orbit of the Moon about the Earth. A few shallow moonquakes with hypocenters located about 100 km below the surface have also been detected, but these occur more infrequently and appear to be unrelated to the lunar tides.

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answers: lunar tides

text: A total solar eclipse occurred on March 28-29, 2006. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.It was visible from a narrow corridor which traversed half the Earth. The magnitude, that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.

text: A total

text: solar eclipse

text: occurred on March 28-29, 2006. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's

text: apparent diameter

text: is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.It was visible from a narrow corridor which traversed half the

text: Earth

text: . The

text: magnitude

text: , that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.

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answers: Solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002345

answers: It was visible from a narrow corridor which traversed half the Earth

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answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: It was visible from a narrow corridor which traversed half the Earth

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answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

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answers: NDQ_002353

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answers: NDQ_002354

answers: A total solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: March 28-29, 2006

answers: NDQ_002357

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answers: NDQ_002358

answers: crescent phase

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answers: March 28

answers: NDQ_002360

answers: The Moon passes between Earth and the Sun

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answers: 29

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answers: partial solar eclipse

text: An annular solar eclipse will occur on January 27, 2074. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on January 27, 2074. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: An annular solar eclipse appears as a partial eclipse

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answers: It will occur on January 27, 2074

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answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

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text: Stationed at NASA Goddard Space Flight Center in Maryland for over 20 years, Rodríguez-Arroyo was the Communications System Lead Engineer for the Lunar Reconnaissance Orbiter Mission (LRO), launched in June 2009 and currently orbiting the moon. Currently, Rodriguez-Arroyo is the Communications System Lead Engineer for the Magnetospheric MultiScale Mission (MMS) to be launched in 2015 and will study the electromagnetic iteration between the Sun and Earth.

text: Stationed at NASA Goddard Space Flight Center in Maryland for over 20 years, Rodríguez-Arroyo was the Communications System Lead Engineer for the Lunar Reconnaissance Orbiter Mission (LRO), launched in June 2009 and currently orbiting the moon. Currently, Rodriguez-Arroyo is the Communications System Lead Engineer for the Magnetospheric MultiScale Mission (MMS) to be launched in 2015 and will study the electromagnetic iteration between the Sun and Earth.

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answers: Reconnaissance

text: is its orbital angular velocity. That of Jupiter contributes the bulk of the Solar System's angular momentum, 60.3%. Then comes Saturn at 24.5%, Neptune at 7.9%, and Uranus at 5.3%. The Sun forms a counterbalance to all of the planets, so it is near the barycenter when Jupiter is on one side and the other three jovian planets are diametrically opposite on the other side, but the Sun moves to 2.17 solar radii away from the barycenter when all jovian planets are in line on other side. The orbital angular momenta of the Sun and all non-jovian planets, moons, and small Solar System bodies, as well as the axial rotation momenta of all bodies, including the Sun, total only about 2%.

text: is its orbital angular velocity. That of Jupiter contributes the bulk of the Solar System's angular momentum, 60.3%. Then comes Saturn at 24.5%, Neptune at 7.9%, and Uranus at 5.3%. The

text: Sun

text: forms a counterbalance to all of the planets, so it is near the barycenter when Jupiter is on one side and the other three jovian planets are diametrically opposite on the other side, but the Sun moves to 2.17 solar radii away from the barycenter when all jovian planets are in line on other side. The orbital angular momenta of the Sun and all non-jovian planets, moons, and

text: small Solar System bodies

text: , as well as the axial rotation momenta of all bodies, including the Sun, total only about 2%.

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answers: Jupiter contributes the bulk of the Solar System's angular momentum

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answers: Neptune at 7.9%, and Uranus at 5.3%

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answers: Jupiter contributes the bulk of the Solar System's angular momentum, 60.3%

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text: Hipparchus was born in Nicaea, Bithynia (now Iznik, Turkey), and probably died on the island of Rhodes. He is known to have been a working astronomer at least from 162 to 127 . Hipparchus is considered the greatest ancient astronomical observer and, by some, the greatest overall astronomer of antiquity. He was the first whose quantitative and accurate models for the motion of the Sun and Moon survive. For this he certainly made use of the observations and perhaps the mathematical techniques accumulated over centuries by the Babylonians and other people from Mesopotamia. He developed trigonometry and constructed trigonometric tables, and he solved several problems of spherical trigonometry. With his solar and lunar theories and his trigonometry, he may have been the first to develop a reliable method to predict solar eclipses. His other reputed achievements include the discovery and measurement of Earth's precession, the compilation of the first comprehensive star catalog of the western world, and possibly the invention of the astrolabe, also of the armillary sphere, which he used during the creation of much of the star catalogue.

text: Hipparchus was born in

text: Nicaea

text: Bithynia

text: (now

text: Iznik

text: Turkey

text: ), and probably died on the island of

text: Rhodes

text: . He is known to have been a working astronomer at least from 162 to 127 . Hipparchus is considered the greatest ancient astronomical observer and, by some, the greatest overall astronomer of

text: antiquity

text: . He was the first whose quantitative and accurate models for the motion of the

text: Sun

text: and

text: Moon

text: survive. For this he certainly made use of the observations and perhaps the mathematical techniques accumulated over centuries by the

text: Babylonia

text: ns and other people from

text: Mesopotamia

text: . He developed trigonometry and constructed trigonometric tables, and he solved several problems of

text: spherical trigonometry

text: . With his solar and

text: lunar

text: theories and his trigonometry, he may have been the first to develop a reliable method to predict

text: solar eclipse

text: s. His other reputed achievements include the discovery and measurement of Earth's precession, the compilation of the first comprehensive

text: star catalog

text: of the western world, and possibly the invention of the

text: astrolabe

text: , also of the

text: armillary sphere

text: , which he used during the creation of much of the star catalogue.

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text: The Moon's orbit around the Earth is inclined at an angle of just over 5 degrees to the plane of the Earth's orbit around the Sun (the ecliptic). Because of this, at the time of a new moon, the Moon will usually pass to the north or south of the Sun. A solar eclipse can occur only when new moon occurs close to one of the points (known as nodes) where the Moon's orbit crosses the ecliptic.

text: The

text: Moon's orbit

text: around the Earth is inclined at an angle of just over 5 degrees to the plane of the Earth's orbit around the Sun (the

text: ecliptic

text: ). Because of this, at the time of a new moon, the Moon will usually pass to the north or south of the Sun. A solar eclipse can occur only when new moon occurs close to one of the points (known as

text: node

text: s) where the Moon's orbit crosses the ecliptic.

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answers: 4

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answers: 4

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answers: new moon

answers: NDQ_002324

answers: north or south

answers: NDQ_002325

answers: new moon

answers: NDQ_002326

answers: A solar eclipse

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: new moon

answers: NDQ_002330

answers: the Sun

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: new moon

answers: NDQ_002334

answers: the Sun

answers: NDQ_002335

answers: new moon

answers: NDQ_002343

answers: The Moon will usually pass to the north or south of the Sun

answers: NDQ_002345

answers: the Moon's orbit crosses the ecliptic

answers: NDQ_002348

answers: The Moon's orbit crosses the ecliptic

answers: NDQ_002350

answers: nodes

answers: NDQ_002351

answers: new moon

answers: NDQ_002352

answers: the ecliptic

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Can occur only when new moon occurs close to one of the points (known as nodes) where the Moon's orbit crosses the ecliptic

answers: NDQ_002355

answers: Moon's orbit crosses the ecliptic

answers: NDQ_002356

answers: The Moon's orbit around the Earth is inclined at an angle of just over 5 degrees

answers: NDQ_002357

answers: The Moon's orbit around the Earth

answers: NDQ_002358

answers: new moon

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Moon will usually pass to the north or south of the Sun

answers: NDQ_002361

answers: the Moon's orbit crosses the ecliptic

answers: NDQ_002362

answers: A solar eclipse

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answers: orbit around the Sun

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answers: the Moon's orbit crosses the ecliptic

answers: NDQ_002365

answers: 5 degrees

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: new moon

text: The phases of the moon are also followed closely, but in practice rarely celebrated in a liturgical manner, except by modern groves with a neopagan focus or women's mysteries. Projects are started on a waxing moon and completed on a waning moon. The night of the full moon is considered a time of rejoicing; while the night of the new moon is a solemn occasion, calling for vigils and meditation.

text: The phases of the moon are also followed closely, but in practice rarely celebrated in a liturgical manner, except by modern groves with a neopagan focus or women's mysteries. Projects are started on a waxing moon and completed on a waning moon. The night of the full moon is considered a time of rejoicing; while the night of the new moon is a solemn occasion, calling for vigils and meditation.

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answers: full moon

answers: NDQ_002324

answers: full moon and waning moon

answers: NDQ_002325

answers: new moon

answers: NDQ_002326

answers: waxing

answers: NDQ_002327

answers: night of the new moon

answers: NDQ_002328

answers: night of the full moon is considered a time of rejoicing

answers: NDQ_002329

answers: waning

answers: NDQ_002330

answers: The night of the new moon

answers: NDQ_002331

answers: night of the new moon

answers: NDQ_002332

answers: waxing

answers: NDQ_002334

answers: The night of the new moon

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: The night of the full moon

answers: NDQ_002345

answers: The night of the full moon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The night of the full moon

answers: NDQ_002351

answers: waxing moon and completed on a waning moon

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The phases of the moon

answers: NDQ_002355

answers: Partially lunar eclipse

answers: NDQ_002356

answers: The night of the full moon

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: waning

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: The phases of the moon

answers: NDQ_002363

answers: phase of the moon

answers: NDQ_002364

answers: full moon

answers: NDQ_002365

answers: a night

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: a waxing moon

answers: NDQ_002368

answers: new moon

text: All eight planets in the Solar System orbit the Sun in the direction that the Sun is rotating, which is counterclockwise when viewed from above the Sun's north pole. Six of the planets also rotate about their axis in this same direction. The exceptions—the planets with retrograde rotation—are Venus and Uranus. Venus's axial tilt is 177 degrees, which means it is spinning almost exactly in the opposite direction to its orbit. Uranus has an axial tilt of 97.77 degrees, so its axis of rotation is approximately parallel with the plane of the Solar System. The reason for Uranus's unusual axial tilt is not known with certainty, but the usual speculation is that during the formation of the Solar System, an Earth-sized protoplanet collided with Uranus, causing the skewed orientation.

text: All eight planets in the Solar System orbit the Sun in the direction that the Sun is rotating, which is

text: counterclockwise

text: when viewed from above the Sun's

text: north pole

text: . Six of the planets also rotate about their axis in this same direction. The exceptions—the planets with retrograde rotation—are

text: Venus

text: and

text: Uranus

text: . Venus's axial tilt is 177 degrees, which means it is spinning almost exactly in the opposite direction to its orbit. Uranus has an axial tilt of 97.77 degrees, so its axis of rotation is approximately parallel with the plane of the Solar System. The reason for Uranus's unusual axial tilt is not known with certainty, but the usual speculation is that during the formation of the Solar System, an Earth-sized

text: protoplanet

text: collided with Uranus, causing the skewed orientation.

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answers: Earth-phase

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answers: Sun's north pole

answers: NDQ_002325

answers: nebula

answers: NDQ_002326

answers: retrograde

answers: NDQ_002327

answers: Earth's shadow

answers: NDQ_002328

answers: Venus's axial tilt

answers: NDQ_002329

answers: Earth-sized

answers: NDQ_002330

answers: the Sun

answers: NDQ_002331

answers: orbit the Sun

answers: NDQ_002332

answers: Venus

answers: NDQ_002334

answers: Sun

answers: NDQ_002335

answers: Earth-phase

answers: NDQ_002343

answers: How long does a lunar eclipse last?

answers: NDQ_002345

answers: Venus's axial tilt

answers: NDQ_002348

answers: Venus's axial tilt

answers: NDQ_002350

answers: When viewed from above the Sun's north pole

answers: NDQ_002351

answers: Uranus

answers: NDQ_002352

answers: Uranus

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Earth-sized protoplanet collided with Uranus

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: It is not known with certainty

answers: NDQ_002357

answers: Uranus

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: retrograde rotation

answers: NDQ_002361

answers: the Sun is rotating

answers: NDQ_002362

answers: the formation of the Solar System

answers: NDQ_002363

answers: plane of the Solar System

answers: NDQ_002364

answers: when viewed from above the Sun's north pole

answers: NDQ_002365

answers: counterclockwise

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: new moon

text: An annular solar eclipse occurred on October 3, 2005 with a magnitude of 0.958. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.It was visible from a narrow corridor through the Iberian peninsula and Africa. A partial eclipse was seen from the much broader path of the Moon's penumbra, including all of Europe, Africa and southwestern Asia.

text: An annular

text: solar eclipse

text: occurred on October 3, 2005 with a magnitude of 0.958. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.It was visible from a narrow corridor through the

text: Iberian peninsula

text: and

text: Africa

text: . A

text: partial eclipse

text: was seen from the much broader path of the

text: Moon

text: 's

text: penumbra

text: , including all of

text: Europe

text: Africa

text: and southwestern

text: Asia

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: penumbra

answers: NDQ_002324

answers: penumbra

answers: NDQ_002325

answers: penumbra

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: Moon passes between Earth and the Sun

answers: NDQ_002330

answers: penumbra

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: penumbra

answers: NDQ_002334

answers: penumbra

answers: NDQ_002335

answers: penumbra

answers: NDQ_002343

answers: Solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: Moon passes between Earth and the Sun

answers: NDQ_002352

answers: Moon's penumbra

answers: NDQ_002353

answers: penumbra

answers: NDQ_002354

answers: An annular solar eclipse occurred on October 3, 2005

answers: NDQ_002355

answers: A partial eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: The Moon passes between Earth and the Sun

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: October

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: penumbra

text: An annular solar eclipse will occur on November 15, 2077. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on November 15, 2077. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 3

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answers: 0

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answers: 4

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

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answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: obscuring the image of the Sun

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: It will occur on November 15, 2077

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On November 15, 2077

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: November

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: November 15

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: crescent

text: 7194 Susanrose (provisional designation: 1993 SR) is a main-belt minor planet.  It was discovered by Henry E. Holt at the Palomar Observatory in San Diego County, California, on September 18, 1993.  It is named after Susan Rose, an American amateur astronomer and astronomy enthusiast. Susan Rose, born Susan F. Campbell, née Brown, Farrell, Aug 9, 1952, Brooklyn, NY, US James Madison HS 1970, Brooklyn College 1974; BS Geology, minor Oceanography and Physics. An avid amateur astronomer since the age of 2, called a moonagazer by her great grandmother who chastised her mother for allowing her to stare at the moon. Member Amateur Observers' Society of NY, AOS, (http://www.aosny.org) 1973–present, Recording Secretary 1989-1992, President 1992-2009, President Emeritus 2009–presentAOS Observatory in Southold, NY, renamed Susan F. Rose Observatory Aug 8, 2009, http://www.skyandtelescope.com/news/home/52891802.htmlRecipient NERAL, Northeast Region of the Astronomical League, 2002 Walter Scott Houston Award, http://www.neral.org/pastawards.htmCaldwell Club Administrator for the Astronomical League, 2001–presentTotal Solar Eclipse, Feb 26, 1979 from Lewistown, Montana, USAnnular Solar Eclipse, May 30, 1984, from Atlanta, Georgia, USTotal Solar Eclipse, July 11, 1991, from Ruiz, MexicoAnnular Solar Eclipse, Jan 4, 1992, from San Francisco, California, USAnnular Solar Eclipse, May 10, 1994, Rochester, New York, USTotal Solar Eclipse, Feb 26, 1998, from SS Veendam in the CaribbeanAnnular Solar Eclipse, June 10, 2002, MexicoHalley's Comet, Galapagos Islands, March 1985Transit of Venus, June 8, 2004, Jones Beach, Long Island, NY, USHall of Science, Queens, NY, Planet Earth Lab Instructor, Planetarium Assistant Director, 1974-1981Air Traffic Controller, JFK Airport, 1981-2008, retired

text: 7194 Susanrose (provisional designation: 1993 SR) is a

text: main-belt

text: minor planet

text: .  It was discovered by

text: Henry E. Holt

text: at the

text: Palomar Observatory

text: in

text: San Diego County

text: California

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answers: 0: The answer is not relevant or complete at all.

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answers: Annular

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answers: Total Solar Eclipse

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answers: Annular

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answers: Total Solar Eclipse

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answers: Annular

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answers: It was discovered by Henry E. Holt

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answers: It was discovered by Henry E. Holt

answers: NDQ_002352

answers: Venus

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Annular Solar Eclipse, June 10, 2002, Mexico

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answers: Partial lunar eclipse

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answers: Annular Solar Eclipse

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answers: June 10, 2002

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answers: NDQ_002362

answers: Total Solar Eclipse, Feb 26, 1979

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answers: total solar eclipse

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answers: 30 minutes

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answers: June 10, 2002

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answers: Annular Solar Eclipse

text: A partial lunar eclipse occurs when only a portion of the moon enters the umbra. When the moon travels completely into the Earth's umbra, one observes a total lunar eclipse. The moon's speed through the shadow is about one kilometer per second (2,300 mph), and totality may last up to nearly 107 minutes. Nevertheless, the total time between the moon's first and last contact with the shadow is much longer and could last up to four hours. The relative distance of the moon from the Earth at the time of an eclipse can affect the eclipse's duration. In particular, when the moon is near its apogee, the farthest point from the Earth in its orbit, its orbital speed is the slowest. The diameter of the umbra does not decrease appreciably within the changes in the orbital distance of the moon. Thus, a totally eclipsed moon occurring near apogee will lengthen the duration of totality.

text: A partial lunar eclipse occurs when only a portion of the moon enters the umbra. When the moon travels completely into the Earth's umbra, one observes a total lunar eclipse. The moon's speed through the shadow is about one kilometer per second (2,300 mph), and totality may last up to nearly 107 minutes. Nevertheless, the total time between the moon's first and last contact with the shadow is much longer and could last up to four hours. The relative distance of the moon from the Earth at the time of an eclipse can affect the eclipse's duration. In particular, when the moon is near its

text: apogee

text: , the farthest point from the Earth in its orbit, its orbital speed is the slowest. The diameter of the umbra does not decrease appreciably within the changes in the orbital distance of the moon. Thus, a totally eclipsed moon occurring near apogee will lengthen the duration of totality.

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answers: partial

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answers: partial lunar eclipse

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answers: lunar eclipse

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answers: total lunar eclipse

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answers: the umbra

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answers: total

answers: NDQ_002343

answers: totality may last up to nearly 107 minutes

answers: NDQ_002345

answers: The moon travels completely into the Earth's umbra

answers: NDQ_002348

answers: When the moon travels completely into the Earth's umbra

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answers: When the moon travels completely into the Earth's umbra

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answers: When the moon travels completely into the Earth's umbra

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answers: umbra

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answers: partial lunar eclipse

answers: NDQ_002354

answers: Solar eclipses are rare.

answers: NDQ_002355

answers: When the moon travels completely into the Earth's umbra

answers: NDQ_002356

answers: It can affect the eclipse's duration

answers: NDQ_002357

answers: When the moon travels completely into the Earth's umbra

answers: NDQ_002358

answers: When the moon travels completely into the Earth's umbra

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answers: When the moon travels completely into the Earth's umbra

answers: NDQ_002360

answers: When the moon travels completely into the Earth's umbra

answers: NDQ_002361

answers: The moon's speed through the shadow

answers: NDQ_002362

answers: the moon's speed through the shadow

answers: NDQ_002363

answers: Earth's

answers: NDQ_002364

answers: When the sun enters the Earth's umbra

answers: NDQ_002365

answers: 107 minutes

answers: NDQ_002366

answers: Earth

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answers: four hours

answers: NDQ_002368

answers: partial lunar eclipse

text: A partial solar eclipse occurred on July 1, 2011. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.This is the first solar eclipse of saros series 156, only visible as a partial solar eclipse in a small area south of South Africa and north of Antarctica. At greatest eclipse, the magnitude is just 0.097. It is the first new saros series to begin since saros 155 began with the partial solar eclipse of June 17, 1928.

text: A partial

text: solar eclipse

text: occurred on July 1, 2011. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.This is the first solar eclipse of

text: saros series 156

text: , only visible as a partial solar eclipse in a small area south of

text: South Africa

text: and north of

text: Antarctica

text: . At greatest eclipse, the

text: magnitude

text: is just 0.097. It is the first new saros series to begin since

text: saros 155

text: began with the partial

text: solar eclipse of June 17, 1928

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answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: the Sun and the Moon

answers: NDQ_002325

answers: partial solar eclipse

answers: NDQ_002326

answers: partial

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: a partial solar eclipse

answers: NDQ_002330

answers: misses the Earth

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses the Earth

answers: NDQ_002335

answers: solar eclipse

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: The Moon passes between Earth and the Sun

answers: NDQ_002348

answers: Solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002350

answers: A partial solar eclipse occurs in a small area south of South Africa and north of Antarctica

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center of the Moon's shadow

answers: NDQ_002353

answers: partial solar eclipse

answers: NDQ_002354

answers: It is the first new series to begin since saros 155 began with the partial solar eclipse of June 17, 1928

answers: NDQ_002355

answers: Solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: A partial solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: July 1, 2011

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: the Sun

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: July 1, 2011

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: partial solar eclipse

text: Tidal flow occurs due to the moving mass of water with speed and direction as caused by the gravitational forces of the sun and the moon, and centrifugal and inertial forces on the Earth's waters. Due to its proximity to the earth, the moon exerts roughly twice the tide raising force of the sun. The gravitational forces of the sun and moon and the centrifugal/inertial forces caused by the rotation of the earth around the center of mass of the earth-moon system create two "bulges" in the Earth's oceans: one closest to the moon, and the other on the opposite side of the globe.(CNW Group, 2008). This kind of energy is unique and different from traditional hydropower that has been around for centuries. There is no need to build a dam. Essentially a turbine is stuck in naturally flowing water. As the water flows, it turns a turbine. That is converted to electricity.

text: Tidal flow occurs due to the moving mass of water with speed and direction as caused by the gravitational forces of the sun and the moon, and centrifugal and inertial forces on the Earth's waters. Due to its proximity to the earth, the moon exerts roughly twice the tide raising force of the sun. The gravitational forces of the sun and moon and the centrifugal/inertial forces caused by the rotation of the earth around the center of mass of the earth-moon system create two "bulges" in the Earth's oceans: one closest to the moon, and the other on the opposite side of the globe.(CNW Group, 2008). This kind of energy is unique and different from traditional hydropower that has been around for centuries. There is no need to build a dam. Essentially a turbine is stuck in naturally flowing water. As the water flows, it turns a turbine. That is converted to electricity.

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answers: NDQ_002323

answers: Earth's

answers: NDQ_002324

answers: one closest to the moon, and the other

answers: NDQ_002325

answers: gibbous

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: Tidal flow

answers: NDQ_002328

answers: Tidal flow

answers: NDQ_002329

answers: roughly twice the tide

answers: NDQ_002330

answers: one closest to the moon

answers: NDQ_002331

answers: Tidal flow

answers: NDQ_002332

answers: the moon

answers: NDQ_002334

answers: Earth's oceans

answers: NDQ_002335

answers: Earth's

answers: NDQ_002343

answers: Tidal flow

answers: NDQ_002345

answers: the moon exerts roughly twice the tide raising force of the sun

answers: NDQ_002348

answers: the moon exerts roughly twice the tide raising force of the sun

answers: NDQ_002350

answers: the opposite side of the globe

answers: NDQ_002351

answers: The gravitational forces of the sun and moon

answers: NDQ_002352

answers: The gravitational forces of the sun and the moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The moon exerts roughly twice the tide raising force of the sun

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: It does not state when it occurs.

answers: NDQ_002357

answers: Earth-moon system

answers: NDQ_002358

answers: the first quarter phase

answers: NDQ_002359

answers: the moon

answers: NDQ_002360

answers: the moon exerts roughly twice the tide raising force of the sun

answers: NDQ_002361

answers: due to its proximity to the earth

answers: NDQ_002362

answers: the rotation of the earth around the center of mass of the earth-moon system

answers: NDQ_002363

answers: sun

answers: NDQ_002364

answers: the sun and the moon

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: roughly twice

answers: NDQ_002368

answers: gibbous

text: With the publication of his Principia roughly eighty years later (1687), Isaac Newton provided a physical theory that accounted for all three of Kepler's laws, a theory based on Newton's laws of motion and his law of universal gravitation. In particular, Newton proposed that the gravitational force between any two bodies was a central force F(r) that varied as the inverse square of the distance r between them. Arguing from his laws of motion, Newton showed that the orbit of any particle acted upon by one such force is always a conic section, specifically an ellipse if it does not go to infinity. However, this conclusion holds only when two bodies are present (the two-body problem); the motion of three bodies or more acting under their mutual gravitation (the n-body problem) remained unsolved for centuries after Newton, although solutions to a few special cases were discovered. Newton proposed that the orbits of planets about the Sun are largely elliptical because the Sun's gravitation is dominant; to first approximation, the presence of the other planets can be ignored. By analogy, the elliptical orbit of the Moon about the Earth was dominated by the Earth's gravity; to first approximation, the Sun's gravity and those of other bodies of the Solar System can be neglected. However, Newton stated that the gradual apsidal precession of the planetary and lunar orbits was due to the effects of these neglected interactions; in particular, he stated that the precession of the Moon's orbit was due to the perturbing effects of gravitational interactions with the Sun.

text: With the publication of his

entity_name: Philosophiæ Naturalis Principia Mathematica

text: Principia

text: roughly eighty years later (1687),

text: Isaac Newton

text: provided a physical theory that accounted for all three of Kepler's laws, a theory based on

text: Newton's laws of motion

text: and his

text: law of universal gravitation

text: . In particular, Newton proposed that the gravitational force between any two bodies was a

text: central force

text: F(r) that varied as the

text: inverse square

text: of the distance r between them. Arguing from his laws of motion, Newton showed that the orbit of any particle acted upon by one such force is always a

text: conic section

text: , specifically an ellipse if it does not go to infinity. However, this conclusion holds only when two bodies are present (the

text: two-body problem

text: ); the motion of three bodies or more acting under their mutual gravitation (the

text: n-body problem

text: ) remained unsolved for centuries after Newton, although solutions to a few

text: special cases

text: were discovered. Newton proposed that the orbits of planets about the Sun are largely elliptical because the Sun's gravitation is dominant; to

text: first approximation

text: , the presence of the other planets can be ignored. By analogy, the elliptical orbit of the

text: Moon

text: about the Earth was dominated by the Earth's gravity; to first approximation, the Sun's gravity and those of other bodies of the Solar System can be neglected. However, Newton stated that the gradual apsidal precession of the planetary and lunar orbits was due to the effects of these neglected interactions; in particular, he stated that the precession of the Moon's orbit was due to the perturbing effects of gravitational interactions with the Sun.

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answers: 0: The answer is not relevant or complete at all.

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answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 4

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answers: 4

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answers: NDQ_002323

answers: apogee

answers: NDQ_002324

answers: the Moon about the Earth

answers: NDQ_002325

answers: precession

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: precession

answers: NDQ_002328

answers: precession

answers: NDQ_002329

answers: a conic section

answers: NDQ_002330

answers: is always a conic section

answers: NDQ_002331

answers: precession

answers: NDQ_002332

answers: the Moon

answers: NDQ_002334

answers: the Earth's gravity

answers: NDQ_002335

answers: Moon's orbit

answers: NDQ_002343

answers: the Moon about the Earth

answers: NDQ_002345

answers: the presence of the other planets

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth's gravity

answers: NDQ_002351

answers: the inverse square of the distance r between them

answers: NDQ_002352

answers: the ellipse if it does not go to infinity

answers: NDQ_002353

answers: the two-body problem

answers: NDQ_002354

answers: solutions to a few special cases

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: the Moon about the Earth

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the inverse square of the distance r between them

answers: NDQ_002360

answers: Moon about the Earth

answers: NDQ_002361

answers: Earth's gravity

answers: NDQ_002362

answers: gravitational interactions with the Sun

answers: NDQ_002363

answers: ellipse

answers: NDQ_002364

answers: two bodies are present

answers: NDQ_002365

answers: about eighty years

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: roughly eighty years

answers: NDQ_002368

answers: crescent

text: The Moon-to-Earth mass ratio of 0.01230 (≈ ) is also notably close to 1 when compared to all other satellite-to-planet ratios. Consequently, some scientists view the Earth-Moon system as a double planet as well, though this is a minority view. Eris's lone satellite, Dysnomia, has a radius somewhere around 1/4 that of Eris; assuming similar densities (Dysnomia's compositional make-up may or may not differ substantially from Eris's), the mass ratio would be near , a value intermediate to the Moon/Earth and Charon/Pluto ratios.

text: The Moon-to-Earth mass ratio of 0.01230 (≈ ) is also notably close to 1 when compared to all other satellite-to-planet ratios. Consequently, some scientists view the Earth-Moon system as a double planet as well, though this is a minority view.

text: Eris

text: 's lone satellite,

text: Dysnomia

text: , has a radius somewhere around 1/4 that of

text: Eris

text: ; assuming similar densities (Dysnomia's compositional make-up may or may not differ substantially from Eris's), the mass ratio would be near , a value intermediate to the Moon/Earth and Charon/Pluto ratios.

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answers: 0

answers: NDQ_002323

answers: Earth-Moon

answers: NDQ_002324

answers: Moon-to-Earth

answers: NDQ_002325

answers: Eris

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: Moon-to-Earth mass ratio

answers: NDQ_002328

answers: the Earth-Moon system as a double planet

answers: NDQ_002329

answers: 1/4

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: Moon-to-Earth mass ratio

answers: NDQ_002332

answers: satellite

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: NDQ_002343

answers: Moon-to-Earth mass ratio

answers: NDQ_002345

answers: some scientists view the Earth-Moon system as a double planet

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Moon-to-Earth mass ratio

answers: NDQ_002352

answers: Eris's

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: This is a minority view

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: Moon-to-Earth mass ratio

answers: NDQ_002357

answers: Earth-Moon

answers: NDQ_002358

answers: Quarter phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Earth-Moon system

answers: NDQ_002361

answers: Earth-Moon system

answers: NDQ_002362

answers: the Earth-Moon system

answers: NDQ_002363

answers: Earth-Moon system

answers: NDQ_002364

answers: Earth-Moon system

answers: NDQ_002365

answers: 0.01230

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 0.01230

answers: NDQ_002368

answers: crescent

text: An annular solar eclipse occurred on January 26, 2009. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.It had a magnitude of 0.92 and was visible from a narrow corridor beginning in the south Atlantic Ocean and sweep eastward 900 km south of Africa, slowly curving northeast through the Indian Ocean.  Its first landfall was in the Cocos Islands followed by southern Sumatra and western Java.  It continued somewhat more easterly across central Borneo, across the northwestern edge of Celebes, then ending just before Mindanao, Philippines.

text: An annular

text: solar eclipse

text: occurred on January 26, 2009. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.It had a

text: magnitude

text: of 0.92 and was visible from a narrow corridor beginning in the south

text: Atlantic Ocean

text: and sweep eastward 900 km south of Africa, slowly curving northeast through the

text: Indian Ocean

text: .  Its first landfall was in the

text: Cocos Islands

text: followed by southern

text: Sumatra

text: and western

text: Java

text: .  It continued somewhat more easterly across central

text: Borneo

text: , across the northwestern edge of

text: Celebes

text: , then ending just before

text: Mindanao

text: Philippines

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answers: 4

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answers: 4

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answers: 4

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answers: NDQ_002367

answers: 0

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answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: Moon and Sun

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: an annular solar eclipse

answers: NDQ_002330

answers: annulus

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: It had a magnitude of 0.92

answers: NDQ_002345

answers: The Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the Sun

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: It had a magnitude of 0.92

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: January 26, 2009

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent

answers: NDQ_002359

answers: January 26, 2009

answers: NDQ_002360

answers: Moon passes between Earth

answers: NDQ_002361

answers: Moon passes between Earth

answers: NDQ_002362

answers: An annular solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial

text: According to Lucio Russo, Seleucus' arguments for a heliocentric theory were probably related to the phenomenon of tides. The annual cycle of tides (which was studied by Seleucus) can indeed hardly be explained in a geocentric system. Seleucus correctly theorized that tides were caused by the Moon, explaining that the interaction was mediated by the pneuma. He noted that the tides varied in time and strength in different parts of the world. According to Lucio Russo, Seleucus ascribed tides both to the Moon and to a whirling motion of the Earth, which could be interpreted as the motion of the Earth around the Earth-Moon center of mass.

text: According to

text: Lucio Russo

text: , Seleucus' arguments for a heliocentric theory were probably related to the phenomenon of

text: tide

text: s. The annual cycle of tides (which was studied by Seleucus) can indeed hardly be explained in a geocentric system. Seleucus correctly theorized that

text: tide

text: s were caused by the

text: Moon

text: , explaining that the interaction was mediated by the

text: pneuma

text: . He noted that the tides varied in time and strength in different parts of the world. According to

text: Lucio Russo

text: , Seleucus ascribed

text: tide

text: s both to the

text: Moon

text: and to a whirling motion of the

text: Earth

text: , which could be interpreted as the motion of the

text: Earth

text: around the

text: Earth

text: Moon

text: center of mass

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answers: 4

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answers: 4

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: Pneuma

answers: NDQ_002324

answers: Earth-Moon

answers: NDQ_002325

answers: pneuma

answers: NDQ_002326

answers: pneuma

answers: NDQ_002327

answers: tides

answers: NDQ_002328

answers: tides

answers: NDQ_002329

answers: annual

answers: NDQ_002330

answers: pneuma

answers: NDQ_002331

answers: tides

answers: NDQ_002332

answers: pneuma

answers: NDQ_002334

answers: pneuma

answers: NDQ_002335

answers: pneuma

answers: NDQ_002343

answers: Tides varied in time and strength

answers: NDQ_002345

answers: Seleucus

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The annual cycle of tides

answers: NDQ_002351

answers: annual cycle of tides

answers: NDQ_002352

answers: pneuma

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The annual cycle of tides

answers: NDQ_002355

answers: Earth-Moon center of mass

answers: NDQ_002356

answers: annual cycle of tides

answers: NDQ_002357

answers: Earth-Moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the lunar cycle

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: Earth-Moon

answers: NDQ_002362

answers: tides

answers: NDQ_002363

answers: center of mass

answers: NDQ_002364

answers: the Moon

answers: NDQ_002365

answers: time

answers: NDQ_002366

answers: annual

answers: NDQ_002367

answers: annual

answers: NDQ_002368

answers: pneuma

text: The Jovilabe is certainly connected to Galileo's efforts to determine the orbital periods of Jupiter's moons, whose discovery he announced in 1610 in Sidereus Nuncius, and to compute the times of their eclipses. Galileo immediately realized that eclipses of Jupiter's moons could provide a precise method to determine longitude. The instrument is engraved with tables showing the mean motions of each of the four moons. Two connected disks of different diameters are rotated by means of a movable rod. They are used to create a "view from the Sun" of the movements of Jupiter's moons observed from the Earth (movements that seem irregular because of the heliocentric motions of the Earth and Jupiter). Galileo began the systematic study of the periods of Jupiter's moons in 1611, developing a micrometer for the purpose. He compiled tables of the periods that he offered, with his telescopes, first to the King of Spain (1611, 1612, 1616, and 1627-1628), then to the States General of Holland (1637-1641). To convince his Spanish interlocutors that Jupiter and its moons could be observed on unstable ground, such as a ship's deck, Galileo designed a special helmet carrying a small telescope on a hinged mount. The device was named the celatone (celata = "helmet" in Italian). In this second proposal, he also described the advantages of applying the pendulum to the clock. Despite the interest they aroused, neither of his proposals were accepted.

text: The Jovilabe is certainly connected to

text: Galileo

text: 's efforts to determine the

text: orbital period

text: s of

text: Jupiter's moons

text: , whose discovery he announced in 1610 in

text: Sidereus Nuncius

text: , and to compute the times of their

text: eclipse

text: s. Galileo immediately realized that

text: eclipse

text: s of

text: Jupiter

text: 's moons could provide a precise method to determine

text: longitude

text: . The instrument is engraved with tables showing the mean motions of each of the four moons. Two connected disks of different diameters are rotated by means of a movable rod. They are used to create a "view from the

text: Sun

text: " of the movements of Jupiter's moons observed from the

text: Earth

text: (movements that seem irregular because of the

text: heliocentric

text: motions of the Earth and Jupiter). Galileo began the systematic study of the periods of Jupiter's moons in 1611, developing a

text: micrometer

text: for the purpose. He compiled tables of the periods that he offered, with his

text: telescope

text: s, first to the King of Spain (1611, 1612, 1616, and 1627-1628), then to the States General of Holland (1637-1641). To convince his Spanish interlocutors that Jupiter and its moons could be observed on unstable ground, such as a ship's deck, Galileo designed a special helmet carrying a small telescope on a hinged mount. The device was named the

text: celatone

text: (celata = "helmet" in Italian). In this second proposal, he also described the advantages of applying the

text: pendulum

text: to the

text: clock

text: . Despite the interest they aroused, neither of his proposals were accepted.

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answers: 1: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: eclipses

answers: NDQ_002324

answers: the Earth and Jupiter

answers: NDQ_002325

answers: eclipses

answers: NDQ_002326

answers: eclipses

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: eclipses

answers: NDQ_002329

answers: four moons

answers: NDQ_002330

answers: the Earth

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: Jovilabe

answers: NDQ_002334

answers: the Earth

answers: NDQ_002335

answers: eclipses

answers: NDQ_002343

answers: The Jovilabe

answers: NDQ_002345

answers: Two connected disks of different diameters are rotated by means of a movable rod

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Jovilabe

answers: NDQ_002351

answers: Galileo began the systematic study of the periods of Jupiter's moons

answers: NDQ_002352

answers: Jupiter's moons

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Jupiter's moons could provide a precise method to determine longitude

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: It is impossible to say

answers: NDQ_002357

answers: eclipses

answers: NDQ_002358

answers: the first quarter phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: The Jovilabe

answers: NDQ_002361

answers: Jupiter's moons

answers: NDQ_002362

answers: heliocentric motions

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Sun

answers: NDQ_002365

answers: times

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1611

answers: NDQ_002368

answers: eclipses

text: When the Moon, as seen from Earth, is a narrow crescent, the Earth as seen from the Moon is almost fully lit by the Sun. Often, the part of the Moon that is not directly lit by the Sun is sufficiently brightly lit by light reflected from the Earth to be easily visible from Earth. This phenomenon is called "earthshine", and is sometimes picturesquely described as "the old moon in the new moon's arms" or, as pictured here, "the new moon in the old moon's arms".

text: When the Moon, as seen from Earth, is a narrow crescent, the Earth as seen from the Moon is almost fully lit by the Sun. Often, the part of the Moon that is not directly lit by the Sun is sufficiently brightly lit by light reflected from the Earth to be easily visible from Earth. This phenomenon is called "

text: earthshine

text: ", and is sometimes picturesquely described as "the old moon in the new moon's arms" or, as pictured here, "the new moon in the old moon's arms".

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answers: crescent

answers: NDQ_002324

answers: the old moon in the new moon's arms

answers: NDQ_002325

answers: crescent

answers: NDQ_002326

answers: narrow crescent

answers: NDQ_002327

answers: Earthshine

answers: NDQ_002328

answers: a narrow crescent

answers: NDQ_002329

answers: When the Moon, as seen from Earth, is a narrow crescent

answers: NDQ_002330

answers: is a narrow crescent

answers: NDQ_002331

answers: Earthshine

answers: NDQ_002332

answers: narrow crescent

answers: NDQ_002334

answers: the part of the Moon that is not directly lit by the Sun

answers: NDQ_002335

answers: crescent

answers: NDQ_002343

answers: It generally lasts between 5-10 minutes

answers: NDQ_002345

answers: Earthshine

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The part of the Moon that is not directly lit by the Sun

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: part of the Moon that is not directly lit by the Sun

answers: NDQ_002353

answers: The part of the Moon that is not directly lit by the Sun

answers: NDQ_002354

answers: The Moon, as seen from Earth, is a narrow crescent

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: It occurs once every month.

answers: NDQ_002357

answers: When the Moon, as seen from Earth, is a narrow crescent

answers: NDQ_002358

answers: The crescent phase

answers: NDQ_002359

answers: The full moon will occur on the 28th

answers: NDQ_002360

answers: The part of the Moon that is not directly lit by the Sun

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: Earthshine

answers: NDQ_002363

answers: Earth as seen from the Moon

answers: NDQ_002364

answers: Earth as seen from the Moon is almost fully lit by the Sun

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: crescent

answers: NDQ_002368

answers: narrow crescent

text: An annular solar eclipse will occur on October 3, 2043. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on October 3, 2043. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: obscuring the image of the Sun

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: (ring)

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: It will occur on October 3, 2043

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On October 3, 2043

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: October

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: 2043

answers: NDQ_002367

answers: 2043

answers: NDQ_002368

answers: crescent

text: This is a list of solar eclipses in the 20th century. During the period 1901 to 2000 there were 228 solar eclipses of which 78 were partial, 73 were annular (two non-central), 71 were total (three non-central) and 6 were hybrids. The greatest number of eclipses in one year was five, in 1935, and one month, July 2000, had two eclipses.

text: This is a list of solar eclipses in the 20th century. During the period 1901 to 2000 there were 228 solar eclipses of which 78 were partial, 73 were annular (two

text: non-central

text: ), 71 were total (three non-central) and 6 were hybrids. The greatest number of eclipses in one year was five, in 1935, and one month, July 2000, had two eclipses.

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answers: There were 228 solar eclipses

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answers: partial lunar eclipse

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answers: July 2000

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text: A total solar eclipse will occur on April 9, 2043. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.It will be unusual in that while it is a total solar eclipse, it is not a central solar eclipse.

text: A total

text: solar eclipse

text: will occur on April 9, 2043. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's

text: apparent diameter

text: is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.It will be unusual in that while it is a total solar eclipse, it is not a central solar eclipse.

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answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon's apparent diameter is larger than the Sun's

answers: NDQ_002350

answers: total solar eclipse

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

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answers: NDQ_002353

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answers: NDQ_002354

answers: It will be unusual

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On April 9, 2043

answers: NDQ_002357

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answers: NDQ_002358

answers: A crescent phase

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text: The approximate age of the moon, and hence the approximate phase, can be calculated for any date by calculating the number of days since a known new moon (such as January 1, 1900 or August 11, 1999) and reducing this modulo 29.530588853 (the length of a synodic month). The difference between two dates can be calculated by subtracting the Julian Day Number of one from that of the other, or there are simpler formulae giving (for instance) the number of days since December 31, 1899. However, this calculation assumes a perfectly circular orbit and makes no allowance for the time of day at which the new moon happened, therefore may be incorrect by several hours (it also becomes less accurate the larger the difference between the required date and the reference date); it is accurate enough to use in a novelty clock application showing moon phase, but specialist usage taking account of lunar apogee and perigee requires a more elaborate calculation.

text: The approximate age of the moon, and hence the approximate phase, can be calculated for any date by calculating the number of days since a known new moon (such as January 1, 1900 or August 11, 1999) and reducing this

text: modulo

text: 29.530588853 (the length of a synodic month). The difference between two dates can be calculated by subtracting the

text: Julian Day Number

text: of one from that of the other, or there are simpler formulae giving (for instance) the number of days since December 31, 1899. However, this calculation assumes a perfectly circular orbit and makes no allowance for the time of day at which the new moon happened, therefore may be incorrect by several hours (it also becomes less accurate the larger the difference between the required date and the reference date); it is accurate enough to use in a novelty clock application showing moon phase, but specialist usage taking account of lunar apogee and perigee requires a more elaborate calculation.

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answers: NDQ_002324

answers: perigee

answers: NDQ_002325

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answers: NDQ_002326

answers: approximate

answers: NDQ_002327

answers: new moon

answers: NDQ_002328

answers: perigee

answers: NDQ_002329

answers: the length of a synodic month

answers: NDQ_002330

answers: perigee

answers: NDQ_002331

answers: new moon

answers: NDQ_002332

answers: phase

answers: NDQ_002334

answers: apogee

answers: NDQ_002335

answers: new moon

answers: NDQ_002343

answers: may be incorrect by several hours

answers: NDQ_002345

answers: the length of a synodic month

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Julian Day Number

answers: NDQ_002351

answers: 29.530588853

answers: NDQ_002352

answers: perigee

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: It is accurate enough to use in a novelty clock application showing moon phase

answers: NDQ_002355

answers: The approximate age of the moon

answers: NDQ_002356

answers: 29.530588853

answers: NDQ_002357

answers: apogee

answers: NDQ_002358

answers: first quarter phase

answers: NDQ_002359

answers: 29.530588853

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: a perfectly circular orbit

answers: NDQ_002363

answers: orbit

answers: NDQ_002364

answers: time of day

answers: NDQ_002365

answers: several hours

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: 29.530588853

answers: NDQ_002368

answers: new moon

text: The Warlpiri people explain a solar eclipse as being the Sun-woman being hidden by the Moon-man as he makes love to her. This explanation is shared by other groups, such as the Wirangu.

text: The

text: Warlpiri people

text: explain a

text: solar eclipse

text: as being the Sun-woman being hidden by the Moon-man as he makes love to her. This explanation is shared by other groups, such as the

text: Wirangu

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answers: 2

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answers: 4

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answers: 0

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answers: 0

answers: NDQ_002323

answers: 0

answers: NDQ_002324

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answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 4

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 4

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: lunar eclipse

answers: NDQ_002324

answers: Moon-man

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: solar eclipse

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: half moon

answers: NDQ_002330

answers: Sun-woman

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: Sun-woman

answers: NDQ_002335

answers: solar eclipse

answers: NDQ_002343

answers: Lunar eclipse

answers: NDQ_002345

answers: Moon-man

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: solar eclipse

answers: NDQ_002351

answers: Moon-man

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Solar eclipses are rare

answers: NDQ_002355

answers: Partially lunar

answers: NDQ_002356

answers: lunar eclipse

answers: NDQ_002357

answers: solar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the full moon

answers: NDQ_002360

answers: Moon-man

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Moon

answers: NDQ_002364

answers: Sun-woman being hidden by the Moon

answers: NDQ_002365

answers: a solar eclipse

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: one month

answers: NDQ_002368

answers: lunar eclipse

text: A partial solar eclipse occurred on March 28, 1968. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on March 28, 1968. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002363

answers: 0

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answers: 5

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answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: Moon passes between Earth and the Sun

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: Moon passes between Earth and the Sun

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on March 28, 1968

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: March 28, 1968

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: March 28

answers: NDQ_002360

answers: The Sun

answers: NDQ_002361

answers: completely or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial solar eclipse

text: While amateur observers were unable to detect transmissions from the lander, Chinese officials reported that the craft was still operating its UV Camera and Telescope as it entered its 14th lunar night on 14 January 2015. On 18 April 2014, Wang Jianyu, deputy secretary general of the Chinese Society of Space Research stated that the failure was not mechanical, but electrical, and they were looking to bypass it. He also explained, "The temperature on the Moon is considerably lower than our previous estimation, adding that "certain components may be suffering from "frostbite". During 15 April, the Chang'e 3 mission, including its Yutu rover, witnessed a total eclipse of the Sun by the Earth from surface of the Moon.

text: While amateur observers were unable to detect transmissions from the lander, Chinese officials reported that the craft was still operating its UV Camera and Telescope as it entered its 14th lunar night on 14 January 2015. On 18 April 2014, Wang Jianyu, deputy secretary general of the Chinese Society of Space Research stated that the failure was not mechanical, but electrical, and they were looking to bypass it. He also explained, "The temperature on the Moon is considerably lower than our previous estimation, adding that "certain components may be suffering from "frostbite". During 15 April, the Chang'e 3 mission, including its Yutu rover, witnessed a

text: total eclipse of the Sun

text: by the Earth from surface of the Moon.

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text: In representations of the Solar System, it is common to draw the trajectory of Earth from the point of view of the Sun, and the trajectory of the Moon from the point of view of Earth. This could give the impression that the Moon orbits Earth in such a way that sometimes it goes backwards when viewed from the Sun's perspective. Because the orbital velocity of the Moon around Earth (1 km/s) is small compared to the orbital velocity of Earth about the Sun (30 km/s), this never happens. There are no rearward loops in the Moon's solar orbit.

text: In representations of the

text: Solar System

text: , it is common to draw the trajectory of Earth from the point of view of the Sun, and the trajectory of the Moon from the point of view of Earth. This could give the impression that the Moon orbits Earth in such a way that sometimes it goes backwards when viewed from the Sun's perspective. Because the orbital velocity of the Moon around Earth (1 km/s) is small compared to the orbital velocity of Earth about the Sun (30 km/s), this never happens. There are no rearward loops in the Moon's solar orbit.

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text: None of Jupiter's moons have more than traces of atmosphere, so their skies are black or very nearly so. For an observer on one of the moons, the most prominent feature of the sky by far would be Jupiter. For an observer on Io, the closest large moon to the planet, Jupiter's apparent diameter would be about 20° (38 times the visible diameter of the Moon, covering 1% of Io's sky). An observer on Metis, the innermost moon, would see Jupiter's apparent diameter increased to 68° (130 times the visible diameter of the Moon, covering 18% of Metis's sky). A "full Jupiter" over Metis shines with about 4% of the Sun's brightness (light on Earth from a full moon is 400 thousand times dimmer than sunlight).

text: None of Jupiter's moons have more than traces of atmosphere, so their skies are black or very nearly so. For an observer on one of the moons, the most prominent feature of the sky by far would be Jupiter. For an observer on

text: Io

text: , the closest large moon to the planet, Jupiter's apparent diameter would be about 20° (38 times the visible diameter of the Moon, covering 1% of Io's sky). An observer on

text: Metis

text: , the innermost moon, would see Jupiter's apparent diameter increased to 68° (130 times the visible diameter of the Moon, covering 18% of Metis's sky). A "full Jupiter" over Metis shines with about 4% of the Sun's brightness (light on Earth from a full moon is 400 thousand times dimmer than sunlight).

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answers: NDQ_002325

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answers: 3

answers: NDQ_002327

answers: 0

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answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 5

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

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answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 0

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 0

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answers: 0

answers: NDQ_002358

answers: 4

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answers: 4

answers: NDQ_002360

answers: 0

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answers: 0

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answers: 4

answers: NDQ_002367

answers: 0

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answers: 0

answers: NDQ_002323

answers: full

answers: NDQ_002324

answers: Jupiter and Metis

answers: NDQ_002325

answers: full

answers: NDQ_002326

answers: full

answers: NDQ_002327

answers: full moon

answers: NDQ_002328

answers: A "full Jupiter" over Metis

answers: NDQ_002329

answers: about 4%

answers: NDQ_002330

answers: Metis

answers: NDQ_002331

answers: full moon

answers: NDQ_002332

answers: full

answers: NDQ_002334

answers: Metis

answers: NDQ_002335

answers: full

answers: NDQ_002343

answers: an observer on one of the moons

answers: NDQ_002345

answers: Jupiter's apparent diameter increased to 68°

answers: NDQ_002348

answers: The moon is entirely dark.

answers: NDQ_002350

answers: light on Earth from a full moon is 400 thousand times dimmer than sunlight

answers: NDQ_002351

answers: A "full Jupiter" over Metis shines with about 4% of the Sun's brightness

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow

answers: NDQ_002354

answers: None of Jupiter's moons have more than traces of atmosphere, so their skies are black

answers: NDQ_002355

answers: Part of the Moon

answers: NDQ_002356

answers: Metis

answers: NDQ_002357

answers: A "full Jupiter" over Metis

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: full moon is 400 thousand times dimmer than sunlight

answers: NDQ_002361

answers: light on Earth from a full moon

answers: NDQ_002362

answers: light on Earth from a full moon

answers: NDQ_002363

answers: sky

answers: NDQ_002364

answers: the Sun's brightness

answers: NDQ_002365

answers: about 4%

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: new moon

text: The Moon makes a complete orbit around Earth with respect to the fixed stars about once every 27.3 days (its sidereal period). However, because Earth is moving in its orbit around the Sun at the same time, it takes slightly longer for the Moon to show the same phase to Earth, which is about 29.5 days (its synodic period). Unlike most satellites of other planets, the Moon orbits closer to the ecliptic plane than to the planet's equatorial plane. The Moon's orbit is subtly perturbed by the Sun and Earth in many small, complex and interacting ways. For example, the plane of the Moon's orbital motion gradually rotates, which affects other aspects of lunar motion. These follow-on effects are mathematically described by Cassini's laws.

text: The Moon makes a complete orbit around Earth with respect to the fixed stars about once every 27.3 days (its

text: sidereal period

text: ). However, because Earth is moving in its orbit around the Sun at the same time, it takes slightly longer for the Moon to show the same

text: phase

text: to Earth, which is about 29.5 days (its

text: synodic period

text: ). Unlike most satellites of other planets, the Moon orbits closer to the

text: ecliptic plane

text: than to the planet's

text: equatorial plane

text: . The Moon's orbit is subtly

text: perturbed

text: by the Sun and Earth in many small, complex and interacting ways. For example, the plane of the Moon's orbital motion

text: gradually rotates

text: , which affects other aspects of lunar motion. These follow-on effects are mathematically described by

text: Cassini's laws

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answers: 2

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answers: 4

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answers: 5

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 2

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answers: 5

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answers: 2

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answers: 4

answers: NDQ_002323

answers: sidereal

answers: NDQ_002324

answers: ecliptic plane

answers: NDQ_002325

answers: sidereal

answers: NDQ_002326

answers: right side

answers: NDQ_002327

answers: sidereal period

answers: NDQ_002328

answers: its synodic period

answers: NDQ_002329

answers: 27.3 days

answers: NDQ_002330

answers: ecliptic plane

answers: NDQ_002331

answers: show the same phase

answers: NDQ_002332

answers: synodic period

answers: NDQ_002334

answers: ecliptic plane

answers: NDQ_002335

answers: sidereal

answers: NDQ_002343

answers: It takes slightly longer for the Moon to show the same phase

answers: NDQ_002345

answers: The Moon orbits closer to the ecliptic plane than to the planet's equatorial plane

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Moon orbits closer to the ecliptic plane

answers: NDQ_002351

answers: its synodic period

answers: NDQ_002352

answers: Moon orbits closer to the ecliptic plane

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Moon makes a complete orbit around Earth with respect to the fixed stars about once every 27.3 days

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: 27.3 days

answers: NDQ_002357

answers: sidereal period

answers: NDQ_002358

answers: sidereal period

answers: NDQ_002359

answers: 27.3 days

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: Earth is moving in its orbit around the Sun

answers: NDQ_002362

answers: the plane of the Moon's orbital motion gradually rotates, which affects other aspects of lunar motion

answers: NDQ_002363

answers: ecliptic plane

answers: NDQ_002364

answers: Earth is moving in its orbit around the Sun at the same time

answers: NDQ_002365

answers: 27.3 days

answers: NDQ_002366

answers: 27.3 days

answers: NDQ_002367

answers: 29.5 days

answers: NDQ_002368

answers: its synodic period

text: Constructions like those in Newton's diagram can be repeated for many different positions of the Moon in its orbit. For each position, the result is a perturbation vector like LS1 or LS2 in the second diagram. Shown here is an often-presented form of the diagram that summarises sizes and directions of the perturbation vectors for many different positions of the Moon in its orbit. Each small arrow is a perturbation vector like LS, applicable to the Moon in the particular position around the orbit from which the arrow begins. The perturbations on the Moon when it is nearly in line along the Earth-Sun axis, i.e. near new or full moon, point outwards, away from the Earth. When the Moon-Earth line is 90° from the Earth-Sun axis they point inwards, towards the Earth, with a size that is only half the maximum size of the axial (outwards) perturbations. (Newton gave a rather good quantitative estimate for the size of the solar perturbing force: at quadrature where it adds to the Earth's attraction he put it at 1/178.725 of the mean terrestrial attraction, and twice as much as that at the new and full moons where it opposes and diminishes the Earth's attraction.)

text: quadrature

text: where it adds to the Earth's attraction he put it at 1/178.725 of the mean terrestrial attraction, and twice as much as that at the new and full moons where it opposes and diminishes the Earth's attraction.)

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answers: 0

answers: NDQ_002323

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answers: 3

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answers: 0

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answers: 0

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 4

answers: NDQ_002334

answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 4

answers: NDQ_002352

answers: 0

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answers: 0

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answers: 0

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answers: 4

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answers: 0

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answers: 4

answers: NDQ_002358

answers: 0

answers: NDQ_002359

answers: 4

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answers: 0

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answers: 4

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answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: full moon

answers: NDQ_002324

answers: full moon, point outwards, away from the Earth

answers: NDQ_002325

answers: full moon

answers: NDQ_002326

answers: full

answers: NDQ_002327

answers: new or full moon

answers: NDQ_002328

answers: diminishes the Earth's attraction

answers: NDQ_002329

answers: quadrature

answers: NDQ_002330

answers: Earth-Sun axis

answers: NDQ_002331

answers: new or full moon

answers: NDQ_002332

answers: full moon

answers: NDQ_002334

answers: the Earth-Sun axis

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: Moon-Earth line is 90°

answers: NDQ_002345

answers: The perturbations on the Moon

answers: NDQ_002348

answers: Moon-Earth line is 90° from the Earth-Sun axis

answers: NDQ_002350

answers: Earth-Sun axis

answers: NDQ_002351

answers: full moons

answers: NDQ_002352

answers: The penumbra

answers: NDQ_002353

answers: When the Moon-Earth line is 90°

answers: NDQ_002354

answers: It adds to the Earth's attraction

answers: NDQ_002355

answers: Moon-Earth line is 90°

answers: NDQ_002356

answers: full moons

answers: NDQ_002357

answers: when it is nearly in line along the Earth-Sun axis

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text: The astronomical phenomena of the solar eclipse and lunar eclipse had been observed in the 4th century BC by astronomers Gan De and Shi Shen; the latter gave instructions on predicting the eclipses based on the relative position of the Moon to the Sun. The philosopher Wang Chong argued against the 'radiating influence' theory of Jing Fang's writing in the 1st century BC and that of Zhang Heng (78–139); the latter two correctly hypothesized that the brightness of the Moon was merely light reflected from the Sun. Jing Fang had written in the 1st century BC of how it was long accepted in China that the Sun and Moon were spherical in shape ('like a crossbow bullet'), not flat. Shen Kuo also wrote of solar and lunar eclipses in this manner, yet expanded upon this to explain why the celestial bodies were spherical, going against the 'flat earth' theory for celestial bodies. However, there is no evidence to suggest that Shen Kuo supported a round earth theory, which was introduced into Chinese science by Matteo Ricci and Xu Guangqi in the 17th century. When the Director of the Astronomical Observatory asked Shen Kuo if the shapes of the Sun and Moon were round like balls or flat like fans, Shen Kuo explained that celestial bodies were spherical because of knowledge of waxing and waning of the Moon. Much like what Zhang Heng had said, Shen Kuo likened the Moon to a ball of silver, which does not produce light, but simply reflects light if provided from another source (the Sun). He explained that when the Sun's light is slanting, the Moon appears full. He then explained if one were to cover any sort of sphere with white powder, and then viewed from the side it would appear to be a crescent, hence he reasoned that celestial bodies were spherical. He also wrote that, although the Sun and Moon were in conjunction and opposition with each other once a month, this did not mean the Sun would be eclipsed every time their paths met, because of the small obliquity of their orbital paths.

text: The astronomical phenomena of the

text: solar eclipse

text: and

text: lunar eclipse

text: had been observed in the 4th century BC by astronomers

text: Gan De

text: and

text: Shi Shen

text: ; the latter gave instructions on predicting the eclipses based on the relative position of the Moon to the Sun. The philosopher Wang Chong argued against the 'radiating influence' theory of

text: Jing Fang

text: 's writing in the 1st century BC and that of

text: Zhang Heng

text: (78–139); the latter two correctly hypothesized that the brightness of the Moon was merely light reflected from the Sun. Jing Fang had written in the 1st century BC of how it was long accepted in China that the Sun and Moon were

text: spherical

text: in shape ('like a

text: crossbow

text: bullet'), not flat. Shen Kuo also wrote of solar and lunar eclipses in this manner, yet expanded upon this to explain why the celestial bodies were spherical, going against the '

text: flat earth

text: ' theory for celestial bodies. However, there is no evidence to suggest that Shen Kuo supported a round earth theory, which was introduced into Chinese science by

text: Matteo Ricci

text: and

text: Xu Guangqi

text: in the 17th century. When the Director of the Astronomical

text: Observatory

text: asked Shen Kuo if the shapes of the Sun and Moon were round like balls or flat like fans, Shen Kuo explained that celestial bodies were spherical because of knowledge of waxing and waning of the Moon. Much like what Zhang Heng had said, Shen Kuo likened the Moon to a ball of silver, which does not produce light, but simply reflects light if provided from another source (the Sun). He explained that when the Sun's light is slanting, the Moon appears full. He then explained if one were to cover any sort of sphere with white powder, and then viewed from the side it would appear to be a crescent, hence he reasoned that celestial bodies were spherical. He also wrote that, although the Sun and Moon were in conjunction and opposition with each other once a month, this did not mean the Sun would be eclipsed every time their paths met, because of the small obliquity of their orbital paths.

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text: A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.This was the first of four partial solar eclipses in 2011, with the others occurring on June 1, 2011, July 1, 2011, and November 25, 2011.

text: A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.This was the first of four partial solar eclipses in 2011, with the others occurring on

text: June 1, 2011

text: July 1, 2011

text: , and

text: November 25, 2011

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text: Book III covers the mediaeval Quadrivium, the four subjects which supplemented the Trivium being mathematics, geometry, music and astronomy. He argues that there are infinitely many numbers, as you can always add one (or any other number) to whatever number you think is the limit. He attributes geometry to Ancient Egypt, arguing that because the River Nile flooded and covered the land with mud, geometry was needed to mark out people's land "with lines and measures". Isidore distinguishes astronomy from astrology, and covers the world, the sky and the celestial sphere, the zodiac, the sun, moon, stars, Milky Way, planets and the names of the stars. He derives the curved (curvus) vault of the heavens from the Latin word for "upside-down" (conversus). He explains eclipses of the sun as the moon coming between the earth and the sun, and eclipses of the moon as happening when it runs into the shadow of the earth. He condemns the Roman naming of the planets after their gods: Jupiter, Saturn, Mars, Venus, and Mercury.

text: Book III covers the mediaeval

text: Quadrivium

text: , the four subjects which supplemented the Trivium being

text: mathematics

text: geometry

text: music

text: and

text: astronomy

text: . He argues that there are infinitely many numbers, as you can always add one (or any other number) to whatever number you think is the limit. He attributes geometry to

text: Ancient Egypt

text: , arguing that because the

text: River Nile

text: flooded and covered the land with mud, geometry was needed to mark out people's land "with lines and measures". Isidore distinguishes astronomy from

text: astrology

text: , and covers the world, the sky and the celestial sphere, the

text: zodiac

text: , the sun, moon, stars,

text: Milky Way

text: , planets and the names of the stars. He derives the curved (curvus) vault of the heavens from the Latin word for "upside-down" (conversus). He explains eclipses of the sun as the moon coming between the earth and the sun, and eclipses of the moon as happening when it runs into the shadow of the earth. He condemns the Roman naming of the planets after their gods: Jupiter, Saturn, Mars, Venus, and Mercury.

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answers: NDQ_002367

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answers: NDQ_002368

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answers: NDQ_002323

answers: eclipses

answers: NDQ_002324

answers: the sun

answers: NDQ_002325

answers: eclipses

answers: NDQ_002326

answers: eclipses

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: eclipses

answers: NDQ_002329

answers: add one

answers: NDQ_002330

answers: earth

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: shadow

answers: NDQ_002334

answers: the earth

answers: NDQ_002335

answers: eclipses

answers: NDQ_002343

answers: eclipses of the moon

answers: NDQ_002345

answers: the moon coming between the earth and the sun

answers: NDQ_002348

answers: when it runs into the shadow of the earth

answers: NDQ_002350

answers: shadow of the earth

answers: NDQ_002351

answers: moon

answers: NDQ_002352

answers: shadow of the earth

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: He explains eclipses of the sun as the moon coming between the earth and the sun

answers: NDQ_002355

answers: eclipses of the moon

answers: NDQ_002356

answers: eclipses of the moon

answers: NDQ_002357

answers: eclipses

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: when it runs into the shadow of the earth

answers: NDQ_002361

answers: the moon coming between the earth and the sun

answers: NDQ_002362

answers: eclipses of the sun

answers: NDQ_002363

answers: the Milky Way

answers: NDQ_002364

answers: moon coming between the earth and the sun

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: one

answers: NDQ_002368

answers: eclipses

text: In the photograph of the Brescia clock above, the triangle, square, and star in the center of the dial show these aspects (the third, fourth, and sixth phases) of (presumably) the moon.

text: In the photograph of the Brescia clock above, the triangle, square, and star in the center of the dial show these aspects (the third, fourth, and sixth phases) of (presumably) the moon.

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answers: fourth

answers: NDQ_002324

answers: fourth, and sixth phases

answers: NDQ_002325

answers: sixth

answers: NDQ_002326

answers: fourth

answers: NDQ_002327

answers: phases

answers: NDQ_002328

answers: phases

answers: NDQ_002329

answers: fourth

answers: NDQ_002330

answers: center of the dial

answers: NDQ_002331

answers: phases

answers: NDQ_002332

answers: sixth phases

answers: NDQ_002334

answers: fourth, and sixth phases

answers: NDQ_002335

answers: sixth

answers: NDQ_002343

answers: (presumably) the moon

answers: NDQ_002345

answers: (presumably) the moon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: (presumably)

answers: NDQ_002351

answers: sixth phases

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: (presumably) the moon

answers: NDQ_002354

answers: (presumably) the moon

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: (presumably)

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: fourth

answers: NDQ_002359

answers: the sixth phase

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: phases

answers: NDQ_002363

answers: phase

answers: NDQ_002364

answers: (presumably) the moon

answers: NDQ_002365

answers: sixth phases

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: sixth

answers: NDQ_002368

answers: fourth

text: The Blue Moon is covered in life-giving water and an atmosphere so dense that enormous creatures hypothetically can take flight. The Blue Moon orbits a Water Cloud Jovian planet (a Jupiter-like planet that is cool enough to have visible rain clouds in its atmosphere) orbiting a close binary star system. The Blue Moon itself is roughly an earth mass but has an air pressure around three times that of Earth's at sea level.

text: The Blue Moon is covered in life-giving water and an

text: atmosphere

text: so dense that enormous creatures hypothetically can take flight. The Blue Moon orbits a

text: Water Cloud Jovian planet

text: (a Jupiter-like planet that is cool enough to have visible rain clouds in its atmosphere) orbiting a close binary star system. The Blue Moon itself is roughly an earth mass but has an air pressure around three times that of Earth's at sea level.

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answers: Blue Moon

answers: NDQ_002324

answers: Blue Moon

answers: NDQ_002325

answers: Blue Moon

answers: NDQ_002326

answers: Blue

answers: NDQ_002327

answers: Blue Moon

answers: NDQ_002328

answers: visible rain clouds

answers: NDQ_002329

answers: roughly an earth mass

answers: NDQ_002330

answers: The Blue Moon

answers: NDQ_002331

answers: Blue Moon

answers: NDQ_002332

answers: Blue Moon

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answers: The Blue Moon

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answers: The Blue Moon

answers: NDQ_002345

answers: The Blue Moon

answers: NDQ_002348

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answers: The Blue Moon

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answers: The Blue Moon

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answers: The Blue Moon

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answers: The Blue Moon

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answers: a close binary star system

answers: NDQ_002363

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answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: three times

answers: NDQ_002368

answers: Blue Moon

text: When the Italian physicist Galileo Galilei first observed the planet in the early 17th century, he found it showed phases like the Moon, varying from crescent to gibbous to full and vice versa. When Venus is furthest from the Sun in the sky, it shows a half-lit phase, and when it is closest to the Sun in the sky, it shows as a crescent or full phase. This could be possible only if Venus orbited the Sun, and this was among the first observations to clearly contradict the Ptolemaic geocentric model that the Solar System was concentric and centred on Earth.

text: When the Italian physicist

text: Galileo Galilei

text: first observed the planet in the early 17th century, he found it showed

text: phases

text: like the Moon, varying from crescent to gibbous to full and vice versa. When Venus is furthest from the Sun in the sky, it shows a

text: half-lit phase

text: , and when it is closest to the Sun in the sky, it shows as a crescent or full phase. This could be possible only if Venus orbited the Sun, and this was among the first observations to clearly contradict the

text: Ptolemaic

text: geocentric model

text: that the Solar System was concentric and centred on Earth.

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answers: gibbous

answers: NDQ_002327

answers: phases

answers: NDQ_002328

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answers: NDQ_002331

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answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002343

answers: When Venus is furthest from the Sun in the sky

answers: NDQ_002345

answers: Venus is furthest from the Sun

answers: NDQ_002348

answers: Venus is furthest

answers: NDQ_002350

answers: When Venus is furthest from the Sun

answers: NDQ_002351

answers: When Venus is furthest from the Sun

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Half-lit

answers: NDQ_002354

answers: Venus is furthest from the Sun in the sky

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: When Venus is furthest from the Sun in the sky

answers: NDQ_002357

answers: When Venus is furthest from the Sun

answers: NDQ_002358

answers: gibbous

answers: NDQ_002359

answers: When Venus is furthest from the Sun in the sky

answers: NDQ_002360

answers: Venus is furthest from the Sun

answers: NDQ_002361

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answers: NDQ_002362

answers: Venus orbited the Sun

answers: NDQ_002363

answers: Solar System

answers: NDQ_002364

answers: When Venus is furthest from the Sun

answers: NDQ_002365

answers: half-lit phase

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: vice versa

answers: NDQ_002368

answers: gibbous

text: "sky, day, god"| Tues-day (< OE Tīwes-dæġ lit. "day of Tīw")| ON tīvar "gods", Týr "Tīw" (the war god)| Iuppiter (Iovis), Old Latin Diū-piter (Diovis) "Jupiter"; diēs "day", deus, dīvus "god"| Zdeús (Di(w)ós) "Zeus"| d(i)yāúḥ (diváḥ, dyōḥ) "heaven", dēváḥ "god"| Av daēva- "demon"| (OCS dĭnĭ (dĭne) "day" < ), Russian divo "miracle"| OPrus deina "day", deiws "god", Lith diena "day", dievas "god"| OIr dīe, W dydd "day"; OIr dia (dē), OW duiu- "God"| tiv "day" Asdovadz  Astwadz "God"  | (gdhinj "I make day"(? mache Tag) < )|||-|  "sun"| sun (< OE sunne)| sauil, sunnō "sun"| sōl "sun"| Homeric hēélios "sun" < *sāwélios| súvar (súraḥ) "sun, light, heavens", sūra-, sūrya "sun"| Av hvarǝ (hūrō) "sun, light, heavens"| OCS slĭnŭce "sun" < *sulnika-, Russian po-solon' "sunwise"| OPrus sauli "sun", sawaiti "week", Lith saulė "sun", savaitė "week"| OIr sūil "eye"; W haul "sun"| Armenian, arev Sun, tsolk reflection, shoghal shine, glare; shogh շող "gleen."| ylli "star" < *sūlo- or *sūli-|||-|  "moon, month"| moon (< OE mōna), month (< OE mōnaþ)| mēna "moon", mēnoþs "month"| mēnsis "month"| Att mḗn, Ion meis, Dor mḗs "month", mḗnē "moon"| mā́s "moon"; mā́sa "month"| Av mā̊ (mā̊ŋhō) "moon"; NPers māh "moon, month"| OCS měsęcĭ "moon, month" < | OPrus miniks "moon", mins "month", Lith mėnulis "moon", mėnesis "month"| OIr mī (mīs) "month" < ;; W mis "month"| amis (amsoy) "month" < | muai "month"| A mañ B meñe "month"; A mañ ñkät B meṃ "moon"||-|  "earth"||| humus "earth"| kʰtʰṓn (kʰtʰonós) "earth", kʰamaí "on the earth"| kṣā́ḥ (acc. kṣā́m, gen. jmáḥ) "earth"| Av zā̊ (acc. ząm, gen. zǝmō) "earth"| OCS zemĭ, zemlja "earth"| OPrus zemê "earth", Lith žemė " earth"| OIr dū "place"; Welsh dyn "man"| degh "place", hogh "earth, soil, land", tsekh "mud, wet soil"| dhe "earth"| A tkaṃ (tkanis), B keṃ "earth"| tēkan (tagnās) "earth"|-|  pl.  "water"| water (< OE wæter)| watō (watins) "water"| Umbrian utur "water", Latin unda "wave"| húdōr (húdatos) "water"| udakám (loc. udán(i), pl. udá), udra "water"| Av aoδa- "spring", vaiδi- "stream"| OCS voda "water", Russian vedro "bucket", | OPrus undan "water", Lith vanduo "water"| OIr u(i)sce "water" < *udeskyo-| get "river" < *wedō, tchur water; terchel to wet| ujë "water"| A wär, B war "water"| wātar (wetenas) "water"|-|  "wood, tree"| tree (< OE trēo)| triu "tree, wood"|| dóru "spear"| dā́ru (drṓs) "wood"| Av dāru- "tree, wood"| OCS drěvo "tree"| OPrus drawê "hole in a tree, hollow tree", Lith drevė "hole in a tree", dirva "soil"| OIr daur "oak", W derwen "oak"| tram "firm",  Western Armenian dzar "tree"| dru "tree"| AB or "wood"| taru "tree"|-|  "wind",  "to blow"| wind (< OE wind); OE wāwan "to blow"| winds "wind"; waian "to blow"| ventus "wind"| áenta (acc.) "wind", áēsi "(he) blows"| vā́taḥ (vānt-) "wind", vāti "(he) blows"| Av vātō "wind", vāiti "(he) blows"| OCS vějǫ (vějetŭ) "to blow"| OPrus witra "wind", Lith vėjas "wind", vėtra "heavy wind"| W gwynt "wind"|  Armenian hov wind|| A want, B yente "wind"| ḫūwanz "wind"|-|  "to snow"| snow (< OE snāw < , snīwan "to snow" < )| snáiws "snow"| nix (nivis) "snow", ninguō (ninguere) "to snow"| nípʰa (acc.) "snow", neípʰei "it snows"| sneha- "snow"| Av snaēža- "to snow"; Shughni žǝnij "snow" < *snaiga-| OCS sněgŭ "snow"| OPrus snaigs "snow", Lith snigti "to snow"| OIr snecht(a)e, W nyf "snow"; OIr snigid "it rains"| W. Armenian, tseun or tsouyn "snow"||||-|  "bonfire"| fire (< OE fȳr < *fuïr)| fōn (funins) "fire"; OHG fuïr (two syllables) < | Umbrian pir "fire" < *pūr, acc. purom-e "into the fire" < *pur-| pũr (purós) "fire"| pāru (pēru) "sun, fire"|| Czech pýř "glowing ash"| OPrus pannu "fire"|| hur (hroy) "fire" < *pū̆r-, hn-oc̣ "furnace" < *pū̆n-|| A por, B puwar, puwār, pwār "fire"| paḫḫur "fire"|-|  "warm"| ?warm (< OE wearm); OE ġierwan "to prepare, cook" < PGerm *garwjan| ?warmjan "to warm"| formus "warm"| tʰermós "warm"| gʰarmáḥ "heat"| Av garǝma- "hot, heat"; OPers Garma-pada-, name of the fourth month, corresponding to June/July, orig. (?) "entrance of the heat"| Russian žar "heat", goret' "to warm" < | OPrus garmê "heat, glowing", Lith žarijos "cinders", žėrėti "to glow"| OIr gorn "fire" < | ǰerm "warm"| Gheg zjarm "fire, heat"| A śärme "heat (of summer)"||-|  "light, brightness"| light (< OE lēoht)| liuhaþ (liuhadis) "light"| lūceō (lūcēre) "to shine", lūx "light"| leukós "bright, shining, white"| rócate "(he) shines", roká- "light", loka- "world, place"| Av raočant- "shining", raočah "light"; OPers raučah "light"| OCS luča "ray, flash" < *loukyā| OPrus lauk "bright", lauksna "star", laukas "field", Lith laukas "outside, field"| OIr luchair "shine"; W llachar "bright", llug "shimmer"| lois (lusoi) "light"|| AB lyuk/luk- "to shine"| luk(k)- "to shine"|-|}

text: "sky, day, god"| Tues-day (<

text: OE

text: Tīwes-dæġ lit. "day of Tīw")|

text: ON

text: tīvar "gods",

text: Týr

text: "Tīw" (the war god)| Iuppiter (Iovis),

text: Old Latin

text: Diū-piter (Diovis) "Jupiter"; diēs "day", deus, dīvus "god"| Zdeús (Di(w)ós) "Zeus"| d(i)yāúḥ (diváḥ, dyōḥ) "heaven", dēváḥ "god"|

text: Av

text: daēva- "demon"| (

text: OCS

text: dĭnĭ (dĭne) "day" < ), Russian divo "miracle"|

text: OPrus

text: deina "day", deiws "god",

text: Lith

text: diena "day", dievas "god"|

text: OIr

text: dīe,

text: W

text: dydd "day";

text: OIr

text: dia (dē),

text: OW

text: duiu- "God"| tiv "day" Asdovadz  Astwadz "God"  | (gdhinj "I make day"(? mache Tag) < )|||-|  "sun"| sun (<

text: OE

text: sunne)| sauil, sunnō "sun"| sōl "sun"|

text: Homeric

text: hēélios "sun" < *sāwélios| súvar (súraḥ) "sun, light, heavens", sūra-, sūrya "sun"|

text: Av

text: hvarǝ (hūrō) "sun, light, heavens"|

text: OCS

text: slĭnŭce "sun" < *sulnika-, Russian po-solon' "sunwise"|

text: OPrus

text: sauli "sun", sawaiti "week",

text: Lith

text: saulė "sun", savaitė "week"|

text: OIr

text: sūil "eye";

text: W

text: haul "sun"| Armenian, arev Sun, tsolk reflection, shoghal shine, glare; shogh շող "gleen."| ylli "star" < *sūlo- or *sūli-|||-|  "moon, month"| moon (<

text: OE

text: mōna), month (<

text: OE

text: mōnaþ)| mēna "moon", mēnoþs "month"| mēnsis "month"|

text: Att

text: mḗn,

text: Ion

text: meis,

text: Dor

text: mḗs "month", mḗnē "moon"| mā́s "moon"; mā́sa "month"|

text: Av

text: mā̊ (mā̊ŋhō) "moon";

text: NPers

text: māh "moon, month"|

text: OCS

text: měsęcĭ "moon, month" < |

text: OPrus

text: miniks "moon", mins "month",

text: Lith

text: mėnulis "moon", mėnesis "month"|

text: OIr

text: mī (mīs) "month" < ;;

text: W

text: mis "month"| amis (amsoy) "month" < | muai "month"| A mañ B meñe "month"; A mañ ñkät B meṃ "moon"||-|  "earth"||| humus "earth"| kʰtʰṓn (kʰtʰonós) "earth", kʰamaí "on the earth"| kṣā́ḥ (acc. kṣā́m, gen. jmáḥ) "earth"|

text: Av

text: zā̊ (acc. ząm, gen. zǝmō) "earth"|

text: OCS

text: zemĭ, zemlja "earth"|

text: OPrus

text: zemê "earth",

text: Lith

text: žemė " earth"|

text: OIr

text: dū "place";

text: Welsh

text: dyn "man"| degh "place", hogh "earth, soil, land", tsekh "mud, wet soil"| dhe "earth"| A tkaṃ (tkanis), B keṃ "earth"| tēkan (tagnās) "earth"|-|  pl.  "water"| water (<

text: OE

text: wæter)| watō (watins) "water"|

text: Umbrian

text: utur "water", Latin unda "wave"| húdōr (húdatos) "water"| udakám (loc. udán(i), pl. udá), udra "water"|

text: Av

text: aoδa- "spring", vaiδi- "stream"|

text: OCS

text: voda "water", Russian vedro "bucket", |

text: OPrus

text: undan "water",

text: Lith

text: vanduo "water"|

text: OIr

text: u(i)sce "water" < *udeskyo-| get "river" < *wedō, tchur water; terchel to wet| ujë "water"| A wär, B war "water"| wātar (wetenas) "water"|-|  "wood, tree"| tree (<

text: OE

text: trēo)| triu "tree, wood"|| dóru "spear"| dā́ru (drṓs) "wood"|

text: Av

text: dāru- "tree, wood"|

text: OCS

text: drěvo "tree"|

text: OPrus

text: drawê "hole in a tree, hollow tree",

text: Lith

text: drevė "hole in a tree", dirva "soil"|

text: OIr

text: daur "oak",

text: W

text: derwen "oak"| tram "firm",  Western Armenian dzar "tree"| dru "tree"| AB or "wood"| taru "tree"|-|  "wind",  "to blow"| wind (<

text: OE

text: wind);

text: OE

text: wāwan "to blow"| winds "wind"; waian "to blow"| ventus "wind"| áenta (acc.) "wind", áēsi "(he) blows"| vā́taḥ (vānt-) "wind", vāti "(he) blows"|

text: Av

text: vātō "wind", vāiti "(he) blows"|

text: OCS

text: vějǫ (vějetŭ) "to blow"|

text: OPrus

text: witra "wind",

text: Lith

text: vėjas "wind", vėtra "heavy wind"|

text: W

text: gwynt "wind"|  Armenian hov wind|| A want, B yente "wind"| ḫūwanz "wind"|-|  "to snow"| snow (<

text: OE

text: snāw < , snīwan "to snow" < )| snáiws "snow"| nix (nivis) "snow", ninguō (ninguere) "to snow"| nípʰa (acc.) "snow", neípʰei "it snows"| sneha- "snow"|

text: Av

text: snaēža- "to snow";

text: Shughni

text: žǝnij "snow" < *snaiga-|

text: OCS

text: sněgŭ "snow"|

text: OPrus

text: snaigs "snow",

text: Lith

text: snigti "to snow"|

text: OIr

text: snecht(a)e,

text: W

text: nyf "snow";

text: OIr

text: snigid "it rains"| W. Armenian, tseun or tsouyn "snow"||||-|  "bonfire"| fire (<

text: OE

text: fȳr < *fuïr)| fōn (funins) "fire";

text: OHG

text: fuïr (two syllables) < |

text: Umbrian

text: pir "fire" < *pūr, acc. purom-e "into the fire" < *pur-| pũr (purós) "fire"| pāru (pēru) "sun, fire"||

text: Czech

text: pýř "glowing ash"|

text: OPrus

text: pannu "fire"|| hur (hroy) "fire" < *pū̆r-, hn-oc̣ "furnace" < *pū̆n-|| A por, B puwar, puwār, pwār "fire"| paḫḫur "fire"|-|  "warm"| ?warm (<

text: OE

text: wearm);

text: OE

text: ġierwan "to prepare, cook" <

text: PGerm

text: *garwjan| ?warmjan "to warm"| formus "warm"| tʰermós "warm"| gʰarmáḥ "heat"|

text: Av

text: garǝma- "hot, heat";

text: OPers

text: Garma-pada-, name of the fourth month, corresponding to June/July, orig. (?) "entrance of the heat"| Russian žar "heat", goret' "to warm" < |

text: OPrus

text: garmê "heat, glowing",

text: Lith

text: žarijos "cinders", žėrėti "to glow"|

text: OIr

text: gorn "fire" < | ǰerm "warm"|

text: Gheg

text: zjarm "fire, heat"| A śärme "heat (of summer)"||-|  "light, brightness"| light (<

text: OE

text: lēoht)| liuhaþ (liuhadis) "light"| lūceō (lūcēre) "to shine", lūx "light"| leukós "bright, shining, white"| rócate "(he) shines", roká- "light", loka- "world, place"|

text: Av

text: raočant- "shining", raočah "light";

text: OPers

text: raučah "light"|

text: OCS

text: luča "ray, flash" < *loukyā|

text: OPrus

text: lauk "bright", lauksna "star", laukas "field",

text: Lith

text: laukas "outside, field"|

text: OIr

text: luchair "shine";

text: W

text: llachar "bright", llug "shimmer"| lois (lusoi) "light"|| AB lyuk/luk- "to shine"| luk(k)- "to shine"|-|}

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answers: tqa2:L_0056/T_0550/5e9f02a00ecf0d2c3cd22178d3938a67

answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 0: The answer is not relevant or complete at all.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracies.

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answers: 3

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answers: 3

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answers: 3

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answers: 0

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answers: 3

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answers: 0

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answers: 0

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answers: 3

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answers: 4

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answers: 0

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answers: 0

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answers: 3

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answers: 0

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answers: 0

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answers: 3

answers: NDQ_002323

answers: Tues-day

answers: NDQ_002324

answers: heavens

answers: NDQ_002325

answers: NDQ_002326

answers: hvar

answers: NDQ_002327

answers: Earth's shadow

answers: NDQ_002328

answers: a new day

answers: NDQ_002329

answers: "sun"

answers: NDQ_002330

answers: NDQ_002331

answers: day

answers: NDQ_002332

answers: sun

answers: NDQ_002334

answers: NDQ_002335

answers: NDQ_002343

answers: A lunar eclipse generally lasts between 5-10 minutes.

answers: NDQ_002345

answers: "sun"| sun

answers: NDQ_002348

answers: During a total lunar eclipse the moon is entirely dark.

answers: NDQ_002350

answers: NDQ_002351

answers: NDQ_002352

answers: NDQ_002353

answers: |||-| "sun"| sun ( OE sunne)| sauil, sunn "sun"| s l "sun"

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: During a partial lunar eclipse, only part of the moon enters Earths umbra.

answers: NDQ_002356

answers: It occurs once every month.

answers: NDQ_002357

answers: The moon is on the opposite side of Earth from the sun.

answers: NDQ_002358

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month.

answers: NDQ_002360

answers: The sun cannot be seen from Earth when a lunar eclipse occurs.

answers: NDQ_002361

answers: The moon cannot be seen from Earth when a solar eclipse occurs.

answers: NDQ_002362

answers: |||-| "sun"| sun ( OE sunne)| sauil, sunn "sun"| s l "sun"| Homeric h élios "sun"  *s wélios| s var (s ra ) "sun, light, heavens", s ra-, s rya "sun"| Av hvar (h r ) "sun, light, heavens"

answers: NDQ_002363

answers: The ecliptic is the celestial ecliptic.

answers: NDQ_002364

answers: "sun"|

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: The moon passes through all of its phases about once every

answers: NDQ_002367

answers: 24 hours

answers: NDQ_002368

answers: Moon phase

text: The Moon is in synchronous rotation with Earth, always showing the same face, with its near side marked by dark volcanic maria that fill the spaces between the bright ancient crustal highlands and the prominent impact craters. It is the second-brightest regularly visible celestial object in Earth's sky, after the Sun, as measured by illuminance on Earth's surface. Its surface is actually dark, although compared to the night sky it appears very bright, with a reflectance just slightly higher than that of worn asphalt. Its prominence in the sky and its regular cycle of phases have made the Moon an important cultural influence since ancient times on language, calendars, art, mythology, and, it is often speculated, the menstrual cycles of the female of the human species.

text: The Moon is in

text: synchronous rotation

text: with Earth, always showing the same face, with its

text: near side

text: marked by dark volcanic

text: maria

text: that fill the spaces between the bright ancient crustal highlands and the prominent

text: impact crater

text: s. It is the second-brightest regularly visible

text: celestial object

text: in Earth's sky, after the Sun, as measured by

text: illuminance

text: on Earth's surface. Its surface is actually dark, although compared to the night sky it appears very bright, with a

text: reflectance

text: just slightly higher than that of worn

text: asphalt

text: . Its prominence in the sky and its regular cycle of

text: phases

text: have made the Moon an important cultural influence since ancient times on

text: language

text: calendar

text: s,

text: art

text: mythology

text: , and, it is often speculated, the menstrual cycles of the female of the human species.

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answers: night

answers: NDQ_002324

answers: highlands and the prominent impact craters

answers: NDQ_002325

answers: night

answers: NDQ_002326

answers: near side

answers: NDQ_002327

answers: synchronous rotation

answers: NDQ_002328

answers: phases

answers: NDQ_002329

answers: phase of phases

answers: NDQ_002330

answers: earth's

answers: NDQ_002331

answers: night

answers: NDQ_002332

answers: The Moon

answers: NDQ_002334

answers: Earth's

answers: NDQ_002335

answers: night

answers: NDQ_002343

answers: Its prominence in the sky and its regular cycle of phases

answers: NDQ_002345

answers: Its surface is actually dark

answers: NDQ_002348

answers: Moon is in synchronous rotation with Earth, always showing the same face

answers: NDQ_002350

answers: The Moon

answers: NDQ_002351

answers: its regular cycle of phases

answers: NDQ_002352

answers: dark volcanic maria

answers: NDQ_002353

answers: The surface is actually dark

answers: NDQ_002354

answers: Earth's sky

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: its regular cycle of phases

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: The Moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: impact craters

answers: NDQ_002363

answers: Earth's

answers: NDQ_002364

answers: Earth's surface

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answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: its regular cycle of phases

answers: NDQ_002368

answers: phase of the moon

text: An annular solar eclipse will occur on February 16, 2045. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on February 16, 2045. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: an annular solar eclipse

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: It will occur on February 16, 2045

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On February 16, 2045

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The Moon passes between Earth and the Sun

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: 2045

answers: NDQ_002367

answers: 2045

answers: NDQ_002368

answers: crescent

text: An annular solar eclipse will occur on October 2, 2024. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on October 2, 2024. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 4

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answers: 4

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answers: 5

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answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: An annular solar eclipse will occur on October 2, 2024

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: (ring)

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: It will occur on October 2, 2024

answers: NDQ_002355

answers: Partially obscuring the image of the Sun

answers: NDQ_002356

answers: On October 2, 2024

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: October 2

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 2024

answers: NDQ_002368

answers: crescent

text: As seen from the Earth, the time it takes for the Moon to return to a node, the draconic month, is less than the time it takes for the Moon to return to the same ecliptic longitude as the Sun: the synodic month. The main reason is that during the time that the Moon has completed an orbit around the Earth, the Earth (and Moon) have completed about  of their orbit around the Sun: the Moon has to make up for this in order to come again into conjunction or opposition with the Sun. Secondly, the orbital nodes of the Moon precess westward in ecliptic longitude, completing a full circle in about  18.60 years, so a draconic month is shorter than a sidereal month. In all, the difference in period between synodic and draconic month is nearly  days. Likewise, as seen from the Earth, the Sun passes both nodes as it moves along its ecliptic path. The period for the Sun to return to a node is called the eclipse or draconic year: about 346.6201 d, which is about  year shorter than a sidereal year because of the precession of the nodes.

text: As seen from the Earth, the time it takes for the Moon to return to a node, the

text: draconic month

text: , is less than the time it takes for the Moon to return to the same ecliptic longitude as the Sun: the

text: synodic month

text: . The main reason is that during the time that the Moon has completed an orbit around the Earth, the Earth (and Moon) have completed about  of their orbit around the Sun: the Moon has to make up for this in order to come again into conjunction or opposition with the Sun. Secondly, the orbital nodes of the Moon

text: precess

text: westward in ecliptic longitude, completing a full circle in about  18.60 years, so a draconic month is shorter than a

text: sidereal month

text: . In all, the difference in period between synodic and draconic month is nearly  days. Likewise, as seen from the Earth, the Sun passes both nodes as it moves along its ecliptic path. The period for the Sun to return to a node is called the

text: eclipse or draconic year

text: : about 346.6201 d, which is about  year shorter than a

text: sidereal year

text: because of the precession of the nodes.

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answers: NDQ_002368

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answers: NDQ_002323

answers: opposition

answers: NDQ_002324

answers: opposition with the Sun

answers: NDQ_002325

answers: opposition

answers: NDQ_002326

answers: opposition

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: opposition

answers: NDQ_002329

answers: a draconic month

answers: NDQ_002330

answers: opposition

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: opposition

answers: NDQ_002334

answers: opposition

answers: NDQ_002335

answers: opposition

answers: NDQ_002343

answers: The difference in period between synodic and draconic month is nearly days

answers: NDQ_002345

answers: the time it takes for the Moon to return to a node

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: nodes

answers: NDQ_002351

answers: Synodic month

answers: NDQ_002352

answers: Moon has to make up for this in order to come again into conjunction

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: about year shorter than a sidereal year because of the precession of the nodes

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: Synodic month

answers: NDQ_002357

answers: opposition

answers: NDQ_002358

answers: Synodic month

answers: NDQ_002359

answers: Synodic month

answers: NDQ_002360

answers: Moon has to make up for this in order to come again into conjunction or opposition with the Sun

answers: NDQ_002361

answers: nodes

answers: NDQ_002362

answers: the Sun passes both nodes as it moves along its ecliptic path

answers: NDQ_002363

answers: longitude

answers: NDQ_002364

answers: opposition with the Sun

answers: NDQ_002365

answers: about year

answers: NDQ_002366

answers: year

answers: NDQ_002367

answers: nearly days

answers: NDQ_002368

answers: opposition

text: This is a list of solar eclipses in the 10th century BC. During the period 1000 to 901 BC there were 226 solar eclipses of which 84 were Partial, 75 were Annular (one non-central), 61 were Total (three non-central), and 6 were hybrids. The greatest number of eclipses in one year was four, occurring in 5 different years: 996 BC, 960 BC, 949 BC, 931 BC, and 913 BC.

text: This is a list of

text: solar eclipses

text: in the 10th century BC. During the period 1000 to 901 BC there were 226 solar eclipses of which 84 were

text: Partial

text: , 75 were

text: Annular

text: (one

text: non-central

text: ), 61 were

text: Total

text: (three non-central), and 6 were hybrids. The greatest number of eclipses in one year was four, occurring in 5 different years: 996 BC, 960 BC, 949 BC, 931 BC, and 913 BC.

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answers: NDQ_002329

answers: Annular

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answers: solar eclipse

answers: NDQ_002332

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answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Partial

answers: NDQ_002351

answers: Partial

answers: NDQ_002352

answers: Annular

answers: NDQ_002353

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answers: The greatest number of eclipses in one year was four

answers: NDQ_002355

answers: Partial

answers: NDQ_002356

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answers: NDQ_002357

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answers: NDQ_002358

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answers: Annular

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answers: NDQ_002365

answers: three non-central

answers: NDQ_002366

answers: 996 BC

answers: NDQ_002367

answers: 960 BC

answers: NDQ_002368

answers: Annular

text: Set in the year AD 2225, mankind has spread from Earth to inhabit nearly all the planets or nearby moons in colonies and settlements. Space travel has grown and improved to the point of being commonplace. For the inhabitants of the solar system, an astronaut career isn't out of the question, and one of the schools set up to train future space voyagers is the Liebe Delta, a space station positioned somewhere in Earth's orbit. This growth is despite the mysterious phenomenon known as the Geduld, a sea of plasma that suddenly erupted from the sun along the Earth's orbital plane in AD 2137. Stretching from the sun to the edge of the solar system, this area of high temperatures and gravity pressures has never been explained.

text: Set in the year AD 2225, mankind has spread from Earth to inhabit nearly all the planets or nearby moons in colonies and settlements. Space travel has grown and improved to the point of being commonplace. For the inhabitants of the solar system, an astronaut career isn't out of the question, and one of the schools set up to train future space voyagers is the Liebe Delta, a space station positioned somewhere in Earth's orbit. This growth is despite the mysterious phenomenon known as the Geduld, a sea of plasma that suddenly erupted from the sun along the Earth's

text: orbital plane

text: in AD 2137. Stretching from the sun to the edge of the solar system, this area of high temperatures and gravity pressures has never been explained.

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answers: NDQ_002324

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answers: NDQ_002325

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answers: NDQ_002326

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answers: NDQ_002327

answers: set up to train future space voyagers

answers: NDQ_002328

answers: the Geduld

answers: NDQ_002329

answers: nearby moons

answers: NDQ_002330

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answers: NDQ_002331

answers: Earth's orbital plane

answers: NDQ_002332

answers: Earth

answers: NDQ_002334

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answers: NDQ_002335

answers: Moonrise

answers: NDQ_002343

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answers: NDQ_002345

answers: Solar eclipse

answers: NDQ_002348

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answers: NDQ_002350

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answers: NDQ_002351

answers: moons

answers: NDQ_002352

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answers: NDQ_002353

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answers: NDQ_002354

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answers: NDQ_002355

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answers: NDQ_002356

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answers: NDQ_002357

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answers: NDQ_002359

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answers: NDQ_002360

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answers: NDQ_002364

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answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: AD 2225

answers: NDQ_002367

answers: quarter moon

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answers: crescent

text: Although there are two Avestan hymns dedicated to the Moon, she is not a prominent divinity. In both the third Nyaish as well as in the seventh Yasht, the 'moon' more commonly spoken of is the physical moon. In these hymns, the phases of the moon are described at length. Ahura Mazda is described to be the cause of the moon's waxing and waning, and the Amesha Spentas evenly distribute the light of the moon over the earth  (Yasht 7.3, Nyaish 3.5). In Yasht 13.14-16, the Fravashis are said to be responsible for keeping the moon and stars on its appointed course. The sun, moon, and stars revolve around the peak of Hara Berezaiti (Yasht 12.25).

text: Although there are two Avestan hymns dedicated to the Moon, she is not a prominent divinity. In both the third Nyaish as well as in the seventh

text: Yasht

text: , the 'moon' more commonly spoken of is the physical moon. In these hymns, the phases of the moon are described at length.

text: Ahura Mazda

text: is described to be the cause of the moon's waxing and waning, and the

text: Amesha Spenta

text: s evenly distribute the light of the moon over the earth  (Yasht 7.3, Nyaish 3.5). In Yasht 13.14-16, the

text: Fravashi

text: s are said to be responsible for keeping the moon and stars on its appointed course. The sun, moon, and stars revolve around the peak of

text: Hara Berezaiti

text: (Yasht 12.25).

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answers: waxing

answers: NDQ_002324

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answers: NDQ_002325

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answers: NDQ_002326

answers: waxing

answers: NDQ_002327

answers: waxing and waning

answers: NDQ_002328

answers: waxing and waning

answers: NDQ_002329

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answers: NDQ_002330

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answers: NDQ_002331

answers: waxing and waning

answers: NDQ_002332

answers: waxing

answers: NDQ_002334

answers: the Earth

answers: NDQ_002335

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answers: NDQ_002343

answers: It is not a prominent divinity

answers: NDQ_002345

answers: The sun, moon, and stars

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The sun, moon, and stars

answers: NDQ_002351

answers: waxing and waning

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: evenly distribute the light of the moon

answers: NDQ_002354

answers: It is not a prominent divinity

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: It is not a prominent divinity

answers: NDQ_002357

answers: waxing

answers: NDQ_002358

answers: waxing

answers: NDQ_002359

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answers: NDQ_002360

answers: the light of the moon over the earth

answers: NDQ_002361

answers: the sun, moon, and stars

answers: NDQ_002362

answers: the Amesha Spentas evenly distribute the light of the moon over the earth

answers: NDQ_002363

answers: peak of Hara Berezaiti

answers: NDQ_002364

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answers: NDQ_002365

answers: 16

answers: NDQ_002366

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answers: NDQ_002367

answers: 3.5

answers: NDQ_002368

answers: waning

text: An annular solar eclipse will occur on December 16, 2085. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on December 16, 2085. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 0

answers: NDQ_002368

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answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: obscuring the image of the Sun

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: December 16, 2085

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: December 16, 2085

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: December

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: December

answers: NDQ_002367

answers: 2085

answers: NDQ_002368

answers: crescent

text: The key difference between a satellite and a quasi-satellite is that the orbit of a satellite of Earth fundamentally depends on the gravity of the Earth–Moon system, whereas the orbit of a quasi-satellite would negligibly change if Earth and the Moon were suddenly removed because a quasi-satellite is orbiting the Sun on an Earth-like orbit in the vicinity of Earth.

text: The key difference between a satellite and a quasi-satellite is that the orbit of a satellite of Earth fundamentally depends on the gravity of the Earth–Moon system, whereas the orbit of a quasi-satellite would negligibly change if Earth and the Moon were suddenly removed because a quasi-satellite is orbiting the Sun on an Earth-like orbit in the vicinity of Earth.

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answers: NDQ_002323

answers: Moon

answers: NDQ_002324

answers: Moon

answers: NDQ_002325

answers: Earth-Moon system

answers: NDQ_002326

answers: Moon phase

answers: NDQ_002327

answers: Earth–Moon system

answers: NDQ_002328

answers: gravity of the Earth–Moon system

answers: NDQ_002329

answers: Earth–Moon

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: orbit

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: Moon

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: Earth–Moon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth–Moon

answers: NDQ_002351

answers: Earth–Moon system

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Earth–Moon system

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: Moon

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: Moon

answers: NDQ_002359

answers: Earth–Moon system

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: Moon

answers: NDQ_002362

answers: gravity

answers: NDQ_002363

answers: Sun

answers: NDQ_002364

answers: Earth and the Moon are suddenly removed

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: crescent

text: A partial solar eclipse will occur on February 27, 2036. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: will occur on February 27, 2036. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 3

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answers: 5

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answers: 4

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002354

answers: 4

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answers: 3

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answers: 0

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answers: 4

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answers: 4

answers: NDQ_002359

answers: 4

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answers: 0

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answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: February 27, 2036

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: It does not say.

answers: NDQ_002345

answers: The Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse will occur on February 27, 2036

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: February 27, 2036

answers: NDQ_002357

answers: Solar eclipse

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: February 27

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: A solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 2036

answers: NDQ_002368

answers: partial

text: In effect, this means that the "tropical year" on the moon is only 347 days long. This is called the draconic year or eclipse year. The "seasons" on the moon fit into this period. For about half of this draconic year, the sun is north of the lunar equator (but at most 1.543°), and for the other half it is south of the lunar equator. Obviously the effect of these seasons is very minor compared to the difference between lunar night and lunar day. At the poles, there are not days and nights of about 15 earth days, but rather the sun will be "up" for 173 days at a time. "Up" here means that the centre of the sun is above the horizon. The sunrise and sunset at the poles each take about 18 days. These polar sunrises and sunsets occur around the time of eclipses (solar or lunar). For example, at the Solar eclipse of March 9, 2016, the moon was near its descending node, and the sun was near the point in the sky where the equator of the moon crosses the ecliptic. When the sun reached that point, the centre of the sun set at the north pole and rose at the south pole.

text: In effect, this means that the "

text: tropical year

text: " on the moon is only 347 days long. This is called the

text: draconic year

text: or eclipse year. The "seasons" on the moon fit into this period. For about half of this draconic year, the sun is north of the lunar equator (but at most 1.543°), and for the other half it is south of the lunar equator. Obviously the effect of these seasons is very minor compared to the difference between lunar night and lunar day. At the poles, there are not days and nights of about 15 earth days, but rather the sun will be "up" for 173 days at a time. "Up" here means that the centre of the sun is above the horizon. The sunrise and sunset at the poles each take about 18 days. These polar sunrises and sunsets occur around the time of eclipses (solar or lunar). For example, at the

text: Solar eclipse of March 9, 2016

text: , the moon was near its descending node, and the sun was near the point in the sky where the equator of the moon crosses the ecliptic. When the sun reached that point, the centre of the sun set at the north pole and rose at the south pole.

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answers: tropical year

answers: NDQ_002324

answers: north pole and south pole

answers: NDQ_002325

answers: lunar night

answers: NDQ_002326

answers: eclipse

answers: NDQ_002327

answers: Solar eclipse

answers: NDQ_002328

answers: Solar eclipse

answers: NDQ_002329

answers: 347 days long

answers: NDQ_002330

answers: the equator

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: draconic

answers: NDQ_002334

answers: equator

answers: NDQ_002335

answers: solar

answers: NDQ_002343

answers: A lunar eclipse generally lasts between 5-10 minutes

answers: NDQ_002345

answers: The sun will be "up" for 173 days at a time. "Up" here means that the centre of the sun is above the horizon

answers: NDQ_002348

answers: The "tropical year" on the moon is only 347 days

answers: NDQ_002350

answers: The sun will be "up" for 173 days at a time

answers: NDQ_002351

answers: the "tropical year" on the moon

answers: NDQ_002352

answers: The "tropical year" on the moon is only 347 days long. This is called the draconic year or eclipse year

answers: NDQ_002353

answers: "Up" here means that the centre of the sun is above the horizon

answers: NDQ_002354

answers: The sunrise and sunset at the poles each take about 18 days

answers: NDQ_002355

answers: The "tropical year" on the moon is only 347 days

answers: NDQ_002356

answers: It occurs once every month.

answers: NDQ_002357

answers: The "tropical year" on the moon is only 347 days long

answers: NDQ_002358

answers: The "tropical year" on the moon

answers: NDQ_002359

answers: 347 days long

answers: NDQ_002360

answers: The "tropical year" on the moon is only 347 days long. This is called the draconic year or eclipse year

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: the "tropical year" on the moon

answers: NDQ_002363

answers: Earth's equator

answers: NDQ_002364

answers: the centre of the sun is above the horizon

answers: NDQ_002365

answers: 15 earth days

answers: NDQ_002366

answers: 347 days

answers: NDQ_002367

answers: 347 days

answers: NDQ_002368

answers: lunar night

text: Space elevator designs for Earth typically have a taper of the tether that provides a uniform stress profile rather than a uniform cross-section. Because the strength requirement of a lunar space elevator is much lower than that of an Earth space elevator, a uniform cross-section is possible for the lunar space elevator. The study done for NASA's Institute of Advanced Concepts states "Current composites have characteristic heights of a few hundred kilometers, which would require taper ratios of about 6 for Mars, 4 for the Moon, and about 6000 for the Earth. The mass of the Moon is small enough that a uniform cross-section lunar space elevator could be constructed, without any taper at all." A uniform cross-section could make it possible for a lunar space elevator to be built in a double-tether pulley configuration. This configuration would greatly simplify repairs of a space elevator compared to a tapered elevator configuration. However a pulley configuration would require a strut at the counterweight hundreds of kilometers long to separate the up-tether from the down-tether and keep them from tangling. A pulley configuration might also allow the system capacity to be gradually expanded by stitching new tether material on at the Lagrange point as the tether rotated.

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answers: lunar

answers: NDQ_002324

answers: Mars, 4 for the Moon

answers: NDQ_002325

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answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: Space elevator designs

answers: NDQ_002328

answers: a pulley configuration

answers: NDQ_002329

answers: Earth

answers: NDQ_002330

answers: Lagrange point

answers: NDQ_002331

answers: Space elevator designs

answers: NDQ_002332

answers: Earth

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: lunar

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: The mass of the Moon is small enough that a uniform cross-section lunar space elevator could be constructed, without any taper at all

answers: NDQ_002348

answers: no taper

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: The study done for NASA's Institute of Advanced Concepts

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow

answers: NDQ_002354

answers: Space elevator designs for Earth typically have a taper of the tether

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: The mass of the Moon

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

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answers: NDQ_002359

answers: Moon

answers: NDQ_002360

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answers: NDQ_002361

answers: The mass of the Moon

answers: NDQ_002362

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answers: NDQ_002363

answers: Moon

answers: NDQ_002364

answers: Earth

answers: NDQ_002365

answers: hundreds of kilometers

answers: NDQ_002366

answers: Earth

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answers: NDQ_002368

answers: crescent

text: For a planet, angular momentum is distributed between the spin of the planet and its revolution in its orbit, and these are often exchanged by various mechanisms. The conservation of angular momentum in the Earth–Moon system results in the transfer of angular momentum from Earth to Moon, due to tidal torque the Moon exerts on the Earth. This in turn results in the slowing down of the rotation rate of Earth, at about 65.7 nanoseconds per day, and in gradual increase of the radius of Moon's orbit, at about 3.82 centimeters per year.

text: For a planet, angular momentum is distributed between the spin of the planet and its revolution in its orbit, and these are often exchanged by various mechanisms. The conservation of angular momentum in the

text: Earth–Moon system

text: results in the transfer of angular momentum from Earth to Moon, due to

text: tidal torque

text: the Moon exerts on the Earth. This in turn results in the slowing down of the rotation rate of Earth, at about 65.7 nanoseconds per day, and in gradual increase of the radius of Moon's orbit, at about 3.82 centimeters per year.

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text: In astronomy,  new moon is the first phase of the Moon, when it orbits as seen from the Earth, the moment when the Moon and the Sun have the same ecliptical longitude.The Moon is not visible at this time except when it is seen in silhouette during a solar eclipse when it is illuminated by earthshine. See the article on phases of the Moon for further details.

text: In astronomy,  new moon is the first

text: phase of the Moon

text: , when it orbits as seen from the Earth, the moment when the

text: Moon

text: and the

text: Sun

text: have the same

text: ecliptical longitude

text: .The Moon is not visible at this time except when it is seen in silhouette during a

text: solar eclipse

text: when it is illuminated by

text: earthshine

text: . See the article on

text: phases of the Moon

text: for further details.

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text: There were 242 lunar eclipse events between -1999 and -1900 (2000 BCE to 1901 BCE)

text: There were 242 lunar eclipse events between -1999 and -1900 (2000 BCE to 1901 BCE)

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answers: NDQ_002323

answers: lunar eclipse

answers: NDQ_002324

answers: lunar

answers: NDQ_002325

answers: lunar eclipse

answers: NDQ_002326

answers: lunar eclipse

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: lunar eclipse

answers: NDQ_002330

answers: lunar

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: lunar

answers: NDQ_002334

answers: lunar

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: between -1999 and -1900

answers: NDQ_002345

answers: solar eclipse

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: A solar eclipse is seen on all of the Earth that is having daytime

answers: NDQ_002351

answers: 29.5 days

answers: NDQ_002352

answers: lunar eclipse

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: 242 lunar eclipse events

answers: NDQ_002355

answers: lunar eclipse

answers: NDQ_002356

answers: lunar eclipse

answers: NDQ_002357

answers: lunar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

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answers: NDQ_002363

answers: lunar

answers: NDQ_002364

answers: lunar eclipse

answers: NDQ_002365

answers: a lunar eclipse

answers: NDQ_002366

answers: 2000 BCE

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: Lunar eclipses can occur only at full moon, where the Moon's orbit allows it to pass through Earth's shadow. Lunar eclipses do not occur every month because the Moon usually passes above or below Earth's shadow (which is mostly restricted to the ecliptic plane). Lunar eclipses can occur only when the full moon occurs near the two nodes of the orbit, either the ascending or descending node. This causes eclipses to only occur about every 6 months, and often 2 weeks before or after a solar eclipse at new moon at the opposite node.

text: Lunar eclipse

text: s can occur only at full moon, where the Moon's orbit allows it to pass through Earth's shadow. Lunar eclipses do not occur every month because the Moon usually passes above or below Earth's shadow (which is mostly restricted to the

text: ecliptic plane

text: ). Lunar eclipses can occur only when the full moon occurs near the two

text: nodes of the orbit

text: , either the ascending or descending node. This causes eclipses to only occur about every 6 months, and often 2 weeks before or after a

text: solar eclipse

text: at

text: new moon

text: at the opposite node.

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answers: NDQ_002323

answers: full moon

answers: NDQ_002324

answers: ecliptic plane

answers: NDQ_002325

answers: new moon

answers: NDQ_002326

answers: full

answers: NDQ_002327

answers: lunar eclipses

answers: NDQ_002328

answers: lunar eclipses

answers: NDQ_002329

answers: new moon

answers: NDQ_002330

answers: Earth's shadow

answers: NDQ_002331

answers: lunar eclipses

answers: NDQ_002332

answers: full moon

answers: NDQ_002334

answers: Earth's shadow

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: It does not occur every month because the Moon usually passes above or below Earth's shadow

answers: NDQ_002345

answers: The Moon's orbit allows it to pass through Earth's shadow

answers: NDQ_002348

answers: Earth's shadow

answers: NDQ_002350

answers: The Moon's orbit allows it to pass through Earth's shadow

answers: NDQ_002351

answers: This causes eclipses to only occur about every 6 months

answers: NDQ_002352

answers: Earth's shadow

answers: NDQ_002353

answers: mostly restricted to the ecliptic plane

answers: NDQ_002354

answers: This causes eclipses to only occur about every 6 months

answers: NDQ_002355

answers: Moon usually passes above or below Earth's shadow

answers: NDQ_002356

answers: about every 6 months

answers: NDQ_002357

answers: Earth's shadow

answers: NDQ_002358

answers: New moon

answers: NDQ_002359

answers: The full moon will occur on the 28th

answers: NDQ_002360

answers: The Moon's orbit allows it to pass through Earth's shadow

answers: NDQ_002361

answers: Moon's orbit allows it to pass through Earth's shadow

answers: NDQ_002362

answers: Lunar eclipses

answers: NDQ_002363

answers: Earth's shadow

answers: NDQ_002364

answers: Earth's shadow

answers: NDQ_002365

answers: 2 weeks

answers: NDQ_002366

answers: 6 months

answers: NDQ_002367

answers: 2 weeks

answers: NDQ_002368

answers: new moon

text: The outermost disc is decorated with a fleur-de-lis which represents the sun, and which orbits the dial once every 24 hours. This indicates the hour of the day, counted from I to XII in Roman numerals in first the right and then the left hemispheres of the clockface. This is an example of a 24-hour analog dial. The tail of the sun's fleur-de-lis points to the day in the lunar month on the inner ring.  The half-black, half-silver moon inside the lunar month ring rotates on its axis to show the correct phase of the moon. The earth is represented as a fixed golden ball in the centre of the dial. The Latin inscription "Pereunt et imputantur" below the main dial may be translated as "The hours pass and are reckoned to our account".

text: The outermost disc is decorated with a

text: fleur-de-lis

text: which represents the sun, and which orbits the dial once every 24 hours. This indicates the hour of the day, counted from I to XII in

text: Roman numerals

text: in first the right and then the left hemispheres of the clockface. This is an example of a

text: 24-hour analog dial

text: . The tail of the sun's fleur-de-lis points to the day in the

text: lunar month

text: on the inner ring.  The half-black, half-silver moon inside the lunar month ring rotates on its axis to show the correct

text: phase of the moon

text: . The earth is represented as a fixed golden ball in the centre of the dial. The Latin inscription "Pereunt et imputantur" below the main dial may be translated as "The hours pass and are reckoned to our account".

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answers: 4

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answers: 3

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answers: 4

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answers: 0

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answers: NDQ_002323

answers: half-silver

answers: NDQ_002324

answers: left and right hemispheres

answers: NDQ_002325

answers: half-black

answers: NDQ_002326

answers: half-silver

answers: NDQ_002327

answers: phase

answers: NDQ_002328

answers: The correct phase of the moon

answers: NDQ_002329

answers: half-black

answers: NDQ_002330

answers: half-black, half-silver moon

answers: NDQ_002331

answers: phase

answers: NDQ_002332

answers: silver

answers: NDQ_002334

answers: The outermost disc

answers: NDQ_002335

answers: half-black

answers: NDQ_002343

answers: half-black, half-silver moon

answers: NDQ_002345

answers: fleur-de-lis which represents the sun

answers: NDQ_002348

answers: half-black, half-silver moon

answers: NDQ_002350

answers: This indicates the hour of the day

answers: NDQ_002351

answers: half-black, half-silver

answers: NDQ_002352

answers: half-black, half-silver

answers: NDQ_002353

answers: half-black, half-silver

answers: NDQ_002354

answers: solar eclipses are rare events

answers: NDQ_002355

answers: half-black, half-silver moon

answers: NDQ_002356

answers: lunar month on the inner ring

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: the correct phase of the moon

answers: NDQ_002359

answers: the full moon will occur on the 28th

answers: NDQ_002360

answers: half-black, half-silver moon

answers: NDQ_002361

answers: half-black, half-silver moon

answers: NDQ_002362

answers: the correct phase of the moon

answers: NDQ_002363

answers: sun

answers: NDQ_002364

answers: the sun

answers: NDQ_002365

answers: 24 hours

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: 24 hours

answers: NDQ_002368

answers: half-black

text: Comet Holmes not only became brighter, but it also swelled in size as its coma expanded. In late October 2007 the coma's apparent diameter increased from 3.3 arcminutes to over 13 arcminutes, about half the diameter of the Moon in the sky. At a distance of around 2 AU, this means that the true diameter of the coma had swelled to over 1 million km, or about 70% of the diameter of the Sun.  By comparison, the Moon is 380,000 km from Earth.   Therefore, during the 2007 outburst of Comet Holmes the coma was a sphere wider than the diameter of the Moon's orbit around Earth.  On 2007  November, the coma had dispersed to a volume larger than the Sun, briefly giving it the largest extended atmosphere in the Solar System.

text: Comet Holmes not only became brighter, but it also swelled in size as its coma expanded. In late October 2007 the

text: coma

text: 's

text: apparent diameter

text: increased from 3.3 arcminutes to over 13 arcminutes, about half the diameter of the Moon in the sky. At a distance of around 2

text: AU

text: , this means that the true diameter of the coma had swelled to over 1 million km, or about 70% of the diameter of the

text: Sun

text: .  By comparison, the

text: Moon

text: is 380,000 km from

text: Earth

text: .   Therefore, during the 2007 outburst of Comet Holmes the coma was a sphere wider than the diameter of the

text: Moon

text: 's orbit around

text: Earth

text: .  On 2007  November, the coma had dispersed to a volume larger than the Sun, briefly giving it the largest extended atmosphere in the Solar System.

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answers: Moon's orbit around Earth

answers: NDQ_002328

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answers: half the diameter

answers: NDQ_002330

answers: half the diameter of the Moon

answers: NDQ_002331

answers: outburst

answers: NDQ_002332

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answers: NDQ_002334

answers: coma

answers: NDQ_002335

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answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: about 70% of the diameter of the Sun

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Moon

answers: NDQ_002351

answers: The coma's apparent diameter increased

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: half the diameter of the Moon

answers: NDQ_002354

answers: Solar eclipses are rare

answers: NDQ_002355

answers: half the diameter of the Moon

answers: NDQ_002356

answers: November

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

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answers: Comet Holmes

answers: NDQ_002363

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answers: 13 arcminutes

answers: NDQ_002366

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answers: quarter moon

answers: NDQ_002368

answers: crescent

text: An annular solar eclipse occurred on June 10, 2002. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: occurred on June 10, 2002. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: NDQ_002326

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answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

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answers: NDQ_002331

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answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

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answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: (ring)

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: An annular solar eclipse

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: Moon passes between Earth and the Sun

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answers: full moon

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answers: partial

text: There is often confusion between a solar and lunar eclipse. While both involve interactions between the sun, Earth, and moon, they are very different in their interactions.

text: There is often confusion between a solar and lunar eclipse. While both involve interactions between the sun, Earth, and moon, they are very different in their interactions.

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text: Sunrise occurs at the prime meridian when the Lunar phase reaches First Quarter, after one fourth of a lunar day. At this location the selenographic colongitude at sunrise is defined as 0°. Thus, by the time of the Full Moon the colongitude increases to 90°; at Last Quarter it is 180°, and at the New Moon the colongitude reaches 270°.  Note that the Moon is nearly invisible from the Earth at New Moon phase except during a solar eclipse.

text: Sunrise occurs at the prime meridian when the

text: Lunar phase

text: reaches First Quarter, after one fourth of a

text: lunar day

text: . At this location the selenographic colongitude at sunrise is defined as 0°. Thus, by the time of the

text: Full Moon

text: the colongitude increases to 90°; at Last Quarter it is 180°, and at the

text: New Moon

text: the colongitude reaches 270°.  Note that the Moon is nearly invisible from the Earth at New Moon phase except during a

text: solar eclipse

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text: Several missions have used Lissajous orbits: ACE at Sun–Earth , DSCOVR at Sun–Earth , WMAP at Sun–Earth , and also the Genesis mission collecting solar particles at .On 14 May 2009, the European Space Agency (ESA) launched into space the Herschel and Planck observatories, both of which use Lissajous orbits at Sun–Earth .ESA's current  Gaia mission also uses a Lissajous orbit at Sun–Earth .In 2011, NASA transferred two of its THEMIS spacecraft from Earth orbit to Lunar orbit by way of Earth-Moon  and  Lissajous orbits.China's lunar orbiter Chang'e 2 left lunar orbit on June 8, 2011 and was placed in a Lissajous orbit at Earth-Sun  until mid-2012 prior to leaving Earth orbit entirely to fly by the asteroid Toutatis.

text: Several missions have used Lissajous orbits:

text: ACE

text: at Sun–Earth ,

text: DSCOVR

text: at Sun–Earth ,

text: WMAP

text: at Sun–Earth , and also the

text: Genesis

text: mission collecting solar particles at .On 14 May 2009, the

text: European Space Agency

text: (ESA) launched into space the

text: Herschel

text: and

text: Planck

text: observatories, both of which use Lissajous orbits at Sun–Earth .ESA's current

text: Gaia mission

text: also uses a Lissajous orbit at Sun–Earth .In 2011, NASA transferred two of its

text: THEMIS

text: spacecraft from Earth orbit to Lunar orbit by way of Earth-Moon  and  Lissajous orbits.China's lunar orbiter

text: Chang'e 2

text: left lunar orbit on June 8, 2011 and was placed in a Lissajous orbit at Earth-Sun  until mid-2012 prior to leaving Earth orbit entirely to fly by the asteroid Toutatis.

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answers: NDQ_002323

answers: Moon

answers: NDQ_002324

answers: Moon

answers: NDQ_002325

answers: Moon

answers: NDQ_002326

answers: Earth-Moon

answers: NDQ_002327

answers: Earth-Moon

answers: NDQ_002328

answers: Earth-Moon

answers: NDQ_002329

answers: Earth-Moon

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: Earth-Moon

answers: NDQ_002332

answers: Lunar

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: Moon

answers: NDQ_002343

answers: Lunar

answers: NDQ_002345

answers: Earth–Sun

answers: NDQ_002348

answers: Earth-Moon

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Earth-Moon

answers: NDQ_002352

answers: Lunar

answers: NDQ_002353

answers: Lissajous

answers: NDQ_002354

answers: Earth–Sun

answers: NDQ_002355

answers: Earth

answers: NDQ_002356

answers: Lunar orbit

answers: NDQ_002357

answers: Earth-Moon

answers: NDQ_002358

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answers: NDQ_002359

answers: Earth-Moon

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: missions have used Lissajous orbits

answers: NDQ_002363

answers: Earth-Moon

answers: NDQ_002364

answers: Earth–Sun

answers: NDQ_002365

answers: Earth–Sun

answers: NDQ_002366

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answers: 1

answers: NDQ_002368

answers: full moon

text:
Planetary exploration missions have often turned to Radio-Isotope devices, whether RHUs or RTGs, to support thermal control and power generation in what are often extreme temperature and energy poor environments. However, for Europe, where these technologies are currently unavailable, employing such devices have important technical and programmatic impacts. While activities investigating the development of RHUs and ultimately RTGs are proceeding within Europe, it is not expected that European devices would be available in the 2018 timeframe of the Lunar Lander mission.
Instead, the Lunar Lander is powered by solar arrays which are wrapped around the body tube. Once landed, the vehicles axis of symmetry will be almost perpendicular to the direction of the Sun ensuring continuously good illumination of the solar cells as the lander rotates with respect to the Sun (due to the rotation of the Moon).
Batteries are used to bridge short periods without solar power. Solar power is unavailable in LLO when the lander goes into lunar eclipse and on the ground, when mountain peaks at the horizon cover the Sun. Landing operations will also be conducted relying solely on battery power.

text: Planetary exploration missions have often turned to Radio-Isotope devices, whether RHUs or RTGs, to support thermal control and power generation in what are often extreme temperature and energy poor environments. However, for Europe, where these technologies are currently unavailable, employing such devices have important technical and programmatic impacts. While activities investigating the development of RHUs and ultimately RTGs are proceeding within Europe, it is not expected that European devices would be available in the 2018 timeframe of the Lunar Lander mission.<br>Instead, the Lunar Lander is powered by solar arrays which are wrapped around the body tube. Once landed, the vehicles axis of symmetry will be almost perpendicular to the direction of the

text: Sun

text: ensuring continuously good illumination of the solar cells as the lander rotates with respect to the Sun (due to the rotation of the Moon). <br>Batteries are used to bridge short periods without solar power. Solar power is unavailable in LLO when the lander goes into lunar

text: eclipse

text: and on the ground, when mountain peaks at the horizon cover the Sun. Landing operations will also be conducted relying solely on battery power.

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answers: NDQ_002325

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answers: NDQ_002326

answers: LLO

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: lunar eclipse

answers: NDQ_002330

answers: LLO

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: LLO

answers: NDQ_002334

answers: LLO

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: Solar power is unavailable in LLO

answers: NDQ_002345

answers: Solar power is unavailable in LLO when the lander goes into lunar eclipse

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: Lunar Lander

answers: NDQ_002352

answers: lunar eclipse

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow.

answers: NDQ_002354

answers: Solar power is unavailable in LLO when the lander goes into lunar eclipse

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: Solar power is unavailable in LLO

answers: NDQ_002357

answers: lunar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Solar power is unavailable

answers: NDQ_002361

answers: Solar power is unavailable

answers: NDQ_002362

answers: rotation of the Moon

answers: NDQ_002363

answers: Moon

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answers: the Sun

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

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answers: lunar eclipse

text: In the Southern Hemisphere the sun passes from east to west through the north, although north of the Tropic of Capricorn the mean sun can be directly overhead or due south at midday. The Sun rotating through the north causes an apparent right-left trajectory through the sky unlike the left-right motion of the Sun when seen from the Northern Hemisphere as it passes through the southern sky. Sun-cast shadows turn anticlockwise throughout the day and sundials have the hours increasing in the anticlockwise direction. During solar eclipses viewed from a point to the south of the Tropic of Capricorn, the Moon moves from left to right on the disc of the Sun (see, for example, photos with timings of the solar eclipse of November 13, 2012), while viewed from a point to the north of the Tropic of Cancer (i.e., in the Northern Hemisphere), the Moon moves from right to left during solar eclipses.

text: In the Southern Hemisphere the sun passes from east to west through the north, although north of the

text: Tropic of Capricorn

text: the

text: mean sun

text: can be directly overhead or due south at midday. The Sun rotating through the north causes an apparent right-left trajectory through the sky unlike the left-right motion of the Sun when seen from the Northern Hemisphere as it passes through the southern sky. Sun-cast shadows turn anticlockwise throughout the day and

text: sundial

text: s have the hours increasing in the anticlockwise direction. During

text: solar eclipse

text: s viewed from a point to the south of the Tropic of Capricorn, the Moon moves from left to right on the disc of the Sun (see, for example, photos with timings of the

text: solar eclipse of November 13, 2012

text: ), while viewed from a point to the north of the Tropic of Cancer (i.e., in the Northern Hemisphere), the Moon moves from right to left during solar eclipses.

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answers: NDQ_002323

answers: crescent

answers: NDQ_002324

answers: the Southern Hemisphere

answers: NDQ_002325

answers: eclipses

answers: NDQ_002326

answers: right-left

answers: NDQ_002327

answers: solar eclipses

answers: NDQ_002328

answers: solar eclipses

answers: NDQ_002329

answers: Capricorn

answers: NDQ_002330

answers: Sun

answers: NDQ_002331

answers: solar eclipses

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: the disc of the Sun

answers: NDQ_002335

answers: Solar eclipses

answers: NDQ_002343

answers: solar eclipses

answers: NDQ_002345

answers: The Sun rotating through the north causes an apparent right-left trajectory through the sky

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: In the Southern Hemisphere

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the Moon moves from left to right

answers: NDQ_002353

answers: Sun-cast shadows

answers: NDQ_002354

answers: the solar eclipse of November 13, 2012

answers: NDQ_002355

answers: Partially eclipsed

answers: NDQ_002356

answers: November 13, 2012

answers: NDQ_002357

answers: solar eclipses

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the full moon

answers: NDQ_002360

answers: The sun passes from east to west through the north

answers: NDQ_002361

answers: Moon moves from left to right on the disc of the Sun

answers: NDQ_002362

answers: the Moon moves from left to right on the disc of the Sun

answers: NDQ_002363

answers: disc

answers: NDQ_002364

answers: the Sun passes from east to west through the north

answers: NDQ_002365

answers: a day

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: crescent

text: The Moon's regular phases make it a very convenient timepiece, and the periods of its waxing and waning form the basis of many of the oldest calendars. Tally sticks, notched bones dating as far back as 20–30,000 years ago, are believed by some to mark the phases of the Moon.The ~30-day month is an approximation of the lunar cycle.The English noun month and its cognates in other Germanic languages stem from Proto-Germanic *mǣnṓth-, which is connected to the above-mentioned Proto-Germanic *mǣnōn, indicating the usage of a lunar calendar among the Germanic peoples (Germanic calendar) prior to the adoption of a solar calendar. The PIE root of moon, *méhnōt, derives from the PIE verbal root *meh-, "to measure", "indicat[ing] a functional conception of the moon, i.e. marker of the month" (cf. the English words measure and menstrual), and echoing the Moon's importance to many ancient cultures in measuring time (see Latin ''mensis'' and Ancient Greek ''μείς'' (meis) or  (mēn), meaning "month").Most historical calendars are lunisolar. The 7th-century Islamic calendar is an exceptional example of a purely lunar calendar. Months are traditionally determined by the visual sighting of the hilal, or earliest crescent moon, over the horizon.

text: The Moon's regular phases make it a very convenient timepiece, and the periods of its waxing and waning form the basis of many of the oldest calendars.

text: Tally stick

text: s, notched bones dating as far back as 20–30,000 years ago, are believed by some to mark the phases of the Moon.The ~30-day month is an approximation of the

text: lunar cycle

text: .The English noun month and its cognates in other Germanic languages stem from Proto-Germanic *mǣnṓth-, which is connected to the above-mentioned Proto-Germanic *mǣnōn, indicating the usage of a

text: lunar calendar

text: among the

text: Germanic peoples

text: Germanic calendar

text: ) prior to the adoption of a

text: solar calendar

text: . The

text: PIE root

text: of moon, *méhnōt, derives from the PIE verbal root *meh-, "to measure", "indicat[ing] a functional conception of the moon, i.e. marker of the month" (

text: cf.

text: the English words measure and menstrual), and echoing the Moon's importance to many ancient cultures in measuring time (see

text: Latin

text: ''mensis'' and

text: Ancient Greek

text: ''μείς'' (meis) or  (mēn), meaning "month").Most historical calendars are

text: lunisolar

text: . The 7th-century

text: Islamic calendar

text: is an exceptional example of a purely

text: lunar calendar

text: . Months are traditionally determined by the visual sighting of the

text: hilal

text: , or earliest crescent moon, over the horizon.

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answers: NDQ_002324

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answers: NDQ_002325

answers: crescent

answers: NDQ_002326

answers: crescent

answers: NDQ_002327

answers: horizon

answers: NDQ_002328

answers: hilal

answers: NDQ_002329

answers: crescent

answers: NDQ_002330

answers: horizon

answers: NDQ_002331

answers: horizon

answers: NDQ_002332

answers: waxing

answers: NDQ_002334

answers: horizon

answers: NDQ_002335

answers: crescent

answers: NDQ_002343

answers: lunar eclipse

answers: NDQ_002345

answers: The 7th-century Islamic calendar

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The English noun month

answers: NDQ_002351

answers: The lunar cycle

answers: NDQ_002352

answers: horizon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The 7th-century Islamic calendar

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: The Moon's regular phases

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: hilal

answers: NDQ_002359

answers: 30-day month

answers: NDQ_002360

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answers: NDQ_002361

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answers: NDQ_002362

answers: phases of the Moon

answers: NDQ_002363

answers: horizon

answers: NDQ_002364

answers: the Moon's regular phases

answers: NDQ_002365

answers: 30 days

answers: NDQ_002366

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answers: NDQ_002367

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answers: NDQ_002368

answers: waning

text: For almost five millennia, the geocentric model of the Earth as the center of the universe had been accepted by all but a few astronomers. In Aristotle's cosmology, Earth's central location was perhaps less significant than its identification as a realm of imperfection, inconstancy, irregularity and change, as opposed to the "heavens", (Moon, Sun, planets, stars) which were regarded as perfect, permanent, unchangeable, and in religious thought, the realm of heavenly beings. The Earth was even composed of different material, the four elements "earth", "water", "fire", and "air", while sufficiently far above its surface (roughly the Moon's orbit), the heavens were composed of different substance called "aether". The heliocentric model that replaced it involved not only the radical displacement of the earth to an orbit around the sun, but its sharing a placement with the other planets implied a universe of heavenly components made from the same changeable substances as the Earth. Heavenly motions no longer needed to be governed by a theoretical perfection, confined to circular orbits.

text: For almost five

text: millennia

text: , the

text: geocentric model

text: of the Earth as the center of the universe had been accepted by all but a few astronomers. In Aristotle's cosmology, Earth's central location was perhaps less significant than its identification as a realm of imperfection, inconstancy, irregularity and change, as opposed to the "heavens", (Moon, Sun, planets, stars) which were regarded as perfect, permanent, unchangeable, and in religious thought, the realm of heavenly beings. The Earth was even composed of different material, the four elements "earth", "water", "fire", and "air", while sufficiently far above its surface (roughly the Moon's orbit), the heavens were composed of different substance called "aether". The

text: heliocentric model

text: that replaced it involved not only the radical displacement of the earth to an orbit around the sun, but its sharing a placement with the other planets implied a universe of heavenly components made from the same changeable substances as the Earth. Heavenly motions no longer needed to be governed by a theoretical perfection, confined to circular orbits.

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answers: NDQ_002343

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answers: NDQ_002345

answers: heliocentric model

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

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answers: The heliocentric model

answers: NDQ_002353

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answers: NDQ_002354

answers: The heliocentric model

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answers: NDQ_002357

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answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The heliocentric model

answers: NDQ_002360

answers: Moon

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answers: NDQ_002362

answers: changeable substances

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answers: the Earth to an orbit around the sun

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answers: a few hours

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answers: millennium

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: crescent

text: are tag-team bosses first appearing in Kirby's Adventure. Mr. Shine appears as a crescent moon with a face and limbs, while Mr. Bright is a sun with similar features. They are the Sun and the Moon in Dreamland. One always stays in the air, raining down projectiles, while the other attacks from the ground. One of their most lethal attacks is when they create a solar eclipse: Mr. Bright will blast the area with flames while Mr. Shine creates a patch of shadow, which is the only safe spot. They return in Kirby's Dream Land 2, Kirby's Dream Land 3, and Kirby: Nightmare in Dreamland. In Kirby Super Star, they literally fought day and night due to a misunderstanding caused by Marx. In the anime, a monster named Slice and Splice in the English dub and Kittari Hattari in the Japanese version uses moon- and sun-shaped staffs to split and paste his enemies. Presumably, this was an ode to Mr, Shine and Mr, Bright. They also appear in Kirby Mass Attack on Strato Patrol EOS mode.

text: are tag-team bosses first appearing in

text: Kirby's Adventure

text: . Mr. Shine appears as a crescent

text: moon

text: with a face and limbs, while Mr. Bright is a

text: sun

text: with similar features. They are the Sun and the Moon in Dreamland. One always stays in the air, raining down projectiles, while the other attacks from the ground. One of their most lethal attacks is when they create a solar eclipse: Mr. Bright will blast the area with flames while Mr. Shine creates a patch of shadow, which is the only safe spot. They return in

text: Kirby's Dream Land 2

text: Kirby's Dream Land 3

text: , and

text: Kirby: Nightmare in Dreamland

text: . In

text: Kirby Super Star

text: , they literally fought day and night due to a misunderstanding caused by Marx. In the anime, a monster named Slice and Splice in the English dub and Kittari Hattari in the Japanese version uses moon- and sun-shaped staffs to split and paste his enemies. Presumably, this was an ode to Mr, Shine and Mr, Bright. They also appear in Kirby Mass Attack on Strato Patrol EOS mode.

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answers: They are the Sun and the Moon in Dreamland

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answers: One of their most lethal attacks

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answers: One always stays in the air, raining down projectiles, while the other attacks from the ground

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text: This is the average period of the Moon's revolution with respect to the line joining the Sun and Earth. The synodic month is the period of the Moon's phases, because the Moon's appearance depends on the position of the Moon with respect to the Sun as seen from the Earth.

text: This is the average period of the Moon's revolution with respect to the line joining the Sun and Earth. The synodic month is the period of the Moon's

text: phases

text: , because the Moon's appearance depends on the position of the Moon with respect to the Sun as seen from the Earth.

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text: During a lunar eclipse, a very small amount of light from the sun does however still reach the Moon, even when the lunar eclipse is total; this is light which has been refracted or bent as it passes through the Earth's atmosphere. This sunlight has been scattered by the dust in the Earth's atmosphere, and thus that light is red, in the same way that sunset and sunrise light is red. This weak red illumination is what causes the eclipsed Moon to be dimly reddish or copper-colored in appearance.

text: During a lunar eclipse, a very small amount of light from the sun does however still reach the Moon, even when the lunar eclipse is total; this is light which has been

text: refracted

text: or bent as it passes through the Earth's atmosphere. This sunlight has been

text: scattered

text: by the dust in the Earth's atmosphere, and thus that light is red, in the same way that sunset and sunrise light is red. This weak red illumination is what causes the eclipsed Moon to be dimly reddish or

text: copper

text: -colored in appearance.

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 3

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answers: NDQ_002367

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answers: 0

answers: NDQ_002323

answers: eclipsed

answers: NDQ_002324

answers: Moon

answers: NDQ_002325

answers: total

answers: NDQ_002326

answers: total

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: Earth's atmosphere

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: total

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: It does however still reach the Moon

answers: NDQ_002345

answers: a very small amount of light from the sun

answers: NDQ_002348

answers: no

answers: NDQ_002350

answers: A lunar eclipse is seen on the Moon

answers: NDQ_002351

answers: 29.5 days

answers: NDQ_002352

answers: The cone-shaped part of the moons shadow is the penumbra

answers: NDQ_002353

answers: The umbra part of a shadow

answers: NDQ_002354

answers: lunar eclipse

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: It occurs once every month

answers: NDQ_002357

answers: lunar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: no

answers: NDQ_002361

answers: no

answers: NDQ_002362

answers: dust in the Earth's atmosphere

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: Earth's atmosphere

answers: NDQ_002365

answers: a lunar eclipse

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: The above descriptions of the lunar phases apply for observers at temperate or high latitudes on the Earth. Observers in tropical latitudes see the Moon with its terminator apparently horizontal during the morning and evening. The crescent Moon can open upward or downward, with the "horns" of the crescent pointing up or down, respectively. When the Sun appears above the Moon in the sky, the crescent opens downward; when the Moon is above the Sun, the crescent opens upward. The crescent Moon is most clearly and brightly visible when the Sun is below the horizon, which implies that the Moon must be above the Sun, and the crescent must open upward. This is therefore the orientation in which the crescent Moon is most often seen from the Earth's tropics. The waxing and waning crescents look very similar. The waxing crescent appears in the western sky in the evening, and the waning crescent in the east, in the morning.

text: The above descriptions of the lunar phases apply for observers at temperate or high latitudes on the Earth. Observers in tropical latitudes see the Moon with its terminator apparently horizontal during the morning and evening. The crescent Moon can open upward or downward, with the "horns" of the crescent pointing up or down, respectively. When the Sun appears above the Moon in the sky, the crescent opens downward; when the Moon is above the Sun, the crescent opens upward. The crescent Moon is most clearly and brightly visible when the Sun is below the horizon, which implies that the Moon must be above the Sun, and the crescent must open upward. This is therefore the orientation in which the crescent Moon is most often seen from the Earth's tropics. The waxing and waning crescents look very similar. The waxing crescent appears in the western sky in the evening, and the waning crescent in the east, in the morning.

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002367

answers: 0

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answers: 0

answers: NDQ_002323

answers: waxing

answers: NDQ_002324

answers: downward; when the Moon is above the Sun

answers: NDQ_002325

answers: waning

answers: NDQ_002326

answers: waxing

answers: NDQ_002327

answers: morning and evening

answers: NDQ_002328

answers: the crescent opens upward

answers: NDQ_002329

answers: waning crescent

answers: NDQ_002330

answers: terminator

answers: NDQ_002331

answers: evening

answers: NDQ_002332

answers: crescent

answers: NDQ_002334

answers: terminator

answers: NDQ_002335

answers: waxing

answers: NDQ_002343

answers: When the Sun appears above the Moon in the sky, the crescent opens downward

answers: NDQ_002345

answers: When the Sun appears above the Moon in the sky, the crescent opens downward

answers: NDQ_002348

answers: Moon must be above the Sun, and the crescent must open upward

answers: NDQ_002350

answers: When the Sun appears above the Moon in the sky

answers: NDQ_002351

answers: The crescent Moon can open upward or downward

answers: NDQ_002352

answers: terminator

answers: NDQ_002353

answers: When the Sun appears above the Moon in the sky

answers: NDQ_002354

answers: When the Sun appears above the Moon in the sky, the crescent opens downward

answers: NDQ_002355

answers: The crescent Moon can open upward or downward

answers: NDQ_002356

answers: It is most often seen from the Earth's tropics

answers: NDQ_002357

answers: When the Sun appears above the Moon in the sky, the crescent opens downward

answers: NDQ_002358

answers: The crescent Moon can open upward or downward

answers: NDQ_002359

answers: the full moon will occur on the 28th of the month

answers: NDQ_002360

answers: Moon must be above the Sun, and the crescent must open upward

answers: NDQ_002361

answers: When the Sun appears above the Moon in the sky

answers: NDQ_002362

answers: When the Sun appears above the Moon in the sky, the crescent opens downward

answers: NDQ_002363

answers: horizon

answers: NDQ_002364

answers: the Sun appears above the Moon in the sky

answers: NDQ_002365

answers: when the Moon is above the Sun

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: waxing

answers: NDQ_002368

answers: crescent

text: A fourth influence occurs because the orbit of the moon around the earth and the orbit the of the earth around the sun are elliptical rather than circular. The effect of this is that the time between high tides changes a little from day to day. The moon takes about 24.8 hours to orbit around the earth, so it takes half this time, 12.4 hours, for the M2 tides to occur. The tides can be predicted far in advance, because the moon and earth have orbits that are predictable. The National Institute of Water and Atmospheric Research (NIWA) run a tidal computer model specific to New Zealand.

text: A fourth influence occurs because the orbit of the moon around the earth and the orbit the of the earth around the sun are

text: elliptical

text: rather than circular. The effect of this is that the time between high tides changes a little from day to day. The moon takes about 24.8 hours to orbit around the earth, so it takes half this time, 12.4 hours, for the M2 tides to occur. The tides can be predicted far in advance, because the moon and earth have orbits that are predictable. The

entity_name: National Institute of Water and Atmospheric Research

text: National Institute of Water and Atmospheric Research

text: (NIWA) run a tidal computer model specific to New Zealand.

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answers: 4

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answers: 0

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answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: M2

answers: NDQ_002324

answers: the sun

answers: NDQ_002325

answers: M2

answers: NDQ_002326

answers: M2

answers: NDQ_002327

answers: high tides

answers: NDQ_002328

answers: M2 tides

answers: NDQ_002329

answers: half this time

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: high tides

answers: NDQ_002332

answers: high tides

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: M2

answers: NDQ_002343

answers: It takes about 24.8 hours to orbit around the earth, so it takes half this time, 12.4 hours

answers: NDQ_002345

answers: The effect of this is that the time between high tides changes a little from day to day

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: It takes half this time, 12.4 hours

answers: NDQ_002351

answers: The time between high tides changes a little from day to day

answers: NDQ_002352

answers: The effect of this is that the time between high tides changes a little from day to day

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The moon takes about 24.8 hours to orbit around the earth

answers: NDQ_002355

answers: Moon takes about 24.8 hours to orbit around the earth

answers: NDQ_002356

answers: It takes about 24.8 hours to orbit around the earth

answers: NDQ_002357

answers: The moon takes about 24.8 hours to orbit around the earth

answers: NDQ_002358

answers: It takes about 24.8 hours to orbit around the earth

answers: NDQ_002359

answers: The moon takes about 24.8 hours to orbit around the earth, so it takes half this time

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: the time between high tides changes a little from day to day

answers: NDQ_002363

answers: Earth's orbit around the sun

answers: NDQ_002364

answers: the earth around the sun

answers: NDQ_002365

answers: 12.4 hours

answers: NDQ_002366

answers: day

answers: NDQ_002367

answers: 12.4 hours

answers: NDQ_002368

answers: M2

text: TRSSCOMM (Technical Research Ship Special COMMunications), an early U.S. Navy earth-moon-earth satellite communication system that relayed ("bounced") messages directly from intelligence-gathering ship to Washington DC by bouncing a microwave signal off the moon, used first on the USS Oxford (15 December 1961). This system consisted of a 16-foot, dish-shaped antenna mounted on a movable platform and capable of bouncing a 10,000 watt microwave signal off a particular spot on the moon and down either to the receiving station at the National Security Agency, Fort Meade, Maryland, or to one of the other Navy SIGINT ships. TRSSCOMM had the advantage of being able to transmit large quantities of intelligence information very rapidly without giving away the ship's location to hostile direction-finding equipment or interfering with incoming signals. Its major disadvantage is that it could only work if the moon was visible and the shipboard hydraulic stabilization system worked properly. This system was replaced by creation of a network of artificial military satellites.

text: TRSSCOMM (Technical Research Ship Special COMMunications), an early

text: U.S. Navy

text: earth-moon-earth

text: satellite communication system that relayed ("bounced") messages directly from intelligence-gathering ship to

text: Washington DC

text: by bouncing a

text: microwave

text: signal off the

text: moon

text: , used first on the

text: USS Oxford

text: (15 December 1961). This system consisted of a 16-foot, dish-shaped

text: antenna

text: mounted on a movable platform and capable of bouncing a 10,000

text: watt

text: microwave

text: signal off a particular spot on the moon and down either to the receiving station at the

text: National Security Agency

text: Fort Meade, Maryland

text: , or to one of the other Navy

text: SIGINT

text: ships. TRSSCOMM had the advantage of being able to transmit large quantities of intelligence information very rapidly without giving away the ship's location to hostile

text: direction-finding

text: equipment or interfering with incoming signals. Its major disadvantage is that it could only work if the moon was visible and the

text: shipboard hydraulic stabilization

text: system worked properly. This system was replaced by creation of a network of artificial

text: military satellite

text: s.

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answers: visible

answers: NDQ_002327

answers: 15 December 1961

answers: NDQ_002328

answers: TRSSCOMM

answers: NDQ_002329

answers: 16-foot

answers: NDQ_002330

answers: TRSSCOMM

answers: NDQ_002331

answers: visible

answers: NDQ_002332

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answers: TRSSCOMM

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answers: Earth

answers: NDQ_002343

answers: lunar eclipse

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answers: TRSSCOMM

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answers: total lunar eclipse

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answers: The moon

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answers: TRSSCOMM

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answers: TRSSCOMM

answers: NDQ_002353

answers: TRSSCOMM

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answers: TRSSCOMM

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answers: TRSSCOMM

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answers: December

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answers: TRSSCOMM

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answers: TRSSCOMM

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answers: TRSSCOMM

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answers: 15 minutes

answers: NDQ_002366

answers: Earth

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answers: 1

answers: NDQ_002368

answers: full moon

text: Many factors can affect the appearance of the Moon during a lunar eclipse.  The Moon's path through the Earth's umbra is important, but so too are the current conditions of the Earth's atmosphere.  While the Earth's shadow blocks any direct light from striking the Moon during a lunar eclipse, some light is refracted through the Earth's atmosphere giving a Moon a red hue.

text: Many factors can affect the appearance of the Moon during a lunar eclipse.  The Moon's path through the Earth's

text: umbra

text: is important, but so too are the current conditions of the

text: Earth's atmosphere

text: .  While the Earth's shadow blocks any direct light from striking the Moon during a lunar eclipse, some light is refracted through the Earth's atmosphere giving a Moon a red hue.

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answers: umbra

answers: NDQ_002326

answers: lunar eclipse

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: Moon

answers: NDQ_002330

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answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: umbra

answers: NDQ_002335

answers: umbra

answers: NDQ_002343

answers: The Moon's path through the Earth's umbra

answers: NDQ_002345

answers: The Moon's path through the Earth's umbra

answers: NDQ_002348

answers: Earth's shadow

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: Moon's path

answers: NDQ_002352

answers: Earth's shadow

answers: NDQ_002353

answers: Some light is refracted through the Earth's atmosphere

answers: NDQ_002354

answers: lunar eclipse

answers: NDQ_002355

answers: The Moon's path

answers: NDQ_002356

answers: lunar eclipse

answers: NDQ_002357

answers: Earth's shadow

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The Moon's path

answers: NDQ_002360

answers: Earth's shadow blocks any direct light from striking the Moon

answers: NDQ_002361

answers: Earth's shadow

answers: NDQ_002362

answers: Moon's path through the Earth's umbra

answers: NDQ_002363

answers: Earth's

answers: NDQ_002364

answers: Earth's shadow blocks any direct light

answers: NDQ_002365

answers: 24 hours

answers: NDQ_002366

answers: Earth's

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: Nineteen moons are known to be massive enough to have relaxed into a rounded shape under their own gravity, and seven of them are more massive than either Eris or Pluto. They are not physically distinct from the dwarf planets, but are not dwarf planets because they do not directly orbit the Sun. The seven that are more massive than Eris are the Moon, the four Galilean moons of Jupiter (Io, Europa, Ganymede, and Callisto), one moon of Saturn (Titan), and one moon of Neptune (Triton). The others are six moons of Saturn (Mimas, Enceladus, Tethys, Dione, Rhea, and Iapetus), five moons of Uranus (Miranda, Ariel, Umbriel, Titania, and Oberon), and one moon of Pluto (Charon). There are additional possibilities among TNOs, including Dysnomia orbiting Eris. Alan Stern calls these moons "satellite planets", one of three categories of planet together with dwarf planets and classical planets. The term planemo ("planetary-mass object") covers all three.

text: Nineteen

text: moons

text: are known to be massive enough to have relaxed into a rounded shape under their own gravity, and seven of them are more massive than either Eris or Pluto. They are not physically distinct from the dwarf planets, but are not dwarf planets because they do not directly orbit the Sun. The seven that are more massive than Eris are the

text: Moon

text: , the four

text: Galilean moons

text: of Jupiter (

text: Io

text: Europa

text: Ganymede

text: , and

text: Callisto

text: ), one moon of Saturn (

text: Titan

text: ), and one moon of Neptune (

text: Triton

text: ). The others are six moons of Saturn (

text: Mimas

text: Enceladus

text: Tethys

text: Dione

text: Rhea

text: , and

text: Iapetus

text: ), five moons of Uranus (

text: Miranda

text: Ariel

text: Umbriel

text: Titania

text: , and

text: Oberon

text: ), and one moon of Pluto (

text: Charon

text: ). There are additional possibilities among TNOs, including

text: Dysnomia

text: orbiting Eris. Alan Stern calls these moons "satellite planets", one of three categories of planet together with dwarf planets and classical planets. The term

text: planemo

text: ("planetary-mass object") covers all three.

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answers: Galilean

answers: NDQ_002324

answers: Eris and Pluto

answers: NDQ_002325

answers: Europa

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: orbiting

answers: NDQ_002328

answers: Dysnomia

answers: NDQ_002329

answers: dwarf planets

answers: NDQ_002330

answers: Ganymede

answers: NDQ_002331

answers: orbiting

answers: NDQ_002332

answers: satellite planets

answers: NDQ_002334

answers: Ganymede

answers: NDQ_002335

answers: Galilean

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: they do not directly orbit the Sun

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Eris

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: Pluto

answers: NDQ_002353

answers: Umbra

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answers: the Sun

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answers: Earths umbra

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answers: Moon

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answers: full moon phase

answers: NDQ_002358

answers: Moon

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: Moon

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answers: moon of Pluto

answers: NDQ_002362

answers: gravity

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answers: Sun

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answers: a few minutes

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answers: Earth

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answers: quarter moon

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answers: rounded shape

text: Because the orbit of the Moon is inclined only about 5.145° to the ecliptic and the Sun is always very near the ecliptic, eclipses always occur on or near it. Because of the inclination of the Moon's orbit, eclipses do not occur at every conjunction and opposition of the Sun and Moon, but only when the Moon is near an ascending or descending node at the same time it is at conjunction or opposition. The ecliptic is so named because the ancients noted that eclipses only occurred when the Moon crossed it.

text: Because the

text: orbit of the Moon

text: is inclined only about 5.145° to the ecliptic and the

text: Sun

text: is always very near the ecliptic,

text: eclipse

text: s always occur on or near it. Because of the inclination of the

text: Moon

text: 's

text: orbit

text: , eclipses do not occur at every

text: conjunction

text: and

text: opposition

text: of the Sun and Moon, but only when the Moon is near an

text: ascending or descending node

text: at the same time it is at conjunction or opposition. The ecliptic is so named because the ancients noted that eclipses only occurred when the Moon crossed it.

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answers: NDQ_002329

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answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

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answers: 4

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answers: 5

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answers: 4

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answers: 3

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answers: opposition

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answers: ascending and descending node

answers: NDQ_002325

answers: eclipses

answers: NDQ_002326

answers: opposition

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: eclipses

answers: NDQ_002329

answers: about 5.145°

answers: NDQ_002330

answers: ecliptic

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: the Moon

answers: NDQ_002334

answers: the ecliptic

answers: NDQ_002335

answers: opposition

answers: NDQ_002343

answers: It does not occur at every conjunction and opposition of the Sun and Moon

answers: NDQ_002345

answers: Because the orbit of the Moon is inclined only about 5.145° to the ecliptic and the Sun is always very near the ecliptic, eclipses always occur on or near it

answers: NDQ_002348

answers: eclipses always occur on or near it

answers: NDQ_002350

answers: The Sun is always very near the ecliptic

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: The ecliptic

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Because of the inclination of the Moon's orbit, eclipses do not occur at every conjunction and opposition

answers: NDQ_002355

answers: Moon is inclined only about 5.145° to the ecliptic

answers: NDQ_002356

answers: Because the orbit of the Moon is inclined only about 5.145° to the ecliptic

answers: NDQ_002357

answers: opposition

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Because the orbit of the Moon is inclined only about 5.145° to the ecliptic

answers: NDQ_002361

answers: eclipses always occur on or near it

answers: NDQ_002362

answers: eclipses

answers: NDQ_002363

answers: the ecliptic

answers: NDQ_002364

answers: the Sun is always very near the ecliptic

answers: NDQ_002365

answers: about 5.145°

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: eclipses

text: Lunar eclipses are grouped by their saros number, each series lasts between 1200 and 1600 years and contains from 69 to 89 lunar eclipses. Lunar eclipses in even series exist at the ascending node of the moon's orbit, and odd series occur at the descending nodes.

text: Lunar eclipses

text: are grouped by their

text: saros number

text: , each series lasts between 1200 and 1600 years and contains from 69 to 89 lunar eclipses. Lunar eclipses in even series exist at the ascending node of the moon's orbit, and odd series occur at the descending nodes.

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answers: ascending

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answers: ascending node and descending nodes

answers: NDQ_002325

answers: descending

answers: NDQ_002326

answers: even

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: lunar eclipses

answers: NDQ_002329

answers: 69 to 89

answers: NDQ_002330

answers: ascending node

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: lunar eclipses

answers: NDQ_002334

answers: ascending node

answers: NDQ_002335

answers: ascending

answers: NDQ_002343

answers: Lunar eclipses

answers: NDQ_002345

answers: Solar eclipses are grouped by their saros number

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Lunar eclipses are grouped by their saros

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Lunar eclipses

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: 69 to 89 lunar eclipses

answers: NDQ_002357

answers: descending nodes

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Lunar eclipses

answers: NDQ_002361

answers: lunar eclipses

answers: NDQ_002362

answers: lunar eclipses

answers: NDQ_002363

answers: orbit

answers: NDQ_002364

answers: node of the moon's orbit

answers: NDQ_002365

answers: 1600 years

answers: NDQ_002366

answers: 1600 years

answers: NDQ_002367

answers: 1600 years

answers: NDQ_002368

answers: descending

text: When the Earth, moon, and sun are in line (sun–Earth–moon, or sun–moon–Earth) the two main influences combine to produce spring tides; when the two forces are opposing each other as when the angle moon–Earth–sun is close to ninety degrees, neap tides result. As the moon moves around its orbit it changes from north of the equator to south of the equator. The alternation in high tide heights becomes smaller, until they are the same (at the lunar equinox, the moon is above the equator), then redevelop but with the other polarity, waxing to a maximum difference and then waning again.

text: When the Earth, moon, and sun are in line (sun–Earth–moon, or sun–moon–Earth) the two main influences combine to produce spring tides; when the two forces are opposing each other as when the angle moon–Earth–sun is close to ninety degrees, neap tides result. As the moon moves around its orbit it changes from north of the equator to south of the equator. The alternation in high tide heights becomes smaller, until they are the same (at the lunar equinox, the moon is above the equator), then redevelop but with the other polarity, waxing to a maximum difference and then waning again.

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: waxing

answers: NDQ_002324

answers: sun–Earth–moon

answers: NDQ_002325

answers: waning

answers: NDQ_002326

answers: waxing

answers: NDQ_002327

answers: lunar equinox

answers: NDQ_002328

answers: neap tides

answers: NDQ_002329

answers: neap

answers: NDQ_002330

answers: sun

answers: NDQ_002331

answers: lunar equinox

answers: NDQ_002332

answers: waxing

answers: NDQ_002334

answers: the Earth

answers: NDQ_002335

answers: waxing

answers: NDQ_002343

answers: It changes from north of the equator to south

answers: NDQ_002345

answers: When the Earth, moon, and sun are in line

answers: NDQ_002348

answers: moon is above the equator

answers: NDQ_002350

answers: When the Earth, moon, and sun are in line

answers: NDQ_002351

answers: As the moon moves around its orbit it changes

answers: NDQ_002352

answers: penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: when the two forces are opposing each other as when the angle moon–Earth–sun is close to ninety degrees

answers: NDQ_002355

answers: Moon–Earth–sun

answers: NDQ_002356

answers: It changes from north of the equator to south of the equator

answers: NDQ_002357

answers: neap tides

answers: NDQ_002358

answers: waxing

answers: NDQ_002359

answers: the lunar equinox

answers: NDQ_002360

answers: when the two forces are opposing each other

answers: NDQ_002361

answers: when the two forces are opposing each other

answers: NDQ_002362

answers: the two main influences combine to produce spring tides

answers: NDQ_002363

answers: orbit

answers: NDQ_002364

answers: the two forces are opposing each other

answers: NDQ_002365

answers: ninety degrees

answers: NDQ_002366

answers: 365 days

answers: NDQ_002367

answers: waxing

answers: NDQ_002368

answers: redevelop

text: Moon: Development work was done on Sonne (sun) to remove the night time errors, this system was called moon. Work was never completed.

text: Moon: Development work was done on Sonne (sun) to remove the night time errors, this system was called moon. Work was never completed.

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text: The Moon, which orbits Earth rather than the Sun, is in opposition to the Sun at full moon. When it is in exact opposition, a lunar eclipse occurs.

text: The

text: Moon

text: , which orbits Earth rather than the Sun, is in opposition to the Sun at

text: full moon

text: . When it is in exact opposition, a

text: lunar eclipse

text: occurs.

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answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002343

answers: It is in opposition to the Sun

answers: NDQ_002345

answers: The Moon

answers: NDQ_002348

answers: When it is in exact opposition

answers: NDQ_002350

answers: no

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answers: 29.5 days

answers: NDQ_002352

answers: The Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: When it is in exact opposition, a lunar eclipse occurs

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: When it is in exact opposition

answers: NDQ_002357

answers: opposition

answers: NDQ_002358

answers: full moon

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

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answers: NDQ_002361

answers: no

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answers: full moon

answers: NDQ_002368

answers: lunar eclipse

text: Sahadeva was very good in Astrology. Duryodhana, on the advice of Shakuni approached Sahadeva in order to seek the right time (muhurta) to start the Mahabharata war so that the Kauravas will be victorious. Sahadeva disclosed the same for the Kauravas in spite of knowing that Kauravas were their enemy, as Sahadeva was known to be very honest. Then, Krishna planned to create an eclipse much before the beginning of the war. In the mean time, both Sun and Moon got shocked by Krishna's thought and appeared before Krishna stating that this will create a huge imbalance in the entire Universe. Then, Krishna declared that as Earth, Moon and Sun are together in one place, this in itself was an eclipse.

text: Sahadeva was very good in Astrology. Duryodhana, on the advice of Shakuni approached Sahadeva in order to seek the right time (muhurta) to start the Mahabharata war so that the Kauravas will be victorious. Sahadeva disclosed the same for the Kauravas in spite of knowing that Kauravas were their enemy, as Sahadeva was known to be very honest. Then, Krishna planned to create an eclipse much before the beginning of the war. In the mean time, both Sun and Moon got shocked by Krishna's thought and appeared before Krishna stating that this will create a huge imbalance in the entire Universe. Then, Krishna declared that as Earth, Moon and Sun are together in one place, this in itself was an eclipse.

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answers: NDQ_002324

answers: Moon and Sun

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: eclipse

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: an eclipse

answers: NDQ_002329

answers: half moon

answers: NDQ_002330

answers: Sun

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: eclipse

answers: NDQ_002334

answers: Sun

answers: NDQ_002335

answers: eclipse

answers: NDQ_002343

answers: It usually lasts between 5-10 minutes

answers: NDQ_002345

answers: Earth, Moon and Sun

answers: NDQ_002348

answers: Moon

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Solar eclipses are rare events

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: It does not say.

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: Moon

answers: NDQ_002362

answers: Sun and Moon

answers: NDQ_002363

answers: Universe

answers: NDQ_002364

answers: Sun and Moon are together in one place

answers: NDQ_002365

answers: a few hours

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: much

answers: NDQ_002368

answers: crescent

text: Due to tidal acceleration, the orbit of the Moon around the Earth becomes about 2.2 cm more distant each year. It is estimated that, in slightly less than 1.4 billion years, the distance from the Earth to the Moon will have increased by 30,400 km. During that period, the apparent angular diameter of the Moon will decrease in size, meaning that it will no longer be able to completely cover the Sun's disk as seen from the Earth. This will be true even when the Moon is at perigee, and the Earth at aphelion. Moreover, the Sun is increasing in diameter by about 5% per billion years. Therefore, the last total solar eclipse on Earth will occur about six hundred million years from now.

text: Due to

text: tidal acceleration

text: , the orbit of the Moon around the Earth becomes about 2.2 cm more distant each year. It is estimated that, in slightly less than 1.4 billion years, the distance from the Earth to the Moon will have increased by 30,400 km. During that period, the apparent angular diameter of the Moon will decrease in size, meaning that it will no longer be able to completely cover the Sun's disk as seen from the Earth. This will be true even when the Moon is at

text: perigee

text: , and the Earth at

text: aphelion

text: . Moreover, the Sun is increasing in diameter by about 5% per billion years. Therefore, the last total solar eclipse on Earth will occur about six hundred million years from now.

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answers: perigee

answers: NDQ_002324

answers: aphelion

answers: NDQ_002325

answers: total solar eclipse

answers: NDQ_002326

answers: total solar eclipse

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: 2.2 cm

answers: NDQ_002330

answers: perigee

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: perigee

answers: NDQ_002334

answers: perigee

answers: NDQ_002335

answers: total solar eclipse

answers: NDQ_002343

answers: It will no longer be able to completely cover the Sun's disk as seen from the Earth

answers: NDQ_002345

answers: the apparent angular diameter of the Moon will decrease in size

answers: NDQ_002348

answers: no longer be able to completely cover the Sun's disk

answers: NDQ_002350

answers: The apparent angular diameter of the Moon

answers: NDQ_002351

answers: the orbit of the Moon around the Earth

answers: NDQ_002352

answers: aphelion

answers: NDQ_002353

answers: total solar eclipse

answers: NDQ_002354

answers: The last total solar eclipse on Earth will occur about six hundred million years from now

answers: NDQ_002355

answers: The apparent angular diameter of the Moon will decrease in size

answers: NDQ_002356

answers: It will no longer be able to completely cover the Sun's disk as seen from the Earth

answers: NDQ_002357

answers: total solar eclipse

answers: NDQ_002358

answers: Moon will decrease in size

answers: NDQ_002359

answers: the last total solar eclipse on Earth

answers: NDQ_002360

answers: it will no longer be able to completely cover the Sun's disk as seen from the Earth

answers: NDQ_002361

answers: it will no longer be able to completely cover the Sun

answers: NDQ_002362

answers: tidal acceleration

answers: NDQ_002363

answers: Earth's disk

answers: NDQ_002364

answers: the Moon is at perigee, and the Earth at aphelion

answers: NDQ_002365

answers: 1.4 billion years

answers: NDQ_002366

answers: year

answers: NDQ_002367

answers: 2.2 cm

answers: NDQ_002368

answers: perigee

text: A partial solar eclipse occurred on June 19, 1917.  A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on June 19, 1917.  A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: partial

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answers: polar regions

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answers: totally

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answers: partly

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answers: NDQ_002328

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answers: part

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answers: misses

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answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: It does not say.

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on June 19, 1917

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: on June 19, 1917

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: The Sun

answers: NDQ_002361

answers: totally or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial

text: A lunar eclipse is potentially alluded to in Acts of the Apostles 2:14-21 ("The sun shall be turned into darkness, And the moon into blood, Before the day of the Lord come"), as pointed out by physicist Colin Humphreys and astronomer Graeme Waddington. There was in fact a lunar eclipse on 3 April AD 33, a date which coincides with one of Newton's astronomically possible crucifixion dates (see above). Humphreys and Waddington have calculated that in ancient Jerusulem this eclipse would have been visible at moonrise at 6.20pm as a 20% partial eclipse (a full moon with a potentially red "bite" missing at the top left of the moon's disc). They propose that a large proportion of the Jewish population would have witnessed this eclipse as they would have been waiting for sunset in the west and immediately afterwards the rise of the anticipated full moon in the east as the prescribed signal to start their household Passover meals. Humphreys and Waddington therefore suggest a scenario where Jesus was crucified and died at 3pm on 3 April AD 33, followed by a red partial lunar eclipse at moonrise at 6.20pm observed by the Jewish population, and that Peter recalls this event when preaching the resurrection to the Jews (Acts of the Apostles 2:14-21). Astronomer Bradley Schaefer agrees with the eclipse date but disputes that the eclipsed moon would have been visible by the time the moon had risen in Jerusalem.

text: A

text: lunar eclipse

text: is potentially alluded to in

text: Acts of the Apostles 2:14-21

text: ("The sun shall be turned into darkness, And the moon into blood, Before the day of the Lord come"), as pointed out by physicist

text: Colin Humphreys

text: Peter

text: recalls this event when preaching the resurrection to the Jews (

text: Acts of the Apostles 2:14-21

text: ). Astronomer Bradley Schaefer agrees with the eclipse date but disputes that the eclipsed moon would have been visible by the time the moon had risen in Jerusalem.

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answers: NDQ_002345

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answers: a 20% partial eclipse

answers: NDQ_002350

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answers: NDQ_002351

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text: On the Sizes and Distances (of the Sun and Moon) (Περὶ μεγεθῶν καὶ ἀποστημάτων [ἡλίου καὶ σελήνης], Peri megethon kai apostematon) is widely accepted as the only extant work written by Aristarchus of Samos, an ancient Greek astronomer who lived circa 310–230 BC. This work calculates the sizes of the Sun and Moon, as well as their distances from the Earth in terms of Earth's radius.

text: On the Sizes and Distances (of the Sun and Moon) (Περὶ μεγεθῶν καὶ ἀποστημάτων [ἡλίου καὶ σελήνης], Peri megethon kai apostematon) is widely accepted as the only extant work written by

text: Aristarchus of Samos

text: , an ancient Greek astronomer who lived circa 310–230 BC. This work calculates the sizes of the

text: Sun

text: and

text: Moon

text: , as well as their distances from the

text: Earth

text: in terms of Earth's radius.

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text: An eclipse does not happen at every new or full moon, because the plane of the orbit of the Moon around the Earth is tilted with respect to the plane of the orbit of the Earth around the Sun (the ecliptic): so as seen from the Earth, when the Moon is nearest to the Sun (new moon) or at largest distance (full moon), the three bodies usually are not exactly on the same line.

text: An eclipse does not happen at every new or full moon, because the plane of the

text: orbit of the Moon

text: around the Earth is tilted with respect to the plane of the orbit of the Earth around the Sun (the

text: ecliptic

text: ): so as seen from the Earth, when the Moon is nearest to the Sun (new moon) or at largest distance (full moon), the three bodies usually are not exactly on the same line.

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answers: NDQ_002329

answers: the Moon is nearest to the Sun

answers: NDQ_002330

answers: the Earth

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: full moon

answers: NDQ_002334

answers: the Earth

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: It does not happen at every new

answers: NDQ_002345

answers: the three bodies usually are not exactly on the same line

answers: NDQ_002348

answers: full moon

answers: NDQ_002350

answers: when the Moon is nearest to the Sun

answers: NDQ_002351

answers: full moon

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: An eclipse is a partial or total eclipse

answers: NDQ_002354

answers: An eclipse does not happen at every new or full moon

answers: NDQ_002355

answers: Moon is nearest to the Sun

answers: NDQ_002356

answers: not every month

answers: NDQ_002357

answers: when the Moon is nearest to the Sun

answers: NDQ_002358

answers: new moon

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: the three bodies usually are not exactly on the same line

answers: NDQ_002361

answers: the three bodies usually are not exactly on the same line

answers: NDQ_002362

answers: the three bodies usually are not exactly on the same line

answers: NDQ_002363

answers: orbit of the Earth around the Sun

answers: NDQ_002364

answers: when the Moon is nearest to the Sun

answers: NDQ_002365

answers: full moon

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: full moon

answers: NDQ_002368

answers: new moon

text: An eclipse is a natural phenomenon. Nevertheless, in some ancient and modern cultures, solar eclipses have been attributed to supernatural causes or regarded as bad omens. A total solar eclipse can be frightening to people who are unaware of its astronomical explanation, as the Sun seems to disappear during the day and the sky darkens in a matter of minutes.

text: An eclipse is a

text: natural phenomenon

text: . Nevertheless, in some ancient and modern cultures, solar eclipses have been attributed to

text: supernatural

text: causes or regarded as bad

text: omen

text: s. A total solar eclipse can be frightening to people who are unaware of its

text: astronomical

text: explanation, as the Sun seems to disappear during the day and the sky darkens in a matter of minutes.

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answers: NDQ_002328

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answers: NDQ_002329

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answers: NDQ_002331

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answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002345

answers: the Sun seems to disappear during the day

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Sun

answers: NDQ_002351

answers: 29.5 days

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: solar eclipses

answers: NDQ_002355

answers: A partial lunar eclipse

answers: NDQ_002356

answers: total lunar eclipse

answers: NDQ_002357

answers: total solar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: total solar eclipse

answers: NDQ_002360

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answers: NDQ_002361

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answers: NDQ_002362

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answers: NDQ_002363

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answers: NDQ_002364

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answers: NDQ_002365

answers: minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: gibbous

text: At the time of Thales' purported prediction it was not yet known that eclipses were caused by the Moon coming between the Earth and the Sun, a fact that would not be discovered until over a century later by either Anaxagoras or Empedocles.

text: At the time of

text: Thales

text: ' purported prediction it was not yet known that eclipses were caused by the Moon coming between the Earth and the Sun, a fact that would not be discovered until over a century later by either

text: Anaxagoras

text: or

text: Empedocles

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answers: eclipses

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answers: Moon and the Sun

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answers: eclipses

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answers: eclipses

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answers: eclipses

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answers: NDQ_002330

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answers: NDQ_002334

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answers: NDQ_002343

answers: Moon coming between the Earth and the Sun

answers: NDQ_002345

answers: Moon coming between the Earth and the Sun

answers: NDQ_002348

answers: Moon coming between the Earth and the Sun

answers: NDQ_002350

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answers: Moon coming between the Earth and the Sun

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: it was not yet known that eclipses were caused by the Moon coming between the Earth and the Sun

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: It was not yet known that eclipses were caused by the Moon coming between the Earth and the Sun

answers: NDQ_002357

answers: eclipses

answers: NDQ_002358

answers: the first quarter phase

answers: NDQ_002359

answers: the Moon coming between the Earth and the Sun

answers: NDQ_002360

answers: Moon coming between the Earth

answers: NDQ_002361

answers: the Moon coming between the Earth

answers: NDQ_002362

answers: eclipses

answers: NDQ_002363

answers: Moon

answers: NDQ_002364

answers: Earth and the Sun

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answers: over a century

answers: NDQ_002366

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answers: over a century

answers: NDQ_002368

answers: eclipses

text: A partial solar eclipse occurred on December 24, 1927. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on December 24, 1927. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 0

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answers: partial

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answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: part of the Moon

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Solar eclipse

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on December 24, 1927

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: December 24, 1927

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: December 24

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial solar eclipse

text: Viewed from Earth, the Moon is just far enough away to have almost the same apparent-sized disk as the Sun. The angular size (or solid angle) of these two bodies match because, although the Sun's diameter is about 400 times as large as the Moon's, it is also 400 times more distant. This allows total and annular solar eclipses to occur on Earth.

text: Viewed from Earth, the Moon is just far enough away to have almost the same apparent-sized disk as the Sun. The

text: angular size

text: (or

text: solid angle

text: ) of these two bodies match because, although the Sun's diameter is about 400 times as large as the Moon's, it is also 400 times more distant. This allows total and annular solar eclipses to occur on Earth.

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answers: annular

answers: NDQ_002324

answers: annular

answers: NDQ_002325

answers: total

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipses

answers: NDQ_002328

answers: solar eclipses

answers: NDQ_002329

answers: just far enough away

answers: NDQ_002330

answers: annular

answers: NDQ_002331

answers: solar eclipses

answers: NDQ_002332

answers: total

answers: NDQ_002334

answers: annular

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: total

answers: NDQ_002345

answers: total and annular solar eclipses

answers: NDQ_002348

answers: total

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Moon's

answers: NDQ_002352

answers: annular

answers: NDQ_002353

answers: annular

answers: NDQ_002354

answers: total and annular

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: It is just far enough away

answers: NDQ_002357

answers: solar eclipses

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: total and annular

answers: NDQ_002361

answers: solar eclipses

answers: NDQ_002362

answers: solar eclipses

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon is just far enough away to have almost the same apparent-sized disk as the Sun

answers: NDQ_002365

answers: total

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter

answers: NDQ_002368

answers: annular

text: The shadow axis passes between the Earth's center and the north pole, the minimum distance from the center of the Earth to the Moon's shadow cone axis is 3,357 kilometers. The average length of the Moon's shadow is 373,320 kilometers. The distance from the Earth to the Moon on 1 May 1185 is 347,727 kilometers. The apparent diameter of the Moon in 1.0736 times more apparent than the sun. The shadow had a maximum width of 280 kilometers. It began on the west coast of Central America and crossed the Atlantic Ocean in a northeasterly direction. The shadow passed through present-day Nicaragua and the island of Haiti. The maximum duration of the eclipse was in the middle of the North Atlantic at coordinates 46 ° N, 37.2 ° W longitude.The solar eclipse is a long total eclipse that lasted for 5 minutes and 10 seconds. The eclipse magnitude is 1.0736. The eclipse was preceded two weeks earlier by a partial lunar eclipse that happened on April 16.

text: The shadow axis passes between the Earth's center and the north pole, the minimum distance from the center of the Earth to the Moon's shadow cone axis is 3,357 kilometers. The average length of the Moon's shadow is 373,320 kilometers. The distance from the Earth to the Moon on 1 May 1185 is 347,727 kilometers. The apparent diameter of the Moon in 1.0736 times more apparent than the sun. The shadow had a maximum width of 280 kilometers. It began on the west coast of Central America and crossed the Atlantic Ocean in a northeasterly direction. The shadow passed through present-day

text: Nicaragua

text: and the island of

text: Haiti

text: . The maximum duration of the eclipse was in the middle of the North Atlantic at coordinates 46 ° N, 37.2 ° W longitude.The solar eclipse is a long total eclipse that lasted for 5 minutes and 10 seconds. The eclipse magnitude is 1.0736. The eclipse was preceded two weeks earlier by a partial lunar eclipse that happened on April 16.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 3

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answers: 3

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answers: 4

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answers: 0

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answers: 4

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answers: 4

answers: NDQ_002362

answers: 4

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answers: 0

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answers: 5

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answers: 5

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

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answers: NDQ_002323

answers: partial lunar eclipse

answers: NDQ_002324

answers: The shadow axis passes between the Earth's center and the north pole

answers: NDQ_002325

answers: total eclipse

answers: NDQ_002326

answers: partial lunar eclipse

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: two weeks earlier

answers: NDQ_002330

answers: The shadow had a maximum width of 280 kilometers

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: total

answers: NDQ_002334

answers: The shadow had a maximum width of 280 kilometers

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: A lunar eclipse usually lasts between 5-10 minutes.

answers: NDQ_002345

answers: It began on the west coast of Central America and crossed the Atlantic Ocean in a northeasterly direction. The shadow passed through present-day Nicaragua and the island of Haiti

answers: NDQ_002348

answers: The lunar eclipse was preceded two weeks earlier by a partial lunar eclipse

answers: NDQ_002350

answers: The shadow passes through present-day Nicaragua and the island of Haiti.

answers: NDQ_002351

answers: The eclipse was preceded two weeks earlier by a partial lunar eclipse that happened on April 16

answers: NDQ_002352

answers: The shadow axis passes between the Earth's center and the north pole

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow.

answers: NDQ_002354

answers: The shadow had a maximum width of 280 kilometers.

answers: NDQ_002355

answers: During a partial lunar eclipse, only part of the moon enters Earths umbra.

answers: NDQ_002356

answers: It was preceded two weeks earlier by a partial lunar eclipse

answers: NDQ_002357

answers: The solar eclipse is a long total eclipse that lasted for 5 minutes and 10 seconds

answers: NDQ_002358

answers: The lunar eclipse was preceded two weeks earlier by a partial lunar eclipse

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month.

answers: NDQ_002360

answers: The apparent diameter of the Moon is 1.0736 times more apparent than the sun.

answers: NDQ_002361

answers: The eclipse was preceded two weeks earlier by a partial lunar eclipse

answers: NDQ_002362

answers: The shadow passes through present-day Nicaragua and the island of Haiti

answers: NDQ_002363

answers: Earth's center

answers: NDQ_002364

answers: the Moon's shadow passes between the Earth's center and the north pole

answers: NDQ_002365

answers: 5 minutes and 10 seconds

answers: NDQ_002366

answers: 1185

answers: NDQ_002367

answers: two weeks

answers: NDQ_002368

answers: partial lunar eclipse

text: The full moon cycle is the period between alignments of the lunar perigee with the sun and the earth, which is about 13.9443 synodic months (about 411.8 days).  Thus approximately every 14th full moon will be a supermoon. However, halfway through the cycle the full moon will be close to apogee, and the new moons immediately before and after can be supermoons.  Thus there may be as many as three supermoons per full moon cycle.

text: The

text: full moon cycle

text: is the period between alignments of the lunar perigee with the sun and the earth, which is about 13.9443 synodic months (about 411.8 days).  Thus approximately every 14th full moon will be a supermoon. However, halfway through the cycle the full moon will be close to apogee, and the new moons immediately before and after can be supermoons.  Thus there may be as many as three supermoons per full moon cycle.

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answers: 5

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answers: 5

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answers: 4

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answers: 3

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answers: 4

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answers: NDQ_002367

answers: 4

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answers: NDQ_002323

answers: full moon

answers: NDQ_002324

answers: perigee

answers: NDQ_002325

answers: full moon

answers: NDQ_002326

answers: full

answers: NDQ_002327

answers: alignments

answers: NDQ_002328

answers: supermoon

answers: NDQ_002329

answers: about 411.8 days

answers: NDQ_002330

answers: perigee

answers: NDQ_002331

answers: alignments

answers: NDQ_002332

answers: full moon

answers: NDQ_002334

answers: perigee

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: about 411.8 days

answers: NDQ_002345

answers: the solar perigee with the sun

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The full moon cycle

answers: NDQ_002351

answers: 411.8 days

answers: NDQ_002352

answers: The lunar perigee

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: solar eclipses are rare events

answers: NDQ_002355

answers: Partially lunar eclipse

answers: NDQ_002356

answers: approximately every 14th full moon

answers: NDQ_002357

answers: alignments

answers: NDQ_002358

answers: full moon

answers: NDQ_002359

answers: 411.8 days

answers: NDQ_002360

answers: full moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: full moon cycle

answers: NDQ_002363

answers: sun

answers: NDQ_002364

answers: alignments of the lunar perigee with the sun

answers: NDQ_002365

answers: 411.8 days

answers: NDQ_002366

answers: 411.8 days

answers: NDQ_002367

answers: 411.8 days

answers: NDQ_002368

answers: new moons

text: An annular solar eclipse will occur on October 14, 2088. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on October 14, 2088. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 0

answers: NDQ_002323

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answers: NDQ_002324

answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 4

answers: NDQ_002328

answers: 4

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: the Moon passes between Earth and the Sun

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: (ring)

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: An annular solar eclipse will occur on October 14, 2088

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On October 14, 2088

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: October

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 2088

answers: NDQ_002368

answers: crescent

text: Writing for Earth & Sky Bruce McClure and Deborah Byrd point out that the referenced verse also says the "sun will be turned into darkness", an apparent reference to a solar eclipse. They note that since the Jewish Calendar is lunar, one sixth of all eclipses will occur during Passover or Sukkot.  Furthermore, there have been 62 tetrads since the first century AD, though only eight of them have coincided with both feasts. Thus, the event is not as unusual as Hagee and Biltz imply. Additionally, three of the four eclipses in the tetrad were not even visible in the biblical homeland of Israel, casting further doubt on Hagee and Biltz's interpretation; even then, only the very end of the last eclipse was visible in Israel. Writing for Space.com, Geoff Gaherty said he was saddened that 'prophets of doom' ... view these life-enriching events as portents of disaster" and said the eclipse was "hardly something to be concerned about".

text: Writing for Earth & Sky Bruce McClure and

text: Deborah Byrd

text: point out that the referenced verse also says the "sun will be turned into darkness", an apparent reference to a

text: solar eclipse

text: . They note that since the

text: Jewish Calendar

text: is lunar, one sixth of all eclipses will occur during Passover or Sukkot.  Furthermore, there have been 62

text: tetrads

text: since the first century AD, though only eight of them have coincided with both feasts. Thus, the event is not as unusual as Hagee and Biltz imply. Additionally, three of the four eclipses in the tetrad were not even visible in the biblical homeland of

text: Israel

text: , casting further doubt on Hagee and Biltz's interpretation; even then, only the very end of the last eclipse was visible in Israel. Writing for

text: Space.com

text: , Geoff Gaherty said he was saddened that 'prophets of doom' ... view these life-enriching events as portents of disaster" and said the eclipse was "hardly something to be concerned about".

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answers: NDQ_002324

answers: sun will be turned into darkness

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: eclipse

answers: NDQ_002327

answers: solar eclipse

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answers: one sixth

answers: NDQ_002330

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answers: NDQ_002331

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answers: eclipse

answers: NDQ_002334

answers: the very end

answers: NDQ_002335

answers: Sukkot

answers: NDQ_002343

answers: The eclipse was "hardly something to be concerned about"

answers: NDQ_002345

answers: the "sun will be turned into darkness"

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The sun will be turned into darkness

answers: NDQ_002351

answers: The Jewish Calendar is lunar

answers: NDQ_002352

answers: The sun will be turned into darkness

answers: NDQ_002353

answers: The sun will be turned into darkness

answers: NDQ_002354

answers: one sixth of all eclipses will occur during Passover or Sukkot

answers: NDQ_002355

answers: Earth & Sky

answers: NDQ_002356

answers: one sixth of all eclipses

answers: NDQ_002357

answers: solar eclipse

answers: NDQ_002358

answers: The eclipse was "hardly something to be concerned about

answers: NDQ_002359

answers: Jewish Calendar

answers: NDQ_002360

answers: The sun will be turned into darkness

answers: NDQ_002361

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answers: NDQ_002362

answers: eclipses

answers: NDQ_002363

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answers: NDQ_002364

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answers: NDQ_002365

answers: the very end

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: one sixth

answers: NDQ_002368

answers: epidermis

text: A full moon is the lunar phase that occurs when the Moon is completely illuminated as seen from Earth. This occurs when Earth is located directly between the Sun and the Moon (more exactly, when the ecliptic longitudes of the Sun and Moon differ by 180 degrees). This means that the hemisphere of the Moon that is facing Earth (the near side) is almost fully illuminated by the Sun and appears round (while the far side is almost completely unilluminated). On some occasions at the time of full moon there is also a lunar eclipse so the moon's face appears reddish due to the rayleigh scattering of blue light in Earth's atmosphere.

text: A full moon is the

text: lunar phase

text: that occurs when the

text: Moon

text: is completely illuminated as seen from

text: Earth

text: . This occurs when Earth is located directly between the

text: Sun

text: and the Moon (more exactly, when the

text: ecliptic longitude

text: s of the Sun and Moon differ by 180 degrees). This means that the hemisphere of the Moon that is facing Earth (the

text: near side

text: ) is almost fully illuminated by the Sun and appears round (while the

text: far side

text: is almost completely unilluminated). On some occasions at the time of full moon there is also a

text: lunar eclipse

text: so the moon's face appears reddish due to the

text: rayleigh scattering

text: of blue light in Earth's

text: atmosphere

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answers: NDQ_002326

answers: full moon

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

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answers: NDQ_002331

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answers: NDQ_002343

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answers: NDQ_002345

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answers: NDQ_002356

answers: On some occasions

answers: NDQ_002357

answers: The far side is almost completely unilluminated

answers: NDQ_002358

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answers: NDQ_002360

answers: Moon is completely illuminated

answers: NDQ_002361

answers: The Moon is completely illuminated

answers: NDQ_002362

answers: rayleigh scattering of blue light

answers: NDQ_002363

answers: longitudes

answers: NDQ_002364

answers: Earth is located directly between the Sun and the Moon

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answers: 180 degrees

answers: NDQ_002366

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text: In Western culture, the four principal lunar phases are new moon, first quarter, full moon, and third quarter (also known as last quarter). These are the instants when the Moon's apparent geocentric celestial longitude minus the Sun's apparent geocentric celestial longitude is 0°, 90°, 180° and 270°, respectively. Each of these phases is instantaneous, lasting theoretically zero time, although they occur at slightly different times when viewed from different points on the Earth. During the intervals between principal phases, the Moon appears either crescent-shaped or gibbous. These shapes, and the periods of time when the Moon shows them, are called the intermediate phases. They last, on average, one-quarter of a synodic month, roughly 7.38 days, but their durations vary slightly because the Moon's orbit is slightly elliptical, and thus its speed in orbit is not constant. The descriptor waxing is used for an intermediate phase when the Moon's apparent size is increasing, from new moon toward full moon, and waning when the size is decreasing.

text: In

text: Western culture

text: , the four principal lunar phases are new moon, first quarter, full moon, and third quarter (also known as last quarter). These are the instants when the Moon's apparent geocentric

text: celestial longitude

text: minus the Sun's apparent geocentric celestial longitude is 0°, 90°, 180° and 270°, respectively. Each of these phases is instantaneous, lasting theoretically zero time, although they occur at slightly different times when viewed from different points on the Earth. During the intervals between principal phases, the Moon appears either

text: crescent

text: -shaped or

text: gibbous

text: . These shapes, and the periods of time when the Moon shows them, are called the intermediate phases. They last, on average, one-quarter of a

text: synodic month

text: , roughly 7.38 days, but their durations vary slightly because the Moon's orbit is slightly

text: elliptical

text: , and thus its speed in orbit is not constant. The descriptor waxing is used for an intermediate phase when the Moon's apparent size is increasing, from new moon toward full moon, and waning when the size is decreasing.

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answers: quarter of a synodic month

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answers: The four principal lunar phases are new moon, first quarter, full moon, and third quarter (also known as last quarter)

answers: NDQ_002348

answers: Moon's apparent geocentric celestial longitude

answers: NDQ_002350

answers: solar eclipse is seen on all of the Earth that is having daytime

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answers: one-quarter of a synodic month

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answers: crescent-shaped

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answers: Umbra

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answers: Solar eclipses are rare events

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answers: Moon's apparent geocentric celestial longitude

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answers: 270°

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answers: third quarter

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answers: When the Moon's apparent geocentric longitude minus the Sun's apparent geocentric longitude is 0°, 90°, 180° and 270°, respectively

answers: NDQ_002361

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answers: the Moon's apparent geocentric longitude minus the Sun's apparent geocentric longitude

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answers: when the Moon's apparent geocentric longitude minus the Sun's apparent geocentric longitude is 0°

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text: A primitive way to determine the distance to the Sun in terms of the distance to the Moon was already proposed by Aristarchus of Samos in his book On the Sizes and Distances of the Sun and Moon. He noted that the Sun, Moon, and Earth form a right triangle (right angle at the Moon) at the moment of first or last quarter moon. He then estimated that the Moon, Earth, Sun angle was 87°. Using correct geometry but inaccurate observational data, Aristarchus concluded that the Sun was slightly less than 20 times farther away than the Moon. The true value of this angle is close to 89° 50', and the Sun is actually about 390 times farther away. He pointed out that the Moon and Sun have nearly equal apparent angular sizes and therefore their diameters must be in proportion to their distances from Earth. He thus concluded that the Sun was around 20 times larger than the Moon; this conclusion, although incorrect, follows logically from his incorrect data. It does suggest that the Sun is clearly larger than the Earth, which could be taken to support the heliocentric model.

text: A primitive way to determine the distance to the Sun in terms of the distance to the Moon was already proposed by

text: Aristarchus of Samos

text: in his book

entity_name: On the Sizes and Distances (Aristarchus)

text: On the Sizes and Distances of the Sun and Moon

text: . He noted that the Sun, Moon, and Earth form a right triangle (right angle at the Moon) at the moment of

text: first or last quarter moon

text: . He then estimated that the Moon, Earth, Sun angle was 87°. Using correct

text: geometry

text: but inaccurate observational data, Aristarchus concluded that the Sun was slightly less than 20 times farther away than the Moon. The true value of this angle is close to 89° 50', and the Sun is actually about 390 times farther away. He pointed out that the Moon and Sun have nearly equal

text: apparent angular sizes

text: and therefore their diameters must be in proportion to their distances from Earth. He thus concluded that the Sun was around 20 times larger than the Moon; this conclusion, although incorrect, follows logically from his incorrect data. It does suggest that the Sun is clearly larger than the Earth, which could be taken to support the heliocentric model.

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answers: total lunar eclipse

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answers: Penumbra

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answers: quarter moon

text: The only close-up images of Ariel were obtained by the Voyager 2 probe, which photographed the moon during its flyby of Uranus in January 1986. The closest approach of Voyager 2 to Ariel was —significantly less than the distances to all other Uranian moons except Miranda. The best images of Ariel have a spatial resolution of about 2 km. They cover about 40% of the surface, but only 35% was photographed with the quality required for geological mapping and crater counting. At the time of the flyby the southern hemisphere of Ariel (like those of the other moons) was pointed towards the Sun, so the northern (dark) hemisphere could not be studied. No other spacecraft has ever visited the Uranian system, and no mission to Uranus and its moons is planned. The possibility of sending the Cassini spacecraft to Uranus was evaluated during its mission extension planning phase. It would take about twenty years to get to the Uranian system after departing Saturn.

text: The only close-up images of Ariel were obtained by the

text: Voyager 2

text: probe, which photographed the moon during its flyby of Uranus in January 1986. The closest approach of Voyager 2 to Ariel was —significantly less than the distances to all other Uranian moons except Miranda. The best images of Ariel have a spatial resolution of about 2 km. They cover about 40% of the surface, but only 35% was photographed with the quality required for

text: geological mapping

text: and crater counting. At the time of the flyby the southern hemisphere of Ariel (like those of the other moons) was pointed towards the Sun, so the northern (dark) hemisphere could not be studied. No other spacecraft has ever visited the Uranian system, and no mission to Uranus and its moons is planned. The possibility of sending the

text: Cassini spacecraft

text: to Uranus was evaluated during its mission extension planning phase. It would take about twenty years to get to the Uranian system after departing Saturn.

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answers: flyby

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answers: northern (dark) hemisphere could not be studied

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answers: The northern (dark) hemisphere could not be studied

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answers: At the time of the flyby the southern hemisphere

answers: NDQ_002356

answers: January 1986

answers: NDQ_002357

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answers: about twenty years

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answers: dark

text: An annual solar eclipse occurred on November 12, 1947. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annual

text: solar eclipse

text: occurred on November 12, 1947. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: partial

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answers: totally or partly

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: annular

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: annular

answers: NDQ_002343

answers: An annular solar eclipse

answers: NDQ_002345

answers: The Moon passes between Earth and the Sun

answers: NDQ_002348

answers: solar eclipse

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: An annual solar eclipse

answers: NDQ_002355

answers: An annular solar eclipse

answers: NDQ_002356

answers: annual

answers: NDQ_002357

answers: solar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: November

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answers: NDQ_002361

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answers: NDQ_002362

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answers: NDQ_002363

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answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: annual

answers: NDQ_002367

answers: 12

answers: NDQ_002368

answers: crescent

text: The physical problem was addressed by Amerigo Vespucci and subsequently by Galileo Galilei; in 1499 Vespucci used knowledge of the position of the moon to determine his position in Brazil. It became of technical importance in the 1720s, as an accurate solution would be applicable to navigation, specifically for the determination of longitude at sea, solved in practice by John Harrison's invention of the Marine chronometer. However the accuracy of the lunar theory was low, due to the perturbing effect of the Sun and planets on the motion of the Moon around the Earth.

text: The physical problem was addressed by

text: Amerigo Vespucci

text: and subsequently by

text: Galileo Galilei

text: ; in 1499 Vespucci used knowledge of the position of the moon to determine his position in Brazil. It became of technical importance in the 1720s, as an accurate solution would be applicable to navigation, specifically for the

text: determination of longitude at sea

text: , solved in practice by

text: John Harrison

text: 's invention of the

text: Marine chronometer

text: . However the accuracy of the

text: lunar theory

text: was low, due to the perturbing effect of the Sun and planets on the motion of the Moon around the Earth.

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answers: lunar

answers: NDQ_002326

answers: right

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answers: the Moon around the Earth

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answers: longitude at sea

answers: NDQ_002329

answers: half moon

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answers: NDQ_002332

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answers: the Moon around the Earth

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answers: total lunar eclipse

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answers: the penumbra

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answers: Umbra

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answers: Solar eclipses are rare events

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answers: Earths umbra

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answers: The full moon phase

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answers: one month

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text: A supermoon is the coincidence of a full moon or a new moon with the closest approach the Moon makes to the Earth on its elliptical orbit, resulting in the largest apparent size of the lunar disk as seen from Earth. The technical name is the perigee-syzygy of the Earth–Moon–Sun system. The term supermoon is not astronomical, but originated in modern astrology. The association of the Moon with both oceanic and crustal tides has led to claims that the supermoon phenomenon may be associated with increased risk of events such as earthquakes and volcanic eruptions, but there is no evidence of such a link.

text: A supermoon is the coincidence of a

text: full moon

text: or a

text: new moon

text: with the closest approach the

text: Moon

text: makes to the Earth on its elliptical orbit, resulting in the largest apparent size of the lunar disk as seen from Earth. The technical name is the perigee-syzygy of the Earth–Moon–Sun system. The term supermoon is not

text: astronomical

text: , but originated in modern

text: astrology

text: . The association of the Moon with both oceanic and

text: crustal tide

text: s has led to claims that the supermoon phenomenon may be associated with increased risk of events such as earthquakes and volcanic eruptions, but there is no evidence of such a link.

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answers: NDQ_002327

answers: A supermoon

answers: NDQ_002328

answers: the largest apparent size of the lunar disk

answers: NDQ_002329

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answers: NDQ_002330

answers: perigee

answers: NDQ_002331

answers: A supermoon

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answers: supermoon

answers: NDQ_002334

answers: perigee

answers: NDQ_002335

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answers: NDQ_002343

answers: A lunar eclipse generally lasts between 5-10 minutes

answers: NDQ_002345

answers: supermoon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth–Moon–Sun system

answers: NDQ_002351

answers: supermoon

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answers: supermoon

answers: NDQ_002355

answers: Earth–Moon–Sun

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answers: full moon or a new moon

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answers: A supermoon

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answers: earthquakes and volcanic eruptions

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text: This is a list of solar eclipses in the 11th century BC. During the period 1100 to 1001 BC there were 238 solar eclipses of which 79 were partial, 91 were annular (two non-central), 68 were total (one non-central), and none were hybrids. The greatest number of eclipses in one year was five, in 1090 BC, and three months, August 1036 BC, July 1025 BC, and June 1014 BC, had two eclipses.

text: This is a list of

text: solar eclipses

text: in the

text: 11th century BC

text: . During the period 1100 to 1001 BC there were 238 solar eclipses of which 79 were

text: partial

text: , 91 were

text: annular

text: (two

text: non-central

text: ), 68 were

text: total

text: (one non-central), and none were

text: hybrids

text: . The greatest number of eclipses in one year was five, in 1090 BC, and three months, August 1036 BC, July 1025 BC, and June 1014 BC, had two eclipses.

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answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

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answers: NDQ_002330

answers: annular

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: annular

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: solar eclipses

answers: NDQ_002345

answers: solar eclipses

answers: NDQ_002348

answers: total

answers: NDQ_002350

answers: solar eclipses

answers: NDQ_002351

answers: three months

answers: NDQ_002352

answers: annular

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: There were 238 solar eclipses

answers: NDQ_002355

answers: partial

answers: NDQ_002356

answers: June 1014 BC

answers: NDQ_002357

answers: solar

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: August

answers: NDQ_002360

answers: solar eclipses

answers: NDQ_002361

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answers: three months

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answers: month

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answers: three months

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answers: partial

text: Because its orbit takes it between the Earth and the Sun, Venus as seen from Earth exhibits visible phases in much the same manner as the Earth's Moon. Galileo Galilei was the first person to observe the phases of Venus in December 1610, an observation which supported Copernicus's then contentious heliocentric description of the Solar System. He also noted changes in the size of Venus's visible diameter when it was in different phases, suggesting that it was farther from Earth when it was full and nearer when it was a crescent. This observation strongly supported the heliocentric model. Venus (and also Mercury) is not visible from Earth when it is full, since at that time it is at superior conjunction, rising and setting concomitantly with the Sun and hence lost in the Sun's glare.

text: Because its

text: orbit

text: takes it between the Earth and the Sun, Venus as seen from Earth exhibits visible

text: phases

text: in much the same manner as the Earth's Moon.

text: Galileo Galilei

text: was the first person to observe the phases of Venus in December 1610, an observation which supported

text: Copernicus

text: 's then contentious

text: heliocentric

text: description of the Solar System. He also noted changes in the size of Venus's visible diameter when it was in different phases, suggesting that it was farther from Earth when it was full and nearer when it was a crescent. This observation strongly supported the heliocentric model. Venus (and also Mercury) is not visible from Earth when it is full, since at that time it is at

text: superior conjunction

text: , rising and setting concomitantly with the Sun and hence lost in the Sun's glare.

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answers: Earth's Moon

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answers: crescent

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answers: Venus as seen from Earth

answers: NDQ_002328

answers: Venus as seen from Earth exhibits visible phases

answers: NDQ_002329

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answers: NDQ_002330

answers: Venus

answers: NDQ_002331

answers: superior conjunction

answers: NDQ_002332

answers: full

answers: NDQ_002334

answers: Venus

answers: NDQ_002335

answers: crescent

answers: NDQ_002343

answers: Earth's Moon

answers: NDQ_002345

answers: Venus as seen from Earth exhibits visible phases

answers: NDQ_002348

answers: Venus

answers: NDQ_002350

answers: Venus (and also Mercury)

answers: NDQ_002351

answers: Earth's Moon

answers: NDQ_002352

answers: Venus

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answers: Umbra

answers: NDQ_002354

answers: Venus is not visible from Earth when it is full

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: Earth's Moon

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answers: Venus

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answers: December

answers: NDQ_002360

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answers: Venus is not visible from Earth when it is full

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answers: rising and setting concomitantly

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answers: a few minutes

answers: NDQ_002366

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answers: crescent

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answers: crescent

text: The gravitational force between the Sun and moon induces the precession in Earth's orbit, which is the major cause of the climate oscillation of Earth that has a period of 19,000 to 23,000 years. It follows that changes in Earth's orbital parameters (e.g., orbital inclination, the angle between Earth's rotation axis and its plane of orbit) is important to the study of Earth's climate, in particular to the study of past ice ages. (See also nodal precession. For precession of the lunar orbit see lunar precession).

text: The gravitational force between the Sun and moon induces the precession in Earth's orbit, which is the major cause of the climate oscillation of Earth that has a period of 19,000 to 23,000 years. It follows that changes in Earth's orbital parameters (e.g., orbital inclination, the angle between Earth's rotation axis and its plane of orbit) is important to the study of Earth's climate, in particular to the study of past ice ages. (See also

text: nodal precession

text: . For precession of the lunar orbit see

text: lunar precession

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answers: lunar

answers: NDQ_002324

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answers: NDQ_002325

answers: Nodal

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: gravitational force

answers: NDQ_002328

answers: climate oscillation

answers: NDQ_002329

answers: 19,000 to 23,000 years

answers: NDQ_002330

answers: Earth's orbit

answers: NDQ_002331

answers: lunar precession

answers: NDQ_002332

answers: moon

answers: NDQ_002334

answers: Earth's orbit

answers: NDQ_002335

answers: lunar

answers: NDQ_002343

answers: Lunar eclipse

answers: NDQ_002345

answers: The gravitational force between the Sun and moon induces the precession

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth's orbit

answers: NDQ_002351

answers: 19,000 to 23,000 years

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: 19,000 to 23,000 years

answers: NDQ_002355

answers: Earth's umbra

answers: NDQ_002356

answers: nodal precession

answers: NDQ_002357

answers: Earth's orbit

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 1st of the month

answers: NDQ_002360

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answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: precession in Earth's orbit

answers: NDQ_002363

answers: plane of orbit

answers: NDQ_002364

answers: the Sun and moon

answers: NDQ_002365

answers: 19,000 to 23,000 years

answers: NDQ_002366

answers: 23,000 years

answers: NDQ_002367

answers: 19,000 to 23,000 years

answers: NDQ_002368

answers: lunar perigee

text: An annular solar eclipse occurred on December 4, 1983. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: occurred on December 4, 1983. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: (ring)

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: An annular solar eclipse

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: It does not say.

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: December

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 4

answers: NDQ_002368

answers: partial

text: Tidal forces arise when the gravitational field is not uniform and gravitation gradients exist. Such indeed is the norm and strictly speaking any object of finite size even in free-fall is subject to tidal effects. These are impossible to remove by inertial motion, except at one single nominated point of the body.The Earth is in free fall but the presence of tides indicates that it is in a non-uniform gravitational field. This non-uniformity is more due to the moon than the sun. The total gravitational field due to the sun is much stronger than that of the moon but it has a minor tidal effect compared with that of the moon because of the relative distances involved. Weight of the earth is essentially due to the sun's gravity. But its state of stress and deformation, represented by the tides, is more due to non uniformity in the gravitational field of the nearby moon.When the size of a region being considered is small relative to its distance from the gravitating mass the assumption of uniform gravitational field holds to a good approximation. Thus a person is small relative to the radius of Earth and the field for a person at the surface of the earth is approximately uniform. The field is strictly not uniform and is responsible for the phenomenon of microgravity. Objects near a black hole are subject to a highly non-uniform gravitational field.

text: Tidal forces

text: microgravity

text: . Objects near a

text: black hole

text: are subject to a highly non-uniform gravitational field.

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answers: NDQ_002323

answers: Tidal

answers: NDQ_002324

answers: the moon

answers: NDQ_002325

answers: black hole

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: Tidal forces

answers: NDQ_002328

answers: tides

answers: NDQ_002329

answers: finite size

answers: NDQ_002330

answers: is impossible to remove by inertial motion

answers: NDQ_002331

answers: Tidal forces

answers: NDQ_002332

answers: black hole

answers: NDQ_002334

answers: surface of the Earth

answers: NDQ_002335

answers: Tides

answers: NDQ_002343

answers: Tidal forces arise when the gravitational field is not uniform

answers: NDQ_002345

answers: This non-uniformity is more due to the moon than the sun

answers: NDQ_002348

answers: nominated point of the body

answers: NDQ_002350

answers: The total gravitational field due to the sun is much stronger than that of the moon

answers: NDQ_002351

answers: This non-uniformity is more due to the moon than the sun

answers: NDQ_002352

answers: Tidal forces arise when the gravitational field is not uniform

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow.

answers: NDQ_002354

answers: The total gravitational field due to the sun is much stronger than that of the moon

answers: NDQ_002355

answers: The Earth is in free fall

answers: NDQ_002356

answers: It does not.

answers: NDQ_002357

answers: This non-uniformity is more due to the moon than the sun

answers: NDQ_002358

answers: The Earth is in free fall

answers: NDQ_002359

answers: The Earth is in free fall

answers: NDQ_002360

answers: Moon is much stronger than that of the sun

answers: NDQ_002361

answers: Earth is in free fall

answers: NDQ_002362

answers: the presence of tides

answers: NDQ_002363

answers: Black hole

answers: NDQ_002364

answers: the sun is much stronger than that of the moon

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: gibbous

text: The Earth's shadow or umbra is as curved as the planet Earth is, and it extends 1.4 million kilometers into space (the antumbra, however, extends indefinitely). When the Sun, the Earth and the Moon are aligned perfectly (or almost perfectly), with the Earth in between the Sun and the Moon, the Earth's shadow falls onto the surface of the Moon which is facing the night side of the Earth, such that observers see the shadow gradually turn the bright full Moon dark, and then light again, creating a lunar eclipse.

text: The Earth's shadow or

text: umbra

text: is as curved as the planet Earth is, and it extends 1.4 million kilometers into space (the

text: antumbra

text: , however, extends indefinitely). When the

text: Sun

text: , the Earth and the

text: Moon

text: are aligned perfectly (or almost perfectly), with the Earth in between the Sun and the Moon, the Earth's shadow falls onto the surface of the Moon which is facing the night side of the Earth, such that observers see the shadow gradually turn the bright full Moon dark, and then light again, creating a

text: lunar eclipse

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answers: antumbra

answers: NDQ_002325

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answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

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answers: lunar eclipse

answers: NDQ_002332

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answers: NDQ_002363

answers: 0

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answers: 4

answers: NDQ_002365

answers: 0

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answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: full

answers: NDQ_002324

answers: umbra

answers: NDQ_002325

answers: full

answers: NDQ_002326

answers: full Moon

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: full Moon

answers: NDQ_002330

answers: umbra

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: full

answers: NDQ_002334

answers: the antumbra

answers: NDQ_002335

answers: full

answers: NDQ_002343

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002345

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002348

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002350

answers: The Earth's shadow falls onto the surface of the Moon

answers: NDQ_002351

answers: full Moon dark, and then light again

answers: NDQ_002352

answers: the antumbra

answers: NDQ_002353

answers: the antumbra

answers: NDQ_002354

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002355

answers: the Earth's shadow falls onto the surface of the Moon

answers: NDQ_002356

answers: It extends 1.4 million kilometers into space

answers: NDQ_002357

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002361

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002362

answers: creating a lunar eclipse

answers: NDQ_002363

answers: Earth's shadow

answers: NDQ_002364

answers: When the Sun, the Earth and the Moon are aligned perfectly

answers: NDQ_002365

answers: 1.4 million kilometers

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: full Moon

answers: NDQ_002368

answers: night

text: A partial solar eclipse occurred on July 21, 1906. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on July 21, 1906. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 5

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: part

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: It does not say.

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: on July 21, 1906

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: July 21, 1906

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: July 21

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial solar eclipse

text: During a total solar eclipse, the Moon's shadow covers only a small fraction of the Earth. The Earth continues to receive at least 92 percent of the amount of sunlight it receives without an eclipse – more if the penumbra of the Moon's shadow partly misses the Earth. Seen from the Moon, the Earth during a total solar eclipse is mostly brilliantly illuminated, with only a small dark patch showing the Moon's shadow. The brilliantly-lit Earth reflects a lot of light to the Moon. If the corona of the eclipsed Sun were not present, the Moon, illuminated by earthlight, would be easily visible from Earth. This would be essentially the same as the earthshine which can frequently be seen when the Moon's phase is a narrow crescent. In reality, the corona, though much less brilliant than the Sun's photosphere, is much brighter than the Moon illuminated by earthlight. Therefore, by contrast, the Moon during a total solar eclipse appears to be black, with the corona surrounding it.

text: During a total solar eclipse, the Moon's shadow covers only a small fraction of the Earth. The Earth continues to receive at least 92 percent of the amount of sunlight it receives without an eclipse – more if the

text: penumbra

text: of the Moon's shadow partly misses the Earth. Seen from the Moon, the Earth during a total solar eclipse is mostly brilliantly illuminated, with only a small dark patch showing the Moon's shadow. The brilliantly-lit Earth reflects a lot of light to the Moon. If the

text: corona

text: of the eclipsed Sun were not present, the Moon, illuminated by earthlight, would be easily visible from Earth. This would be essentially the same as the

text: earthshine

text: which can frequently be seen when the Moon's

text: phase

text: is a narrow crescent. In reality, the corona, though much less brilliant than the Sun's

text: photosphere

text: , is much brighter than the Moon illuminated by earthlight. Therefore, by contrast, the Moon during a total solar eclipse appears to be black, with the corona surrounding it.

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answers: 5

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answers: 4

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answers: 4

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answers: 4

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answers: crescent

answers: NDQ_002324

answers: Moon's shadow

answers: NDQ_002325

answers: total solar eclipse

answers: NDQ_002326

answers: a narrow crescent

answers: NDQ_002327

answers: total solar eclipse

answers: NDQ_002328

answers: total solar eclipse

answers: NDQ_002329

answers: a narrow crescent

answers: NDQ_002330

answers: penumbra

answers: NDQ_002331

answers: total solar eclipse

answers: NDQ_002332

answers: black

answers: NDQ_002334

answers: penumbra

answers: NDQ_002335

answers: total solar eclipse

answers: NDQ_002343

answers: It generally lasts between 5-10 minutes.

answers: NDQ_002345

answers: The Earth continues to receive at least 92 percent of the amount of sunlight it receives without an eclipse

answers: NDQ_002348

answers: The corona

answers: NDQ_002350

answers: The Moon's shadow covers only a small fraction of the Earth

answers: NDQ_002351

answers: Moon's phase is a narrow crescent

answers: NDQ_002352

answers: Moon's shadow covers only a small fraction of the Earth

answers: NDQ_002353

answers: Moon's shadow partly misses the Earth

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: The Moon's shadow covers only a small fraction of the Earth

answers: NDQ_002356

answers: It occurs once every month

answers: NDQ_002357

answers: total solar eclipse

answers: NDQ_002358

answers: Narrow crescent

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: The Moon's shadow covers only a small fraction of the Earth

answers: NDQ_002361

answers: The Moon's shadow covers only a small fraction of the Earth

answers: NDQ_002362

answers: a total solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon's shadow covers only a small fraction of the Earth

answers: NDQ_002365

answers: total

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: narrow crescent

text: Although she only lived to be twenty-nine, Wang Zhenyi was very accomplished in the academic world. She excelled in astronomy and mathematics. One of her contributions was being able to describe her views of celestial phenomena in her article, "Dispute of the Procession of the Equinoxes." She was able to explain and simply prove how equinoxes move and then how to calculate their movement. She wrote many other articles such as "Dispute of Longitude and Stars" as well as "The Explanation of a Lunar Eclipse." She commented on the number of stars; the revolving direction of the sun, the moon, and the planets Venus, Jupiter, Mars, Mercury, and Saturn; as well as describing the relationship between lunar and solar eclipses. Not only did she study the research of other astronomers, but she was also able to do her own original research.

text: Although she only lived to be twenty-nine, Wang Zhenyi was very accomplished in the academic world. She excelled in astronomy and mathematics. One of her contributions was being able to describe her views of celestial phenomena in her article, "Dispute of the Procession of the Equinoxes." She was able to explain and simply prove how equinoxes move and then how to calculate their movement. She wrote many other articles such as "Dispute of Longitude and Stars" as well as "The Explanation of a Lunar Eclipse." She commented on the number of stars; the revolving direction of the sun, the moon, and the planets Venus, Jupiter, Mars, Mercury, and Saturn; as well as describing the relationship between lunar and solar eclipses. Not only did she study the research of other astronomers, but she was also able to do her own original research.

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answers: Lunar Eclipse

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answers: Eclipse

text: This eclipse occurred at the descending node of the moon's orbit. Lunar eclipses are always paired with a solar eclipse either 2 weeks before or after at new moon in the opposite node. In this case, it was followed by a partial solar eclipse at the ascending node on January 4, 2011, visible from Europe, northern Africa, and western Asia.

text: This eclipse occurred at the descending node of the moon's orbit. Lunar eclipses are always paired with a solar eclipse either 2 weeks before or after at

text: new moon

text: in the opposite node. In this case, it was followed by a partial

text: solar eclipse

text: at the ascending node on

text: January 4, 2011

text: , visible from Europe, northern Africa, and western Asia.

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text: The display on the clock is based upon the geocentric model, which was not superseded until the advent of heliocentrism in the late 16th century.  The earth is represented by a green sphere positioned in the centre of the clock face.  The sun points to the hour of day. The gold/black orb represents the moon, and shows the lunar phases.  At full moon, it is golden and at new moon it is black.  For intermediate phases it is partially black and gold in proportion to the phase.

text: The display on the clock is based upon the

text: geocentric model

text: , which was not superseded until the advent of

text: heliocentrism

text: in the late 16th century.  The earth is represented by a green sphere positioned in the centre of the clock face.  The sun points to the hour of day. The gold/black orb represents the moon, and shows the lunar phases.  At full moon, it is golden and at new moon it is black.  For intermediate phases it is partially black and gold in proportion to the phase.

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text: The major activities of predicting the phases of moon take place in the Pakistan Naval Observatory, Department of Mathematics of the Karachi University and the Institute of Space and Planetary Astrophysics (ISPA), where the institutes provide scientific background of the motion of lunar phases and appearances to the ministry of religious affairs.

text: The major activities of predicting the phases of moon take place in the

text: Pakistan Naval Observatory

text: , Department of Mathematics of the

text: Karachi University

text: and the

entity_name: Institute of Space and Planetary Astrophysics

text: Institute of Space and Planetary Astrophysics

text: (ISPA), where the institutes provide scientific background of the motion of lunar phases and appearances to the ministry of religious affairs.

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text: Schyrleus was a determined anticopernican.  In the foreword of its book, which includes a dedication to Jesus Christ and Ferdinand III, Schyrleus boldly declared that after having meditated for a long time on the systems of Ptolemy, Copernicus, Tycho Brahe, and other astronomers, he was convinced that all of these scientists had advanced superfluous theories.  He dedicated the moons of Jupiter to Pope Urban VIII, calling them Astres Urbanoctavianes.  He also wrote that Saturn had two "companions," and that they were periodically eclipsed by the planet. He deduced that they had their own independent orbits, and that they illuminated Saturn, which needed light as it was a hundred times less lit by the sun than the Earth.  He tells us that in 1642, in Cologne, he saw pass in front of the Sun a troop (turnam) of shooting stars that followed one another during a period fourteen days, and that the glare of the Sun was considerably weakened by it.

text: Schyrleus was a determined

text: anticopernican

text: .  In the foreword of its book, which includes a dedication to

text: Jesus Christ

text: and

text: Ferdinand III

text: , Schyrleus boldly declared that after having meditated for a long time on the systems of

text: Ptolemy

text: Copernicus

text: Tycho Brahe

text: , and other astronomers, he was convinced that all of these scientists had advanced superfluous theories.  He dedicated the

text: moons of Jupiter

text: to Pope

text: Urban VIII

text: , calling them Astres Urbanoctavianes.  He also wrote that

text: Saturn

text: had two "companions," and that they were periodically eclipsed by the planet. He deduced that they had their own independent

text: orbit

text: s, and that they illuminated Saturn, which needed light as it was a hundred times less lit by the sun than the

text: Earth

text: .  He tells us that in 1642, in

text: Cologne

text: , he saw pass in front of the Sun a troop (turnam) of shooting stars that followed one another during a period fourteen days, and that the glare of the Sun was considerably weakened by it.

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answers: 4

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answers: 14 days

answers: NDQ_002366

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answers: 0

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answers: NDQ_002323

answers: eclipsed

answers: NDQ_002324

answers: moons of Jupiter

answers: NDQ_002325

answers: eclipsed

answers: NDQ_002326

answers: turnam

answers: NDQ_002327

answers: eclipsed

answers: NDQ_002328

answers: eclipsed

answers: NDQ_002329

answers: fourteen days

answers: NDQ_002330

answers: Jupiter

answers: NDQ_002331

answers: eclipsed

answers: NDQ_002332

answers: "companions"

answers: NDQ_002334

answers: the Sun

answers: NDQ_002335

answers: eclipsed

answers: NDQ_002343

answers: between 5-10 minutes

answers: NDQ_002345

answers: Schyrleus

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: the Sun

answers: NDQ_002351

answers: fourteen days

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: in 1642, in Cologne, he saw pass in front of the Sun a troop (turnam) of shooting stars that followed one another during a period fourteen days

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: total lunar eclipse

answers: NDQ_002357

answers: eclipsed

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: the glare of the Sun

answers: NDQ_002361

answers: moons of Jupiter

answers: NDQ_002362

answers: the moons of Jupiter

answers: NDQ_002363

answers: Sun

answers: NDQ_002364

answers: the Sun is considerably weakened

answers: NDQ_002365

answers: fourteen days

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: fourteen days

answers: NDQ_002368

answers: crescent

text: Lunar eclipses are related by many different eclipse cycles. The Saros cycle (18 years and 10 days) repeats the most consistently due three coinciding periods, and continue over 70 events (1200+ years). Eclipses are identified by a Saros number and a member index within each series.

text: Lunar eclipses are related by many different

text: eclipse cycle

text: s. The

text: Saros cycle

text: (18 years and 10 days) repeats the most consistently due three coinciding periods, and continue over 70 events (1200+ years). Eclipses are identified by a Saros number and a member index within each series.

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answers: 4

answers: NDQ_002367

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answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: eclipses

answers: NDQ_002324

answers: Lunar

answers: NDQ_002325

answers: Eclipses

answers: NDQ_002326

answers: Eclipses

answers: NDQ_002327

answers: Eclipses

answers: NDQ_002328

answers: Eclipses

answers: NDQ_002329

answers: three coinciding periods

answers: NDQ_002330

answers: Saros

answers: NDQ_002331

answers: Eclipses

answers: NDQ_002332

answers: Lunar

answers: NDQ_002334

answers: Saros number

answers: NDQ_002335

answers: Eclipses

answers: NDQ_002343

answers: lunar eclipses

answers: NDQ_002345

answers: Saros cycle

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: No

answers: NDQ_002351

answers: 18 years and 10 days

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: 1200+ years

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: The Saros cycle

answers: NDQ_002357

answers: Eclipses

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The Saros cycle

answers: NDQ_002360

answers: Lunar

answers: NDQ_002361

answers: eclipses

answers: NDQ_002362

answers: eclipses

answers: NDQ_002363

answers: lunar

answers: NDQ_002364

answers: lunar eclipses

answers: NDQ_002365

answers: 10 days

answers: NDQ_002366

answers: 1200+ years

answers: NDQ_002367

answers: 18 years and 10 days

answers: NDQ_002368

answers: eclipses

text: Graha (from Sanskrit ग्रह gráha—seizing, laying hold of, holding) is a 'cosmic influencer' on the living beings of mother Bhumidevi (Earth). In Hindu astrology, the Navagraha (Sanskrit: नवग्रह, nine seizers or nine influencers) are some of these major influencers.  All the navagraha have relative movement with respect to the background of fixed stars in the zodiac. This includes the planets:  Mars, Mercury, Jupiter, Venus, and Saturn, the Sun, the Moon, as well as positions in the sky, Rahu (north or ascending lunar node) and Ketu (south or descending lunar node).

text: Graha (from Sanskrit ग्रह gráha—seizing, laying hold of, holding) is a 'cosmic influencer' on the living beings of mother

text: Bhumidevi

text: (Earth). In

text: Hindu astrology

text: , the

text: Navagraha

text: (Sanskrit: नवग्रह, nine seizers or nine influencers) are some of these major influencers.  All the navagraha have relative movement with respect to the background of fixed stars in the

text: zodiac

text: . This includes the planets:

text: Mars

text: Mercury

text: Jupiter

text: Venus

text: , and

text: Saturn

text: , the

text: Sun

text: , the

text: Moon

text: , as well as positions in the sky,

text: Rahu

text: (north or ascending

text: lunar node

text: ) and

text: Ketu

text: (south or descending lunar node).

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answers: NDQ_002329

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answers: NDQ_002330

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answers: NDQ_002331

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 4

answers: NDQ_002367

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answers: NDQ_002368

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answers: NDQ_002323

answers: ascending

answers: NDQ_002324

answers: north or ascending lunar node) and Ketu

answers: NDQ_002325

answers: descending

answers: NDQ_002326

answers: Ketu

answers: NDQ_002327

answers: ascending lunar node

answers: NDQ_002328

answers: ascending lunar node

answers: NDQ_002329

answers: lunar node

answers: NDQ_002330

answers: Rahu

answers: NDQ_002331

answers: Graha

answers: NDQ_002332

answers: Rahu

answers: NDQ_002334

answers: Ketu

answers: NDQ_002335

answers: ascending

answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: Sun, the Moon

answers: NDQ_002348

answers: Moon

answers: NDQ_002350

answers: The Sun

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The Sun

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: It does not say

answers: NDQ_002357

answers: north or ascending lunar node

answers: NDQ_002358

answers: The Moon

answers: NDQ_002359

answers: the Moon

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: The Moon

answers: NDQ_002362

answers: relative movement with respect to the background of fixed stars

answers: NDQ_002363

answers: fixed stars

answers: NDQ_002364

answers: the Sun

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: one month

answers: NDQ_002368

answers: descending

text: Considering the Earth–Moon system as a binary planet, its centre of gravity is within Earth, about  or 72.6% of the Earth's radius from the centre of the Earth. This centre of gravity remains on the line between the centres of the earth and Moon as the Earth completes its diurnal rotation. The path of the Earth–Moon system in its solar orbit is defined as the movement of this mutual centre of gravity around the sun. Consequently, Earth's centre veers inside and outside the solar orbital path during each synodic month as the Moon moves in its orbit around the common centre of gravity.

text: Considering the Earth–Moon system as a

text: binary planet

text: , its centre of gravity is within Earth, about  or 72.6% of the Earth's radius from the centre of the Earth. This centre of gravity remains on the line between the centres of the earth and Moon as the Earth completes its diurnal rotation. The path of the Earth–Moon system in its solar orbit is defined as the movement of this mutual centre of gravity around the sun. Consequently, Earth's centre veers inside and outside the solar orbital path during each synodic month as the Moon moves in its orbit around the common centre of gravity.

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answers: NDQ_002328

answers: Earth's centre veers inside

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answers: NDQ_002330

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answers: NDQ_002331

answers: synodic month

answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002343

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answers: NDQ_002345

answers: Earth's centre veers inside and outside the solar orbital path

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth's centre veers inside

answers: NDQ_002351

answers: Synodic month

answers: NDQ_002352

answers: The path of the Earth–Moon system

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow

answers: NDQ_002354

answers: Earth's centre veers inside and outside the solar orbital path during each synodic month

answers: NDQ_002355

answers: Earth's centre

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answers: Synodic month

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answers: Earth's centre veers inside and outside

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answers: NDQ_002359

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answers: NDQ_002362

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answers: NDQ_002363

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answers: Moon moves in its orbit around the common centre of gravity

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answers: NDQ_002367

answers: synodic month

answers: NDQ_002368

answers: lunar perigee

text: While the Moon is orbiting the Earth, the Earth is progressing in its orbit around the Sun. After completing a sidereal month the Moon must move a little further to reach the new position having the same angular distance from the Sun. This longer period is called the synodic month (, sunodikos, meaning "pertaining to a synod, i.e., a meeting" [in this case of the Sun and the Moon]).

text: While the Moon is orbiting the Earth, the Earth is progressing in its orbit around the Sun. After completing a sidereal month the Moon must move a little further to reach the new position having the same angular distance from the Sun. This longer period is called the synodic month (, sunodikos, meaning "pertaining to a synod, i.e., a meeting" [in this case of the Sun and the Moon]).

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answers: NDQ_002324

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answers: NDQ_002325

answers: sidereal

answers: NDQ_002326

answers: sidereal

answers: NDQ_002327

answers: sidereal month

answers: NDQ_002328

answers: a synod

answers: NDQ_002329

answers: sidereal month

answers: NDQ_002330

answers: the Earth

answers: NDQ_002331

answers: sidereal month

answers: NDQ_002332

answers: synodic month

answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002343

answers: sidereal month

answers: NDQ_002345

answers: The Earth is progressing in its orbit around the Sun

answers: NDQ_002348

answers: The Moon is orbiting the Earth

answers: NDQ_002350

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answers: NDQ_002351

answers: sidereal month

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Sidereal

answers: NDQ_002354

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answers: NDQ_002355

answers: Moon must move a little further

answers: NDQ_002356

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answers: NDQ_002359

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answers: NDQ_002360

answers: Moon must move a little further

answers: NDQ_002361

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answers: NDQ_002362

answers: a synod

answers: NDQ_002363

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answers: NDQ_002364

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answers: NDQ_002365

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answers: NDQ_002366

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answers: NDQ_002367

answers: sidereal month

answers: NDQ_002368

answers: sidereal month

text: Solar and lunar eclipses were scientifically explained by Aryabhata. He states that the Moon and planets shine by reflected sunlight. Instead of the prevailing cosmogony in which eclipses were caused by Rahu and Ketu (identified as the pseudo-planetary lunar nodes), he explains eclipses in terms of shadows cast by and falling on Earth. Thus, the lunar eclipse occurs when the moon enters into the Earth's shadow (verse gola.37). He discusses at length the size and extent of the Earth's shadow (verses gola.38–48) and then provides the computation and the size of the eclipsed part during an eclipse. Later Indian astronomers improved on the calculations, but Aryabhata's methods provided the core. His computational paradigm was so accurate that 18th-century scientist Guillaume Le Gentil, during a visit to Pondicherry, India, found the Indian computations of the duration of the lunar eclipse of 30 August 1765 to be short by 41 seconds, whereas his charts (by Tobias Mayer, 1752) were long by 68 seconds.

text: Solar and lunar eclipses were scientifically explained by Aryabhata. He states that the

text: Moon

text: and planets shine by reflected sunlight. Instead of the prevailing cosmogony in which eclipses were caused by

text: Rahu

text: and

text: Ketu

text: (identified as the pseudo-planetary

text: lunar nodes

text: ), he explains eclipses in terms of shadows cast by and falling on Earth. Thus, the lunar eclipse occurs when the moon enters into the Earth's shadow (verse gola.37). He discusses at length the size and extent of the Earth's shadow (verses gola.38–48) and then provides the computation and the size of the eclipsed part during an eclipse. Later Indian astronomers improved on the calculations, but Aryabhata's methods provided the core. His computational paradigm was so accurate that 18th-century scientist

text: Guillaume Le Gentil

text: , during a visit to Pondicherry, India, found the Indian computations of the duration of the

text: lunar eclipse

text: of 30 August 1765 to be short by 41 seconds, whereas his charts (by Tobias Mayer, 1752) were long by 68 seconds.

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text: Newton, by calculating from Kepler's laws, and supposing the orbits of the planets to be circles round the sun in the centre, had already proved that the force of the sun acting upon the different planets must vary as the inverse square of the distances of the planets from the sun. He therefore was led to inquire whether, if the Earth's attraction extended to the moon, the force at that distance would be of the exact magnitude necessary to retain the moon in its orbit. He found that the moon by her motion in her orbit was deflected from the tangent in every minute of time through a space of thirteen feet. But by observing the distance through which a body would fall in one second of time at the Earth's surface, and by calculating from that on the supposition of the force diminishing in the ratio of the inverse square of the distance, he found that the Earth's attraction at the distance of the moon would draw a body through 15 ft. (4.57 metres) in one minute. Newton regarded the discrepancy between the results as a proof of the inaccuracy of his conjecture, and "laid aside at that time any further thoughts of this matter."  (See Newton's cannonball.)

text: Newton, by calculating from

text: Kepler's laws

text: Newton's cannonball

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text: The far side of the Moon is often improperly called the dark side of the Moon. The first scene of the show had a caption stating the location of the nuclear waste disposal storage being on the dark side of the Moon, although the caption also stated it was September 9, 1999, so the caption meant it was the dark side of the Moon on September  9.  It was also referred to as "the far side" by the character Ouma during the episode. The far side of the Moon, while always away from Earth, will still be illuminated by the sun, thus there is no area of the Moon that is permanently dark. This error was noted by Isaac Asimov, who wrote two articles on the scientific inaccuracies of the show. Unfortunately there was a new moon on September 9, 1999 so the far side was illuminated and the near side was the "dark side" on that date. (This can be seen on a moon-phase calculator, e.g. StarDate.)

text: The

text: far side of the Moon

text: is often improperly called the dark side of the Moon. The first scene of the show had a caption stating the location of the nuclear waste disposal storage being on the dark side of the Moon, although the caption also stated it was September 9, 1999, so the caption meant it was the dark side of the Moon on September  9.  It was also referred to as "the far side" by the character Ouma during the episode. The far side of the Moon, while always away from

text: Earth

text: , will still be illuminated by the

text: sun

text: , thus there is no area of the Moon that is permanently dark. This error was noted by

text: Isaac Asimov

text: , who wrote two articles on the scientific inaccuracies of the show. Unfortunately there was a new moon on September 9, 1999 so the far side was illuminated and the near side was the "dark side" on that date. (This can be seen on a moon-phase calculator, e.g. StarDate.)

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answers: NDQ_002323

answers: new moon

answers: NDQ_002324

answers: far side of the Moon

answers: NDQ_002325

answers: new moon

answers: NDQ_002326

answers: far side

answers: NDQ_002327

answers: new moon

answers: NDQ_002328

answers: no area of the Moon that is permanently dark

answers: NDQ_002329

answers: phase

answers: NDQ_002330

answers: far side of the Moon

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: far side

answers: NDQ_002334

answers: far side of the Moon

answers: NDQ_002335

answers: new moon

answers: NDQ_002343

answers: The far side of the Moon

answers: NDQ_002345

answers: The far side of the Moon will still be illuminated by the sun

answers: NDQ_002348

answers: The far side of the Moon

answers: NDQ_002350

answers: The far side of the Moon

answers: NDQ_002351

answers: The far side of the Moon

answers: NDQ_002352

answers: The far side of the Moon

answers: NDQ_002353

answers: There is no area of the Moon that is permanently dark

answers: NDQ_002354

answers: There was a new moon on September 9, 1999

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: there was a new moon

answers: NDQ_002357

answers: The far side of the Moon

answers: NDQ_002358

answers: new moon

answers: NDQ_002359

answers: The far side of the Moon

answers: NDQ_002360

answers: The far side of the Moon

answers: NDQ_002361

answers: The far side of the Moon

answers: NDQ_002362

answers: the sun

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the sun is directly overhead

answers: NDQ_002365

answers: September 9

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: new moon

answers: NDQ_002368

answers: new moon

text: Sedna has the longest orbital period of any known object in the Solar System of comparable size or larger, calculated at around 11,400 years. Its orbit is extremely eccentric, with an aphelion estimated at 937 AU and a perihelion at about 76 AU. This perihelion was the largest of that of any known Solar System object until the discovery of . When Sedna was discovered it was 89.6 AU from the Sun approaching perihelion, and was the most distant object in the Solar System observed. Eris was later detected by the same survey near aphelion at 97 AU. Only the orbits of some long-period comets extend farther than that of Sedna; they are too dim to be discovered except when approaching perihelion in the inner Solar System. Even as Sedna nears its perihelion in mid 2076, the Sun would appear merely as an extremely bright star-like pinpoint in its sky, 100 times brighter than a full moon on Earth (for comparison, the Sun appears from Earth to be roughly 400,000 times brighter than the full Moon), and too far away to be visible as a disc to the naked eye.

text: Sedna has the longest

text: orbital period

text: of any known object in the Solar System of comparable size or larger, calculated at around 11,400 years. Its

text: orbit

text: is extremely

text: eccentric

text: , with an

text: aphelion

text: estimated at 937 AU and a

text: perihelion

text: at about 76 AU. This perihelion was the largest of that of any known Solar System object until the discovery of . When Sedna was discovered it was 89.6 AU from the Sun approaching perihelion, and was the most distant object in the Solar System observed.

text: Eris

text: was later detected by the same survey near aphelion at 97 AU. Only the orbits of some long-period comets extend farther than that of Sedna; they are too dim to be discovered except when approaching perihelion in the inner Solar System. Even as Sedna nears its perihelion in mid 2076, the Sun would appear merely as an extremely bright star-like pinpoint in its sky, 100 times brighter than a full moon on Earth (for comparison, the Sun appears from Earth to be roughly 400,000 times brighter than the full Moon), and too far away to be visible as a disc to the naked eye.

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answers: full

answers: NDQ_002324

answers: aphelion

answers: NDQ_002325

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answers: full

answers: NDQ_002327

answers: perihelion

answers: NDQ_002328

answers: perihelion

answers: NDQ_002329

answers: 76 AU

answers: NDQ_002330

answers: perihelion

answers: NDQ_002331

answers: perihelion

answers: NDQ_002332

answers: full

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answers: perihelion

answers: NDQ_002335

answers: full

answers: NDQ_002343

answers: Its orbit is extremely eccentric

answers: NDQ_002345

answers: The Sun would appear merely as an extremely bright star-like pinpoint in its sky

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Sun

answers: NDQ_002351

answers: Sedna

answers: NDQ_002352

answers: perihelion

answers: NDQ_002353

answers: The umbra part of a shadow

answers: NDQ_002354

answers: the Sun would appear merely as an extremely bright star-like pinpoint in its sky

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: Its orbit is extremely eccentric

answers: NDQ_002357

answers: perihelion

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: the Sun would appear merely as an extremely bright star-like pinpoint in its sky

answers: NDQ_002361

answers: the Sun would appear merely as an extremely bright star-like pinpoint in its sky

answers: NDQ_002362

answers: Sedna

answers: NDQ_002363

answers: Solar System

answers: NDQ_002364

answers: full moon on Earth

answers: NDQ_002365

answers: 11400 years

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: around 11,400 years

answers: NDQ_002368

answers: perihelion

text: There are several different periods associated with the lunar orbit. The sidereal month is the time it takes to make one complete orbit around Earth with respect to the fixed stars. It is about 27.32 days. The synodic month is the time it takes the Moon to reach the same visual phase. This varies notably throughout the year, but averages around 29.53 days. The synodic period is longer than the sidereal period because the Earth–Moon system moves in its orbit around the Sun during each sidereal month, hence a longer period is required to achieve a similar alignment of Earth, the Sun, and the Moon. The anomalistic month is the time between perigees and is about 27.55 days. The Earth–Moon separation determines the strength of the lunar tide raising force.

text: There are several different periods associated with the lunar orbit. The

text: sidereal month

text: is the time it takes to make one complete orbit around Earth with respect to the fixed stars. It is about 27.32 days. The

text: synodic month

text: is the time it takes the Moon to reach the same visual

text: phase

text: . This varies notably throughout the year, but averages around 29.53 days. The synodic period is longer than the sidereal period because the Earth–Moon system moves in its orbit around the

text: Sun

text: during each sidereal month, hence a longer period is required to achieve a similar alignment of Earth, the Sun, and the Moon. The

text: anomalistic month

text: is the time between perigees and is about 27.55 days. The Earth–Moon separation determines the strength of the lunar tide raising force.

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answers: 3

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answers: 0

answers: NDQ_002329

answers: 2

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answers: NDQ_002331

answers: 0

answers: NDQ_002332

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answers: NDQ_002334

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answers: 3

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answers: 3

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: visual

answers: NDQ_002324

answers: sidereal month and the anomalistic month

answers: NDQ_002325

answers: sidereal

answers: NDQ_002326

answers: visual

answers: NDQ_002327

answers: sidereal month

answers: NDQ_002328

answers: perigees

answers: NDQ_002329

answers: about 27.32 days

answers: NDQ_002330

answers: Earth–Moon separation

answers: NDQ_002331

answers: tide

answers: NDQ_002332

answers: visual phase

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: visual

answers: NDQ_002343

answers: The Earth–Moon separation determines the strength of the lunar tide raising force

answers: NDQ_002345

answers: Earth–Moon separation determines the strength of the lunar tide raising force

answers: NDQ_002348

answers: The Earth–Moon separation

answers: NDQ_002350

answers: sidereal month

answers: NDQ_002351

answers: The synodic month

answers: NDQ_002352

answers: visual phase

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Solar eclipses are rare events

answers: NDQ_002355

answers: sidereal month

answers: NDQ_002356

answers: It is about 27.32 days

answers: NDQ_002357

answers: Earth–Moon separation

answers: NDQ_002358

answers: visual phase

answers: NDQ_002359

answers: The synodic month

answers: NDQ_002360

answers: Earth–Moon separation

answers: NDQ_002361

answers: sidereal month

answers: NDQ_002362

answers: Earth–Moon system moves in its orbit around the Sun

answers: NDQ_002363

answers: Earth–Moon system

answers: NDQ_002364

answers: alignment of Earth, the Sun, and the Moon

answers: NDQ_002365

answers: 29.53 days

answers: NDQ_002366

answers: year

answers: NDQ_002367

answers: 29.53 days

answers: NDQ_002368

answers: visual phase

text: Eclipses occur only near the lunar nodes:Solar eclipses occur when the passage of the Moon through a node coincides with the new moon; lunar eclipses occur when passage coincides with the full moon. A lunar eclipse may occur if there is a full moon within 11° 38' (Celestial Longitude), of a node, and a solar eclipse may occur if there is a new moon within 17° 25' of a node.

text: Eclipse

text: s occur only near the lunar nodes:

text: Solar eclipse

text: s occur when the passage of the Moon through a node coincides with the

text: new moon

text: lunar eclipse

text: s occur when passage coincides with the

text: full moon

text: . A lunar eclipse may occur if there is a full moon within 11° 38' (Celestial Longitude), of a node, and a solar eclipse may occur if there is a new moon within 17° 25' of a node.

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answers: NDQ_002325

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answers: NDQ_002326

answers: 3

answers: NDQ_002327

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answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 4

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 4

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 5

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 3

answers: NDQ_002357

answers: 0

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answers: 3

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 4

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 4

answers: NDQ_002323

answers: full moon

answers: NDQ_002324

answers: the lunar nodes

answers: NDQ_002325

answers: full moon

answers: NDQ_002326

answers: full moon

answers: NDQ_002327

answers: Eclipses

answers: NDQ_002328

answers: lunar eclipses

answers: NDQ_002329

answers: 11° 38'

answers: NDQ_002330

answers: 11° 38'

answers: NDQ_002331

answers: Eclipses

answers: NDQ_002332

answers: full

answers: NDQ_002334

answers: solar eclipse

answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: It generally lasts between 5-10 minutes.

answers: NDQ_002345

answers: The passage of the Moon through a node coincides with the new moon

answers: NDQ_002348

answers: The moon is entirely dark.

answers: NDQ_002350

answers: A solar eclipse is seen on all of the Earth that is having daytime

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Partial lunar eclipses occur when passage coincides with the full moon

answers: NDQ_002356

answers: It occurs once every month.

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: Full moon

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: lunar eclipses

answers: NDQ_002361

answers: solar eclipses

answers: NDQ_002362

answers: Eclipses

answers: NDQ_002363

answers: celestial longitude

answers: NDQ_002364

answers: the passage of the Moon through a node coincides with the new moon

answers: NDQ_002365

answers: 17° 25'

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: 17° 25'

answers: NDQ_002368

answers: new moon

text: A partial solar eclipse occurred on October 2, 1978. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on October 2, 1978. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 5

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answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

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answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partly obscuring

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly obscuring

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on October 2, 1978

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: on October 2, 1978

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: A crescent phase

answers: NDQ_002359

answers: October 2

answers: NDQ_002360

answers: The Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: partial

text: Solar sailing, an experimental method of spacecraft propulsion, uses radiation pressure from the Sun as a motive force. The idea of interplanetary travel by light was mentioned by Jules Verne in From the Earth to the Moon.

text: Solar sailing, an experimental method of

text: spacecraft propulsion

text: , uses radiation pressure from the Sun as a motive force. The idea of interplanetary travel by light was mentioned by

text: Jules Verne

text: in From the Earth to the Moon.

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text: The lunar phase or phase of the moon is the shape of the illuminated (sunlit) portion of the Moon as seen by an observer on Earth.  The lunar phases change cyclically as the Moon orbits the Earth, according to the changing positions of the  Moon and Sun relative to the Earth. The Moon's rotation is tidally locked by the Earth's gravity, therefore the same lunar surface always faces Earth. This face is variously sunlit depending on the position of the Moon in its orbit. Therefore, the portion of this hemisphere that is visible to an observer on Earth can vary from about 100% (full moon) to 0% (new moon). The lunar terminator is the boundary between the illuminated and darkened hemispheres. Each of the four "intermediate" lunar phases (see below) is roughly seven days (~7.4 days) but this varies slightly due to the elliptical shape of the Moon's orbit. Aside from some craters near the lunar poles such as Shoemaker, all parts of the Moon see around 14.77 days of sunlight, followed by 14.77 days of "night". (The side of the Moon facing away from the Earth is sometimes called the "dark side", which is a misnomer.

text: The lunar phase or phase of the moon is the shape of the illuminated (sunlit) portion of the

text: Moon

text: as seen by an observer on

text: Earth

text: .  The lunar phases change cyclically as the Moon

text: orbit

text: s the Earth, according to the changing positions of the

text: Moon

text: and

text: Sun

text: relative to the

text: Earth

text: . The Moon's rotation is

text: tidally locked

text: by the Earth's gravity, therefore the same lunar surface always faces Earth. This face is variously sunlit depending on the position of the Moon in its orbit. Therefore, the portion of this hemisphere that is visible to an observer on Earth can vary from about 100% (

text: full moon

text: ) to 0% (

text: new moon

text: ). The

text: lunar terminator

text: is the boundary between the illuminated and darkened hemispheres. Each of the four "intermediate" lunar phases (see below) is roughly seven days (~7.4 days) but this varies slightly due to the elliptical shape of the Moon's orbit. Aside from some craters near the lunar poles such as

text: Shoemaker

text: , all parts of the Moon see around 14.77 days of sunlight, followed by 14.77 days of "night". (The side of the Moon facing away from the Earth is sometimes called the "dark side", which is a misnomer.

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text: Lunar Eclipse is the second solo album by David Bryan from the band Bon Jovi. Released in 2000, it features all the songs from his first album "On a Full Moon", released in 1995, except for "Awakening" and "Midnight Voodoo". Instead of those two tracks it features two brand new tracks, "Second Chance" and "I Can Love". Also, this version of the Bon Jovi song In These Arms has David on vocals, in contrast to the instrumental version from the first album.

text: Lunar Eclipse is the second solo album by

text: David Bryan

text: from the band

text: Bon Jovi

text: . Released in 2000, it features all the songs from his first album "

text: On a Full Moon

text: ", released in 1995, except for "Awakening" and "Midnight Voodoo". Instead of those two tracks it features two brand new tracks, "Second Chance" and "I Can Love". Also, this version of the

text: Bon Jovi

text: song

text: In These Arms

text: has David on vocals, in contrast to the instrumental version from the first album.

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text: A total lunar eclipse will take place on July 27, 2018. The moon will pass through the center of the Earth's shadow. This will be the first central lunar eclipse since the June 15, 2011 lunar eclipse.

text: A total

text: lunar eclipse

text: will take place on July 27, 2018. The moon will pass through the

text: center of the Earth's shadow

text: . This will be the first central lunar eclipse since the

text: June 15, 2011 lunar eclipse

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answers: It will take place on July 27, 2018.

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answers: lunar eclipse

text: As it moves around its orbit, Venus displays phases like those of the Moon in a telescopic view. The planet presents a small "full" image when it is on the opposite side of the Sun. It shows a larger "quarter phase" when it is at its maximum elongations from the Sun, and is at its brightest in the night sky, and presents a much larger "thin crescent" in telescopic views as it comes around to the near side between Earth and the Sun. Venus is at its largest and presents its "new phase" when it is between Earth and the Sun. Its atmosphere can be seen in a telescope by the halo of light refracted around it.

text: As it moves around its orbit,

text: Venus displays phases

text: like those of the

text: Moon

text: in a

text: telescopic

text: view. The planet presents a small "full" image when it is on the opposite side of the Sun. It shows a larger "quarter phase" when it is at its maximum elongations from the Sun, and is at its brightest in the night sky, and presents a much larger "thin crescent" in telescopic views as it comes around to the near side between Earth and the Sun. Venus is at its largest and presents its "new phase" when it is between Earth and the Sun. Its atmosphere can be seen in a telescope by the halo of light refracted around it.

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answers: NDQ_002327

answers: phases

answers: NDQ_002328

answers: Venus displays phases like those of the Moon

answers: NDQ_002329

answers: "quarter phase"

answers: NDQ_002330

answers: a telescopic view

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answers: Moon

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answers: Venus displays phases like those of the Moon

answers: NDQ_002348

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answers: When it is between Earth and the Sun

answers: NDQ_002351

answers: phases like those of the Moon

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: The planet presents a small "full" image

answers: NDQ_002354

answers: Venus displays phases like those of the Moon

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: Venus

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answers: Venus presents a small "full" image when it is on the opposite side of the Sun

answers: NDQ_002363

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answers: NDQ_002368

answers: quarter phase

text: A total solar eclipse will occur on September 23, 2090. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.This solar eclipse will be the first total solar eclipse visible from the United Kingdom mainland since August 11, 1999.

text: A total

text: solar eclipse

text: will occur on September 23, 2090. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's

text: apparent diameter

text: is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.This solar eclipse will be the first total solar eclipse visible from the

text: United Kingdom

text: mainland since

text: August 11, 1999

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answers: 4

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answers: 4

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answers: 4

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answers: 0

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answers: 5

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answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial solar eclipse

answers: NDQ_002324

answers: totality and partial solar eclipse

answers: NDQ_002325

answers: total solar eclipse

answers: NDQ_002326

answers: partial solar eclipse

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: total solar eclipse

answers: NDQ_002329

answers: partial solar eclipse

answers: NDQ_002330

answers: totality

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial solar eclipse

answers: NDQ_002334

answers: totality

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: The Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: total solar eclipse

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: total solar eclipse

answers: NDQ_002353

answers: total solar eclipse

answers: NDQ_002354

answers: The United Kingdom mainland since August 11, 1999

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On September 23, 2090

answers: NDQ_002357

answers: total solar eclipse

answers: NDQ_002358

answers: A crescent phase

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: total solar eclipse

answers: NDQ_002362

answers: total solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: when the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 2090

answers: NDQ_002368

answers: partial solar eclipse

text: Note that there are three main moving points: the Sun, the Moon, and the (ascending) node; and that there are three main periods, when each of the three possible pairs of moving points meet one another: the synodic month when the Moon returns to the Sun, the draconic month when the Moon returns to the node, and the eclipse year when the Sun returns to the node.  These three 2-way relations are not independent (i.e. both the synodic month and eclipse year are dependent on the apparent motion of the Sun, both the draconic month and eclipse year are dependent on the motion of the nodes), and indeed the eclipse year can be described as the beat period of the synodic and draconic months (i.e. the period of the difference between the synodic and draconic months); in formula:

text: Note that there are three main moving points: the Sun, the Moon, and the (ascending) node; and that there are three main periods, when each of the three possible pairs of moving points meet one another: the synodic month when the Moon returns to the Sun, the draconic month when the Moon returns to the node, and the eclipse year when the Sun returns to the node.  These three 2-way relations are not independent (i.e. both the synodic month and eclipse year are dependent on the apparent motion of the Sun, both the draconic month and eclipse year are dependent on the motion of the nodes), and indeed the eclipse year can be described as the

text: beat period

text: of the synodic and draconic months (i.e. the period of the difference between the synodic and draconic months); in formula:

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answers: NDQ_002323

answers: eclipse

answers: NDQ_002324

answers: the (ascending) node

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: eclipse

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: eclipse

answers: NDQ_002329

answers: draconic month

answers: NDQ_002330

answers: the node

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: eclipse

answers: NDQ_002334

answers: the node

answers: NDQ_002335

answers: eclipse

answers: NDQ_002343

answers: The beat period of the synodic month

answers: NDQ_002345

answers: the Sun returns to the node

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The Sun returns to the node

answers: NDQ_002351

answers: Synodic month

answers: NDQ_002352

answers: the (ascending) node

answers: NDQ_002353

answers: the umbra part of a shadow

answers: NDQ_002354

answers: solar eclipses are rare

answers: NDQ_002355

answers: Moon enters Earths umbra

answers: NDQ_002356

answers: synodic month

answers: NDQ_002357

answers: Synodic month

answers: NDQ_002358

answers: synodic month

answers: NDQ_002359

answers: Synodic month

answers: NDQ_002360

answers: Moon returns to the Sun

answers: NDQ_002361

answers: the Moon returns to the Sun

answers: NDQ_002362

answers: the apparent motion of the Sun, both the draconic month and eclipse year are dependent on the motion of the nodes

answers: NDQ_002363

answers: node

answers: NDQ_002364

answers: the Sun returns to the node

answers: NDQ_002365

answers: the eclipse year

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: synodic month

answers: NDQ_002368

answers: eclipse

text: A partial solar eclipse occurred on February 14, 1953. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on February 14, 1953. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: partial

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answers: solar eclipse

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answers: part

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answers: partial

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answers: misses

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answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

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answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on February 14, 1953

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: It's impossible to say

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answers: The full moon phase

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answers: A crescent phase

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answers: February 14

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answers: completely or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

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answers: Earth

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answers: the Moon passes between Earth and the Sun

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answers: total or partly

answers: NDQ_002366

answers: Earth

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answers: partial solar eclipse

text: An annular solar eclipse will occur on July 3, 2084. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on July 3, 2084. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: annular

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answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

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answers: An annular solar eclipse appears as a partial eclipse

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answers: obscuring the image of the Sun

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answers: totally

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answers: Moon passes between Earth and the Sun

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answers: Moon passes between Earth and the Sun

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answers: totally or partly

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answers: no

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answers: The time between two full moon phases is 29.5 days

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answers: (ring)

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answers: Partially

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answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On July 3, 2084

answers: NDQ_002357

answers: full moon

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answers: crescent phase

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answers: The Moon passes between Earth and the Sun

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answers: Moon passes between Earth and the Sun

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answers: the Moon passes between Earth and the Sun

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answers: crescent

text: An annular solar eclipse occurred on December 25, 1935. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.This was the 5th solar eclipse in 1935, the maximum possible. The next time this will occur is 2206.

text: An annular

text: solar eclipse

text: occurred on December 25, 1935. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.This was the 5th solar eclipse in 1935, the maximum possible. The next time this will occur is 2206.

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answers: 4

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 4

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: annulus (ring)

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: annular solar eclipse

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: annular

answers: NDQ_002343

answers: The next time this will occur is 2206.

answers: NDQ_002345

answers: An annular solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The next time this will occur is 2206.

answers: NDQ_002352

answers: The next time this will occur is 2206.

answers: NDQ_002353

answers: An annular eclipse appears as a partial eclipse

answers: NDQ_002354

answers: The next time this will occur is 2206.

answers: NDQ_002355

answers: Partially obscuring the image of the Sun

answers: NDQ_002356

answers: The next time this will occur is 2206.

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: The next time this will occur is 2206.

answers: NDQ_002359

answers: The next time this will occur is 2206.

answers: NDQ_002360

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002361

answers: The Moon passes between Earth and the Sun

answers: NDQ_002362

answers: An annular solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: December 25, 1935

answers: NDQ_002366

answers: 2206.

answers: NDQ_002367

answers: one month

answers: NDQ_002368

answers: partial

text: In 1979, Freitas and Valdes conducted a photographic search of the vicinity of the Earth-Moon triangular libration points  and , and of the solar-synchronized positions in the associated halo orbits, seeking possible orbiting extraterrestrial interstellar probes, but found nothing to a detection limit of about 14th magnitude. The authors conducted a second, more comprehensive photographic search for probes in 1982 that examined the five Earth-Moon Lagrangian positions and included the solar-synchronized positions in the stable L4/L5 libration orbits, the potentially stable nonplanar orbits near L1/L2, Earth-Moon , and also  in the Sun-Earth system. Again no extraterrestrial probes were found to limiting magnitudes of 17–19th magnitude near L3/L4/L5, 10–18th magnitude for /, and 14–16th magnitude for Sun-Earth .

text: In 1979, Freitas and Valdes conducted a photographic search of the vicinity of the Earth-Moon triangular libration points  and , and of the solar-synchronized positions in the associated halo orbits, seeking possible orbiting extraterrestrial interstellar probes, but found nothing to a detection limit of about 14th magnitude. The authors conducted a second, more comprehensive photographic search for probes in 1982 that examined the five Earth-Moon

text: Lagrangian positions

text: and included the solar-synchronized positions in the stable L4/L5 libration orbits, the potentially stable nonplanar orbits near L1/L2, Earth-Moon , and also  in the Sun-Earth system. Again no extraterrestrial probes were found to limiting magnitudes of 17–19th magnitude near L3/L4/L5, 10–18th magnitude for /, and 14–16th magnitude for Sun-Earth .

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answers: 0

answers: NDQ_002323

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answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 0

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 0

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 0

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

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answers: 0

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

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answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

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answers: NDQ_002365

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answers: NDQ_002366

answers: 0

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: halo

answers: NDQ_002324

answers: Moon

answers: NDQ_002325

answers: NDQ_002326

answers: 17–19th

answers: NDQ_002327

answers: libration points

answers: NDQ_002328

answers: halo orbits

answers: NDQ_002329

answers: L4/L5

answers: NDQ_002330

answers: Lagrangian positions

answers: NDQ_002331

answers: Lagrangian positions

answers: NDQ_002332

answers: halo

answers: NDQ_002334

answers: Earth-Moon

answers: NDQ_002335

answers: halo

answers: NDQ_002343

answers: Earth-Moon

answers: NDQ_002345

answers: Solar eclipse

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth-Moon

answers: NDQ_002351

answers: Moon

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Earth-Moon

answers: NDQ_002355

answers: Earth-Moon

answers: NDQ_002356

answers: Moon

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: Moon

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: the Sun-Earth system

answers: NDQ_002363

answers: orbits

answers: NDQ_002364

answers: Earth-Moon

answers: NDQ_002365

answers: 10–18th

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

text: An annular solar eclipse will occur on July 2, 2038. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on July 2, 2038. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 0

answers: NDQ_002323

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answers: NDQ_002324

answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 4

answers: NDQ_002328

answers: 4

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: obscuring the image of the Sun

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Partially obscuring the image of the Sun

answers: NDQ_002356

answers: July 2, 2038

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The Moon passes between Earth and the Sun

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 2038

answers: NDQ_002368

answers: crescent

text: Gamma (denoted as γ) of an eclipse describes how centrally the shadow of the Moon or Earth strikes the other. The distance, when the axis of the shadow cone passes closest to Earth or Moon's center, is stated as a fraction of the equatorial radius of the Earth. The sign of gamma defines, for a solar eclipse, if the axis of the shadow passes north or south of the center of the Earth; a positive value means north. For a lunar eclipse it defines whether the axis of the Earth's shadow passes north or south of the Moon; a positive value means south. For solar eclipses the Earth is defined as that half which is exposed to the Sun (this changes with the seasons and is not related directly to the Earth's poles or equator, thus the Earth's center is wherever the Sun is directly overhead).

text: Gamma (denoted as

text: γ

text: ) of an

text: eclipse

text: describes how centrally the

text: shadow

text: of the

text: Moon

text: or

text: Earth

text: strikes the other. The distance, when the axis of the shadow cone passes closest to Earth or Moon's center, is stated as a fraction of the

text: equatorial radius

text: of the Earth. The sign of gamma defines, for a solar eclipse, if the axis of the shadow passes north or south of the center of the Earth; a positive value means north. For a lunar eclipse it defines whether the axis of the Earth's shadow passes north or south of the Moon; a positive value means south. For solar eclipses the Earth is defined as that half which is exposed to the Sun (this changes with the seasons and is not related directly to the Earth's poles or equator, thus the Earth's center is wherever the

text: Sun

text: is

text: directly overhead

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answers: NDQ_002323

answers: lunar eclipse

answers: NDQ_002324

answers: shadow cone passes closest to Earth or Moon's center

answers: NDQ_002325

answers: lunar eclipse

answers: NDQ_002326

answers: south

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: half which is exposed to the Sun

answers: NDQ_002330

answers: Earth's center

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: Moon

answers: NDQ_002334

answers: Moon's center

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: It defines whether the axis of the Earth's shadow passes north or south

answers: NDQ_002345

answers: The Earth is defined as that half which is exposed to the Sun

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: half which is exposed to the Sun

answers: NDQ_002351

answers: Moon's center

answers: NDQ_002352

answers: For a lunar eclipse

answers: NDQ_002353

answers: Gamma

answers: NDQ_002354

answers: It defines how centrally the shadow of the Moon strikes the other

answers: NDQ_002355

answers: The Earth is defined as that half which is exposed to the Sun

answers: NDQ_002356

answers: For a lunar eclipse

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: Moon's center

answers: NDQ_002359

answers: The sign of gamma

answers: NDQ_002360

answers: The Earth is defined as that half which is exposed to the Sun

answers: NDQ_002361

answers: For solar eclipses the Earth is defined as that half which is exposed to the Sun

answers: NDQ_002362

answers: a solar eclipse

answers: NDQ_002363

answers: Earth's center

answers: NDQ_002364

answers: the Earth is exposed to the Sun

answers: NDQ_002365

answers: a solar eclipse

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: There were 255 lunar eclipse events between -1899 and -1800 (1900 BCE to 1801 BCE)

text: There were 255 lunar eclipse events between -1899 and -1800 (1900 BCE to 1801 BCE)

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answers: lunar eclipse

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answers: lunar

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answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: half moon

answers: NDQ_002330

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answers: NDQ_002331

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answers: NDQ_002332

answers: lunar

answers: NDQ_002334

answers: lunar

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: between -1899 and -1800

answers: NDQ_002345

answers: solar eclipse

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: A lunar eclipse is seen on the Earth that is having daytime.

answers: NDQ_002351

answers: 29.5 days

answers: NDQ_002352

answers: lunar eclipse

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: 255 lunar eclipse events

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: lunar eclipse

answers: NDQ_002357

answers: lunar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

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answers: NDQ_002363

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answers: NDQ_002364

answers: lunar eclipse

answers: NDQ_002365

answers: a lunar eclipse

answers: NDQ_002366

answers: 1900 BCE

answers: NDQ_002367

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answers: NDQ_002368

answers: lunar eclipse

text: When the inclination of the moon's orbit to the earth's equator is at its minimum of 18°20′, the centre of the moon's disk will be above the horizon every day as far north and as far south as 90°−18°20' or 71°40' latitude, whereas when the inclination is at its maximum of 28°36' the centre of the moon's disk will only be above the horizon every day for latitudes less than 90°−28°36' or 61°24'. At higher latitudes there will be a period of at least a day each month when the moon does not rise, but there will also be a period of at least a day each month during which the moon does not set. This is similar to the behaviour of the sun, but with a period of 27.3 days instead of 365 days. Note that a point on the moon can actually be visible when it is below the horizon by about 34 arc minutes, due to refraction (see Sunrise).

text: When the inclination of the moon's orbit to the earth's equator is at its minimum of 18°20′, the centre of the moon's disk will be above the horizon every day as far north and as far south as 90°−18°20' or 71°40' latitude, whereas when the inclination is at its maximum of 28°36' the centre of the moon's disk will only be above the horizon every day for latitudes less than 90°−28°36' or 61°24'. At higher latitudes there will be a period of at least a day each month when the moon does not rise, but there will also be a period of at least a day each month during which the moon does not set. This is similar to the behaviour of the sun, but with a period of 27.3 days instead of 365 days. Note that a point on the moon can actually be visible when it is below the horizon by about 34 arc minutes, due to refraction (see

text: Sunrise

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answers: 3

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answers: 0

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answers: 2

answers: NDQ_002330

answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 4

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answers: 0

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answers: 0

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answers: 0

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answers: 4

answers: NDQ_002352

answers: 0

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answers: 0

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answers: 0

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answers: 4

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answers: 0

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answers: 0

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answers: 4

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answers: 4

answers: NDQ_002360

answers: 0

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answers: 0

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 27.3 days

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: Sunrise

answers: NDQ_002324

answers: when the inclination of the moon's orbit to the earth's equator is at its minimum of 18°20′

answers: NDQ_002325

answers: Set

answers: NDQ_002326

answers: Sunrise

answers: NDQ_002327

answers: Sunrise

answers: NDQ_002328

answers: the moon does not rise

answers: NDQ_002329

answers: 27.3 days

answers: NDQ_002330

answers: centre of the moons disk

answers: NDQ_002331

answers: Sunrise

answers: NDQ_002332

answers: rise

answers: NDQ_002334

answers: horizon

answers: NDQ_002335

answers: Sunrise

answers: NDQ_002343

answers: about 34 arc minutes, due to refraction

answers: NDQ_002345

answers: The centre of the moon's disk will only be above the horizon every day for latitudes less than 90° 28°36' or 61°24'

answers: NDQ_002348

answers: at least a day each month during which the moon does not set

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: At higher latitudes there will be a period of at least a day each month when the moon does not rise

answers: NDQ_002352

answers: horizon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: solar eclipses are rare events

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: at least a day each month

answers: NDQ_002357

answers: 71°40' latitude

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: full moon will occur on the 28th of the month

answers: NDQ_002360

answers: This similar to the behaviour of the sun, but with a period of 27.3 days instead of 365 days

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: the moon's orbit to the earth's equator

answers: NDQ_002363

answers: horizon

answers: NDQ_002364

answers: when the inclination of the moon's orbit to the earth's equator is at its minimum

answers: NDQ_002365

answers: 27.3 days

answers: NDQ_002366

answers: 27.3 days

answers: NDQ_002367

answers: 27.3 days

answers: NDQ_002368

answers: rise

text: Before the battle in Babylon, Alexander states that the lunar eclipse which some of his men thought was a bad omen means that "the Persian moon will be eclipsed by the Macedonian Sun" with which Aristander the seer agrees. After victory in Babylon, Darius III flees to the Caspian Gates to build and gather up an army; the dispirited commanders of Darius III kill him. In his will, Darius tells Alexander, "Take my daughter, Roxane, for your wife...that our worlds may become as one." Alexander then orders the lords of Persia that had committed regicide to be impaled upon stakes for their betrayal against their former kings.

text: Before the battle in Babylon, Alexander states that the

text: lunar eclipse

text: which some of his men thought was a bad omen means that "the Persian moon will be eclipsed by the Macedonian Sun" with which

text: Aristander

text: the seer agrees. After victory in Babylon, Darius III flees to the Caspian Gates to build and gather up an army; the dispirited commanders of Darius III kill him. In his will, Darius tells Alexander, "Take my daughter,

text: Roxane

text: , for your wife...that

text: our worlds may become as one

text: ." Alexander then orders the lords of Persia that had committed

text: regicide

text: to be impaled upon stakes for their betrayal against their former kings.

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answers: 3

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

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answers: 4

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answers: 5

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answers: 4

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answers: 4

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answers: 0

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answers: 4

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answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 4

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 4

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answers: 0

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: lunar eclipse

answers: NDQ_002324

answers: the Persian moon

answers: NDQ_002325

answers: lunar eclipse

answers: NDQ_002326

answers: eclipsed

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: lunar eclipse

answers: NDQ_002330

answers: the Persian

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: Persian

answers: NDQ_002334

answers: the Persian moon

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: It usually lasts between 5-10 minutes.

answers: NDQ_002345

answers: the Macedonian Sun

answers: NDQ_002348

answers: The Persian moon will be eclipsed

answers: NDQ_002350

answers: No

answers: NDQ_002351

answers: lunar eclipse

answers: NDQ_002352

answers: the Persian moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Lunar eclipse

answers: NDQ_002355

answers: Partially eclipsed

answers: NDQ_002356

answers: It occurs once every month.

answers: NDQ_002357

answers: lunar eclipse

answers: NDQ_002358

answers: The Persian moon will be eclipsed

answers: NDQ_002359

answers: the Persian moon will be eclipsed

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: eclipses

answers: NDQ_002363

answers: Sun

answers: NDQ_002364

answers: the Sun

answers: NDQ_002365

answers: the duration of the day

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: one month

answers: NDQ_002368

answers: lunar eclipse

text: Eclipses can only occur when the Sun, Earth, and Moon are all in a straight line (termed "syzygy"). Solar eclipses occur at new moon, when the Moon is between the Sun and Earth. In contrast, lunar eclipses occur at full moon, when Earth is between the Sun and Moon. The apparent size of the Moon is roughly the same as that of the Sun, with both being viewed at close to one-half a degree wide. The Sun is much larger than the Moon but it is the precise vastly greater distance that gives it the same apparent size as the much closer and much smaller Moon from the perspective of Earth. The variations in apparent size, due to the non-circular orbits, are nearly the same as well, though occurring in different cycles. This makes possible both total (with the Moon appearing larger than the Sun) and annular (with the Moon appearing smaller than the Sun) solar eclipses. In a total eclipse, the Moon completely covers the disc of the Sun and the solar corona becomes visible to the naked eye. Because the distance between the Moon and Earth is very slowly increasing over time, the angular diameter of the Moon is decreasing. Also, as it evolves toward becoming a red giant, the size of the Sun, and its apparent diameter in the sky, are slowly increasing. The combination of these two changes means that hundreds of millions of years ago, the Moon would always completely cover the Sun on solar eclipses, and no annular eclipses were possible. Likewise, hundreds of millions of years in the future, the Moon will no longer cover the Sun completely, and total solar eclipses will not occur.

text: Eclipses can only occur when the Sun, Earth, and Moon are all in a straight line (termed "

text: syzygy

text: Solar eclipse

text: s occur at

text: new moon

text: , when the Moon is between the Sun and Earth. In contrast,

text: lunar eclipse

text: s occur at

text: full moon

text: , when Earth is between the Sun and Moon. The apparent size of the Moon is roughly the same as that of the Sun, with both being viewed at close to one-half a degree wide. The Sun is much larger than the Moon but it is the precise vastly greater distance that gives it the same apparent size as the much closer and much smaller Moon from the perspective of Earth. The variations in apparent size, due to the non-circular orbits, are nearly the same as well, though occurring in different cycles. This makes possible both

text: total

text: (with the Moon appearing larger than the Sun) and

text: annular

text: (with the Moon appearing smaller than the Sun) solar eclipses. In a total eclipse, the Moon completely covers the disc of the Sun and the solar

text: corona

text: becomes visible to the

text: naked eye

text: . Because the distance between the Moon and Earth is very slowly increasing over time, the angular diameter of the Moon is decreasing. Also, as it evolves toward becoming a

text: red giant

text: , the size of the Sun, and its apparent diameter in the sky, are slowly increasing. The combination of these two changes means that hundreds of millions of years ago, the Moon would always completely cover the Sun on solar eclipses, and no annular eclipses were possible. Likewise, hundreds of millions of years in the future, the Moon will no longer cover the Sun completely, and total solar eclipses will not occur.

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answers: 0

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answers: full moon

answers: NDQ_002324

answers: solar corona

answers: NDQ_002325

answers: full moon

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: lunar eclipses

answers: NDQ_002328

answers: lunar eclipses

answers: NDQ_002329

answers: new moon

answers: NDQ_002330

answers: solar corona

answers: NDQ_002331

answers: lunar eclipses

answers: NDQ_002332

answers: full moon

answers: NDQ_002334

answers: solar corona

answers: NDQ_002335

answers: full moon

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answers: It is the precise vastly greater distance

answers: NDQ_002345

answers: Because the distance between the Moon and Earth is very slowly increasing over time

answers: NDQ_002348

answers: the Moon completely covers the disc of the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: lunar eclipses occur at full moon

answers: NDQ_002352

answers: the solar corona

answers: NDQ_002353

answers: annular

answers: NDQ_002354

answers: Likewise, hundreds of millions of years in the future, the Moon will no longer cover the Sun completely, and total solar eclipses will not occur

answers: NDQ_002355

answers: Moon appears smaller than the Sun

answers: NDQ_002356

answers: It does not say.

answers: NDQ_002357

answers: Earth is between the Sun and Moon

answers: NDQ_002358

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answers: NDQ_002359

answers: The apparent size of the Moon

answers: NDQ_002360

answers: Moon appears larger than the Sun

answers: NDQ_002361

answers: Moon is between the Sun and Earth

answers: NDQ_002362

answers: the variations in apparent size, due to the non-circular orbits

answers: NDQ_002363

answers: Earth's orbit

answers: NDQ_002364

answers: the Moon completely covers the disc of the Sun

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answers: a few minutes

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answers: month

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text: The context of the essay was to reply to the treatise Libra astronomica ac philosophica of 1619 by Orazio Grassi, a Jesuit mathematician at the Collegio Romano, which used the pseudonym of Lotario Sarsi Sigensano. The debate between Galileo and Grassi started in 1618, when the latter published Disputatio astronomica de tribus cometis anni MDCXVIII, in which he asserted that comets are celestial bodies. Grassi adopted Tycho Brahe's Tychonic system, in which the other planets of the solar system orbit around the sun, which, in turn, orbits around the earth. In his Disputatio Grassi referenced many of Galileo's observations, such as the surface of the moon and the phases of Venus, without mentioning him.Grassi argued from the apparent absence of observable parallax that comets move beyond the moon. Galileo mistakenly believed that comets are an optical illusion.

text: The context of the essay was to reply to the treatise Libra astronomica ac philosophica of 1619 by

text: Orazio Grassi

text: , a

text: Jesuit

text: mathematician at the

text: Collegio Romano

text: , which used the

text: pseudonym

text: of Lotario Sarsi Sigensano. The debate between Galileo and Grassi started in 1618, when the latter published Disputatio astronomica de tribus cometis anni MDCXVIII, in which he asserted that comets are celestial bodies. Grassi adopted

text: Tycho Brahe

text: 's

text: Tychonic system

text: , in which the other planets of the

text: solar system

text: orbit around the

text: sun

text: , which, in turn, orbits around the

text: earth

text: . In his Disputatio Grassi referenced many of Galileo's observations, such as the surface of the

text: moon

text: and the phases of

text: Venus

text: , without mentioning him.Grassi argued from the apparent absence of observable

text: parallax

text: that comets move beyond the moon. Galileo mistakenly believed that comets are an optical illusion.

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answers: phases

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answers: the surface of the moon

answers: NDQ_002325

answers: Parallax

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: parallax

answers: NDQ_002328

answers: comets move beyond the moon

answers: NDQ_002329

answers: phases

answers: NDQ_002330

answers: surface of the moon

answers: NDQ_002331

answers: phases

answers: NDQ_002332

answers: phases

answers: NDQ_002334

answers: comets move beyond the moon

answers: NDQ_002335

answers: Moonrise

answers: NDQ_002343

answers: Lunar eclipse

answers: NDQ_002345

answers: solar eclipse

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: Galileo

answers: NDQ_002352

answers: Galileo

answers: NDQ_002353

answers: Parallax

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: total lunar eclipse

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: the first quarter phase

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: moon

answers: NDQ_002361

answers: solar eclipse

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answers: orbit around the sun

answers: NDQ_002363

answers: celestial bodies

answers: NDQ_002364

answers: the sun

answers: NDQ_002365

answers: an hour

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1618

answers: NDQ_002368

answers: phase

text: Though life is confirmed only on Earth, many think that extraterrestrial life is not only plausible, but probable or inevitable. Other planets and moons in the Solar System and other planetary systems are being examined for evidence of having once supported simple life, and projects such as SETI are trying to detect radio transmissions from possible alien civilizations. Other locations within the Solar System that may host microbial life include the subsurface of Mars, the upper atmosphere of Venus, and subsurface oceans on some of the moons of the giant planets.Beyond the Solar System, the region around another main-sequence star that could support Earth-like life on an Earth-like planet is known as the habitable zone. The inner and outer radii of this zone vary with the luminosity of the star, as does the time interval during which the zone survives. Stars more massive than the Sun have a larger habitable zone, but remain on the main sequence for a shorter time interval. Small red dwarfs have the opposite problem, with a smaller habitable zone that is subject to higher levels of magnetic activity and the effects of tidal locking from close orbits. Hence, stars in the intermediate mass range such as the Sun may have a greater likelihood for Earth-like life to develop. The location of the star within a galaxy may also affect the likelihood of life forming. Stars in regions with a greater abundance of heavier elements that can form planets, in combination with a low rate of potentially habitat-damaging supernova events, are predicted to have a higher probability of hosting planets with complex life. The variables of the Drake equation are used to discuss the conditions in planetary systems where civilization is most likely to exist. Use of the equation to predict the amount of extraterrestrial life, however, is difficult; because many of the variables are unknown, the equation functions as more of a mirror to what its user already thinks. As a result, the number of civilizations in the galaxy can be estimated as low as 9.1 x 10^-11 or as high as 156 million; for the calculations, see Drake equation.

text: Though life is confirmed only on Earth, many think that

text: extraterrestrial life

text: is not only plausible, but probable or inevitable. Other planets and

text: moons

text: in the

text: Solar System

text: and other

text: planetary system

text: s are being examined for evidence of having once supported simple life, and projects such as

entity_name: Search for extraterrestrial intelligence

text: SETI

text: are trying to detect radio transmissions from possible alien civilizations. Other locations within the

text: Solar System

text: that may host

text: microbial

text: life include the subsurface of

text: Mars

text: , the upper atmosphere of

text: Venus

text: , and subsurface oceans on some of the

text: moons

text: of the

text: giant planet

text: s.Beyond the Solar System, the region around another

text: main-sequence star

text: that could support Earth-like life on an Earth-like planet is known as the

text: habitable zone

text: . The inner and outer radii of this zone vary with the luminosity of the star, as does the time interval during which the zone survives. Stars more massive than the Sun have a larger habitable zone, but remain on the main sequence for a shorter time interval. Small

text: red dwarf

text: s have the opposite problem, with a smaller habitable zone that is subject to higher levels of magnetic activity and the effects of

text: tidal locking

text: from close orbits. Hence, stars in the intermediate mass range such as the Sun may have a greater likelihood for Earth-like life to develop. The location of the star within a galaxy may also affect the likelihood of life forming. Stars in regions with a greater abundance of heavier elements that can form planets, in combination with a low rate of potentially

text: habitat

text: -damaging

text: supernova

text: events, are predicted to have a higher probability of hosting planets with complex life. The variables of the

text: Drake equation

text: are used to discuss the conditions in planetary systems where civilization is most likely to exist. Use of the equation to predict the amount of extraterrestrial life, however, is difficult; because many of the variables are unknown, the equation functions as more of a mirror to what its user already thinks. As a result, the number of civilizations in the galaxy can be estimated as low as 9.1 x 10^-11 or as high as 156 million; for the calculations, see

text: Drake equation

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text: A lunar eclipse occurs when the Moon passes within Earth's umbra (shadow). As the eclipse begins, the Earth's shadow first darkens the Moon slightly.  Then, the shadow begins to "cover" part of the Moon, turning it a dark red-brown color (typically - the color can vary based on atmospheric conditions).  The Moon appears to be reddish because of Rayleigh scattering (the same effect that causes sunsets to appear reddish) and the refraction of that light by the Earth's atmosphere into its umbra.The following simulation shows the approximate appearance of the Moon passing through the earth's shadow. The Moon's brightness is exaggerated within the umbral shadow. The southern portion of the Moon was closest to the center of the shadow, making it darkest, and most red in appearance.

text: A lunar eclipse occurs when the Moon passes within Earth's

text: umbra

text: (shadow). As the eclipse begins, the Earth's shadow first darkens the Moon slightly.  Then, the shadow begins to "cover" part of the Moon, turning it a dark red-brown color (typically - the color can vary based on atmospheric conditions).  The Moon appears to be reddish because of

text: Rayleigh scattering

text: (the same effect that causes sunsets to appear reddish) and the refraction of that light by the Earth's atmosphere into its umbra.The following simulation shows the approximate appearance of the Moon passing through the earth's shadow. The Moon's brightness is exaggerated within the umbral shadow. The southern portion of the Moon was closest to the center of the shadow, making it darkest, and most red in appearance.

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answers: It depends on atmospheric conditions

answers: NDQ_002345

answers: A lunar eclipse occurs when the Moon passes within Earth's umbra (shadow).

answers: NDQ_002348

answers: Earth's shadow

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answers: A lunar eclipse occurs when the Moon passes within Earth's umbra

answers: NDQ_002351

answers: Moon passes within Earth's umbra (shadow)

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answers: The southern portion of the Moon was closest to the center of the shadow

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answers: Solar eclipses are rare events.

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answers: Yes

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text: According to Bunun legend, in times long past, two suns shone down upon the earth and made it unbearably hot. A father and a son endured numerous hardships and finally shot down one of the suns, which then became the moon. In its wrath, the moon demanded that father and son would return to their own people to tell them that they henceforth had to obey three commandments or face annihilation. The first was that they had to constantly observe the waxing and waning of the moon and conduct all rituals and work according to its rhythm. The second commandment stated that all Bunun had to conduct rituals throughout their lives to honor the spirits of heaven and earth. The third commandment told them of forbidden behaviours, and forced them to become an orderly and peaceful tribe.

text: According to Bunun legend, in times long past, two suns shone down upon the earth and made it unbearably hot. A father and a son endured numerous hardships and finally shot down one of the suns, which then became the moon. In its wrath, the moon demanded that father and son would return to their own people to tell them that they henceforth had to obey three commandments or face annihilation. The first was that they had to constantly observe the waxing and waning of the moon and conduct all rituals and work according to its rhythm. The second commandment stated that all Bunun had to conduct rituals throughout their lives to honor the spirits of heaven and earth. The third commandment told them of forbidden behaviours, and forced them to become an orderly and peaceful tribe.

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answers: waxing

answers: NDQ_002324

answers: the moon

answers: NDQ_002325

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answers: NDQ_002326

answers: waxing

answers: NDQ_002327

answers: shoot down one of the suns

answers: NDQ_002328

answers: waxing and waning

answers: NDQ_002329

answers: waxing and waning

answers: NDQ_002330

answers: Waxing and waning

answers: NDQ_002331

answers: two suns shone down upon the earth

answers: NDQ_002332

answers: waxing

answers: NDQ_002334

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answers: NDQ_002335

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answers: NDQ_002343

answers: Waxing and waning

answers: NDQ_002345

answers: the moon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: the moon

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answers: waxing and waning

answers: NDQ_002352

answers: the penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: suns shone down upon the earth

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: It does not say.

answers: NDQ_002357

answers: waxing

answers: NDQ_002358

answers: Waxing and waning

answers: NDQ_002359

answers: the full moon

answers: NDQ_002360

answers: the moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: the waxing and waning of the moon

answers: NDQ_002363

answers: suns

answers: NDQ_002364

answers: two suns shone down upon the earth

answers: NDQ_002365

answers: waning

answers: NDQ_002366

answers: month

answers: NDQ_002367

answers: waxing

answers: NDQ_002368

answers: waning

text: A total lunar eclipse has the direct sunlight completely blocked by the earth's shadow. The only light seen is refracted through the earth's shadow. This light looks red for the same reason that the sunset looks red, due to rayleigh scattering of the more blue light. Because of its reddish color, a total lunar eclipse is sometimes called a blood moon.

text: A total lunar eclipse has the direct sunlight completely blocked by the earth's shadow. The only light seen is refracted through the earth's shadow. This light looks red for the same reason that the sunset looks red, due to

text: rayleigh scattering

text: of the more blue light. Because of its reddish color, a total lunar eclipse is sometimes called a blood moon.

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answers: total lunar eclipse

answers: NDQ_002324

answers: direct sunlight completely blocked

answers: NDQ_002325

answers: total lunar eclipse

answers: NDQ_002326

answers: total lunar eclipse

answers: NDQ_002327

answers: total lunar eclipse

answers: NDQ_002328

answers: total lunar eclipse

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answers: NDQ_002330

answers: earth's shadow

answers: NDQ_002331

answers: total lunar eclipse

answers: NDQ_002332

answers: total lunar eclipse

answers: NDQ_002334

answers: earth's shadow

answers: NDQ_002335

answers: total lunar eclipse

answers: NDQ_002343

answers: It usually lasts between 5-10 minutes.

answers: NDQ_002345

answers: direct sunlight completely blocked by the earth's shadow

answers: NDQ_002348

answers: direct sunlight completely blocked by the earth's shadow

answers: NDQ_002350

answers: A total lunar eclipse is sometimes called a blood moon

answers: NDQ_002351

answers: total lunar eclipse

answers: NDQ_002352

answers: direct sunlight completely blocked by the earth's shadow

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: A total lunar eclipse

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: It occurs once every month.

answers: NDQ_002357

answers: total lunar eclipse

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: total lunar eclipse

answers: NDQ_002360

answers: direct sunlight completely blocked by the earth's shadow

answers: NDQ_002361

answers: no

answers: NDQ_002362

answers: sunlight

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: direct sunlight completely blocked by the earth's shadow

answers: NDQ_002365

answers: total lunar eclipse

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: eclipse

text: Authorized by Congress in 1849, the American Nautical Almanac Office was founded and attached to the Department of the Navy with Charles Henry Davis as the first superintendent.  The American Ephemeris and Nautical Almanac was first published in 1852, containing data for the year 1855. Its data was originally calculated by human "computers", such as Chauncey Wright and Joseph Winlock. Between 1855 and 1881 it had two parts, the first for the meridian of Greenwich contained data on the Sun, Moon, lunar distances, Venus, Mars, Jupiter, and Saturn, which was published separately as The American Nautical Almanac. The second part contained data for the meridian of Washington on the Sun, Moon, planets, principal stars, eclipses, occultations, and other phenomena. Beginning in 1882, data for Mercury, Uranus, and Neptune was added to the first part, with eclipses, occultations, and other phenomena forming a separate third part. In 1916, The American Nautical Almanac ceased to be a reprint of the first part of the American Ephemeris and Nautical Almanac, becoming a separately prepared volume for the navigator. In 1937, the American Ephemeris and Nautical Almanac was divided into seven parts, with data for the meridian of Washington substantially reduced, then eliminated beginning in 1951. Data for Pluto was added in 1950.

text: Authorized by Congress in 1849, the American Nautical Almanac Office was founded and attached to the

text: Department of the Navy

text: with

text: Charles Henry Davis

text: as the first superintendent.  The American Ephemeris and Nautical Almanac was first published in 1852, containing data for the year 1855. Its data was originally calculated by human "computers", such as

text: Chauncey Wright

text: and

text: Joseph Winlock

text: . Between 1855 and 1881 it had two parts, the first for the

text: meridian of Greenwich

text: contained data on the

text: Sun

text: Moon

text: lunar distances

text: Venus

text: Mars

text: Jupiter

text: , and

text: Saturn

text: , which was published separately as The American Nautical Almanac. The second part contained data for the

text: meridian of Washington

text: on the Sun, Moon, planets, principal stars,

text: eclipse

text: s,

text: occultation

text: s, and other phenomena. Beginning in 1882, data for

text: Mercury

text: Uranus

text: , and

text: Neptune

text: was added to the first part, with eclipses, occultations, and other phenomena forming a separate third part. In 1916, The American Nautical Almanac ceased to be a reprint of the first part of the American Ephemeris and Nautical Almanac, becoming a separately prepared volume for the navigator. In 1937, the American Ephemeris and Nautical Almanac was divided into seven parts, with data for the meridian of Washington substantially reduced, then eliminated beginning in 1951. Data for

text: Pluto

text: was added in 1950.

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answers: eclipses

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answers: eclipsed

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: eclipses

answers: NDQ_002329

answers: Between 1855 and 1881 it had two parts

answers: NDQ_002330

answers: occultations

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answers: eclipses

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answers: NDQ_002334

answers: occultations

answers: NDQ_002335

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answers: NDQ_002343

answers: Moon

answers: NDQ_002345

answers: Between 1855 and 1881 it had two parts

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: solar eclipse

answers: NDQ_002351

answers: Between 1855 and 1881

answers: NDQ_002352

answers: Moon

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Between 1855 and 1881 it had two parts

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: between 1855 and 1881

answers: NDQ_002357

answers: Moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: lunar distances, Venus, Mars, Jupiter, and Saturn

answers: NDQ_002363

answers: meridian

answers: NDQ_002364

answers: the Sun

answers: NDQ_002365

answers: one hour

answers: NDQ_002366

answers: year

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: crescent

text: The Moon's appearance is considerably more complex. Its motion, like the Sun, is between two limits — known as lunistices rather than solstices. However, its travel between lunistices is considerably faster. It takes a sidereal month to complete its cycle rather than the year-long trek of the Sun. This is further complicated as the lunistices marking the limits of the Moon's movement move on an 18.6 year cycle. For slightly over nine years the extreme limits of the moon are outside the range of sunrise. For the remaining half of the cycle the Moon never exceeds the limits of the range of sunrise. However, much lunar observation was concerned with the phase of the Moon. The cycle from one New Moon to the next runs on an entirely different cycle, the Synodic month. Thus when examining sites for lunar significance the data can appear sparse due the extremely variable nature of the moon. See Moon for more details.

text: The Moon's appearance is considerably more complex. Its motion, like the Sun, is between two limits — known as

text: lunistices

text: rather than solstices. However, its travel between lunistices is considerably faster. It takes a

text: sidereal month

text: to complete its cycle rather than the year-long trek of the Sun. This is further complicated as the lunistices marking the limits of the Moon's movement move on

text: an 18.6 year cycle

text: . For slightly over nine years the extreme limits of the moon are outside the range of sunrise. For the remaining half of the cycle the Moon never exceeds the limits of the range of sunrise. However, much lunar observation was concerned with the

text: phase

text: of the Moon. The cycle from one

text: New Moon

text: to the next runs on an entirely different cycle, the

text: Synodic month

text: . Thus when examining sites for lunar significance the data can appear sparse due the extremely variable nature of the moon. See

text: Moon

text: for more details.

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answers: NDQ_002367

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answers: NDQ_002323

answers: New Moon

answers: NDQ_002324

answers: solstices

answers: NDQ_002325

answers: New Moon

answers: NDQ_002326

answers: New Moon

answers: NDQ_002327

answers: sunrise

answers: NDQ_002328

answers: New Moon

answers: NDQ_002329

answers: half of the cycle

answers: NDQ_002330

answers: the range of sunrise

answers: NDQ_002331

answers: solstices

answers: NDQ_002332

answers: New Moon

answers: NDQ_002334

answers: range of sunrise

answers: NDQ_002335

answers: New Moon

answers: NDQ_002343

answers: Lunar eclipse

answers: NDQ_002345

answers: The Moon's appearance

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: solstices

answers: NDQ_002351

answers: New Moon to the next

answers: NDQ_002352

answers: Penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The Moon's appearance

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: It takes a sidereal month

answers: NDQ_002357

answers: solstices

answers: NDQ_002358

answers: New Moon

answers: NDQ_002359

answers: Synodic month

answers: NDQ_002360

answers: Lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: travel between lunistices

answers: NDQ_002363

answers: solstices

answers: NDQ_002364

answers: the Sun

answers: NDQ_002365

answers: year

answers: NDQ_002366

answers: 18.6 year cycle

answers: NDQ_002367

answers: Synodic month

answers: NDQ_002368

answers: New Moon

text: The Moon's orbit around the Earth is an ellipse, as is the Earth's orbit around the Sun. The apparent sizes of the Sun and Moon therefore vary. The magnitude of an eclipse is the ratio of the apparent size of the Moon to the apparent size of the Sun during an eclipse. An eclipse that occurs when the Moon is near its closest distance to Earth (i.e., near its perigee) can be a total eclipse because the Moon will appear to be large enough to completely cover the Sun's bright disk or photosphere; a total eclipse has a magnitude greater than 1. Conversely, an eclipse that occurs when the Moon is near its farthest distance from Earth (i.e., near its apogee) can only be an annular eclipse because the Moon will appear to be slightly smaller than the Sun; the magnitude of an annular eclipse is less than 1. Slightly more solar eclipses are annular than total because, on average, the Moon lies too far from Earth to cover the Sun completely. A hybrid eclipse occurs when the magnitude of an eclipse changes during the event from less to greater than one, so the eclipse appears to be total at some locations on Earth and annular at other locations.

text: The Moon's orbit around the Earth is an

text: ellipse

text: , as is the Earth's orbit around the Sun. The apparent sizes of the Sun and Moon therefore vary. The

text: magnitude of an eclipse

text: is the ratio of the apparent size of the Moon to the apparent size of the Sun during an eclipse. An eclipse that occurs when the Moon is near its closest distance to Earth (i.e., near its

text: perigee

text: ) can be a total eclipse because the Moon will appear to be large enough to completely cover the Sun's bright disk or

text: photosphere

text: ; a total eclipse has a magnitude greater than 1. Conversely, an eclipse that occurs when the Moon is near its farthest distance from Earth (i.e., near its

text: apogee

text: ) can only be an annular eclipse because the Moon will appear to be slightly smaller than the Sun; the magnitude of an annular eclipse is less than 1. Slightly more solar eclipses are annular than total because, on average, the Moon lies too far from Earth to cover the Sun completely. A hybrid eclipse occurs when the magnitude of an eclipse changes during the event from less to greater than one, so the eclipse appears to be total at some locations on Earth and annular at other locations.

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 0

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answers: NDQ_002323

answers: annular

answers: NDQ_002324

answers: Sun and Moon

answers: NDQ_002325

answers: total

answers: NDQ_002326

answers: hybrid

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: total eclipse

answers: NDQ_002329

answers: an annular eclipse

answers: NDQ_002330

answers: perigee

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: total

answers: NDQ_002334

answers: perigee

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: an annular eclipse

answers: NDQ_002345

answers: An eclipse that occurs when the Moon is near its closest distance to Earth

answers: NDQ_002348

answers: Moon lies too far from Earth to cover the Sun completely

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: Moon's orbit around the Earth is an ellipse

answers: NDQ_002352

answers: The Moon will appear to be slightly smaller than the Sun

answers: NDQ_002353

answers: annular

answers: NDQ_002354

answers: Solar eclipses are rare events.

answers: NDQ_002355

answers: Moon lies too far from Earth to cover the Sun

answers: NDQ_002356

answers: It's impossible to say

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: Moon lies too far from Earth to cover the Sun completely

answers: NDQ_002361

answers: Moon lies too far from Earth to cover the Sun

answers: NDQ_002362

answers: Earth's orbit around the Sun

answers: NDQ_002363

answers: Earth's orbit around the Sun

answers: NDQ_002364

answers: the Moon will appear to be large enough to completely cover the Sun's bright disk

answers: NDQ_002365

answers: an annular eclipse

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: perigee

text: Solar eclipses occur when one of at least three of Pluto's moons passes between Pluto and the Sun, casting a shadow on Pluto. This occurs when one of the satellites' orbital nodes (the points where their orbits cross Pluto's ecliptic) lines up with Pluto and the Sun. Due to Pluto's large axial tilt, this can only occur at two points in Pluto's orbit, at perihelion and aphelion.

text: Solar eclipses

text: occur when one of at least three of Pluto's moons passes between Pluto and the Sun, casting a shadow on Pluto. This occurs when one of the satellites'

text: orbital node

text: s (the points where their orbits cross Pluto's

text: ecliptic

text: ) lines up with Pluto and the Sun. Due to Pluto's large axial tilt, this can only occur at two points in Pluto's orbit, at perihelion and aphelion.

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text: Lunar Eclipse is a 1999 Chinese film and the directorial debut from Sixth Generation director Wang Quan'an. It is also the feature film debut of Wang's most frequent collaborator/muse Yu Nan. Unlike his next two films, which focus on rural communities, Lunar Eclipse is an urban drama following the wife of a newlywed couple (Yu Nan) who becomes mesmerized by an amateur photographer (Wu Chao) who claims to have once been in love with a woman who looked just like her. The film was produced by the Beijing Film Studio.

text: Lunar Eclipse is a

text: 1999 Chinese film

text: and the

text: directorial debut

text: from Sixth Generation director

text: Wang Quan'an

text: . It is also the feature film debut of Wang's most frequent collaborator/muse

text: Yu Nan

text: . Unlike his next two films, which focus on rural communities, Lunar Eclipse is an urban drama following the wife of a newlywed couple (Yu Nan) who becomes mesmerized by an amateur photographer (Wu Chao) who claims to have once been in love with a woman who looked just like her. The film was produced by the

text: Beijing Film Studio

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text: A partial solar eclipse occurred on August 30, 1924. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on August 30, 1924. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 0

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answers: partial

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answers: polar regions

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answers: totally

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answers: partly

answers: NDQ_002327

answers: solar eclipse

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answers: solar eclipse

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answers: part of the Moon

answers: NDQ_002330

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answers: partial

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answers: It does not say.

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

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answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

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answers: Partially

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answers: A partial solar eclipse occurred on August 30, 1924

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: It's impossible to say

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

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answers: August

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answers: Moon passes between Earth and the Sun

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answers: Moon passes between Earth and the Sun

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answers: Earth

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answers: the Moon passes between Earth and the Sun

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answers: total or partly

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answers: Earth

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answers: quarter moon

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answers: partial solar eclipse

text: Former U.S. President George W. Bush, in an address about his Vision for Space Exploration, suggested that the Moon may serve as a cost-effective construction, launching and fueling site for future space exploration missions. As President Bush noted, "(Lunar) soil contains raw materials that might be harvested and processed into rocket fuel or breathable air."  For example, the proposed Ares V heavy-lift rocket system could cost-effectively deliver raw materials from Earth to a docking station, (connected to the lunar elevator as a counterweight,) where future spacecraft could be built and launched, while extracted lunar resources could be shipped up from a base on the Moon's surface, near the elevator's anchoring point. If the elevator was connected somehow to a lunar base built near the Moon's north pole, then workers could also mine the water ice which is known to exist there, providing an ample source of readily accessible water for the crew at the elevator's docking station. Also, since the total energy needed for transit between the Moon and Mars is considerably less than for between Earth and Mars, this concept could lower some of the engineering obstacles to sending humans to Mars.

text: Former

text: U.S. President

text: George W. Bush

text: , in an address about his

text: Vision for Space Exploration

text: , suggested that the Moon may serve as a cost-effective construction, launching and fueling

text: site

text: for future space exploration missions. As President Bush noted, "(Lunar) soil contains raw materials that might be harvested and processed into rocket fuel or breathable air."  For example, the proposed

text: Ares V

text: heavy-lift rocket system could cost-effectively deliver

text: raw material

text: s from Earth to a

text: docking station

text: , (connected to the lunar elevator as a counterweight,) where future spacecraft could be built and launched, while extracted lunar resources could be shipped up from a base on the Moon's surface, near the elevator's anchoring point. If the elevator was connected somehow to a lunar base built near the Moon's north pole, then workers could also mine the water ice which is known to exist there, providing an ample source of readily accessible water for the crew at the elevator's docking station. Also, since the total energy needed for transit between the Moon and Mars is considerably less than for between Earth and Mars, this concept could lower some of the engineering obstacles to sending humans to Mars.

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text: Unlike a solar eclipse, which can be viewed only from a certain relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of the Earth. A lunar eclipse lasts for a few hours, whereas a total solar eclipse lasts for only a few minutes at any given place, due to the smaller size of the Moon's shadow. Also unlike solar eclipses, lunar eclipses are safe to view without any eye protection or special precautions, as they are dimmer than the full moon.

text: Unlike a

text: solar eclipse

text: , which can be viewed only from a certain relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of the Earth. A lunar eclipse lasts for a few hours, whereas a total solar eclipse lasts for only a few minutes at any given place, due to the smaller size of the Moon's shadow. Also unlike solar eclipses, lunar eclipses are safe to view without any eye protection or special precautions, as they are dimmer than the full moon.

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answers: A lunar eclipse

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answers: lunar eclipse

text: The proximity of the Moon in relation to Earth and Earth in relation to the Sun also has an effect on tidal ranges.  The Moon moves around Earth in an elliptic orbit that takes about 29 days to complete.  The gravitational force is greatest when the Moon is at perigee — closest to Earth — and least when it is at apogee — farthest from Earth — about two weeks after perigee.  The Moon has a larger effect on the tides than the Sun, but the Sun’s position also has an influence on the tides.  Earth moves around the Sun in an elliptic orbit that takes a little over 365 days to complete.  Its gravitational force is greatest when the Earth is at perihelion — closest to the Sun in early January — and least when the Earth is at aphelion — farthest from the Sun in early July.

text: The proximity of the Moon in relation to Earth and Earth in relation to the Sun also has an effect on tidal ranges.  The Moon moves around Earth in an elliptic orbit that takes about 29 days to complete.  The gravitational force is greatest when the Moon is at

text: perigee

text: — closest to Earth — and least when it is at

text: apogee

text: — farthest from Earth — about two weeks after perigee.  The Moon has a larger effect on the tides than the Sun, but the Sun’s position also has an influence on the tides.  Earth moves around the Sun in an

text: elliptic orbit

text: that takes a little over 365 days to complete.  Its

text: gravitational force

text: is greatest when the Earth is at perihelion — closest to the Sun in early January — and least when the Earth is at aphelion — farthest from the Sun in early July.

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answers: 0

answers: NDQ_002323

answers: 0

answers: NDQ_002324

answers: perihelion

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 0

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 4

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

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answers: 4

answers: NDQ_002352

answers: 0

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answers: 0

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answers: 0

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 4

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 2

answers: NDQ_002368

answers: 3

answers: NDQ_002323

answers: perigee

answers: NDQ_002324

answers: aphelion

answers: NDQ_002325

answers: apogee

answers: NDQ_002326

answers: perigee

answers: NDQ_002327

answers: perihelion

answers: NDQ_002328

answers: aphelion

answers: NDQ_002329

answers: about two weeks after

answers: NDQ_002330

answers: apogee

answers: NDQ_002331

answers: perihelion

answers: NDQ_002332

answers: apogee

answers: NDQ_002334

answers: apogee

answers: NDQ_002335

answers: perigee

answers: NDQ_002343

answers: about two weeks after perigee

answers: NDQ_002345

answers: The Moon has a larger effect on the tides than the Sun

answers: NDQ_002348

answers: The Moon has a larger effect on the tides than the Sun

answers: NDQ_002350

answers: Earth in relation to the Sun

answers: NDQ_002351

answers: about two weeks after perigee

answers: NDQ_002352

answers: apogee

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: The Moon has a larger effect on the tides than the Sun

answers: NDQ_002355

answers: Moon moves around Earth in an elliptic orbit

answers: NDQ_002356

answers: Its gravitational force is greatest when the Earth is at perihelion

answers: NDQ_002357

answers: apogee

answers: NDQ_002358

answers: about two weeks after perigee

answers: NDQ_002359

answers: about two weeks after perigee

answers: NDQ_002360

answers: Moon has a larger effect on the tides

answers: NDQ_002361

answers: Earth in relation to the Sun

answers: NDQ_002362

answers: the Sun’s position also has an influence on the tides

answers: NDQ_002363

answers: Earth moves around the Sun

answers: NDQ_002364

answers: the Earth is at aphelion

answers: NDQ_002365

answers: 29 days

answers: NDQ_002366

answers: 29 days

answers: NDQ_002367

answers: 29 days

answers: NDQ_002368

answers: perigee

text: The Moon's phases do not repeat very regularly: the time between two similar syzygies may vary between 29.272 and 29.833 days (see new moon for a detailed account). The reason is that the orbit of the Moon is elliptic, its velocity is not constant, so the time of the true syzygy will differ from the mean syzygy.

text: The Moon's

text: phases

text: do not repeat very regularly: the time between two similar syzygies may vary between 29.272 and 29.833 days (see

text: new moon

text: for a detailed account). The reason is that the orbit of the Moon is elliptic, its velocity is not constant, so the time of the true syzygy will differ from the mean syzygy.

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answers: 4

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answers: 4

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answers: 0

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answers: 3

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answers: 0

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answers: 0

answers: NDQ_002323

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answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 0

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 0

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 0

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 29.272

answers: NDQ_002368

answers: 4

answers: NDQ_002323

answers: new moon

answers: NDQ_002324

answers: Moon's phases

answers: NDQ_002325

answers: new moon

answers: NDQ_002326

answers: new moon

answers: NDQ_002327

answers: new moon

answers: NDQ_002328

answers: new moon

answers: NDQ_002329

answers: 29.272

answers: NDQ_002330

answers: true syzygy

answers: NDQ_002331

answers: new moon

answers: NDQ_002332

answers: new moon

answers: NDQ_002334

answers: Moon's shadow

answers: NDQ_002335

answers: new moon

answers: NDQ_002343

answers: Moon's phases do not repeat very regularly

answers: NDQ_002345

answers: The time between two similar syzygies may vary between 29.272 and 29.833 days

answers: NDQ_002348

answers: Moon's phases

answers: NDQ_002350

answers: The Moon's phases

answers: NDQ_002351

answers: The Moon's phases do not repeat very regularly

answers: NDQ_002352

answers: Moon's phases do not repeat very regularly

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Moon's phases do not repeat very regularly

answers: NDQ_002355

answers: Partially lunar eclipse

answers: NDQ_002356

answers: Moon's phases do not repeat very regularly

answers: NDQ_002357

answers: The Moon's phases

answers: NDQ_002358

answers: The Moon's phases

answers: NDQ_002359

answers: 29.833 days

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: its velocity is not constant

answers: NDQ_002363

answers: orbit of the Moon

answers: NDQ_002364

answers: The Moon's phases

answers: NDQ_002365

answers: 29.272

answers: NDQ_002366

answers: 29.272

answers: NDQ_002367

answers: 29.272

answers: NDQ_002368

answers: new moon

text: A partial solar eclipse occurred on May 9, 1967. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on May 9, 1967. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partly obscuring

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: Moon passes between Earth and the Sun

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on May 9, 1967

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: It's impossible to say

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: May

answers: NDQ_002360

answers: The Sun

answers: NDQ_002361

answers: completely or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: May 9, 1967

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial solar eclipse

text: The only natural satellite of earth i.e.moon takes about 27.3 days to make one complete orbit around the earth. The earth orbits around the sun once every 365.2422 days (= earth’s orbital speed of 29.79 km per second). The earth and the moon in 27.3 days have moved as a system about 1/12 of the ways around the sun. This means that from one full moon to the next full moon, the moon must travel 2.2 extra days before it appears full moon. This is due to the curve of the earth’s orbit around the sun. The moon is still making one complete orbit (circle) in 27.3 days. But to line up with the earth and sun to become a full moon again it takes 29.531 days which means 354.372 days per lunar year. This makes a variance of 10.87 days a year between a lunar year and a solar year of 365.2422 days per year. To compensate this difference, the additional mass is been added after every 32.5 months on an average.

text: The only natural satellite of

text: earth

text: i.e.

text: moon

text: takes about 27.3 days to make one complete orbit around the earth. The earth orbits around the sun once every 365.2422 days (= earth’s orbital speed of 29.79 km per second). The earth and the moon in 27.3 days have moved as a system about 1/12 of the ways around the sun. This means that from one full moon to the next full moon, the moon must travel 2.2 extra days before it appears full moon. This is due to the curve of the earth’s orbit around the sun. The moon is still making one complete orbit (circle) in 27.3 days. But to line up with the earth and sun to become a full moon again it takes 29.531 days which means 354.372 days per lunar year. This makes a variance of 10.87 days a year between a lunar year and a solar year of 365.2422 days per year. To compensate this difference, the additional mass is been added after every 32.5 months on an average.

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answers: NDQ_002326

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answers: NDQ_002327

answers: full moon

answers: NDQ_002328

answers: it appears full moon

answers: NDQ_002329

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answers: NDQ_002330

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answers: NDQ_002332

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answers: NDQ_002334

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answers: NDQ_002335

answers: full moon

answers: NDQ_002343

answers: The moon must travel 2.2 extra days before it appears full moon

answers: NDQ_002345

answers: The only natural satellite of earth i.e.moon takes about 27.3 days to make one complete orbit around the earth

answers: NDQ_002348

answers: The moon must travel 2.2 extra days before it appears full moon

answers: NDQ_002350

answers: Earth orbits around the sun

answers: NDQ_002351

answers: To line up with the earth and sun to become a full moon again it takes 29.531 days

answers: NDQ_002352

answers: To compensate this difference, the additional mass is been added after every 32.5 months on an average

answers: NDQ_002353

answers: Light is only partly blocked in the umbra part of a shadow.

answers: NDQ_002354

answers: Earth orbits around the sun once every 365.2422 days

answers: NDQ_002355

answers: Part of the moon enters Earths umbra

answers: NDQ_002356

answers: 32.5 months

answers: NDQ_002357

answers: The earth orbits around the sun once every 365.2422 days

answers: NDQ_002358

answers: The moon must travel 2.2 extra days before it appears full moon

answers: NDQ_002359

answers: The moon must travel 2.2 extra days before it appears full moon

answers: NDQ_002360

answers: Earth orbits around the sun once every 365.2422 days

answers: NDQ_002361

answers: The moon must travel 2.2 extra days before it appears full moon

answers: NDQ_002362

answers: the curve of the earth’s orbit around the sun

answers: NDQ_002363

answers: Earth’s orbit around the sun

answers: NDQ_002364

answers: the sun is completely obscured by clouds

answers: NDQ_002365

answers: 29.531 days

answers: NDQ_002366

answers: 32.5 months

answers: NDQ_002367

answers: 354.372 days

answers: NDQ_002368

answers: full moon

text: The system also models the phases of the moon. The moon pointer holds a shaft along its length, on which is mounted a small gear named r, which meshes to the sun pointer at B0 (the connection between B0 and the rest of B is not visible in the original mechanism, so whether b0 is the current date/mean sun pointer or a hypothetical true sun pointer is not known). The gear rides around the dial with the moon, but is also geared to the sun — the effect is to perform a differential gear operation, so the gear turns at the synodic month period, measuring in effect, the angle of the difference between the sun and moon pointers.  The gear drives a small ball that appears through an opening in the moon pointer's face, painted longitudinally half white and half black, displaying the phases pictorially. It turns with a modelled rotational period of 29.53 days; the modern value for the synodic month is 29.530589 days.

text: The system also models the

text: phases of the moon

text: . The moon pointer holds a shaft along its length, on which is mounted a small gear named r, which meshes to the sun pointer at B0 (the connection between B0 and the rest of B is not visible in the original mechanism, so whether b0 is the current date/mean sun pointer or a hypothetical true sun pointer is not known). The gear rides around the dial with the moon, but is also geared to the sun — the effect is to perform a

text: differential gear

text: operation, so the gear turns at the synodic month period, measuring in effect, the angle of the difference between the sun and moon pointers.  The gear drives a small ball that appears through an opening in the moon pointer's face, painted longitudinally half white and half black, displaying the phases pictorially. It turns with a modelled rotational period of 29.53 days; the modern value for the synodic month is 29.530589 days.

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answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 0

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 3

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 0

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: half white

answers: NDQ_002324

answers: white and half black

answers: NDQ_002325

answers: half white

answers: NDQ_002326

answers: half white

answers: NDQ_002327

answers: phases

answers: NDQ_002328

answers: phases

answers: NDQ_002329

answers: 29.53 days

answers: NDQ_002330

answers: half white and half black

answers: NDQ_002331

answers: phase

answers: NDQ_002332

answers: half white

answers: NDQ_002334

answers: is not known

answers: NDQ_002335

answers: moon pointer

answers: NDQ_002343

answers: The gear drives a small ball

answers: NDQ_002345

answers: the angle of the difference between the sun and moon pointers

answers: NDQ_002348

answers: half white and half black

answers: NDQ_002350

answers: The gear drives a small ball

answers: NDQ_002351

answers: 29.53 days

answers: NDQ_002352

answers: half white and half black

answers: NDQ_002353

answers: half white and half black

answers: NDQ_002354

answers: The gear rides around the dial with the moon

answers: NDQ_002355

answers: Moon pointer holds a shaft

answers: NDQ_002356

answers: synodic month

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: The gear rides around the dial with the moon

answers: NDQ_002359

answers: 29.53 days

answers: NDQ_002360

answers: The gear rides around the dial with the moon

answers: NDQ_002361

answers: The gear rides around the dial with the moon

answers: NDQ_002362

answers: the angle of the difference between the sun and moon pointers

answers: NDQ_002363

answers: sun

answers: NDQ_002364

answers: angle of difference between the sun and moon pointers

answers: NDQ_002365

answers: 29.53 days

answers: NDQ_002366

answers: 29.53

answers: NDQ_002367

answers: 29.53 days

answers: NDQ_002368

answers: phases

text: An annular solar eclipse occurred on April 7, 1940. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: occurred on April 7, 1940. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 0

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answers: 0

answers: NDQ_002323

answers: 0

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answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 4

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partial

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: (ring)

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: An annular solar eclipse occurred on April 7, 1940

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: It's impossible to say

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 4

answers: NDQ_002368

answers: partial

text: V1191 Cygni is the variable star designation for an overcontact binary star system in the constellation Cygnus. First found to be variable in 1965, it is a W Ursae Majoris variable with a maximum apparent magnitude 10.82. It drops by 0.33 magnitudes during primary eclipses with a period of 0.3134 days, while dropping by 0.29 magnitudes during secondary eclipses. The primary star, which is also the cooler star, appears to have a spectral type of F6V, while the secondary is slightly cooler with a spectral type of G5V. With a mass of 1.29 solar masses and a luminosity of 2.71 solar luminosities, it is slightly more massive and luminous than the sun, while the secondary is only around 1/10 as massive and less than half as luminous. With a separation of 2.20 solar radii, the mass transfer of about 2×10 solar masses per year from the secondary to the primary is one of the highest known for a system of its type.

text: V1191 Cygni is the

text: variable star designation

text: for an

text: overcontact binary

text: star system

text: in the constellation

text: Cygnus

text: . First found to be variable in 1965, it is a

text: W Ursae Majoris variable

text: with a maximum

text: apparent magnitude

text: 10.82. It drops by 0.33 magnitudes during primary eclipses with a period of 0.3134 days, while dropping by 0.29 magnitudes during secondary eclipses. The primary star, which is also the cooler star, appears to have a

text: spectral type

text: of F6V, while the secondary is slightly cooler with a spectral type of G5V. With a mass of 1.29

text: solar mass

text: es and a luminosity of 2.71

text: solar luminosities

text: , it is slightly more massive and luminous than the sun, while the secondary is only around 1/10 as massive and less than half as luminous. With a separation of 2.20

text: solar radii

text: , the

text: mass transfer

text: of about 2×10 solar masses per year from the secondary to the primary is one of the highest known for a system of its type.

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answers: 0

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answers: 0

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answers: 0

answers: NDQ_002323

answers: 0

answers: NDQ_002324

answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 0

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 0

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 0

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 0

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 0.3134 days

answers: NDQ_002366

answers: 0

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial eclipses

answers: NDQ_002324

answers: primary eclipses

answers: NDQ_002325

answers: eclipses

answers: NDQ_002326

answers: secondary

answers: NDQ_002327

answers: eclipses

answers: NDQ_002328

answers: primary eclipses

answers: NDQ_002329

answers: half as luminous

answers: NDQ_002330

answers: drops by 0.33 magnitudes

answers: NDQ_002331

answers: eclipses

answers: NDQ_002332

answers: secondary

answers: NDQ_002334

answers: drops by 0.33 magnitudes

answers: NDQ_002335

answers: eclipses

answers: NDQ_002343

answers: period of 0.3134 days

answers: NDQ_002345

answers: It drops by 0.33 magnitudes during primary eclipses with a period of 0.3134 days

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: primary eclipses

answers: NDQ_002351

answers: 0.3134 days

answers: NDQ_002352

answers: secondary eclipses

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: It drops by 0.33 magnitudes during primary eclipses

answers: NDQ_002355

answers: partial lunar eclipses

answers: NDQ_002356

answers: 0.3134 days

answers: NDQ_002357

answers: eclipses

answers: NDQ_002358

answers: first quarter phase

answers: NDQ_002359

answers: 0.3134 days

answers: NDQ_002360

answers: lunar eclipses

answers: NDQ_002361

answers: primary eclipses

answers: NDQ_002362

answers: primary eclipses

answers: NDQ_002363

answers: solar radii

answers: NDQ_002364

answers: primary eclipses

answers: NDQ_002365

answers: 0.3134 days

answers: NDQ_002366

answers: 0.3134 days

answers: NDQ_002367

answers: 0.3134 days

answers: NDQ_002368

answers: primary eclipses

text: A solar eclipse occurs when the moon passes between the Earth and the sun, casting a shadow on Earth that temporarily obscures part or all of the sun's disc.  Eclipses can occur only when all three bodies are properly aligned.  Partial eclipses, in which only a portion of the sun's surface is obscured, are relatively common due to the width of the moon's outer shadow, or penumbra, which may be several hundred miles wide.  Total eclipses occur when the moon's inner shadow, or umbra, reaches the surface of the earth, completely obscuring the sun over a much narrower portion of the ground.  If the moon is too far away at the time of an eclipse, its umbra may not reach the Earth's surface, and only a partial eclipse will be visible.

text: A

text: solar eclipse

text: occurs when the

text: moon

text: passes between the

text: Earth

text: and the

text: sun

text: , casting a shadow on Earth that temporarily obscures part or all of the sun's disc.  Eclipses can occur only when all three bodies are properly aligned.  Partial eclipses, in which only a portion of the sun's surface is obscured, are relatively common due to the width of the moon's outer shadow, or penumbra, which may be several hundred miles wide.  Total eclipses occur when the moon's inner shadow, or umbra, reaches the surface of the earth, completely obscuring the sun over a much narrower portion of the ground.  If the moon is too far away at the time of an eclipse, its umbra may not reach the Earth's surface, and only a partial eclipse will be visible.

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answers: 0

answers: NDQ_002323

answers: 0

answers: NDQ_002324

answers: penumbra

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 4

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 3

answers: NDQ_002330

answers: 5

answers: NDQ_002331

answers: 5

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 4

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 5

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 4

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 2

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: Penumbra

answers: NDQ_002324

answers: penumbra, or umbra

answers: NDQ_002325

answers: umbra

answers: NDQ_002326

answers: Partial

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: Partial eclipses

answers: NDQ_002330

answers: umbra

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: umbra

answers: NDQ_002334

answers: penumbra

answers: NDQ_002335

answers: umbra

answers: NDQ_002343

answers: Partial eclipses

answers: NDQ_002345

answers: The moon passes between the Earth and the sun

answers: NDQ_002348

answers: The moon's inner shadow

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The moon passes between the Earth and the sun

answers: NDQ_002352

answers: penumbra

answers: NDQ_002353

answers: Partial

answers: NDQ_002354

answers: If the moon is too far away, its umbra may not reach the Earth's surface

answers: NDQ_002355

answers: Partial eclipses

answers: NDQ_002356

answers: It is relatively common

answers: NDQ_002357

answers: Partial eclipses

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The full moon will occur on the 28th

answers: NDQ_002360

answers: The moon passes between the Earth and the sun

answers: NDQ_002361

answers: If the moon is too far away

answers: NDQ_002362

answers: a solar eclipse

answers: NDQ_002363

answers: sun's disc

answers: NDQ_002364

answers: moon's inner shadow, or umbra, reaches the surface of the earth

answers: NDQ_002365

answers: temporarily

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: Penumbra

text: Tau Canis Majoris is a Beta Lyrae-type eclipsing multiple star system that varies from magnitude 4.32 to 4.37 over 1.28 days. Its four main component stars are hot O-type stars, with a combined mass 80 times that of the Sun and shining with 500,000 times its luminosity, but little is known of their individual properties. A fifth component, a magnitude 10 star, lies at a distance of . The system is only 5 million years old. UW Canis Majoris is another Beta Lyrae-type star 3000 light-years from Earth; it is an eclipsing binary that ranges in magnitude from a minimum of 5.3 to a maximum of 4.8. It has a period of 4.4 days; its components are two massive hot blue stars, one a blue supergiant of spectral type O7.5-8 Iab, while its companion is a slightly cooler, less evolved and less luminous supergiant of spectral type O9.7Ib. The stars are 200,000 and 63,000 times as luminous as the Sun. However the fainter star is the more massive at 19 solar masses to the primary's 16. R Canis Majoris is another eclipsing binary that varies from magnitude 5.7 to 6.34 over 1.13 days, with a third star orbiting these two every 93 years. The shortness of the orbital period and the low ratio between the two main components make this an unusual Algol-type system.

text: Tau Canis Majoris

text: is a

text: Beta Lyrae-type

text: eclipsing multiple star system that varies from magnitude 4.32 to 4.37 over 1.28 days. Its four main component stars are hot O-type stars, with a combined mass 80 times that of the Sun and shining with 500,000 times its luminosity, but little is known of their individual properties. A fifth component, a magnitude 10 star, lies at a distance of . The system is only 5 million years old.

text: UW Canis Majoris

text: is another Beta Lyrae-type star 3000 light-years from Earth; it is an

text: eclipsing binary

text: that ranges in magnitude from a minimum of 5.3 to a maximum of 4.8. It has a period of 4.4 days; its components are two massive hot blue stars, one a

text: blue supergiant

text: of spectral type O7.5-8 Iab, while its companion is a slightly cooler, less evolved and less luminous supergiant of spectral type O9.7Ib. The stars are 200,000 and 63,000 times as luminous as the Sun. However the fainter star is the more massive at 19

text: solar mass

text: es to the primary's 16.

text: R Canis Majoris

text: is another eclipsing binary that varies from magnitude 5.7 to 6.34 over 1.13 days, with a third star orbiting these two every 93 years. The shortness of the orbital period and the low ratio between the two main components make this an unusual Algol-type system.

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answers: 0

answers: NDQ_002323

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answers: NDQ_002324

answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 0

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 0

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 0

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

answers: NDQ_002361

answers: 0

answers: NDQ_002362

answers: 0

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 0

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: Phase of the Moon

answers: NDQ_002324

answers: Canis Majoris

answers: NDQ_002325

answers: Canis Majoris

answers: NDQ_002326

answers: right side

answers: NDQ_002327

answers: eclipsing

answers: NDQ_002328

answers: eclipsing

answers: NDQ_002329

answers: The shortness of the orbital period

answers: NDQ_002330

answers: canis majoris

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: Canis Majoris

answers: NDQ_002334

answers: canis majoris

answers: NDQ_002335

answers: Phase of the Moon

answers: NDQ_002343

answers: 1.13 days

answers: NDQ_002345

answers: Its four main component stars are hot O-type stars

answers: NDQ_002348

answers: Tau Canis Majoris

answers: NDQ_002350

answers: It has a period of 4.4 days

answers: NDQ_002351

answers: UW Canis Majoris

answers: NDQ_002352

answers: Canis Majoris

answers: NDQ_002353

answers: The shortness of the orbital period

answers: NDQ_002354

answers: This is an unusual Algol-type system

answers: NDQ_002355

answers: The system is only 5 million years old

answers: NDQ_002356

answers: It has a period of 4.4 days

answers: NDQ_002357

answers: Canis Majoris

answers: NDQ_002358

answers: Canis Majoris

answers: NDQ_002359

answers: 1.28 days

answers: NDQ_002360

answers: Canis Majoris

answers: NDQ_002361

answers: Canis Majoris

answers: NDQ_002362

answers: orbiting these two every 93 years

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: Earth

answers: NDQ_002365

answers: 1.28 days

answers: NDQ_002366

answers: 1.28 days

answers: NDQ_002367

answers: 1.28 days

answers: NDQ_002368

answers: lunar eclipse

text: In 1960, 1963, and 1978, W. H. McCrea proposed the protoplanet theory, in which the Sun and planets individually coalesced from matter within the same cloud, with the smaller planets later captured by the Sun's larger gravity. It includes fission in a protoplanetary nebula and there is no solar nebula. Agglomerations of floccules (which are presumed to compose the supersonic turbulence assumed to occur in the interstellar material from which stars are born) formed the Sun and protoplanets, the latter splitting to form planets. The 2 portions can not remain gravitationally bound to each other,  are at a mass ratio of at least 8 to 1, and for inner planets they go into independent orbits while for outer planets one of the portions exits the Solar System. The inner protoplanets were Venus-Mercury and Earth-Mars. The moons of the greater planets were formed from "droplets" in the neck connecting the 2 portions of the dividing protoplanet and these droplets could account for some of the asteroids. Terrestrial planets would have no major moons which does not account for Luna.  It predicts certain observations such as the similar angular velocity of Mars and Earth with similar rotation periods and axial tilts. In this scheme there are 6 principal planets: 2 terrestrial, Venus and Earth, 2 major, Jupiter and Saturn, and 2 outer, Uranus and Neptune; and 3 lesser planets: Mercury, Mars, and Pluto.

text: In 1960, 1963, and 1978,

text: W. H. McCrea

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text: An annular solar eclipse occurred on July 31, 1962. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: occurred on July 31, 1962. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: NDQ_002327

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answers: NDQ_002332

answers: partial

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answers: Earth

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answers: totally

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answers: Moon passes between Earth and the Sun

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

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answers: no

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answers: The time between two full moon phases is 29.5 days

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answers: (ring)

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answers: Partially

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answers: An annular solar eclipse occurred on July 31, 1962

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

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answers: The Moon passes between Earth and the Sun

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text: The combined effect of the Sun and Moon on the Earth's oceans, the tide, is greatest when the Moon is either new or full. At a lunar perigee, the tidal force is somewhat stronger, resulting in perigean spring tides.  But, even at its most powerful, this force is still relatively weak, causing tidal differences of inches at most.

text: The combined effect of the Sun and Moon on the Earth's oceans, the

text: tide

text: , is

text: greatest

text: when the Moon is either

text: new

text: or

text: full

text: . At a lunar perigee, the tidal force is somewhat stronger, resulting in

text: perigean spring tide

text: s.  But, even at its most powerful, this force is still relatively weak, causing tidal differences of inches at most.

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answers: Moon and Sun

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answers: new or full

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answers: perigean spring tides

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answers: new or full

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answers: perigee

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answers: It generally lasts between 5-10 minutes.

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answers: Moon is either new or full

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answers: Moon is either new or full

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answers: If the Moon is new or full

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answers: full

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answers: Perigee

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answers: Umbra

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answers: Partially lunar eclipse

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answers: Moon is either new or full

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answers: new

text: This eclipse at the moon's ascending node was the second of two lunar eclipses to occur in 2007. The first at the descending node was on March 3, 2007.

text: This eclipse at the moon's

text: ascending node

text: was the second of two lunar eclipses to occur in 2007. The

text: first at the descending node

text: was on March 3, 2007.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracies.

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answers: ascending

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answers: descending node

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answers: ascending

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answers: a quarter moon

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answers: ascending node

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answers: ascending

answers: NDQ_002343

answers: This eclipse at the moon's ascending node was the second of two lunar eclipses

answers: NDQ_002345

answers: The first at the descending node was on March 3, 2007.

answers: NDQ_002348

answers: The moon's ascending node

answers: NDQ_002350

answers: An eclipse at the moon's ascending node

answers: NDQ_002351

answers: The first at the descending node was on March 3, 2007.

answers: NDQ_002352

answers: The cone-shaped part of the moons shadow is the penumbra.

answers: NDQ_002353

answers: This eclipse at the moon's ascending node

answers: NDQ_002354

answers: Lunar eclipses are rare events.

answers: NDQ_002355

answers: This eclipse at the moon's ascending node

answers: NDQ_002356

answers: The first lunar eclipse at the descending node was on March 3, 2007.

answers: NDQ_002357

answers: The lunar eclipse occurs when the moon is on the opposite side of Earth from the sun.

answers: NDQ_002358

answers: The crescent phase of the moon occurs after the first quarter phase.

answers: NDQ_002359

answers: If the new moon occurs on the 1st of the month, the full moon will occur on the 28th of the month.

answers: NDQ_002360

answers: Moon's ascending node

answers: NDQ_002361

answers: When a solar eclipse occurs, the moon cannot be seen from Earth

answers: NDQ_002362

answers: lunar eclipses

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answers: Moon's ascending node

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answers: the moon's ascending node

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answers: 3 minutes

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answers: Earth

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: descending

text: After one saros, the Moon will have completed roughly an integer number of lunar orbit cycles and synodic, draconic, and anomalistic periods (241, 223, 242, and 239) and the Earth-Sun-Moon geometry will be nearly identical: the Moon will have the same phase and be at the same node and the same distance from the Earth. In addition, because the saros is close to 18 years in length (about 11 days longer), the earth will be nearly the same distance from the sun, and tilted to it in nearly the same orientation (same season). Given the date of an eclipse, one saros later a nearly identical eclipse can be predicted. During this 18-year period, about 40 other solar and lunar eclipses take place, but with a somewhat different geometry. One saros equaling 18.03 years is not equal to a perfect integer number of lunar orbits (earth revolutions with respect to the fixed stars of 27.32166 days sidereal month), therefore, even though the relative geometry of the Earth-Sun-Moon system will be nearly identical after a saros, the Moon will be in a slightly different position with respect to the stars for each eclipse in a Saros series.  The axis of rotation of the Earth-Moon system exhibits a precession period of 18.59992 years).

text: After one saros, the Moon will have completed roughly an integer number of lunar orbit cycles and synodic, draconic, and anomalistic periods (241, 223, 242, and 239) and the Earth-Sun-Moon geometry will be nearly identical: the Moon will have the same phase and be at the same node and the same distance from the Earth. In addition, because the saros is close to 18 years in length (about 11 days longer), the earth will be nearly the same distance from the sun, and tilted to it in nearly the same orientation (same season). Given the date of an eclipse, one saros later a nearly identical eclipse can be predicted. During this 18-year period, about 40 other solar and lunar eclipses take place, but with a somewhat different geometry. One saros equaling 18.03 years is not equal to a perfect integer number of lunar orbits (earth revolutions with respect to the fixed stars of 27.32166 days

text: sidereal month

text: ), therefore, even though the relative geometry of the Earth-Sun-Moon system will be nearly identical after a saros, the Moon will be in a slightly different position with respect to the stars for each eclipse in a Saros series.  The axis of rotation of the Earth-Moon system exhibits a

text: precession

text: period of 18.59992 years).

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answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: right

answers: NDQ_002327

answers: eclipse

answers: NDQ_002328

answers: eclipse

answers: NDQ_002329

answers: 11 days longer

answers: NDQ_002330

answers: the Earth-Sun-Moon geometry

answers: NDQ_002331

answers: eclipse

answers: NDQ_002332

answers: phase

answers: NDQ_002334

answers: Earth-Sun-Moon geometry

answers: NDQ_002335

answers: eclipse

answers: NDQ_002343

answers: about 11 days longer

answers: NDQ_002345

answers: The axis of rotation of the Earth-Moon system exhibits a precession period of 18.59992 years

answers: NDQ_002348

answers: Moon will have the same phase

answers: NDQ_002350

answers: Earth-Sun-Moon

answers: NDQ_002351

answers: sidereal month

answers: NDQ_002352

answers: Moon will have the same phase and be at the same node

answers: NDQ_002353

answers: The Moon will have the same phase

answers: NDQ_002354

answers: During this 18-year period, about 40 other solar and lunar eclipses take place

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: 27.32166 days sidereal month

answers: NDQ_002357

answers: Earth-Sun-Moon geometry

answers: NDQ_002358

answers: Moon will have the same phase and be at the same node

answers: NDQ_002359

answers: sidereal month

answers: NDQ_002360

answers: Moon will have the same phase and be at the same node and the same distance from the Earth

answers: NDQ_002361

answers: The Moon will have the same phase

answers: NDQ_002362

answers: Earth-Sun-Moon geometry

answers: NDQ_002363

answers: axis of rotation

answers: NDQ_002364

answers: Earth will be nearly the same distance from the sun, and tilted to it in nearly the same orientation

answers: NDQ_002365

answers: 11 days

answers: NDQ_002366

answers: saros

answers: NDQ_002367

answers: 11 days longer

answers: NDQ_002368

answers: saros

text: It is a relatively rare central eclipse where the moon passes in front of the center of the Earth's shadow. It was the "longest and deepest lunar eclipse to be seen in 7 years". In the total lunar eclipse of July 16, 2000 the moon passed within two arc minutes of the center of the Earth's shadow. In comparison, this still very deep eclipse was off-center by over 12 minutes of arc. The next total lunar eclipse of a longer duration was on June 15, 2011.

text: It is a relatively rare

text: central

text: eclipse where the moon passes in front of the center of the Earth's shadow. It was the "longest and deepest lunar eclipse to be seen in 7 years". In the

text: total lunar eclipse of July 16, 2000

text: the moon passed within two arc minutes of the center of the Earth's shadow. In comparison, this still very deep eclipse was off-center by over 12 minutes of arc. The next total lunar eclipse of a longer duration was on

text: June 15, 2011

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answers: NDQ_002327

answers: 5

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 5

answers: NDQ_002332

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answers: NDQ_002334

answers: 0

answers: NDQ_002335

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answers: 4

answers: NDQ_002345

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answers: NDQ_002348

answers: 4

answers: NDQ_002350

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answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 0

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 4

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 4

answers: NDQ_002361

answers: 0

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answers: NDQ_002363

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answers: NDQ_002364

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answers: 4

answers: NDQ_002367

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answers: NDQ_002323

answers: total

answers: NDQ_002324

answers: center

answers: NDQ_002325

answers: total

answers: NDQ_002326

answers: total lunar eclipse

answers: NDQ_002327

answers: total lunar eclipse

answers: NDQ_002328

answers: total lunar eclipse

answers: NDQ_002329

answers: the moon passes in front of the center of the Earth's shadow

answers: NDQ_002330

answers: Earth's shadow

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: total

answers: NDQ_002334

answers: Earth's shadow

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: The next total lunar eclipse of a longer duration was on June 15, 2011.

answers: NDQ_002345

answers: The moon passes in front of the Earth's shadow

answers: NDQ_002348

answers: Earth's shadow

answers: NDQ_002350

answers: The moon passes in front of the center of the Earth's shadow

answers: NDQ_002351

answers: The next total lunar eclipse of a longer duration was on June 15, 2011.

answers: NDQ_002352

answers: The next total lunar eclipse of a longer duration was on June 15, 2011.

answers: NDQ_002353

answers: The moon passes in front of the Earth's shadow.

answers: NDQ_002354

answers: The next total lunar eclipse of a longer duration was on June 15, 2011.

answers: NDQ_002355

answers: The moon passes in front of the Earth's shadow.

answers: NDQ_002356

answers: June 15, 2011

answers: NDQ_002357

answers: Earth's shadow

answers: NDQ_002358

answers: The next total lunar eclipse of a longer duration

answers: NDQ_002359

answers: The next total lunar eclipse of a longer duration was on June 15, 2011.

answers: NDQ_002360

answers: Earth's shadow

answers: NDQ_002361

answers: The moon cannot be seen from Earth.

answers: NDQ_002362

answers: Earth's shadow

answers: NDQ_002363

answers: Earth's shadow

answers: NDQ_002364

answers: the Earth's shadow

answers: NDQ_002365

answers: 12 minutes

answers: NDQ_002366

answers: 7 years

answers: NDQ_002367

answers: 7 years

answers: NDQ_002368

answers: total lunar eclipse

text: A partial solar eclipse will occur on July 12, 2094. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: will occur on July 12, 2094. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

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answers: 4

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answers: 0

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answers: 3

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 5

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answers: 0

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answers: 4

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 3

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answers: 0

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answers: 4

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answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

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answers: 4

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answers: 4

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answers: 0

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answers: 5

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answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: July 12, 2094

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: The Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse will occur on July 12, 2094

answers: NDQ_002355

answers: Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth

answers: NDQ_002356

answers: on July 12, 2094

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: July 12

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: A partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 12

answers: NDQ_002368

answers: partial

text: A full moon is often thought of as an event of a full night's duration. This is somewhat misleading because the Moon seen from Earth is continuously becoming larger and/or smaller (though much too slowly to notice with the naked eye). Its absolute maximum size occurs at the moment expansion has stopped. For any given location, about half of these absolute maximum full moons will be potentially visible, as the other half occur during the day, when the full moon is below the horizon. Many almanacs list full moons not just by date, but by their exact time as well, usually in Coordinated Universal Time (UTC). Typical monthly calendars that include phases of the Moon may be offset by one day if intended for use in a different time zone.

text: A full moon is often thought of as an event of a full night's duration. This is somewhat misleading because the Moon seen from Earth is continuously becoming larger and/or smaller (though much too slowly to notice with the

text: naked eye

text: ). Its absolute maximum size occurs at the moment expansion has stopped. For any given location, about half of these absolute maximum full moons will be potentially visible, as the other half occur during the day, when the full moon is below the horizon. Many

text: almanac

text: s list full moons not just by date, but by their exact time as well, usually in

text: Coordinated Universal Time

text: (UTC). Typical monthly

text: calendars

text: that include phases of the Moon may be offset by one day if intended for use in a different

text: time zone

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answers: A full moon

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answers: the other half occur during the day

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answers: half of these absolute maximum full moons

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answers: A lunar eclipse generally lasts between 5-10 minutes

answers: NDQ_002345

answers: Its absolute maximum size occurs at the moment expansion has stopped

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answers: Its absolute maximum size occurs at the moment expansion has stopped

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answers: full moons will be potentially visible

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answers: The other half occur during the day

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answers: Solar eclipses are rare events

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text: The eclipse was part of Saros series 136, as was the solar eclipse of July 11, 1991, which was slightly longer, lasting up to 6 minutes 53 seconds (previous eclipses of the same saros series on June 30, 1973 and June 20, 1955, were longer, lasting 7 min 04 and 7 min 08, respectively). The next event from this series will be on August 2, 2027. The exceptional duration was a result of the Moon being near perigee, with the apparent diameter of the Moon 8% larger than the Sun (magnitude 1.080) and the Earth being near aphelion where the Sun appeared slightly smaller.

text: The eclipse was part of

text: Saros series

text: 136, as was the

text: solar eclipse of July 11, 1991

text: , which was slightly longer, lasting up to 6 minutes 53 seconds (previous eclipses of the same saros series on June 30, 1973 and June 20, 1955, were longer, lasting 7 min 04 and 7 min 08, respectively). The next event from this series will be on August 2, 2027. The exceptional duration was a result of the

text: Moon

text: being near

text: perigee

text: , with the apparent diameter of the Moon 8% larger than the

text: Sun

text: magnitude

text: 1.080) and the Earth being near

text: aphelion

text: where the Sun appeared slightly smaller.

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answers: 8% larger than the Sun

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answers: 6 minutes 53 seconds

answers: NDQ_002345

answers: The eclipse was part of Saros series 136

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answers: total lunar eclipse

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answers: Earth being near aphelion

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answers: The eclipse was part of Saros series 136

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answers: Umbra

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answers: The eclipse was part of Saros series 136

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answers: Moon being near perigee

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answers: August 2, 2027

answers: NDQ_002357

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answers: 7 minutes 04

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text: The WMAP spacecraft arrived at the Kennedy Space Center on April 20, 2001. After being tested for two months, it was launched via Delta II 7425 rocket on June 30, 2001. It began operating on its internal power five minutes before its launching, and so continued operating until the solar panel array deployed. The WMAP was activated and monitored while it cooled. On July 2, it began working, first with in-flight testing (from launching until August 17), then began constant, formal work. Afterwards, it effected three Earth-Moon phase loops, measuring its sidelobes, then flew by the Moon on July 30, en route to the Sun-Earth  Lagrangian point, arriving there on October 1, 2001, becoming the first CMB observation mission posted there.

text: The WMAP spacecraft arrived at the Kennedy Space Center on April 20, 2001. After being tested for two months, it was launched via Delta II 7425 rocket on June 30, 2001. It began operating on its internal power five minutes before its launching, and so continued operating until the solar panel array deployed. The WMAP was activated and monitored while it cooled. On July 2, it began working, first with in-flight testing (from launching until August 17), then began constant, formal work. Afterwards, it effected three Earth-Moon phase loops, measuring its

text: sidelobe

text: s, then flew by the Moon on July 30, en route to the Sun-Earth

text: Lagrangian point

text: , arriving there on October 1, 2001, becoming the first CMB observation mission posted there.

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answers: right

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answers: flew by the Moon

answers: NDQ_002328

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answers: NDQ_002329

answers: sidelobes

answers: NDQ_002330

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answers: NDQ_002331

answers: Lagrangian point

answers: NDQ_002332

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answers: NDQ_002334

answers: sidelobes

answers: NDQ_002335

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answers: 5-10 minutes

answers: NDQ_002345

answers: The WMAP

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: The WMAP was activated and monitored while it cooled

answers: NDQ_002352

answers: the Moon

answers: NDQ_002353

answers: Sidelobes

answers: NDQ_002354

answers: the first CMB observation mission posted there

answers: NDQ_002355

answers: partial lunar eclipse

answers: NDQ_002356

answers: July 30

answers: NDQ_002357

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answers: NDQ_002358

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answers: NDQ_002363

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answers: 1 hour

answers: NDQ_002366

answers: Earth

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text: An annular solar eclipse will occur on March 20, 2053. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on March 20, 2053. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: an annular solar eclipse

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: It will occur on March 20, 2053

answers: NDQ_002355

answers: Partially obscuring the image of the Sun

answers: NDQ_002356

answers: March 20, 2053

answers: NDQ_002357

answers: full moon

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: March

answers: NDQ_002360

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answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

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answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: 2053

answers: NDQ_002367

answers: 2053

answers: NDQ_002368

answers: crescent

text: A partial solar eclipse will occur on September 23, 2033. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: will occur on September 23, 2033. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's

text: shadow

text: misses the Earth.

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answers: NDQ_002325

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answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: part of the Moon

answers: NDQ_002330

answers: misses

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answers: solar eclipse

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answers: The Moon passes between Earth and the Sun

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

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answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

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answers: It will occur on September 23, 2033

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

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answers: on September 23, 2033

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answers: full moon phase

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answers: September 23

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answers: totally or partly

answers: NDQ_002366

answers: Earth

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answers: 2033

answers: NDQ_002368

answers: partial

text: Minokawa is a giant bird that belongs to the dragon family. Early people believed this creature is so big that it can swallow (or cover) the sun to explain the occurrence of eclipses.  It is even described as a giant bird named Minokawa that lives in outer space which can devour the sun and the moon, and would try to do the same with the earth.

text: Minokawa is a giant bird that belongs to the

text: dragon

text: family. Early people believed this creature is so big that it can swallow (or cover) the sun to explain the occurrence of eclipses.  It is even described as a giant bird named Minokawa that lives in outer space which can devour the sun and the moon, and would try to do the same with the earth.

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text: A partial solar eclipse occurred on July 19, 1917. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on July 19, 1917. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: It does not say.

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

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answers: The Moon passes between Earth and the Sun

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answers: no

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answers: The time between two full moon phases is 29.5 days

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answers: July 19, 1917

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

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answers: It's impossible to say

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answers: partial solar eclipse

text: The solar eclipse of October 25, 2022, is a partial solar eclipse that will be visible from Europe, the Middle East, and Western Asia. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: The solar eclipse of October 25, 2022, is a partial

text: solar eclipse

text: that will be visible from Europe, the Middle East, and Western Asia. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: NDQ_002325

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answers: totally

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answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

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answers: part of the Moon

answers: NDQ_002330

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answers: NDQ_002331

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answers: NDQ_002332

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answers: misses

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answers: totally

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answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: when the Moon passes between Earth and the Sun

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answers: totally or partly obscuring

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answers: no

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answers: Moon passes between Earth and the Sun

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answers: The center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002355

answers: Solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: The solar eclipse of October 25, 2022

answers: NDQ_002357

answers: The solar eclipse

answers: NDQ_002358

answers: The first quarter phase of the moon

answers: NDQ_002359

answers: October 25

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: completely or partly

answers: NDQ_002362

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answers: NDQ_002363

answers: Earth

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answers: the Moon passes between Earth and the Sun

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answers: total or partly

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answers: partial solar eclipse

text: Regardless of the culture, all lunar months approximate the mean length of the synodic month, or how long it takes on average to pass through each phase (new, half, full moon) and back again. It takes 29–30  days. The moon completes its orbit around the earth in 27.3 days (the sidereal month), but due to the Earth's motion around the sun it has not finished a full (synodic) cycle until it reaches the point in its orbit where the sun is in the same position.

text: Regardless of the culture, all lunar months approximate the mean length of the synodic month, or how long it takes on average to pass through each phase (

text: new

text: half

text: full moon

text: ) and back again. It takes 29–30

text: day

text: s. The moon completes its orbit around the earth in 27.3 days (the sidereal month), but due to the Earth's motion around the sun it has not finished a full (synodic) cycle until it reaches the point in its orbit where the sun is in the same position.

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answers: it takes 29–30 days

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answers: NDQ_002332

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answers: NDQ_002334

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answers: It takes 29–30 days

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answers: It takes 29–30 days

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answers: Umbra

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answers: Earth's umbra

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answers: It takes 29–30 days

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answers: It takes 29–30 days

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answers: Earth's motion around the sun

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answers: the sun is in the same position

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answers: 29–30 days

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answers: half

text: An annular solar eclipse occurred on July 10, 1907. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: occurred on July 10, 1907. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: Moon passes between Earth and the Sun

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answers: The time between two full moon phases is 29.5 days.

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answers: An annular solar eclipse occurred on July 10, 1907.

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text: A partial solar eclipse occurred on August 9, 1953. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on August 9, 1953. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: The Moon passes between Earth and the Sun

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

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answers: no

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answers: The Moon passes between Earth and the Sun

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answers: A partial solar eclipse occurred on August 9, 1953

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answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

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answers: It's impossible to say

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answers: partial solar eclipse

text: If the Moon just revolved around the Earth, there would be no way to tell what fraction of the Moon's or the Earth's gravity was caused by each form of mass, since only the total can be measured. However, the orbit of the Moon is also strongly affected by the gravity of the sun—in essence, Earth and Moon are in freefall around the sun. If the energy portion of mass behaves differently from the conventional portion, then the Earth and the Moon will fall differently toward the Sun, and the orbit of the Moon around the Earth will be affected. For example, suppose the energy part of the mass does affect gravity, but does not affect inertia. Then:

text: If the Moon just revolved around the Earth, there would be no way to tell what fraction of the Moon's or the Earth's gravity was caused by each form of mass, since only the total can be measured. However, the orbit of the Moon is also strongly affected by the gravity of the sun—in essence, Earth and Moon are in freefall around the sun. If the energy portion of mass behaves differently from the conventional portion, then the Earth and the Moon will fall differently toward the Sun, and the orbit of the Moon around the Earth will be affected. For example, suppose the energy part of the mass does affect gravity, but does not affect inertia. Then:

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answers: NDQ_002326

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answers: NDQ_002327

answers: Earth and Moon are in freefall

answers: NDQ_002328

answers: the Earth and the Moon will fall differently toward the Sun

answers: NDQ_002329

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answers: NDQ_002330

answers: Earth

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answers: Earth and Moon are in freefall around the sun

answers: NDQ_002345

answers: Earth and Moon are in freefall around the sun

answers: NDQ_002348

answers: Earth and Moon are in freefall around the sun

answers: NDQ_002350

answers: Earth and Moon are in freefall around the sun

answers: NDQ_002351

answers: The orbit of the Moon is also strongly affected by the gravity of the sun

answers: NDQ_002352

answers: the Earth and the Moon will fall differently toward the Sun

answers: NDQ_002353

answers: the Earth and the Moon will fall differently toward the Sun

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answers: Earth and Moon are in freefall around the sun

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answers: Earth and Moon are in freefall around the sun

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answers: Earth and Moon are in freefall around the sun

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answers: Earth and Moon are in freefall around the sun

answers: NDQ_002358

answers: The first quarter phase of the Moon

answers: NDQ_002359

answers: Earth and Moon are in freefall around the sun

answers: NDQ_002360

answers: Moon will fall differently toward the Sun

answers: NDQ_002361

answers: Moon are in freefall around the sun

answers: NDQ_002362

answers: Earth and Moon are in freefall around the sun

answers: NDQ_002363

answers: Earth and Moon are in freefall around the sun

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answers: Earth and Moon are in freefall around the sun

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answers: Earth and Moon are in freefall around the sun

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answers: first quarter moon

answers: NDQ_002368

answers: phase of the Moon

text: China has pursued an ambitious program of lunar exploration, beginning with Chang'e 1, which successfully orbited the Moon from 5 November 2007 until its controlled lunar impact on 1 March 2009. In its sixteen-month mission, it obtained a full image map of the Moon. China followed up this success with Chang'e 2 beginning in October 2010, which reached the Moon over twice as fast as Chang'e 1, mapped the Moon at a higher resolution over an eight-month period, then left lunar orbit in favor of an extended stay at the Earth–Sun L2 Lagrangian point, before finally performing a flyby of asteroid 4179 Toutatis on 13 December 2012, and then heading off into deep space. On 14 December 2013, Chang'e 3 improved upon its orbital mission predecessors by landing a lunar lander onto the Moon's surface, which in turn deployed a lunar rover, named Yutu (Chinese: 玉兔; literally "Jade Rabbit"). In so doing, Chang'e 3 made the first lunar soft landing since Luna 24 in 1976, and the first lunar rover mission since Lunokhod 2 in 1973. China intends to launch another rover mission (Chang'e 4) before 2020, followed by a sample return mission (Chang'e 5) soon after.

text: China has pursued an ambitious

text: program of lunar exploration

text: , beginning with

text: Chang'e 1

text: , which successfully orbited the Moon from 5 November 2007 until its controlled lunar impact on 1 March 2009. In its sixteen-month mission, it obtained a full image map of the Moon. China followed up this success with

text: Chang'e 2

text: beginning in October 2010, which reached the Moon over twice as fast as Chang'e 1, mapped the Moon at a higher resolution over an eight-month period, then left lunar orbit in favor of an extended stay at the Earth–Sun L2

text: Lagrangian point

text: , before finally performing a flyby of asteroid

text: 4179 Toutatis

text: on 13 December 2012, and then heading off into deep space. On 14 December 2013,

text: Chang'e 3

text: improved upon its orbital mission predecessors by landing a lunar

text: lander

text: onto the Moon's surface, which in turn deployed a

text: lunar rover

text: , named Yutu (Chinese: 玉兔; literally "Jade Rabbit"). In so doing, Chang'e 3 made the first lunar

text: soft landing

text: since

text: Luna 24

text: in 1976, and the first lunar rover mission since

text: Lunokhod 2

text: in 1973. China intends to launch another rover mission (

text: Chang'e 4

text: ) before 2020, followed by a

text: sample return mission

text: Chang'e 5

text: ) soon after.

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answers: lunar impact

answers: NDQ_002324

answers: Lagrangian point

answers: NDQ_002325

answers: lunar impact

answers: NDQ_002326

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answers: NDQ_002327

answers: lunar impact

answers: NDQ_002328

answers: controlled lunar impact

answers: NDQ_002329

answers: eight-month

answers: NDQ_002330

answers: L2 Lagrangian point

answers: NDQ_002331

answers: Lagrangian point

answers: NDQ_002332

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answers: NDQ_002334

answers: L2 Lagrangian point

answers: NDQ_002335

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answers: NDQ_002343

answers: Luna 24

answers: NDQ_002345

answers: Chang'e 3

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth–Sun

answers: NDQ_002351

answers: Chang'e 3

answers: NDQ_002352

answers: Chang'e 3

answers: NDQ_002353

answers: Chang'e 3

answers: NDQ_002354

answers: China has pursued an ambitious program of lunar exploration

answers: NDQ_002355

answers: Partially lunar

answers: NDQ_002356

answers: 1 March

answers: NDQ_002357

answers: 1 March 2009

answers: NDQ_002358

answers: 1 March 2009

answers: NDQ_002359

answers: November

answers: NDQ_002360

answers: lunar impact

answers: NDQ_002361

answers: solar eclipse

answers: NDQ_002362

answers: asteroid 4179 Toutatis

answers: NDQ_002363

answers: Moon

answers: NDQ_002364

answers: Earth–Sun

answers: NDQ_002365

answers: 1 March 2009

answers: NDQ_002366

answers: 1 March

answers: NDQ_002367

answers: 16-month

answers: NDQ_002368

answers: Moon at a higher resolution

text: From one day to the next, the view of the Moon would change very differently for an observer on Mars than for an observer on Earth. The phase of the Moon as seen from Mars would not change much from day to day; it would match the phase of the Earth, and would only gradually change as both Earth and Moon move in their orbits around the Sun. On the other hand, an observer on Mars would see the Moon rotate, with the same period as its orbital period, and would see far side features that can never be seen from Earth.

text: From one day to the next, the view of the Moon would change very differently for an observer on Mars than for an observer on Earth. The

text: phase of the Moon

text: as seen from Mars would not change much from day to day; it would match the phase of the Earth, and would only gradually change as both Earth and Moon move in their orbits around the Sun. On the other hand, an observer on Mars would see the Moon rotate, with the same period as its orbital period, and would see far side features that can never be seen from Earth.

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answers: NDQ_002326

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answers: NDQ_002327

answers: phase

answers: NDQ_002328

answers: phase of the Moon as seen from Mars

answers: NDQ_002329

answers: phase of the Moon

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: day

answers: NDQ_002332

answers: phase

answers: NDQ_002334

answers: far side features

answers: NDQ_002335

answers: phase

answers: NDQ_002343

answers: How long does a lunar eclipse last?

answers: NDQ_002345

answers: Earth

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth would not change much from day to day

answers: NDQ_002351

answers: The phase of the Moon as seen from Mars would not change much from day to day

answers: NDQ_002352

answers: far side features

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: never be seen from Earth

answers: NDQ_002355

answers: Earths umbra

answers: NDQ_002356

answers: It would not change much from day to day

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The phase of the Moon

answers: NDQ_002360

answers: Moon

answers: NDQ_002361

answers: far side features

answers: NDQ_002362

answers: Earth and Moon move in their orbits around the Sun

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: Moon move in their orbits around the Sun

answers: NDQ_002365

answers: one day

answers: NDQ_002366

answers: day

answers: NDQ_002367

answers: day to day

answers: NDQ_002368

answers: rotate

text: As observed from the Earth, a solar eclipse occurs when the Moon passes in front of the Sun. The type of solar eclipse event depends on the distance of the Moon from the Earth during the event. A total solar eclipse occurs when the Earth intersects the umbra portion of the Moon's shadow. When the umbra does not reach the surface of the Earth, the Sun is only partially occulted, resulting in an annular eclipse. Partial solar eclipses occur when the viewer is inside the penumbra.

text: As observed from the Earth, a

text: solar eclipse

text: occurs when the Moon passes in front of the Sun. The type of solar eclipse event depends on the distance of the Moon from the Earth during the event. A total solar eclipse occurs when the Earth intersects the umbra portion of the Moon's shadow. When the umbra does not reach the surface of the Earth, the Sun is only partially occulted, resulting in an annular eclipse. Partial solar eclipses occur when the viewer is inside the penumbra.

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answers: NDQ_002323

answers: penumbra

answers: NDQ_002324

answers: umbra and penumbra

answers: NDQ_002325

answers: total

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: Partial solar eclipses

answers: NDQ_002330

answers: penumbra

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: penumbra

answers: NDQ_002334

answers: umbra

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: Moon passes in front of the Sun

answers: NDQ_002345

answers: when the umbra portion of the Moon's shadow

answers: NDQ_002348

answers: Moon passes in front of the Sun

answers: NDQ_002350

answers: It is observed from the Earth

answers: NDQ_002351

answers: Moon passes in front of the Sun

answers: NDQ_002352

answers: umbra

answers: NDQ_002353

answers: When the umbra does not reach the surface of the Earth

answers: NDQ_002354

answers: It depends on the distance of the Moon from the Earth during the event

answers: NDQ_002355

answers: Partial solar eclipses

answers: NDQ_002356

answers: The type of solar eclipse event

answers: NDQ_002357

answers: When the umbra does not reach the surface of the Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: Moon passes in front of the Sun

answers: NDQ_002360

answers: Moon passes in front of the Sun

answers: NDQ_002361

answers: when the umbra portion of the Moon's shadow

answers: NDQ_002362

answers: a solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes in front of the Sun

answers: NDQ_002365

answers: during the event

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: penumbra

text: A partial solar eclipse occurred on December 13, 1974. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on December 13, 1974. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: Solar eclipses are rare events

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: December 13, 1974

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: December 13

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: completely or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 12

answers: NDQ_002368

answers: partial

text: A lunar eclipse occurs when the Moon passes within Earth's umbra (shadow). As the eclipse begins, Earth's shadow first darkens the Moon slightly.  Then, the shadow begins to "cover" part of the Moon, turning it a dark red-brown color (typically – the color can vary based on atmospheric conditions). The Moon appears to be reddish because of Rayleigh scattering (the same effect that causes sunsets to appear reddish) and the refraction of that light by Earth's atmosphere into its umbra.

text: A lunar eclipse occurs when the Moon passes within Earth's

text: umbra

text: (shadow). As the eclipse begins, Earth's shadow first darkens the Moon slightly.  Then, the shadow begins to "cover" part of the Moon, turning it a dark red-brown color (typically – the color can vary based on atmospheric conditions). The Moon appears to be reddish because of

text: Rayleigh scattering

text: (the same effect that causes sunsets to appear reddish) and the refraction of that light by Earth's atmosphere into its umbra.

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answers: NDQ_002323

answers: umbra

answers: NDQ_002324

answers: umbra

answers: NDQ_002325

answers: umbra

answers: NDQ_002326

answers: dark red-brown

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: A lunar eclipse

answers: NDQ_002329

answers: part of the Moon

answers: NDQ_002330

answers: Earth's

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: umbra

answers: NDQ_002334

answers: Earth's

answers: NDQ_002335

answers: umbra

answers: NDQ_002343

answers: It can vary based on atmospheric conditions

answers: NDQ_002345

answers: The Moon appears to be reddish because of Rayleigh scattering

answers: NDQ_002348

answers: Earth's shadow

answers: NDQ_002350

answers: Earth's umbra (shadow)

answers: NDQ_002351

answers: Moon passes within Earth's umbra

answers: NDQ_002352

answers: umbra

answers: NDQ_002353

answers: part of the Moon

answers: NDQ_002354

answers: Solar eclipses are rare.

answers: NDQ_002355

answers: Yes

answers: NDQ_002356

answers: It depends on atmospheric conditions

answers: NDQ_002357

answers: Earth's umbra

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: Earth's shadow

answers: NDQ_002361

answers: The Moon appears to be reddish

answers: NDQ_002362

answers: Rayleigh scattering

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes within Earth's umbra

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answers: typically

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answers: Earth's

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: A partial solar eclipse occurred on June 1, 2011. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.This eclipse is the second of four partial solar eclipses in 2011, with the others occurring on January 4, 2011, July 1, 2011, and November 25, 2011.

text: A

text: partial solar eclipse

text: occurred on June 1, 2011. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.This eclipse is the second of four partial solar eclipses in 2011, with the others occurring on

text: January 4, 2011

text: July 1, 2011

text: , and

text: November 25, 2011

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answers: partial

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answers: polar regions

answers: NDQ_002325

answers: totally

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answers: totally

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: a partial solar eclipse

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: total

answers: NDQ_002343

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A partial solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: The Moon passes between Earth and the Sun

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: The Moon's shadow

answers: NDQ_002353

answers: partial solar eclipse

answers: NDQ_002354

answers: A partial solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002355

answers: The center of the Moon's shadow misses the Earth.

answers: NDQ_002356

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: A crescent phase occurs after the first quarter phase.

answers: NDQ_002359

answers: July 1, 2011

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth and the Sun

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: January 4

answers: NDQ_002368

answers: crescent

text: A total solar eclipse occurred on 11 August 1999 with an eclipse magnitude of 1.029. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.The path of the Moon's shadow began in the Atlantic Ocean and, before noon, was traversing the southern United Kingdom, northern France, Belgium, Luxembourg, southern Germany, Austria, Slovenia, Croatia, Hungary, and northern FR Yugoslavia (Vojvodina). Its maximum was at 11:03 UTC at  in Romania (next to a town called Ocnele Mari near Râmnicu Vâlcea); and it continued across Bulgaria, the Black Sea, Turkey, Iran, southern Pakistan and Srikakulam in India and ended in the Bay of Bengal.

text: A total

text: solar eclipse

text: occurred on 11 August 1999 with an

text: eclipse magnitude

text: of 1.029. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's

text: apparent diameter

text: is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.The path of the

text: Moon

text: 's shadow began in the

text: Atlantic Ocean

text: and, before noon, was traversing the southern

text: United Kingdom

text: , northern

text: France

text: Belgium

text: Luxembourg

text: , southern

text: Germany

text: Austria

text: Slovenia

text: Croatia

text: Hungary

text: , and northern

text: FR Yugoslavia

text: Vojvodina

text: ). Its maximum was at 11:03 UTC at  in

text: Romania

text: (next to a town called

text: Ocnele Mari

text: near

text: Râmnicu Vâlcea

text: ); and it continued across

text: Bulgaria

text: , the

text: Black Sea

text: Turkey

text: Iran

text: , southern

text: Pakistan

text: and

text: Srikakulam

text: in

text: India

text: and ended in the

text: Bay of Bengal

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answers: partial solar eclipse

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answers: totality

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answers: total solar eclipse

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answers: total solar eclipse

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answers: solar eclipse

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answers: total solar eclipse

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answers: partial solar eclipse

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answers: totality occurs in a narrow path

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answers: solar eclipse

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answers: total solar eclipse

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answers: totality occurs in a narrow path

answers: NDQ_002335

answers: total solar eclipse

answers: NDQ_002343

answers: Its maximum was at 11:03 UTC

answers: NDQ_002345

answers: The Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness

answers: NDQ_002348

answers: Solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002350

answers: total solar eclipse

answers: NDQ_002351

answers: Its maximum was at 11:03 UTC at in Romania

answers: NDQ_002352

answers: total solar eclipse

answers: NDQ_002353

answers: total solar eclipse

answers: NDQ_002354

answers: Its maximum was at 11:03 UTC at in Romania

answers: NDQ_002355

answers: The Moon passes between Earth and the Sun

answers: NDQ_002356

answers: Its maximum was at 11:03 UTC at in Romania

answers: NDQ_002357

answers: total solar eclipse

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: August

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: total solar eclipse

answers: NDQ_002362

answers: total solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: when the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totality

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial solar eclipse

text: In the 2nd century CE, Ptolemy estimated the mean distance of the Sun as  times Earth's radius. To determine this value, Ptolemy started by measuring the Moon's parallax, finding what amounted to a horizontal lunar parallax of 1° 26′, which was much too large. He then derived a maximum lunar distance of 64 Earth radii. Because of cancelling errors in his parallax figure, his theory of the Moon's orbit, and other factors, this figure was approximately correct. He then measured the apparent sizes of the Sun and the Moon and concluded that the apparent diameter of the Sun was equal to the apparent diameter of the Moon at the Moon's greatest distance, and from records of lunar eclipses, he estimated this apparent diameter, as well as the apparent diameter of the shadow cone of Earth traversed by the Moon during a lunar eclipse. Given these data, the distance of the Sun from Earth can be trigonometrically computed to be  Earth radii. This gives a ratio of solar to lunar distance of approximately 19, matching Aristarchus's figure. Although Ptolemy's procedure is theoretically workable, it is very sensitive to small changes in the data, so much so that changing a measurement by a few percent can make the solar distance infinite.

text: In the 2nd century CE,

text: Ptolemy

text: estimated the mean distance of the Sun as  times

text: Earth's radius

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answers: NDQ_002328

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answers: NDQ_002330

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answers: NDQ_002331

answers: 4

answers: NDQ_002332

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answers: NDQ_002343

answers: 4

answers: NDQ_002345

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answers: NDQ_002348

answers: 4

answers: NDQ_002350

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answers: NDQ_002358

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answers: 4

answers: NDQ_002360

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answers: NDQ_002361

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answers: NDQ_002362

answers: 4

answers: NDQ_002363

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answers: NDQ_002364

answers: 4

answers: NDQ_002365

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answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: lunar eclipse

answers: NDQ_002324

answers: the Moon's shadow cone

answers: NDQ_002325

answers: eclipse

answers: NDQ_002326

answers: lunar eclipse

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: 1° 26′

answers: NDQ_002330

answers: shadow cone

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: maximum lunar distance

answers: NDQ_002334

answers: shadow cone

answers: NDQ_002335

answers: lunar eclipse

answers: NDQ_002343

answers: during a lunar eclipse

answers: NDQ_002345

answers: Ptolemy

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth's

answers: NDQ_002351

answers: the Moon's orbit

answers: NDQ_002352

answers: shadow cone

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: records of lunar eclipses

answers: NDQ_002355

answers: Partial lunar eclipse

answers: NDQ_002356

answers: Ptolemy

answers: NDQ_002357

answers: lunar eclipse

answers: NDQ_002358

answers: lunar parallax

answers: NDQ_002359

answers: full moon

answers: NDQ_002360

answers: lunar eclipse

answers: NDQ_002361

answers: lunar eclipse

answers: NDQ_002362

answers: lunar eclipses

answers: NDQ_002363

answers: Earth's shadow

answers: NDQ_002364

answers: Earth traversed by the Moon during a lunar eclipse

answers: NDQ_002365

answers: 1° 26′

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: approximately 19

answers: NDQ_002368

answers: eclipses

text: A partial solar eclipse will occur on July 22, 2047. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: will occur on July 22, 2047. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: July 22, 2047

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse will occur on July 22, 2047

answers: NDQ_002355

answers: Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth

answers: NDQ_002356

answers: July 22, 2047

answers: NDQ_002357

answers: The full moon phase

answers: NDQ_002358

answers: Moon passes between Earth and the Sun

answers: NDQ_002359

answers: July 22, 2047

answers: NDQ_002360

answers: Moon passes between Earth and the Sun

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: A partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 2047

answers: NDQ_002368

answers: partial

text: A shadow cast by the Earth on the Moon is a lunar eclipse. Conversely, a shadow cast by the Moon on the Earth is a solar eclipse.

text: A shadow cast by the

text: Earth

text: on the

text: Moon

text: is a

text: lunar eclipse

text: . Conversely, a shadow cast by the Moon on the Earth is a

text: solar eclipse

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answers: 2

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answers: 0

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answers: 0

answers: NDQ_002323

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answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 5

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 4

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 4

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 5

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 4

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 3

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 4

answers: NDQ_002361

answers: 4

answers: NDQ_002362

answers: 4

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 4

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: lunar eclipse

answers: NDQ_002324

answers: Moon and Earth

answers: NDQ_002325

answers: lunar eclipse

answers: NDQ_002326

answers: lunar eclipse

answers: NDQ_002327

answers: lunar eclipse

answers: NDQ_002328

answers: lunar eclipse

answers: NDQ_002329

answers: lunar eclipse

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: lunar eclipse

answers: NDQ_002332

answers: lunar

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: solar eclipse

answers: NDQ_002343

answers: It generally lasts between 5-10 minutes

answers: NDQ_002345

answers: a solar eclipse

answers: NDQ_002348

answers: the moon is entirely dark

answers: NDQ_002350

answers: It is not.

answers: NDQ_002351

answers: 29.5 days

answers: NDQ_002352

answers: penumbra

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: solar eclipse

answers: NDQ_002355

answers: A partial lunar eclipse, only part of the moon enters Earths umbra

answers: NDQ_002356

answers: It's impossible to say

answers: NDQ_002357

answers: full moon phase

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: The full moon will occur on the 28th of the month

answers: NDQ_002360

answers: The sun cannot be seen

answers: NDQ_002361

answers: Moon cannot be seen from Earth

answers: NDQ_002362

answers: shadow cast by the Earth

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: shadow cast by the Earth on the Moon

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: lunar eclipse

text: This is a directory of lists of geological features on planets excepting Earth, moons and asteroids ordered by increasing distance from the Sun.

text: This is a directory of lists of geological features on

text: planet

text: s excepting

text: Earth

text: moon

text: s and

text: asteroid

text: s ordered by increasing distance from the

text: Sun

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answers: 0

answers: tqa2:L_0056/T_0551/6405ee242b064c77ff8f14e1329aaa2f

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answers: 0

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answers: 2

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answers: 0

answers: tqa2:L_0056/T_0551/57f0c6c69fd063e9a2821bfddd17fe34

answers: 0

answers: tqa2:L_0056/T_0551/46353e4535c5c7c1cd316ebe156a84f5

answers: 3

answers: tqa2:L_0056/T_0551/1471412cc8ffae5c85839f52af5c275c

answers: 0

answers: tqa2:L_0056/T_0551/dc1ed6431bfad12e65f2c6a604f4be5d

answers: 0

answers: tqa2:L_0056/T_0551/21a30d8ebf5733ec63a8eca4da9edd16

answers: 0

answers: NDQ_002323

answers: 0

answers: NDQ_002324

answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 0

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 0

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

answers: NDQ_002343

answers: 0

answers: NDQ_002345

answers: 0

answers: NDQ_002348

answers: 0

answers: NDQ_002350

answers: 0

answers: NDQ_002351

answers: 0

answers: NDQ_002352

answers: 0

answers: NDQ_002353

answers: 0

answers: NDQ_002354

answers: 0

answers: NDQ_002355

answers: 3

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 0

answers: NDQ_002358

answers: 0

answers: NDQ_002359

answers: 3

answers: NDQ_002360

answers: 3

answers: NDQ_002361

answers: 3

answers: NDQ_002362

answers: 0

answers: NDQ_002363

answers: 0

answers: NDQ_002364

answers: 0

answers: NDQ_002365

answers: 0

answers: NDQ_002366

answers: 0

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: Earth

answers: NDQ_002324

answers: moons

answers: NDQ_002325

answers: Moons

answers: NDQ_002326

answers: Moon

answers: NDQ_002327

answers: Moons

answers: NDQ_002328

answers: Geological features

answers: NDQ_002329

answers: distance from the Sun

answers: NDQ_002330

answers: Earth

answers: NDQ_002331

answers: Moons

answers: NDQ_002332

answers: moons

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: Earth

answers: NDQ_002343

answers: Moons

answers: NDQ_002345

answers: Earth

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: Earth

answers: NDQ_002351

answers: moons

answers: NDQ_002352

answers: Moons

answers: NDQ_002353

answers: Umbra

answers: NDQ_002354

answers: Earth

answers: NDQ_002355

answers: Earth

answers: NDQ_002356

answers: Moons

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: moons

answers: NDQ_002359

answers: moons

answers: NDQ_002360

answers: Moons

answers: NDQ_002361

answers: moons

answers: NDQ_002362

answers: asteroids

answers: NDQ_002363

answers: distance from the Sun

answers: NDQ_002364

answers: distance from the Sun

answers: NDQ_002365

answers: an hour

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: crescent

text: A wet moon (also called a Cheshire moon) is a lunar phase when the "horns" of the crescent moon point up at an angle, away from the horizon, so the moon's crescent takes on the appearance of a bowl or a smile. A wet moon occurs when the crescent moon is near the horizon at a point more or less directly above the sun's (invisible) position below the horizon.  This in turn is determined by the earth's and moon's positions in their orbits, the inclination of these orbits relative to one another and to the earth's axis, and observer's latitude on the earth.  Wet moons occur routinely in the tropics (where the sun and moon rise and set nearly vertically), and rarely in polar regions (where the sun and moon rise and set at a glancing angle or not at all).

text: A wet moon (also called a Cheshire moon) is a

text: lunar phase

text: when the "horns" of the

text: crescent moon

text: point up at an angle, away from the

text: horizon

text: , so the moon's crescent takes on the appearance of a

text: bowl

text: or a

text: smile

text: . A wet moon occurs when the crescent moon is near the horizon at a point more or less directly above the sun's (invisible) position below the horizon.  This in turn is determined by the earth's and moon's positions in their orbits, the inclination of these orbits relative to one another and to the earth's axis, and observer's latitude on the earth.  Wet moons occur routinely in the tropics (where the sun and moon rise and set nearly vertically), and rarely in polar regions (where the sun and moon rise and set at a glancing angle or not at all).

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answers: 0

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answers: tqa2:L_0056/T_0550/d0799427b9a3bd6091b5bd05d752b967

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answers: 0

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answers: 0

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answers: 4

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answers: 4

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answers: 0

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answers: 0

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answers: 4

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answers: tqa2:L_0056/T_0550/c63b3b92b2207cbfbfb7cb0c221f499c

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answers: 0

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answers: 4

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answers: 4

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answers: 0

answers: tqa2:L_0056/T_0551/97fe0f43ae0e7f174f09af636105a82e

answers: 0

answers: tqa2:L_0056/T_0551/63ef149f7a3c0585ef37bf3eab51061d

answers: 0

answers: tqa2:L_0056/T_0551/1bf9e3848e2b870faa8bcc96a62696a4

answers: 4

answers: tqa2:L_0056/T_0551/6405ee242b064c77ff8f14e1329aaa2f

answers: 0

answers: tqa2:L_0056/T_0551/2d113dfd310e3b8b4a46f4fa6df0159c

answers: 0

answers: tqa2:L_0056/T_0551/af031713061d98d0528d35ab19bfb408

answers: 4

answers: tqa2:L_0056/T_0551/04b40228beeb1f7ea790c07ba4dcd47c

answers: 4

answers: tqa2:L_0056/T_0551/57f0c6c69fd063e9a2821bfddd17fe34

answers: 0

answers: tqa2:L_0056/T_0551/46353e4535c5c7c1cd316ebe156a84f5

answers: 0

answers: tqa2:L_0056/T_0551/1471412cc8ffae5c85839f52af5c275c

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answers: tqa2:L_0056/T_0551/21a30d8ebf5733ec63a8eca4da9edd16

answers: 0

answers: NDQ_002323

answers: 0

answers: NDQ_002324

answers: 0

answers: NDQ_002325

answers: 0

answers: NDQ_002326

answers: 3

answers: NDQ_002327

answers: 0

answers: NDQ_002328

answers: 0

answers: NDQ_002329

answers: 2

answers: NDQ_002330

answers: 0

answers: NDQ_002331

answers: 0

answers: NDQ_002332

answers: 0

answers: NDQ_002334

answers: 0

answers: NDQ_002335

answers: 0

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answers: 4

answers: NDQ_002352

answers: 0

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answers: 0

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answers: 0

answers: NDQ_002355

answers: 4

answers: NDQ_002356

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: crescent

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: crescent

answers: NDQ_002326

answers: wet

answers: NDQ_002327

answers: A wet moon

answers: NDQ_002328

answers: A wet moon

answers: NDQ_002329

answers: a lunar phase

answers: NDQ_002330

answers: sun's

answers: NDQ_002331

answers: setting

answers: NDQ_002332

answers: Cheshire moon

answers: NDQ_002334

answers: sun's

answers: NDQ_002335

answers: crescent

answers: NDQ_002343

answers: A lunar eclipse generally lasts between 5-10 minutes

answers: NDQ_002345

answers: The sun's (invisible) position below the horizon

answers: NDQ_002348

answers: total lunar eclipse

answers: NDQ_002350

answers: The sun's (invisible) position below the horizon

answers: NDQ_002351

answers: The "horns" of the crescent moon point up at an angle

answers: NDQ_002352

answers: the sun's (invisible) position below the horizon

answers: NDQ_002353

answers: The sun's (invisible) position

answers: NDQ_002354

answers: polar regions

answers: NDQ_002355

answers: The sun's (invisible) position below the horizon

answers: NDQ_002356

answers: Wet moons occur routinely in the tropics

answers: NDQ_002357

answers: the sun's (invisible) position

answers: NDQ_002358

answers: A wet moon

answers: NDQ_002359

answers: The full moon will occur on the 28th

answers: NDQ_002360

answers: the sun's

answers: NDQ_002361

answers: sun's

answers: NDQ_002362

answers: A wet moon occurs when the crescent moon is near the horizon at a point more or less directly above the sun's (invisible) position below the horizon

answers: NDQ_002363

answers: sun's

answers: NDQ_002364

answers: the sun and moon rise and set nearly vertically

answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth's

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: crescent

text: A partial solar eclipse occurred on June 21, 1982. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

text: A partial

text: solar eclipse

text: occurred on June 21, 1982. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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answers: 4

answers: NDQ_002327

answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002355

answers: 3

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answers: 0

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answers: 0

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

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answers: 4

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answers: 5

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answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

answers: NDQ_002368

answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: polar regions

answers: NDQ_002325

answers: totally

answers: NDQ_002326

answers: partly

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: partly obscuring

answers: NDQ_002330

answers: misses

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: misses

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002348

answers: The Moon passes between Earth and the Sun

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The Moon passes between Earth and the Sun

answers: NDQ_002352

answers: the center

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: A partial solar eclipse occurred on June 21, 1982

answers: NDQ_002355

answers: A solar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: June 21, 1982

answers: NDQ_002357

answers: Moon passes between Earth and the Sun

answers: NDQ_002358

answers: A crescent phase

answers: NDQ_002359

answers: the 28th of the month

answers: NDQ_002360

answers: The Sun

answers: NDQ_002361

answers: completely or partly obscuring

answers: NDQ_002362

answers: partial solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: total or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: quarter moon

answers: NDQ_002368

answers: partial solar eclipse

text: An annular solar eclipse will occur on April 10, 2089. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An

text: annular

text: solar eclipse

text: will occur on April 10,

text: . A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: 3

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answers: 4

answers: NDQ_002328

answers: 4

answers: NDQ_002329

answers: 3

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answers: 0

answers: NDQ_002331

answers: 4

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answers: 0

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answers: 4

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answers: 0

answers: NDQ_002353

answers: 4

answers: NDQ_002354

answers: 4

answers: NDQ_002355

answers: 4

answers: NDQ_002356

answers: 0

answers: NDQ_002357

answers: 4

answers: NDQ_002358

answers: 4

answers: NDQ_002359

answers: 4

answers: NDQ_002360

answers: 0

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answers: 4

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answers: 4

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answers: NDQ_002364

answers: 5

answers: NDQ_002365

answers: 4

answers: NDQ_002366

answers: 4

answers: NDQ_002367

answers: 0

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answers: 0

answers: NDQ_002323

answers: partial

answers: NDQ_002324

answers: partial eclipse

answers: NDQ_002325

answers: annular

answers: NDQ_002326

answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

answers: NDQ_002329

answers: an annular solar eclipse

answers: NDQ_002330

answers: An annular solar eclipse appears as a partial eclipse

answers: NDQ_002331

answers: solar eclipse

answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

answers: NDQ_002335

answers: totally

answers: NDQ_002343

answers: The Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

answers: NDQ_002350

answers: no

answers: NDQ_002351

answers: The time between two full moon phases is 29.5 days.

answers: NDQ_002352

answers: annulus

answers: NDQ_002353

answers: Partially

answers: NDQ_002354

answers: It will occur on April 10, 2089

answers: NDQ_002355

answers: Partially obscuring the image of the Sun

answers: NDQ_002356

answers: On April 10, 2089

answers: NDQ_002357

answers: Earth

answers: NDQ_002358

answers: crescent phase

answers: NDQ_002359

answers: the 28th

answers: NDQ_002360

answers: solar eclipse

answers: NDQ_002361

answers: Moon passes between Earth and the Sun

answers: NDQ_002362

answers: solar eclipse

answers: NDQ_002363

answers: Earth

answers: NDQ_002364

answers: the Moon passes between Earth and the Sun

answers: NDQ_002365

answers: totally or partly

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 4

answers: NDQ_002368

answers: crescent

text: An annular solar eclipse will occur on October 25, 2041. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

text: An annular

text: solar eclipse

text: will occur on October 25, 2041. A

text: solar eclipse

text: occurs when the

text: Moon

text: passes between

text: Earth

text: and the

text: Sun

text: , thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's

text: apparent diameter

text: is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an

text: annulus

text: (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

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answers: NDQ_002325

answers: annular

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answers: annular

answers: NDQ_002327

answers: solar eclipse

answers: NDQ_002328

answers: solar eclipse

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answers: An annular solar eclipse appears as a partial eclipse

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answers: NDQ_002332

answers: partial

answers: NDQ_002334

answers: Earth

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answers: totally

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answers: Moon passes between Earth and the Sun

answers: NDQ_002345

answers: Moon passes between Earth and the Sun

answers: NDQ_002348

answers: totally or partly

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answers: no

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answers: The time between two full moon phases is 29.5 days

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answers: (ring)

answers: NDQ_002353

answers: partial

answers: NDQ_002354

answers: It will occur on October 25, 2041

answers: NDQ_002355

answers: A partial lunar eclipse occurs when the Moon passes between Earth and the Sun

answers: NDQ_002356

answers: On October 25, 2041

answers: NDQ_002357

answers: full moon

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answers: crescent phase

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answers: October 25

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answers: Moon passes between Earth and the Sun

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answers: the Moon passes between Earth and the Sun

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answers: crescent

text: Spaceports have been proposed for locations on the Moon, Mars, orbiting the Earth, at Sun-Earth and Earth-Moon Lagrange points, and at other locations in the solar system.  Human-tended outposts on the Moon or Mars, for example, will be spaceports by definition. The 2012 Space Studies Program of the International Space University studied the economic benefit of a network of spaceports throughout the solar system beginning from Earth and expanding outwardly in phases, within its team project Operations And Service Infrastructure for Space (OASIS). Its analysis claimed that the first phase, placing the "Node 1" spaceport with space tug services in Low Earth Orbit (LEO), would be commercially profitable and reduce transportation costs to geosynchronous orbit by as much as 44% (depending on the launch vehicle).  The second phase would add a Node 2 spaceport on the lunar surface to provide services including lunar ice mining and delivery of rocket propellants back to Node 1.  This would enable lunar surface activities and further reduce transportation costs within and out from cislunar space.  The third phase would add a Node 3 spaceport on the Martian moon Phobos to enable refueling and resupply prior to Mars surface landings, missions beyond Mars, and return trips to Earth.  In addition to propellant mining and refueling, the network of spaceports could provide services such as power storage and distribution, in-space assembly and repair of spacecraft, communications relay, shelter, construction and leasing of infrastructure, maintaining spacecraft positioned for future use, and logistics.

text: Spaceports have been proposed for locations on the

text: Moon

text: Mars

text: , orbiting the Earth, at Sun-Earth and Earth-Moon

text: Lagrange point

text: s, and at other locations in the

text: solar system

text: .  Human-tended outposts on the Moon or Mars, for example, will be spaceports by definition. The 2012 Space Studies Program of the

text: International Space University

text: studied the economic benefit of a network of spaceports throughout the solar system beginning from Earth and expanding outwardly in phases, within its team project Operations And Service Infrastructure for Space (OASIS). Its analysis claimed that the first phase, placing the "Node 1" spaceport with space tug services in

text: Low Earth Orbit

text: (LEO), would be commercially profitable and reduce transportation costs to

text: geosynchronous orbit

text: by as much as 44% (depending on the launch vehicle).  The second phase would add a Node 2 spaceport on the lunar surface to provide services including

text: lunar ice

text: mining and delivery of rocket

text: propellant

text: s back to Node 1.  This would enable lunar surface activities and further reduce transportation costs within and out from

text: cislunar

text: space.  The third phase would add a Node 3 spaceport on the Martian moon

text: Phobos

text: to enable refueling and resupply prior to Mars surface landings, missions beyond Mars, and return trips to Earth.  In addition to propellant mining and refueling, the network of spaceports could provide services such as power storage and distribution, in-space assembly and repair of spacecraft, communications relay, shelter, construction and leasing of infrastructure, maintaining spacecraft positioned for future use, and logistics.

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answers: NDQ_002327

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answers: Moon

answers: NDQ_002361

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answers: NDQ_002362

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answers: NDQ_002363

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answers: NDQ_002364

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answers: NDQ_002365

answers: a few minutes

answers: NDQ_002366

answers: Earth

answers: NDQ_002367

answers: 1

answers: NDQ_002368

answers: ice mining

text: Dunthorne is particularly remembered for his study of the phenomenon of the changing apparent speed of the Moon in its orbit. Edmond Halley in about 1695 had already suggested on the basis of comparison between contemporary observations and on the other hand ancient records for the timing of ancient eclipses, that the Moon was very gradually accelerating in its orbit.  (It was not yet known in Halley's or in Dunthorne's time that what is actually happening is a slowing-down of the Earth's rate of rotation – see Ephemeris time.) Dunthorne's computations, based in part on records of ancient accounts of eclipses, confirmed the apparent acceleration; and he was the first to quantify the effect, which he put at +10" (arcseconds/century^2) in terms of the difference of lunar longitude.  Dunthorne's estimate is not far from those assessed later, e.g. in 1786 by de Lalande and still not very far away from the values from about 10" to nearly 13" being derived about a century later.

text: Dunthorne is particularly remembered for his study of the phenomenon of the changing apparent speed of the

text: Moon

text: in its

text: orbit