text: is a small asteroid that is a Near-Earth object, a Potentially Hazardous Asteroid (PHA), and an Aten asteroid. This asteroid was discovered December 8, 1998, by Lincoln Near-Earth Asteroid Research (LINEAR), and was found to have frequent approaches to the Earth, Venus, and Mercury.

text: is a small

entity_name: Asteroid

text: asteroid

text: that is a

entity_name: Near-Earth object

text: Near-Earth object

text: , a

entity_name: Potentially hazardous object

text: Potentially Hazardous Asteroid

text: (PHA), and an

entity_name: Aten asteroid

text: Aten asteroid

text: . This asteroid was discovered December 8, 1998, by

entity_name: Lincoln Near-Earth Asteroid Research

text: Lincoln Near-Earth Asteroid Research

text: (LINEAR), and was found to have frequent approaches to the Earth,

entity_name: Venus

text: Venus

text: , and

entity_name: Mercury (planet)

text: Mercury

method: UvABottomUpChangeOrder

method: UNH-tfidf-stem

method: UNH-tfidf-ptsim

method: UNH-tfidf-lem

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answers: small

answers: NDQ_003822

answers: Small asteroid

answers: NDQ_003823

answers: The Earth, Venus, and Mercury

answers: NDQ_003824

answers: LINEAR

answers: NDQ_003825

answers: Small asteroid

answers: NDQ_003826

answers: Near Earth

answers: NDQ_003827

answers: frequent approaches to the Earth

answers: NDQ_003828

answers: Earth, Venus, and Mercury

answers: NDQ_003829

answers: Earth, Venus, and Mercury

answers: NDQ_003830

answers: Earth, Venus, and Mercury

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2015.

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2015.

method: dangnt-nlp

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

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answers: near-Earth

answers: NDQ_003822

answers: near-Earth

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: 0.00256 AU

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: AU

answers: NDQ_003827

answers: passed more than 1 lunar distance

answers: NDQ_003828

answers: Mars

answers: NDQ_003829

answers: 0.00256 AU

answers: NDQ_003830

answers: near-Earth asteroids

text: 4486 Mithra, provisional designation , is an eccentric asteroid and slow rotator, classified as near-Earth asteroid and potentially hazardous object, approximately 2 kilometers in diameter. It belongs to the Apollos group of asteroids and is a suspected contact-binary. It was discovered on 22 September 1987, by Belgian astronomer Eric Elst and Bulgarian astronomer Vladimir Shkodrov at Rozhen Observatory, in the Smolyan Province of Bulgaria.

text: 4486 Mithra, provisional designation , is an eccentric

text: asteroid

text: and

entity_name: List of slow rotators (minor planets)

text: slow rotator

text: , classified as

text: near-Earth

text: asteroid and

text: potentially hazardous object

text: , approximately 2 kilometers in diameter. It belongs to the

entity_name: Apollo asteroid

text: Apollo

text: s group of asteroids and is a suspected

entity_name: Contact binary (small Solar System body)

text: contact-binary

text: . It was discovered on 22 September 1987, by Belgian astronomer

entity_name: Eric Walter Elst

text: Eric Elst

text: and Bulgarian astronomer

entity_name: Vladimir Shkodrov

text: Vladimir Shkodrov

text: at

entity_name: Rozhen Observatory

text: Rozhen Observatory

text: , in the Smolyan Province of Bulgaria.

method: UNH-ecn

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answers: an eccentric asteroid

answers: NDQ_003822

answers: Apollos group

answers: NDQ_003823

answers: contact-binary

answers: NDQ_003824

answers: 4486 Mithra

answers: NDQ_003825

answers: Apollos group

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answers: Apollos group

answers: NDQ_003827

answers: potentially hazardous object

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answers: 4486 Mithra

answers: NDQ_003829

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answers: potentially hazardous object

text: The first near-Earth object to be visited by a spacecraft was asteroid 433 Eros when NASA's Near Earth Asteroid Rendezvous probe orbited it from February 2001 until landing on the asteroid surface in February 2002. A second near-Earth asteroid, 25143 Itokawa, was visited in September 2005 by the JAXA Hayabusa mission, which succeeded in taking material samples back to Earth. A third near-Earth asteroid, 4179 Toutatis, was explored by CNSA's Chang'e 2 spacecraft during a flyby in December 2012.

text: The first near-Earth object to be visited by a spacecraft was asteroid

entity_name: 433 Eros

text: 433 Eros

text: when

entity_name: NASA

text: NASA

text: 's

entity_name: NEAR Shoemaker

text: Near Earth Asteroid Rendezvous

text: probe orbited it from February 2001 until landing on the asteroid surface in February 2002. A second near-Earth asteroid,

entity_name: 25143 Itokawa

text: 25143 Itokawa

text: , was visited in September 2005 by the

entity_name: JAXA

text: JAXA

entity_name: Hayabusa

text: Hayabusa

text: mission, which succeeded in taking material samples back to Earth. A third near-Earth asteroid,

entity_name: 4179 Toutatis

text: 4179 Toutatis

text: , was explored by

entity_name: China National Space Administration

text: CNSA's

entity_name: Chang'e 2

text: Chang'e 2

text: spacecraft during a flyby in December 2012.

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answers: Near Earth

answers: NDQ_003822

answers: 433 Eros

answers: NDQ_003823

answers: Asteroids do not have craters.

answers: NDQ_003824

answers: The first near-Earth object to be visited by a spacecraft

answers: NDQ_003825

answers: 433 Eros

answers: NDQ_003826

answers: Near Earth

answers: NDQ_003827

answers: orbited

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answers: 433 Eros

answers: NDQ_003829

answers: 433 Eros

answers: NDQ_003830

answers: near-Earth objects to be visited by a spacecraft

text: With a semimajor axis of 2.628, the asteroid is orbiting between the 3:1 and 5:2 Kirkwood gaps in the main belt. Its orbital eccentricity is larger than the median value of 0.07 for the main belt, and the inclination is larger than the median of below 4°. But most of the main-belt asteroids have an eccentricity of no more than 0.4 and an inclination of up to 30°, so the orbit of 23 Thalia is not unusual for a main-belt asteroid.

text: With a

entity_name: Semi-major and semi-minor axes

text: semimajor axis

text: of 2.628, the asteroid is orbiting between the 3:1 and 5:2

entity_name: Kirkwood gap

text: Kirkwood gap

text: s in the

entity_name: Asteroid belt

text: main belt

text: . Its orbital eccentricity is larger than the median value of 0.07 for the main belt, and the inclination is larger than the median of below 4°. But most of the main-belt asteroids have an eccentricity of no more than 0.4 and an inclination of up to 30°, so the orbit of 23 Thalia is not unusual for a main-belt asteroid.

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answers: Its orbital eccentricity is larger than the median value of 0.07

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answers: 23 Thalia is not unusual for a main-belt asteroid

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answers: 23 Thalia

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answers: 23 Thalia is not unusual for a main-belt asteroid

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answers: main-belt asteroids

text: Planetesimals from the outer disc are embedded in all parts of the asteroid belt, remaining as P- and D-type asteroids. While Jupiter's resonances sweep across the asteroid belt outer disk planetesimals are captured by its inner resonances, evolve to lower eccentricities via secular resonances with in these resonances, and are released onto stable orbits as Jupiter's resonances move on. Others planetesimals are implanted in the asteroid belt during encounters with the ice giant, either directly leaving them with aphelia higher than that of the ice giant's perihelia, or by removing them from a resonance. Jumps in Jupiter's semi-major axis during its encounters with the ice giant shift the locations of its resonances, releasing some objects and capturing others. Many of those remaining after its final jump, along with others captured by the sweeping resonances as Jupiter migrates to its current location, survive as parts of the resonant populations such as the Hildas, Thule, and those in the 2:1 resonance. Objects originating in the asteroid belt can also be captured in the 2:1 resonance, along with a few among the Hilda population. The excursions the ice giant makes into the asteroid belt allows the icy planetesimals to be implanted farther into the asteroid belt, with a few reaching the inner asteroid belt with semi-major axis less than 2.5 AU. Some objects later drift into unstable resonances due to diffusion or the Yarkovsky effect and enter Earth-crossing orbits, with the Tagish Lake meteorite representing a possible fragment of an object that originated in the outer planetesimal disk. Numerical simulations of this process can roughly reproduce the distribution of P- and D-type asteroids and the size of the largest bodies, with differences such as an excess of objects smaller than 10 km being attributed to losses from collisions or the Yarkovsky effect, and the specific evolution of the planets in the model.

text: Planetesimals from the outer disc are embedded in all parts of the asteroid belt, remaining as

entity_name: P-type asteroid

text: P-

text: and

entity_name: D-type asteroid

text: D-type asteroid

text: s. While Jupiter's resonances sweep across the asteroid belt outer disk planetesimals are captured by its inner resonances, evolve to lower eccentricities via secular resonances with in these resonances, and are released onto stable orbits as Jupiter's resonances move on. Others planetesimals are implanted in the asteroid belt during encounters with the ice giant, either directly leaving them with

entity_name: Perihelion and aphelion

text: aphelia

text: higher than that of the ice giant's

text: perihelia

text: , or by removing them from a resonance. Jumps in Jupiter's semi-major axis during its encounters with the ice giant shift the locations of its resonances, releasing some objects and capturing others. Many of those remaining after its final jump, along with others captured by the sweeping resonances as Jupiter migrates to its current location, survive as parts of the resonant populations such as the Hildas,

entity_name: 279 Thule

text: Thule

text: , and those in the 2:1 resonance. Objects originating in the asteroid belt can also be captured in the 2:1 resonance, along with a few among the Hilda population. The excursions the ice giant makes into the asteroid belt allows the icy planetesimals to be implanted farther into the asteroid belt, with a few reaching the inner asteroid belt with semi-major axis less than 2.5 AU. Some objects later drift into unstable resonances due to diffusion or the

entity_name: Yarkovsky effect

text: Yarkovsky effect

text: and enter

text: Earth-crossing orbits

text: , with the

entity_name: Tagish Lake (meteorite)

text: Tagish Lake meteorite

text: representing a possible fragment of an object that originated in the outer planetesimal disk. Numerical simulations of this process can roughly reproduce the distribution of P- and D-type asteroids and the size of the largest bodies, with differences such as an excess of objects smaller than 10 km being attributed to losses from collisions or the Yarkovsky effect, and the specific evolution of the planets in the model.

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answers: planets

text: 218 Bianca is a sizeable Main belt asteroid. It is an S-type asteroid.

text: 218 Bianca is a sizeable

text: Main belt

text: asteroid

text: . It is an

entity_name: S-type asteroid

text: S-type asteroid

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answers: sizeable

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answers: 218 Bianca

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answers: no

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answers: It is an S-type asteroid

answers: NDQ_003825

answers: 218 Bianca

answers: NDQ_003826

answers: Main belt

answers: NDQ_003827

answers: sizeable

answers: NDQ_003828

answers: 218 Bianca

answers: NDQ_003829

answers: 218 Bianca

answers: NDQ_003830

answers: S-type asteroid

text: 443 Photographica is a typical Main belt asteroid. It is classified as an S-type asteroid.

text: 443 Photographica is a typical

text: Main belt

text: asteroid

text: . It is classified as an

text: S-type asteroid

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answers: Main belt

answers: NDQ_003827

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answers: classified

answers: NDQ_003822

answers: 443 Photographica

answers: NDQ_003823

answers: 443 Photographica

answers: NDQ_003824

answers: 443 Photographica is a typical Main belt asteroid

answers: NDQ_003825

answers: 443 Photographica

answers: NDQ_003826

answers: Main belt

answers: NDQ_003827

answers: orbit the Earth

answers: NDQ_003828

answers: 443 Photographica

answers: NDQ_003829

answers: 443 Photographica

answers: NDQ_003830

answers: classified as an S-type asteroid

text: is an Apollo near-Earth asteroid roughly 1.6 km in diameter that came within 6.5 million km (4 million miles, 17 lunar distances) of Earth on November 5, 2012. It was discovered on August 9, 2007 by LINEAR. It was studied by the 70 m (230 ft) Goldstone Deep Space Network antenna as it came near Earth, which resulted in radar images and other data about the asteroid, such as its rotation rate. It has an Apollo type orbit and is classified as a potentially hazardous asteroid (PHA).

text: is an

text: Apollo

entity_section: Near-Earth asteroids

text: near-Earth asteroid

text: roughly 1.6 km in diameter that came within 6.5 million km (4 million miles, 17

entity_name: Lunar distance (astronomy)

text: lunar distances

text: ) of Earth on November 5, 2012. It was discovered on August 9, 2007 by

text: LINEAR

text: . It was studied by the 70 m (230 ft) Goldstone Deep Space Network antenna as it came near Earth, which resulted in radar images and other data about the asteroid, such as its rotation rate. It has an Apollo type orbit and is classified as a

text: potentially hazardous asteroid

text: (PHA).

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answers: potentially hazardous asteroid

answers: NDQ_003822

answers: potentially hazardous asteroid

answers: NDQ_003823

answers: It was studied by the 70 m

answers: NDQ_003824

answers: It was studied by the 70 m

answers: NDQ_003825

answers: potentially hazardous asteroid

answers: NDQ_003826

answers: Earth

answers: NDQ_003827

answers: potentially hazardous asteroid

answers: NDQ_003828

answers: 17 lunar distances

answers: NDQ_003829

answers: potentially hazardous asteroid

answers: NDQ_003830

answers: potentially hazardous

text: Being the largest body in the asteroid belt, Ceres could become the main base and transport hub for future asteroid mining infrastructure, allowing mineral resources to be transported to Mars, the Moon, and Earth. Because of its small escape velocity combined with large amounts of water ice, it also could serve as a source of water, fuel, and oxygen for ships going through and beyond the asteroid belt. Transportation from Mars or the Moon to Ceres would be even more energy-efficient than transportation from Earth to the Moon.

text: Being the largest body in the asteroid belt, Ceres could become the main base and transport hub for future asteroid mining infrastructure, allowing mineral resources to be transported to

entity_name: Mars

text: Mars

text: , the

entity_name: Moon

text: Moon

text: , and Earth. Because of its small escape velocity combined with large amounts of water ice, it also could serve as a source of water, fuel, and oxygen for ships going through and beyond the asteroid belt. Transportation from Mars or the Moon to Ceres would be even more energy-efficient than transportation from Earth to the Moon.

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answers: The largest body in the asteroid belt

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answers: mining

text: The Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx) is a NASA asteroid study and sample return mission. The launch occurred on 8 September 2016. Its mission is to study asteroid 101955 Bennu, a carbonaceous asteroid, and return a sample to Earth in 2023 for detailed analysis. The material returned is expected to enable scientists to learn more about the formation and evolution of the Solar System, its initial stages of planet formation, and the source of organic compounds that led to the formation of life on Earth. If successful, OSIRIS-REx will be the first US spacecraft to return samples from an asteroid.

text: The Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx) is a

text: NASA

text: asteroid study and

entity_name: Sample-return mission

text: sample return mission

text: . The launch occurred on 8 September 2016. Its mission is to study asteroid

text: 101955 Bennu

text: , a

entity_name: C-type asteroid

text: carbonaceous asteroid

text: , and return a sample to Earth in 2023 for detailed analysis. The material returned is expected to enable scientists to learn more about the

entity_name: Formation and evolution of the Solar System

text: formation and evolution of the Solar System

text: , its initial stages of planet formation, and the source of

text: organic compound

text: s that led to the

text: formation of life

text: on Earth. If successful, OSIRIS-REx will be the first US spacecraft to return samples from an asteroid.

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answers: carbonaceous

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answers: 101955 Bennu

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answers: Its mission is to study asteroid 101955 Bennu

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answers: NASA asteroid study and sample return mission

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answers: 101955 Bennu

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answers: 101955 Bennu

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answers: The source of organic compounds

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answers: the source of organic compounds that led to the formation of life on Earth

text: The asteroid is a member of the Eos family, an orbital group of more than 4,000 asteroids, which are well known for mostly being of stony composition. It is classified as a metallic M-type by the NEOWISE mission, as a stony S-type by the Collaborative Asteroid Lightcurve Link (CALL), and as a LS-type – a transitional form between plain S-types and rare L-type asteroids – by the large-scale survey performed by the Pan-STARRS1 telescope.

text: The asteroid is a member of the

text: Eos family

text: , an orbital group of more than 4,000 asteroids, which are well known for mostly being of stony composition. It is classified as a metallic

text: M-type

text: by the

text: NEOWISE

text: mission, as a stony

text: S-type

text: by the Collaborative Asteroid Lightcurve Link (CALL), and as a LS-type – a transitional form between plain S-types and rare

text: L-type asteroids

text: – by the large-scale survey performed by the

text: Pan-STARRS

text: 1 telescope.

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answers: are well known for mostly being of stony composition

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answers: are well known for mostly being of stony composition

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answers: It is classified as a metallic M-type

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text: ) is the smallest identified dwarf planet in the Solar System, but is significantly the largest object in the asteroid belt. It was discovered on 1 January 1801 by Giuseppe Piazzi, and is named after Ceres, the Roman goddess of growing plants, the harvest, and of motherly love. It was the first asteroid discovered, taking up about one-third of the entire mass of its asteroid belt. The classification of Ceres has changed more than once and has been the subject of some disagreement. Johann Elert Bode believed Ceres to be the "missing planet" he had proposed to exist between Mars and Jupiter, at a distance of 419 million km (2.8 AU) from the Sun. Ceres was assigned a planetary symbol, and remained listed as a planet in astronomy books and tables for about half a century. The 2006 debate surrounding Pluto and what constitutes a planet led to Ceres being considered for reclassification as a planet, but in the end Ceres and Pluto were classified as the first members of the new dwarf planet category.

text: ) is the smallest identified

text: dwarf planet

text: in the Solar System, but is significantly the largest object in the

text: asteroid belt

text: . It was discovered on 1 January 1801 by Giuseppe Piazzi, and is named after Ceres, the Roman goddess of growing plants, the harvest, and of motherly love. It was the first asteroid discovered, taking up about one-third of the entire mass of its asteroid belt. The classification of Ceres has changed more than once and has been the subject of some disagreement.

text: Johann Elert Bode

text: believed Ceres to be the "missing planet" he had proposed to exist between

text: Mars

text: and

text: Jupiter

text: , at a distance of 419 million km (2.8

text: AU

text: ) from the Sun. Ceres was assigned a planetary symbol, and

text: remained listed as a planet

text: in astronomy books and tables for about half a century. The 2006 debate surrounding Pluto and what constitutes a

text: planet

text: led to Ceres being considered for reclassification as a planet, but in the end Ceres and Pluto were classified as the first members of the new

text: dwarf planet

text: category.

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answers: are significantly the largest object in the asteroid belt

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answers: asteroids are too small to have impacts with other objects

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answers: The classification of Ceres has changed more than once and has been the subject of some disagreement

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answers: are significantly the largest object in the asteroid belt

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answers: 2.8 AU from the Sun

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answers: It was the first asteroid discovered, taking up about one-third of the entire mass of its asteroid belt

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answers: The classification of Ceres has changed more than once and has been the subject of some disagreement

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answers: dwarf planet

text: The place is most noted for the rauks in the area, including Gotland's largest rauk the Jungfrun ("The Maiden"). One of the asteroids in the asteroid belt, 10103 Jungfrun, is named after it.

text: The place is most noted for the

text: rauk

text: s in the area, including Gotland's largest rauk the Jungfrun ("The Maiden"). One of the

text: asteroid

text: s in the

text: asteroid belt

text: 10103 Jungfrun

text: , is

text: named

text: after it.

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answers: asteroid belt

text: With an orbital period of 368.95 days,  is in a near 1:1 orbital resonance with Earth, and also has about the same orbit around the Sun as Earth. Unlike most near-Earth asteroids that simply fly by when they approach Earth, the Earth catches up with this asteroid from behind so that the asteroid then pauses in the vicinity of Earth. While in the vicinity of Earth, the asteroid moves in a helical (corkscrew) pattern that resembles an orbit around the Earth, like the Earth has a new moon. But it is not really a moon, because the asteroid is not gravitationally bound to the Earth, and eventually the asteroid moves on away from Earth and continues its orbit around the Sun.  was in this helical pattern from about 1997 to 2005, making the closest approach to Earth on 6 April 2001, and will not make another close approach until 2092.

text: With an

text: orbital period

text: of 368.95 days,  is in a near 1:1

text: orbital resonance

text: with

text: Earth

text: , and also has about the same orbit around the Sun as Earth. Unlike most near-Earth asteroids that simply fly by when they approach Earth, the Earth catches up with this asteroid from behind so that the asteroid then pauses in the vicinity of Earth. While in the vicinity of Earth, the asteroid moves in a

text: helical

text: (corkscrew) pattern that resembles an orbit around the Earth, like the Earth has a new moon. But it is not really a moon, because the asteroid is not gravitationally bound to the Earth, and eventually the asteroid moves on away from Earth and continues its orbit around the Sun.  was in this helical pattern from about 1997 to 2005, making the closest approach to Earth on 6 April 2001, and will not make another close approach until 2092.

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answers: is not gravitationally bound to the Earth

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answers: most near-Earth asteroids

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answers: It is not really a moon, because the asteroid is not gravitationally bound to the Earth, and eventually the asteroid moves on away from Earth

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answers: While in the vicinity of Earth, the asteroid moves in a helical (corkscrew) pattern that resembles an orbit around the Earth

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answers: While in the vicinity of Earth, the asteroid moves in a helical (corkscrew) pattern that resembles an orbit around the Earth, like the Earth has a new moon

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text: However, we do see evidence for asteroidal space weathering.  For years there had been a so-called "conundrum" in the planetary science community because, in general, the spectra of asteroids do not match the spectra of our collection of meteorites. Particularly, the spectra of S-type asteroids, did not match the spectra of the most abundant type of meteorites, ordinary chondrites (OCs). The asteroid spectra tended to be redder with a steep curvature in the visible wavelengths. However, Binzel et al. have identified near Earth asteroids with spectral properties covering the range from S-type to spectra similar to those of OC meteorites, suggesting an ongoing process is occurring that can alter the spectra of OC material to look like S-type asteroids. There is also evidence of regolith alteration from Galileo's flybys of Gaspra and Ida showing spectral differences at fresh craters. With time, the spectra of Ida and Gaspra appear to redden and lose spectral contrast. Evidence from NEAR Shoemaker's x-ray measurements of Eros indicate an ordinary chondrite composition despite a red-sloped, S-type spectrum, again suggesting that some process has altered the optical properties of the surface. Results from the Hayabusa spacecraft at the asteroid Itokawa, also ordinary chondrite in composition, shows spectral evidence of space weathering.  In addition, definitive evidence of space weathering alteration has been identified in the grains of soil returned by the Hayabusa spacecraft.  Because Itokawa is so small (550 m diameter), it was thought that the low gravity would not allow for the development of a mature regolith, however, preliminary examination of the returned samples reveals the presence of nanophase iron and other space weathering effects on several grains.  In addition, there is evidence that weathering patinas can and do develop on rock surfaces on the asteroid.  Such coatings are likely similar to the patinas found on lunar rocks.

text: However, we do see evidence for asteroidal space weathering.  For years there had been a so-called "conundrum" in the planetary science community because, in general, the spectra of asteroids do not match the spectra of our collection of meteorites. Particularly, the spectra of

text: S-type asteroid

text: s, did not match the spectra of the most abundant type of meteorites,

text: ordinary chondrite

text: s (OCs). The asteroid spectra tended to be redder with a steep curvature in the visible wavelengths. However, Binzel et al. have identified near Earth asteroids with spectral properties covering the range from S-type to spectra similar to those of OC meteorites, suggesting an ongoing process is occurring that can alter the spectra of OC material to look like S-type asteroids. There is also evidence of regolith alteration from

text: Galileo

text: 's flybys of

text: Gaspra

text: and

text: Ida

text: showing spectral differences at fresh craters. With time, the spectra of Ida and Gaspra appear to redden and lose spectral contrast. Evidence from

text: NEAR Shoemaker

text: 's x-ray measurements of

text: Eros

text: indicate an ordinary chondrite composition despite a red-sloped, S-type spectrum, again suggesting that some process has altered the optical properties of the surface. Results from the

text: Hayabusa

text: spacecraft at the asteroid

text: Itokawa

text: , also ordinary chondrite in composition, shows spectral evidence of space weathering.  In addition, definitive evidence of space weathering alteration has been identified in the grains of soil returned by the Hayabusa spacecraft.  Because Itokawa is so small (550 m diameter), it was thought that the low gravity would not allow for the development of a mature regolith, however, preliminary examination of the returned samples reveals the presence of nanophase iron and other space weathering effects on several grains.  In addition, there is evidence that weathering patinas can and do develop on rock surfaces on the asteroid.  Such coatings are likely similar to the patinas found on lunar rocks.

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answers: space weathering

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answers: Itokawa

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answers: Earth

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answers: space weathering

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answers: near Earth

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answers: meteorites

text: In a 2013 article in Wired Science, David Portree provides an overview of NEO science and proposed asteroidal missions, with an emphasis on the outcome of two conferences held in the 1970s. The International Astronomical Union minor planets workshop was held in Tucson, Arizona in March 1971 and a consensus "emerged that launching spacecraft to asteroids would be 'premature'.""In January 1978, NASA’s Office of Space Science held a workshop at the University of Chicago to "assess the state of asteroid studies and consider options for the future."

text: In a 2013 article in

text: Wired Science

text: , David Portree provides an overview of NEO science and proposed asteroidal missions, with an emphasis on the outcome of two conferences held in the 1970s. The

text: International Astronomical Union

text: minor planets workshop was held in

text: Tucson, Arizona

text: in March 1971 and a consensus "

text: emerged

text: that launching spacecraft to asteroids would be 'premature'.""In January 1978, NASA’s Office of Space Science held a workshop at the

text: University of Chicago

text: to "assess the state of asteroid studies and consider options for the future."

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text: Reviewing Marten's 2012 show Plank Salad for The Guardian, Adrian Searle concluded, "Marten makes you want to look very closely at the things she makes and the traces she leaves. Her way of thinking, with its word salads and trap-door metaphors, is dangerously infectious. I hate the idea of artists as rising stars, because they all too often turn into next year’s burned-out asteroids. But imagine what Marten might do with an asteroid. Rarely have I been so struck."

text: Reviewing Marten's 2012 show Plank Salad for

text: The Guardian

text: Adrian Searle

text: concluded, "Marten makes you want to look very closely at the things she makes and the traces she leaves. Her way of thinking, with its word salads and trap-door metaphors, is dangerously infectious. I hate the idea of artists as rising stars, because they all too often turn into next year’s burned-out asteroids. But imagine what Marten might do with an asteroid. Rarely have I been so struck."

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text: A prominent example of a linear resonance is the ν secular resonance between asteroids and Saturn. Asteroids which approach it have their eccentricity slowly increased until they become Mars-crossers, at which point they are usually ejected from the asteroid belt due to a close encounter with Mars. This resonance forms the inner and "side" boundaries of the asteroid belt around 2 AU, and at inclinations of about 20°.

text: A prominent example of a linear resonance is the ν secular resonance between

text: asteroid

text: s and

text: Saturn

text: . Asteroids which approach it have their eccentricity slowly increased until they become

text: Mars-crossers

text: , at which point they are usually ejected from the

text: asteroid belt

text: due to a close encounter with

text: Mars

text: . This resonance forms the inner and "side" boundaries of the asteroid belt around 2

text: AU

text: , and at

text: inclination

text: s of about 20°.

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answers: No

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answers: Asteroid belt around 2 AU

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answers: Mars-crossers

text: The terrestrial Planet V hypothesis was later examined by Ramon Brasser and Alessandro Morbidelli. Their work was the first to focus on the magnitude of the bombardment caused by Planet V. Brasser and Morbidelli calculated that to create the Late Heavy Bombardment Planet V would have to remove 95% of the pre-LHB main asteroid belt or 98% of the inner asteroid belt (semi-major axis < 2.5 AU). Depleting the main asteroid belt by 95% with a 0.5 Mars-mass Planet V was found to require it remain in an orbit crossing the entire asteroid belt for 300 Million years. This orbital evolution was not observed in any simulations, Planet V typically entered an Earth-crossing orbit resulting in a short dynamic lifetime before entering such an orbit. In a few percent of simulations Planet V remained in the inner belt long enough to produce the LHB. However, producing the LHB from the inner asteroid belt would require the inner asteroid belt to have begun with 4–13 times the mass, and 10-24 time the orbital density, as the rest of the asteroid belt.

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answers: main asteroid belt

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answers: main asteroid belt

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answers: Earth-crossing orbit

answers: NDQ_003828

answers: The terrestrial Planet V hypothesis

answers: NDQ_003829

answers: The terrestrial Planet V hypothesis

answers: NDQ_003830

answers: Earth-crossing

text: In earlier works, asteroids provided grist for theories as to their origin – specifically, the theory that the asteroids are remnants of an exploded planet. This naturally leads to SF plot-lines dealing with the possibility that the planet had been inhabited, and if so – that the inhabitants caused its destruction themselves, by war or gross environmental mismanagement. A further extension is from the past of the existing asteroids to the possible future destruction of Earth or other planets and their rendering into new asteroids.

text: In earlier works, asteroids provided grist for theories as to their origin – specifically, the theory that the asteroids are remnants of an exploded planet. This naturally leads to SF plot-lines dealing with the possibility that the planet had been inhabited, and if so – that the inhabitants caused its destruction themselves, by war or gross environmental mismanagement. A further extension is from the past of the existing asteroids to the possible future destruction of Earth or other planets and their rendering into new asteroids.

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answers: 4

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answers: 4

answers: NDQ_003821

answers: remnants of an exploded planet

answers: NDQ_003822

answers: are remnants of an exploded planet

answers: NDQ_003823

answers: asteroids provided grist for theories

answers: NDQ_003824

answers: asteroids provided grist for theories

answers: NDQ_003825

answers: are remnants of an exploded planet

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: destruction

answers: NDQ_003828

answers: Earth or other planets

answers: NDQ_003829

answers: destruction of Earth or other planets

answers: NDQ_003830

answers: asteroids provided grist for theories

text: According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, the asteroid measures 5.2 and 5.6 kilometers in diameter, based on a very high albedo of 0.41 and 0.39, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – taken from the Flora family's largest member and namesake, the asteroid 8 Flora – and calculates a larger diameter of 6.5 kilometers. As of 2016, no rotational light-curve has yet been obtained, and the asteroid's rotation period remains unknown.

text: According to the surveys carried out by NASA's

text: Wide-field Infrared Survey Explorer

text: and its subsequent

text: NEOWISE

text: mission, the asteroid measures 5.2 and 5.6 kilometers in diameter, based on a very high

text: albedo

text: of 0.41 and 0.39, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – taken from the Flora family's largest member and namesake, the asteroid

text: 8 Flora

text: – and calculates a larger diameter of 6.5 kilometers. As of 2016, no rotational

text: light-curve

text: has yet been obtained, and the asteroid's

text: rotation period

text: remains unknown.

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answers: NDQ_003821

answers: 4

answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 2

answers: NDQ_003825

answers: 4

answers: NDQ_003826

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answers: NDQ_003827

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answers: NDQ_003828

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answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: diameter

answers: NDQ_003822

answers: the Flora family

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: As of 2016, no rotational light-curve has yet been obtained

answers: NDQ_003825

answers: the Flora family

answers: NDQ_003826

answers: the Flora family

answers: NDQ_003827

answers: rotate

answers: NDQ_003828

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003829

answers: The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24

answers: NDQ_003830

answers: asteroid

text: The perihelion secular resonance between asteroids and Saturn (ν = g − g) helps shape the asteroid belt. Asteroids which approach it have their eccentricity slowly increased until they become Mars-crossers, at which point they are usually ejected from the asteroid belt by a close pass to Mars. This resonance forms the inner and "side" boundaries of the asteroid belt around 2 AU, and at inclinations of about 20°.

text: The

text: perihelion secular resonance

text: between

text: asteroid

text: s and

text: Saturn

text: (ν = g − g) helps shape the asteroid belt. Asteroids which approach it have their eccentricity slowly increased until they become

text: Mars-crossers

text: , at which point they are usually ejected from the

text: asteroid belt

text: by a close pass to

text: Mars

text: . This resonance forms the inner and "side" boundaries of the

text: asteroid belt

text: around 2

text: AU

text: , and at

text: inclination

text: s of about 20°.

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answers: NDQ_003821

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answers: NDQ_003826

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answers: NDQ_003828

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answers: NDQ_003829

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answers: NDQ_003830

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answers: NDQ_003821

answers: the asteroid belt

answers: NDQ_003822

answers: the asteroid belt

answers: NDQ_003823

answers: Asteroids do not have craters

answers: NDQ_003824

answers: Asteroids which approach it have their eccentricity slowly increased until they become Mars-crossers

answers: NDQ_003825

answers: the asteroid belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Mars-crossers

answers: NDQ_003828

answers: Mars-crossers

answers: NDQ_003829

answers: Mars-crossers

answers: NDQ_003830

answers: Mars-crossers

text: The Collaborative Asteroid Lightcurve Link (CALL) classifies the asteroid as a member of the Eunomia family, a large group of S-type asteroids and the most prominent family in the intermediate main-belt, while, based on its concurring orbital elements, Alvarez-Candal from the Universidad Nacional de Córdoba and others, group the asteroid into the Maria family, which is named after its namesake, the asteroid 170 Maria. It is an old-type asteroid family, about  years old, located near the area of a 3:1 resonances with Jupiter that supplies near-Earth asteroids to the inner Solar System (also see Kirkwood gap). It is estimated that every 100 million years, about 37 to 75 Maria asteroids larger than 1 kilometer become near-Earth objects.

text: The Collaborative Asteroid Lightcurve Link (CALL) classifies the asteroid as a member of the

text: Eunomia family

text: , a large group of

text: S-type

text: asteroids and the most prominent family in the intermediate main-belt, while, based on its concurring orbital elements, Alvarez-Candal from the Universidad Nacional de Córdoba and others, group the asteroid into the

text: Maria family

text: , which is named after its namesake, the asteroid

text: 170 Maria

text: . It is an old-type asteroid family, about  years old, located near the area of a 3:1

text: resonances

text: with Jupiter that supplies near-Earth asteroids to the inner Solar System (also see

text: Kirkwood gap

text: ). It is estimated that every 100 million years, about 37 to 75 Maria asteroids larger than 1 kilometer become

text: near-Earth object

text: s.

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answers: asteroids

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answers: S-type

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answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: It is estimated that every 100 million years

answers: NDQ_003825

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answers: NDQ_003826

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answers: asteroids

text: In 2014, May co-founded Asteroid Day with Apollo 9 astronaut Rusty Schweickart, B612 Foundation COO Danica Remy and German filmmaker Grigorij Richters. Asteroid Day is a global awareness campaign where people from around the world come together to learn about asteroids and what we can do to protect our planet.

text: In 2014, May co-founded

text: Asteroid Day

text: with

text: Apollo 9

text: astronaut

text: Rusty Schweickart

text: B612 Foundation

text: COO Danica Remy and German filmmaker

text: Grigorij Richters

text: Asteroid Day

text: is a global awareness campaign where people from around the world come together to learn about asteroids and what we can do to protect our planet.

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answers: our planet

answers: NDQ_003822

answers: learn about

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answers: Asteroids do not have craters

answers: NDQ_003824

answers: Asteroid Day

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answers: learn about

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answers: B612

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answers: protect

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answers: Asteroid Day

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answers: Asteroid Day

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 3.0 kilometers in diameter and its surface has a high albedo of 0.35, while the Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.24 (in accordance with the family's largest member and namesake, 8 Flora) and calculates a diameter of 2.7 kilometers.  A large-scale survey by Pan-STARRS (PS1) assigns an LS-type, presumably an intermediary spectral type between the common stony S-types and the rather rare and reddish L-type asteroids.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 3.0 kilometers in diameter and its surface has a high

text: albedo

text: of 0.35, while the Collaborative Asteroid Lightcurve Link (CALL) assumes an albedo of 0.24 (in accordance with the family's largest member and namesake,

text: 8 Flora

text: ) and calculates a diameter of 2.7 kilometers.  A large-scale survey by

text: Pan-STARRS

text: (PS1) assigns an LS-type, presumably an intermediary

text: spectral type

text: between the common stony S-types and the rather rare and reddish

text: L-type asteroid

text: s.

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answers: diameter

answers: NDQ_003822

answers: 8 Flora

answers: NDQ_003823

answers: The asteroid measures 3.0 kilometers in diameter

answers: NDQ_003824

answers: NASA's Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: 8 Flora

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: albedo of 0.24

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answers: The asteroid measures 3.0 kilometers in diameter

answers: NDQ_003830

answers: asteroids

text: The asteroid belt formed from the primordial solar nebula as a group of planetesimals. Planetesimals are the smaller precursors of the protoplanets. Between Mars and Jupiter, however, gravitational perturbations from Jupiter imbued the protoplanets with too much orbital energy for them to accrete into a planet. Collisions became too violent, and instead of fusing together, the planetesimals and most of the protoplanets shattered. As a result, 99.9% of the asteroid belt's original mass was lost in the first 100 million years of the Solar System's history. Some fragments eventually found their way into the inner Solar System, leading to meteorite impacts with the inner planets. Asteroid orbits continue to be appreciably perturbed whenever their period of revolution about the Sun forms an orbital resonance with Jupiter. At these orbital distances, a Kirkwood gap occurs as they are swept into other orbits.

text: The asteroid belt formed from the primordial

text: solar nebula

text: as a group of

text: planetesimal

text: s. Planetesimals are the smaller precursors of the

text: protoplanet

text: s. Between Mars and Jupiter, however,

text: gravitational

text: perturbations from Jupiter imbued the protoplanets with too much orbital energy for them to

text: accrete

text: into a planet. Collisions became too violent, and instead of fusing together, the planetesimals and most of the protoplanets shattered. As a result, 99.9% of the asteroid belt's original mass was lost in the first 100 million years of the Solar System's history. Some fragments eventually found their way into the inner

text: Solar System

text: , leading to meteorite impacts with the inner planets. Asteroid orbits continue to be appreciably

text: perturbed

text: whenever their period of revolution about the Sun forms an

text: orbital resonance

text: with Jupiter. At these orbital distances, a

text: Kirkwood gap

text: occurs as they are swept into other orbits.

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answers: smaller precursors of the protoplanets

answers: NDQ_003822

answers: are the smaller precursors of the protoplanets

answers: NDQ_003823

answers: meteorite impacts

answers: NDQ_003824

answers: The asteroid belt formed from the primordial solar nebula

answers: NDQ_003825

answers: are the smaller precursors of the protoplanets

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: meteorite impacts

answers: NDQ_003828

answers: meteorite impacts

answers: NDQ_003829

answers: It could cause humans to go extinct

answers: NDQ_003830

answers: protoplanets

text: 16 Psyche is one of the ten most-massive asteroids in the asteroid belt. It is over 200 kilometers in diameter and contains a little less than 1% of the mass of the entire asteroid belt.  It is thought to be the exposed iron core of a protoplanet. It is the most massive metallic M-type asteroid. Psyche was discovered by the Italian astronomer Annibale de Gasparis on 17 March 1852 from Naples and named after the Greek mythological figure Psyche.

text: 16 Psyche is one of the

text: ten most-massive

text: asteroid

text: s in the

text: asteroid belt

text: . It is over 200 kilometers in diameter and contains a little less than 1% of the mass of the entire asteroid belt.  It is thought to be the exposed iron core of a

text: protoplanet

text: . It is the most massive metallic

text: M-type asteroid

text: . Psyche was discovered by the Italian astronomer

text: Annibale de Gasparis

text: on 17 March 1852 from

text: Naples

text: and named after the

text: Greek mythological figure

text: Psyche

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answers: NDQ_003822

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answers: 16 Psyche

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answers: 16 Psyche

answers: NDQ_003825

answers: in the asteroid belt

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: protoplanet

answers: NDQ_003828

answers: 16 Psyche

answers: NDQ_003829

answers: 16 Psyche

answers: NDQ_003830

answers: protoplanet

text: is an Apollo near-Earth asteroid and potentially hazardous object discovered on 5 October 2004 by NEAT at Mount Palomar. It has the fourth smallest geocentric Minimum Orbital Intersection Distance of any asteroid, after 2008 TC3 which exploded in Earth's atmosphere in 2008, 1994 GV, and 2014 AA which also impacted the Earth in 2014. The asteroid, however, will not make any significant close approaches to Earth in at least the next century.

text: is an

text: Apollo

text: near-Earth asteroid

text: and

text: potentially hazardous object

text: discovered on 5 October 2004 by

text: NEAT

text: at

text: Mount Palomar

text: . It has the fourth smallest geocentric

text: Minimum Orbital Intersection Distance

text: of any asteroid, after

text: 2008 TC3

text: which exploded in Earth's atmosphere in 2008,

text: 1994 GV

text: , and

text: 2014 AA

text: which also impacted the Earth in 2014. The asteroid, however, will not make any significant close approaches to Earth in at least the next century.

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answers: NDQ_003821

answers: potentially hazardous object

answers: NDQ_003822

answers: The fourth smallest geocentric Minimum Orbital Intersection Distance of any

answers: NDQ_003823

answers: 2014 AA which also impacted the Earth in 2014

answers: NDQ_003824

answers: NEAT at Mount Palomar

answers: NDQ_003825

answers: The fourth smallest geocentric Minimum Orbital Intersection Distance of any

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: impact the Earth

answers: NDQ_003828

answers: 2014 AA

answers: NDQ_003829

answers: exploded in Earth's atmosphere

answers: NDQ_003830

answers: potentially hazardous object

text: In the 1980s and 1990s, NASA considered a spacecraft mission to the asteroid, including a tie-in with McDonald's. The mission plan called for a launch in 1995 and a flyby of Hamburga in early 1998.

text: In the 1980s and 1990s, NASA considered a spacecraft mission to the asteroid, including a tie-in with

text: McDonald's

text: . The mission plan called for a launch in 1995 and a flyby of Hamburga in early 1998.

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answers: NDQ_003821

answers: spacecraft

answers: NDQ_003822

answers: Hamburga

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: asteroid

answers: NDQ_003825

answers: Hamburga

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: flyby

answers: NDQ_003828

answers: Mars

answers: NDQ_003829

answers: Hamburga

answers: NDQ_003830

answers: flyby

text: If one uses the simple definition of an Amor (1.3000 AU > perihelion > 1.0000 AU), then asteroids whose perihelion is between 1.0000 AU (Earth's semi-major axis) and 1.0167 AU (Earth's aphelion) are Amor outer Earth-grazer asteroids, while those between 0.9833 AU (Earth's perihelion) and 1.0000 AU are considered Apollo outer Earth-grazer asteroids.

text: If one uses the simple definition of an Amor (1.3000 AU > perihelion > 1.0000 AU), then asteroids whose perihelion is between 1.0000 AU (Earth's semi-major axis) and 1.0167 AU (Earth's aphelion) are Amor outer Earth-grazer asteroids, while those between 0.9833 AU (Earth's perihelion) and 1.0000 AU are considered Apollo outer Earth-grazer asteroids.

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answers: Earth's perihelion

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answers: Earth's perihelion

answers: NDQ_003830

answers: Earth-grazer

text: A probable parent body for this group is the S-type asteroid 6 Hebe, with less likely candidates being 3 Juno and 7 Iris. It is supposed that these meteorites arise from impacts onto small near-Earth asteroids broken off from  6 Hebe in the past, rather than originating from 6 Hebe directly.

text: A probable parent body for this group is the

text: S-type asteroid

text: 6 Hebe

text: , with less likely candidates being

text: 3 Juno

text: and

text: 7 Iris

text: . It is supposed that these meteorites arise from impacts onto small

text: near-Earth asteroid

text: s broken off from

text: 6 Hebe

text: in the past, rather than originating from 6 Hebe directly.

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answers: asteroids

answers: NDQ_003822

answers: 6 Hebe

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroids

answers: NDQ_003825

answers: 6 Hebe

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: broken off from 6 Hebe

answers: NDQ_003828

answers: 6 Hebe

answers: NDQ_003829

answers: The S-type asteroid 6 Hebe

answers: NDQ_003830

answers: meteorites

text: The asteroid's orbit also undergoes a slow, back-and-forth twist over multiple decades. "The asteroid's loops around Earth drift a little ahead or behind from year to year, but when they drift too far forward or backward, Earth's gravity is just strong enough to reverse the drift and hold onto the asteroid so that it never wanders farther away than about 100 times the distance of the moon," said Chodas. "The same effect also prevents the asteroid from approaching much closer than about 38 times the distance of the moon. In effect, this small asteroid is caught in a little dance with Earth."

text: The asteroid's orbit also undergoes a slow, back-and-forth twist over multiple decades. "The asteroid's loops around Earth drift a little ahead or behind from year to year, but when they drift too far forward or backward, Earth's

text: gravity

text: is just strong enough to reverse the drift and hold onto the asteroid so that it never wanders farther away than about 100 times the distance of

text: the moon

text: ," said Chodas. "The same effect also prevents the asteroid from approaching much closer than about 38 times

text: the distance of the moon

text: . In effect, this small asteroid is caught in a little dance with Earth."

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text: The majority of known asteroids orbit within the asteroid belt between the orbits of Mars and Jupiter, generally in relatively low-eccentricity (i.e. not very elongated) orbits. This belt is now estimated to contain between 1.1 and 1.9 million asteroids larger than  in diameter, and millions of smaller ones. These asteroids may be remnants of the protoplanetary disk, and in this region the accretion of planetesimals into planets during the formative period of the Solar System was prevented by large gravitational perturbations by Jupiter.

text: The majority of known asteroids orbit within the asteroid belt between the orbits of

text: Mars

text: and

text: Jupiter

text: , generally in relatively low-

text: eccentricity

text: (i.e. not very elongated) orbits. This belt is now estimated to contain between 1.1 and 1.9 million asteroids larger than  in diameter, and millions of smaller ones. These asteroids may be remnants of the

text: protoplanetary disk

text: , and in this region the

text: accretion

text: of

text: planetesimal

text: s into planets during the formative period of the Solar System was prevented by large gravitational perturbations by

text: Jupiter

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answers: remnants of the protoplanetary disk

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answers: NDQ_003830

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text: As of 2016, the United States, Japan, the European Space Agency and the People's Republic of China have conducted missions to minor planets. Most missions to date that have reached their targets have been to asteroids, however the Dawn and New Horizons spacecraft have visited the dwarf planets Ceres and Pluto respectively, and the former is currently in orbit there.

text: As of 2016, the

text: United States

text: Japan

text: , the

text: European Space Agency

text: and the

text: People's Republic of China

text: have conducted missions to

text: minor planet

text: s. Most missions to date that have reached their targets have been to

text: asteroid

text: s, however the

text: Dawn

text: and

text: New Horizons

text: spacecraft have visited the

text: dwarf planet

text: s

text: Ceres

text: and

text: Pluto

text: respectively, and the former is currently in orbit there.

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answers: minor planets

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answers: Most missions to date that have reached their targets

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answers: Dawn and New Horizons spacecraft

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answers: Most missions to date that have reached their targets

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answers: Most missions to date that have reached their targets

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answers: minor planets

text: , is an eccentric, rare-type asteroid, suspected tumbler and relatively slow rotator from the group of Apollo asteroids. It is classified as near-Earth object and potentially hazardous asteroid, and measures approximately 2.2 kilometers in diameter. The asteroid was discovered on 14 July 1999, by the U.S. Lincoln Near-Earth Asteroid Research (LINEAR) team at Lincoln Laboratory's Experimental Test Site, Socorro, New Mexico, at an apparent magnitude of 18, using a 1.0-meter reflector.

text: , is an eccentric, rare-type

text: asteroid

text: , suspected tumbler and relatively

text: slow rotator

text: from the group of

text: Apollo asteroid

text: s. It is classified as

text: near-Earth object

text: and

text: potentially hazardous asteroid

text: , and measures approximately 2.2 kilometers in diameter. The asteroid was discovered on 14 July 1999, by the U.S. Lincoln Near-Earth Asteroid Research (

text: LINEAR

text: ) team at

text: Lincoln Laboratory's Experimental Test Site

text: , Socorro, New Mexico, at an

text: apparent magnitude

text: of 18, using a 1.0-meter

text: reflector

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answers: NDQ_003821

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answers: NDQ_003822

answers: 4

answers: NDQ_003823

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answers: NDQ_003824

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answers: NDQ_003825

answers: 4

answers: NDQ_003826

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answers: NDQ_003827

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answers: 0

answers: NDQ_003829

answers: 4

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: Near-Earth object

answers: NDQ_003822

answers: Apollo asteroids

answers: NDQ_003823

answers: The asteroid was discovered on 14 July 1999

answers: NDQ_003824

answers: It is classified as near-Earth object

answers: NDQ_003825

answers: Apollo asteroids

answers: NDQ_003826

answers: Near-Earth

answers: NDQ_003827

answers: potentially hazardous

answers: NDQ_003828

answers: It is classified as near-Earth object

answers: NDQ_003829

answers: potentially hazardous asteroid

answers: NDQ_003830

answers: potentially hazardous

text: |-id=505| 121505 Andrewliounis ||  || Andrew J. Liounis (b. 1991) contributed to the NASA OSIRIS-REx Asteroid Sample Return mission as an Optical Navigation engineer. |-id=506| 121506 Chrislorentson ||  || C. Chris Lorentson (b. 1968) contributed to the NASA OSIRIS-REx Asteroid Sample Return, Lunar Reconnaissance Orbiter, Mars Science Laboratory, Hubble Space Telescope, SWIFT, GLAST and Cassini Missions as a Contamination Control Engineer for NASA-Goddard Space Flight Center. |-id=537| 121537 Lorenzdavid ||  || David Lorenz (b. 1958) is the Touch and Go Campaign lead for the Osiris-REx mission. David was responsible for returning Landsat-4 to full operations following an on-orbit failure. He has worked on the Solar Max Repair Mission, the UARS mission and various GOES spacecraft.|-id=540| 121540 Jamesmarsh ||  || Jimmy Marsh (b. 1969) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Proposal Manager. |-id=542| 121542 Alindamashiku ||  || Alinda K. Mashiku (b. 1982), an aerospace engineer at NASA’s Goddard Space Flight Center, is a member of the Flight Dynamics Team for the NASA OSIRIS-REx Asteroid Sample Return Mission, investigating nonlinear and hybrid estimation techniques for statistical orbit determination and aerocapture analysis. |-id=557| 121557 Paulmason ||  || Paul Mason (b. 1966) is the lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission. He also worked as an Attitude Control Analyst on the Solar Dynamics Observatory, LADEE, and SPIRIT Missions to name a few.|-id=593| 121593 Kevinmiller ||  || Kevin Miller (b. 1957) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as a member of the proposal team then as the first Deputy Project Manager/Resources. He has worked for NASA Goddard Space Flight Center since 1989 in project management on numerous space flight missions. |-id=594| 121594 Zubritsky ||  || Elizabeth Zubritsky (b. 1967) supports the OSIRIS-REx Asteroid Sample Return Mission at NASA's Goddard Space Flight Center by writing news releases and assisting with media relations. She serves the planetary science community by promoting fundamental research and missions like OSIRIS-REx, MAVEN and LRO.|}

text: 121505 Andrewliounis

text: ||  || Andrew J. Liounis (b. 1991) contributed to the NASA OSIRIS-REx Asteroid Sample Return mission as an Optical Navigation engineer. |-id=506|

text: 121506 Chrislorentson

text: ||  || C. Chris Lorentson (b. 1968) contributed to the NASA OSIRIS-REx Asteroid Sample Return, Lunar Reconnaissance Orbiter, Mars Science Laboratory, Hubble Space Telescope, SWIFT, GLAST and Cassini Missions as a Contamination Control Engineer for NASA-Goddard Space Flight Center. |-id=537|

text: 121537 Lorenzdavid

text: ||  || David Lorenz (b. 1958) is the Touch and Go Campaign lead for the Osiris-REx mission. David was responsible for returning Landsat-4 to full operations following an on-orbit failure. He has worked on the Solar Max Repair Mission, the UARS mission and various GOES spacecraft.|-id=540|

text: 121540 Jamesmarsh

text: ||  || Jimmy Marsh (b. 1969) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Proposal Manager. |-id=542|

text: 121542 Alindamashiku

text: ||  || Alinda K. Mashiku (b. 1982), an aerospace engineer at NASA’s Goddard Space Flight Center, is a member of the Flight Dynamics Team for the NASA OSIRIS-REx Asteroid Sample Return Mission, investigating nonlinear and hybrid estimation techniques for statistical orbit determination and aerocapture analysis. |-id=557|

text: 121557 Paulmason

text: ||  || Paul Mason (b. 1966) is the lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission. He also worked as an Attitude Control Analyst on the Solar Dynamics Observatory, LADEE, and SPIRIT Missions to name a few.|-id=593|

text: 121593 Kevinmiller

text: ||  || Kevin Miller (b. 1957) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as a member of the proposal team then as the first Deputy Project Manager/Resources. He has worked for NASA Goddard Space Flight Center since 1989 in project management on numerous space flight missions. |-id=594|

text: 121594 Zubritsky

text: ||  || Elizabeth Zubritsky (b. 1967) supports the OSIRIS-REx Asteroid Sample Return Mission at NASA's Goddard Space Flight Center by writing news releases and assisting with media relations. She serves the planetary science community by promoting fundamental research and missions like OSIRIS-REx, MAVEN and LRO.|}

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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: 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: 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: 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: 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: 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: 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: 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: 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.

answers: tqa2:L_0095/T_0928/a8d8d49e954e77249b69c93ea794380b

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

answers: tqa2:L_0095/T_0928/caaf8dfb698c0d1d1c936ff9f83f45f0

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

answers: tqa2:L_0095/T_0928/7365169cb2f6c8b1ab754607df6b5aee

answers: 4: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

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

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answers: 1: The answer is not relevant or complete, with substantial shortcomings.

answers: NDQ_003821

answers: 4

answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 3: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003824

answers: 3: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: 4

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 3: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003829

answers: 4: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003830

answers: 4: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003821

answers: b. 1966) is the lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission, investigating nonlinear and hybrid estimation techniques for statistical orbit determination and aerocapture analysis.

answers: NDQ_003822

answers: 1966) is the lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission. He also worked as an Attitude Control Analyst on the Solar Dynamics Observatory, LADEE, and SPIRIT Missions to name a few.

answers: NDQ_003823

answers: || || Asteroids are too small to have impacts with other objects so they don't have craters.

answers: NDQ_003824

answers: id=557| 121557

answers: NDQ_003825

answers: 1966) is the lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission. He also worked as an Attitude Control Analyst on the Solar Dynamics Observatory, LADEE, and SPIRIT Missions to name a few.

answers: NDQ_003826

answers: 557| 121557

answers: NDQ_003827

answers: p>Kevin Miller/p> p>Kevin Miller/p>

answers: NDQ_003828

answers: 557| 121557

answers: NDQ_003829

answers: || || Kevin Miller is an aerospace engineer at NASA's Goddard Space Flight Center, investigating nonlinear and hybrid estimation techniques for statistical orbit determination and aerocapture analysis.

answers: NDQ_003830

answers: || Kevin Miller is an aerospace engineer at NASA's Goddard Space Flight Center. He's a member of the Flight Dynamics Team for the NASA OSIRIS-REx Asteroid Sample Return Mission, investigating nonlinear and hybrid estimation techniques for statistical orbit determination and aerocapture analysis.

text: 45 Eugenia is a large  asteroid of the asteroid belt. It is famed as one of the first asteroids to be found to have a moon orbiting it. It is also the second known triple asteroid, after 87 Sylvia.

text: 45 Eugenia is a large

text: asteroid

text: of the

text: asteroid belt

text: . It is famed as one of the first asteroids to be found to have a

text: moon

text: orbiting it. It is also the second known triple asteroid, after

text: 87 Sylvia

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answers: asteroid belt

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answers: asteroid

answers: NDQ_003822

answers: 45 Eugenia

answers: NDQ_003823

answers: no

answers: NDQ_003824

answers: 87 Sylvia

answers: NDQ_003825

answers: 45 Eugenia

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: orbiting it

answers: NDQ_003828

answers: 45 Eugenia

answers: NDQ_003829

answers: 45 Eugenia

answers: NDQ_003830

answers: have a moon orbiting it

text: Asteroids with satellites, also known as binary asteroids, make up about 15% of all asteroids less than 10 km in diameter in the main belt and near-Earth population and most are thought to be formed by the YORP effect causing an asteroid to spin so fast that it breaks up. As of 2012, and where the rotation is known, all satellites of asteroids orbit the asteroid in the same direction as the asteroid is rotating.

text: Asteroids with satellites, also known as binary asteroids, make up about 15% of all asteroids less than 10 km in diameter in the

text: main belt

text: and

text: near-Earth

text: population and most are thought to be formed by the

text: YORP effect

text: causing an asteroid to spin so fast that it breaks up. As of 2012, and where the rotation is known, all

text: satellites of asteroids

text: orbit the asteroid in the same direction as the asteroid is rotating.

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answers: main belt

answers: NDQ_003827

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answers: NDQ_003821

answers: 10 km in diameter

answers: NDQ_003822

answers: Asteroids with satellites

answers: NDQ_003823

answers: Asteroids with satellites

answers: NDQ_003824

answers: Asteroids with satellites

answers: NDQ_003825

answers: Asteroids with satellites

answers: NDQ_003826

answers: main belt

answers: NDQ_003827

answers: orbit the asteroid

answers: NDQ_003828

answers: YORP effect

answers: NDQ_003829

answers: YORP effect

answers: NDQ_003830

answers: asteroids with satellites

text: However, it is becoming increasingly common for the term "asteroid" to be restricted to minor planets of the inner Solar System. Therefore, this article will restrict itself for the most part to the classical asteroids: objects of the asteroid belt, Jupiter trojans, and near-Earth objects.

text: However, it is becoming increasingly common for the term "asteroid" to be restricted to minor planets of the inner Solar System. Therefore, this article will restrict itself for the most part to the classical asteroids: objects of the

text: asteroid belt

text: Jupiter trojan

text: s, and

text: near-Earth object

text: s.

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answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

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answers: NDQ_003821

answers: minor planets

answers: NDQ_003822

answers: objects of the asteroid belt

answers: NDQ_003823

answers: Asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: This article will restrict itself for the most part to the classical asteroids

answers: NDQ_003825

answers: objects of the asteroid belt

answers: NDQ_003826

answers: solar system

answers: NDQ_003827

answers: minor planets

answers: NDQ_003828

answers: Jupiter trojans

answers: NDQ_003829

answers: It is becoming increasingly common

answers: NDQ_003830

answers: minor planets

text: 132524 APL—previously known by its provisional designation, —is an asteroid in the asteroid belt approximately 2.3 kilometers across.

text: 132524 APL—previously known by its provisional designation, —is an

text: asteroid

text: in the

text: asteroid belt

text: approximately 2.3 kilometers across.

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answers: NDQ_003821

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answers: asteroid belt

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answers: NDQ_003821

answers: approximately 2.3 kilometers across

answers: NDQ_003822

answers: 132524 APL

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 132524 APL

answers: NDQ_003825

answers: 132524 APL

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: be known by its provisional designation

answers: NDQ_003828

answers: 132524

answers: NDQ_003829

answers: 132524 APL

answers: NDQ_003830

answers: asteroid belt

text: According to the survey carried out by NASA's space-based Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the body has a high albedo of 0.34 with a corresponding diameter of 1.80 kilometers. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a slightly larger diameter of 1.88 kilometers, as the lower the body's albedo (reflectivity), the higher its diameter, at a constant absolute magnitude (brightness).

text: According to the survey carried out by NASA's space-based

text: Wide-field Infrared Survey Explorer

text: with its subsequent

text: NEOWISE

text: mission, the body has a high

text: albedo

text: of 0.34 with a corresponding diameter of 1.80 kilometers. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a slightly larger diameter of 1.88 kilometers, as the lower the body's albedo (reflectivity), the higher its diameter, at a constant absolute magnitude (brightness).

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answers: stony

answers: NDQ_003822

answers: stony

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003825

answers: stony

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: stony

answers: NDQ_003828

answers: NEOWISE mission

answers: NDQ_003829

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003830

answers: asteroids

text: Asteroids are minor planets, especially those of the inner Solar System. The larger ones have also been called planetoids. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disc of a planet and was not observed to have the characteristics of an active comet. As minor planets in the outer Solar System were discovered and found to have volatile-based surfaces that resemble those of comets, they were often distinguished from asteroids of the asteroid belt. In this article, the term "asteroid" refers to the minor planets of the inner Solar System including those co-orbital with Jupiter.

text: Asteroids are

text: minor planet

text: s, especially those of the

text: inner Solar System

text: . The larger ones have also been called planetoids. These terms have historically been applied to any astronomical object orbiting the

text: Sun

text: that did not show the disc of a planet and was not observed to have the characteristics of an active

text: comet

text: . As

text: minor planets in the outer Solar System

text: were discovered and found to have volatile-based surfaces that resemble those of comets, they were often distinguished from asteroids of the

text: asteroid belt

text: . In this article, the term "asteroid" refers to the minor planets of the inner Solar System including those co-orbital with

text: Jupiter

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answers: NDQ_003821

answers: minor planets

answers: NDQ_003822

answers: minor planets of the inner Solar System

answers: NDQ_003823

answers: The larger ones have also been called planetoids

answers: NDQ_003824

answers: Asteroids are minor planets

answers: NDQ_003825

answers: minor planets of the inner Solar System

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: orbiting the Sun

answers: NDQ_003828

answers: Asteroids

answers: NDQ_003829

answers: Asteroids are minor planets, especially those of the inner Solar System

answers: NDQ_003830

answers: minor planets

text: The rapid traverse of resonances through the asteroid belt leaves its population and the overall distribution of its orbital elements largely preserved. The asteroid belt's depletion, the mixing of its taxonomical classes, and the excitation of its orbits, yielding a distribution of inclinations peaked near 10° and eccentricities peaked near 0.1, therefore must have occurred earlier. These may be the product of Jupiter's Grand Tack, provided that a few hundred million years elapsed between it and the Nice model instability for interactions with the terrestrial planets to remove an excess of higher eccentricity asteroids. Gravitational stirring by planetary embryos embedded in the asteroid belt could also produce its depletion, mixing, and excitation. However, most if not all of the embryos must have been lost before the instability. An initially small mass asteroid belt could have its inclinations and eccentricities excited by secular resonances that hopped across the asteroid belt if Jupiter's and Saturn's orbits became chaotic while in resonance.

text: The rapid traverse of resonances through the asteroid belt leaves its population and the overall distribution of its

text: orbital elements

text: largely preserved. The asteroid belt's depletion, the mixing of its

text: taxonomical classes

text: , and the excitation of its orbits, yielding a distribution of inclinations peaked near 10° and eccentricities peaked near 0.1, therefore must have occurred earlier. These may be the product of Jupiter's

text: Grand Tack

text: , provided that a few hundred million years elapsed between it and the Nice model instability for interactions with the terrestrial planets to remove an excess of higher eccentricity asteroids. Gravitational stirring by

text: planetary embryo

text: s embedded in the asteroid belt could also produce its depletion, mixing, and excitation. However, most if not all of the embryos must have been lost before the instability. An initially small mass asteroid belt could have its inclinations and eccentricities excited by secular resonances that hopped across the asteroid belt if Jupiter's and Saturn's orbits became chaotic while in resonance.

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answers: 4

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answers: NDQ_003830

answers: 4

answers: NDQ_003821

answers: small mass

answers: NDQ_003822

answers: belt

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: rapid traverse of resonances through the asteroid belt

answers: NDQ_003825

answers: belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: interactions with the terrestrial planets

answers: NDQ_003828

answers: Jupiter's Grand Tack

answers: NDQ_003829

answers: Jupiter's and Saturn's orbits became chaotic while in resonance

answers: NDQ_003830

answers: orbital elements largely preserved

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 4.5 kilometers in diameter and its surface has an albedo of 0.29, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.2 kilometers.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 4.5 kilometers in diameter and its surface has an

text: albedo

text: of 0.29, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.2 kilometers.

answers: tqa2:L_0095/T_0925/13a3e914a11d75fa8dfbb3285de67ae0

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answers: The survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer

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answers: stony asteroids

text: In May 2011, NASA announced the OSIRIS-REx sample return mission to asteroid 1999 RQ36, and is expected to launch in 2016.

text: In May 2011, NASA announced the

text: OSIRIS-REx

text: sample return mission to asteroid

text: 1999 RQ36

text: , and is expected to launch in 2016.

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answers: asteroid

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answers: 1999 RQ36

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answers: Asteroids do not have craters

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answers: OSIRIS-REx sample return mission

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answers: asteroid belt

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answers: sample

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answers: It could cause humans to go extinct.

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answers: sample return missions

text: The Stump Arena covers much of the asteroid. From a vontage point near the arena, an observer can view the skies of the Stump Asteroid.

text: The Stump Arena covers much of the asteroid. From a vontage point near the arena, an observer can view the skies of the Stump Asteroid.

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text: Reitsema retired in 2008 from Ball Aerospace & Technologies Corp. in Boulder, Colorado. He is a consultant to NASA and the aerospace industry in mission design and Near-Earth Objects. He is the Mission Director for the B612 Foundation's Sentinel program that will find Near Earth Asteroids and identify potential Earth impact threats. He is listed in Who's Who in America. Main-belt asteroid 13327 Reitsema was named in recognition of his achievements.

text: Reitsema retired in 2008 from

text: Ball Aerospace & Technologies Corp.

text: in

text: Boulder, Colorado

text: . He is a consultant to NASA and the aerospace industry in mission design and

text: Near-Earth Objects

text: . He is the Mission Director for the

text: B612 Foundation

text: 's

text: Sentinel program

text: that will find Near Earth Asteroids and identify potential Earth impact threats. He is listed in

text: Who's Who in America

text: Main-belt

text: asteroid

text: 13327 Reitsema

text: was named in recognition of his achievements.

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answers: 13327

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text: 2201 Oljato, provisional designation , is stony and extremely eccentric asteroid, classified as near-Earth object. It measures approximately 2 kilometers in diameter and is a sizable member of the Apollo asteroids, a subgroup of near-Earth asteroids which cross the orbit of Earth. It was discovered by American astronomer Henry L. Giclas at the U.S Lowell Observatory in Flagstaff, Arizona, on 12 December 1947. After its discovery, the body became a lost asteroid for 32 years and was recovered under the provisional designation , by the American astronomers Passey and Bus at the Californian Palomar Observatory in 1979.

text: 2201 Oljato, provisional designation , is stony and extremely eccentric

text: asteroid

text: , classified as

text: near-Earth object

text: . It measures approximately 2 kilometers in diameter and is a sizable member of the

text: Apollo asteroids

text: , a subgroup of near-Earth asteroids which cross the orbit of Earth. It was discovered by American astronomer

text: Henry L. Giclas

text: at the U.S

text: Lowell Observatory

text: in Flagstaff, Arizona, on 12 December 1947. After its discovery, the body became a

text: lost asteroid

text: for 32 years and was recovered under the provisional designation , by the American astronomers Passey and Bus at the Californian Palomar Observatory in 1979.

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answers: NDQ_003821

answers: near-Earth object

answers: NDQ_003822

answers: Apollo asteroids

answers: NDQ_003823

answers: It measures approximately 2 kilometers in diameter

answers: NDQ_003824

answers: 2201 Oljato

answers: NDQ_003825

answers: Apollo asteroids

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: cross the orbit of Earth

answers: NDQ_003828

answers: 2201 Oljato

answers: NDQ_003829

answers: 2201 Oljato

answers: NDQ_003830

answers: cross the orbit of Earth

text: |-id=103| 120103 Dolero ||  || Dominique Lherault, maiden name of the discoverer's wife |-id=112| 120112 Elizabethacton ||  || Elizabeth A. Acton (b. 1981) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Project Support Specialist. |-id=120| 120120 Kankelborg ||  || Charles Kankelborg, American astrophysicist |-id=121| 120121 Libbyadelman ||  || Libby Adelman (b. 1971) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Instrument Manager for the OLA, OVIRS and REXIS instruments. |-id=141| 120141 Lucaslara ||  || Lucas Lara Garrido, Spanish astrophysicist |-id=153| 120153 Hoekenga ||  || B. Christine Hoekenga (b. 1981) worked on the OSIRIS-REx mission as the social media lead in the Principal Investigator's office.|-id=174| 120174 Jeffjenny ||  || Jeffrey and Jennifer, son and daughter of the discoverer |-id=186| 120186 Suealeman ||  || Sue Aleman (b. 1957) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Chief Safety and Mission Assurance Officer. |-id=188| 120188 Amyaqueche ||  || Amy A. Aqueche (b. 1975) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as the Contracting Officer (CO). Prior to OSIRIS-REx, she served as the NASA CO for MAVEN and the USACE CO in support of Ft. Stewart and Hunter Army Air Field Operations in Savannah, Georgia. |-id=191| 120191 Tombagg ||  || Thomas C. Bagg III (b. 1952) is the Risk Manager for the OSIRIS-REx Asteroid Sample Return Mission. Prior to this role, he supported the GSFC SBIR program, the HST SM4, NOAA-N and NOAA-N Prime missions. He helped develop the GSFC Systems Engineering Education Development Program.|-id=196| 120196 Kevinballou ||  || Kevin M. Ballou (b. 1969), an engineer at the NASA Goddard Space Flight Center, contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as C&DH Electrical Systems Engineer. |}

text: 120103 Dolero

text: ||  || Dominique Lherault, maiden name of the discoverer's wife |-id=112|

text: 120112 Elizabethacton

text: ||  || Elizabeth A. Acton (b. 1981) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Project Support Specialist. |-id=120|

text: 120120 Kankelborg

text: Charles Kankelborg

text: , American astrophysicist |-id=121|

text: 120121 Libbyadelman

text: ||  || Libby Adelman (b. 1971) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Instrument Manager for the OLA, OVIRS and REXIS instruments. |-id=141|

text: 120141 Lucaslara

text: Lucas Lara Garrido

text: , Spanish astrophysicist |-id=153|

text: 120153 Hoekenga

text: ||  || B. Christine Hoekenga (b. 1981) worked on the OSIRIS-REx mission as the social media lead in the Principal Investigator's office.|-id=174|

text: 120174 Jeffjenny

text: ||  || Jeffrey and Jennifer, son and daughter of the discoverer |-id=186|

text: 120186 Suealeman

text: ||  || Sue Aleman (b. 1957) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Chief Safety and Mission Assurance Officer. |-id=188|

text: 120188 Amyaqueche

text: ||  || Amy A. Aqueche (b. 1975) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as the Contracting Officer (CO). Prior to OSIRIS-REx, she served as the NASA CO for MAVEN and the USACE CO in support of Ft. Stewart and Hunter Army Air Field Operations in Savannah, Georgia. |-id=191|

text: 120191 Tombagg

text: ||  || Thomas C. Bagg III (b. 1952) is the Risk Manager for the OSIRIS-REx Asteroid Sample Return Mission. Prior to this role, he supported the GSFC SBIR program, the HST SM4, NOAA-N and NOAA-N Prime missions. He helped develop the GSFC Systems Engineering Education Development Program.|-id=196|

text: 120196 Kevinballou

text: ||  || Kevin M. Ballou (b. 1969), an engineer at the NASA Goddard Space Flight Center, contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as C&DH Electrical Systems Engineer. |}

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answers: NDQ_003821

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answers: NDQ_003822

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answers: NDQ_003824

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answers: NDQ_003827

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answers: NDQ_003828

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answers: NDQ_003830

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answers: NDQ_003821

answers: he served as the NASA CO for MAVEN and the USACE CO in support of Ft.

answers: NDQ_003822

answers: |-id=191| 120191 Tombagg

answers: NDQ_003823

answers: REx mission.

answers: NDQ_003824

answers: NASA's OSIRIS-REx mission

answers: NDQ_003825

answers: |-id=191| 120191 Tombagg

answers: NDQ_003826

answers: NASA OSIRIS-REx

answers: NDQ_003827

answers: Prior to OSIRIS-REx, he served as the USACE CO in support of Ft. Stewart and Hunter Army Air Field Operations in Savannah, Georgia.

answers: NDQ_003828

answers: NASA OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003829

answers: NDQ_003830

answers: Prior to OSIRIS-REx, he served as the NASA CO for MAVEN and the USACE CO in support of Ft.

text: Many databases, for instance the JPL Small-Body Database (JPL SBDB), only list asteroids with a perihelion greater than 1.3 AU as Mars-crossers. An asteroid with a perihelion less than this is classed as a near-Earth object even though it is crossing the orbit of Mars as well as crossing (or coming near to) that of Earth. Nevertheless, these objects are listed on this page. A grazer is an object with a perihelion below the aphelion of Mars (1.67 AU) but above the Martian perihelion (1.38 AU). The JPL SBDB lists 13,500 Mars-crossing asteroids (MCAs). Only 18 MCAs are brighter than absolute magnitude (H) 12.5, which typically makes these asteroids with H<12.5 more than 13 km in diameter depending on the albedo. The smallest known MCAs have an absolute magnitude (H) of around 24 and are typically less than 100 meters in diameter.

text: Many databases, for instance the

text: JPL Small-Body Database

text: (JPL SBDB), only list asteroids with a

text: perihelion

text: greater than 1.3

text: AU

text: as Mars-crossers. An asteroid with a perihelion less than this is classed as a

text: near-Earth object

text: even though it is crossing the orbit of Mars as well as crossing (or coming near to) that of Earth. Nevertheless, these objects are listed on this page. A grazer is an object with a perihelion below the aphelion of Mars (1.67 AU) but above the Martian perihelion (1.38 AU). The JPL SBDB lists 13,500 Mars-crossing asteroids (MCAs). Only 18 MCAs are brighter than

text: absolute magnitude (H)

text: 12.5, which typically makes these asteroids with H<12.5 more than 13 km in diameter depending on the

text: albedo

text: . The smallest known MCAs have an absolute magnitude (H) of around 24 and are typically less than 100 meters in diameter.

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answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: JPL Small-Body Database (JPL SBDB)

answers: NDQ_003825

answers: Mars-crossing asteroids

answers: NDQ_003826

answers: perihelion

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answers: crossing (or coming near to) that of Earth

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answers: The smallest known MCAs have an absolute magnitude (H) of around 24

answers: NDQ_003829

answers: Mars-crossing asteroids (MCAs)

answers: NDQ_003830

answers: Mars-crossing asteroids

text: When the mode starts, only the Start Mission target is lit. Picard sees asteroids and asks for suggestions. Mr. Data suggests that "we can destroy the asteroids in our path." A counter shows a value of 20,000,000 starts to count down. When the player hits the initial target, an asteroid blows up, and it sets the value for all the other shots. (If the count down reaches 5 million, the asteroid self-destructs, and all other asteroid hits are set at 5 million.) Then the other targets light up as asteroids to hit. Completing 4 asteroid hits (including the opening "point set" asteroid) awards one Artifact; getting all the asteroids awards a second Artifact.

text: When the mode starts, only the Start Mission target is lit. Picard sees asteroids and asks for suggestions. Mr. Data suggests that "we can destroy the asteroids in our path." A counter shows a value of 20,000,000 starts to count down. When the player hits the initial target, an asteroid blows up, and it sets the value for all the other shots. (If the count down reaches 5 million, the asteroid self-destructs, and all other asteroid hits are set at 5 million.) Then the other targets light up as asteroids to hit. Completing 4 asteroid hits (including the opening "point set" asteroid) awards one Artifact; getting all the asteroids awards a second Artifact.

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text: In an interview with Derek during the June 1, 2006 episode of Slacker Astronomy, the naming of Asteroids 106545 Colanduno and 106537 McCarthy was announced to the world. The asteroids were named in homage to the hosts of Skepticality by their discoverer the late  Jeff Medkeff, who said, "My naming of these asteroids for you is a token of my esteem for you and your accomplishments."

text: In an interview with Derek during the June 1, 2006 episode of

text: Slacker Astronomy

text: , the naming of Asteroids

text: 106545 Colanduno

text: and

text: 106537 McCarthy

text: was announced to the world. The asteroids were named in homage to the hosts of Skepticality by their discoverer the late

text: Jeff Medkeff

text: , who said, "My naming of these asteroids for you is a token of my esteem for you and your accomplishments."

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answers: discoverer

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answers: accomplishments

text: (also written (53319) 1999 JM8) is a Potentially hazardous asteroid, near-Earth asteroid and Mars-crosser asteroid discovered by LINEAR. Radar imaging by Goldstone and Arecibo has revealed the asteroid to have an effective diameter of 6.4 km. Like the asteroid 4179 Toutatis, its rotation speed is unusually slow and possibly chaotic. It is the largest Potentially hazardous object known.

text: (also written (53319) 1999 JM8) is a

text: Potentially hazardous asteroid

text: near-Earth

text: asteroid

text: and

text: Mars-crosser asteroid

text: discovered by

text: LINEAR

text: Radar imaging

text: by

text: Goldstone

text: and

text: Arecibo

text: has revealed the asteroid to have an effective diameter of 6.4 km. Like the asteroid

text: 4179 Toutatis

text: , its rotation speed is unusually slow and possibly chaotic. It is the largest Potentially hazardous object known.

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answers: Hazardous

answers: NDQ_003822

answers: 53319) 1999 JM8 is a Potentially hazardous asteroid

answers: NDQ_003823

answers: (also written) 53319

answers: NDQ_003824

answers: It is the largest Potentially hazardous object known

answers: NDQ_003825

answers: 53319) 1999 JM8 is a Potentially hazardous asteroid

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: Mars-crosser asteroid

answers: NDQ_003828

answers: Mars-crosser asteroid

answers: NDQ_003829

answers: It is the largest Potentially hazardous object known

answers: NDQ_003830

answers: Hazardous

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 4.1 kilometers in diameter and its surface has an albedo of 0.24, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 4.3 kilometers.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 4.1 kilometers in diameter and its surface has an

text: albedo

text: of 0.24, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 4.3 kilometers.

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answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: diameter

answers: NDQ_003822

answers: stony

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: NEOWISE mission

answers: NDQ_003825

answers: stony

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: stony

answers: NDQ_003828

answers: 4.3 kilometers

answers: NDQ_003829

answers: It could cause humans to go extinct

answers: NDQ_003830

answers: stony asteroids

text: more than 1,600 new near-Earth asteroids have been discovered by various search teams and catalogued as potentially hazardous objects.  NASA has yet to select a target for ARM, but for planning purposes it is currently using a near Earth asteroid named (341843) 2008 EV5 of about  in diameter to pick up  a single  boulder from it. Other candidate parent asteroids are Itokawa, Bennu, and Ryugu. The decision on the target asteroid will be announced in 2019, allowing additional time to find alternative targets.<ref name='steps 2015'/>

text: more than 1,600 new

text: near-Earth asteroids

text: have been discovered by various search teams and catalogued as

text: potentially hazardous object

text: s.  NASA has yet to select a target for ARM, but for planning purposes it is currently using a near Earth asteroid named

text: (341843) 2008 EV5

text: of about  in diameter to pick up  a single  boulder from it. Other candidate parent asteroids are

text: Itokawa

text: Bennu

text: , and

text: Ryugu

text: . The decision on the target asteroid will be announced in 2019, allowing additional time to find alternative targets.<ref name='steps 2015'/>

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answers: potentially hazardous objects

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answers: 1,600 new near-Earth

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answers: (341843) 2008 EV5

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answers: NASA has yet to select a target for ARM

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text: It is classified as an Apollo asteroid because it is a near-Earth asteroid with a semi-major axis larger than Earth's.

text: It is classified as an

text: Apollo asteroid

text: because it is a

text: near-Earth asteroid

text: with a semi-major axis larger than Earth's.

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answers: near-Earth

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answers: near-Earth

answers: NDQ_003823

answers: asteroids

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answers: It is classified as an Apollo asteroid

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: Near Earth

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answers: larger than Earth's

answers: NDQ_003828

answers: An Apollo asteroid

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct.

answers: NDQ_003830

answers: Earth's

text: A rotational light-curve was obtained from photometric observations made at the U.S. Palomar Transient Factory in May 2010. It gave a rotation period of  hours with a brightness amplitude of 0.31 in magnitude (U=2). According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 4.6 kilometers in diameter and its surface has an albedo of 0.21, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 4.4 kilometers.

text: A rotational

text: light-curve

text: was obtained from

text: photometric

text: observations made at the U.S.

text: Palomar Transient Factory

text: in May 2010. It gave a

text: rotation period

text: of  hours with a brightness amplitude of 0.31 in

text: magnitude

text: ). According to the survey carried out by the

text: NEOWISE

text: mission of NASA's space-based

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 4.6 kilometers in diameter and its surface has an

text: albedo

text: of 0.21, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 4.4 kilometers.

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text: None of the asteroids in the outer part of the asteroid belt can ever attain this brightness. Even Hygiea and Interamnia rarely reach magnitudes of above 10.0. This is due to the different distribution of spectral types within different sections of the asteroid belt being such that the highest-albedo asteroids are all concentrated closer to Mars, and much lower albedo C and D types being common in the outer belt.

text: None of the asteroids in the outer part of the asteroid belt can ever attain this brightness. Even Hygiea and Interamnia rarely reach magnitudes of above 10.0. This is due to the different distribution of spectral types within different sections of the asteroid belt being such that the highest-albedo asteroids are all concentrated closer to

text: Mars

text: , and much lower albedo

text: C

text: and

text: D

text: types being common in the outer belt.

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answers: asteroids

text: 243 Ida () is an asteroid in the Koronis family of the asteroid belt. It was discovered on 29 September 1884 by Austrian astronomer Johann Palisa and named after a nymph from Greek mythology. Later telescopic observations categorized Ida as an S-type asteroid, the most numerous type in the inner asteroid belt. On 28 August 1993, Ida was visited by the unmanned Galileo spacecraft, while en route to Jupiter. It was the second asteroid visited by a spacecraft and the first found to have a natural satellite.

text: 243 Ida () is an

text: asteroid

text: in the

text: Koronis family

text: of the

text: asteroid belt

text: . It was discovered on 29 September 1884 by

text: Austria

text: n astronomer

text: Johann Palisa

text: and named after a

text: nymph

text: from Greek mythology. Later telescopic observations categorized Ida as an

text: S-type asteroid

text: , the most numerous type in the inner asteroid belt. On 28 August 1993, Ida was visited by the unmanned

text: Galileo

text: spacecraft, while en route to

text: Jupiter

text: . It was the second asteroid visited by a spacecraft and the first found to have a

text: natural satellite

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answers: unmanned Galileo spacecraft

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answers: 243 Ida

answers: NDQ_003830

answers: have a natural satellite

text: The trains took them through a tunnel into the Columbiad Cannon. As the blast-off occurred, trains were suddenly propelled out of the Columbiad to the top of the dome. The space travel started with riders crossing asteroid fields until they got swallowed by Colonel Impey Barbicane's Bluemoon Mining Machine, an industrial space machine built by the President of the Gun Club to extract mineral resources from asteroids. Escaping the danger of this device, trains headed to a huge asteroid which they crossed through a small fissure. This journey came afterwards to the climax of the ride, the Moon itself (with a smiling face, as seen in Georges Méliès' 1902 movie adaptation of the novel). On the right, one could notice that Jules Verne himself, with the proper equipment, had landed on a nearby asteroid. Then trains headed back to Earth, crossing other asteroid fields. When riders reached the atmosphere, bolts and light rays were visible around the train as it heated up. Trains finally entered the Electro-de-Velocitor, a machine that stopped them suddenly so that their speed would be reduced when they headed back to the station.

text: The trains took them through a tunnel into the Columbiad Cannon. As the blast-off occurred, trains were suddenly propelled out of the Columbiad to the top of the dome. The space travel started with riders crossing asteroid fields until they got swallowed by Colonel Impey Barbicane's Bluemoon Mining Machine, an industrial space machine built by the President of the Gun Club to extract mineral resources from asteroids. Escaping the danger of this device, trains headed to a huge asteroid which they crossed through a small fissure. This journey came afterwards to the climax of the ride, the Moon itself (with a smiling face, as seen in

text: Georges Méliès

text: ' 1902

text: movie adaptation

text: of the novel). On the right, one could notice that Jules Verne himself, with the proper equipment, had landed on a nearby asteroid. Then trains headed back to Earth, crossing other asteroid fields. When riders reached the atmosphere, bolts and light rays were visible around the train as it heated up. Trains finally entered the Electro-de-Velocitor, a machine that stopped them suddenly so that their speed would be reduced when they headed back to the station.

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answers: Then trains headed back to Earth, crossing other asteroid fields

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answers: extract mineral resources

text: 196 Philomela is a large and bright main-belt asteroid. It is an S-type asteroid.

text: 196 Philomela is a large and bright

text: main-belt

text: asteroid

text: . It is an

text: S-type asteroid

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answers: It is an S-type asteroid

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answers: 196 Philomela

answers: NDQ_003829

answers: S-type asteroid

answers: NDQ_003830

answers: 196 Philomela

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 3.5 kilometers in diameter and its surface has a very high albedo of 0.39. The Collaborative Asteroid Lightcurve Link (CALL) disagrees with the findings by the space-based mission and assumes a standard albedo for carbonaceous asteroids of 0.057, with a correspondingly larger diameter of 8.0 kilometers. As with 1696 Nurmela, another member of the Baptistina family, CALL assumes this asteroid's composition (also see carbonaceous chondrites) to differ significantly from the much brighter asteroid 298 Baptistina, which is considered to be an interloper in its own family.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 3.5 kilometers in diameter and its surface has a very high

text: albedo

text: of 0.39. The Collaborative Asteroid Lightcurve Link (CALL) disagrees with the findings by the space-based mission and assumes a standard albedo for carbonaceous asteroids of 0.057, with a correspondingly larger diameter of 8.0 kilometers. As with

text: 1696 Nurmela

text: , another member of the Baptistina family, CALL assumes this asteroid's composition (also see

text: carbonaceous chondrites

text: ) to differ significantly from the much brighter asteroid

text: 298 Baptistina

text: , which is considered to be an interloper in its own family.

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answers: carbonaceous

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answers: carbonaceous

answers: NDQ_003823

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003824

answers: The Collaborative Asteroid Lightcurve Link

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answers: carbonaceous

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answers: asteroid belt

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answers: interloper

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answers: 1696 Nurmela

answers: NDQ_003829

answers: It is considered to be an interloper in its own family

answers: NDQ_003830

answers: carbonaceous asteroids

text: The albedos of planets, satellites and asteroids can be used to infer much about their properties. The study of albedos, their dependence on wavelength, lighting angle ("phase angle"), and variation in time comprises a major part of the astronomical field of photometry. For small and far objects that cannot be resolved by telescopes, much of what we know comes from the study of their albedos. For example, the absolute albedo can indicate the surface ice content of outer Solar System objects, the variation of albedo with phase angle gives information about regolith properties, whereas unusually high radar albedo is indicative of high metal content in asteroids.

text: The albedos of

text: planet

text: s,

text: satellites

text: and

text: asteroid

text: s can be used to infer much about their properties. The study of albedos, their dependence on wavelength, lighting angle ("phase angle"), and variation in time comprises a major part of the astronomical field of

text: photometry

text: . For small and far objects that cannot be resolved by telescopes, much of what we know comes from the study of their albedos. For example, the absolute albedo can indicate the surface ice content of outer

text: Solar System

text: objects, the variation of albedo with phase angle gives information about

text: regolith

text: properties, whereas unusually high radar albedo is indicative of high metal content in

text: asteroid

text: s.

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answers: NDQ_003821

answers: small and far objects

answers: NDQ_003822

answers: high metal content

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: For small and far objects that cannot be resolved by telescopes

answers: NDQ_003825

answers: high metal content

answers: NDQ_003826

answers: Solar System

answers: NDQ_003827

answers: high metal content

answers: NDQ_003828

answers: The albedos of planets, satellites and asteroids can be used to infer much about their properties

answers: NDQ_003829

answers: It could cause humans to go extinct

answers: NDQ_003830

answers: albedos

text: The other Eunomian asteroids are quite regularly distributed in orbital space around Eunomia. The next largest member identified by the  analysis was 258 Tyche of 65 km diameter. However, its orbit lies at the very margin of what can be considered the family region, and it may well be an interloper. The largest clear family members are about 30 km diameter, with several asteroids in this size range.

text: The other Eunomian asteroids are quite regularly distributed in orbital space around Eunomia. The next largest member identified by the  analysis was

text: 258 Tyche

text: of 65 km diameter. However, its orbit lies at the very margin of what can be considered the family region, and it may well be an interloper. The largest clear family members are about 30 km diameter, with several asteroids in this size range.

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answers: NDQ_003821

answers: diameter

answers: NDQ_003822

answers: Eunomian

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroids

answers: NDQ_003825

answers: Eunomian

answers: NDQ_003826

answers: the family region

answers: NDQ_003827

answers: interloper

answers: NDQ_003828

answers: It may well be an interloper

answers: NDQ_003829

answers: It may well be an interloper

answers: NDQ_003830

answers: asteroids

text: M-type asteroids are asteroids of partially known composition; they are moderately bright (albedo 0.1–0.2). Some, but not all, are made of nickel–iron, either pure or mixed with small amounts of stone. These are thought to be pieces of the metallic core of differentiated asteroids that were fragmented by impacts, and are thought to be the source of iron meteorites. M-type asteroids are the third most common asteroid type.

text: M-type asteroids are

text: asteroid

text: s of partially known composition; they are moderately bright (

text: albedo

text: 0.1–0.2). Some, but not all, are made of

text: nickel

text: iron

text: , either pure or mixed with small amounts of stone. These are thought to be pieces of the metallic core of differentiated asteroids that were fragmented by impacts, and are thought to be the source of

text: iron meteorite

text: s. M-type asteroids are the third most common asteroid type.

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answers: NDQ_003821

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answers: NDQ_003822

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answers: NDQ_003823

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answers: NDQ_003824

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answers: NDQ_003825

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answers: NDQ_003826

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answers: NDQ_003828

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answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: partially known composition

answers: NDQ_003822

answers: M-type asteroids

answers: NDQ_003823

answers: M-type asteroids

answers: NDQ_003824

answers: Some, but not all

answers: NDQ_003825

answers: M-type asteroids

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: fragmented by impacts

answers: NDQ_003828

answers: M-type asteroids

answers: NDQ_003829

answers: M-type asteroids

answers: NDQ_003830

answers: iron meteorites

text: Engineers of the Asteroid Redirect Mission are contemplating in its early conceptual phase the use of laser communications.

text: Engineers of the

text: Asteroid Redirect Mission

text: are contemplating in its early conceptual phase the use of laser communications.

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answers: NDQ_003821

answers: 0

answers: NDQ_003822

answers: 0

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 2

answers: NDQ_003825

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answers: NDQ_003826

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answers: NDQ_003828

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answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: orbiting a planet

answers: NDQ_003822

answers: Redirect Mission

answers: NDQ_003823

answers: Asteroid Redirect Mission

answers: NDQ_003824

answers: Asteroid Redirect Mission

answers: NDQ_003825

answers: Redirect Mission

answers: NDQ_003826

answers: Asteroid Redirect

answers: NDQ_003827

answers: laser communications

answers: NDQ_003828

answers: Asteroid Redirect Mission

answers: NDQ_003829

answers: Asteroid Redirect Mission

answers: NDQ_003830

answers: use of laser communications

text: Several asteroids have collided with earth in recent geological history. The Chicxulub asteroid, for example, is theorized to have caused the extinction of the non-avian dinosaurs 66 million years ago at the end of the Cretaceous. If such an object struck Earth it could have a serious impact on civilization. It is even possible that humanity would be completely destroyed. For this to occur, the asteroid would need to be at least  in diameter, but probably between 3 and 10 km (2–6 miles). Asteroids with a 1 km diameter have impacted the Earth on average once every 500,000 years. Larger asteroids are less common. Small near-Earth asteroids are regularly observed.

text: Several asteroids have collided with earth in recent geological history. The

text: Chicxulub asteroid

text: , for example, is theorized to have caused the extinction of the non-avian dinosaurs 66 million years ago at the

text: end of the Cretaceous

text: . If such an object struck Earth it could have a serious impact on civilization. It is even possible that humanity would be completely destroyed. For this to occur, the asteroid would need to be at least  in diameter, but probably between 3 and 10 km (2–6 miles). Asteroids with a 1 km diameter have impacted the Earth on average once every 500,000 years. Larger asteroids are less common. Small

text: near-Earth asteroid

text: s are regularly observed.

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answers: an object

answers: NDQ_003822

answers: collided with earth

answers: NDQ_003823

answers: Small near-Earth asteroids

answers: NDQ_003824

answers: Small near-Earth asteroids are regularly observed

answers: NDQ_003825

answers: collided with earth

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: collided with earth

answers: NDQ_003828

answers: It is even possible that humanity would be completely destroyed

answers: NDQ_003829

answers: It is even possible that humanity would be completely destroyed

answers: NDQ_003830

answers: collided with earth

text: The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,226 days). Its orbit is tilted by 5 degrees to the plane of the ecliptic and shows a notable eccentricity of 0.20. The body rotates around its axis once every 10.4 hours and has an albedo of 0.18 and 0.36, according to two different observations made by the Wide-field Infrared Survey Explorer. The Collaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24, a figure more in line with those typically found for Flora asteroids.

text: The

text: S-type

text: asteroid is a member of the

text: Flora family

text: , one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.8–2.7

text: AU

text: once every 3 years and 4 months (1,226 days). Its orbit is

text: tilted

text: by 5 degrees to the plane of the

text: ecliptic

text: and shows a notable

text: eccentricity

text: of 0.20. The body

text: rotates

text: around its axis once every 10.4 hours and has an

text: albedo

text: of 0.18 and 0.36, according to two different observations made by the

text: Wide-field Infrared Survey Explorer

text: . The Collaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24, a figure more in line with those typically found for Flora asteroids.

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answers: NDQ_003826

answers: main-belt

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answers: stony

answers: NDQ_003822

answers: Flora family

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: The body rotates around its axis once every 10.4 hours

answers: NDQ_003825

answers: Flora family

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: orbits the Sun

answers: NDQ_003828

answers: The S-type asteroid

answers: NDQ_003829

answers: The S-type asteroid

answers: NDQ_003830

answers: orbits the Sun

text: Geographos was to be explored by the U.S.'s Clementine mission; however, a malfunctioning thruster ended the mission before it could approach the asteroid.

text: Geographos was to be explored by the U.S.'s

text: Clementine mission

text: ; however, a malfunctioning thruster ended the mission before it could approach the asteroid.

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text: The Karin family or Karin cluster is an asteroid family and sub-group of the Koronis family. It consists of at least 90 main-belt asteroids. What makes them special is that scientists have used the orbits of 13 members to calculate backwards until they were all found to share the same orbit — that of the parent body from which they all originated.

text: The Karin family or Karin cluster is an

text: asteroid family

text: and sub-group of the

text: Koronis family

text: . It consists of at least 90

text: main-belt

text: asteroid

text: s. What makes them special is that scientists have used the orbits of 13 members to calculate backwards until they were all found to share the same orbit — that of the parent body from which they all originated.

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answers: Karin family

answers: NDQ_003829

answers: The Karin family or Karin cluster

answers: NDQ_003830

answers: share the same orbit

text: Based on an absolute magnitude of 21.4, the asteroid has an estimated diameter of about .  is noted for a close approach to Earth on 27 December 1976 at a distance of about . As of November 2011 with an observation arc of 40 days, the JPL Small-Body Database showed that the uncertainty region of the asteroid during the 1976 close approach could result in a pass anywhere from 0.001 AU to 0.018 AU from Earth. During the 1976 close approach the asteroid reached about apparent magnitude 14.

text: Based on an

text: absolute magnitude

text: of 21.4, the asteroid has an estimated diameter of about .  is noted for a close approach to Earth on 27 December 1976 at a distance of about . As of November 2011 with an observation arc of 40 days, the

text: JPL Small-Body Database

text: showed that the uncertainty region of the asteroid during the 1976 close approach could result in a pass anywhere from 0.001 AU to 0.018 AU from Earth. During the 1976 close approach the asteroid reached about

text: apparent magnitude

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answers: Small-Body

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answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: The asteroid has an estimated diameter of about.

answers: NDQ_003825

answers: Small-Body

answers: NDQ_003826

answers: AU

answers: NDQ_003827

answers: 0.001 AU to 0.018 AU

answers: NDQ_003828

answers: The asteroid reached about apparent magnitude 14.

answers: NDQ_003829

answers: As of November 2011 with an observation arc of 40 days

answers: NDQ_003830

answers: close approach to Earth

text: An Earth-crosser is a near-Earth asteroid whose orbit crosses that of Earth as observed from the ecliptic pole of Earth's orbit. The known numbered Earth-crossers are listed here. Those Earth-crossers whose semi-major axes are smaller than Earth's are Aten asteroids; the remaining ones are Apollo asteroids. (See also the Amor asteroids.)

text: An Earth-crosser is a

text: near-Earth asteroid

text: whose

text: orbit

text: crosses that of

text: Earth

text: as observed from the

text: ecliptic pole

text: of Earth's orbit. The known numbered Earth-crossers are listed here. Those Earth-crossers whose

text: semi-major axes

text: are smaller than Earth's are

text: Aten asteroid

text: s; the remaining ones are

text: Apollo asteroid

text: s. (See also the

text: Amor asteroid

text: s.)

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answers: ecliptic

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answers: near-Earth

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answers: Earth-crossers

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answers: Earth-crosser

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answers: Earth-crossers

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answers: Earth-crossers

text: According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 8.2 kilometers in diameter and its surface has an albedo of 0.29, while the Collaborative Asteroid Lightcurve Link (CALL) assumes a standard albedo for stony asteroids of 0.21, and calculates a diameter of 9.2 kilometers.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's space-based

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 8.2 kilometers in diameter and its surface has an

text: albedo

text: of 0.29, while the Collaborative Asteroid Lightcurve Link (CALL) assumes a standard albedo for stony asteroids of 0.21, and calculates a diameter of 9.2 kilometers.

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answers: NDQ_003821

answers: diameter

answers: NDQ_003822

answers: stony

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: stony

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: stony

answers: NDQ_003828

answers: asteroid

answers: NDQ_003829

answers: It could cause humans to go extinct

answers: NDQ_003830

answers: stony asteroids

text: It is the namesake and the first numbered body of the Atira asteroids, a new subclass of near-Earth asteroids, which have their orbits entirely within that of Earth and are therefore alternatively called Interior-Earth Objects (IEO). As of 2015, there are only 16 known members of the Atira group of asteroids. Atiras are similar to the larger group of Aten asteroids, as both are near-Earth objects and both have a semi-major axis smaller than that of Earth (< 1.0 AU). However, and contrary to Aten asteroids, the aphelion for Atiras is always smaller than Earth's perihelion (

text: It is the namesake and the first numbered body of the

text: Atira asteroids

text: , a new subclass of near-Earth asteroids, which have their orbits entirely within that of Earth and are therefore alternatively called Interior-Earth Objects (IEO). As of 2015, there are only 16 known members of the Atira group of asteroids. Atiras are similar to the larger group of

text: Aten asteroid

text: s, as both are near-Earth objects and both have a

text: semi-major axis

text: smaller than that of Earth (< 1.0

text: AU

text: ). However, and contrary to Aten asteroids, the

text: aphelion

text: for Atiras is always smaller than Earth's

text: perihelion

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text: Due to its high eccentricity and semi-major axis of 0.57 and 2.5 AU, respectively, it is a typical Amor III asteroid. It has both, a 1:3 orbital resonance with Jupiter and a close to 4:1 resonance with Earth. In addition, because its orbit also lies within the asteroid belt, it is often classified as a main-belt asteroid.

text: Due to its high eccentricity and semi-major axis of 0.57 and 2.5 AU, respectively, it is a typical

text: Amor III asteroid

text: . It has both, a 1:3

text: orbital resonance

text: with

text: Jupiter

text: and a close to 4:1 resonance with Earth. In addition, because its orbit also lies within the asteroid belt, it is often classified as a

text: main-belt

text: asteroid.

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answers: Its orbit also lies within the asteroid belt

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answers: Because its orbit also lies within the asteroid belt

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text: When found, asteroids were seen as a class of objects distinct from comets, and there was no unified term for the two until "small Solar System body" was coined in 2006. The main difference between an asteroid and a comet is that a comet shows a coma due to sublimation of near surface ices by solar radiation. A few objects have ended up being dual-listed because they were first classified as minor planets but later showed evidence of cometary activity. Conversely, some (perhaps all) comets are eventually depleted of their surface volatile ices and become asteroid-like. A further distinction is that comets typically have more eccentric orbits than most asteroids; most "asteroids" with notably eccentric orbits are probably dormant or extinct comets.

text: When found, asteroids were seen as a class of objects distinct from comets, and there was no unified term for the two until "small Solar System body" was coined in 2006. The main difference between an asteroid and a comet is that a comet shows a coma due to

text: sublimation

text: of near surface ices by solar radiation. A few objects have ended up being dual-listed because they were first classified as minor planets but later showed evidence of cometary activity. Conversely, some (perhaps all) comets are eventually depleted of their surface

text: volatile ices

text: and become asteroid-like. A further distinction is that comets typically have more eccentric orbits than most asteroids; most "asteroids" with notably eccentric orbits are probably dormant or extinct comets.

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answers: 4

answers: NDQ_003826

answers: 0

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: small Solar System body

answers: NDQ_003822

answers: small Solar System body

answers: NDQ_003823

answers: Small Solar System body

answers: NDQ_003824

answers: Small Solar System body

answers: NDQ_003825

answers: small Solar System body

answers: NDQ_003826

answers: Solar System

answers: NDQ_003827

answers: show evidence of cometary activity

answers: NDQ_003828

answers: a comet

answers: NDQ_003829

answers: It's impossible to say

answers: NDQ_003830

answers: cometary activity

text: The Belt Community: Being as the asteroid belt is ungovernably large, the Belt community consists of widely spread independent and corporate mining operations, with Ceres at its core as the primary trading post. Although conventional law enforcement throughout the belt is impossible, Ceres itself is governed under the just (if not heavy-handed) watch of the Autocrat. Once plagued by rock wars (vicious skirmishes which typically arose due to disputes over mining rights), the death penalty has been frequently employed to keep the population in check. Although the secrets of the Autocrat are closely guarded, the Belt Community has developed a device called the Core cracker, and quite seriously offered to blow up the planet Mercury both to create a second asteroid belt and assist VISOR in the terraforming of Venus.

text: The Belt Community: Being as the

text: asteroid belt

text: is ungovernably large, the Belt community consists of widely spread independent and corporate mining operations, with

text: Ceres

text: at its core as the primary trading post. Although conventional law enforcement throughout the belt is impossible, Ceres itself is governed under the just (if not heavy-handed) watch of the

text: Autocrat

text: . Once plagued by rock wars (vicious skirmishes which typically arose due to disputes over mining rights), the

text: death penalty

text: has been frequently employed to keep the population in check. Although the secrets of the Autocrat are closely guarded, the Belt Community has developed a device called the

text: Core cracker

text: , and quite seriously offered to blow up the planet

text: Mercury

text: both to create a second asteroid belt and assist VISOR in the

text: terraforming of Venus

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answers: NDQ_003821

answers: belt

answers: NDQ_003822

answers: belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroid belt

answers: NDQ_003825

answers: belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: blow up the planet Mercury

answers: NDQ_003828

answers: Earth

answers: NDQ_003829

answers: the death penalty

answers: NDQ_003830

answers: terraforming

text: Contrary to popular imagery, the asteroid belt is mostly empty. The asteroids are spread over such a large volume that it would be improbable to reach an asteroid without aiming carefully. Nonetheless, hundreds of thousands of asteroids are currently known, and the total number ranges in the millions or more, depending on the lower size cutoff. Over 200 asteroids are known to be larger than 100 km, and a survey in the infrared wavelengths has shown that the asteroid belt has 0.7–1.7 million asteroids with a diameter of 1 km or more. The apparent magnitudes of most of the known asteroids are 11–19, with the median at about 16.

text: Contrary to popular imagery, the asteroid belt is mostly empty. The asteroids are spread over such a large volume that it would be improbable to reach an asteroid without aiming carefully. Nonetheless, hundreds of thousands of asteroids are currently known, and the total number ranges in the millions or more, depending on the lower size cutoff. Over 200 asteroids are known to be larger than 100 km, and a survey in the infrared wavelengths has shown that the asteroid belt has 0.7–1.7 million asteroids with a diameter of 1 km or more. The

text: apparent magnitude

text: s of most of the known asteroids are 11–19, with the median at about 16.

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answers: larger than 100 km

answers: NDQ_003822

answers: hundreds of thousands of asteroids

answers: NDQ_003823

answers: It would be improbable to reach an asteroid without aiming carefully

answers: NDQ_003824

answers: It would be improbable to reach an asteroid without aiming carefully

answers: NDQ_003825

answers: hundreds of thousands of asteroids

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: be larger than 100 km

answers: NDQ_003828

answers: It would be improbable to reach an asteroid without aiming carefully

answers: NDQ_003829

answers: It would be improbable to reach an asteroid without aiming carefully

answers: NDQ_003830

answers: the total number ranges in the millions or more, depending on the lower size cutoff

text: On the night this minor planet was discovered at Brorfelde Observatory, Poul Jensen also discovered the Jupiter trojan , the 12-kilometer size main-belt asteroid , as well as , , , and , all main-belt asteroids of inner, middle and outer region of the asteroid belt, respectively.

text: On the night this minor planet was discovered at Brorfelde Observatory, Poul Jensen also discovered the Jupiter trojan , the 12-kilometer size main-belt asteroid , as well as , , , and , all main-belt asteroids of inner, middle and outer region of the

text: asteroid belt

text: , respectively.

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answers: NDQ_003821

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answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 0

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: minor planet

answers: NDQ_003822

answers: main-belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 12-kilometer size

answers: NDQ_003825

answers: main-belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: 12-kilometer size

answers: NDQ_003828

answers: Jupiter trojan

answers: NDQ_003829

answers: Jupiter trojan

answers: NDQ_003830

answers: minor planet

text: |-| 26301 Hellawillis ||  || 26301 Hellawillis Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Hella Willis mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Sheboygan North High School, Sheboygan, Wisconsin.|-id=302| 26302 Zimolzak ||  || 26302 Zimolzak Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Matt Zimolzak mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the William Fremd High School, Palatine, Illinois.|-id=307| 26307 Friedafein ||  || 26307 Friedafein Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Frieda Rose Fein (b. 1991) is a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors, for her behavioral and social sciences project. She attends the John Adams High School, South Bend, Indiana.|-id=314| 26314 Škvorecký ||  || Josef Škvorecký, Czech writer † ‡ |-id=319| 26319 Miyauchi ||  || Miyauchi town is situated in the southern part of Nanyo city, Yamagata, Japan. |-id=323| 26323 Wuqijin ||  || 26323 Wuqijin Discovered 1998 Nov. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Wu Qijin (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her animal-sciences project. She attends the Fuzhou No. 1 Middle School, Fuzhou, Fujian, China.|-id=328| 26328 Litomyšl || 1998 WQ || Litomyšl, Czech Republic † |-id=331| 26331 Kondamuri ||  || 26331 Kondamuri Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Neil Kondamuri (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his animal-sciences project. He attends the Munster High School, Munster, Indiana, U.S.A.|-id=332| 26332 Alyssehrlich ||  || 26332 Alyssehrlich Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Alyssa Chelsea Ehrlich (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her animal-sciences project. She attends the South Side High School, Rockville Centre, New York, U.S.A.|-id=333| 26333 Joachim ||  || 26333 Joachim Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gabriel Thailand Joachim (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his animal-sciences project. He attends the Cibola High School, Albuquerque, New Mexico, U.S.A.|-id=334| 26334 Melimcdowell ||  || 26334 Melimcdowell Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Melissa Severn McDowell (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her animal-sciences team project. She attends the Saint Joseph's Academy, Baton Rouge, Louisiana, U.S.A.|-id=336| 26336 Mikemcdowell ||  || 26336 Mikemcdowell Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Charles McDowell (b. 1995) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his animal-sciences team project. He attends the Catholic High School, Baton Rouge, Louisiana, U.S.A.|-id=337| 26337 Matthewagam ||  || 26337 Matthewagam Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Matthew Samuel Agam (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his behavioral- and social-sciences project. He attends the Beaverton High School, Beaverton, Oregon, U.S.A.|-id=340| 26340 Evamarková ||  || Eva Marková, Czech astronomer † |-id=345| 26345 Gedankien ||  || 26345 Gedankien Discovered 1998 Dec. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tamara Gedankien (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her behavioral- and social-sciences project. She attends the Escola Brasileira Israelita Chaim Nachman Bialik, Sao Paulo, Brazil.|-id=355| 26355 Grueber ||  || Johannes Grueber, 17th-century Austrian Jesuit priest, missionary, mathematician, astronomer at the Chinese imperial court, and author of the first European travelogue of Tibet †|-id=356| 26356 Aventini ||  || Andrea Aventini, Italian amateur astronomer †|-id=357| 26357 Laguerre ||  || Edmond Nicolas Laguerre, 19th-century French mathematician |-id=368| 26368 Alghunaim ||  || 26368 Alghunaim Discovered 1999 Feb. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Abdulaziz Khalid Alghunaim (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his behavioral- and social-sciences project. He attends the Asrary School, Riyadh, Saudi Arabia.|-id=376| 26376 Roborosa ||  || Róbert "Robo" Rosa, 20th-century Slovak amateur astronomer and computer graphic designer |-id=386| 26386 Adelinacozma ||  || 26386 Adelinacozma Discovered 1999 Sept. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Adelina Corina Cozma (b. 1995) was awarded second place in the 2010 Intel International Science and Engineering Fair for her behavioral- and social-sciences project. She attends the Bayview Secondary School, Richmond Hill, Ontario, Canada.|-id=389| 26389 Poojarambhia ||  || 26389 Poojarambhia Discovered 1999 Oct. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Pooja Rambhia (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her biochemistry project. She attends the Jericho High School, Jericho, New York, U.S.A.|-id=390| 26390 Rušin ||  || Vojtech Rušin, Slovak solar physicist |-id=393| 26393 Scaffa ||  || 26393 Scaffa Discovered 1999 Nov. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Alejandro Mariano Scaffa (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his biochemistry project. He attends the Escola Americana de Campinas, Campinas, Sao Paulo, Brazil.|-id=394| 26394 Kandola ||  || 26394 Kandola Discovered 1999 Nov. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Manjinder Singh Kandola (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his biochemistry project. He attends the Queens High School for the Sciences at York College, Jamaica, New York, U.S.A.|-id=395| 26395 Megkurohara ||  || 26395 Megkurohara Discovered 1999 Nov. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Megan M. Kurohara (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her biochemistry team project. She attends the Hilo High School, Hilo, Hawaii, U.S.A.|-id=396| 26396 Chengjingjie ||  || 26396 Chengjingjie Discovered 1999 Nov. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Cheng Jingjie (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for her cellular- and molecular-biology project. She attends the Raffles Girls' School, Singapore.|-id=397| 26397 Carolynsinow ||  || 26397 Carolynsinow Discovered 1999 Nov. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Carolyn Sinow (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for her cellular- and molecular-biology project. She attends the Palos Verdes Peninsula High School, Rolling Hills Estates, California, U.S.A.|-id=399| 26399 Rileyennis ||  || 26399 Rileyennis Discovered 1999 Nov. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Riley C. Ennis (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology project. He attends the Thomas Jefferson High School for Science and Technology, Alexandria, Virginia, U.S.A.|-id=400| 26400 Roshanpalli ||  || 26400 Roshanpalli Discovered 1999 Nov. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Roshan Palli (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology team project. He attends the Paul Laurence Dunbar High School, Lexington, Kentucky, U.S.A.|}

text: 26301 Hellawillis

text: ||  || 26301 Hellawillis Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Hella Willis mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Sheboygan North High School, Sheboygan, Wisconsin.|-id=302|

text: 26302 Zimolzak

text: ||  || 26302 Zimolzak Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Matt Zimolzak mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the William Fremd High School, Palatine, Illinois.|-id=307|

text: 26307 Friedafein

text: ||  || 26307 Friedafein Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Frieda Rose Fein (b. 1991) is a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors, for her behavioral and social sciences project. She attends the John Adams High School, South Bend, Indiana.|-id=314|

text: 26314 Škvorecký

text: Josef Škvorecký

text: , Czech writer † ‡ |-id=319|

text: 26319 Miyauchi

text: Miyauchi town

text: is situated in the southern part of

text: Nanyo city

text: , Yamagata, Japan. |-id=323|

text: 26323 Wuqijin

text: ||  || 26323 Wuqijin Discovered 1998 Nov. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Wu Qijin (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her animal-sciences project. She attends the Fuzhou No. 1 Middle School, Fuzhou, Fujian, China.|-id=328|

text: 26328 Litomyšl

text: || 1998 WQ ||

text: Litomyšl

text: , Czech Republic † |-id=331|

text: 26331 Kondamuri

text: ||  || 26331 Kondamuri Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Neil Kondamuri (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his animal-sciences project. He attends the Munster High School, Munster, Indiana, U.S.A.|-id=332|

text: 26332 Alyssehrlich

text: ||  || 26332 Alyssehrlich Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Alyssa Chelsea Ehrlich (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her animal-sciences project. She attends the South Side High School, Rockville Centre, New York, U.S.A.|-id=333|

text: 26333 Joachim

text: ||  || 26333 Joachim Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gabriel Thailand Joachim (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his animal-sciences project. He attends the Cibola High School, Albuquerque, New Mexico, U.S.A.|-id=334|

text: 26334 Melimcdowell

text: ||  || 26334 Melimcdowell Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Melissa Severn McDowell (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her animal-sciences team project. She attends the Saint Joseph's Academy, Baton Rouge, Louisiana, U.S.A.|-id=336|

text: 26336 Mikemcdowell

text: ||  || 26336 Mikemcdowell Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Charles McDowell (b. 1995) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his animal-sciences team project. He attends the Catholic High School, Baton Rouge, Louisiana, U.S.A.|-id=337|

text: 26337 Matthewagam

text: ||  || 26337 Matthewagam Discovered 1998 Nov. 21 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Matthew Samuel Agam (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his behavioral- and social-sciences project. He attends the Beaverton High School, Beaverton, Oregon, U.S.A.|-id=340|

text: 26340 Evamarková

text: Eva Marková

text: , Czech astronomer † |-id=345|

text: 26345 Gedankien

text: ||  || 26345 Gedankien Discovered 1998 Dec. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tamara Gedankien (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her behavioral- and social-sciences project. She attends the Escola Brasileira Israelita Chaim Nachman Bialik, Sao Paulo, Brazil.|-id=355|

text: 26355 Grueber

text: Johannes Grueber

text: , 17th-century Austrian Jesuit priest, missionary, mathematician, astronomer at the Chinese imperial court, and author of the first European travelogue of Tibet †|-id=356|

text: 26356 Aventini

text: Andrea Aventini

text: , Italian amateur astronomer †|-id=357|

text: 26357 Laguerre

text: Edmond Nicolas Laguerre

text: , 19th-century French mathematician |-id=368|

text: 26368 Alghunaim

text: ||  || 26368 Alghunaim Discovered 1999 Feb. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Abdulaziz Khalid Alghunaim (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his behavioral- and social-sciences project. He attends the Asrary School, Riyadh, Saudi Arabia.|-id=376|

text: 26376 Roborosa

text: ||  || Róbert "Robo" Rosa, 20th-century Slovak amateur astronomer and computer graphic designer |-id=386|

text: 26386 Adelinacozma

text: ||  || 26386 Adelinacozma Discovered 1999 Sept. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Adelina Corina Cozma (b. 1995) was awarded second place in the 2010 Intel International Science and Engineering Fair for her behavioral- and social-sciences project. She attends the Bayview Secondary School, Richmond Hill, Ontario, Canada.|-id=389|

text: 26389 Poojarambhia

text: ||  || 26389 Poojarambhia Discovered 1999 Oct. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Pooja Rambhia (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her biochemistry project. She attends the Jericho High School, Jericho, New York, U.S.A.|-id=390|

text: 26390 Rušin

text: Vojtech Rušin

text: , Slovak solar physicist |-id=393|

text: 26393 Scaffa

text: ||  || 26393 Scaffa Discovered 1999 Nov. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Alejandro Mariano Scaffa (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his biochemistry project. He attends the Escola Americana de Campinas, Campinas, Sao Paulo, Brazil.|-id=394|

text: 26394 Kandola

text: ||  || 26394 Kandola Discovered 1999 Nov. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Manjinder Singh Kandola (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his biochemistry project. He attends the Queens High School for the Sciences at York College, Jamaica, New York, U.S.A.|-id=395|

text: 26395 Megkurohara

text: ||  || 26395 Megkurohara Discovered 1999 Nov. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Megan M. Kurohara (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her biochemistry team project. She attends the Hilo High School, Hilo, Hawaii, U.S.A.|-id=396|

text: 26396 Chengjingjie

text: ||  || 26396 Chengjingjie Discovered 1999 Nov. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Cheng Jingjie (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for her cellular- and molecular-biology project. She attends the Raffles Girls' School, Singapore.|-id=397|

text: 26397 Carolynsinow

text: ||  || 26397 Carolynsinow Discovered 1999 Nov. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Carolyn Sinow (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for her cellular- and molecular-biology project. She attends the Palos Verdes Peninsula High School, Rolling Hills Estates, California, U.S.A.|-id=399|

text: 26399 Rileyennis

text: ||  || 26399 Rileyennis Discovered 1999 Nov. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Riley C. Ennis (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology project. He attends the Thomas Jefferson High School for Science and Technology, Alexandria, Virginia, U.S.A.|-id=400|

text: 26400 Roshanpalli

text: ||  || 26400 Roshanpalli Discovered 1999 Nov. 15 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Roshan Palli (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology team project. He attends the Paul Laurence Dunbar High School, Lexington, Kentucky, U.S.A.|}

answers: tqa2:L_0095/T_0925/13a3e914a11d75fa8dfbb3285de67ae0

answers: 0

answers: tqa2:L_0095/T_0925/c97ca9689dbb0692fcedf4ef38e4dcd9

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

answers: tqa2:L_0095/T_0925/ac80ea830a0039b32717a07ad258c159

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

answers: tqa2:L_0095/T_0925/45a741381354600c6041b1e31f57402b

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

answers: tqa2:L_0095/T_0925/343636ec587116e3ad123b813e9e3c83

answers: 0

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answers: tqa2:L_0095/T_0926/60d9698858e0d8abae18257034d0497c

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

answers: tqa2:L_0095/T_0926/0990e4d9e1abcc7e956e63667360010f

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

answers: tqa2:L_0095/T_0926/fd585af86e92f63914a9fdb739d4fd7a

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

answers: tqa2:L_0095/T_0926/9b12944e431bbeb2042fe667bfeb5688

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

answers: tqa2:L_0095/T_0926/a38c610fd23c272bd44f4833d1184b6b

answers: 0

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answers: Fuzhou High School

answers: NDQ_003824

answers: University of California, Berkeley.

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answers: asteroid belt

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answers: kvoreck

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answers: Fuzhou High School

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answers: kvoreck , Czech writer

answers: NDQ_003830

answers: Near-Earth Asteroid Research Team

text: The Near Earth Asteroid Rendezvous space probe was renamed "NEAR Shoemaker" in his honor. It arrived at asteroid 433 Eros in February 2000, and landed on the asteroid after a year of orbital study. He was previously honored with the asteroid 2074 Shoemaker, discovered and named by his colleague Eleanor F. Helin.

text: The

text: Near Earth Asteroid Rendezvous

text: space probe was renamed "NEAR Shoemaker" in his honor. It arrived at asteroid

text: 433 Eros

text: in February 2000, and landed on the asteroid after a year of orbital study. He was previously honored with the asteroid

text: 2074 Shoemaker

text: , discovered and named by his colleague

text: Eleanor F. Helin

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answers: space probe

answers: NDQ_003822

answers: 433 Eros

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: The Near Earth Asteroid Rendezvous space probe

answers: NDQ_003825

answers: 433 Eros

answers: NDQ_003826

answers: Near Earth

answers: NDQ_003827

answers: orbital

answers: NDQ_003828

answers: 433 Eros

answers: NDQ_003829

answers: 433 Eros

answers: NDQ_003830

answers: orbital study

text: Examination of samples recovered from the Moon indicates that the impactors were thermally evolved objects.  E-type asteroids, an example of this type, are uncommon in the main belt  but become more common toward the inner belt and would be expected to be most common in E-belt.  The Hungaria asteroids, which are a remnant of the E-belt in this model, contain a sizable fraction of E-type asteroids.

text: Examination of samples recovered from the Moon indicates that the impactors were thermally evolved objects.

text: E-type asteroid

text: s, an example of this type, are uncommon in the main belt  but become more common toward the inner belt and would be expected to be most common in E-belt.  The Hungaria asteroids, which are a remnant of the E-belt in this model, contain a sizable fraction of E-type asteroids.

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text: Classified as a Sr-subtype in the SMASS taxonomy, the S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,224 days). Its orbit has an eccentricity of 0.12 and an inclination of 5° with respect to the ecliptic. It has a rotation period of 8.6 hours and an albedo of 0.24, as assumed by the Collaborative Asteroid Lightcurve Link.

text: Classified as a Sr-subtype in the

text: SMASS

text: taxonomy, the

text: S-type

text: asteroid is a member of the

text: Flora family

text: , one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.0–2.5

text: AU

text: once every 3 years and 4 months (1,224 days). Its orbit has an

text: eccentricity

text: of 0.12 and an

text: inclination

text: of 5

text: with respect to the

text: ecliptic

text: . It has a

text: rotation period

text: of 8.6 hours and an

text: albedo

text: of 0.24, as assumed by the Collaborative Asteroid Lightcurve Link.

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answers: Flora family

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: The S-type asteroid

answers: NDQ_003825

answers: Flora family

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: orbits the Sun

answers: NDQ_003828

answers: S-type asteroid

answers: NDQ_003829

answers: SMASS taxonomy

answers: NDQ_003830

answers: orbits the Sun

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 3.4 kilometers in diameter and its surface has an albedo of 0.259, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.9 kilometers.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 3.4 kilometers in diameter and its surface has an

text: albedo

text: of 0.259, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.9 kilometers.

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answers: diameter

answers: NDQ_003822

answers: stony

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: NEOWISE mission

answers: NDQ_003825

answers: stony

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: stony

answers: NDQ_003828

answers: 3.9 kilometers

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: stony asteroids

text: is the preliminary baseline target of a proposed sample-return NASA mission called ARM. Besides the asteroid , several other asteroids, including Itokawa and Bennu, are being considered for this mission.

text: is the preliminary baseline target of a proposed

text: sample-return

text: NASA

text: mission called

text: ARM

text: . Besides the asteroid , several other asteroids, including

text: Itokawa

text: and

text: Bennu

text: , are being considered for this mission.

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answers: several other asteroids

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answers: several other asteroids

answers: NDQ_003826

answers: asteroid belt

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answers: sample-return

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answers: NDQ_003829

answers: Itokawa and Bennu

answers: NDQ_003830

answers: sample-return

text: In reality asteroids, even in the asteroid belt, are spaced extremely far apart. Proto-planets in the process of formation and planetary rings may look like that, but the Sun's asteroid belt does not. (The asteroid belt in the HD 69830 system may, however.) The asteroids are spread over such a high volume that it would be highly improbable even to pass close to a random asteroid. For example, the numerous space probes sent to the outer solar system, just across the main asteroid belt, have never had any problems, and asteroid rendezvous missions have elaborate targeting procedures. The movie 2001: A Space Odyssey is unusual in that it does portray realistically the ship's "encounter" with a lone asteroid pair.

text: In reality asteroids, even in the asteroid belt, are spaced extremely far apart. Proto-planets in the process of formation and planetary rings may look like that, but the Sun's asteroid belt does not. (The asteroid belt in the

text: HD 69830

text: system may, however.) The asteroids are spread over such a high volume that it would be highly improbable even to pass close to a random asteroid. For example, the numerous

text: space probe

text: s sent to the outer solar system, just across the main asteroid belt, have never had any problems, and asteroid rendezvous missions have elaborate targeting procedures. The movie

text: 2001: A Space Odyssey

text: is unusual in that it does portray realistically the ship's "encounter" with a lone asteroid pair.

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answers: random

answers: NDQ_003822

answers: are spaced extremely far apart

answers: NDQ_003823

answers: It would be highly improbable even to pass close to a random asteroid

answers: NDQ_003824

answers: It would be highly improbable even to pass close to a random asteroid.

answers: NDQ_003825

answers: are spaced extremely far apart

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: pass close to a random asteroid

answers: NDQ_003828

answers: It would be highly improbable even to pass close to a random asteroid

answers: NDQ_003829

answers: It would be highly improbable

answers: NDQ_003830

answers: space probes sent to the outer solar system

text: |-id=105| 134105 Josephfust ||  || Joseph Fust (b. 1958) is the United Launch Alliance spacecraft integration engineer for the OSIRIS-REx Asteroid Sample Return Mission. He was the spacecraft integration engineer for the MAVEN mission to Mars. He also serves as spacecraft integrator for various United States Air Force and National Security missions. |-id=109| 134109 Britneyburch ||  || Britney Burch (b. 1982) is a structural dynamics analyst with the NASA Launch Services Program and is the primary loads analyst for the OSIRIS-REx Asteroid Sample Return Mission. She has previously served as an analyst with the Mars MAVEN mission and the Pegasus/IRIS mission. |-id=112| 134112 Jeremyralph ||  || Jeremy Ralph (b. 1983) is the United Launch Alliance Flight Design Engineer for the Atlas V rocket, launching the OSIRIS-REx Asteroid Sample Return Mission to 101955 Bennu. He also assisted on the SDO, MSL and LDCM missions. |-id=124| 134124 Subirachs || 2005 AM || Josep Maria Subirachs, Catalan sculptor and painter |-id=125| 134125 Shaundaly ||  || Shaun Daly (b. 1979) is the KSC Launch Services Program Integration Engineer for the OSIRIS-REx Asteroid Sample Return Mission. He has served in the aerospace industry since 1997 both for the USAF as a Crew Chief during Operation Enduring Freedom and for NASA as an avionics engineer on 25 missions.|-id=127| 134127 Basher ||  || Benjamin Asher (b. 1990) is an Embry-Riddle Aeronautical University alumnus and a member of the flight design team at a.i. solutions, Inc. in support of NASA’s Launch Services Program for the OSIRIS-REx Asteroid Sample Return Mission. He is also a member of the flight design team in support of the TESS mission. |-id=130| 134130 Apáczai || || János Apáczai Csere, Hungarian polyglot and mathematician |-id=131| 134131 Skipowens ||  || Skip Owens (b. 1975) is the NASA LSP Integration Engineer for the OSIRISREx Asteroid Sample Return Mission. He was also a LSP Flight Design Engineer for over a dozen NASA missions. Before starting with LSP in 2001, he worked spacecraft mission design at Goddard Spaceflight Center for the EO-1 and WMAP missions. |-id=135| 134135 Steigerwald ||  || William Steigerwald (b. 1967) worked on the OSIRIS-REx Asteroid Sample Return Mission as a science writer. He has worked for over 19 years as a writer for a wide range of NASA missions in planetary science, astrobiology, astrophysics and heliophysics|-id=138| 134138 Laurabayley ||  || Laura C. Bayley (b. 1988) is a student engineer at the Massachusetts Institute of Technology responsible for test planning and assembly of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=146| 134146 Pronoybiswas ||  || Pronoy K. Biswas (b. 1992) is a student engineer at the Massachusetts Institute of Technology responsible for designing and implementing the avionics system for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=150| 134150 Bralower ||  || Harrison L. Bralower (b. 1988) worked as a student engineer at the Massachusetts Institute of Technology where he designed the detector assembly mount for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=160| 134160 Pluis ||  || Pluis, nickname of Aina Vandenabeele, the discoverer's niece, who died of leukemia at six months of age (this minor planet is a tribute to all children with cancer) |-id=169| 134169 Davidcarte ||  || David B. Carte (b. 1991) worked as a student engineer at the Massachusetts Institute of Technology where he was responsible for the structural design and testing of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=174| 134174 Jameschen ||  || Shuyi James Chen (b. 1988) worked as a student engineer at the Massachusetts Institute of Technology where he was the lead avionics and software engineer in the development of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=178| 134178 Markchodas ||  || Mark A. Chodas (b. 1990) is a student engineer at the Massachusetts Institute of Technology working as the Lead Systems Engineer ensuring that all system components meet science requirements for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=180| 134180 Nirajinamdar ||  || Niraj K. Inamdar (b. 1986) worked as a student engineer at the Massachusetts Institute of Technology where he conducted the preliminary performance modeling in the development of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |}

text: 134105 Josephfust

text: ||  || Joseph Fust (b. 1958) is the United Launch Alliance spacecraft integration engineer for the OSIRIS-REx Asteroid Sample Return Mission. He was the spacecraft integration engineer for the MAVEN mission to Mars. He also serves as spacecraft integrator for various United States Air Force and National Security missions. |-id=109|

text: 134109 Britneyburch

text: ||  || Britney Burch (b. 1982) is a structural dynamics analyst with the NASA Launch Services Program and is the primary loads analyst for the OSIRIS-REx Asteroid Sample Return Mission. She has previously served as an analyst with the Mars MAVEN mission and the Pegasus/IRIS mission. |-id=112|

text: 134112 Jeremyralph

text: ||  || Jeremy Ralph (b. 1983) is the United Launch Alliance Flight Design Engineer for the Atlas V rocket, launching the OSIRIS-REx Asteroid Sample Return Mission to

text: 101955 Bennu

text: . He also assisted on the SDO, MSL and LDCM missions. |-id=124|

text: 134124 Subirachs

text: || 2005 AM ||

text: Josep Maria Subirachs

text: , Catalan sculptor and painter |-id=125|

text: 134125 Shaundaly

text: ||  || Shaun Daly (b. 1979) is the KSC Launch Services Program Integration Engineer for the OSIRIS-REx Asteroid Sample Return Mission. He has served in the aerospace industry since 1997 both for the USAF as a Crew Chief during Operation Enduring Freedom and for NASA as an avionics engineer on 25 missions.|-id=127|

text: 134127 Basher

text: ||  || Benjamin Asher (b. 1990) is an Embry-Riddle Aeronautical University alumnus and a member of the flight design team at a.i. solutions, Inc. in support of NASA’s Launch Services Program for the OSIRIS-REx Asteroid Sample Return Mission. He is also a member of the flight design team in support of the TESS mission. |-id=130|

text: 134130 Apáczai

text: János Apáczai Csere

text: , Hungarian polyglot and mathematician |-id=131|

text: 134131 Skipowens

text: ||  || Skip Owens (b. 1975) is the NASA LSP Integration Engineer for the OSIRISREx Asteroid Sample Return Mission. He was also a LSP Flight Design Engineer for over a dozen NASA missions. Before starting with LSP in 2001, he worked spacecraft mission design at Goddard Spaceflight Center for the EO-1 and WMAP missions. |-id=135|

text: 134135 Steigerwald

text: ||  || William Steigerwald (b. 1967) worked on the OSIRIS-REx Asteroid Sample Return Mission as a science writer. He has worked for over 19 years as a writer for a wide range of NASA missions in planetary science, astrobiology, astrophysics and heliophysics|-id=138|

text: 134138 Laurabayley

text: ||  || Laura C. Bayley (b. 1988) is a student engineer at the Massachusetts Institute of Technology responsible for test planning and assembly of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=146|

text: 134146 Pronoybiswas

text: ||  || Pronoy K. Biswas (b. 1992) is a student engineer at the Massachusetts Institute of Technology responsible for designing and implementing the avionics system for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=150|

text: 134150 Bralower

text: ||  || Harrison L. Bralower (b. 1988) worked as a student engineer at the Massachusetts Institute of Technology where he designed the detector assembly mount for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=160|

text: 134160 Pluis

text: ||  || Pluis, nickname of Aina Vandenabeele, the discoverer's niece, who died of leukemia at six months of age (this minor planet is a tribute to all children with cancer) |-id=169|

text: 134169 Davidcarte

text: ||  || David B. Carte (b. 1991) worked as a student engineer at the Massachusetts Institute of Technology where he was responsible for the structural design and testing of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=174|

text: 134174 Jameschen

text: ||  || Shuyi James Chen (b. 1988) worked as a student engineer at the Massachusetts Institute of Technology where he was the lead avionics and software engineer in the development of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=178|

text: 134178 Markchodas

text: ||  || Mark A. Chodas (b. 1990) is a student engineer at the Massachusetts Institute of Technology working as the Lead Systems Engineer ensuring that all system components meet science requirements for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=180|

text: 134180 Nirajinamdar

text: ||  || Niraj K. Inamdar (b. 1986) worked as a student engineer at the Massachusetts Institute of Technology where he conducted the preliminary performance modeling in the development of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |}

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answers: NDQ_003821

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answers: NDQ_003822

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answers: NDQ_003823

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answers: NDQ_003824

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answers: NDQ_003825

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answers: NDQ_003826

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answers: Space Telescope

answers: NDQ_003822

answers: OSIRIS-REx Asteroid Sample Return Mission

answers: NDQ_003823

answers: Jeremy Ralph is the United Launch Alliance Flight Design Engineer for the Atlas V rocket, launching the OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003824

answers: Return Mission.

answers: NDQ_003825

answers: OSIRIS-REx Asteroid Sample Return Mission

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: NASA's Mars MAVEN mission

answers: NDQ_003828

answers: Jeremy Ralph is the United Launch Alliance Flight Design Engineer for the Atlas V rocket, launching the OSIRIS-REx Asteroid Sample Return Mission to 101955 Bennu. He also assisted on the SDO, MSL, and LDCM missions.

answers: NDQ_003829

answers: avionics engineering team for the Atlas V rocket.

answers: NDQ_003830

answers: a.i. solutions, Inc.

text: 1566 Icarus ( ) is an Apollo asteroid (a subclass of near-Earth asteroid) that at perihelion comes closer to the Sun than Mercury, i.e. it is a Mercury-crossing asteroid. It is also a Venus and Mars-crosser. It is named after Icarus of Greek mythology, who flew too close to the Sun. It was discovered on 27 June 1949 by Walter Baade at Palomar Observatory. From 1949 until the discovery of 3200 Phaethon in 1983, it was known as the asteroid that passed closest to the Sun.

text: 1566 Icarus ( ) is an

text: Apollo asteroid

text: (a subclass of

text: near-Earth asteroid

text: ) that at

text: perihelion

text: comes closer to the

text: Sun

text: than

text: Mercury

text: , i.e. it is a

text: Mercury-crossing asteroid

text: . It is also a

text: Venus

text: and

text: Mars-crosser

text: . It is named after

text: Icarus

text: of

text: Greek mythology

text: , who flew too close to the Sun. It was discovered on 27 June 1949 by

text: Walter Baade

text: at

text: Palomar Observatory

text: . From 1949 until the discovery of

text: 3200 Phaethon

text: in 1983, it was known as the asteroid that passed closest to the Sun.

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answers: near-Earth asteroid

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answers: Mercury-crossing

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text: C-type asteroids are carbonaceous asteroids. They are the most common variety, forming around 75% of known asteroids.  They are distinguished by a very low albedo because their composition includes a large amount of carbon, in addition to rocks and minerals.  They occur most frequently at the outer edge of the asteroid belt, 3.5 astronomical units (AU) from the Sun, where 80% of the asteroids are of this type, whereas only 40% of asteroids at 2 AU from the Sun are C-type.  The proportion of C-types may actually be greater than this, because C-types are much darker than most other asteroid types except D-types and others common only at the extreme outer edge of the asteroid belt.

text: C-type asteroids are

text: carbon

text: aceous

text: asteroid

text: s. They are the most common variety, forming around 75% of known

text: asteroid

text: s.  They are distinguished by a very low

text: albedo

text: because their composition includes a large amount of carbon, in addition to rocks and minerals.  They occur most frequently at the outer edge of the asteroid belt, 3.5

text: astronomical units

text: (AU) from the Sun, where 80% of the asteroids are of this type, whereas only 40% of asteroids at 2 AU from the Sun are C-type.  The proportion of C-types may actually be greater than this, because C-types are much darker than most other asteroid types except

text: D-types

text: and others common only at the extreme outer edge of the

text: asteroid belt

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answers: asteroids

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answers: carbonaceous

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answers: C-type asteroids

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answers: C-type asteroids

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answers: carbonaceous

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answers: asteroid belt

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answers: 3.5 astronomical units

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answers: C-type

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answers: C-type asteroids

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answers: C-type asteroids

text: Composition is calculated from three primary sources: albedo, surface spectrum, and density. The last can only be determined accurately by observing the orbits of moons the asteroid might have. So far, every asteroid with moons has turned out to be a rubble pile, a loose conglomeration of rock and metal that may be half empty space by volume. The investigated asteroids are as large as 280 km in diameter, and include 121 Hermione (268×186×183 km), and 87 Sylvia (384×262×232 km). Only half a dozen asteroids are larger than 87 Sylvia, though none of them have moons; however, some smaller asteroids are thought to be more massive, suggesting they may not have been disrupted, and indeed 511 Davida, the same size as Sylvia to within measurement error, is estimated to be two and a half times as massive, though this is highly uncertain. The fact that such large asteroids as Sylvia can be rubble piles, presumably due to disruptive impacts, has important consequences for the formation of the Solar System: Computer simulations of collisions involving solid bodies show them destroying each other as often as merging, but colliding rubble piles are more likely to merge. This means that the cores of the planets could have formed relatively quickly.

text: Composition is calculated from three primary sources:

text: albedo

text: , surface spectrum, and density. The last can only be determined accurately by observing the orbits of moons the asteroid might have. So far, every asteroid with moons has turned out to be a rubble pile, a loose conglomeration of rock and metal that may be half empty space by volume. The investigated asteroids are as large as 280 km in diameter, and include

text: 121 Hermione

text: (268×186×183 km), and

text: 87 Sylvia

text: (384×262×232 km). Only half a dozen asteroids are

text: larger than 87 Sylvia

text: , though none of them have moons; however, some smaller asteroids are thought to be more massive, suggesting they may not have been disrupted, and indeed

text: 511 Davida

text: , the same size as Sylvia to within measurement error, is estimated to be two and a half times as massive, though this is highly uncertain. The fact that such large asteroids as Sylvia can be rubble piles, presumably due to disruptive impacts, has important consequences for the formation of the Solar System: Computer simulations of collisions involving solid bodies show them destroying each other as often as merging, but colliding rubble piles are more likely to merge. This means that the cores of the planets could have formed relatively quickly.

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answers: loose conglomeration of rock and metal

answers: NDQ_003822

answers: are as large as 280 km in diameter

answers: NDQ_003823

answers: no

answers: NDQ_003824

answers: So far, every asteroid with moons has turned out to be a rubble pile

answers: NDQ_003825

answers: are as large as 280 km in diameter

answers: NDQ_003826

answers: Solar System

answers: NDQ_003827

answers: rubble piles

answers: NDQ_003828

answers: 87 Sylvia

answers: NDQ_003829

answers: This means that the cores of the planets could have formed relatively quickly

answers: NDQ_003830

answers: has important consequences for the formation of the Solar System

text: NEODyS (Near Earth Objects Dynamic Site) is an Italian and Spanish service that provides information on Near Earth Objects with a convenient Web-based interface. It is based on a continually and (almost) automatically maintained database of near earth asteroid orbits. This site provides a number of services to the NEO community. The main service is an impact monitoring system (CLOMON2) of all near-Earth asteroids covering a period until the year 2100.

text: NEODyS (Near Earth Objects Dynamic Site) is an Italian and Spanish service that provides information on

text: Near Earth Object

text: s with a convenient Web-based interface. It is based on a continually and (almost) automatically maintained database of near earth asteroid orbits. This site provides a number of services to the NEO community. The main service is an impact monitoring system (CLOMON2) of all

text: near-Earth asteroid

text: s covering a period until the year 2100.

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answers: impact monitoring system (CLOMON2)

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answers: impact monitoring system

text: 37 Fides ( ) is a large main-belt asteroid. It was discovered by German astronomer Karl Theodor Robert Luther on October 5, 1855, and named after Fides, the Roman goddess of loyalty. Fides was the last of the main-belt asteroids to be assigned an iconic symbol. 37 Fides is also a S-type asteroid in the Tholen classification system.

text: 37 Fides ( ) is a large

text: main-belt

text: asteroid

text: . It was discovered by German astronomer

text: Karl Theodor Robert Luther

text: on October 5, 1855, and named after

text: Fides

text: , the

text: Roman

text: goddess of

text: loyalty

text: . Fides was the last of the main-belt asteroids to be assigned an

text: iconic symbol

text: . 37 Fides is also a S-type asteroid in the

text: Tholen classification

text: system.

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answers: main-belt

answers: NDQ_003822

answers: main-belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: astronomer Karl Theodor Robert Luther

answers: NDQ_003825

answers: main-belt

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answers: main-belt

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answers: be assigned an iconic symbol

answers: NDQ_003828

answers: 37 Fides

answers: NDQ_003829

answers: 37 Fides

answers: NDQ_003830

answers: astronomer

text: Based on NASA's space-based WISE and its subsequent NEOWISE mission, the asteroid has an albedo of 0.11 and 0.12, and a diameter of 19.9 and 20.0 kilometers, respectively, while the Collaborative Asteroid Lightcurve Link (CALL) assumes a lower albedo of 0.06, which translates into a larger diameter of 26.6 kilometers, as the lower the albedo (reflectivity), the higher the body's diameter, for a given absolute magnitude (brightness).

text: Based on NASA's space-based

text: WISE

text: and its subsequent

text: NEOWISE

text: mission, the asteroid has an

text: albedo

text: of 0.11 and 0.12, and a diameter of 19.9 and 20.0 kilometers, respectively, while the Collaborative Asteroid Lightcurve Link (CALL) assumes a lower albedo of 0.06, which translates into a larger diameter of 26.6 kilometers, as the lower the albedo (reflectivity), the higher the body's diameter, for a given absolute magnitude (brightness).

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answers: body

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answers: albedo (reflectivity)

answers: NDQ_003823

answers: asteroids do not have impacts with other objects

answers: NDQ_003824

answers: WISE and its subsequent NEOWISE mission

answers: NDQ_003825

answers: albedo (reflectivity)

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answers: asteroid belt

answers: NDQ_003827

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answers: NDQ_003828

answers: NEOWISE

answers: NDQ_003829

answers: The asteroid has an albedo of 0.11 and 0.12, and a diameter of 19.9 and 20.0 kilometers, respectively

answers: NDQ_003830

answers: asteroid

text: Once Brooke convinces the Geotopians that preventing the asteroid's fall is more important than their lost youth, they and the herd help with Buck's plan, which is to fill up a geyser with the crystals so that the pressure launches them into space to draw the asteroid away. The dromaeosaurs attempt to intervene, but Buck convinces Roger that they will not be able to survive the asteroid, and he in turn convinces Gavin and Gertie to help. The plan works, and the asteroid is pulled back into space. The herd then departs back home, including Sid, who parts ways from Brooke, but just after they leave, an asteroid piece falls inside a hot spring, giving it rejuvenating properties and making the Geotopians and Sid's grandmother, who stayed behind with them, regain their youth. After the herd returns, Manny reconciles with Julian, Peaches and Julian celebrate their wedding, Diego and Shira become heroes to the kids who were scared of them before, and a rejuvenated Brooke appears during the ceremony to reunite with Sid.

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answers: pulled back into space

answers: NDQ_003822

answers: dromaeosaurs

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answers: asteroids

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answers: asteroid

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answers: dromaeosaurs

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answers: Geotopians

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answers: fall

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answers: The herd then departs back home

answers: NDQ_003829

answers: Roger that they will not be able to survive

answers: NDQ_003830

answers: lose their youth

text: There are only 14 known Amor asteroids whose average distance from the Sun is beyond the asteroid belt. Their semi-major axes are greater than 3.57 AU and they are called Amor IV asteroids. All are Jupiter crossers. Though they have very high eccentricities (0.65 to 0.75), their orbits are not as eccentric as those of most Damocloids and comets, which tend to have eccentricities around 0.9. The only named Amor IV asteroid is 3552 Don Quixote and the only other numbered Amor IV asteroid is . So far, no Amor asteroid has been discovered that crosses the orbit of Saturn.

text: There are only 14 known Amor asteroids whose average distance from the Sun is beyond the asteroid belt. Their semi-major axes are greater than 3.57 AU and they are called Amor IV asteroids. All are Jupiter crossers. Though they have very high eccentricities (0.65 to 0.75), their orbits are not as eccentric as those of most

text: Damocloid

text: s and comets, which tend to have eccentricities around 0.9. The only named Amor IV asteroid is

text: 3552 Don Quixote

text: and the only other numbered Amor IV asteroid is . So far, no Amor asteroid has been discovered that

text: crosses the orbit of Saturn

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text: The commercial competition was won by a design called 'Foresight' created by SpaceWorks Enterprises, Inc. SpaceWorks proposed a simple orbiter with only two instruments and a radio beacon at a cost of ~140 million USD, launched aboard a Minotaur IV between 2012 and 2014, to arrive at Apophis five to ten months later. It would then rendezvous with, observe, and track the asteroid. Foresight would orbit the asteroid to gather data with a multi-spectral imager for one month. It would then leave orbit and fly in formation with Apophis around the Sun at a range of two kilometres (1.2 miles). The spacecraft would use laser ranging to the asteroid and radio tracking from Earth for ten months to accurately determine the asteroid's orbit and how it might change.

text: The commercial competition was won by a design called 'Foresight' created by

text: SpaceWorks Enterprises, Inc.

text: SpaceWorks proposed a simple orbiter with only two instruments and a radio beacon at a cost of ~140 million USD, launched aboard a

text: Minotaur IV

text: between 2012 and 2014, to arrive at Apophis five to ten months later. It would then rendezvous with, observe, and track the asteroid. Foresight would orbit the asteroid to gather data with a

text: multi-spectral image

text: r for one month. It would then leave orbit and fly in formation with Apophis around the Sun at a range of two kilometres (1.2 miles). The spacecraft would use laser ranging to the asteroid and radio tracking from Earth for ten months to accurately determine the asteroid's orbit and how it might change.

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answers: Apophis

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answers: Asteroids are too small to have impacts with other objects

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answers: SpaceWorks proposed a simple orbiter with only two instruments and a radio beacon

answers: NDQ_003825

answers: Apophis

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answers: the Sun

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answers: fly in formation

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answers: SpaceWorks Enterprises, Inc.

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answers: orbit and how it might change

text: The Near Earth Asteroid Rendezvous – Shoemaker (NEAR Shoemaker), renamed after its 1996 launch in honor of planetary scientist Eugene Shoemaker, was a robotic space probe designed by the Johns Hopkins University Applied Physics Laboratory for NASA to study the near-Earth asteroid Eros from close orbit over a period of a year. The mission succeeded in closing in with the asteroid and orbited it several times, finally terminating by touching down on the asteroid on 12 February 2001.

text: The Near Earth Asteroid Rendezvous – Shoemaker (NEAR Shoemaker), renamed after its 1996 launch in honor of planetary scientist

text: Eugene Shoemaker

text: , was a

text: robotic

text: space probe

text: designed by the

text: Johns Hopkins University

text: Applied Physics Laboratory

text: for

text: NASA

text: to study the

text: near-Earth asteroid

text: Eros

text: from close orbit over a period of a year. The mission succeeded in closing in with the asteroid and orbited it several times, finally terminating by touching down on the asteroid on 12 February 2001.

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answers: near-Earth

answers: NDQ_003822

answers: Eros

answers: NDQ_003823

answers: It does not have craters

answers: NDQ_003824

answers: The Near Earth Asteroid Rendezvous

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answers: Near Earth

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answers: touch down

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answers: Eros

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: planetary

text: 433 Eros is an S-type near-Earth asteroid approximately  in size, the second-largest near-Earth asteroid after 1036 Ganymed. It was discovered in 1898 and was the first near-Earth asteroid discovered. It was the first asteroid orbited by an Earth probe (in 2000). It belongs to the Amor group.

text: 433 Eros is an

text: S-type

text: near-Earth asteroid

text: approximately  in size, the second-largest near-Earth

text: asteroid

text: after

text: 1036 Ganymed

text: . It was discovered in 1898 and was the first near-Earth asteroid discovered. It was the first asteroid orbited by an Earth probe (in 2000). It belongs to the

text: Amor

text: group.

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answers: orbited by an Earth probe

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text: |-| 26501 Sachiko ||  || Sachiko Nagata, teacher of Oshibana, the Japanese art of arranging pressed flowers |-id=502| 26502 Traviscole ||  || 26502 Traviscole Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Travis Cole Sylvester (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environmental-management project. He attends the Greybull High School, Greybull, Wyoming, U.S.A.|-id=503| 26503 Avicramer ||  || 26503 Avicramer Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Avilash Kalpathy Cramer (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the West Linn High School, West Linn, Oregon, U.S.A.|-id=504| 26504 Brandonli ||  || 26504 Brandonli Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Brandon Li (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the Jericho High School, Jericho, New York, U.S.A.|-id=505| 26505 Olextokarev ||  || 26505 Olextokarev Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Olexandr Tokarev (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the Chemical Ecological Lyceum, Dnipropetrovsk, Ukraine.|-id=507| 26507 Mikelin ||  || 26507 Mikelin Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Lin (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management team project. He attends the Robert Louis Stevenson Upper School, Pebble Beach, California, U.S.A.|-id=508| 26508 Jimmylin ||  || 26508 Jimmylin Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jimmy Lin (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management team project. He attends the Robert Louis Stevenson Upper School, Pebble Beach, California, U.S.A.|-id=513| 26513 Newberry ||  || 26513 Newberry Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. William Cummings Newberry (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for his materials-and-bioengineering project. He attends the Greenwich High School, Greenwich, Connecticut, U.S.A.|-id=518| 26518 Bhuiyan ||  || 26518 Bhuiyan Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mubarrat Nuvid Bhuiyan (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering project. She attends the Jericho High School, Jericho, New York, U.S.A.|-id=522| 26522 Juliapoje ||  || 26522 Juliapoje Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Julia Elizabeth Poje (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering project. She attends the Valley Stream South High School, Valley Stream, New York, U.S.A.|-id=526| 26526 Jookayhyun ||  || 26526 Jookayhyun Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joo Kay Hyun (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering project. She attends the Changduk Girls High School, Seoul, South Korea.|-id=527| 26527 Leasure ||  || 26527 Leasure Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Audrey Christine Leasure (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering team project. She attends the Lake Highland Preparatory School, Orlando, Florida, U.S.A.|-id=528| 26528 Genniferubin ||  || 26528 Genniferubin Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gennifer Reid Rubin (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering team project. She attends the Lake Highland Preparatory School, Orlando, Florida, U.S.A.|-id=530| 26530 Lucferreira ||  || 26530 Lucferreira Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Lucas Strasburg Ferreira (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his materials-and-bioengineering team project. He attends the Fundacao Escola Tecnica Liberato Salzano Vieira da Cunha, Novo Hamburgo, Rio Grande do Sul, Brazil.|-id=532| 26532 Eduardoboff ||  || 26532 Eduardoboff Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Eduardo Trierweiler Boff (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his materials-and-bioengineering team project. He attends the Fundacao Escola Tecnica Liberato Salzano Vieira da Cunha, Novo Hamburgo, Rio Grande do Sul, Brazil.|-id=533| 26533 Aldering ||  || Greg Aldering (b. 1962), a member of Supernova Cosmology Project studying the use of Type Ia supernovae for determining cosmological parameters. |-id=537| 26537 Shyamalbuch ||  || 26537 Shyamalbuch Discovered 2000 Feb. 28 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shyamal Buch (b. 1995) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation project. He attends the Vista del Lago High School, Folsom, California, U.S.A.|-id=541| 26541 Garyross ||  || Gary Ross (b. 1945) has served on the executive board of the Grand Rapids Astronomical Society and Warren Astronomical Society in southern Michigan. He has also been instrumental in the operation of the James C. Veen observatory in Lowell, Michigan, for over 40 years. |-id=544| 26544 Ajjarapu ||  || 26544 Ajjarapu Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Avanthi Sai Ajjarapu (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation project. She attends the Ames High School, Ames, Iowa, U.S.A.|-id=545| 26545 Meganperkins ||  || 26545 Meganperkins Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Megan Lynn Perkins (b. 1994) was awarded first place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation project. She attends the duPont Manual High School, Louisville, Kentucky, U.S.A.|-id=546| 26546 Arulmani ||  || 26546 Arulmani Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Dheevesh Arulmani (b. 1995) was awarded second place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation project. He attends the Gordon Graydon Memorial Secondary School, Mississauga, Ontario, Canada.|-id=548| 26548 Joykutty ||  || 26548 Joykutty Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Anna Maria Joykutty (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation project. She attends the American Heritage School, Plantation, Florida, U.S.A.|-id=549| 26549 Tankanran ||  || 26549 Tankanran Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tan Kan-Ran (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation team project. He attends the Beijing No. 4 High School, Beijing, China.|-id=551| 26551 Shenliangbo ||  || 26551 Shenliangbo Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shen Liang-Bo (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation team project. He attends the Beijing No. 4 High School, Beijing, China.|-id=557| 26557 Aakritijain ||  || 26557 Aakritijain Discovered 2000 Feb. 28 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Aakriti Jain (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation team project. She attends the Lynbrook High School, San Jose, California, U.S.A.|-id=559| 26559 Chengcheng ||  || 26559 Chengcheng Discovered 2000 Mar. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Cheng Cheng (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation team project. She attends the Lynbrook High School, San Jose, California, U.S.A.|-id=575| 26575 Andreapugh ||  || 26575 Andreapugh Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Andrea Aleah Pugh (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for her environmental-science project. She attends the Saginaw Arts and Sciences Academy, Saginaw, Michigan, U.S.A.|-id=578| 26578 Cellinekim ||  || 26578 Cellinekim Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Celline Kim (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her environmental-science project. She attends the Manhasset High School, Manhasset, New York, U.S.A.|-id=586| 26586 Harshaw ||  || 26586 Harshaw Discovered 2000 Mar. 10 by R. Hill at the Catalina Sky Survey. Richard Harshaw (b. 1951) is an Arizona amateur astronomer who makes measurements of double stars. He has served in numerous official positions with astronomy clubs.|-id=591| 26591 Robertreeves ||  || 26591 Robertreeves Discovered 2000 Mar. 2 by R. Hill at the Catalina Sky Survey. Robert Reeves (b. 1946) is the author of several books on digital astronomical imaging and of numerous popular articles on various topics in astronomy and space science.|-id=592| 26592 Maryrenfro ||  || Mary Renfro Reeves (born 1957) is a physical therapist in San Antonio, Texas |-id=593| 26593 Perrypat ||  || Perry Remaklus (b. 1939) and Patricia Remaklus (b. 1941), the founders, owners, and operators of the Willmann-Bell astronomy book publishing firm and long-time members of the Springfield Telescope Makers. |}

text: 26501 Sachiko

text: ||  || Sachiko Nagata, teacher of

text: Oshibana

text: , the Japanese art of arranging pressed flowers |-id=502|

text: 26502 Traviscole

text: ||  || 26502 Traviscole Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Travis Cole Sylvester (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environmental-management project. He attends the Greybull High School, Greybull, Wyoming, U.S.A.|-id=503|

text: 26503 Avicramer

text: ||  || 26503 Avicramer Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Avilash Kalpathy Cramer (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the West Linn High School, West Linn, Oregon, U.S.A.|-id=504|

text: 26504 Brandonli

text: ||  || 26504 Brandonli Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Brandon Li (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the Jericho High School, Jericho, New York, U.S.A.|-id=505|

text: 26505 Olextokarev

text: ||  || 26505 Olextokarev Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Olexandr Tokarev (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the Chemical Ecological Lyceum, Dnipropetrovsk, Ukraine.|-id=507|

text: 26507 Mikelin

text: ||  || 26507 Mikelin Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Lin (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management team project. He attends the Robert Louis Stevenson Upper School, Pebble Beach, California, U.S.A.|-id=508|

text: 26508 Jimmylin

text: ||  || 26508 Jimmylin Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jimmy Lin (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management team project. He attends the Robert Louis Stevenson Upper School, Pebble Beach, California, U.S.A.|-id=513|

text: 26513 Newberry

text: ||  || 26513 Newberry Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. William Cummings Newberry (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for his materials-and-bioengineering project. He attends the Greenwich High School, Greenwich, Connecticut, U.S.A.|-id=518|

text: 26518 Bhuiyan

text: ||  || 26518 Bhuiyan Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mubarrat Nuvid Bhuiyan (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering project. She attends the Jericho High School, Jericho, New York, U.S.A.|-id=522|

text: 26522 Juliapoje

text: ||  || 26522 Juliapoje Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Julia Elizabeth Poje (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering project. She attends the Valley Stream South High School, Valley Stream, New York, U.S.A.|-id=526|

text: 26526 Jookayhyun

text: ||  || 26526 Jookayhyun Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joo Kay Hyun (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering project. She attends the Changduk Girls High School, Seoul, South Korea.|-id=527|

text: 26527 Leasure

text: ||  || 26527 Leasure Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Audrey Christine Leasure (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering team project. She attends the Lake Highland Preparatory School, Orlando, Florida, U.S.A.|-id=528|

text: 26528 Genniferubin

text: ||  || 26528 Genniferubin Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gennifer Reid Rubin (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for her materials-and-bioengineering team project. She attends the Lake Highland Preparatory School, Orlando, Florida, U.S.A.|-id=530|

text: 26530 Lucferreira

text: ||  || 26530 Lucferreira Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Lucas Strasburg Ferreira (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his materials-and-bioengineering team project. He attends the Fundacao Escola Tecnica Liberato Salzano Vieira da Cunha, Novo Hamburgo, Rio Grande do Sul, Brazil.|-id=532|

text: 26532 Eduardoboff

text: ||  || 26532 Eduardoboff Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Eduardo Trierweiler Boff (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his materials-and-bioengineering team project. He attends the Fundacao Escola Tecnica Liberato Salzano Vieira da Cunha, Novo Hamburgo, Rio Grande do Sul, Brazil.|-id=533|

text: 26533 Aldering

text: ||  || Greg Aldering (b. 1962), a member of Supernova Cosmology Project studying the use of Type Ia supernovae for determining cosmological parameters. |-id=537|

text: 26537 Shyamalbuch

text: ||  || 26537 Shyamalbuch Discovered 2000 Feb. 28 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shyamal Buch (b. 1995) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation project. He attends the Vista del Lago High School, Folsom, California, U.S.A.|-id=541|

text: 26541 Garyross

text: ||  || Gary Ross (b. 1945) has served on the executive board of the Grand Rapids Astronomical Society and Warren Astronomical Society in southern Michigan. He has also been instrumental in the operation of the James C. Veen observatory in Lowell, Michigan, for over 40 years. |-id=544|

text: 26544 Ajjarapu

text: ||  || 26544 Ajjarapu Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Avanthi Sai Ajjarapu (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation project. She attends the Ames High School, Ames, Iowa, U.S.A.|-id=545|

text: 26545 Meganperkins

text: ||  || 26545 Meganperkins Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Megan Lynn Perkins (b. 1994) was awarded first place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation project. She attends the duPont Manual High School, Louisville, Kentucky, U.S.A.|-id=546|

text: 26546 Arulmani

text: ||  || 26546 Arulmani Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Dheevesh Arulmani (b. 1995) was awarded second place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation project. He attends the Gordon Graydon Memorial Secondary School, Mississauga, Ontario, Canada.|-id=548|

text: 26548 Joykutty

text: ||  || 26548 Joykutty Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Anna Maria Joykutty (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation project. She attends the American Heritage School, Plantation, Florida, U.S.A.|-id=549|

text: 26549 Tankanran

text: ||  || 26549 Tankanran Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tan Kan-Ran (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation team project. He attends the Beijing No. 4 High School, Beijing, China.|-id=551|

text: 26551 Shenliangbo

text: ||  || 26551 Shenliangbo Discovered 2000 Feb. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shen Liang-Bo (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his energy-and-transportation team project. He attends the Beijing No. 4 High School, Beijing, China.|-id=557|

text: 26557 Aakritijain

text: ||  || 26557 Aakritijain Discovered 2000 Feb. 28 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Aakriti Jain (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation team project. She attends the Lynbrook High School, San Jose, California, U.S.A.|-id=559|

text: 26559 Chengcheng

text: ||  || 26559 Chengcheng Discovered 2000 Mar. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Cheng Cheng (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her energy-and-transportation team project. She attends the Lynbrook High School, San Jose, California, U.S.A.|-id=575|

text: 26575 Andreapugh

text: ||  || 26575 Andreapugh Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Andrea Aleah Pugh (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for her environmental-science project. She attends the Saginaw Arts and Sciences Academy, Saginaw, Michigan, U.S.A.|-id=578|

text: 26578 Cellinekim

text: ||  || 26578 Cellinekim Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Celline Kim (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her environmental-science project. She attends the Manhasset High School, Manhasset, New York, U.S.A.|-id=586|

text: 26586 Harshaw

text: ||  || 26586 Harshaw Discovered 2000 Mar. 10 by R. Hill at the Catalina Sky Survey. Richard Harshaw (b. 1951) is an Arizona amateur astronomer who makes measurements of double stars. He has served in numerous official positions with astronomy clubs.|-id=591|

text: 26591 Robertreeves

text: ||  || 26591 Robertreeves Discovered 2000 Mar. 2 by R. Hill at the Catalina Sky Survey. Robert Reeves (b. 1946) is the author of several books on digital astronomical imaging and of numerous popular articles on various topics in astronomy and space science.|-id=592|

text: 26592 Maryrenfro

text: ||  || Mary Renfro Reeves (born 1957) is a physical therapist in

text: San Antonio, Texas

text: 26593 Perrypat

text: ||  || Perry Remaklus (b. 1939) and Patricia Remaklus (b. 1941), the founders, owners, and operators of the Willmann-Bell astronomy book publishing firm and long-time members of the Springfield Telescope Makers. |}

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answers: NDQ_003821

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

answers: NDQ_003830

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answers: Near-Earth Asteroid Research Team at Socorro.

answers: NDQ_003822

answers: Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro.

answers: NDQ_003823

answers: || || 26505 Mikelin

answers: NDQ_003824

answers: || || 26507 Mike

answers: NDQ_003825

answers: Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro.

answers: NDQ_003826

answers: || || 26507 Mikelin

answers: NDQ_003827

answers: Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Olexandr Tokarev was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the Chemical Ecological Lyceum, Dnipropetrovsk, Ukraine.

answers: NDQ_003828

answers: |-id=507| 26507 Mikelin

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct.

answers: NDQ_003830

answers: 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Olexandr Tokarev (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his environomental-management project. He attends the Chemical Ecological Lyceum, Dnipropetrovsk, Ukraine.

text: , the steadily growing number of known Apollo asteroids has reached a total of 8,180 members. It is by far the largest group of near-Earth objects, compared to the Aten, Amor and Atira asteroids. Currently, there are 1,133 numbered Apollos. Asteroids are not numbered until they have been observed at two or more oppositions. There are also 1,472 Apollo asteroids large enough, and may get close enough to Earth to be known as potentially hazardous asteroids.

text: , the steadily growing number of known Apollo asteroids has reached a total of 8,180 members. It is by far the largest group of

text: near-Earth object

text: s, compared to the

text: Aten

text: Amor

text: and

text: Atira

text: asteroids. Currently, there are 1,133

text: numbered

text: Apollos. Asteroids are not numbered until they have been observed at two or more

text: oppositions

text: . There are also 1,472 Apollo asteroids large enough, and may get close enough to Earth to be known as

text: potentially hazardous asteroids

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answers: large enough

answers: NDQ_003822

answers: Near-Earth objects

answers: NDQ_003823

answers: Asteroids are not numbered until they have been observed at two or more oppositions

answers: NDQ_003824

answers: Asteroids are not numbered until they have been observed

answers: NDQ_003825

answers: Near-Earth objects

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answers: near-Earth

answers: NDQ_003827

answers: potentially hazardous

answers: NDQ_003828

answers: The steadily growing number of known Apollo asteroids

answers: NDQ_003829

answers: 1,472 Apollo asteroids large enough

answers: NDQ_003830

answers: potentially hazardous

text: Observations show that asteroids larger than 125 km in diameter have rotation rates that follow a Maxwellian frequency distribution, while smaller asteroids (in the 50 to 125 km size range) show a small excess of fast rotators. The smallest asteroids (size less than 50 km) show a clear excess of very fast and slow rotators, and this becomes even more pronounced as smaller populations are measured. These results suggest that one or more size-dependent mechanisms are depopulating the centre of the spin rate distribution in favour of the extremes. The YORP effect is a prime candidate. It is not capable of significantly modifying the spin rates of large asteroids by itself, so a different explanation must be sought for objects such as 253 Mathilde.

text: Observations show that asteroids larger than 125 km in diameter have rotation rates that follow a

text: Maxwellian frequency distribution

text: , while smaller asteroids (in the 50 to 125 km size range) show a small excess of fast rotators. The smallest asteroids (size less than 50 km) show a clear excess of very fast and slow rotators, and this becomes even more pronounced as smaller populations are measured. These results suggest that one or more size-dependent mechanisms are depopulating the centre of the spin rate distribution in favour of the extremes. The YORP effect is a prime candidate. It is not capable of significantly modifying the spin rates of large asteroids by itself, so a different explanation must be sought for objects such as

text: 253 Mathilde

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text: Originally planned for 2017, then 2020,<ref name='steps 2015'/> the mission was recently pushed to December 2021 within a constant budget cap of $1.25 billion. The launch vehicle could be either a Delta IV Heavy, SLS or Falcon Heavy. The boulder should arrive in lunar orbit by late 2025. If the Asteroid Redirect Mission and the Space Launch System or an equivalent heavy launch vehicle are both completed on schedule, a crewed mission to the asteroid brought to lunar orbit could be launched in late 2026.

text: Originally planned for 2017, then 2020,<ref name='steps 2015'/> the mission was recently pushed to December 2021 within a constant budget cap of $1.25 billion. The launch vehicle could be either a

text: Delta IV Heavy

text: SLS

text: or

text: Falcon Heavy

text: . The boulder should arrive in lunar orbit by late 2025. If the Asteroid Redirect Mission and the

text: Space Launch System

text: or an equivalent heavy launch vehicle are both completed on schedule, a crewed mission to the asteroid brought to lunar orbit could be launched in late 2026.

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answers: NDQ_003822

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answers: NDQ_003823

answers: Asteroids do not have craters

answers: NDQ_003824

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answers: NDQ_003828

answers: The boulder should arrive in lunar orbit

answers: NDQ_003829

answers: It could cause humans to go extinct

answers: NDQ_003830

answers: lunar orbit

text: The title on the game's cover art is Phantom of the Asteroids, but the loading screen says Phantoms of the Asteroid, while the title screen says Phantom of the Asteroid. Sources variously use all three titles to refer to the game.

text: The title on the game's

text: cover art

text: is Phantom of the Asteroids, but the loading screen says Phantoms of the Asteroid, while the

text: title screen

text: says Phantom of the Asteroid. Sources variously use all three titles to refer to the game.

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answers: Asteroids

answers: NDQ_003822

answers: Phantom of the Asteroid

answers: NDQ_003823

answers: It's impossible to say

answers: NDQ_003824

answers: Asteroids

answers: NDQ_003825

answers: Phantom of the Asteroid

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answers: Asteroid Belt

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answers: Asteroids

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answers: Phantom of the Asteroid

answers: NDQ_003830

answers: Asteroids

text: In 1981, a proposal for an asteroid mission was submitted to the European Space Agency (ESA). Named the Asteroidal Gravity Optical and Radar Analysis (AGORA), this spacecraft was to launch some time in 1990–1994 and perform two flybys of large asteroids. The preferred target for this mission was Vesta. AGORA would reach the asteroid belt either by a gravitational slingshot trajectory past Mars or by means of a small ion engine. However, the proposal was refused by the ESA. A joint NASA–ESA asteroid mission was then drawn up for a Multiple Asteroid Orbiter with Solar Electric Propulsion (MAOSEP), with one of the mission profiles including an orbit of Vesta. NASA indicated they were not interested in an asteroid mission. Instead, the ESA set up a technological study of a spacecraft with an ion drive. Other missions to the asteroid belt were proposed in the 1980s by France, Germany, Italy and the United States, but none were approved. Exploration of Vesta by fly-by and impacting penetrator was the second main target of the first plan of the multi-aimed Soviet Vesta mission, developed in cooperation with European countries for realisation in 1991–1994 but canceled due to the Soviet Union disbanding.

text: In 1981, a proposal for an asteroid mission was submitted to the

text: European Space Agency

text: (ESA). Named the Asteroidal Gravity Optical and Radar Analysis (AGORA), this

text: spacecraft

text: was to launch some time in 1990–1994 and perform two flybys of large asteroids. The preferred target for this mission was Vesta. AGORA would reach the asteroid belt either by a

text: gravitational slingshot

text: trajectory past Mars or by means of a small

text: ion engine

text: . However, the proposal was refused by the ESA. A joint

text: NASA

text: –ESA asteroid mission was then drawn up for a Multiple Asteroid Orbiter with Solar Electric Propulsion (MAOSEP), with one of the mission profiles including an orbit of Vesta. NASA indicated they were not interested in an asteroid mission. Instead, the ESA set up a technological study of a spacecraft with an ion drive. Other missions to the asteroid belt were proposed in the 1980s by France, Germany, Italy and the United States, but none were approved. Exploration of Vesta by fly-by and

text: impacting penetrator

text: was the second main target of the first plan of the multi-aimed Soviet

text: Vesta mission

text: , developed in cooperation with European countries for realisation in 1991–1994 but canceled due to the Soviet Union disbanding.

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answers: large

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answers: Vesta

answers: NDQ_003823

answers: The preferred target for this mission was Vesta

answers: NDQ_003824

answers: The proposal was refused by the ESA

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answers: Vesta

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answers: asteroid belt

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answers: flybys

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answers: Vesta

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answers: The preferred target for this mission was Vesta

answers: NDQ_003830

answers: Explorer of Vesta

text: The asteroid exploration mission by the Institute of Space and Astronautical Science (ISAS) originated in 1986–1987 when the scientists investigated the feasibility of a sample return mission to Anteros and concluded that the technology was not yet developed. Between 1987 and 1994, joint ISAS / NASA group studied several missions: an asteroid rendezvous mission later became NEAR, and a comet sample return mission later became Stardust.

text: The asteroid exploration mission by the

entity_name: Institute of Space and Astronautical Science

text: Institute of Space and Astronautical Science

text: (ISAS) originated in 1986–1987 when the scientists investigated the feasibility of a sample return mission to

text: Anteros

text: and concluded that the technology was not yet developed. Between 1987 and 1994, joint ISAS / NASA group studied several missions: an asteroid rendezvous mission later became

text: NEAR

text: , and a comet sample return mission later became

text: Stardust

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answers: exploration

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answers: Asteroids do not have craters

answers: NDQ_003824

answers: The asteroid exploration mission

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answers: NDQ_003827

answers: rendezvous

answers: NDQ_003828

answers: The asteroid exploration mission

answers: NDQ_003829

answers: The asteroid exploration mission

answers: NDQ_003830

answers: sample return missions

text: Pallas, minor-planet designation 2 Pallas, is the second asteroid to have been discovered (after Ceres), and it is one of the largest asteroids in the Solar System. With an estimated 7% of the mass of the asteroid belt, it is the third-most-massive asteroid, being 10–30% less massive than Vesta. It is  in diameter, somewhat smaller than Vesta. It is likely a remnant protoplanet.

text: Pallas,

text: minor-planet designation

text: 2 Pallas, is the second

text: asteroid

text: to have been discovered (after

text: Ceres

text: ), and it is one of the

text: largest asteroids

text: in the

text: Solar System

text: . With an estimated 7% of the mass of the

text: asteroid belt

text: , it is the third-most-massive asteroid, being 10–30% less massive than

text: Vesta

text: . It is  in diameter, somewhat smaller than Vesta. It is likely a remnant

text: protoplanet

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answers: It is likely a remnant protoplanet

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answers: the Solar System

text: On 3 May 1996 the asteroid 5757 Tichá was named in her honour (M.P.C. 27128), while she named her discovery, the main-belt asteroid 8307 Peltan, after several members of her family.

text: On 3 May 1996 the asteroid

text: 5757 Tichá

text: was named in her honour (

text: M.P.C.

text: 27128), while she named her discovery, the main-belt asteroid

text: 8307 Peltan

text: , after several members of her family.

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text: |-id=211| 121211 Nikeshadavis ||  || Nikesha Davis (b. 1983) is the deputy lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission. Prior to serving in this role, she worked as an Attitude Control Analyst on the Global Precipitation Measurement Mission and the proposal team for the GEDI Mission.|-id=232| 121232 Zerin ||  || ZERIN (Zentrum für Rieskrater- und Impaktforschung Nördlingen, "Center for Ries Crater and Impact Studies Nördlingen"), a scientific institute for impact research and, in particular, documentation of the Nördlinger Ries Crater |-id=236| 121236 Adrianagutierrez ||  || Adriana Manrique Gutierrez (b. 1986) is an Animator at NASA Goddard's Conceptual Image Lab. She is part of the production team working on a series of animated films for the OSIRIS-REx Asteroid Sample Return Mission.|-id=237| 121237 Zachdolch ||  || Zachary Dolch (b. 1984), a planner/scheduler for the OSIRIS-REx Asteroid Sample Return Mission. |}

text: 121211 Nikeshadavis

text: ||  || Nikesha Davis (b. 1983) is the deputy lead NASA Attitude Control Analyst for the OSIRIS-REx Asteroid Sample Return Mission. Prior to serving in this role, she worked as an Attitude Control Analyst on the Global Precipitation Measurement Mission and the proposal team for the GEDI Mission.|-id=232|

text: 121232 Zerin

text: ZERIN

text: (Zentrum für Rieskrater- und Impaktforschung Nördlingen, "Center for Ries Crater and Impact Studies Nördlingen"), a scientific institute for impact research and, in particular, documentation of the

text: Nördlinger Ries Crater

text: 121236 Adrianagutierrez

text: ||  || Adriana Manrique Gutierrez (b. 1986) is an Animator at NASA Goddard's Conceptual Image Lab. She is part of the production team working on a series of animated films for the OSIRIS-REx Asteroid Sample Return Mission.|-id=237|

text: 121237 Zachdolch

text: ||  || Zachary Dolch (b. 1984), a planner/scheduler for the OSIRIS-REx Asteroid Sample Return Mission. |}

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text: |-id=026| 129026 Conormcmenamin ||  || Conor Brendan McMenamin (b. 1989) is a student engineer at the Massachusetts Institute of Technology working as the Thermal Engineer guiding the design and stable temperature performance of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=050| 129050 Lowellcogburn ||  || Lowell Cogburn (b. 1955) is the OSIRIS REx spacecraft lead dynamics analyst responsible for Touch and Go dynamic analysis and Sample Return Capsule release dynamic analysis. He was the Dynamics lead on the GRAIL lunar mission. |-id=051| 129051 Chrismay ||  || Chris May (b. 1972) is the Thermal Lead for the OSIRIS-REx spacecraft. He was the Thermal Lead for the GRAIL lunar mission and thermal engineer on the Mars Phoenix lander, Mars Reconnaissance Orbiter and Mars Odyssey missions. |-id=052| 129052 Nîmeshdave ||  || Nîmesh Dave (b. 1972) is the OSIRIS-REx spacecraft structures Certified Principal Engineer (CPE). He was the structures CPE on the GRAIL lunar mission, and mechanical design engineer on ORION and MSL Aeroshell. |-id=053| 129053 Derekshannon ||  || Derek Shannon (b. 1976) is the OSIRIS-REx spacecraft Mechanical Analysis Lead and mechanical Certified Test Conductor. He held the same role on the GRAIL misson, and was a stress analyst on Juno and MSL Aeroshell. |-id=060| 129060 Huntskretsch ||  || Hunts Kretsch (b. 1957) is the OSIRIS-REx Sample Return Capsule (SRC) Certified Principal Engineer. |-id=061| 129061 Karlfortney ||  || Karl Fortney (b. 1962) is the OSIRIS-REx spacecraft Mechanisms Certified Principal Engineer. He was a mechanical engineer on the MAVEN and Juno missions as well as the MSL Aeroshell. |-id=063| 129063 Joshwood ||  || Josh Wood (b. 1977) is the flight system System Design Lead and CPE at Lockheed Martin for the OSIRIS-REx Asteroid Sample Return Mission. He was also Systems/ Electrical/Payload Accommodations Engineer for the GRAIL program, and the STL lead for the Phoenix Mars Lander. |-id=064| 129064 Jeanneladewig ||  || Jeanne Ladewig (b. 1957) is the flight system Payload Accommodation Lead Engineer and the TAGCAMS CPE at Lockheed Martin for the OSIRIS-REx Mission and the Payload Accommodation Lead Engineer on the Juno and Phoenix missions. She has multi-mission experience working payloads on NASA interplanetary missions. |-id=068| 129068 Alexmay ||  || Alex May (b. 1981) is the flight system Touch-And-Go Mission Phase Lead at Lockheed Martin for the OSIRIS-REx Mission. Alex has worked on a number of missions and research programs developing proximity operations technologies within System Engineering and Guidance, Navigation and Control teams. |-id=071| 129071 Catriegle ||  || Cat Riegle (b. 1976) is the flight system Contamination Control Lead at Lockheed Martin for the OSIRIS-REx Mission. She has supported multiple NASA interplanetary missions helping to ensure that contamination control and planetary protection requirements are met. |-id=073| 129073 Sandyfreund ||  || Sandy Freund (b. 1979) is the flight system Fault Protection Lead and Launch and SRC Release Mission Phase lead at Lockheed Martin on the OSIRIS-REx Mission. She was the fault protection lead on MAVEN and was a mission operations development lead on the Phoenix Mission's EDL critical mission phase. |-id=078| 129078 Animoo ||  || Animoo, title of artistic work by Laurent "Lillo" Steidle, Swiss geologist and painter |-id=082| 129082 Oliviabillett ||  || Olivia Billett (b. 1980) is the flight system Lead Software Systems Engineer, Science Mission Phase lead and flight system CPE delegate at Lockheed Martin on the OSIRIS-REx mission. She previously served as the SSE on the MAVEN mission, and supported multiple interplanetary missions within Mission Operations. |-id=092| 129092 Snowdonia ||  || Snowdon, the highest peak in Wales |-id=095| 129095 Martyschmitzer ||  || Martin Schmitzer (b. 1970) is the RF Subsystem Lead for the OSIRIS-REx Asteroid Sample Return Mission. He served as the RF lead for the GRAIL mission, MRO and Odyssey Mars missions, and Spitzer Space Telescope and was a team member on the Stardust comet sample return mission and 1998 Mars Surveyor Program. |-id=096| 129096 Andrewleung ||  || Andrew Leung (b. 1986) is the EPS ATLO Lead for the OSIRIS-REx Asteroid Sample Return Mission. Prior to serving in this role, he was the PDDU CPE delegate, SASM and BCM Card Lead for OSIRIS-REx, and a card level electronics engineer for the ISIS airship program. |-id=099| 129099 Spoelhof ||  || William Spoelhof, American president of Calvin College † |-id=100| 129100 Aaronammons ||  || Aaron Ammons (b. 1970) is the Command And Data Handling (C&DH) Certified Principal Engineer Lead for the OSIRIS-REx Asteroid Sample Return Mission. He was a team member to the Advanced Programs Low Power Avionics study and on the C&DH team for the GRAIL mission. |}

text: 129026 Conormcmenamin

text: ||  || Conor Brendan McMenamin (b. 1989) is a student engineer at the Massachusetts Institute of Technology working as the Thermal Engineer guiding the design and stable temperature performance of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=050|

text: 129050 Lowellcogburn

text: ||  || Lowell Cogburn (b. 1955) is the OSIRIS REx spacecraft lead dynamics analyst responsible for Touch and Go dynamic analysis and Sample Return Capsule release dynamic analysis. He was the Dynamics lead on the GRAIL lunar mission. |-id=051|

text: 129051 Chrismay

text: ||  || Chris May (b. 1972) is the Thermal Lead for the OSIRIS-REx spacecraft. He was the Thermal Lead for the GRAIL lunar mission and thermal engineer on the Mars Phoenix lander, Mars Reconnaissance Orbiter and Mars Odyssey missions. |-id=052|

text: 129052 Nîmeshdave

text: ||  || Nîmesh Dave (b. 1972) is the OSIRIS-REx spacecraft structures Certified Principal Engineer (CPE). He was the structures CPE on the GRAIL lunar mission, and mechanical design engineer on ORION and MSL Aeroshell. |-id=053|

text: 129053 Derekshannon

text: ||  || Derek Shannon (b. 1976) is the OSIRIS-REx spacecraft Mechanical Analysis Lead and mechanical Certified Test Conductor. He held the same role on the GRAIL misson, and was a stress analyst on Juno and MSL Aeroshell. |-id=060|

text: 129060 Huntskretsch

text: ||  || Hunts Kretsch (b. 1957) is the OSIRIS-REx Sample Return Capsule (SRC) Certified Principal Engineer. |-id=061|

text: 129061 Karlfortney

text: ||  || Karl Fortney (b. 1962) is the OSIRIS-REx spacecraft Mechanisms Certified Principal Engineer. He was a mechanical engineer on the MAVEN and Juno missions as well as the MSL Aeroshell. |-id=063|

text: 129063 Joshwood

text: ||  || Josh Wood (b. 1977) is the flight system System Design Lead and CPE at Lockheed Martin for the OSIRIS-REx Asteroid Sample Return Mission. He was also Systems/ Electrical/Payload Accommodations Engineer for the GRAIL program, and the STL lead for the Phoenix Mars Lander. |-id=064|

text: 129064 Jeanneladewig

text: ||  || Jeanne Ladewig (b. 1957) is the flight system Payload Accommodation Lead Engineer and the TAGCAMS CPE at Lockheed Martin for the OSIRIS-REx Mission and the Payload Accommodation Lead Engineer on the Juno and Phoenix missions. She has multi-mission experience working payloads on NASA interplanetary missions. |-id=068|

text: 129068 Alexmay

text: ||  || Alex May (b. 1981) is the flight system Touch-And-Go Mission Phase Lead at Lockheed Martin for the OSIRIS-REx Mission. Alex has worked on a number of missions and research programs developing proximity operations technologies within System Engineering and Guidance, Navigation and Control teams. |-id=071|

text: 129071 Catriegle

text: ||  || Cat Riegle (b. 1976) is the flight system Contamination Control Lead at Lockheed Martin for the OSIRIS-REx Mission. She has supported multiple NASA interplanetary missions helping to ensure that contamination control and planetary protection requirements are met. |-id=073|

text: 129073 Sandyfreund

text: ||  || Sandy Freund (b. 1979) is the flight system Fault Protection Lead and Launch and SRC Release Mission Phase lead at Lockheed Martin on the OSIRIS-REx Mission. She was the fault protection lead on MAVEN and was a mission operations development lead on the Phoenix Mission's EDL critical mission phase. |-id=078|

text: 129078 Animoo

text: ||  || Animoo, title of artistic work by Laurent "Lillo" Steidle, Swiss geologist and painter |-id=082|

text: 129082 Oliviabillett

text: ||  || Olivia Billett (b. 1980) is the flight system Lead Software Systems Engineer, Science Mission Phase lead and flight system CPE delegate at Lockheed Martin on the OSIRIS-REx mission. She previously served as the SSE on the MAVEN mission, and supported multiple interplanetary missions within Mission Operations. |-id=092|

text: 129092 Snowdonia

text: Snowdon

text: , the highest peak in Wales |-id=095|

text: 129095 Martyschmitzer

text: ||  || Martin Schmitzer (b. 1970) is the RF Subsystem Lead for the OSIRIS-REx Asteroid Sample Return Mission. He served as the RF lead for the GRAIL mission, MRO and Odyssey Mars missions, and Spitzer Space Telescope and was a team member on the Stardust comet sample return mission and 1998 Mars Surveyor Program. |-id=096|

text: 129096 Andrewleung

text: ||  || Andrew Leung (b. 1986) is the EPS ATLO Lead for the OSIRIS-REx Asteroid Sample Return Mission. Prior to serving in this role, he was the PDDU CPE delegate, SASM and BCM Card Lead for OSIRIS-REx, and a card level electronics engineer for the ISIS airship program. |-id=099|

text: 129099 Spoelhof

text: William Spoelhof

text: , American president of

text: Calvin College

text: † |-id=100|

text: 129100 Aaronammons

text: ||  || Aaron Ammons (b. 1970) is the Command And Data Handling (C&DH) Certified Principal Engineer Lead for the OSIRIS-REx Asteroid Sample Return Mission. He was a team member to the Advanced Programs Low Power Avionics study and on the C&DH team for the GRAIL mission. |}

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answers: NDQ_003821

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answers: NDQ_003822

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answers: NDQ_003823

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answers: NDQ_003824

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answers: NDQ_003825

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answers: NDQ_003826

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answers: NDQ_003827

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

answers: NDQ_003828

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answers: NDQ_003829

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answers: NDQ_003821

answers: X-ray Imaging Spectrometer aboard the OSIRIS-REx Sample Return Mission

answers: NDQ_003822

answers: The OSIRIS-REx Asteroid Sample Return Mission is part of the OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003823

answers: ) is the OSIRIS-REx Sample Return Capsule (SRC) Certified Principal Engineer.

answers: NDQ_003824

answers: Despite the fact that asteroids are too small for a manned mission to visit them, they're still a mystery because they're too far away from Earth.

answers: NDQ_003825

answers: The OSIRIS-REx Asteroid Sample Return Mission is part of the OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003826

answers: 1957) is the OSIRIS-REx Sample Return Capsule (SRC) Certified Principal Engineer.

answers: NDQ_003827

answers: X-ray Imaging Spectrometer

answers: NDQ_003828

answers: 1978) is the OSIRIS-REx Sample Return Capsule (SRC) Certified Principal Engineer.

answers: NDQ_003829

answers: x Sample Return Capsule (SRC) Certified Principal Engineer.

answers: NDQ_003830

answers: X-ray Imaging Spectrometer aboard the OSIRIS-REx sample return mission.

text: , 15,448 NEOs have been discovered: 106 near-Earth comets and 15,342 near-Earth asteroids. Of those there are 1,120 Aten asteroids, 5,903 Amor asteroids, and 8,303 Apollo asteroids. There are 1,756 NEOs that are classified as potentially hazardous asteroids (PHAs). Currently, 157 known PHAs and 874 known NEAs have an absolute magnitude of 17.75 or brighter, which roughly corresponds to at least 1 km in size; and 7,441 known NEAs are larger than about 140 meters in size.

text: , 15,448 NEOs have been discovered: 106 near-Earth comets and 15,342 near-Earth asteroids. Of those there are 1,120

text: Aten asteroid

text: s, 5,903

text: Amor asteroid

text: s, and 8,303

text: Apollo asteroid

text: s. There are 1,756 NEOs that are classified as

text: potentially hazardous asteroid

text: s (PHAs). Currently, 157 known PHAs and 874 known NEAs have an

text: absolute magnitude

text: of 17.75 or brighter, which roughly corresponds to at least 1

text: km

text: in size; and 7,441 known NEAs are larger than about 140 meters in size.

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answers: NEOs

answers: NDQ_003822

answers: 15,342 near-Earth

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 15342 near-Earth asteroids

answers: NDQ_003825

answers: 15,342 near-Earth

answers: NDQ_003826

answers: NEOs

answers: NDQ_003827

answers: potentially hazardous asteroids

answers: NDQ_003828

answers: 15,342 near-Earth asteroids

answers: NDQ_003829

answers: NEOs that are classified as potentially hazardous asteroids

answers: NDQ_003830

answers: NEOs

text: An early system of asteroid taxonomy was established in 1975 from the doctoral thesis work of David J. Tholen. This was based upon observations of a group of 110 asteroids. The U-type classification was used as a miscellaneous class for asteroids with unusual spectra that didn't fit into the C and S-type asteroid classifications. In 1976, some of these U-type asteroids with unusual moderate albedo levels were labeled as M-type.

text: An early system of asteroid taxonomy was established in 1975 from the

text: doctoral thesis

text: work of

text: David J. Tholen

text: . This was based upon observations of a group of 110 asteroids. The U-type classification was used as a miscellaneous class for asteroids with unusual spectra that didn't fit into the

text: C

text: and

text: S-type asteroid

text: classifications. In 1976, some of these U-type asteroids with unusual moderate

text: albedo

text: levels were labeled as

text: M-type

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answers: asteroids

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answers: taxonomy

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroid taxonomy

answers: NDQ_003825

answers: taxonomy

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: U-type

answers: NDQ_003828

answers: Mars

answers: NDQ_003829

answers: This was based upon observations of a group of 110 asteroids

answers: NDQ_003830

answers: taxonomy

text: 38 Leda  is a large, dark main-belt asteroid that was discovered by French astronomer J. Chacornac on January 12, 1856, and named after Leda, the mother of Helen of Troy in Greek mythology. In the Tholen classification system, it is categorized as a carbonaceous C-type asteroid, while the Bus asteroid taxonomy system lists it as a Cgh asteroid.

text: 38 Leda  is a large, dark

text: main-belt

text: asteroid

text: that was discovered by French astronomer

text: J. Chacornac

text: on January 12, 1856, and named after

text: Leda

text: , the mother of

text: Helen of Troy

text: in

text: Greek mythology

text: . In the

text: Tholen classification

text: system, it is categorized as a carbonaceous

text: C-type asteroid

text: , while the Bus

text: asteroid taxonomy

text: system lists it as a Cgh asteroid.

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answers: NDQ_003821

answers: astronomer

answers: NDQ_003822

answers: Cgh asteroid

answers: NDQ_003823

answers: It does not have craters.

answers: NDQ_003824

answers: asteroids are too small for nasa missions

answers: NDQ_003825

answers: Cgh asteroid

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: name after Leda

answers: NDQ_003828

answers: 38 Leda

answers: NDQ_003829

answers: 38 Leda

answers: NDQ_003830

answers: astronomers

text: Spacecraft visits to minor planets have mostly been flybys, and have ranged from dedicated missions to incidental flybys and targets of opportunity for spacecraft that have already completed their missions. The first spacecraft to visit an asteroid was Galileo, which flew past 951 Gaspra in October 1991; an incidental encounter while the probe was en route to Jupiter. The first dedicated mission was NEAR Shoemaker, which was launched in February 1996, and entered orbit around 433 Eros in February 2000, having first flown past 253 Mathilde. NEAR was also the first spacecraft to land on an asteroid, surviving what was intended to be an impact with Eros at 20:01 on 12 February 2001 at the planned end of its mission. As a result of its unexpected survival, the spacecraft's mission was extended until 1 March to allow data to be collected from the surface.

text: Spacecraft visits to minor planets have mostly been flybys, and have ranged from dedicated missions to incidental flybys and targets of opportunity for spacecraft that have already completed their missions. The first spacecraft to visit an asteroid was

text: Galileo

text: , which flew past

text: 951 Gaspra

text: in October 1991; an incidental encounter while the probe was en route to

text: Jupiter

text: . The first dedicated mission was

text: NEAR Shoemaker

text: , which was launched in February 1996, and entered orbit around

text: 433 Eros

text: in February 2000, having first flown past

text: 253 Mathilde

text: . NEAR was also the first spacecraft to land on an asteroid, surviving what was intended to be an impact with Eros at 20:01 on 12 February 2001 at the planned end of its mission. As a result of its unexpected survival, the spacecraft's mission was extended until 1 March to allow data to be collected from the surface.

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answers: minor planets

answers: NDQ_003822

answers: minor planets

answers: NDQ_003823

answers: The first spacecraft to visit an asteroid

answers: NDQ_003824

answers: Spacecraft visits to minor planets

answers: NDQ_003825

answers: minor planets

answers: NDQ_003826

answers: minor planets

answers: NDQ_003827

answers: flybys

answers: NDQ_003828

answers: The first spacecraft to visit an asteroid

answers: NDQ_003829

answers: As a result of its unexpected survival

answers: NDQ_003830

answers: minor planets

text: The combination of this fine asteroid dust, as well as ejected cometary material, produces the zodiacal light. This faint auroral glow can be viewed at night extending from the direction of the Sun along the plane of the ecliptic. Asteroid particles that produce the visible zodiacal light average about 40 μm in radius. The typical lifetimes of main-belt zodiacal cloud particles are about 700,000 years. Thus, to maintain the bands of dust, new particles must be steadily produced within the asteroid belt. It was once thought that collisions of asteroids form a major component of the zodiacal light.  However, computer simulations by Nesvorný and colleagues attributed 85 percent of the zodiacal-light dust to fragmentations of Jupiter-family comets, rather than to comets and collisions between asteroids in the asteroid belt. At most 10 percent of the dust is attributed to the asteroid belt.

text: The combination of this fine asteroid dust, as well as ejected cometary material, produces the

text: zodiacal light

text: . This faint auroral glow can be viewed at night extending from the direction of the

text: Sun

text: along the plane of the

text: ecliptic

text: . Asteroid particles that produce the visible zodiacal light average about 40 μm in radius. The typical lifetimes of main-belt zodiacal cloud particles are about 700,000 years. Thus, to maintain the bands of dust, new particles must be steadily produced within the asteroid belt. It was once thought that collisions of asteroids form a major component of the

text: zodiacal light

text: .  However, computer simulations by Nesvorný and colleagues attributed 85 percent of the zodiacal-light dust to fragmentations of Jupiter-family comets, rather than to comets and collisions between asteroids in the asteroid belt. At most 10 percent of the dust is attributed to the asteroid belt.

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answers: dust

answers: NDQ_003822

answers: dust

answers: NDQ_003823

answers: It was once thought that collisions of asteroids form a major component

answers: NDQ_003824

answers: It was once thought that collisions of asteroids form a major component

answers: NDQ_003825

answers: dust

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: collide

answers: NDQ_003828

answers: Jupiter-family comets

answers: NDQ_003829

answers: The typical lifetimes of main-belt zodiacal cloud particles are about 700,000 years

answers: NDQ_003830

answers: Zodiacal light

text: An asteroid with an Earth-crossing orbit is not necessarily in danger of colliding with Earth. The orbit of an Earth-crossing asteroid may not even intersect with that of Earth. This apparent contradiction arises because many asteroids have highly inclined orbits, so although they may have a perihelion less than that of Earth, their paths can never cross. An asteroid for which there is some possibility of a collision with Earth at a future date and which is above a certain size is classified as a potentially hazardous asteroid (PHA). Specifically, an asteroid is a PHA if its Earth minimum orbital intersection distance (MOID) is <0.05 AU and its absolute magnitude is 22 or less. The concept of PHA is intended to replace the now abandoned strict definition of ECA (Earth-crossing asteroid) which existed for a few years. Determining if an asteroid was an ECA required calculation of its orbits millennia into the future, including planetary gravitational perturbations, to assess whether a collision with Earth was possible and this has proved to be impractical.

text: An asteroid with an Earth-crossing orbit is not necessarily in danger of colliding with Earth. The orbit of an Earth-crossing asteroid may not even intersect with that of Earth. This apparent contradiction arises because many asteroids have highly inclined orbits, so although they may have a

text: perihelion

text: less than that of Earth, their paths can never cross. An asteroid for which there is some possibility of a collision with Earth at a future date and which is above a certain size is classified as a

text: potentially hazardous asteroid

text: (PHA). Specifically, an asteroid is a PHA if its Earth

text: minimum orbital intersection distance

text: (MOID) is <0.05

text: AU

text: and its

text: absolute magnitude

text: is 22 or less. The concept of PHA is intended to replace the now abandoned strict definition of ECA (Earth-crossing asteroid) which existed for a few years. Determining if an asteroid was an ECA required calculation of its orbits millennia into the future, including planetary gravitational perturbations, to assess whether a collision with Earth was possible and this has proved to be impractical.

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answers: NDQ_003821

answers: Earth-crossing asteroid

answers: NDQ_003822

answers: Earth-crossing asteroid

answers: NDQ_003823

answers: The orbit of an Earth-crossing asteroid may not even intersect with that of Earth

answers: NDQ_003824

answers: An asteroid with an Earth-crossing orbit is not necessarily in danger of colliding with Earth

answers: NDQ_003825

answers: Earth-crossing asteroid

answers: NDQ_003826

answers: Earth-crossing

answers: NDQ_003827

answers: Earth-crossing

answers: NDQ_003828

answers: An asteroid with an Earth-crossing orbit is not necessarily in danger of colliding with Earth

answers: NDQ_003829

answers: This apparent contradiction arises because many asteroids have highly inclined orbits

answers: NDQ_003830

answers: collision with Earth

text: The scientific goals of the VISTA surveys, which started in 2010, include many of the most exciting problems in astrophysics today, ranging from the nature of dark energy to the threat of near-Earth asteroids.

text: The scientific goals of the VISTA surveys, which started in 2010, include many of the most exciting problems in astrophysics today, ranging from the nature of dark energy to the threat of near-Earth asteroids.

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text: For example, there are very few asteroids with semimajor axis near 2.50 AU, period 3.95 years, which would make three orbits for each orbit of Jupiter (hence, called the 3:1 orbital resonance). Other orbital resonances correspond to orbital periods whose lengths are simple fractions of Jupiter's. The weaker resonances lead only to a depletion of asteroids, while spikes in the histogram are often due to the presence of a prominent asteroid family (see List of asteroid families).

text: For example, there are very few asteroids with semimajor axis near 2.50

text: AU

text: , period 3.95 years, which would make three orbits for each orbit of Jupiter (hence, called the 3:1 orbital resonance). Other orbital resonances correspond to orbital periods whose lengths are simple fractions of Jupiter's. The weaker resonances lead only to a depletion of asteroids, while spikes in the histogram are often due to the presence of a prominent

text: asteroid family

text: (see

text: List of asteroid families

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text: EURONEAR, the European Near Earth Asteroids Research, is a research project which aims to develop a research network which will search, discover and monitor near-Earth asteroids (NEAs) and potentially hazardous asteroids (PHAs) using two automated dedicated 1–2 metre telescopes located in both hemispheres and other facilities available to the members of the network. As of 2016, the Minor Planet Center directly credits EURONEAR with the discovery of 8 minor planets in 2008 (see also :Category:Discoveries by EURONEAR).

text: EURONEAR, the European Near Earth Asteroids Research, is a research project which aims to develop a research network which will search, discover and monitor

text: near-Earth asteroid

text: s (NEAs) and

text: potentially hazardous asteroids

text: (PHAs) using two automated dedicated 1–2 metre telescopes located in both hemispheres and other facilities available to the members of the network. As of 2016, the

text: Minor Planet Center

text: directly credits EURONEAR with the discovery of 8 minor planets in 2008 (see also

text: :Category:Discoveries by EURONEAR

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answers: minor planets

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answers: Near-Earth asteroids

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answers: potentially hazardous asteroids

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text: Perhaps the most visually striking and scientifically compelling application of ISAR is in the deep space imaging of asteroids. A particularly beautiful example of this is the so-called "dog's bone" 216 Kleopatra asteroid, which lies roughly 20% further away from the earth than does the sun. The asteroid is only 60 miles wide at its midpoint. Yet the imagery is crisp and "feels" like an optical image. This has been cited as akin to using a Los Angeles telescope the size of the human eye's lens to image a car in New York. Of course the "trick" here is that the asteroid is presented amongst a very sparse background, allowing for substantial disambiguation.

text: Perhaps the most visually striking and scientifically compelling application of ISAR is in the deep space imaging of asteroids. A particularly beautiful example of this is the so-called "dog's bone"

text: 216 Kleopatra

text: asteroid, which lies roughly 20% further away from the earth than does the sun. The asteroid is only 60 miles wide at its midpoint. Yet the imagery is crisp and "feels" like an optical image. This has been cited as akin to using a Los Angeles telescope the size of the human eye's lens to image a car in New York. Of course the "trick" here is that the asteroid is presented amongst a very sparse background, allowing for substantial disambiguation.

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answers: asteroids

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answers: deep space imaging

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answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: Deep space imaging of asteroids

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answers: deep space imaging

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answers: deep space

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answers: NDQ_003828

answers: 216 Kleopatra

answers: NDQ_003829

answers: 216 Kleopatra asteroid

answers: NDQ_003830

answers: deep space imaging

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2013.

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2013.

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

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answers: near-Earth

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answers: near-Earth

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answers: asteroids do not have craters

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answers: near-Earth

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answers: passed more than 1 lunar distance

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answers: 0.00256 AU

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answers: 0.00256 AU

answers: NDQ_003830

answers: near-Earth asteroids

text: 3198 Wallonia (1981 YH1) is a Mars-crossing asteroid discovered on December 30, 1981 by François Dossin at Haute-Provence Observatory. With an absolute magnitude (H) of 13, the asteroid is about ~10 km in diameter. It is one of the largest Mars-crossing asteroids as few Mars-crossing asteroids have an absolute magnitude brighter than 13.

text: 3198 Wallonia (1981 YH1) is a

text: Mars-crossing asteroid

text: discovered on December 30, 1981 by

text: François Dossin

text: at

text: Haute-Provence Observatory

text: . With an

text: absolute magnitude (H)

text: of 13, the asteroid is about ~10 km in diameter. It is one of the largest Mars-crossing asteroids as few Mars-crossing asteroids have an absolute magnitude brighter than 13.

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answers: 3198 Wallonia (1981 YH1)

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text: 204 Kallisto is a fairly typical, although sizeable Main belt asteroid. It is classified as an S-type asteroid. Like other asteroids of its type, it is light in colour.

text: 204 Kallisto is a fairly typical, although sizeable

text: Main belt

text: asteroid

text: . It is classified as an

text: S-type asteroid

text: . Like other asteroids of its type, it is light in colour.

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answers: sizeable

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answers: 204 Kallisto

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answers: 204 Kallisto

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answers: 204 Kallisto

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answers: light in colour

text: 434 Hungaria is a relatively small asteroid orbiting in the inner asteroid belt. It is an E-type (high-albedo) asteroid. It is the namesake of the Hungaria asteroids, which orbit the Sun on the inside of the 1:4 Kirkwood gap, standing out of the core of the asteroid belt.

text: 434 Hungaria is a relatively small

text: asteroid

text: orbiting in the inner

text: asteroid belt

text: . It is an

text: E-type

text: (high-

text: albedo

text: ) asteroid. It is the namesake of the

text: Hungaria asteroids

text: , which orbit the Sun on the inside of the 1:4

text: Kirkwood gap

text: , standing out of the core of the asteroid belt.

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text: In October 2013, the UN committee approved several measures to deal with terrestrial asteroid impacts, including the creation of an International Asteroid Warning Network (IAWN) to act as a clearing house for shared information on dangerous asteroids and for any future terrestrial impact events that are identified. A UN Space Missions Planning Advisory Group will also coordinate joint studies of the technologies for deflection missions, and as well provide oversight of actual missions. This is due to deflection missions typically involving a progressive movement of an asteroid's predicted impact point across the surface of the Earth (and also across the territories of uninvolved countries) until the NEO has been deflected either ahead of, or behind the planet at the point their orbits intersect. Schweickart states that an initial framework of international cooperation at the UN is needed to guide the policy makers of its member nations on several important NEO-related aspects.

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text: His most notable discoveries include the potentially hazardous object and Aten asteroid 3362 Khufu, which he co-discovered with Maria A. Barucci, as well as the near-Earth object, Mars-crosser and Aten asteroid, 3551 Verenia. Together with Eleanor Helin he co-discovered the minor planets 3360 Syrinx, 6065 Chesneau, 6435 Daveross and 7163 Barenboim.

text: His most notable discoveries include the

text: potentially hazardous object

text: and

text: Aten

text: asteroid

text: 3362 Khufu

text: , which he co-discovered with

text: Maria A. Barucci

text: , as well as the

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text: Aten

text: asteroid,

text: 3551 Verenia

text: . Together with

text: Eleanor Helin

text: he co-discovered the minor planets

text: 3360 Syrinx

text: 6065 Chesneau

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text: The Lincoln Laboratory's Experimental Test Site (ETS) is an electro-optical test facility located on the grounds of the White Sands Missile Range in Socorro, New Mexico. The ETS is operated by the laboratory for the Air Force; its principal mission is the development, evaluation, and transfer of advanced electro-optical space surveillance technologies. The ETS has been a contributing sensor to the U.S. Air Force Space Command. A spin-off program for NASA, Lincoln Near-Earth Asteroid Research (LINEAR), uses the ground-based electro-optical deep-space surveillance telescopes at White Sands to discover comets and asteroids, in particular near-Earth objects. A large percentage share of all known minor planets in the Solar System have been discovered through this program. As of 2016, the Minor Planet Center credits LINEAR with the discovery of 147,183 numbered minor planets from 1997 to 2015. In terms of the total number of discoveries, LINEAR is the most successful asteroid survey program ever conducted.

text: The Lincoln Laboratory's Experimental Test Site (ETS) is an electro-optical test facility located on the grounds of the

text: White Sands Missile Range

text: in

text: Socorro

text: New Mexico

text: . The ETS is operated by the laboratory for the Air Force; its principal mission is the development, evaluation, and transfer of advanced electro-optical space surveillance technologies. The ETS has been a contributing sensor to the U.S.

text: Air Force Space Command

text: . A spin-off program for NASA,

text: Lincoln Near-Earth Asteroid Research

text: (LINEAR), uses the ground-based electro-optical deep-space surveillance telescopes at White Sands to discover

text: comet

text: s and

text: asteroid

text: s, in particular

text: near-Earth object

text: s. A large percentage share of all known

text: minor planet

text: s in the Solar System have been discovered through this program. As of 2016, the

text: Minor Planet Center

text: credits LINEAR with the discovery of 147,183 numbered minor planets from 1997 to 2015. In terms of the total number of discoveries, LINEAR is the most successful asteroid

text: survey program

text: ever conducted.

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text: Asteroids can be classified into three major types according to their spectra.  The original categories were created by Clark R. Chapman, David Morrison, and Ben Zellner in 1975, and further expanded by David J. Tholen in 1984. In what is now known as the Tholen classification, the C-types are made of carbonaceous material, S-types consist mainly of silicates, and X-types are 'metallic'.  There are other classifications for unusual asteroids.  C- and S-type asteroids are the most common asteroids. In 2002 the Tholen classification was further "evolved" into the SMASS classification, expanding the number of categories from 14 to 26 to account for more precise spectroscopic analysis of the asteroids.

text: Asteroids can be classified into three major types according to their spectra.  The original categories were created by Clark R. Chapman, David Morrison, and Ben Zellner in 1975, and further expanded by

text: David J. Tholen

text: in 1984. In what is now known as the

text: Tholen classification

text: , the

text: C-types

text: are made of carbonaceous material,

text: S-types

text: consist mainly of

text: silicates

text: , and

text: X-types

text: are 'metallic'.  There are other classifications for unusual asteroids.  C- and S-type asteroids are the most common asteroids. In 2002 the Tholen classification was further "evolved" into the

text: SMASS classification

text: , expanding the number of categories from 14 to 26 to account for more precise spectroscopic analysis of the asteroids.

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answers: made of carbonaceous material

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answers: C- and S-type asteroids

answers: NDQ_003823

answers: Asteroids can be classified into three major types according to their spectra

answers: NDQ_003824

answers: spectroscopic analysis

answers: NDQ_003825

answers: C- and S-type asteroids

answers: NDQ_003826

answers: SMASS

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answers: be classified into three major types

answers: NDQ_003828

answers: In what is now known as the Tholen classification

answers: NDQ_003829

answers: Asteroids can be classified into three major types according to their spectra

answers: NDQ_003830

answers: spectroscopic analysis

text: Another, larger near-Earth asteroid, 2004 FH passed just two weeks prior to .

text: Another, larger near-Earth asteroid,

text: 2004 FH

text: passed just two weeks prior to .

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answers: near-Earth

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answers: asteroid

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answers: near-Earth

text: In 1961, the International Astronomical Union defined a meteoroid as "a solid object moving in interplanetary space, of a size considerably smaller than an asteroid and considerably larger than an atom". In 1995, Beech and Steel, writing in the Quarterly Journal of the Royal Astronomical Society, proposed a new definition where a meteoroid would be between 100 µm and 10 meters across. In 2010, following the discovery of asteroids below 10 m in size, Rubin and Grossman revised the previous definition of meteoroid to objects between 10 µm and 1 m in diameter in order to maintain the distinction. According to Rubin and Grossman, the minimum size of an asteroid is given by what can be discovered from Earth-bound telescopes, so the distinction between meteoroid and asteroid is fuzzy. Some of the smallest asteroids discovered (based on absolute magnitude H) are  with H = 33.2 and  with H = 32.1 both with an estimated size of 1 meter. Objects smaller than meteoroids are classified as micrometeoroids and cosmic dust. The Minor Planet Center does not use the term "meteoroid".

text: In 1961, the

text: International Astronomical Union

text: defined a meteoroid as "a solid object moving in interplanetary space, of a size considerably smaller than an

text: asteroid

text: and considerably larger than an atom". In 1995, Beech and Steel, writing in the

text: Quarterly Journal of the Royal Astronomical Society

text: , proposed a new definition where a meteoroid would be between 100

text: µm

text: and 10 meters across. In 2010, following the discovery of asteroids below 10 m in size, Rubin and Grossman revised the previous definition of meteoroid to objects between 10 µm and 1 m in diameter in order to maintain the distinction. According to Rubin and Grossman, the minimum size of an asteroid is given by what can be discovered from Earth-bound telescopes, so the distinction between meteoroid and asteroid is fuzzy. Some of the smallest asteroids discovered (based on

text: absolute magnitude

text: H) are  with H = 33.2 and  with H = 32.1 both with an estimated size of 1 meter. Objects smaller than meteoroids are classified as

text: micrometeoroid

text: s and

text: cosmic dust

text: . The

text: Minor Planet Center

text: does not use the term "meteoroid".

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answers: solid object moving in interplanetary space

answers: NDQ_003822

answers: Objects smaller than meteoroids

answers: NDQ_003823

answers: asteroids are too small to have impacts

answers: NDQ_003824

answers: the minimum size of an asteroid is given by what can be discovered from Earth-bound telescopes

answers: NDQ_003825

answers: Objects smaller than meteoroids

answers: NDQ_003826

answers: interplanetary space

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answers: be discovered from Earth-bound telescopes

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answers: a solid object moving in interplanetary space

answers: NDQ_003829

answers: According to Rubin and Grossman

answers: NDQ_003830

answers: minor planets

text: ESA had originally identified two NEOs as possible targets for its Quijote mission:  and (10302) 1989 ML. Neither asteroid represents a threat to Earth. In a subsequent study, two different possibilities were selected: the Amor asteroid 2003 SM84 and 99942 Apophis; the latter is of particular significance to Earth as it will make a close approach in 2029 and 2036. In 2005, ESA announced at the 44th annual Lunar and Planetary Science Conference that its mission would be combined into a joint ESA-NASA Asteroid Impact & Deflection Assessment (AIDA) mission, proposed for 2019–2022. The target selected for AIDA will be a binary asteroid, so that the deflection effect could also be observed from Earth by timing the rotation period of the binary pair. AIDA's new target, a component of binary asteroid 65803 Didymos, will be impacted at a velocity of 22,530 km/h (14,000 mph)

text: ESA had originally identified two NEOs as possible targets for its Quijote mission:  and

text: (10302) 1989 ML

text: . Neither asteroid represents a threat to Earth. In a subsequent study, two different possibilities were selected: the

text: Amor asteroid

text: 2003 SM84

text: and

text: 99942 Apophis

text: ; the latter is of particular significance to Earth as it will make a close approach in 2029 and 2036. In 2005, ESA announced at the 44th annual

text: Lunar and Planetary Science Conference

text: that its mission would be combined into a joint ESA-NASA

text: Asteroid Impact & Deflection Assessment

text: (AIDA) mission, proposed for 2019–2022. The target selected for AIDA will be a

text: binary asteroid

text: , so that the deflection effect could also be observed from Earth by timing the rotation period of the binary pair. AIDA's new target, a component of binary asteroid

text: 65803 Didymos

text: , will be impacted at a velocity of 22,530 km/h (14,000 mph)

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answers: NEOs

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answers: NEOs

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answers: Asteroids do not have craters

answers: NDQ_003824

answers: Neither asteroid represents a threat to Earth

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answers: NEOs

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answers: NEOs

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answers: impact

answers: NDQ_003828

answers: 99942 Apophis

answers: NDQ_003829

answers: Neither asteroid represents a threat to Earth

answers: NDQ_003830

answers: NEOs

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 7.2 kilometers in diameter and its surface has an albedo of 0.149, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.3 kilometers, based on an absolute magnitude of 13.38.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 7.2 kilometers in diameter and its surface has an

text: albedo

text: of 0.149, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.3 kilometers, based on an absolute magnitude of 13.38.

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answers: NDQ_003821

answers: diameter

answers: NDQ_003822

answers: stony

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: NEOWISE mission of NASA's Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: stony

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: stony

answers: NDQ_003828

answers: asteroid

answers: NDQ_003829

answers: The asteroid measures 7.2 kilometers in diameter

answers: NDQ_003830

answers: stony asteroids

text: is a small asteroid that is a Near-Earth object and an Apollo asteroid.

text: is a small

text: asteroid

text: that is a

text: Near-Earth object

text: and an

text: Apollo asteroid

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answers: Near-Earth object

answers: NDQ_003822

answers: asteroid

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: asteroid

answers: NDQ_003825

answers: asteroid

answers: NDQ_003826

answers: Near Earth

answers: NDQ_003827

answers: Apollo asteroid

answers: NDQ_003828

answers: Near-Earth object

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct

answers: NDQ_003830

answers: Near-Earth objects

text: 25143 Itokawa (;  ) is an Apollo and Mars-crosser asteroid. It was the first asteroid to be the target of a sample return mission, the Japanese space probe Hayabusa, and the smallest asteroid photographed by a spacecraft.

text: 25143 Itokawa (;  ) is an

text: Apollo

text: and

text: Mars-crosser asteroid

text: . It was the first asteroid to be the target of a

text: sample return mission

text: , the Japanese

text: space probe

text: Hayabusa

text: , and the smallest asteroid photographed by a spacecraft.

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text: This center is headed by Dr. Noah Brosch from Tel Aviv University and operates the three telescopes of the Wise Observatory. For the purpose of NEO studies, a special wide-field 0.46-m telescope was acquired by Tel Aviv University and is operating at the Wise Observatory located near Mitzpe Ramon. The telescope facilitated the discovery of several tens of new asteroids and is now intensely used to study asteroid rotation and asteroid pair properties. Following the cessation of funding from ISA, the asteroid studies are continuing at the Wise Observatory with no specific financial support.

text: This center is headed by Dr.

text: Noah Brosch

text: from

text: Tel Aviv University

text: and operates the three telescopes of the

text: Wise Observatory

text: . For the purpose of NEO studies, a special wide-field 0.46-m telescope was acquired by

text: Tel Aviv University

text: and is operating at the

text: Wise Observatory

text: located near

text: Mitzpe Ramon

text: . The telescope facilitated the discovery of several tens of new asteroids and is now intensely used to study asteroid rotation and asteroid pair properties. Following the cessation of funding from ISA, the

text: asteroid

text: studies are continuing at the

text: Wise Observatory

text: with no specific financial support.

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answers: It could cause humans to go extinct

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text: 15 Eunomia is a very large asteroid in the inner asteroid belt. It is the largest of the stony (S-type) asteroids, and somewhere between the 8th-to-12th-largest main-belt asteroid overall (uncertainty in diameters causes uncertainty in its ranking). It is the largest Eunomian asteroid, and is estimated to contain 1% of the mass of the asteroid belt.

text: 15 Eunomia is a very large

text: asteroid

text: in the inner

text: asteroid belt

text: . It is the largest of the stony (

text: S-type

text: ) asteroids, and somewhere between the 8th-to-12th-largest main-belt asteroid overall (uncertainty in diameters causes uncertainty in its ranking). It is the largest

text: Eunomian asteroid

text: , and is estimated to contain 1% of the mass of the asteroid belt.

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answers: main-belt

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answers: 15 Eunomia

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answers: main-belt

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answers: inner asteroid belt

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answers: 15 Eunomia

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answers: 15 Eunomia

answers: NDQ_003830

answers: asteroid belt

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 4.9 kilometers in diameter and its surface has an albedo of 0.29, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.7 kilometers based on an absolute magnitude of 13.6.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 4.9 kilometers in diameter and its surface has an

text: albedo

text: of 0.29, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.7 kilometers based on an absolute magnitude of 13.6.

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answers: diameter

answers: NDQ_003822

answers: stony

answers: NDQ_003823

answers: Its surface has an albedo of 0.29

answers: NDQ_003824

answers: NASA's Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: stony

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: stony

answers: NDQ_003828

answers: 4.9 kilometers

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: stony asteroids

text: A list of known near-Earth asteroid close approaches less than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2010.

text: A list of known

text: near-Earth asteroid

text: close approaches less than 1

text: lunar distance

text: km

text: or 0.00256

text: AU

text: ) from Earth in 2010.

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

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answers: near-Earth

answers: NDQ_003822

answers: near-Earth

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: 0.00256 AU

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: AU

answers: NDQ_003827

answers: 0.00256 AU

answers: NDQ_003828

answers: asteroid

answers: NDQ_003829

answers: asteroid close approaches less than 1 lunar distance

answers: NDQ_003830

answers: close approaches

text: 263 Dresda is a typical Main belt asteroid. It belongs to the Koronis family of asteroids.

text: 263 Dresda is a typical

text: Main belt

text: asteroid

text: . It belongs to the

text: Koronis family

text: of asteroids.

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text: The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.0–2.6 AU once every 3 years and 6 months (1,266 days). Its orbit has an eccentricity of 0.15 and an inclination of 4° with respect to the ecliptic. The first observation of Alfiuccio is a precovery that was taken at the Chinese Xinglong Station in 1996. It extended the asteroid's observation arc by 2 years prior to its official discovery observation.

text: The

text: S-type

text: asteroid is a member of the

text: Flora family

text: , one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.0–2.6

text: AU

text: once every 3 years and 6 months (1,266 days). Its orbit has an

text: eccentricity

text: of 0.15 and an

text: inclination

text: of 4

text: with respect to the

text: ecliptic

text: . The first observation of Alfiuccio is a

text: precovery

text: that was taken at the Chinese

text: Xinglong Station

text: in 1996. It extended the asteroid's

text: observation arc

text: by 2 years prior to its official discovery observation.

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answers: main-belt

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answers: stony

answers: NDQ_003822

answers: Flora family

answers: NDQ_003823

answers: The S-type asteroid is a member of the Flora family

answers: NDQ_003824

answers: Alfiuccio is a member of the Flora family

answers: NDQ_003825

answers: Flora family

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: orbits the Sun

answers: NDQ_003828

answers: It orbits the Sun at a distance of 2.0–2.6 AU

answers: NDQ_003829

answers: Alfiuccio

answers: NDQ_003830

answers: orbits the Sun

text: 1575 Winifred, provisional designation , is a stony Phocaea asteroid and slow rotator from the inner regions of the asteroid belt, approximately 9.5 kilometers in diameter. It was discovered on 20 April 1950, by astronomer R. C. Cameron of Indiana University during the Indiana Asteroid Program at Goethe Link Observatory in Indiana, United States.

text: 1575 Winifred, provisional designation , is a stony Phocaea

text: asteroid

text: and

text: slow rotator

text: from the inner regions of the

text: asteroid belt

text: , approximately 9.5 kilometers in diameter. It was discovered on 20 April 1950, by astronomer R. C. Cameron of

text: Indiana University

text: during the

text: Indiana Asteroid Program

text: at

text: Goethe Link Observatory

text: in Indiana, United States.

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answers: astronomers

text: A contact binary is a small Solar System body that is composed of two bodies that have gravitated toward each other until they touch. This means contact binaries have odd shapes. Comet Churyumov–Gerasimenko and Comet Tuttle are most likely contact binaries. Asteroids suspected of being contact binaries include the unusually elongated 624 Hektor and the bilobated 216 Kleopatra and 4769 Castalia. 25143 Itokawa, which was photographed by the Hayabusa probe, also appears to be a contact binary which has resulted in an elongated, bent body. About 10–15% of near-Earth asteroids larger than 200 meters are expected to be contact binaries with two lobes in mutual contact.

text: A contact binary is a

text: small Solar System body

text: that is composed of two bodies that have gravitated toward each other until they touch. This means contact binaries have odd shapes.

text: Comet Churyumov–Gerasimenko

text: and

text: Comet Tuttle

text: are most likely contact binaries.

text: Asteroid

text: s suspected of being contact binaries include the unusually elongated

text: 624 Hektor

text: and the

text: bilobated

text: 216 Kleopatra

text: and

text: 4769 Castalia

text: 25143 Itokawa

text: , which was photographed by the

text: Hayabusa

text: probe, also appears to be a contact binary which has resulted in an elongated, bent body. About 10–15% of

text: near-Earth asteroid

text: s larger than 200 meters are expected to be contact binaries with two lobes in mutual contact.

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answers: Solar System body

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answers: 10–15% of near-Earth asteroids

answers: NDQ_003823

answers: contact binaries have odd shapes

answers: NDQ_003824

answers: Hayabusa probe

answers: NDQ_003825

answers: 10–15% of near-Earth asteroids

answers: NDQ_003826

answers: Solar System

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answers: contact binaries

answers: NDQ_003828

answers: 25143 Itokawa

answers: NDQ_003829

answers: 10–15% of near-Earth asteroids

answers: NDQ_003830

answers: contact binaries

text: |-id=608| 121608 Mikemoreau ||  || Michael C. Moreau (b. 1972), an engineer at NASA’s Goddard Space Flight Center, leads the Navigation Team for the OSIRIS-REx Asteroid Sample Return Mission. He grew up on a dairy farm in Vermont, and is known for his contributions to techniques for autonomous spacecraft navigation.|-id=609| 121609 Josephnicholas ||  || Joseph B. Nicholas (b. 1988) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as tracking data analysis algorithm developer. He has also worked on developing high-degree lunar gravity fields as part of the GRAIL gravity team at NASA GSFC.|-id=615| 121615 Marknoteware ||  || Mark D. Noteware (b. 1958) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Mission Assurance Engineer. He served previously as Senior Quality Engineer for DSCOVR program, Advanced Seal Delivery System Quality Engineer, and Bio-Detection System Quality Engineer. |-id=631| 121631 Josephnuth ||  || Joseph A. Nuth (b. 1953) contributed to NASA’s OSIRIS-REx Asteroid Sample Return Mission as Deputy Project Scientist, and is the Senior Scientist for Primitive Bodies at Goddard Space Flight Center. He served as Chief of the GSFC Astrochemistry Lab and Discipline Scientist for the Origins of Solar Systems Programs. |-id=633| 121633 Ronperison ||  || Ronald Perison (b. 1962) contributed to the OSIRIS-REx mission as the Chief Safety and Mission Assurance Officer. His 28 years of aerospace experience in aircraft and satellite systems includes the USAF, Johns Hopkins University and NASA on the TIMED, Hubble Space Telescope and THEMIS missions. |-id=637| 121637 Druscillaperry ||  || Druscilla D. Perry (b. 1961) is the OVIRS Resource Analyst for the OSIRIS-REx mission. She was also part of the Resources Team for the Magnetospheric Multiscale Mission and a Financial Analyst for the Multidisciplinary Engineering and Technology Support Contract as part of the Business Management Office Team.|-id=654| 121654 Michaelpryzby ||  || Michael S. Pryzby (b. 1967) is the Instrument Systems Engineer on the OSIRIS-REx Mission. Prior to this, he was the Lead Spacecraft Systems Engineer on the Lunar Reconnaissance Orbiter. In his career, he has supported NASA GSFC for over 25 years.|-id=655| 121655 Nitapszcolka ||  || Nita Aanderud Pszcolka (b. 1965) is the Project Support Manager for the OSIRIS-REx Asteroid Sample Return Mission. She is a member of the Goddard business support team utilizing project support skills and techniques for the planning, direction, coordination and evaluation of all project support activities.|-id=656| 121656 Jamesrogers ||  || James E. Rogers (b. 1964) is the Planning and Scheduling Lead for the OSIRIS-REx Asteroid Sample Return Mission. He also was the Planning and Scheduling Lead for the TDRS K/L and STEREO Missions, and a Scheduling Team Member on several Hubble Servicing Missions. |-id=659| 121659 Blairrussell ||  || Blair Russell (b. 1970) provided mechanical engineering oversight of hardware development for the OSIRIS-REx Asteroid Sample Return Mission. Working closely with spacecraft and instrument teams, he ensured a robust, structurally sound mechanical system. Prior to this work he supported the GPM and JWST Missions. |}

text: 121608 Mikemoreau

text: ||  || Michael C. Moreau (b. 1972), an engineer at NASA’s Goddard Space Flight Center, leads the Navigation Team for the OSIRIS-REx Asteroid Sample Return Mission. He grew up on a dairy farm in Vermont, and is known for his contributions to techniques for autonomous spacecraft navigation.|-id=609|

text: 121609 Josephnicholas

text: ||  || Joseph B. Nicholas (b. 1988) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as tracking data analysis algorithm developer. He has also worked on developing high-degree lunar gravity fields as part of the GRAIL gravity team at NASA GSFC.|-id=615|

text: 121615 Marknoteware

text: ||  || Mark D. Noteware (b. 1958) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Mission Assurance Engineer. He served previously as Senior Quality Engineer for DSCOVR program, Advanced Seal Delivery System Quality Engineer, and Bio-Detection System Quality Engineer. |-id=631|

text: 121631 Josephnuth

text: ||  || Joseph A. Nuth (b. 1953) contributed to NASA’s OSIRIS-REx Asteroid Sample Return Mission as Deputy Project Scientist, and is the Senior Scientist for Primitive Bodies at Goddard Space Flight Center. He served as Chief of the GSFC Astrochemistry Lab and Discipline Scientist for the Origins of Solar Systems Programs. |-id=633|

text: 121633 Ronperison

text: ||  || Ronald Perison (b. 1962) contributed to the OSIRIS-REx mission as the Chief Safety and Mission Assurance Officer. His 28 years of aerospace experience in aircraft and satellite systems includes the USAF, Johns Hopkins University and NASA on the TIMED, Hubble Space Telescope and THEMIS missions. |-id=637|

text: 121637 Druscillaperry

text: ||  || Druscilla D. Perry (b. 1961) is the OVIRS Resource Analyst for the OSIRIS-REx mission. She was also part of the Resources Team for the Magnetospheric Multiscale Mission and a Financial Analyst for the Multidisciplinary Engineering and Technology Support Contract as part of the Business Management Office Team.|-id=654|

text: 121654 Michaelpryzby

text: ||  || Michael S. Pryzby (b. 1967) is the Instrument Systems Engineer on the OSIRIS-REx Mission. Prior to this, he was the Lead Spacecraft Systems Engineer on the Lunar Reconnaissance Orbiter. In his career, he has supported NASA GSFC for over 25 years.|-id=655|

text: 121655 Nitapszcolka

text: ||  || Nita Aanderud Pszcolka (b. 1965) is the Project Support Manager for the OSIRIS-REx Asteroid Sample Return Mission. She is a member of the Goddard business support team utilizing project support skills and techniques for the planning, direction, coordination and evaluation of all project support activities.|-id=656|

text: 121656 Jamesrogers

text: ||  || James E. Rogers (b. 1964) is the Planning and Scheduling Lead for the OSIRIS-REx Asteroid Sample Return Mission. He also was the Planning and Scheduling Lead for the TDRS K/L and STEREO Missions, and a Scheduling Team Member on several Hubble Servicing Missions. |-id=659|

text: 121659 Blairrussell

text: ||  || Blair Russell (b. 1970) provided mechanical engineering oversight of hardware development for the OSIRIS-REx Asteroid Sample Return Mission. Working closely with spacecraft and instrument teams, he ensured a robust, structurally sound mechanical system. Prior to this work he supported the GPM and JWST Missions. |}

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answers: NDQ_003822

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

answers: NDQ_003830

answers: 4

answers: NDQ_003821

answers: NASA's Goddard Space Flight Center

answers: NDQ_003822

answers: TIMED, Hubble Space Telescope, and THEMIS missions.

answers: NDQ_003823

answers: Observer for the OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003824

answers: Despite the fact that the OSIRIS-REx Asteroid Sample Return Mission is still in its infancy, it's still a big step forward in the search for extraterrestrial life.

answers: NDQ_003825

answers: TIMED, Hubble Space Telescope, and THEMIS missions.

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: The OSIRIS-REx Asteroid Sample Return Mission is part of NASA's OSIRIS-REx Asteroid Sample Return Mission, which aims to return samples of near-earth asteroids to Earth.

answers: NDQ_003828

answers: Deputy Chief Safety and Mission Assurance Officer for the OSIRIS-REx Asteroid Sample Return Mission. Her 28 years of aerospace experience includes the USAF, Johns Hopkins University, and NASA on the TIMED, Hubble Space Telescope, and THEMIS missions.

answers: NDQ_003829

answers: REx Asteroid Sample Return Mission.

answers: NDQ_003830

answers: Sample Return Mission

text: After the first four asteroids were discovered, there wouldn't be another discovered for 38 years (Astraea). The first four gained popularity as full-fledged planets, but the rapid development of  telescopes led to new asteroids being frequently discovered in what is now known as the main-belt. Some astronomers grouped the first 10 asteroids alongside the first four asteroids as planets until the reclassification that was decided upon after the discovery of Hygiea, the 10th known asteroid.

text: After the first four asteroids were discovered, there wouldn't be another discovered for 38 years (

text: Astraea

text: ). The first four gained popularity as full-fledged planets, but the rapid development of  telescopes led to new asteroids being frequently discovered in what is now known as the

text: main-belt

text: . Some astronomers grouped the first 10 asteroids alongside the first four asteroids as planets until the reclassification that was decided upon after the discovery of Hygiea, the 10th known asteroid.

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answers: known

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answers: were discovered

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answers: asteroids

answers: NDQ_003824

answers: asteroids

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answers: were discovered

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: gain popularity as full-fledged planets

answers: NDQ_003828

answers: Hygiea

answers: NDQ_003829

answers: It's impossible to say

answers: NDQ_003830

answers: planets

text: Because of their forced launch, the Pasteur docks at Saint Helier, a medium-sized Floral asteroid of the Gladholders to pick up supplies.  While there, they are surprised multiple times, but what shocks them most is that the asteroid's inhabitants have apparently discovered, through powerful telescopes, human life on Venus, co-existing with the Mycora.

text: Because of their forced launch, the Pasteur docks at Saint Helier, a medium-sized Floral

text: asteroid

text: of the Gladholders to pick up supplies.  While there, they are surprised multiple times, but what shocks them most is that the asteroid's inhabitants have apparently discovered, through powerful telescopes, human life on Venus, co-existing with the Mycora.

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answers: human life on Venus

text: According to Ouyang Ziyuan's report to the 16th Conference of the Chinese Academy of Sciences, Chang'e 2 departed from L2 on 15 April 2012, and began a mission to the asteroid 4179 Toutatis. The flyby was successfully achieved on 13 December 2012 at 16:30:09 Beijing Time (08:30:09 GMT). Close-up images of the asteroid, with a resolution of up to  per pixel, were later published online. The flyby was the first time an unmanned spacecraft had imaged the asteroid so closely. Chang'e-2 came as close as  to Toutatis, and took pictures of the asteroid at a relative velocity of  per second. China thus became the fourth space agency to conduct a successful mission to an asteroid, after NASA, Europe's ESA and Japan's JAXA.

text: According to

text: Ouyang Ziyuan

text: 's report to the 16th Conference of the

text: Chinese Academy of Sciences

text: , Chang'e 2 departed from L2 on 15 April 2012, and began a mission to the asteroid

text: 4179 Toutatis

text: . The flyby was successfully achieved on 13 December 2012 at 16:30:09 Beijing Time (08:30:09 GMT). Close-up images of the asteroid, with a resolution of up to  per pixel, were later published online. The flyby was the first time an unmanned spacecraft had imaged the asteroid so closely. Chang'e-2 came as close as  to Toutatis, and took pictures of the asteroid at a relative velocity of  per second. China thus became the fourth space agency to conduct a successful mission to an asteroid, after

text: NASA

text: , Europe's

text: ESA

text: and Japan's

text: JAXA

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answers: asteroid

text: In addition to the listed objects, three asteroids have been imaged by spacecraft at distances too large to resolve features (over 100,000 km), and are hence not considered as "visited". Asteroid 132524 APL was imaged by New Horizons in 2006 at a distance of 101,867 km, 2685 Masursky by Cassini in 2000 at a distance of 1,600,000 km, and 307 Nike by Pioneer 10 in 1972 at a distance of 8,800,000 km. The Hubble Space Telescope, a spacecraft in Earth orbit, has imaged several large asteroids, including 2 Pallas and 3 Juno.

text: In addition to the listed objects, three asteroids have been imaged by spacecraft at distances too large to resolve features (over 100,000 km), and are hence not considered as "visited". Asteroid

text: 132524 APL

text: was imaged by

text: New Horizons

text: in 2006 at a distance of 101,867 km,

text: 2685 Masursky

text: by

text: Cassini

text: in 2000 at a distance of 1,600,000 km, and

text: 307 Nike

text: by

text: Pioneer 10

text: in 1972 at a distance of 8,800,000 km. The

text: Hubble Space Telescope

text: , a spacecraft in Earth orbit, has imaged several large asteroids, including

text: 2 Pallas

text: and

text: 3 Juno

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answers: in Earth orbit

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answers: The Hubble Space Telescope

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answers: have been imaged by spacecraft

text: 65 Cybele is one of the largest asteroids in the Solar System and is located in the outer asteroid belt. It gives its name to the Cybele family of asteroids that orbit outward from the Sun from the 2:1 orbital resonance with Jupiter. Cybele is a X-type asteroid, meaning that it is dark in color and carbonaceous in composition. It was discovered in 1861 by Ernst Tempel and named after Cybele, the earth goddess.

text: 65 Cybele is one of the

text: largest

text: asteroid

text: s in the

text: Solar System

text: and is located in the outer

text: asteroid belt

text: . It gives its name to the

text: Cybele family of asteroids

text: that orbit outward from the Sun from the 2:1

text: orbital resonance

text: with

text: Jupiter

text: . Cybele is a

text: X-type asteroid

text: , meaning that it is dark in color and carbonaceous in composition. It was discovered in 1861 by

text: Ernst Tempel

text: and named after

text: Cybele

text: , the earth goddess.

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answers: NDQ_003821

answers: 4

answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 0

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: outer asteroid belt

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: in the Solar System

answers: NDQ_003822

answers: Cybele family

answers: NDQ_003823

answers: asteroids orbit outward from the Sun

answers: NDQ_003824

answers: It gives its name to the Cybele family of asteroids

answers: NDQ_003825

answers: Cybele family

answers: NDQ_003826

answers: outer asteroid belt

answers: NDQ_003827

answers: orbit outward

answers: NDQ_003828

answers: 65 Cybele

answers: NDQ_003829

answers: 65 Cybele

answers: NDQ_003830

answers: orbit outward from the Sun

text: |-| 26201 Sayonisaha ||  || Sayoni Saha (born 1994) is a finalist in the 2012 Intel Science Talent Search, a science competition for high-school seniors, for her behavioral and social-sciences project. |-id=205| 26205 Kuratowski ||  || Kazimierz Kuratowski, 20th-century Polish mathematician |-id=210| 26210 Lingas ||  || Lingas plateau, in the Parc national des Cévennes (Cévennes National Park), site of the Observatoire des Pises |-id=214| 26214 Kalinga ||  || UNESCO's Kalinga Prize (bearing the old name of the Indian state of Orissa) |-id=223| 26223 Enari ||  || 26223 Enari Discovered 1997 Dec. 3 by N. Sato at Chichibu. On 2001 Nov. 23, Akihiko Enari (b. 1980) became the first amateur radio operator (call sign JK1ZAM) in Japan to succeed in contacting the International Space Station in the course of the NASA program "Amateur Radio on the ISS".|-id=232| 26232 Antink ||  || 26232 Antink Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Suzanne Antink mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Palo Alto Senior High School, Palo Alto, California.|-id=233| 26233 Jimbraun ||  || 26233 Jimbraun Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jim Braun mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Naperville Central High School, Naperville, Illinois.|-id=234| 26234 Leslibrinson ||  || 26234 Leslibrinson Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Leslie Brinson mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the North Carolina School of Science & Mathematics, Durham, North Carolina.|-id=235| 26235 Annemaduggan ||  || 26235 Annemaduggan Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Annemarie Duggan mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Shrewsbury High School, Shrewsbury, Massachusetts.|-id=238| 26238 Elduval ||  || 26238 Elduval Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Elizabeth Duval mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Montgomery Blair High School, Silver Spring, Maryland.|-id=240| 26240 Leigheriks ||  || 26240 Leigheriks Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Leigh Eriks mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Catholic Central High School, Grand Rapids, Michigan.|-id=243| 26243 Sallyfenska ||  || 26243 Sallyfenska Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Sally Fenska mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Miami High School, Miami, Oklahoma.|-id=246| 26246 Mikelake ||  || 26246 Mikelake Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Lake mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Half Hollow Hills High School West, Dix Hills, New York.|-id=247| 26247 Doleonardi ||  || 26247 Doleonardi Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Donna Leonardi mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Academy for Medical Science Technology, Hackensack, New Jersey.|-id=248| 26248 Longenecker ||  || 26248 Longenecker Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Nevin Longenecker mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the John Adams High School, South Bend, Indiana.|-id=250| 26250 Shaneludwig ||  || 26250 Shaneludwig Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shane Ludwig mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Woodcrest Christian School, Riverside, California.|-id=251| 26251 Kiranmanne ||  || 26251 Kiranmanne Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Kiran Manne mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Albuquerque Academy, Albuquerque, New Mexico.|-id=255| 26255 Carmarques ||  || 26255 Carmarques Discovered 1998 Aug. 24 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Carlos Marques mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the State University of New York College of Technology at Farmingdale.|-id=259| 26259 Marzigliano ||  || 26259 Marzigliano Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gerard Marzigliano mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Division Avenue High School, Levittown, New York.|-id=264| 26264 McIntyre ||  || 26264 McIntyre Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Nancy McIntyre mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Chaminade College Preparatory, West Hills, California.|-id=266| 26266 Andrewmerrill ||  || 26266 Amdrewmerrill Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Andrew Merrill mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Catlin Gabel School, Portland, Oregon.|-id=267| 26267 Nickmorgan ||  || 26267 Nickmorgan Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Nicholas Morgan mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Staples High School, Westport, Connecticut.|-id=268| 26268 Nardi ||  || 26268 Nardi Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Patricia Nardi mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the George W. Hewlett High School, Hewlett, New York.|-id=269| 26269 Marciaprill ||  || 26269 Marciaprill Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Marcia Prill mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Madison High School, Madison, New Jersey.|-id=271| 26271 Lindapuster ||  || 26271 Lindapuster Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Linda Puster mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Plano West Senior High School, Plano, Texas.|-id=273| 26273 Kateschafer ||  || 26273 Kateschafer Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Katherine Schafer mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Harker School, San Jose, California.|-id=275| 26275 Jefsoulier ||  || Jean Frančois Soulier (b. 1966), a specialized educator and dedicated comet observer. |-id=276| 26276 Natrees ||  || Nathaniel Paul Rees, grandson of the discoverer |-id=277| 26277 Ianrees ||  || Ian Hudson Rees, grandson of the discoverer |-id=291| 26291 Terristaples ||  || 26291 Terristaples Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Terri Staples mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Red River High School, Grand Forks, North Dakota.|-id=293| 26293 Van Muyden ||  || 26293 Van Muyden Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David Van Muyden mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Davis Senior High School, Davis, California.|-id=295| 26295 Vilardi ||  || 26295 Vilardi Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Virginia Vilardi mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Wetumpka High School, Wetumpka, Alabama.|-id=298| 26298 Dunweathers ||  || 26298 Dunweathers Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Duncan Weathers mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Texas Academy of Mathematics & Science, Denton, Texas.|-id=300| 26300 Herbweiss ||  || 26300 Herbweiss Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Herb Weiss mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the South Side High School, Rockville Centre, New York.|}

text: 26201 Sayonisaha

text: ||  || Sayoni Saha (born 1994) is a finalist in the 2012 Intel Science Talent Search, a science competition for high-school seniors, for her behavioral and social-sciences project. |-id=205|

text: 26205 Kuratowski

text: Kazimierz Kuratowski

text: , 20th-century Polish mathematician |-id=210|

text: 26210 Lingas

text: Lingas plateau

text: , in the

text: Parc national des Cévennes

text: (Cévennes National Park), site of the

text: Observatoire des Pises

text: 26214 Kalinga

text: ||  || UNESCO's

text: Kalinga Prize

text: (bearing the old name of the Indian state of Orissa) |-id=223|

text: 26223 Enari

text: ||  || 26223 Enari Discovered 1997 Dec. 3 by N. Sato at Chichibu. On 2001 Nov. 23, Akihiko Enari (b. 1980) became the first amateur radio operator (call sign JK1ZAM) in Japan to succeed in contacting the International Space Station in the course of the NASA program "Amateur Radio on the ISS".|-id=232|

text: 26232 Antink

text: ||  || 26232 Antink Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Suzanne Antink mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Palo Alto Senior High School, Palo Alto, California.|-id=233|

text: 26233 Jimbraun

text: ||  || 26233 Jimbraun Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jim Braun mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Naperville Central High School, Naperville, Illinois.|-id=234|

text: 26234 Leslibrinson

text: ||  || 26234 Leslibrinson Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Leslie Brinson mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the North Carolina School of Science & Mathematics, Durham, North Carolina.|-id=235|

text: 26235 Annemaduggan

text: ||  || 26235 Annemaduggan Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Annemarie Duggan mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Shrewsbury High School, Shrewsbury, Massachusetts.|-id=238|

text: 26238 Elduval

text: ||  || 26238 Elduval Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Elizabeth Duval mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Montgomery Blair High School, Silver Spring, Maryland.|-id=240|

text: 26240 Leigheriks

text: ||  || 26240 Leigheriks Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Leigh Eriks mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Catholic Central High School, Grand Rapids, Michigan.|-id=243|

text: 26243 Sallyfenska

text: ||  || 26243 Sallyfenska Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Sally Fenska mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Miami High School, Miami, Oklahoma.|-id=246|

text: 26246 Mikelake

text: ||  || 26246 Mikelake Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Lake mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Half Hollow Hills High School West, Dix Hills, New York.|-id=247|

text: 26247 Doleonardi

text: ||  || 26247 Doleonardi Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Donna Leonardi mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Academy for Medical Science Technology, Hackensack, New Jersey.|-id=248|

text: 26248 Longenecker

text: ||  || 26248 Longenecker Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Nevin Longenecker mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the John Adams High School, South Bend, Indiana.|-id=250|

text: 26250 Shaneludwig

text: ||  || 26250 Shaneludwig Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shane Ludwig mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Woodcrest Christian School, Riverside, California.|-id=251|

text: 26251 Kiranmanne

text: ||  || 26251 Kiranmanne Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Kiran Manne mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Albuquerque Academy, Albuquerque, New Mexico.|-id=255|

text: 26255 Carmarques

text: ||  || 26255 Carmarques Discovered 1998 Aug. 24 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Carlos Marques mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the State University of New York College of Technology at Farmingdale.|-id=259|

text: 26259 Marzigliano

text: ||  || 26259 Marzigliano Discovered 1998 Aug. 17 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gerard Marzigliano mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Division Avenue High School, Levittown, New York.|-id=264|

text: 26264 McIntyre

text: ||  || 26264 McIntyre Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Nancy McIntyre mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Chaminade College Preparatory, West Hills, California.|-id=266|

text: 26266 Andrewmerrill

text: ||  || 26266 Amdrewmerrill Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Andrew Merrill mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Catlin Gabel School, Portland, Oregon.|-id=267|

text: 26267 Nickmorgan

text: ||  || 26267 Nickmorgan Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Nicholas Morgan mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Staples High School, Westport, Connecticut.|-id=268|

text: 26268 Nardi

text: ||  || 26268 Nardi Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Patricia Nardi mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the George W. Hewlett High School, Hewlett, New York.|-id=269|

text: 26269 Marciaprill

text: ||  || 26269 Marciaprill Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Marcia Prill mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Madison High School, Madison, New Jersey.|-id=271|

text: 26271 Lindapuster

text: ||  || 26271 Lindapuster Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Linda Puster mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Plano West Senior High School, Plano, Texas.|-id=273|

text: 26273 Kateschafer

text: ||  || 26273 Kateschafer Discovered 1998 Sept. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Katherine Schafer mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Harker School, San Jose, California.|-id=275|

text: 26275 Jefsoulier

text: ||  || Jean Frančois Soulier (b. 1966), a specialized educator and dedicated comet observer. |-id=276|

text: 26276 Natrees

text: ||  || Nathaniel Paul Rees, grandson of the discoverer |-id=277|

text: 26277 Ianrees

text: ||  || Ian Hudson Rees, grandson of the discoverer |-id=291|

text: 26291 Terristaples

text: ||  || 26291 Terristaples Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Terri Staples mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Red River High School, Grand Forks, North Dakota.|-id=293|

text: 26293 Van Muyden

text: ||  || 26293 Van Muyden Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David Van Muyden mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Davis Senior High School, Davis, California.|-id=295|

text: 26295 Vilardi

text: ||  || 26295 Vilardi Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Virginia Vilardi mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. She teaches at the Wetumpka High School, Wetumpka, Alabama.|-id=298|

text: 26298 Dunweathers

text: ||  || 26298 Dunweathers Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Duncan Weathers mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the Texas Academy of Mathematics & Science, Denton, Texas.|-id=300|

text: 26300 Herbweiss

text: ||  || 26300 Herbweiss Discovered 1998 Sept. 26 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Herb Weiss mentored a finalist in the 2010 Intel Science Talent Search (STS), a science competition for high school seniors. He teaches at the South Side High School, Rockville Centre, New York.|}

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answers: || || 26234 Leslibrinson

answers: NDQ_003822

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answers: id=223| 26223 Enari

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answers: 26233 Jimbraun

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answers: 26233 Jimbraun

answers: NDQ_003829

answers: || || Leslibrin

answers: NDQ_003830

answers: || || Leslibrinson

text: 7796 Járacimrman (; sometimes spelt Jaracimrman) is an asteroid orbiting in the asteroid belt between Mars and Jupiter. It belongs to the IIa family of asteroids. It cannot approach the Earth nearer than 197 million km.

text: 7796 Járacimrman (; sometimes spelt Jaracimrman) is an

text: asteroid

text: orbiting in the

text: asteroid belt

text: between

text: Mars

text: and

text: Jupiter

text: . It belongs to the IIa family of asteroids. It cannot approach the

text: Earth

text: nearer than 197 million km.

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answers: between Mars and Jupiter

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answers: orbiting

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answers: IIa family

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answers: asteroids

answers: NDQ_003824

answers: It cannot approach the Earth nearer than 197 million km

answers: NDQ_003825

answers: IIa family

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answers: asteroid belt

answers: NDQ_003827

answers: approach the Earth

answers: NDQ_003828

answers: 197 million km

answers: NDQ_003829

answers: It cannot approach the Earth

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answers: orbiting in the asteroid belt

text: The Baptistina family is an asteroid family that was probably produced by the breakup of an asteroid  across 80 million years ago following an impact with a smaller body. The two largest presumed remnants of the parent asteroid are main-belt asteroids 298 Baptistina and 1696 Nurmela.

text: The Baptistina family is an

text: asteroid family

text: that was probably produced by the breakup of an

text: asteroid

text: across 80 million years ago following an impact with a smaller body. The two largest presumed remnants of the parent asteroid are

text: main-belt

text: asteroids

text: 298 Baptistina

text: and

text: 1696 Nurmela

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answers: asteroids

answers: NDQ_003822

answers: main-belt

answers: NDQ_003823

answers: no

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answers: main-belt

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answers: impact with a smaller body

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answers: 80 million years ago

answers: NDQ_003829

answers: impact with a smaller body

answers: NDQ_003830

answers: asteroids

text: Given the size of the SL9 impactors, it is likely that this object was less than one kilometer in diameter.Finding water at the site would indicate that the impactor was a comet, as opposed to an asteroid or a very small, icy moon. At first it was believed that the object was more likely to be a comet since comets generally have more planet crossing orbits. At the distance of Jupiter (5.2 AU) most small comets are not close enough to the Sun to be very active, and so would be hard to detect. Small kilometer-sized asteroids would also be hard to detect, however, and recent work by Orton et al. and Hammel et al. has strongly suggested the impactor was an asteroid, as it left only one impact site, did not reduce Jovian decametric radiation emission by contributing significant dust to the Jovian magnetosphere, and produced high altitude dusty debris full of silica, very different than what was produced by SL9.

text: Given the size of the SL9 impactors, it is likely that this object was less than one kilometer in diameter.Finding water at the site would indicate that the impactor was a comet, as opposed to an asteroid or a very small, icy moon. At first it was believed that the object was more likely to be a comet since comets generally have more planet crossing orbits. At the distance of Jupiter (5.2 AU) most small comets are not close enough to the Sun to be very

text: active

text: , and so would be hard to detect. Small kilometer-sized asteroids would also be hard to detect, however, and recent work by Orton et al. and Hammel et al. has strongly suggested the impactor was an asteroid, as it left only one impact site, did not reduce Jovian decametric radiation emission by contributing significant dust to the Jovian magnetosphere, and produced high altitude dusty debris full of silica, very different than what was produced by SL9.

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answers: Small kilometer-sized asteroids

answers: NDQ_003822

answers: Small kilometer-sized

answers: NDQ_003823

answers: Small kilometer-sized asteroids would also be hard to detect

answers: NDQ_003824

answers: Small kilometer-sized asteroids would also be hard to detect

answers: NDQ_003825

answers: Small kilometer-sized

answers: NDQ_003826

answers: 5.2 AU

answers: NDQ_003827

answers: impact

answers: NDQ_003828

answers: SL9 is an asteroid

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct.

answers: NDQ_003830

answers: comets generally have more planet crossing orbits

text: 17246 Christophedumas, provisional designation , is a binary asteroid from the main-belt and member of the Koronis family, about 5 kilometers in diameter. It was discovered on 5 April 2000, by the Lincoln Near-Earth Asteroid Research (LINEAR) program at Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico. It is known to possess an asteroid moon, designated S/2004 (17246) 1. The S-type asteroid orbits the Sun at a distance of 2.8–2.9 AU once every 4 years and 9 months (1,748 days) and shows an eccentricity of 0.02 and an inclination of 2 degrees from the plane of the ecliptic.

text: 17246 Christophedumas, provisional designation , is a

text: binary

text: asteroid

text: from the

text: main-belt

text: and member of the

text: Koronis family

text: , about 5 kilometers in diameter. It was discovered on 5 April 2000, by the

text: Lincoln Near-Earth Asteroid Research

text: (LINEAR) program at

text: Lincoln Laboratory's Experimental Test Site

text: near Socorro, New Mexico. It is known to possess an

text: asteroid moon

text: , designated S/2004 (17246) 1. The

text: S-type asteroid

text: orbits the Sun at a distance of 2.8–2.9

text: AU

text: once every 4 years and 9 months (1,748 days) and shows an

text: eccentricity

text: of 0.02 and an

text: inclination

text: of 2 degrees from the plane of the

text: ecliptic

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answers: Koronis family

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answers: It is known to possess an asteroid moon

answers: NDQ_003824

answers: It is known to possess an asteroid moon, designated S/2004 (17246) 1

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answers: Koronis family

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answers: main-belt

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answers: orbits the Sun

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answers: 17246 Christophedumas

answers: NDQ_003829

answers: It is known to possess an asteroid moon

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answers: moons

text: In 2013 it was used to image the Near-Earth asteroid 2013 XY8.

text: In 2013 it was used to image the Near-Earth asteroid

text: 2013 XY8

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answers: Near-Earth

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answers: 2013 XY8

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answers: no craters

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answers: Asteroids are too small for nasa missions to visit

answers: NDQ_003825

answers: 2013 XY8

answers: NDQ_003826

answers: Near-Earth

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answers: 2013 XY8

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answers: Near-Earth

text: The Augusta family is a small asteroid family in the main asteroid belt. The largest asteroids of the family include 254 Augusta an 5535 Annefrank.

text: The Augusta family is a small

text: asteroid family

text: in the

text: main asteroid belt

text: . The largest asteroids of the family include

text: 254 Augusta

text: an

text: 5535 Annefrank

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answers: 2

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answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

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answers: NDQ_003828

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answers: NDQ_003829

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answers: NDQ_003830

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answers: NDQ_003821

answers: asteroids

answers: NDQ_003822

answers: Augusta family

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroid family

answers: NDQ_003825

answers: Augusta family

answers: NDQ_003826

answers: main asteroid belt

answers: NDQ_003827

answers: asteroid belt

answers: NDQ_003828

answers: 254 Augusta

answers: NDQ_003829

answers: 5535 Annefrank

answers: NDQ_003830

answers: asteroids

text: The expression "asteroid belt" came into use in the very early 1850s, although it is hard to pinpoint who coined the term. The first English use seems to be in the 1850 translation (by E. C. Otté) of Alexander von Humboldt's Cosmos: "[...] and the regular appearance, about the 13th of November and the 11th of August, of shooting stars, which probably form part of a belt of asteroids intersecting the Earth's orbit and moving with planetary velocity". Other early appearances occur in Robert James Mann's A Guide to the Knowledge of the Heavens, "The orbits of the asteroids are placed in a wide belt of space, extending between the extremes of [...]". The American astronomer Benjamin Peirce seems to have adopted that terminology and to have been one of its promoters. One hundred asteroids had been located by mid-1868, and in 1891 the introduction of astrophotography by Max Wolf accelerated the rate of discovery still further. A total of 1,000 asteroids had been found by 1921, 10,000 by 1981, and 100,000 by 2000. Modern asteroid survey systems now use automated means to locate new minor planets in ever-increasing quantities.

text: The expression "asteroid belt" came into use in the very early 1850s, although it is hard to pinpoint who coined the term. The first English use seems to be in the 1850 translation (by E. C. Otté) of Alexander von Humboldt's Cosmos: "[...] and the regular appearance, about the 13th of November and the 11th of August, of shooting stars, which probably form part of a belt of asteroids intersecting the Earth's orbit and moving with planetary velocity". Other early appearances occur in

text: Robert James Mann

text: 's A Guide to the Knowledge of the Heavens, "The orbits of the asteroids are placed in a wide belt of space, extending between the extremes of [...]". The American astronomer

text: Benjamin Peirce

text: seems to have adopted that terminology and to have been one of its promoters. One hundred asteroids had been located by mid-1868, and in 1891 the introduction of

text: astrophotography

text: by

text: Max Wolf

text: accelerated the rate of discovery still further. A total of 1,000 asteroids had been found by 1921, 10,000 by 1981, and 100,000 by 2000. Modern asteroid survey systems now use automated means to locate new minor planets in ever-increasing quantities.

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answers: minor planets

answers: NDQ_003822

answers: shooting stars

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: Modern asteroid survey systems now use automated means to locate new minor planets

answers: NDQ_003825

answers: shooting stars

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answers: asteroid belt

answers: NDQ_003827

answers: intersect the Earth's orbit

answers: NDQ_003828

answers: The American astronomer Benjamin Peirce

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answers: It is hard to pinpoint who coined the term

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answers: minor planets

text: A powerful tool for astronaut training will be the continuing use of analog environments, including NASA Extreme Environment Mission Operations (NOAA NEEMO), NASA's Desert Research and Technology Studies (Desert RATS), Envihab (planned), Flight Analog Research Unit, Haughton-Mars Project (HMP), or even the ISS (in-flight). In fact, at NEEMO a total of 15 mission astronauts (known as aquanauts) have been trained for future missions to asteroids.<ref name="Moskowitz:2011">MOSKOWITZ, Clara. 2011. Astronauts Set to Become Aquanauts for Undersea 'Asteroid' Mission. [online]. [Accessed 26 February 2012]. Available from World Wide Web:

text: A powerful tool for astronaut training will be the continuing use of analog environments, including NASA Extreme Environment Mission Operations (

text: NOAA NEEMO

text: ), NASA's Desert Research and Technology Studies (

text: Desert RATS

text: Envihab

text: (planned),

text: Flight Analog Research Unit

text: , Haughton-Mars Project (

text: HMP

text: ), or even the ISS (in-flight). In fact, at NEEMO a total of 15 mission astronauts (known as

text: aquanauts

text: ) have been trained for future missions to asteroids.<ref name="Moskowitz:2011">MOSKOWITZ, Clara. 2011. Astronauts Set to Become Aquanauts for Undersea 'Asteroid' Mission. [online]. [Accessed 26 February 2012]. Available from World Wide Web:

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answers: Mars

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answers: NASA Extreme Environment Mission Operations

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answers: Asteroids don't have craters.

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answers: NASA Extreme Environment Mission Operations

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answers: NASA Extreme Environment Mission Operations

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answers: The ISS

answers: NDQ_003830

answers: missions to asteroids

text: This is successful, and Jack and his friends eventually escape on Trigger. Once in space, they hear a message claiming to be from a woman named Molpe, a refugee from the fictional planet of "Ligeia". After some debate, Jack orders the refugees' rescue, only to find that the humanoids have metamorphosed into dangerous asteroids. After escaping them, Trigger lands on what appears to be an asteroid. One of the characters, however, identifies it as a silla, a creature that traps spaceships. Trigger escapes this threat as well, only to fall into a black hole that parallels the mythological Charybdis.

text: This is successful, and Jack and his friends eventually escape on Trigger. Once in space, they hear a message claiming to be from a woman named

text: Molpe

text: , a refugee from the fictional planet of "Ligeia". After some debate, Jack orders the refugees' rescue, only to find that the humanoids have metamorphosed into dangerous asteroids. After escaping them, Trigger lands on what appears to be an asteroid. One of the characters, however, identifies it as a

text: silla

text: , a creature that traps spaceships. Trigger escapes this threat as well, only to fall into a

text: black hole

text: that parallels the mythological

text: Charybdis

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answers: The humanoids have metamorphosed into dangerous asteroids

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answers: asteroids

text: |-id=126| 130126 Stillmanchase ||  || Stillman Chase (b. 1932) is the Systems Engineer for the OTES instrument on OSIRIS-REx Asteroid Sample Return Mission. He was an instrument Co-Investigator on Mariners 2, 6, 7, 9 and 10, Vikings 1 & 2, Pioneers 10 & 11 and Mars Global Surveyor. Chase was an instrument Principal Investigator on Mariner 10.|-id=127| 130127 Zoltanfarkas ||  || Zoltan Farkas (b. 1975) is a mechanical engineer for the OTES instrument on the OSIRIS-REx Asteroid Sample Return Mission. He has designed and fabricated components to enhance electron-microscopes, flight hardware for Mini-TES, THEMIS instruments, and ultra-high pressure instrumentations for ALVIN submersible.|-id=128| 130128 Tarafisher ||  || Tara Fisher (b. 1968) was the Program Administrator for the Thermal Emission Spectrometer Instrument on the OSIRIS-REx Asteroid Sample Return Mission.|-id=158| 130158 Orsonjohn ||  || Orson John (b .1987) was a member of OSIRIS-REx Safety and Mission Assurance team serving as the reliability engineer for OTES as well as serving in a similar role on MAVEN and ATLAS. He is now serving as a quality engineer for the ATLAS/ ICESat-2 mission during Integration and Testing.|-id=161| 130161 Iankubik ||  || Ian Kubik (b. 1988) is a Mechanical Engineer for the OTES instrument on the OSIRIS-REx Asteroid Sample Return Mission. This is his first major engineering role since graduating from Arizona State University.|}

text: 130126 Stillmanchase

text: ||  || Stillman Chase (b. 1932) is the Systems Engineer for the OTES instrument on OSIRIS-REx Asteroid Sample Return Mission. He was an instrument Co-Investigator on Mariners 2, 6, 7, 9 and 10, Vikings 1 & 2, Pioneers 10 & 11 and Mars Global Surveyor. Chase was an instrument Principal Investigator on Mariner 10.|-id=127|

text: 130127 Zoltanfarkas

text: ||  || Zoltan Farkas (b. 1975) is a mechanical engineer for the OTES instrument on the OSIRIS-REx Asteroid Sample Return Mission. He has designed and fabricated components to enhance electron-microscopes, flight hardware for Mini-TES, THEMIS instruments, and ultra-high pressure instrumentations for ALVIN submersible.|-id=128|

text: 130128 Tarafisher

text: ||  || Tara Fisher (b. 1968) was the Program Administrator for the Thermal Emission Spectrometer Instrument on the OSIRIS-REx Asteroid Sample Return Mission.|-id=158|

text: 130158 Orsonjohn

text: ||  || Orson John (b .1987) was a member of OSIRIS-REx Safety and Mission Assurance team serving as the reliability engineer for OTES as well as serving in a similar role on MAVEN and ATLAS. He is now serving as a quality engineer for the ATLAS/ ICESat-2 mission during Integration and Testing.|-id=161|

text: 130161 Iankubik

text: ||  || Ian Kubik (b. 1988) is a Mechanical Engineer for the OTES instrument on the OSIRIS-REx Asteroid Sample Return Mission. This is his first major engineering role since graduating from Arizona State University.|}

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answers: OSIRIS-REx is an asteroid sample return mission.

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answers: asteroid belt

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answers: The OSIRIS-REx Asteroid Sample Return Mission is a mission to return samples of near-earth asteroids.

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text: The Massalia or Massalian family of asteroids is a grouping of S-type asteroids in the inner main belt at very low inclination. About 0.8% of known asteroids belong to this family.

text: The Massalia or Massalian

text: family of asteroids

text: is a grouping of

text: S-type

text: asteroid

text: s in the inner

text: main belt

text: at very low inclination. About 0.8% of known asteroids belong to this family.

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answers: low inclination

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answers: asteroids belong to this family

text: 255 Oppavia is a sizeable Main belt asteroid. It classified as a dark P-type asteroid.

text: 255 Oppavia is a sizeable

text: Main belt

text: asteroid

text: . It classified as a dark

text: P-type asteroid

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answers: asteroid

text: Deep Space Habitat (DSH) is a 2012 proposed NASA conceptual design to support a crew of 4 for exploration beyond Low Earth orbit. Initial concept missions include 60-day and 500-day mission configurations, composed of International Space Station-derived hardware, the Orion crew capsule and various support craft. The Habitat would be equipped with at least one International Docking System Standard (IDSS) docking system. Developing a Deep Space Habitat would allow a crew to live and work safely in space for up to one year on missions to explore cis-lunar space and some near-Earth asteroids. It would also provide experience favorable for designing longer-duration habitats that could be used for manned missions to Mars and more distant asteroids.

text: Deep Space Habitat (DSH) is a 2012 proposed

text: NASA

text: conceptual design to support a crew of 4 for exploration beyond

text: Low Earth orbit

text: . Initial concept missions include 60-day and 500-day mission configurations, composed of

text: International Space Station

text: -derived hardware, the

text: Orion crew capsule

text: and various support craft. The Habitat would be equipped with at least one

text: International Docking System Standard

text: (IDSS) docking system. Developing a Deep Space Habitat would allow a crew to live and work safely in space for up to one year on missions to explore cis-lunar space and some near-Earth asteroids. It would also provide experience favorable for designing longer-duration habitats that could be used for

text: manned missions to Mars

text: and more distant asteroids.

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answers: NDQ_003822

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answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: Deep Space Habitat would allow a crew to live and work safely in space for up to one year on missions to explore cis-lunar space and some near-Earth asteroids

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: Low Earth orbit

answers: NDQ_003827

answers: orbit

answers: NDQ_003828

answers: The Habitat would be equipped with at least one International Docking System Standard

answers: NDQ_003829

answers: The Habitat would be equipped with at least one International Docking System Standard (IDSS) docking system

answers: NDQ_003830

answers: exploration beyond Low Earth orbit

text: 7 Iris is a large main-belt asteroid orbiting the Sun between Mars and Jupiter. It is the fourth-brightest object in the asteroid belt. It is classified as an S-type asteroid, meaning that it has a stony composition.

text: 7 Iris is a large

text: main-belt

text: asteroid orbiting the Sun between Mars and Jupiter. It is the fourth-brightest object in the

text: asteroid belt

text: . It is classified as an

text: S-type asteroid

text: , meaning that it has a

text: stony

text: composition.

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answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

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answers: NDQ_003828

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answers: NDQ_003830

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answers: NDQ_003821

answers: orbiting the Sun

answers: NDQ_003822

answers: 7 Iris

answers: NDQ_003823

answers: 7 Iris

answers: NDQ_003824

answers: 7 Iris

answers: NDQ_003825

answers: 7 Iris

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: Jupiter

answers: NDQ_003828

answers: 7 Iris

answers: NDQ_003829

answers: 7 Iris

answers: NDQ_003830

answers: orbiting the Sun

text: is an Aten-family asteroid, and as such is often near the glare of the Sun as the asteroid seldom travels outside Earth's orbit when the Earth is nearby. The orbit is poorly determined since the asteroid has an observation arc of only 9 days creating an orbital uncertainty of 7. Since the asteroid has not been observed since 14 March 2000, the uncertainty region has kept increasing. During the 2014 approach, 17 February 2014 was the first day that the nominal orbit had a solar elongation more than 90 degrees from the Sun making it easier to recover under a dark sky. Using the nominal orbit, the asteroid was expected to have an apparent magnitude of about 16 and pass  from Earth. Closest approach (perigee-geocentrical) was around 00:15 UTC on 18 February plus or minus about 13 hours. Even with an observation arc of 9 days, it was known that the minimum possible close approach distance to Earth on 18 February 2014 was  with a small chance that the asteroid would pass as far as  from Earth. Due to the uncertainty region of the asteroid, the asteroid could have been 75 degrees from the nominal position in the sky on 18 February 2014.

text: is an

text: Aten-family asteroid

text: , and as such is often near the glare of the Sun as the asteroid seldom travels outside Earth's orbit when the Earth is nearby. The orbit is poorly determined since the asteroid has an observation arc of only 9 days creating an

text: orbital uncertainty

text: of 7. Since the asteroid has not been observed since 14 March 2000, the uncertainty region has kept increasing. During the 2014 approach, 17 February 2014 was the first day that the

text: nominal

text: orbit had a

text: solar elongation

text: more than 90 degrees from the Sun making it easier to recover under a dark sky. Using the nominal orbit, the asteroid was expected to have an

text: apparent magnitude

text: of about 16 and pass  from Earth. Closest approach (

text: perigee

text: -geocentrical) was around 00:15 UTC on 18 February plus or minus about 13 hours. Even with an observation arc of 9 days, it was known that the minimum possible close approach distance to Earth on 18 February 2014 was  with a small chance that the asteroid would pass as far as  from Earth. Due to the uncertainty region of the asteroid, the asteroid could have been 75 degrees from the nominal position in the sky on 18 February 2014.

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answers: NDQ_003821

answers: an Aten-family asteroid

answers: NDQ_003822

answers: Aten-family

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: The orbit is poorly determined since the asteroid has not been observed since 14 March 2000

answers: NDQ_003825

answers: Aten-family

answers: NDQ_003826

answers: uncertainty region

answers: NDQ_003827

answers: travels outside Earth's orbit

answers: NDQ_003828

answers: The orbit is poorly determined since the asteroid has an observation arc of only 9 days

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct

answers: NDQ_003830

answers: Earth's orbit

text: 259 Aletheia is a very large main-belt asteroid that was discovered by German–American astronomer Christian Peters on June 28, 1886, at Litchfield Observatory, Clinton, New York. The dark and heterogeneously composed X-type (Tholen: CP-type) asteroid contains primitive carbonaceous materials, responsible for its low albedo of 0.04. Aletheia measures about 185 kilometers in diameter and belongs to the largest asteroids of the main-belt. It has a semi-major axis of 3.1 AU and an orbit inclined by 11 degrees with a period of 5.55 years.

text: 259 Aletheia is a very large

text: main-belt

text: asteroid

text: that was discovered by German–American astronomer

text: Christian Peters

text: on June 28, 1886, at

text: Litchfield Observatory

text: , Clinton, New York. The dark and heterogeneously composed

text: X-type

text: (Tholen:

text: C

text: P

text: -type) asteroid contains primitive

text: carbonaceous

text: materials, responsible for its low albedo of 0.04. Aletheia measures about 185 kilometers in diameter and belongs to the

text: largest asteroids

text: of the main-belt. It has a semi-major axis of 3.1

text: AU

text: and an orbit inclined by 11 degrees with a period of 5.55 years.

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answers: astronomer

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answers: main-belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: astronomer Christian Peters

answers: NDQ_003825

answers: main-belt

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: main-belt

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answers: 259 Aletheia

answers: NDQ_003829

answers: It has a semi-major axis of 3.1 AU

answers: NDQ_003830

answers: astronomers

text: Asteroid mining has also been seriously considered. A NASA design study evaluated a 10,000 ton mining vehicle (to be assembled in orbit) that would return a 500,000 ton asteroid fragment to geostationary orbit. Only about 3,000 tons of the mining ship would be traditional aerospace-grade payload. The rest would be reaction mass for the mass-driver engine, which could be arranged to be the spent rocket stages used to launch the payload. Assuming that 100% of the returned asteroid was useful, and that the asteroid miner itself couldn't be reused, that represents nearly a 95% reduction in launch costs. However, the true merits of such a method would depend on a thorough mineral survey of the candidate asteroids; thus far, we have only estimates of their composition. One proposal is to capture the asteroid Apophis into earth orbit and convert it into 150 solar power satellites of 5 GW each or the larger asteroid 1999 AN10  which is 50x the size of  Apophis and large enough to build 7,500 5-Gigawatt Solar Power Satellites

text: Asteroid mining

text: has also been seriously considered. A NASA design study evaluated a 10,000 ton mining vehicle (to be assembled in orbit) that would return a 500,000 ton asteroid fragment to geostationary orbit. Only about 3,000 tons of the mining ship would be traditional aerospace-grade payload. The rest would be reaction mass for the mass-driver engine, which could be arranged to be the spent rocket stages used to launch the payload. Assuming that 100% of the returned asteroid was useful, and that the asteroid miner itself couldn't be reused, that represents nearly a 95% reduction in launch costs. However, the true merits of such a method would depend on a thorough mineral survey of the candidate asteroids; thus far, we have only estimates of their composition. One proposal is to capture the asteroid

text: Apophis

text: into earth orbit and convert it into 150 solar power satellites of 5 GW each or the larger asteroid 1999 AN10  which is 50x the size of  Apophis and large enough to build 7,500 5-Gigawatt Solar Power Satellites

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answers: ton

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answers: mining

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answers: asteroids do not have craters

answers: NDQ_003824

answers: Thus far, we have only estimates of their composition

answers: NDQ_003825

answers: mining

answers: NDQ_003826

answers: geostationary

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answers: mining

answers: NDQ_003828

answers: 1999 AN10

answers: NDQ_003829

answers: Asteroid mining has also been seriously considered

answers: NDQ_003830

answers: mining

text: According to the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 16.3 kilometers in diameter and its surface has a low albedo of 0.088, The Collaborative Asteroid Lightcurve Link (CALL) assumes a typical albedo for carbonaceous asteroids of 0.08 and calculates a somewhat smaller diameter of 12.6 kilometers.

text: According to the

text: NEOWISE

text: mission of NASA's space-based

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 16.3 kilometers in diameter and its surface has a low

text: albedo

text: of 0.088, The Collaborative Asteroid Lightcurve Link (CALL) assumes a typical albedo for carbonaceous asteroids of 0.08 and calculates a somewhat smaller diameter of 12.6 kilometers.

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answers: carbonaceous asteroids

text: (374158) 2004 UL is an outstandingly eccentric asteroid, classified as near-Earth object and potentially hazardous asteroid. It is known for having the second-smallest perihelion of any known asteroid, after . It measures between 0.5 and 1.2 kilometers in diameter and was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) at Lincoln Lab's ETS on 18 October 2004.

text: (374158) 2004 UL is an outstandingly eccentric

text: asteroid

text: , classified as

text: near-Earth object

text: and

text: potentially hazardous asteroid

text: . It is known for having the second-smallest

text: perihelion

text: of any known asteroid, after . It measures between 0.5 and 1.2 kilometers in diameter and was discovered by the

text: Lincoln Near-Earth Asteroid Research

text: (LINEAR) at

text: Lincoln Lab's ETS

text: on 18 October 2004.

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answers: any known asteroid

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answers: (374158) 2004 UL

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answers: (LINEAR)

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answers: 374158) 2004 UL

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answers: (374158) 2004 UL

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answers: potentially hazardous

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answers: (374158) 2004 UL

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answers: (374158) 2004 UL

answers: NDQ_003830

answers: potentially hazardous asteroid

text: Near-Earth objects (NEOs) are asteroids, comets and large meteoroids that come close to or collide with Earth. Spaceguard is the collective name for some of the efforts to discover and study NEOs, though these efforts are not sufficiently  funded.

text: Near-Earth object

text: s (NEOs) are

text: asteroid

text: s,

text: comet

text: s and large meteoroids that come close to or

text: collide with Earth

text: Spaceguard

text: is the collective name for some of the efforts to discover and study NEOs, though these efforts are not sufficiently  funded.

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answers: NDQ_003821

answers: large meteoroids

answers: NDQ_003822

answers: NEOs

answers: NDQ_003823

answers: No

answers: NDQ_003824

answers: Spaceguard

answers: NDQ_003825

answers: NEOs

answers: NDQ_003826

answers: NEOs

answers: NDQ_003827

answers: collide with Earth

answers: NDQ_003828

answers: NEOs

answers: NDQ_003829

answers: NEOs

answers: NDQ_003830

answers: NEOs

text: is a small near-Earth asteroid in the Apollo asteroid family. It will be a quasi-satellite of Earth until around 2600.

text: is a small

text: near-Earth asteroid

text: in the

text: Apollo asteroid

text: family. It will be a

text: quasi-satellite

text: of

text: Earth

text: until around 2600.

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answers: near-Earth

answers: NDQ_003822

answers: asteroid family

answers: NDQ_003823

answers: Small near-Earth asteroid

answers: NDQ_003824

answers: Small near-Earth asteroid

answers: NDQ_003825

answers: asteroid family

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: quasi-satellite

answers: NDQ_003828

answers: Earth

answers: NDQ_003829

answers: 2600

answers: NDQ_003830

answers: quasi-satellite

text: A rotational light-curve of this asteroid was obtained from photometric observations made at the U.S. Palomar Transient Factory in October 2013. The light-curve gave a rotation period of  hours with a brightness variation of 0.11 in magnitude (U=2). According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 12.1 kilometers in diameter and its surface has an albedo of 0.084, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 11.3 kilometers, based on an absolute magnitude of 13.46.

text: A rotational

text: light-curve

text: of this asteroid was obtained from photometric observations made at the U.S.

text: Palomar Transient Factory

text: in October 2013. The light-curve gave a

text: rotation period

text: of  hours with a brightness variation of 0.11 in

text: magnitude

text: ). According to the survey carried out by the

text: NEOWISE

text: mission of NASA's space-based

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 12.1 kilometers in diameter and its surface has an

text: albedo

text: of 0.084, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 11.3 kilometers, based on an absolute magnitude of 13.46.

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answers: carbonaceous

answers: NDQ_003822

answers: carbonaceous

answers: NDQ_003823

answers: Its surface has an albedo of 0.084

answers: NDQ_003824

answers: NASA's space-based Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: carbonaceous

answers: NDQ_003826

answers: Palomar

answers: NDQ_003827

answers: rotate

answers: NDQ_003828

answers: The asteroid measures 12.1 kilometers

answers: NDQ_003829

answers: The asteroid measures 12.1 kilometers in diameter

answers: NDQ_003830

answers: carbonaceous

text: is a small asteroid that is a Near-Earth object and an Aten asteroid.

text: is a small

text: asteroid

text: that is a

text: Near-Earth object

text: and an

text: Aten asteroid

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answers: NDQ_003823

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answers: Asteroid could cause humans to go extinct

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answers: Near-Earth objects

text: |-id=308| 120308 Deebradel ||  || Deanna Bradel (b. 1964), a Financial Manager for the NASA OSIRIS-REx Asteroid Sample Return Mission. |-id=347| 120347 Salacia ||  || Salacia, Roman goddess of salt water, Neptune’s wife. |-id=349| 120349 Kalas ||  || John and Elizabeth Kalas are active in proselytizing the night sky at public events |-id=350| 120350 Richburns ||  || Rich Burns (b. 1967) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as SSMO Project Manager.|-id=351| 120351 Beckymasterson ||  || Rebecca A. Masterson (b. 1975) is a research engineer at the Massachusetts Institute of Technology serving tirelessly in the central role of Instrument Manager for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=352| 120352 Gordonwong ||  || Gordon H. Wong (b. 1969) is a software engineer who has shown great patience and dedicated support to the effort required in the design, build, test, and flight of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=353| 120353 Katrinajackson ||  || Katrina Jackson (b. 1989) is a video producer for the OSIRIS-REx Asteroid Sample Return Mission and the Hubble Space Telescope at NASA's Goddard Space Flight Center.|-id=354| 120354 Mikejones ||  || Michael Paul Jones (b. 1991) worked as a student engineer at the Massachusetts Institute of Technology where he designed and implemented the solar X-ray monitor as a comparison instrument for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=361| 120361 Guido || 2005 NZ || Ernesto Guido, Italian amateur astronomer, discoverer of several minor planets |-id=364| 120364 Stevecooley ||  || Steve Cooley (b. 1961) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Lead Flight Dynamics Engineer (proposal/Phase A). |-id=368| 120368 Phillipcoulter ||  || Phillip Coulter (b. 1973), an Optical Engineer working at the NASA Goddard Space Flight Center. |-id=375| 120375 Kugel ||  || François Kugel, comet observer |}

text: 120308 Deebradel

text: ||  || Deanna Bradel (b. 1964), a Financial Manager for the NASA OSIRIS-REx Asteroid Sample Return Mission. |-id=347|

text: 120347 Salacia

text: Salacia

text: , Roman goddess of salt water, Neptune’s wife. |-id=349|

text: 120349 Kalas

text: ||  || John and Elizabeth Kalas are active in proselytizing the night sky at public events |-id=350|

text: 120350 Richburns

text: ||  || Rich Burns (b. 1967) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as SSMO Project Manager.|-id=351|

text: 120351 Beckymasterson

text: ||  || Rebecca A. Masterson (b. 1975) is a research engineer at the Massachusetts Institute of Technology serving tirelessly in the central role of Instrument Manager for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=352|

text: 120352 Gordonwong

text: ||  || Gordon H. Wong (b. 1969) is a software engineer who has shown great patience and dedicated support to the effort required in the design, build, test, and flight of the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=353|

text: 120353 Katrinajackson

text: ||  || Katrina Jackson (b. 1989) is a video producer for the OSIRIS-REx Asteroid Sample Return Mission and the Hubble Space Telescope at NASA's Goddard Space Flight Center.|-id=354|

text: 120354 Mikejones

text: ||  || Michael Paul Jones (b. 1991) worked as a student engineer at the Massachusetts Institute of Technology where he designed and implemented the solar X-ray monitor as a comparison instrument for the student-built Regolith X-ray Imaging Spectrometer aboard the OSIRIS-REx Asteroid Sample Return Mission. |-id=361|

text: 120361 Guido

text: || 2005 NZ ||

text: Ernesto Guido

text: , Italian amateur astronomer, discoverer of several minor planets |-id=364|

text: 120364 Stevecooley

text: ||  || Steve Cooley (b. 1961) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Lead Flight Dynamics Engineer (proposal/Phase A). |-id=368|

text: 120368 Phillipcoulter

text: ||  || Phillip Coulter (b. 1973), an Optical Engineer working at the NASA Goddard Space Flight Center. |-id=375|

text: 120375 Kugel

text: ||  || François Kugel, comet observer |}

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answers: NDQ_003830

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answers: NDQ_003821

answers: Asteroid Sample Return Mission

answers: NDQ_003822

answers: |-id=354| 120354

answers: NDQ_003823

answers: OSIRIS-REx.

answers: NDQ_003824

answers: NASA's OSIRIS-REx Asteroid Sample Return Mission

answers: NDQ_003825

answers: |-id=354| 120354

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Spectrometer

answers: NDQ_003828

answers: OSIRIS-REx Asteroid Sample Return Mission

answers: NDQ_003829

answers: X-ray Imaging Spectrometer aboard the OSIRIS-REx Sample Return Mission.

answers: NDQ_003830

answers: OSIRIS-REx Asteroid Sample Return Mission

text: 1333 Cevenola, provisional designation 1934 DA, is a stony, binary asteroid from the asteroid belt about 15 kilometers in diameter. It was discovered on 20 February 1934, by French female astronomer Odette Bancilhon at Algiers Observatory, Algeria in Northern Africa. The S-type asteroid is a member of the Eunomia family. More specifically, it is estimated to have a Sq spectral type, which would also agree with its family classification. It orbits the Sun at a distance of 2.3–3.0 AU once every four and a half years (1,561 days). Cevenolas orbit is mildly eccentric (0.13) and tilted by 15 degrees to the ecliptic.

text: 1333 Cevenola, provisional designation 1934 DA, is a stony, binary

text: asteroid

text: from the

text: asteroid belt

text: about 15 kilometers in diameter. It was discovered on 20 February 1934, by French female astronomer

text: Odette Bancilhon

text: at

text: Algiers Observatory

text: , Algeria in Northern Africa. The

text: S-type

text: asteroid is a member of the

text: Eunomia family

text: . More specifically, it is estimated to have a Sq

text: spectral type

text: , which would also agree with its family classification. It orbits the Sun at a distance of 2.3–3.0

text: AU

text: once every four and a half years (1,561 days). Cevenolas orbit is mildly eccentric (0.13) and

text: tilted

text: by 15 degrees to the ecliptic.

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answers: orbits the Sun

text: There are 127 asteroids with 134 moons in the asteroid belt. Asteroids with light blue backgrounds are double asteroids, with similarly-sized components, and a Barycenter outside of the larger object. very light blue asteroids might be double asteroids, but due to errors in their size and orbit, it is uncertain.

text: There are 127 asteroids with 134 moons in the asteroid belt. Asteroids with light blue backgrounds are double asteroids, with similarly-sized components, and a

text: Barycenter

text: outside of the larger object. very light blue asteroids might be double asteroids, but due to errors in their size and orbit, it is uncertain.

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answers: asteroid belt

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answers: larger object

answers: NDQ_003822

answers: are double asteroids

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 127 asteroids with 134 moons

answers: NDQ_003825

answers: are double asteroids

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: moons

answers: NDQ_003828

answers: 134

answers: NDQ_003829

answers: Asteroids with light blue backgrounds

answers: NDQ_003830

answers: are double asteroids

text: This asteroid has been approaching the Earth at twenty-five yearly intervals ever since, leaving a succession of disasters in its wake, and has now crash-landed near Windsor Castle.

text: This asteroid has been approaching the Earth at twenty-five yearly intervals ever since, leaving a succession of disasters in its wake, and has now crash-landed near

text: Windsor Castle

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answers: approaching

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answers: approaching the Earth

answers: NDQ_003823

answers: asteroids do not have craters

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answers: asteroids are too small for nasa missions

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answers: crash-landed

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answers: Crash-landed near Windsor Castle

answers: NDQ_003830

answers: disasters

text: 488 Kreusa is an asteroid orbiting the Sun in the asteroid belt.

text: 488 Kreusa is an

text: asteroid

text: orbiting the

text: Sun

text: in the

text: asteroid belt

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answers: orbiting the Sun

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answers: 488 Kreusa

answers: NDQ_003823

answers: 488 Kreusa

answers: NDQ_003824

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answers: asteroid belt

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answers: orbit the Sun

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answers: asteroid belt

answers: NDQ_003829

answers: 488 Kreusa

answers: NDQ_003830

answers: orbiting the Sun

text: A list of known near-Earth asteroid close approaches less than 1 lunar distance () from Earth in 2016.

text: A list of known

text: near-Earth asteroid

text: close approaches less than 1

text: lunar distance

text: () from Earth in 2016.

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

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answers: near-Earth

answers: NDQ_003822

answers: Near-Earth asteroid

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: Asteroids are too small for nasa missions to visit them.

answers: NDQ_003825

answers: Near-Earth asteroid

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: close approaches

answers: NDQ_003828

answers: An asteroid the size of Mars

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct

answers: NDQ_003830

answers: close approaches less than 1 lunar distance

text: 379 Huenna is a large asteroid orbiting in the asteroid belt. It is part of the Themis family, and thus a C-type asteroid and consequently composed mainly of carbonaceous material.

text: 379 Huenna is a large

text: asteroid

text: orbiting in the

text: asteroid belt

text: . It is part of the

text: Themis family

text: , and thus a

text: C-type asteroid

text: and consequently composed mainly of

text: carbon

text: aceous material.

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answers: carbonaceous material

text: A young man awakens in an emergency escape pod finding himself on the surface of an asteroid and having no memory of his identity or how he ended up in this situation. He adopts the name 'Derec' from the name on his space suit, which he later finds out is only the suit's manufacturer. He is soon rescued by a colony of robots who are mining the asteroid in search of something hidden there.  Their mission is surrounded in the utmost secrecy such that Derec is not told what they searching for nor allowed to communicate with the outside world. However, the robots send a message to their commander asking what to do and continue their work.

text: A young man awakens in an emergency

text: escape pod

text: finding himself on the surface of an asteroid and having no memory of his identity or how he ended up in this situation. He adopts the name 'Derec' from the name on his

text: space suit

text: , which he later finds out is only the suit's manufacturer. He is soon rescued by a colony of

text: robot

text: s who are mining the asteroid in search of something hidden there.  Their mission is surrounded in the utmost secrecy such that Derec is not told what they searching for nor allowed to communicate with the outside world. However, the robots send a message to their commander asking what to do and continue their work.

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answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: something hidden there

text: The asteroid achieved its most notable recognition when scientists revealed that it contained over "10,000 tons of gold and 100,000 tons of platinum", or an approximate value at the time of its discovery of "$90 billion for the gold and a cool trillion dollars for the platinum, plus loose change for the asteroid's 10 billion tons of iron and a billion tons of nickel." In 2012 the estimated value of 100,000 tons of platinum was worth approximately five trillion US dollars. The delta-v for a spacecraft rendezvous with this asteroid from low earth orbit is 7.1 km/s.

text: The asteroid achieved its most notable recognition when scientists revealed that it contained over "10,000 tons of gold and 100,000 tons of

text: platinum

text: ", or an approximate value at the time of its discovery of "$90 billion for the gold and a cool trillion dollars for the platinum, plus loose change for the asteroid's 10 billion tons of iron and a billion tons of nickel." In 2012 the estimated value of 100,000 tons of platinum was worth approximately five trillion US dollars. The

text: delta-v

text: for a spacecraft rendezvous with this asteroid from

text: low earth orbit

text: is 7.1 km/s.

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answers: NDQ_003821

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answers: 2

answers: NDQ_003825

answers: 4

answers: NDQ_003826

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answers: NDQ_003821

answers: low Earth orbit

answers: NDQ_003822

answers: contain over "10,000 tons of gold

answers: NDQ_003823

answers: asteroids do not have impacts with other objects

answers: NDQ_003824

answers: Delta-V for a spacecraft rendezvous with this asteroid from low earth orbit is 7.1 km/s

answers: NDQ_003825

answers: contain over "10,000 tons of gold

answers: NDQ_003826

answers: low earth orbit

answers: NDQ_003827

answers: rendezvous

answers: NDQ_003828

answers: 7.1 km/s

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: gold and 100,000 tons of platinum

text: The body is classified as both a C and S-type asteroid by the Collaborative Asteroid Lightcurve Link (CALL) and Pan-STARRS survey of magnitudes, respectively.According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures 22.28 kilometers in diameter and its surface has a high albedo of 0.708, while CALL assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 23.21 kilometers.

text: The body is classified as both a

text: C

text: and

text: S-type

text: asteroid by the Collaborative Asteroid Lightcurve Link (CALL) and

text: Pan-STARRS

text: survey of magnitudes, respectively.According to the survey carried out by NASA's

text: Wide-field Infrared Survey Explorer

text: with its subsequent

text: NEOWISE

text: mission, the asteroid measures 22.28 kilometers in diameter and its surface has a high

text: albedo

text: of 0.708, while CALL assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 23.21 kilometers.

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answers: carbonaceous

answers: NDQ_003822

answers: carbonaceous

answers: NDQ_003823

answers: Its surface has a high albedo

answers: NDQ_003824

answers: NASA's Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: carbonaceous

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: carbonaceous

answers: NDQ_003828

answers: NEOWISE mission

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: carbonaceous asteroids

text: The high population of the asteroid belt makes for a very active environment, where collisions between asteroids occur frequently (on astronomical time scales). Collisions between main-belt bodies with a mean radius of 10 km are expected to occur about once every 10 million years. A collision may fragment an asteroid into numerous smaller pieces (leading to the formation of a new asteroid family). Conversely, collisions that occur at low relative speeds may also join two asteroids. After more than 4 billion years of such processes, the members of the asteroid belt now bear little resemblance to the original population.

text: The high population of the asteroid belt makes for a very active environment, where collisions between asteroids occur frequently (on astronomical time scales). Collisions between main-belt bodies with a mean radius of 10 km are expected to occur about once every 10 million years. A collision may fragment an asteroid into numerous smaller pieces (leading to the formation of a new

text: asteroid family

text: ). Conversely, collisions that occur at low relative speeds may also join two asteroids. After more than 4 billion years of such processes, the members of the asteroid belt now bear little resemblance to the original population.

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answers: NDQ_003830

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answers: NDQ_003821

answers: main-belt

answers: NDQ_003822

answers: collisions between asteroids

answers: NDQ_003823

answers: Collisions

answers: NDQ_003824

answers: collisions that occur at low relative speeds may also join two asteroids

answers: NDQ_003825

answers: collisions between asteroids

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Collisions

answers: NDQ_003828

answers: A collision may fragment an asteroid into numerous smaller pieces

answers: NDQ_003829

answers: A collision may fragment an asteroid into numerous smaller pieces

answers: NDQ_003830

answers: collisions between asteroids occur frequently

text: The asteroid is classified as both, C-type and X-type on the Tholen scheme. It is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. The body orbits the Sun at a distance of 1.6–2.2 AU once every 2 years and 8 months (964 days). Its orbit is tilted by 25 degrees to the plane of the ecliptic and shows an eccentricity of 0.15. Contrary to the expected low albedo for dark, carbonaceous CX-type asteroids, the Collaborative Asteroid Lightcurve Link (CALL) assumes a high albedo of 0.40 for the body. This is rather typical for the descendants of the E-belt, a hypothesized population of primordial asteroids, from which the E-type Hungarian asteroids with high inclinations and a semi-major axis of 1.9 AU are thought to have originated.

text: The asteroid is classified as both,

text: C-type

text: and

text: X-type

text: on the

text: Tholen scheme

text: . It is a member of the

text: Hungaria family

text: , which form the innermost dense concentration of asteroids in the Solar System. The body orbits the Sun at a distance of 1.6–2.2

text: AU

text: once every 2 years and 8 months (964 days). Its orbit is

text: tilted

text: by 25 degrees to the plane of the

text: ecliptic

text: and shows an

text: eccentricity

text: of 0.15. Contrary to the expected low albedo for dark, carbonaceous CX-type asteroids, the Collaborative Asteroid Lightcurve Link (CALL) assumes a high

text: albedo

text: of 0.40 for the body. This is rather typical for the descendants of the

text: E-belt

text: , a hypothesized population of primordial asteroids, from which the

text: E-type

text: Hungarian asteroids with high inclinations and a semi-major axis of 1.9 AU are thought to have originated.

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answers: member of the Hungaria family

answers: NDQ_003822

answers: Hungaria family

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: The body orbits the Sun at a distance of 1.6–2.2 AU

answers: NDQ_003825

answers: Hungaria family

answers: NDQ_003826

answers: ecliptic

answers: NDQ_003827

answers: orbits the Sun

answers: NDQ_003828

answers: The asteroid is classified as both, C-type and X-type on the Tholen scheme

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct.

answers: NDQ_003830

answers: asteroids

text: 11885 Summanus (also designated 1990 SS) is an asteroid that is a Near-Earth Object (NEO) and an Apollo asteroid.

text: 11885 Summanus (also designated 1990 SS) is an

text: asteroid

text: that is a

text: Near-Earth Object

text: (NEO) and an

text: Apollo asteroid

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answers: Near-Earth Object

answers: NDQ_003822

answers: 11885 Summanus

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 11885 Summanus

answers: NDQ_003825

answers: 11885 Summanus

answers: NDQ_003826

answers: Near-Earth

answers: NDQ_003827

answers: Apollo

answers: NDQ_003828

answers: 11885 Summanus

answers: NDQ_003829

answers: 11885 Summanus

answers: NDQ_003830

answers: Apollo asteroid

text: 145 Adeona is a rather large main-belt asteroid. Its surface is very dark, and, based upon its classification as a C-type asteroid, is probably composed of primitive carbonaceous material. The Adeona family of asteroids is named after it.

text: 145 Adeona is a rather large

text: main-belt

text: asteroid

text: . Its surface is very dark, and, based upon its classification as a

text: C-type asteroid

text: , is probably composed of primitive

text: carbon

text: aceous material. The

text: Adeona family

text: of asteroids is named after it.

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answers: NDQ_003821

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answers: NDQ_003823

answers: 0

answers: NDQ_003824

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answers: 4

answers: NDQ_003826

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answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: asteroids

answers: NDQ_003822

answers: The Adeona family

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 145 Adeona

answers: NDQ_003825

answers: The Adeona family

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: 145 Adeona

answers: NDQ_003828

answers: 145 Adeona

answers: NDQ_003829

answers: 145 Adeona

answers: NDQ_003830

answers: carbonaceous material

text: As of 2016, the asteroid's effective size, its composition and albedo, as well as its rotation period and shape remain unknown. Based on an absolute magnitude of 15.1, it measures between 3 and 6 kilometers in diameter, assuming an albedo in the range of 0.05 to 0.25. Since near-Earth asteroids are often of a silicaceous rather than of a carbonaceous composition, with higher albedos, typically above 0.20, the asteroid's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter, at a constant absolute magnitude (brightness).

text: As of 2016, the asteroid's effective size, its composition and albedo, as well as its

text: rotation period

text: and shape remain unknown. Based on an absolute

text: magnitude

text: of 15.1, it measures between 3 and 6 kilometers in diameter, assuming an

text: albedo

text: in the range of 0.05 to 0.25. Since near-Earth asteroids are often of a

text: silicaceous

text: rather than of a

text: carbonaceous

text: composition, with higher albedos, typically above 0.20, the asteroid's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter, at a constant absolute magnitude (brightness).

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answers: NDQ_003821

answers: 4

answers: NDQ_003822

answers: 4

answers: NDQ_003823

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answers: NDQ_003824

answers: 2

answers: NDQ_003825

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answers: NDQ_003826

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answers: 4

answers: NDQ_003828

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answers: NDQ_003821

answers: near-Earth

answers: NDQ_003822

answers: near-Earth

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: The asteroid's effective size, its composition and albedo, as well as its rotation period and shape remain unknown

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: albedos

answers: NDQ_003828

answers: Based on an absolute magnitude of 15.1, it measures between 3 and 6 kilometers in diameter

answers: NDQ_003829

answers: Based on an absolute magnitude of 15.1, it measures between 3 and 6 kilometers in diameter

answers: NDQ_003830

answers: asteroids

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 8.4 kilometers in diameter and its surface has an albedo of 0.17, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 12.9 kilometers, based on an absolute magnitude of 13.18.

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 8.4 kilometers in diameter and its surface has an

text: albedo

text: of 0.17, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 12.9 kilometers, based on an absolute magnitude of 13.18.

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answers: NDQ_003821

answers: 4

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answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 2

answers: NDQ_003825

answers: 4

answers: NDQ_003826

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answers: NEOWISE mission of NASA's Wide-field Infrared Survey Explorer

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answers: carbonaceous

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answers: asteroid belt

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answers: carbonaceous

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answers: The asteroid measures 8.4 kilometers in diameter

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answers: carbonaceous asteroids

text: 90 Antiope ( ) is a double asteroid in the outer asteroid belt. It was discovered on October 1, 1866, by Robert Luther. In 2000, it was found to consist of two almost-equally-sized bodies orbiting each other. At average diameters of about 88 km and 84 km, both components are among the 500 largest asteroids. Antiope is a member of the Themis family of asteroids that share similar orbital elements.

text: 90 Antiope ( ) is a

text: double asteroid

text: in the outer

text: asteroid belt

text: . It was discovered on October 1, 1866, by

text: Robert Luther

text: . In 2000, it was found to consist of two almost-equally-sized bodies orbiting each other. At average diameters of about 88 km and 84 km, both components are among the 500 largest

text: asteroid

text: s. Antiope is a member of the

text: Themis family

text: of asteroids that share similar

text: orbital elements

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answers: asteroid belt

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answers: a double asteroid

answers: NDQ_003822

answers: Themis family

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: 90 Antiope

answers: NDQ_003825

answers: Themis family

answers: NDQ_003826

answers: outer asteroid belt

answers: NDQ_003827

answers: orbiting each other

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answers: 90 Antiope

answers: NDQ_003829

answers: 90 Antiope

answers: NDQ_003830

answers: share similar orbital elements

text: The first spacecraft to traverse the asteroid belt was Pioneer 10, which entered the region on 16 July 1972. At the time there was some concern that the debris in the belt would pose a hazard to the spacecraft, but it has since been safely traversed by 12 spacecraft without incident. Pioneer 11, Voyagers 1 and 2 and Ulysses passed through the belt without imaging any asteroids. Galileo imaged 951 Gaspra in 1991 and 243 Ida in 1993, NEAR imaged 253 Mathilde in 1997, Cassini imaged 2685 Masursky in 2000, Stardust imaged 5535 Annefrank in 2002, New Horizons imaged 132524 APL in 2006, Rosetta imaged 2867 Šteins in September 2008 and 21 Lutetia in July 2010, and Dawn orbited Vesta between July 2011 and September 2012 and has orbited Ceres since March 2015. On its way to Jupiter, Juno traversed the asteroid belt without collecting science data. Due to the low density of materials within the belt, the odds of a probe running into an asteroid are now estimated at less than one in a billion.

text: The first spacecraft to traverse the asteroid belt was

text: Pioneer 10

text: , which entered the region on 16 July 1972. At the time there was some concern that the debris in the belt would pose a hazard to the spacecraft, but it has since been safely traversed by 12 spacecraft without incident.

text: Pioneer 11

text: Voyagers 1 and 2

text: and

text: Ulysses

text: passed through the belt without imaging any asteroids.

text: Galileo

text: imaged

text: 951 Gaspra

text: in 1991 and

text: 243 Ida

text: in 1993,

text: NEAR

text: imaged

text: 253 Mathilde

text: in 1997,

text: Cassini

text: imaged

text: 2685 Masursky

text: in 2000,

text: Stardust

text: imaged

text: 5535 Annefrank

text: in 2002,

text: New Horizons

text: imaged

text: 132524 APL

text: in 2006,

text: Rosetta

text: imaged

text: 2867 Šteins

text: in September 2008 and

text: 21 Lutetia

text: in July 2010, and

text: Dawn

text: orbited

text: Vesta

text: between July 2011 and September 2012 and has orbited

text: Ceres

text: since March 2015. On its way to Jupiter,

text: Juno

text: traversed the asteroid belt without collecting science data. Due to the low density of materials within the belt, the odds of a probe running into an asteroid are now estimated at less than one in a billion.

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answers: debris in the belt

answers: NDQ_003822

answers: the asteroid belt

answers: NDQ_003823

answers: It has since been safely traversed by 12 spacecraft without incident

answers: NDQ_003824

answers: Pioneer 11, Voyagers 1 and 2 and Ulysses passed through the belt without imaging any asteroids

answers: NDQ_003825

answers: the asteroid belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: run into a probe

answers: NDQ_003828

answers: The odds of a probe running into an asteroid are now estimated at less than one in a billion

answers: NDQ_003829

answers: The odds of a probe running into an asteroid are now estimated at less than one in a billion

answers: NDQ_003830

answers: due to the low density of materials

text: One more alternative to explosive deflection is to move the asteroid slowly over a time. Tiny constant thrust accumulates to deviate an object sufficiently from its predicted course. Edward T. Lu and Stanley G. Love have proposed using a large heavy unmanned spacecraft hovering over an asteroid to gravitationally pull the latter into a non-threatening orbit. The spacecraft and the asteroid mutually attract one another. If the spacecraft counters the force towards the asteroid by, e.g., an ion thruster, the net effect is that the asteroid is accelerated towards the spacecraft and thus slightly deflected from its orbit. While slow, this method has the advantage of working irrespective of the asteroid composition or spin rate – rubble pile asteroids would be difficult to deflect by means of nuclear detonations while a pushing device would be hard or inefficient to mount on a fast rotating asteroid. A gravity tractor would likely have to spend several years beside the asteroid to be effective.

text: One more alternative to explosive deflection is to move the asteroid slowly over a time. Tiny constant thrust accumulates to deviate an object sufficiently from its predicted course.

text: Edward T. Lu

text: and

text: Stanley G. Love

text: have proposed using a large heavy unmanned spacecraft hovering over an asteroid to gravitationally pull the latter into a non-threatening orbit. The spacecraft and the asteroid mutually attract one another. If the spacecraft counters the force towards the asteroid by, e.g., an

text: ion thruster

text: , the net effect is that the asteroid is accelerated towards the spacecraft and thus slightly deflected from its orbit. While slow, this method has the advantage of working irrespective of the asteroid composition or spin rate –

text: rubble pile

text: asteroids would be difficult to deflect by means of nuclear detonations while a pushing device would be hard or inefficient to mount on a fast rotating asteroid. A gravity tractor would likely have to spend several years beside the asteroid to be effective.

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answers: object

answers: NDQ_003822

answers: rubble pile

answers: NDQ_003823

answers: Tiny constant thrust accumulates

answers: NDQ_003824

answers: A gravity tractor would likely have to spend several years beside the asteroid to be effective

answers: NDQ_003825

answers: rubble pile

answers: NDQ_003826

answers: orbit

answers: NDQ_003827

answers: Gravity tractor

answers: NDQ_003828

answers: The spacecraft and the asteroid mutually attract one another

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: alternative to explosive deflection

text: |-id=313| 121313 Tamsin ||  || Frank Tamsin, Belgian amateur astronomer, editor of the Belgian astronomical magazine Heelal since 1998 and secretary general of the Vereniging Voor Sterrenkunde (VVS, Flemish Amateur Astronomers Association) and the Volkssterrenwacht vzw Beisbroek/Observatoire de Beisbroek (Public Observatory Beisbroek) in Bruges |-id=315| 121315 Mikelentz ||  || Michael W. Lentz (b. 1968) is an artist in the Conceptual Image Lab at GSFC. He worked for over three years to develop art and animation for the OSIRIS-REx Asteroid Sample Return Mission to illustrate the scope and magnitude of the scientific endeavor to study the asteroid Bennu.|-id=327| 121327 Andreweaker ||  || Andrew C. Eaker (b. 1961) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Project Scheduler. Prior missions include LRO (Lunar Reconnaissance Orbiter) and GLAST (Gamma-Ray Large Area Space Telescope). |-id=328| 121328 Devlynrfennell ||  || Devlyn R. Fennell (b. 1978) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission on Data/Configuration Management. |-id=329| 121329 Getzandanner ||  || Kenneth M. Getzandanner (b. 1988), an Aerospace Engineer at NASA Goddard Space Flight Center, contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as a member of the Flight Dynamics Team. |-id=332| 121332 Jasonhair ||  || Jason Hair (b. 1977), the OSIRIS-REx Visible and near InfraRed Spectrometer Instrument Manager, overseeing instrument development, integration and testing. |-id=352| 121352 Taylorhale ||  || Taylor Hale (b. 1965) is an instrument systems engineer for the OSIRIS-REx Asteroid Sample Return Mission. Prior to OSIRIS-REx, he was the lead engineer on the Landsat-8 Thermal Infrared Sensor instrument developed at Goddard.|}

text: 121313 Tamsin

text: ||  || Frank Tamsin, Belgian amateur astronomer, editor of the Belgian astronomical magazine Heelal since 1998 and secretary general of the

text: Vereniging Voor Sterrenkunde

text: (VVS, Flemish Amateur Astronomers Association) and the

text: Volkssterrenwacht vzw Beisbroek

text: /Observatoire de Beisbroek (Public Observatory Beisbroek) in Bruges |-id=315|

text: 121315 Mikelentz

text: ||  || Michael W. Lentz (b. 1968) is an artist in the Conceptual Image Lab at GSFC. He worked for over three years to develop art and animation for the OSIRIS-REx Asteroid Sample Return Mission to illustrate the scope and magnitude of the scientific endeavor to study the asteroid Bennu.|-id=327|

text: 121327 Andreweaker

text: ||  || Andrew C. Eaker (b. 1961) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as Project Scheduler. Prior missions include LRO (Lunar Reconnaissance Orbiter) and GLAST (Gamma-Ray Large Area Space Telescope). |-id=328|

text: 121328 Devlynrfennell

text: ||  || Devlyn R. Fennell (b. 1978) contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission on Data/Configuration Management. |-id=329|

text: 121329 Getzandanner

text: ||  || Kenneth M. Getzandanner (b. 1988), an Aerospace Engineer at NASA Goddard Space Flight Center, contributed to the NASA OSIRIS-REx Asteroid Sample Return Mission as a member of the Flight Dynamics Team. |-id=332|

text: 121332 Jasonhair

text: ||  || Jason Hair (b. 1977), the OSIRIS-REx Visible and near InfraRed Spectrometer Instrument Manager, overseeing instrument development, integration and testing. |-id=352|

text: 121352 Taylorhale

text: ||  || Taylor Hale (b. 1965) is an instrument systems engineer for the OSIRIS-REx Asteroid Sample Return Mission. Prior to OSIRIS-REx, he was the lead engineer on the Landsat-8 Thermal Infrared Sensor instrument developed at Goddard.|}

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

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answers: NDQ_003821

answers: 4: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003822

answers: 5: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003823

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answers: 5: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003826

answers: 4

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

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answers: | 121332

answers: NDQ_003822

answers: 13134

answers: NDQ_003823

answers: NASA's OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003824

answers: The OSIRIS-REx Asteroid Sample Return Mission is a NASA mission to study asteroid Bennu, which was discovered by the European Space Agency (ESA) in 2013. The asteroid has a diameter of about a quarter of the size of Earth. The asteroid has a diameter of about a quarter of the size of Earth. The asteroid has a diameter of about a quarter of the size of Earth. The asteroid has a diameter of about a quarter of the size of Earth. The asteroid has a diameter of about a quarter of the size of Earth. The asteroid has a diameter of about a quarter of the size of Earth.

answers: NDQ_003825

answers: 13134

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: 332| 121332

answers: NDQ_003828

answers: The asteroid Bennu, which is the size of the moon of Earth, was discovered by astronomer Frank Tamsin in 1998. The asteroid, which has a diameter of about a quarter of Earth's, was discovered by astronomer Frank Tamsin in 1998. The asteroid, which has a diameter of about a quarter of Earth's, was discovered by astronomer Frank Tamsin in 1998.

answers: NDQ_003829

answers: The asteroid Bennu, which has a mass of more than 100 times the size of the Earth, has been dubbed "the biggest asteroid to hit the Earth in a very long time," according to a NASA press release. The asteroid, which has a diameter of more than a quarter of a mile, has been dubbed "the biggest asteroid to hit the Earth in a very long time," according to a NASA press release. The asteroid, which has a diameter of more than a quarter of a mile, has been dubbed "the biggest asteroid to hit the Earth in a very long time," according to a NASA press release. The asteroid, which has a diameter of more than a quarter of a mile, has been dubbed "the biggest asteroid to hit the Earth in a very long time," according to a NASA press release. The asteroid, which has a diameter of more than a quarter of a mile, has been dubbed "the biggest asteroid to hit the Earth in a very long time," according to a NASA press release.

answers: NDQ_003830

answers: id=315| 121315

text: 334 Chicago is a very large main-belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material.

text: 334 Chicago is a very large

text: main-belt

text: asteroid

text: . It is classified as a

text: C-type asteroid

text: and is probably composed of

text: carbon

text: aceous material.

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answers: composed of carbonaceous material

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answers: C-type

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answers: C-type asteroid

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answers: C-type

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answers: carbonaceous material

text: 387 Aquitania is a fairly large main-belt asteroid. It is classified as an S-type asteroid.

text: 387 Aquitania is a fairly large

text: main-belt

text: asteroid

text: . It is classified as an

text: S-type asteroid

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answers: fairly large

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answers: 387 Aquitania

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answers: 387 Aquitania

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answers: 387 Aquitania

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answers: 387 Aquitania

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answers: are classified as an S-type asteroid

text: Near-Earth object detection technology greatly improved around 1998, so objects being detected as of 2004 could have been missed only a decade earlier due to a lack of dedicated Near-Earth sky surveys. As dedicated Near-Earth sky surveys improve, smaller and smaller asteroids are regularly being discovered. The small near-Earth asteroids  and 2014 AA are the only two asteroids discovered before impacting into Earth. Scientists estimate that several dozen asteroids in the 6 to 12 meter size range fly by Earth at a distance closer than the moon every year, but only a fraction of these are actually detected.

text: Near-Earth object

text: detection technology greatly improved around 1998, so objects being detected as of 2004 could have been missed only a decade earlier due to a lack of dedicated Near-Earth sky surveys. As dedicated Near-Earth sky surveys improve, smaller and smaller asteroids are regularly being discovered. The small near-Earth asteroids  and

text: 2014 AA

text: are the only two asteroids discovered before impacting into Earth. Scientists estimate that several dozen asteroids in the 6 to 12 meter size range fly by Earth at a distance

entity_name: List of asteroid close approaches to Earth in 2013

text: closer than the moon every year

text: , but only a fraction of these are actually detected.

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answers: 6 to 12 meter size range

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answers: are regularly being discovered

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answers: As dedicated Near-Earth sky surveys improve

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answers: 2014 AA

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answers: asteroids are regularly being discovered

text: 388 Charybdis is a very large main-belt asteroid. It is classified as a C-type asteroid and is probably composed of privitive carbonates. It was discovered by Auguste Charlois on March 7, 1894, in Nice. It is probably named after the monster in Greek mythology.

text: 388 Charybdis is a very large

text: main-belt

text: asteroid

text: . It is classified as a

text: C-type asteroid

text: and is probably composed of privitive

text: carbonate

text: s. It was discovered by

text: Auguste Charlois

text: on March 7, 1894, in

text: Nice

text: . It is probably named after

text: the monster

text: in

text: Greek mythology

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answers: very large

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answers: C-type

answers: NDQ_003823

answers: 388 Charybdis

answers: NDQ_003824

answers: 388 Charybdis

answers: NDQ_003825

answers: C-type

answers: NDQ_003826

answers: main-belt

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answers: name after the monster in Greek mythology

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answers: 388 Charybdis

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answers: 388 Charybdis

answers: NDQ_003830

answers: monster in Greek mythology

text: Because they lie within the asteroid belt, several Amor III asteroids also belong to subgroups of the asteroid belt. For instance, the first Alinda asteroid (in 1:3 resonance with Jupiter and close to a 4:1 resonance with Earth) discovered was 887 Alinda.

text: Because they lie within the asteroid belt, several Amor III asteroids also belong to subgroups of the asteroid belt. For instance, the first

text: Alinda asteroid

text: (in 1:3 resonance with Jupiter and close to a 4:1 resonance with Earth) discovered was

text: 887 Alinda

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answers: asteroids

answers: NDQ_003822

answers: the asteroid belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: Because they lie within the asteroid belt

answers: NDQ_003825

answers: the asteroid belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: 1:3 resonance with Jupiter

answers: NDQ_003828

answers: 887 Alinda

answers: NDQ_003829

answers: 887 Alinda

answers: NDQ_003830

answers: Earth

text: According to the space-based surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 15.7 and 14.2 kilometers in diameter, respectively. Conversely, the Collaborative Asteroid Lightcurve Link calculates a diameter of only 7.5 kilometers, due to an assumed albedo of 0.20, which is untypically high for a carbonaceous asteroid.

text: According to the space-based surveys carried out by the Japanese

text: Akari

text: satellite and the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 15.7 and 14.2 kilometers in diameter, respectively. Conversely, the Collaborative Asteroid Lightcurve Link calculates a diameter of only 7.5 kilometers, due to an assumed albedo of 0.20, which is untypically high for a

text: carbonaceous

text: asteroid.

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answers: diameter

answers: NDQ_003822

answers: carbonaceous

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answers: asteroids do not have impacts with other objects

answers: NDQ_003824

answers: NASA's Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: carbonaceous

answers: NDQ_003826

answers: asteroid belt

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answers: NDQ_003828

answers: 14.2 kilometers in diameter

answers: NDQ_003829

answers: The asteroid measures 15.7 and 14.2 kilometers in diameter

answers: NDQ_003830

answers: carbonaceous asteroid

text: A human mission to an asteroid would be a new step in the history of spaceflight, by sending astronauts the Moon's orbit where a previous robotic mission called Asteroid Redirect Mission would place a retrieved asteroid.

text: A human mission to an asteroid would be a new step in the

text: history of spaceflight

text: , by sending astronauts the Moon's orbit where a previous robotic mission called

text: Asteroid Redirect Mission

text: would place a retrieved asteroid.

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answers: spaceflight

answers: NDQ_003822

answers: Asteroid

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: Asteroid Redirect Mission

answers: NDQ_003825

answers: Asteroid

answers: NDQ_003826

answers: orbit

answers: NDQ_003827

answers: retrieved

answers: NDQ_003828

answers: The Moon

answers: NDQ_003829

answers: Asteroid Redirect Mission

answers: NDQ_003830

answers: spaceflight

text: As a non-governmental organization it has conducted two lines of related research to help detect NEOs that could one day strike the Earth, and find the technological means to divert their path to avoid such collisions. The organization has publicized the true rate of "city-killer" type impacts of the same magnitude as the explosive 1908 Tunguska event, a rate which is from three to ten times greater than previously believed, or about every century on average. It also assisted the Association of Space Explorers in helping the United Nations establish the International Asteroid Warning Network, as well as a  Space Missions Planning Advisory Group to provide oversight on proposed asteroid deflection missions.

text: As a

text: non-governmental organization

text: it has conducted two lines of related research to help detect NEOs that could one day strike the Earth, and find the technological means to divert their path to avoid such collisions. The organization has publicized the true rate of "city-killer" type impacts of the same magnitude as the explosive

text: 1908 Tunguska event

text: , a rate which is from three to ten times greater than previously believed, or about every century on average. It also assisted the

text: Association of Space Explorers

text: in helping the

text: United Nations

text: establish the

entity_name: United Nations Committee on the Peaceful Uses of Outer Space

entity_section: Near-Earth object deflection and disaster response

text: International Asteroid Warning Network

text: , as well as a  Space Missions Planning Advisory Group to provide oversight on proposed

text: asteroid deflection

text: missions.

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answers: NDQ_003824

answers: Space Missions Planning Advisory Group

answers: NDQ_003825

answers: NEOs

answers: NDQ_003826

answers: NEOs

answers: NDQ_003827

answers: strike the Earth

answers: NDQ_003828

answers: 1908 Tunguska event

answers: NDQ_003829

answers: "city-killer" type impacts

answers: NDQ_003830

answers: could one day strike the Earth

text: Another way in which asteroids could be considered a source of danger is by depicting them as a hazard to navigation, especially threatening to ships traveling from Earth to the outer parts of the Solar System and thus needing to pass the Asteroid Belt (or make a time- and fuel-consuming detour around it). In this context, asteroids serve the same role in space travel stories as reefs and underwater rocks in the older genre of seafaring adventure stories. And like such hazards, asteroids could also be used by bold outlaws to avoid pursuit. Representations of the Asteroid Belt in film tend to make it unrealistically cluttered with dangerous rocks, so dense that adventurous measures must be taken to avoid an impact, giving dramatic visual images which the true nearly empty space would not provide. One of the best-known examples of this is the Hoth system in The Empire Strikes Back.

text: Hoth

text: system in

text: The Empire Strikes Back

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answers: NDQ_003826

answers: Asteroid Belt

answers: NDQ_003827

answers: 0

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answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: dangerous rocks

answers: NDQ_003822

answers: could be considered a source of danger

answers: NDQ_003823

answers: The true nearly empty space would not provide

answers: NDQ_003824

answers: asteroids

answers: NDQ_003825

answers: could be considered a source of danger

answers: NDQ_003826

answers: Asteroid Belt

answers: NDQ_003827

answers: be used by bold outlaws to avoid pursuit

answers: NDQ_003828

answers: The Empire Strikes Back

answers: NDQ_003829

answers: asteroids could also be used by bold outlaws to avoid pursuit

answers: NDQ_003830

answers: asteroids could be considered a source of danger

text: |-id=602| 128602 Careyparish ||  || Carey Parish (b. 1971) was responsible for oversight of the Propulsion subsystem on the OSIRIS-REx mission, managing all aspects of the effort. In addition Carey has contributed directly to the success of the GRAIL, Phoenix and MRO Missions. |-id=604| 128604 Markfisher ||  || Mark Fisher (b. 1964) is responsible for developing the mission control area for the OSIRIS-REx Asteroid Sample Return Mission. Mark also led the Spitzer flight operations team to safely operate the mission well past its intended design life. |-id=607| 128607 Richhund ||  || Rich Hund (b. 1956) is the lead for the Structures, Mechanisms, Propulsion, Sample Return Capsule, and Touch-and-Go Sample Acquisition Mechanism development on the OSIRIS-REx Asteroid Sample Return Mission. He was also responsible for the development and delivery of the MSL aeroshell. |-id=608| 128608 Chucklove ||  || Charles Love (b. 1955) is the Flight System Mission Assurance Manager for the OSIRIS-REx Asteroid Sample Return Mission. He also contributed to the success of the Mars Reconnaissance Orbiter, Spitzer, Odyssey, Stardust, Genesis and Phoenix missions. |-id=610| 128610 Stasiahabenicht ||  || Anastasia Habenicht (b. 1971) is the software lead for the flight system on the OSIRIS-REx Asteroid Sample Return Mission. Stasia also contributed directly to the success of many NASA missions including MAVEN, Phoenix, the Orbital Space Plane and NASA’s advanced space transportation efforts. |-id=611| 128611 Paulnowak ||  || Paul Nowak (b. 1957) is the Flight System Business Manager for the OSIRIS-REx Asteroid Sample Return Mission. In addition, Paul has been the business manager contributing significantly to other NASA missions by overseeing the development on the MAVEN, JUNO, GRAIL and the Phoenix Lander missions.|-id=614| 128614 Juliabest ||  || Julia Best (b 1975) is the planning lead for the flight system on the OSIRIS-REx Asteroid Sample Return Mission. Prior to serving in this role she was a member of the GOES-R development team. |-id=615| 128615 Jimharris ||  || Jim Harris (b. 1953) is the OSIRIS-REx Touch and Go Sample Acquisition Mechanism Certified Principal Engineer. He was also the mechanism designer on the MSL aeroshell program, Genesis sample return mission and Stardust sample return mission. |-id=622| 128622 Rudiš || 2004 RU || Viktor Rudiš, Czech architect |-id=627| 128627 Ottmarsheim ||  || Ottmarsheim, Alsace, France |-id=633| 128633 Queyras ||  || Queyras, a valley of the French Alps |}

text: 128602 Careyparish

text: ||  || Carey Parish (b. 1971) was responsible for oversight of the Propulsion subsystem on the OSIRIS-REx mission, managing all aspects of the effort. In addition Carey has contributed directly to the success of the GRAIL, Phoenix and MRO Missions. |-id=604|

text: 128604 Markfisher

text: ||  || Mark Fisher (b. 1964) is responsible for developing the mission control area for the OSIRIS-REx Asteroid Sample Return Mission. Mark also led the Spitzer flight operations team to safely operate the mission well past its intended design life. |-id=607|

text: 128607 Richhund

text: ||  || Rich Hund (b. 1956) is the lead for the Structures, Mechanisms, Propulsion, Sample Return Capsule, and Touch-and-Go Sample Acquisition Mechanism development on the OSIRIS-REx Asteroid Sample Return Mission. He was also responsible for the development and delivery of the MSL aeroshell. |-id=608|

text: 128608 Chucklove

text: ||  || Charles Love (b. 1955) is the Flight System Mission Assurance Manager for the OSIRIS-REx Asteroid Sample Return Mission. He also contributed to the success of the Mars Reconnaissance Orbiter, Spitzer, Odyssey, Stardust, Genesis and Phoenix missions. |-id=610|

text: 128610 Stasiahabenicht

text: ||  || Anastasia Habenicht (b. 1971) is the software lead for the flight system on the OSIRIS-REx Asteroid Sample Return Mission. Stasia also contributed directly to the success of many NASA missions including MAVEN, Phoenix, the Orbital Space Plane and NASA’s advanced space transportation efforts. |-id=611|

text: 128611 Paulnowak

text: ||  || Paul Nowak (b. 1957) is the Flight System Business Manager for the OSIRIS-REx Asteroid Sample Return Mission. In addition, Paul has been the business manager contributing significantly to other NASA missions by overseeing the development on the MAVEN, JUNO, GRAIL and the Phoenix Lander missions.|-id=614|

text: 128614 Juliabest

text: ||  || Julia Best (b 1975) is the planning lead for the flight system on the OSIRIS-REx Asteroid Sample Return Mission. Prior to serving in this role she was a member of the GOES-R development team. |-id=615|

text: 128615 Jimharris

text: ||  || Jim Harris (b. 1953) is the OSIRIS-REx Touch and Go Sample Acquisition Mechanism Certified Principal Engineer. He was also the mechanism designer on the MSL aeroshell program, Genesis sample return mission and Stardust sample return mission. |-id=622|

text: 128622 Rudiš

text: || 2004 RU || Viktor Rudiš, Czech architect |-id=627|

text: 128627 Ottmarsheim

text: Ottmarsheim

text: , Alsace, France |-id=633|

text: 128633 Queyras

text: Queyras

text: , a valley of the

text: French Alps

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answers: 0

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

answers: tqa2:L_0095/T_0928/49cd92b788121957eb5e274ffc82abe5

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

answers: tqa2:L_0095/T_0928/2a91d8c1f29ebbc512088786aa3df85a

answers: 4: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

answers: tqa2:L_0095/T_0928/7bd73dcce2cf908fccee721432d16cdd

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

answers: tqa2:L_0095/T_0928/a8d8d49e954e77249b69c93ea794380b

answers: 0

answers: tqa2:L_0095/T_0928/caaf8dfb698c0d1d1c936ff9f83f45f0

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

answers: tqa2:L_0095/T_0928/7365169cb2f6c8b1ab754607df6b5aee

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

answers: tqa2:L_0095/T_0928/7db41b9066a9f307226a9a059de1b18f

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

answers: tqa2:L_0095/T_0928/d9e0357488457cb085e2aa552ae6def9

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

answers: NDQ_003821

answers: 0

answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

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

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: 3

answers: NDQ_003827

answers: 0

answers: NDQ_003828

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

answers: NDQ_003829

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

answers: NDQ_003830

answers: 4

answers: NDQ_003821

answers: Sample Return Mission

answers: NDQ_003822

answers: Phoenix missions.

answers: NDQ_003823

answers: NASA's MAVEN, Phoenix, and Orbital Space Plane missions.

answers: NDQ_003824

answers: NASA missions including MAVEN, Phoenix, the Orbital Space Plane, and NASA's advanced space transportation efforts.

answers: NDQ_003825

answers: Phoenix missions.

answers: NDQ_003826

answers: Mars

answers: NDQ_003827

answers: Mars Reconnaissance Orbiter,

answers: NDQ_003828

answers: The OSIRIS-REx Asteroid Sample Return Mission is part of NASA's mission to return a sample of an asteroid the size of Mars to Earth.

answers: NDQ_003829

answers: Mission, the Orbital Space Plane, and the GRAIL mission.

answers: NDQ_003830

answers: Mars Reconnaissance Orbiter

text: The NEAR Shoemaker mission in 2000 orbited the large near-Earth asteroid 433 Eros, and was even successfully landed there, though it had not been designed with this maneuver in mind.  The Japanese ion-drive spacecraft Hayabusa in 2005 also orbited the small near-Earth asteroid 25143 Itokawa, landing on it briefly and returning grains of its surface material to Earth.  Another powerful ion-drive mission, Dawn, has orbited the large asteroid Vesta (July 2011–September 2012) and later moved on to the dwarf planet Ceres, arriving in March 2015.

text: The

text: NEAR Shoemaker

text: mission in 2000 orbited the large near-Earth asteroid

text: 433 Eros

text: , and was even successfully landed there, though it had not been designed with this maneuver in mind.  The Japanese

text: ion-drive

text: spacecraft

text: Hayabusa

text: in 2005 also orbited the small

text: near-Earth asteroid

text: 25143 Itokawa

text: , landing on it briefly and returning grains of its surface material to Earth.  Another powerful ion-drive mission,

text: Dawn

text: , has orbited the large asteroid

text: Vesta

text: (July 2011–September 2012) and later moved on to the dwarf planet

text: Ceres

text: , arriving in March 2015.

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answers: NDQ_003821

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answers: NDQ_003829

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answers: NDQ_003830

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answers: NDQ_003821

answers: near-Earth

answers: NDQ_003822

answers: 433 Eros

answers: NDQ_003823

answers: Small asteroids do not have craters

answers: NDQ_003824

answers: The NEAR Shoemaker mission in 2000 orbited the large near-Earth asteroid 433 Eros, and was even successfully landed there

answers: NDQ_003825

answers: 433 Eros

answers: NDQ_003826

answers: Near Earth

answers: NDQ_003827

answers: successfully landed

answers: NDQ_003828

answers: 433 Eros

answers: NDQ_003829

answers: It had not been designed with this maneuver in mind

answers: NDQ_003830

answers: dwarf planets

text: Baetslé takes 6.08 hours for a full a rotation around its axis. Two observations by the Infrared Astronomical Satellite, IRAS, showed an absolute magnitude of 13.40 and a low geometric albedo of 0.03. While the size, rotational period and orbital data are commonly found among main-belt asteroids, the albedo was exceptionally low and suggested that the body's composition could be mostly carbonaceous. However, subsequent observations by the Wide-field Infrared Survey Explorer's NEOWISE mission gave a higher albedo of 0.22 and 0.30 and the Collaborative Asteroid Lightcurve Link derives a value of 0.33, assuming the body to be of a stony rather than of a carbonaceous composition. This also concurs with the fact that, based on its orbital elements, the asteroid is a member of the Flora family, one of the largest groups of rather bright and stony asteroids in the main-belt.

text: Baetslé takes 6.08 hours for a full a

text: rotation

text: around its axis. Two observations by the Infrared Astronomical Satellite,

text: IRAS

text: , showed an

text: absolute magnitude

text: of 13.40 and a low

text: geometric albedo

text: of 0.03. While the size, rotational period and orbital data are commonly found among main-belt asteroids, the albedo was exceptionally low and suggested that the body's composition could be mostly

text: carbonaceous

text: . However, subsequent observations by the

text: Wide-field Infrared Survey Explorer

text: 's

text: NEOWISE

text: mission gave a higher albedo of 0.22 and 0.30 and the Collaborative Asteroid Lightcurve Link derives a value of 0.33, assuming the body to be of a

text: stony

text: rather than of a carbonaceous composition. This also concurs with the fact that, based on its orbital elements, the asteroid is a member of the

text: Flora family

text: , one of the largest groups of rather bright and stony asteroids in the main-belt.

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answers: asteroids

answers: NDQ_003822

answers: main-belt

answers: NDQ_003823

answers: It does not have craters.

answers: NDQ_003824

answers: Infrared Astronomical Satellite, IRAS

answers: NDQ_003825

answers: main-belt

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: orbital data are commonly found

answers: NDQ_003828

answers: Baetslé

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answers: Baetslé

answers: NDQ_003830

answers: orbital data are commonly found

text: The Planet V hypothesis posits that a fifth terrestrial planet created the Late Heavy Bombardment when its meta-stable orbit entered the inner asteroid belt. The hypothetical fifth terrestrial planet, Planet V, had a mass less than half of Mars and originally orbited between Mars and the asteroid belt. Planet V's orbit became unstable due to perturbations from the other inner planets causing it to intersect the inner asteroid belt. After close encounters with Planet V, many asteroids entered Earth-crossing orbits producing the Late Heavy Bombardment. Planet V was ultimately lost, likely plunging into the Sun. In numerical simulations, an uneven distribution of asteroids, with the asteroids heavily concentrated toward the inner asteroid belt, has been shown to be necessary to produce the LHB via this mechanism. An alternate version of this hypothesis in which the lunar impactors are debris resulting from Planet V impacting Mars, forming the Borealis Basin, has been proposed to explain a low number of giant lunar basins relative to craters and a lack of evidence of cometary impactors.

text: The Planet V hypothesis posits that a fifth

text: terrestrial planet

text: Borealis Basin

text: , has been proposed to explain a low number of giant lunar basins relative to craters and a lack of evidence of cometary impactors.

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answers: belt

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answers: the inner asteroid belt

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answers: no

answers: NDQ_003824

answers: Planet V

answers: NDQ_003825

answers: the inner asteroid belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Earth-crossing orbits

answers: NDQ_003828

answers: planet V's orbit became unstable due to perturbations from the other inner planets causing it to intersect the inner asteroid belt

answers: NDQ_003829

answers: Earth-crossing orbits producing the Late Heavy Bombardment

answers: NDQ_003830

answers: Earth-crossing orbits

text: A list of known near-Earth asteroid close approaches less than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2015.

text: A list of known

text: near-Earth asteroid

text: close approaches less than 1

text: lunar distance

text: km

text: or 0.00256

text: AU

text: ) from Earth in 2015.

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

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text: On 9 May 2003, Hayabusa (meaning, Peregrine falcon), was launched from an M-V rocket.  The goal of the mission was to collect samples from a small near-Earth asteroid named 25143 Itokawa. The craft rendezvoused with the asteroid in September 2005. It was confirmed that the spacecraft successfully landed on the asteroid in November 2005, after some initial confusion regarding the incoming data. Hayabusa returned to Earth with samples from the asteroid on 13 June 2010.

text: On 9 May 2003,

text: Hayabusa

text: (meaning,

text: Peregrine falcon

text: ), was launched from an

text: M-V

text: rocket.  The goal of the mission was to collect samples from a small

text: near-Earth asteroid

text: named

text: 25143 Itokawa

text: . The craft

text: rendezvoused

text: with the asteroid in September 2005. It was confirmed that the spacecraft successfully landed on the asteroid in November 2005, after some initial confusion regarding the incoming data. Hayabusa returned to Earth with samples from the asteroid on 13 June 2010.

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answers: Hayabusa returned to Earth with samples from the asteroid on 13 June 2010.

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answers: The craft rendezvoused with the asteroid in September 2005

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text: The Near Earth Asteroid Prospector, or NEAP, was a concept for a small innovative commercial spacecraft mission by the private company SpaceDev. The goal was to fly NEAP to a targeted near-Earth asteroid residing beyond Earth's orbit, successfully land one or more scientific instruments on the asteroid, communicate the scientific data to Earth, and claim the asteroid as private property. The project ran into fundraising difficulties. One of the most likely candidates was 4660 Nereus.

text: The Near Earth Asteroid Prospector, or NEAP, was a concept for a small innovative

text: commercial spacecraft

text: mission by the private company

text: SpaceDev

text: . The goal was to fly NEAP to a targeted

text: near-Earth asteroid

text: residing beyond

text: Earth's orbit

text: , successfully land one or more scientific instruments on the asteroid, communicate the scientific data to Earth, and claim the asteroid as private property. The project ran into fundraising difficulties. One of the most likely candidates was

text: 4660 Nereus

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answers: The Near Earth Asteroid Prospector

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answers: residing beyond Earth's orbit

text: On January 9, 2129, the asteroid will come within 3,639,998 kilometers of 3 Juno, one of the largest asteroids in the main-belt, and will pass it with a relative velocity of 6.597 km/s.

text: On January 9, 2129, the asteroid will come within 3,639,998 kilometers of

text: 3 Juno

text: , one of the largest asteroids in the main-belt, and will pass it with a relative velocity of 6.597 km/s.

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answers: NDQ_003821

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answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 0

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: 4

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: one of the largest

answers: NDQ_003822

answers: main-belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroids

answers: NDQ_003825

answers: main-belt

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: pass it with a relative velocity

answers: NDQ_003828

answers: 3 Juno

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: asteroids

text: |-id=611| 26611 Madzlandon ||  || 26611 Madzlandon Discovered 2000 Mar. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Madeline Maley Landon (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her environmental-science project. She attends the Friendswood High School, Friendswood, Texas, U.S.A.|-id=612| 26612 Sunsetastro ||  || Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan. |-id=618| 26618 Yixinli ||  || 26618 Yixinli Discovered 2000 Apr. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Yixin Li (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her environmental-science team project. She attends the Ballard High School, Louisville, Kentucky, U.S.A.|-id=620| 26620 Yihuali ||  || 26620 Yihuali Discovered 2000 Apr. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Yihua Li (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her environmental-science team project. She attends the Ballard High School, Louisville, Kentucky, U.S.A.|-id=622| 26622 Maxwimberley ||  || 26622 Maxwimberley Discovered 2000 Apr. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Maxim Ilya Wimberley (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his mathematical-sciences project. He attends the Liberal Arts and Science Academy, Austin, Texas, U.S.A.|-id=629| 26629 Zahller ||  || Cordelia Zahller Luginbuhl (the discoverer's mother), and the Zahller family |-id=634| 26634 Balasubramanian ||  || 26634 Balasubramanian Discovered 2000 Apr. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Anirudha Balasubramanian (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his mathematical-sciences project. He attends the Saint Albans School, Washington, D.C., U.S.A.|-id=639| 26639 Murgaš ||  || Jozef Murgaš, 19th-20th-century Slovak inventor, architect, botanist, painter, patriot, and Roman Catholic priest |-id=640| 26640 Bahýľ ||  || Ján Bahýľ, 19th-20th-century Slovak inventor and aeronautical pioneer |-id=642| 26642 Schlenoff ||  || 26642 Schlenoff Discovered 2000 May 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Philip Samuel Schlenoff (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Maclay School, Tallahassee, Florida, U.S.A.|-id=653| 26653 Amymeyer ||  || 26653 Amymeyer Discovered 2000 Sept. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Amy Elizabeth Meyer (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Oakville Senior High School, St. Louis, Missouri, U.S.A.|-id=656| 26656 Samarenae ||  || 26656 Samarenae Discovered 2000 Sept. 27 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Samantha Renae Prabakaran (b. 1996) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Fort Myers High School, Fort Myers, Florida, U.S.A.|-id=659| 26659 Skirda ||  || 26659 Skirda Discovered 2000 Nov. 1 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Olga Y. Skirda (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Health Careers High School, San Antonio, Texas, U.S.A.|-id=660| 26660 Samahalpern ||  || 26660 Samahalpern Discovered 2000 Nov. 1 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Samantha Brooke Halpern (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Roslyn High School, Roslyn Heights, New York, U.S.A.|-id=661| 26661 Kempelen ||  || Wolfgang von Kempelen, 18th-century Austrian polymath, mechanic and inventor |-id=664| 26664 Jongwon ||  || 26664 Jongwon Discovered 2000 Dec. 20 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jong Hyuck Won (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Langley High School, McLean, Virginia, U.S.A.|-id=665| 26665 Sidjena ||  || 26665 Sidjena Discovered 2000 Dec. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Siddhartha Gautama Jena (b. 1994) was awarded first place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the International Academy, Bloomfield Hills, Michigan, U.S.A.|-id=666| 26666 Justinto ||  || 26666 Justinto Discovered 2000 Dec. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Justin To (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Oak Grove High School, San Jose, California, U.S.A.|-id=667| 26667 Sherwinwu ||  || 26667 Sherwinwu Discovered 2001 Jan. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Sherwin Zhang Wu (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Detroit Country Day School, Beverly Hills, Michigan, U.S.A.|-id=668| 26668 Tonyho ||  || 26668 Tonyho Discovered 2001 Jan. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tony Ho (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences team project. He attends the Lynbrook High School, San Jose, California, U.S.A.|-id=671| 26671 Williamlopes ||  || 26671 Williamlopes Discovered 2001 Feb. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. William Lopes (b. 1989) was awarded second place in the 2010 Intel International Science and Engineering Fair for his microbiology project. He attends the Fundacao Escola Tecnica Liberato Salzano Vieira da Cunha, Novo Hamburgo, Rio Grande do Sul, Brazil.|-id=672| 26672 Ericabrooke ||  || 26672 Ericabrooke Discovered 2001 Feb. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Erica Brooke Portnoy (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her microbiology project. She attends the Commack High School, Commack, New York, U.S.A.|-id=679| 26679 Thomassilver ||  || 26679 Thomassilver Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Thomas Scott Silver (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his microbiology project. He attends the Bergen Academy for Medical Science and Technology, Hackensack, New Jersey, U.S.A.|-id=680| 26680 Wangchristi ||  || 26680 Wangchristi Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Wang Kun Christina (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her microbiology project. She attends the Shanghai American School, Shanghai, China.|-id=681| 26681 Niezgay ||  || 26681 Niezgay Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Augusto German Niez Gay (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his microbiology project. He attends the Instituto San Jose Adoratrices, Concordia, Entre Rios, Argentina.|-id=682| 26682 Evanfletcher ||  || 26682 Evanfletcher Discovered 2001 Mar. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Evan Haley Fletcher (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his physics-and-astronomy project. He attends the Kalamazoo Area Mathematics and Science Center, Kalamazoo, Michigan, U.S.A.|-id=685| 26685 Khojandi ||  || 26685 Khojandi Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Aryan Iden Khojandi (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his physics-and-astronomy project. He attends the Thomas Jefferson High School for Science and Technology, Alexandria, Virginia, U.S.A.|-id=686| 26686 Ellenprice ||  || 26686 Ellenprice Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Ellen Marie Price (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her physics-and-astronomy project. She attends the Jefferson County International Baccalaureate School, Birmingham, Alabama, U.S.A.|-id=688| 26688 Wangenevieve ||  || 26688 Wangenevieve Discovered 2001 Mar. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Genevieve Ying Wang (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her physics-and-astronomy team project. She attends the Grosse Pointe South High School, Grosse Pointe Farms, Michigan, U.S.A.|-id=689| 26689 Smorrison ||  || 26689 Smorrison Discovered 2001 Mar. 23 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Stephen J. Morrison (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his physics-and-astronomy team project. He attends the Grosse Pointe North High School, Grosse Pointe Woods, Michigan, U.S.A.|-id=691| 26691 Lareegardner ||  || 26691 Lareegardner Discovered 2001 Mar. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Laree Danielle Gardner (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her physics-and-astronomy team project. She attends the Grosse Pointe North High School, Grosse Pointe Woods, Michigan, U.S.A.|-id=694| 26694 Wenxili ||  || 26694 Wenxili Discovered 2001 Mar. 16 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Wenxi Li (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her plant-sciences project. She attends the Thomas Chilton Jasper High School, Plano, Texas, U.S.A.|-id=696| 26696 Gechenzhang ||  || 26696 Gechenzhang Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gechen Zhang (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his plant-sciences project. He attends the Rockwood Summit High School, Fenton, Missouri, U.S.A.|-id=699| 26699 Masoncole ||  || 26699 Masoncole Discovered 2001 Mar. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mason Cole McFarland (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his plant-sciences project. He attends the Jefferson County International Baccalaureate School, Birmingham, Alabama, U.S.A.|}

text: 26611 Madzlandon

text: ||  || 26611 Madzlandon Discovered 2000 Mar. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Madeline Maley Landon (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her environmental-science project. She attends the Friendswood High School, Friendswood, Texas, U.S.A.|-id=612|

text: 26612 Sunsetastro

text: ||  || Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan. |-id=618|

text: 26618 Yixinli

text: ||  || 26618 Yixinli Discovered 2000 Apr. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Yixin Li (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her environmental-science team project. She attends the Ballard High School, Louisville, Kentucky, U.S.A.|-id=620|

text: 26620 Yihuali

text: ||  || 26620 Yihuali Discovered 2000 Apr. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Yihua Li (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her environmental-science team project. She attends the Ballard High School, Louisville, Kentucky, U.S.A.|-id=622|

text: 26622 Maxwimberley

text: ||  || 26622 Maxwimberley Discovered 2000 Apr. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Maxim Ilya Wimberley (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his mathematical-sciences project. He attends the Liberal Arts and Science Academy, Austin, Texas, U.S.A.|-id=629|

text: 26629 Zahller

text: ||  || Cordelia Zahller Luginbuhl (the discoverer's mother), and the Zahller family |-id=634|

text: 26634 Balasubramanian

text: ||  || 26634 Balasubramanian Discovered 2000 Apr. 29 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Anirudha Balasubramanian (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his mathematical-sciences project. He attends the Saint Albans School, Washington, D.C., U.S.A.|-id=639|

text: 26639 Murgaš

text: Jozef Murgaš

text: , 19th-20th-century Slovak inventor, architect, botanist, painter, patriot, and Roman Catholic priest |-id=640|

text: 26640 Bahýľ

text: ||  || Ján Bahýľ, 19th-20th-century Slovak inventor and aeronautical pioneer |-id=642|

text: 26642 Schlenoff

text: ||  || 26642 Schlenoff Discovered 2000 May 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Philip Samuel Schlenoff (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Maclay School, Tallahassee, Florida, U.S.A.|-id=653|

text: 26653 Amymeyer

text: ||  || 26653 Amymeyer Discovered 2000 Sept. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Amy Elizabeth Meyer (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Oakville Senior High School, St. Louis, Missouri, U.S.A.|-id=656|

text: 26656 Samarenae

text: ||  || 26656 Samarenae Discovered 2000 Sept. 27 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Samantha Renae Prabakaran (b. 1996) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Fort Myers High School, Fort Myers, Florida, U.S.A.|-id=659|

text: 26659 Skirda

text: ||  || 26659 Skirda Discovered 2000 Nov. 1 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Olga Y. Skirda (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Health Careers High School, San Antonio, Texas, U.S.A.|-id=660|

text: 26660 Samahalpern

text: ||  || 26660 Samahalpern Discovered 2000 Nov. 1 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Samantha Brooke Halpern (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her medicine and health-sciences project. She attends the Roslyn High School, Roslyn Heights, New York, U.S.A.|-id=661|

text: 26661 Kempelen

text: Wolfgang von Kempelen

text: , 18th-century Austrian polymath, mechanic and inventor |-id=664|

text: 26664 Jongwon

text: ||  || 26664 Jongwon Discovered 2000 Dec. 20 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jong Hyuck Won (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Langley High School, McLean, Virginia, U.S.A.|-id=665|

text: 26665 Sidjena

text: ||  || 26665 Sidjena Discovered 2000 Dec. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Siddhartha Gautama Jena (b. 1994) was awarded first place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the International Academy, Bloomfield Hills, Michigan, U.S.A.|-id=666|

text: 26666 Justinto

text: ||  || 26666 Justinto Discovered 2000 Dec. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Justin To (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Oak Grove High School, San Jose, California, U.S.A.|-id=667|

text: 26667 Sherwinwu

text: ||  || 26667 Sherwinwu Discovered 2001 Jan. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Sherwin Zhang Wu (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences project. He attends the Detroit Country Day School, Beverly Hills, Michigan, U.S.A.|-id=668|

text: 26668 Tonyho

text: ||  || 26668 Tonyho Discovered 2001 Jan. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tony Ho (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his medicine and health-sciences team project. He attends the Lynbrook High School, San Jose, California, U.S.A.|-id=671|

text: 26671 Williamlopes

text: ||  || 26671 Williamlopes Discovered 2001 Feb. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. William Lopes (b. 1989) was awarded second place in the 2010 Intel International Science and Engineering Fair for his microbiology project. He attends the Fundacao Escola Tecnica Liberato Salzano Vieira da Cunha, Novo Hamburgo, Rio Grande do Sul, Brazil.|-id=672|

text: 26672 Ericabrooke

text: ||  || 26672 Ericabrooke Discovered 2001 Feb. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Erica Brooke Portnoy (b. 1993) was awarded first place in the 2010 Intel International Science and Engineering Fair for her microbiology project. She attends the Commack High School, Commack, New York, U.S.A.|-id=679|

text: 26679 Thomassilver

text: ||  || 26679 Thomassilver Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Thomas Scott Silver (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his microbiology project. He attends the Bergen Academy for Medical Science and Technology, Hackensack, New Jersey, U.S.A.|-id=680|

text: 26680 Wangchristi

text: ||  || 26680 Wangchristi Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Wang Kun Christina (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her microbiology project. She attends the Shanghai American School, Shanghai, China.|-id=681|

text: 26681 Niezgay

text: ||  || 26681 Niezgay Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Augusto German Niez Gay (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his microbiology project. He attends the Instituto San Jose Adoratrices, Concordia, Entre Rios, Argentina.|-id=682|

text: 26682 Evanfletcher

text: ||  || 26682 Evanfletcher Discovered 2001 Mar. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Evan Haley Fletcher (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his physics-and-astronomy project. He attends the Kalamazoo Area Mathematics and Science Center, Kalamazoo, Michigan, U.S.A.|-id=685|

text: 26685 Khojandi

text: ||  || 26685 Khojandi Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Aryan Iden Khojandi (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his physics-and-astronomy project. He attends the Thomas Jefferson High School for Science and Technology, Alexandria, Virginia, U.S.A.|-id=686|

text: 26686 Ellenprice

text: ||  || 26686 Ellenprice Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Ellen Marie Price (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her physics-and-astronomy project. She attends the Jefferson County International Baccalaureate School, Birmingham, Alabama, U.S.A.|-id=688|

text: 26688 Wangenevieve

text: ||  || 26688 Wangenevieve Discovered 2001 Mar. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Genevieve Ying Wang (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her physics-and-astronomy team project. She attends the Grosse Pointe South High School, Grosse Pointe Farms, Michigan, U.S.A.|-id=689|

text: 26689 Smorrison

text: ||  || 26689 Smorrison Discovered 2001 Mar. 23 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Stephen J. Morrison (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his physics-and-astronomy team project. He attends the Grosse Pointe North High School, Grosse Pointe Woods, Michigan, U.S.A.|-id=691|

text: 26691 Lareegardner

text: ||  || 26691 Lareegardner Discovered 2001 Mar. 19 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Laree Danielle Gardner (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her physics-and-astronomy team project. She attends the Grosse Pointe North High School, Grosse Pointe Woods, Michigan, U.S.A.|-id=694|

text: 26694 Wenxili

text: ||  || 26694 Wenxili Discovered 2001 Mar. 16 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Wenxi Li (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for her plant-sciences project. She attends the Thomas Chilton Jasper High School, Plano, Texas, U.S.A.|-id=696|

text: 26696 Gechenzhang

text: ||  || 26696 Gechenzhang Discovered 2001 Mar. 18 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Gechen Zhang (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his plant-sciences project. He attends the Rockwood Summit High School, Fenton, Missouri, U.S.A.|-id=699|

text: 26699 Masoncole

text: ||  || 26699 Masoncole Discovered 2001 Mar. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mason Cole McFarland (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his plant-sciences project. He attends the Jefferson County International Baccalaureate School, Birmingham, Alabama, U.S.A.|}

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answers: Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

answers: NDQ_003822

answers: Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

answers: NDQ_003823

answers: || Asteroids are too small to have impacts with other objects, so they don't have craters.

answers: NDQ_003824

answers: Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

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answers: Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

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answers: Near-Earth

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answers: Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

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answers: || || Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

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answers: || Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

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answers: Founded in 1975, the Sunset Astronomical Society serves the Saginaw-Bay City-Midland tri-cities area of mid-Michigan.

text: In "Mission: Mission Creek High", he builds a new lab, re-installs Eddy, and becomes rich again when he makes a contract with the government to make a rocket system to protect the Earth from rogue asteroids.

text: In "Mission: Mission Creek High", he builds a new lab, re-installs Eddy, and becomes rich again when he makes a contract with the government to make a rocket system to protect the Earth from rogue asteroids.

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answers: rogue asteroids

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answers: protect the Earth

text: The Observatorio Astronómico de La Sagra (OLS and observatory code J75) is an observatory located in the province of Granada, Spain. It uses four robotic telescopes both designed and built (hardware and software) by the scientists of the Observatorio Astronómico de Mallorca (OAM) who operate them remotely by telecontrol daily, discharging data from Mallorca using the Internet, to process them by means of sophisticated algorithms designed "in house" which helped to detect asteroid 2012 DA14. among the other 1706 asteroids, with a 12th place in the ranking of asteroid  discoveries. Its activities include, as part of its La Sagra Sky Survey (LSSS), tracking Small Solar System Bodies, particularly Near Earth Objects, and Space Debris.

text: The Observatorio Astronómico de La Sagra (OLS and

text: observatory code

text: J75) is an

text: observatory

text: located in the

text: province of Granada

text: Spain

text: . It uses four

text: robotic telescope

text: s both designed and built (

text: hardware

text: and

text: software

text: ) by the scientists of the

text: Observatorio Astronómico de Mallorca

text: (OAM) who operate them remotely by

text: telecontrol

text: daily, discharging data from

text: Mallorca

text: using the

text: Internet

text: , to process them by means of sophisticated algorithms designed "in house" which helped to detect asteroid

text: 2012 DA14

text: . among the other 1706

text: asteroid

text: s, with a 12th place in the ranking of asteroid  discoveries. Its activities include, as part of its La Sagra Sky Survey (LSSS), tracking

text: Small Solar System Bodies

text: , particularly

text: Near Earth Objects

text: , and

text: Space Debris

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text: Apophis is one of two asteroids that were considered by the European Space Agency as the target of its Don Quijote mission concept to study the effects of impacting an asteroid.

text: Apophis is one of two asteroids that were considered by the

text: European Space Agency

text: as the target of its

text: Don Quijote mission concept

text: to study the effects of impacting an asteroid.

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answers: Apophis

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answers: Don Quijote mission

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answers: Apophis

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answers: impacting an asteroid

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answers: impact

text: Thule was the first discovered member of the Thule dynamical group, which as of 2008 is known to consist of three objects: 279 Thule, , and .The orbits of these bodies are unusual. They orbit in the outermost edge of the asteroid belt in a 4:3 orbital resonance with Jupiter, the result of the periodic force Jupiter exerts on a body with Thule's orbital period, in the same way (though with the reverse effect) as the Kirkwood gaps in the more inner parts of the asteroid belt.

text: Thule was the first discovered member of the Thule dynamical group, which as of 2008 is known to consist of three objects: 279 Thule, , and .The orbits of these bodies are unusual. They orbit in the outermost edge of the asteroid belt in a 4:3

text: orbital resonance

text: with

text: Jupiter

text: , the result of the periodic force Jupiter exerts on a body with Thule's orbital period, in the same way (though with the reverse effect) as the

text: Kirkwood gap

text: s in the more inner parts of the asteroid belt.

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answers: asteroid belt

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answers: body

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answers: the asteroid belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: They orbit in the outermost edge of the asteroid belt

answers: NDQ_003825

answers: the asteroid belt

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: orbital resonance with Jupiter

answers: NDQ_003828

answers: Thule dynamical group

answers: NDQ_003829

answers: Thule dynamical group

answers: NDQ_003830

answers: The orbits of these bodies are unusual

text: Asteroid 6097 was discovered on October 29, 1991 by Kin Endate and Kazuro Watanabe at Kitami. The Main-belt asteroid was given the name 6097 Koishikawa in honor of Masahiro Koishikawa.

text: Asteroid 6097

text: was discovered on October 29, 1991 by

text: Kin Endate

text: and

text: Kazuro Watanabe

text: at

text: Kitami

text: . The

text: Main-belt asteroid

text: was given the name 6097 Koishikawa in honor of Masahiro Koishikawa.

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answers: discovered

answers: NDQ_003822

answers: 6097 Koishikawa

answers: NDQ_003823

answers: no

answers: NDQ_003824

answers: Asteroid 6097 was discovered

answers: NDQ_003825

answers: 6097 Koishikawa

answers: NDQ_003826

answers: Main-belt

answers: NDQ_003827

answers: be discovered

answers: NDQ_003828

answers: 6097 Koishikawa

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: asteroid

text: |-| 26401 Sobotište || 1999 WX || Sobotište, a village in southwestern Slovakia, home of an astronomical observatory |-id=411| 26411 Jocorbferg ||  || 26411 Jocorbferg Discovered 1999 Dec. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joseph Corbett Ferguson (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology team project. He attends the Paul Laurence Dunbar High School, Lexington, Kentucky, U.S.A.|-id=412| 26412 Charlesyu ||  || 26412 Charlesyu Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Charles Cheng Yu (b. 1994) was awarded first place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology team project. He attends the Wheatley School, Old Westbury, New York, U.S.A.|-id=414| 26414 Amychyao ||  || 26414 Amychyao Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Amy Cindy Chyao (b. 1994) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her chemistry project. She attends the Williams High School, Plano, Texas, U.S.A.|-id=417| 26417 Michaelgord ||  || 26417 Michaelgord Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Aaron Gord (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry project. He attends the Dayton Christian High School, Miamisburg, Ohio, U.S.A.|-id=422| 26422 Marekbuchman ||  || 26422 Marekbuchman Discovered 1999 Dec. 12 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Marek Buchman (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry project. He attends the School for Extraordinary Gifted Children, Bratislava, Slovakia.|-id=424| 26424 Jacquelihung ||  || 26424 Jacquelihung Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Hung Jacqueline (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for her chemistry team project. She attends the Taipei Municipal First Girls' Senior High School, Taipei City, Chinese Taipei.|-id=425| 26425 Linchichieh ||  || 26425 Linchichieh Discovered 1999 Dec. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Lin Chi-Chieh (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for her chemistry team project. She attends the Taipei Municipal First Girls' Senior High School, Taipei City, Chinese Taipei.|-id=426| 26426 Koechl ||  || 26426 Koechl Discovered 1999 Dec. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Juergen Koechl (b. 1990) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry team project. He attends the HTL Braunau am Inn, Braunau am Inn, Austria.|-id=429| 26429 Andiwagner ||  || 26429 Andiwagner Discovered 1999 Dec. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Andreas Wagner (b. 1990) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry team project. He attends the HTL Braunau am Inn, Braunau am Inn, Austria.|-id=430| 26430 Thomwilkason ||  || 26430 Thomwilkason Discovered 1999 Dec. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Thomas Frederick Wilkason (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his computer-science project. He attends the Mount de Sales Academy, Macon, Georgia, U.S.A.|-id=433| 26433 Michaelyurko ||  || 26433 Michaelyurko Discovered 1999 Dec. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Christopher Yurko (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his computer-science project. He attends the Detroit Catholic Central High School, Novi, Michigan, U.S.A.|-id=441| 26441 Nanayakkara ||  || 26441 Nanayakkara Discovered 2000 Jan. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Ganindu Nanayakkara (b. 1990) was awarded first place in the 2010 Intel International Science and Engineering Fair for his computer-science project. He attends the Ananda College, Colombo, Sri Lanka.|-id=442| 26442 Matfernandez ||  || 26442 Matfernandez Discovered 2000 Jan. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Matthew Fernandez (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his computer-science team project. He attends the Oregon Episcopal School, Portland, Oregon, U.S.A.|-id=447| 26447 Akrishnan ||  || 26447 Akrishnan Discovered 2000 Jan. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Akash Krishnan (b. 1994) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his computer-science team project. He attends the Oregon Episcopal School, Portland, Oregon, U.S.A.|-id=448| 26448 Tongjili ||  || 26448 Tongjili Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tongji Li (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science project. She attends the Hershey High School, Hershey, Pennsylvania, U.S.A.|-id=450| 26450 Tanyapetach ||  || 26450 Tanyapetach Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tanya Nicole Petach (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science project. She attends the Fairview High School, Boulder, Colorado, U.S.A.|-id=451| 26451 Khweis ||  || 26451 Khweis Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Majdolene Ziad Khweis (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her earth-science project. She attends the Taos High School, Taos, New Mexico, U.S.A.|-id=455| 26455 Priyamshah ||  || 26455 Priyamshah Discovered 2000 Jan. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Priyam C. Shah (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for his earth-science team project. He attends the Sunset High School, Portland, Oregon, U.S.A.|-id=457| 26457 Naomishah ||  || 26457 Naomishah Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Naomi C. Shah (b. 1995) was awarded first place in the 2010 Intel International Science and Engineering Fair for her earth-science team project. She attends the Sunset High School, Portland, Oregon, U.S.A.|-id=458| 26458 Choihyuna ||  || 26458 Choihyuna Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Choi Hyun-A (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science team project. She attends the Damyang High School, Damyang-gun, Jeollanam-do, South Korea.|-id=459| 26459 Shinsubin ||  || 26459 Shinsubin Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shin Subin (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science team project. She attends the Damyang High School, Damyang-gun, Jeollanam-do, South Korea.|-id=462| 26462 Albertcui ||  || 26462 Albertcui Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Albert Cui (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering project. He attends the Hillcrest High School, Midvale, Utah, U.S.A.|-id=466| 26466 Zarrin ||  || 26466 Zarrin Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David Andrew Zarrin (b. 1995) was awarded first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering project. He attends the Saratoga High School, Saratoga, California, U.S.A.|-id=467| 26467 Jamespopper ||  || 26467 Jamespopper Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. James Sinclair Popper (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering project. He attends the Marlborough College, Marlborough, Wiltshire, United Kingdom.|-id=468| 26468 Ianchan ||  || 26468 Ianchan Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Ian Chan (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Plano East Senior High School, Plano, Texas, U.S.A.|-id=471| 26471 Tracybecker ||  || Tracy Michelle Becker (b. 1986) determined the shapes of the components of asteroid , the first triple-asteroid system discovered in the near-Earth population. She did this work as a student working at the Arecibo Observatory, earning a Ph.D. in 2016. |-id=474| 26474 Davidsimon ||  || 26474 Davidsimon Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David Szabolcs Simon (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Szent Margit Secondary School, Budapest, Hungary.|-id=475| 26475 Krisztisugar ||  || 26475 Krisztisugar Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Krisztina Sugar (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for her electrical- and mechanical-engineering team project. She attends the Szent Margit Secondary School, Budapest, Hungary.|-id=478| 26478 Cristianrosu ||  || 26478 Cristianrosu Discovered 2000 Jan. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Cristian Emilian Rosu (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Emanuil Gojdu National College, Oradea, Bihor, Romania.|-id=488| 26488 Beiser ||  || 26488 Beiser Discovered 2000 Jan. 7 by the Lowell Observatory Near-Earth Object Search at the Anderson Mesa Station. Antoinette S. Beiser (b. 1956), Lowell Observatory's librarian for twenty years, now concentrates on fundraising.|-id=493| 26493 Paulsucala ||  || 26493 Paulsucala Discovered 2000 Jan. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Paul Stelian Sucala (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Silvania National College, Zalau, Rhode Island, U.S.A.|-id=495| 26495 Eichorn ||  || Will Eichorn (b. 1943), an amateur astronomer and retired Dow Chemical optical technician, living in Bay City, Michigan. |-id=498| 26498 Dinotina ||  || Dino and Tina Grifoni, uncle and aunt of Andrea Boattini †|-id=500| 26500 Toshiohino ||  || Toshio Hino, Japanese astronomer |}

text: 26401 Sobotište

text: || 1999 WX ||

text: Sobotište

text: , a village in southwestern Slovakia, home of an astronomical observatory |-id=411|

text: 26411 Jocorbferg

text: ||  || 26411 Jocorbferg Discovered 1999 Dec. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joseph Corbett Ferguson (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology team project. He attends the Paul Laurence Dunbar High School, Lexington, Kentucky, U.S.A.|-id=412|

text: 26412 Charlesyu

text: ||  || 26412 Charlesyu Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Charles Cheng Yu (b. 1994) was awarded first place in the 2010 Intel International Science and Engineering Fair for his cellular- and molecular-biology team project. He attends the Wheatley School, Old Westbury, New York, U.S.A.|-id=414|

text: 26414 Amychyao

text: ||  || 26414 Amychyao Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Amy Cindy Chyao (b. 1994) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her chemistry project. She attends the Williams High School, Plano, Texas, U.S.A.|-id=417|

text: 26417 Michaelgord

text: ||  || 26417 Michaelgord Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Aaron Gord (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry project. He attends the Dayton Christian High School, Miamisburg, Ohio, U.S.A.|-id=422|

text: 26422 Marekbuchman

text: ||  || 26422 Marekbuchman Discovered 1999 Dec. 12 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Marek Buchman (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry project. He attends the School for Extraordinary Gifted Children, Bratislava, Slovakia.|-id=424|

text: 26424 Jacquelihung

text: ||  || 26424 Jacquelihung Discovered 1999 Dec. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Hung Jacqueline (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for her chemistry team project. She attends the Taipei Municipal First Girls' Senior High School, Taipei City, Chinese Taipei.|-id=425|

text: 26425 Linchichieh

text: ||  || 26425 Linchichieh Discovered 1999 Dec. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Lin Chi-Chieh (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for her chemistry team project. She attends the Taipei Municipal First Girls' Senior High School, Taipei City, Chinese Taipei.|-id=426|

text: 26426 Koechl

text: ||  || 26426 Koechl Discovered 1999 Dec. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Juergen Koechl (b. 1990) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry team project. He attends the HTL Braunau am Inn, Braunau am Inn, Austria.|-id=429|

text: 26429 Andiwagner

text: ||  || 26429 Andiwagner Discovered 1999 Dec. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Andreas Wagner (b. 1990) was awarded second place in the 2010 Intel International Science and Engineering Fair for his chemistry team project. He attends the HTL Braunau am Inn, Braunau am Inn, Austria.|-id=430|

text: 26430 Thomwilkason

text: ||  || 26430 Thomwilkason Discovered 1999 Dec. 10 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Thomas Frederick Wilkason (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his computer-science project. He attends the Mount de Sales Academy, Macon, Georgia, U.S.A.|-id=433|

text: 26433 Michaelyurko

text: ||  || 26433 Michaelyurko Discovered 1999 Dec. 14 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Michael Christopher Yurko (b. 1993) was awarded second place in the 2010 Intel International Science and Engineering Fair for his computer-science project. He attends the Detroit Catholic Central High School, Novi, Michigan, U.S.A.|-id=441|

text: 26441 Nanayakkara

text: ||  || 26441 Nanayakkara Discovered 2000 Jan. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Ganindu Nanayakkara (b. 1990) was awarded first place in the 2010 Intel International Science and Engineering Fair for his computer-science project. He attends the Ananda College, Colombo, Sri Lanka.|-id=442|

text: 26442 Matfernandez

text: ||  || 26442 Matfernandez Discovered 2000 Jan. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Matthew Fernandez (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his computer-science team project. He attends the Oregon Episcopal School, Portland, Oregon, U.S.A.|-id=447|

text: 26447 Akrishnan

text: ||  || 26447 Akrishnan Discovered 2000 Jan. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Akash Krishnan (b. 1994) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his computer-science team project. He attends the Oregon Episcopal School, Portland, Oregon, U.S.A.|-id=448|

text: 26448 Tongjili

text: ||  || 26448 Tongjili Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tongji Li (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science project. She attends the Hershey High School, Hershey, Pennsylvania, U.S.A.|-id=450|

text: 26450 Tanyapetach

text: ||  || 26450 Tanyapetach Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Tanya Nicole Petach (b. 1994) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science project. She attends the Fairview High School, Boulder, Colorado, U.S.A.|-id=451|

text: 26451 Khweis

text: ||  || 26451 Khweis Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Majdolene Ziad Khweis (b. 1993) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for her earth-science project. She attends the Taos High School, Taos, New Mexico, U.S.A.|-id=455|

text: 26455 Priyamshah

text: ||  || 26455 Priyamshah Discovered 2000 Jan. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Priyam C. Shah (b. 1992) was awarded first place in the 2010 Intel International Science and Engineering Fair for his earth-science team project. He attends the Sunset High School, Portland, Oregon, U.S.A.|-id=457|

text: 26457 Naomishah

text: ||  || 26457 Naomishah Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Naomi C. Shah (b. 1995) was awarded first place in the 2010 Intel International Science and Engineering Fair for her earth-science team project. She attends the Sunset High School, Portland, Oregon, U.S.A.|-id=458|

text: 26458 Choihyuna

text: ||  || 26458 Choihyuna Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Choi Hyun-A (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science team project. She attends the Damyang High School, Damyang-gun, Jeollanam-do, South Korea.|-id=459|

text: 26459 Shinsubin

text: ||  || 26459 Shinsubin Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Shin Subin (b. 1992) was awarded second place in the 2010 Intel International Science and Engineering Fair for her earth-science team project. She attends the Damyang High School, Damyang-gun, Jeollanam-do, South Korea.|-id=462|

text: 26462 Albertcui

text: ||  || 26462 Albertcui Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Albert Cui (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering project. He attends the Hillcrest High School, Midvale, Utah, U.S.A.|-id=466|

text: 26466 Zarrin

text: ||  || 26466 Zarrin Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David Andrew Zarrin (b. 1995) was awarded first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering project. He attends the Saratoga High School, Saratoga, California, U.S.A.|-id=467|

text: 26467 Jamespopper

text: ||  || 26467 Jamespopper Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. James Sinclair Popper (b. 1992) was awarded best of category and first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering project. He attends the Marlborough College, Marlborough, Wiltshire, United Kingdom.|-id=468|

text: 26468 Ianchan

text: ||  || 26468 Ianchan Discovered 2000 Jan. 5 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Ian Chan (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Plano East Senior High School, Plano, Texas, U.S.A.|-id=471|

text: 26471 Tracybecker

text: ||  || Tracy Michelle Becker (b. 1986) determined the shapes of the components of asteroid , the first triple-asteroid system discovered in the near-Earth population. She did this work as a student working at the Arecibo Observatory, earning a Ph.D. in 2016. |-id=474|

text: 26474 Davidsimon

text: ||  || 26474 Davidsimon Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David Szabolcs Simon (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Szent Margit Secondary School, Budapest, Hungary.|-id=475|

text: 26475 Krisztisugar

text: ||  || 26475 Krisztisugar Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Krisztina Sugar (b. 1991) was awarded second place in the 2010 Intel International Science and Engineering Fair for her electrical- and mechanical-engineering team project. She attends the Szent Margit Secondary School, Budapest, Hungary.|-id=478|

text: 26478 Cristianrosu

text: ||  || 26478 Cristianrosu Discovered 2000 Jan. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Cristian Emilian Rosu (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Emanuil Gojdu National College, Oradea, Bihor, Romania.|-id=488|

text: 26488 Beiser

text: ||  || 26488 Beiser Discovered 2000 Jan. 7 by the Lowell Observatory Near-Earth Object Search at the Anderson Mesa Station. Antoinette S. Beiser (b. 1956), Lowell Observatory's librarian for twenty years, now concentrates on fundraising.|-id=493|

text: 26493 Paulsucala

text: ||  || 26493 Paulsucala Discovered 2000 Jan. 30 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Paul Stelian Sucala (b. 1991) was awarded first place in the 2010 Intel International Science and Engineering Fair for his electrical- and mechanical-engineering team project. He attends the Silvania National College, Zalau, Rhode Island, U.S.A.|-id=495|

text: 26495 Eichorn

text: ||  || Will Eichorn (b. 1943), an amateur astronomer and retired Dow Chemical optical technician, living in

text: Bay City, Michigan

text: . |-id=498|

text: 26498 Dinotina

text: ||  || Dino and Tina Grifoni, uncle and aunt of

text: Andrea Boattini

text: 26500 Toshiohino

text: Toshio Hino

text: , Japanese astronomer |}

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answers: 26411 Jocorbferg

answers: NDQ_003822

answers: 26411 Jocorbferg was discovered on Dec. 6, 1999, by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro.

answers: NDQ_003823

answers: 26411 Jocorbferg

answers: NDQ_003824

answers: |-id=411| 26411 Jocorbferg

answers: NDQ_003825

answers: 26411 Jocorbferg was discovered on Dec. 6, 1999, by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro.

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: a village in southwestern Slovakia, home of an astronomical observatory

answers: NDQ_003828

answers: || 26411 Jocorbferg

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct.

answers: NDQ_003830

answers: Near-Earth Asteroid Research Team

text: In 1998, the United States Congress mandated the Spaceguard Survey – detection of 90% of near-earth asteroids over 1 km diameter (that threaten global devastation) by 2008. Several surveys have undertaken "Spaceguard" activities (an umbrella term), including Lincoln Near-Earth Asteroid Research (LINEAR), Spacewatch, Near-Earth Asteroid Tracking (NEAT), Lowell Observatory Near-Earth-Object Search (LONEOS), Catalina Sky Survey (CSS), Campo Imperatore Near-Earth Object Survey (CINEOS), Japanese Spaceguard Association, Asiago-DLR Asteroid Survey (ADAS) and Near-Earth Object WISE (NEOWISE). In 2011, it was estimated that 93% of near-Earth asteroids larger than 1 km in diameter have been found, thus the original Spaceguard goal has been met. In 2005, in the USA, the original Spaceguard mandate was extended by the George E. Brown, Jr. Near-Earth Object Survey Act, which calls for NASA to detect 90% of NEOs with diameters of 140 meters or greater, by 2020.

text: In 1998, the

text: United States Congress

text: mandated the Spaceguard Survey – detection of 90% of near-earth asteroids over 1 km diameter (that threaten global devastation) by 2008. Several

text: surveys

text: have undertaken "

text: Spaceguard

text: " activities (an umbrella term), including

text: Lincoln Near-Earth Asteroid Research

text: (LINEAR),

text: Spacewatch

text: Near-Earth Asteroid Tracking

text: (NEAT),

entity_name: Lowell Observatory Near-Earth-Object Search

text: Lowell Observatory Near-Earth-Object Search

text: (LONEOS),

text: Catalina Sky Survey

text: (CSS),

entity_name: Campo Imperatore Near-Earth Object Survey

text: Campo Imperatore Near-Earth Object Survey

text: (CINEOS),

text: Japanese Spaceguard Association

text: Asiago-DLR Asteroid Survey

text: (ADAS) and

text: Near-Earth Object WISE

text: (NEOWISE). In 2011, it was estimated that 93% of near-Earth asteroids larger than 1 km in diameter have been found, thus the original Spaceguard goal has been met. In 2005, in the USA, the original Spaceguard mandate was extended by the George E. Brown, Jr. Near-Earth Object Survey Act, which calls for NASA to detect 90% of NEOs with diameters of 140 meters or greater, by 2020.

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answers: threaten global devastation

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answers: Mars

answers: NDQ_003829

answers: Threaten global devastation

answers: NDQ_003830

answers: threaten global devastation

text: Based on observations by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid has an albedo of 0.128 and 0.122 with a diameter of  9.3 and 9.1 kilometers, respectively. The Collaborative Asteroid Lightcurve Link (CALL) calculates a smaller diameter of 5.4 kilometers based on an assumed albedo of 0.20, untypically high for a carbonaceous asteroid.

text: Based on observations by the Japanese

text: Akari

text: satellite and the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid has an

text: albedo

text: of 0.128 and 0.122 with a diameter of  9.3 and 9.1 kilometers, respectively. The Collaborative Asteroid Lightcurve Link (CALL) calculates a smaller diameter of 5.4 kilometers based on an assumed albedo of 0.20, untypically high for a

text: carbonaceous

text: asteroid.

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answers: carbonaceous

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answers: carbonaceous

answers: NDQ_003823

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003824

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003825

answers: carbonaceous

answers: NDQ_003826

answers: asteroid belt

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answers: carbonaceous

answers: NDQ_003828

answers: untypically high

answers: NDQ_003829

answers: The Collaborative Asteroid Lightcurve Link

answers: NDQ_003830

answers: carbonaceous asteroid

text: Near-Earth asteroids, or NEAs, are asteroids that have orbits that pass close to that of Earth. Asteroids that actually cross Earth's orbital path are known as Earth-crossers. , 14,464 near-Earth asteroids are known and the number over one kilometre in diameter is estimated to be 900–1,000.

text: Near-Earth asteroids, or NEAs, are asteroids that have orbits that pass close to that of Earth. Asteroids that actually cross Earth's orbital path are known as Earth-crossers. , 14,464 near-Earth asteroids are known and the number over one kilometre in diameter is estimated to be 900–1,000.

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answers: 0

answers: NDQ_003821

answers: one kilometre in diameter

answers: NDQ_003822

answers: Near-Earth asteroids

answers: NDQ_003823

answers: Earth-crossers

answers: NDQ_003824

answers: 14,464 near-Earth asteroids are known

answers: NDQ_003825

answers: Near-Earth asteroids

answers: NDQ_003826

answers: Near-Earth

answers: NDQ_003827

answers: Earth-crossers

answers: NDQ_003828

answers: Earth-crossers

answers: NDQ_003829

answers: Asteroids that actually cross Earth's orbital path

answers: NDQ_003830

answers: Earth-crossers

text: |-id=468| 121468 Msovinskihaskell ||  || Marjorie (Sovinski) Haskell (b. 1979) is the Materials and Processes Engineer for the OSIRIS-REx Asteroid Sample Return Mission and the OVIRS instrument. Prior to OSIRIS-REx, she served as the MPE for the SMAP Radiometer and has also supported the Solar Orbiter, LCRD, and ASTRO-H programs as MPE.|-id=479| 121479 Hendershot ||  || James Hendershot (b. 1957), the Payload Team Instrument Manager at Goddard Space Flight Center for the OCAMS and OTES instruments on the OSIRIS-REx Asteroid Sample Return Mission. |-id=480| 121480 Dolanhighsmith ||  || Dolan E. Highsmith (b. 1970) contributed to the Navigation Teams of the ESA Mars Express mission and the NASA MRO, MSL, MAVEN and OSIRIS-REx missions. |-id=481| 121481 Reganhoward ||  || Regan Howard (b. 1948) contributed to the OSIRIS-REx Asteroid Sample Return mission as the Electromagnetics Compatibility Lead. He is a member of the MAVEN flight team. He was a systems engineer on the MAVEN Mars Scout mission and on the development teams for the Dawn, MESSENGER and ICESat-1 missions. |-id=483| 121483 Griffinjayne ||  || Griffin Owen Jayne (b. 1992) contributed to the NASA OSIRIS-REx Asteroid Sample Return mission as Contamination Control Engineer. He also works as a Thermal Coatings Development Engineer, helping to improve existing coatings and develop new coatings to better meet mission thermal requirements. |-id=486| 121486 Sarahkirby ||  || Sarah Kirby Smith (b. 1982) is the Earned Value Management Specialist for the OSIRIS-REx Asteroid Sample Return Mission. She also worked at the Naval Air Systems Command on the F35 Joint Strike Fighter and at Lockheed Martin on the Littoral Combat Ship and Non-Line of Sight Launch System projects.|}

text: 121468 Msovinskihaskell

text: ||  || Marjorie (Sovinski) Haskell (b. 1979) is the Materials and Processes Engineer for the OSIRIS-REx Asteroid Sample Return Mission and the OVIRS instrument. Prior to OSIRIS-REx, she served as the MPE for the SMAP Radiometer and has also supported the Solar Orbiter, LCRD, and ASTRO-H programs as MPE.|-id=479|

text: 121479 Hendershot

text: ||  || James Hendershot (b. 1957), the Payload Team Instrument Manager at Goddard Space Flight Center for the OCAMS and OTES instruments on the OSIRIS-REx Asteroid Sample Return Mission. |-id=480|

text: 121480 Dolanhighsmith

text: ||  || Dolan E. Highsmith (b. 1970) contributed to the Navigation Teams of the ESA Mars Express mission and the NASA MRO, MSL, MAVEN and OSIRIS-REx missions. |-id=481|

text: 121481 Reganhoward

text: ||  || Regan Howard (b. 1948) contributed to the OSIRIS-REx Asteroid Sample Return mission as the Electromagnetics Compatibility Lead. He is a member of the MAVEN flight team. He was a systems engineer on the MAVEN Mars Scout mission and on the development teams for the Dawn, MESSENGER and ICESat-1 missions. |-id=483|

text: 121483 Griffinjayne

text: ||  || Griffin Owen Jayne (b. 1992) contributed to the NASA OSIRIS-REx Asteroid Sample Return mission as Contamination Control Engineer. He also works as a Thermal Coatings Development Engineer, helping to improve existing coatings and develop new coatings to better meet mission thermal requirements. |-id=486|

text: 121486 Sarahkirby

text: ||  || Sarah Kirby Smith (b. 1982) is the Earned Value Management Specialist for the OSIRIS-REx Asteroid Sample Return Mission. She also worked at the Naval Air Systems Command on the F35 Joint Strike Fighter and at Lockheed Martin on the Littoral Combat Ship and Non-Line of Sight Launch System projects.|}

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

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answers: 4: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

answers: tqa2:L_0095/T_0928/49cd92b788121957eb5e274ffc82abe5

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

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answers: 4

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answers: 0

answers: NDQ_003821

answers: 0

answers: NDQ_003822

answers: 5: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 3

answers: NDQ_003825

answers: 5: The answer is mostly relevant and complete, with noticeable gaps or inaccuracies.

answers: NDQ_003826

answers: 0

answers: NDQ_003827

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

answers: NDQ_003828

answers: 0

answers: NDQ_003829

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

answers: NDQ_003830

answers: 4

answers: NDQ_003821

answers: NASA's OSIRIS-REx Asteroid Sample Return Mission.

answers: NDQ_003822

answers: OSIRIS-REx mission

answers: NDQ_003823

answers: Asteroids are too small to have impacts with other objects so they don't have craters.

answers: NDQ_003824

answers: REx Asteroid Sample Return Mission.

answers: NDQ_003825

answers: OSIRIS-REx mission

answers: NDQ_003826

answers: Mars Orbiter

answers: NDQ_003827

answers: Space Center.

answers: NDQ_003828

answers: x Asteroid Sample Return mission.

answers: NDQ_003829

answers: formerly served as a systems engineer on the MAVEN Mars Scout mission.

answers: NDQ_003830

answers: NASA Goddard Space Flight Center

text: Based on an absolute magnitude of 17.3, the asteroid is calculated to measure between 1 and 2 kilometers in diameter, assuming an albedo in the range of 0.05 to 0.25. Since asteroids in the inner main-belt are often of a silicaceous rather than of a carbonaceous composition, with higher albedos, typically around 0.20, the asteroid's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter at a constant absolute magnitude (brightness).

text: Based on an absolute

text: magnitude

text: of 17.3, the asteroid is calculated to measure between 1 and 2 kilometers in diameter, assuming an

text: albedo

text: in the range of 0.05 to 0.25. Since asteroids in the inner main-belt are often of a

text: silicaceous

text: rather than of a

text: carbonaceous

text: composition, with higher albedos, typically around 0.20, the asteroid's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter at a constant absolute magnitude (brightness).

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answers: 0

answers: NDQ_003821

answers: 4

answers: NDQ_003822

answers: 4

answers: NDQ_003823

answers: 0

answers: NDQ_003824

answers: 2

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: 4

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: 1 and 2 kilometers in diameter

answers: NDQ_003822

answers: the inner main-belt

answers: NDQ_003823

answers: asteroids in the inner main-belt

answers: NDQ_003824

answers: Based on an absolute magnitude of 17.3, the asteroid is calculated to measure between 1 and 2 kilometers in diameter

answers: NDQ_003825

answers: the inner main-belt

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: higher albedos

answers: NDQ_003828

answers: The asteroid is calculated to measure between 1 and 2 kilometers in diameter

answers: NDQ_003829

answers: Based on an absolute magnitude of 17.3

answers: NDQ_003830

answers: asteroids

text: Based on an absolute magnitude of 16.5, the asteroid is calculated to measure between 1 and 3 kilometers in diameter, assuming an albedo in the range of 0.05 to 0.25. Since asteroids in the inner main-belt are often of a silicaceous rather than of a carbonaceous composition, with higher albedos, typically around 0.20, the asteroid's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter, for a given absolute magnitude (brightness).

text: Based on an absolute

text: magnitude

text: of 16.5, the asteroid is calculated to measure between 1 and 3 kilometers in diameter, assuming an

text: albedo

text: in the range of 0.05 to 0.25. Since asteroids in the inner main-belt are often of a

text: silicaceous

text: rather than of a

text: carbonaceous

text: composition, with higher albedos, typically around 0.20, the asteroid's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter, for a given absolute magnitude (brightness).

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answers: NDQ_003821

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answers: NDQ_003821

answers: 1 and 3 kilometers in diameter

answers: NDQ_003822

answers: in the inner main-belt

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: Based on an absolute magnitude of 16.5, the asteroid is calculated to measure between 1 and 3 kilometers in diameter

answers: NDQ_003825

answers: in the inner main-belt

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: higher albedos, typically around 0.20

answers: NDQ_003828

answers: The asteroid is calculated to measure between 1 and 3 kilometers

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: asteroids

text: The first Japanese asteroid probe, Hayabusa, returned to Earth on 13 June, having landed on 25143 Itokawa in an effort to collect samples. It was also the world's first successful sample return mission from an asteroid.

text: The first Japanese

text: asteroid

text: probe,

text: Hayabusa

text: , returned to Earth on 13 June, having landed on

text: 25143 Itokawa

text: in an effort to collect samples. It was also the world's first successful

text: sample return mission

text: from an asteroid.

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answers: NDQ_003821

answers: probe

answers: NDQ_003822

answers: 25143 Itokawa

answers: NDQ_003823

answers: Itokawa

answers: NDQ_003824

answers: The first Japanese asteroid probe

answers: NDQ_003825

answers: 25143 Itokawa

answers: NDQ_003826

answers: Earth

answers: NDQ_003827

answers: landed

answers: NDQ_003828

answers: 25143 Itokawa

answers: NDQ_003829

answers: The first Japanese asteroid probe

answers: NDQ_003830

answers: samples

text: Jupiter-family comets and long-period comets appear to follow very different fading laws. The JFCs are active over a lifetime of about 10,000 years or ~1,000 orbits whereas long-period comets fade much faster. Only 10% of the long-period comets survive more than 50 passages to small perihelion and only 1% of them survive more than 2,000 passages. Eventually most of the volatile material contained in a comet nucleus evaporates, and the comet becomes a small, dark, inert lump of rock or rubble that can resemble an asteroid. Some asteroids in elliptical orbits are now identified as extinct comets. Roughly six percent of the near-Earth asteroids are thought to be extinct comet nuclei.

text: Jupiter-family comets and long-period comets appear to follow very different fading laws. The JFCs are active over a lifetime of about 10,000 years or ~1,000 orbits whereas long-period comets fade much faster. Only 10% of the long-period comets survive more than 50 passages to small perihelion and only 1% of them survive more than 2,000 passages. Eventually most of the volatile material contained in a comet nucleus evaporates, and the comet becomes a small, dark, inert lump of rock or rubble that can resemble an

text: asteroid

text: . Some asteroids in elliptical orbits are now identified as extinct comets. Roughly six percent of the near-Earth asteroids are thought to be extinct comet nuclei.

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answers: small, dark, inert lump of rock or rubble

answers: NDQ_003822

answers: can resemble an asteroid

answers: NDQ_003823

answers: Eventually most of the volatile material contained in a comet nucleus evaporates

answers: NDQ_003824

answers: Eventually most of the volatile material contained in a comet nucleus evaporates

answers: NDQ_003825

answers: can resemble an asteroid

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answers: perihelion

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answers: extinct comet nuclei

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answers: The JFCs

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: comet nuclei

text: is an Amor near-Earth asteroid  in diameter. It was discovered on August 19, 1998, by the Lincoln Near Earth Asteroid Research (LINEAR) program located near Socorro, New Mexico.  has an observation arc of 14 years and a well-determined orbit.

text: is an

text: Amor

text: near-Earth asteroid

text: in diameter. It was discovered on August 19, 1998, by the

text: Lincoln Near Earth Asteroid Research

text: (LINEAR) program located near

text: Socorro, New Mexico

text: .  has an observation arc of 14 years and a well-determined

text: orbit

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answers: diameter

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answers: near-Earth

answers: NDQ_003823

answers: It was discovered on August 19, 1998

answers: NDQ_003824

answers: It was discovered on August 19, 1998

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: Near Earth

answers: NDQ_003827

answers: orbit

answers: NDQ_003828

answers: Mars

answers: NDQ_003829

answers: Asteroid could cause humans to go extinct

answers: NDQ_003830

answers: Near Earth Asteroid Research

text: A gravitational keyhole is a tiny region of space where a planet's gravity would alter the orbit of a passing asteroid such that the asteroid would collide with that planet on a given future orbital pass. The word "keyhole" contrasts the large uncertainty of trajectory calculations (between the time of the observations of the asteroid and the first encounter with the planet) with the relatively narrow bundle(s) of critical trajectories. The term was coined by P. W. Chodas in 1999. It gained some public interest when it became clear, in January 2005, that the Asteroid (99942) Apophis would miss the Earth in 2029 but may go through one or another keyhole leading to impacts in 2036 or 2037. Further research has since been done, however, which revealed the probability of the asteroid passing through the keyhole was extremely insignificant.

text: A gravitational keyhole is a tiny region of space where a planet's gravity would alter the orbit of a passing

text: asteroid

text: such that the asteroid would collide with that planet on a given future orbital pass. The word "keyhole" contrasts the large uncertainty of

text: trajectory calculations

text: (between the time of the observations of the asteroid and the first encounter with the planet) with the relatively narrow bundle(s) of critical trajectories. The term was coined by P. W. Chodas in 1999. It gained some public interest when it became clear, in January 2005, that the Asteroid

text: (99942) Apophis

text: would miss the Earth in 2029 but may go through one or another keyhole leading to impacts in 2036 or 2037. Further research has since been done, however, which revealed the probability of the asteroid passing through the keyhole was extremely insignificant.

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answers: passing

answers: NDQ_003822

answers: gravitational keyhole

answers: NDQ_003823

answers: Asteroid (99942) Apophis

answers: NDQ_003824

answers: It gained some public interest when it became clear, in January 2005, that the Asteroid (99942) Apophis would miss the Earth in 2029

answers: NDQ_003825

answers: gravitational keyhole

answers: NDQ_003826

answers: space

answers: NDQ_003827

answers: collide with that planet

answers: NDQ_003828

answers: Asteroid (99942) Apophis

answers: NDQ_003829

answers: However, which revealed the probability of the asteroid passing through the keyhole was extremely insignificant

answers: NDQ_003830

answers: keyhole

text: Asteroid Bennu is a B-type asteroid which is the target of the OSIRIS-REx mission. The mission seeks to characterize the asteroid by mapping the surface, studying the Yarkovsky Effect, and retrieving a sample of the asteroid to return in 2023. The spacecraft will launch in 2016.

text: Asteroid

text: Bennu

text: is a B-type asteroid which is the target of the

text: OSIRIS-REx

text: mission. The mission seeks to characterize the asteroid by mapping the surface, studying the

text: Yarkovsky Effect

text: , and retrieving a sample of the asteroid to return in 2023. The spacecraft will launch in 2016.

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answers: NDQ_003821

answers: B-type asteroid

answers: NDQ_003822

answers: B-type

answers: NDQ_003823

answers: The Yarkovsky Effect

answers: NDQ_003824

answers: The spacecraft will launch in 2016.

answers: NDQ_003825

answers: B-type

answers: NDQ_003826

answers: B-type

answers: NDQ_003827

answers: Yarkovsky Effect

answers: NDQ_003828

answers: Asteroid Bennu is a B-type asteroid

answers: NDQ_003829

answers: The Yarkovsky Effect

answers: NDQ_003830

answers: the Yarkovsky Effect

text: As their orbits evolved many of the E-belt asteroids would have acquired orbits similar to those of the Hungaria asteroids with high inclinations and semimajor axis between 1.8 and 2.0 AU.  Because orbits in this region are dynamically sticky these objects would form a quasi-stable reservoir.  As this population of the E-belt asteroids leaked from this reservoir they would produce a long-lived tail of impacts after the traditional end of the late heavy bombardment at 3.7 billion years ago.  A remnant representing roughly 0.1 – 0.4% of the original E-belt asteroids would remain as the current Hungaria asteroids.

text: As their orbits evolved many of the E-belt asteroids would have acquired orbits similar to those of the

text: Hungaria asteroids

text: with high inclinations and semimajor axis between 1.8 and 2.0 AU.  Because orbits in this region are dynamically sticky these objects would form a quasi-stable reservoir.  As this population of the E-belt asteroids leaked from this reservoir they would produce a long-lived tail of impacts after the traditional end of the late heavy bombardment at 3.7 billion years ago.  A remnant representing roughly 0.1 – 0.4% of the original E-belt asteroids would remain as the current Hungaria asteroids.

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answers: NDQ_003821

answers: objects

answers: NDQ_003822

answers: Hungaria

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroids are too small for nasa missions to visit them

answers: NDQ_003825

answers: Hungaria

answers: NDQ_003826

answers: E-belt

answers: NDQ_003827

answers: impact

answers: NDQ_003828

answers: 3.7 billion years ago

answers: NDQ_003829

answers: Because orbits in this region are dynamically sticky

answers: NDQ_003830

answers: Hungaria asteroids

text: Arthur C. Clarke coined the term in his novel Rendezvous with Rama (1972) where SPACEGUARD was the name of an early warning system created following a catastrophic asteroid impact. This name was later adopted by a number of real life efforts to discover and study near-Earth objects.A 1992 US Congressional study produced a "Spaceguard Survey Report" which led to a mandate that NASA locate 90% of near-Earth asteroids larger than 1 km within 10 years.  This is often referred to as the "Spaceguard Goal."  A number of efforts which receive money through NASA are all considered to be working on the "Spaceguard Project."

text: Arthur C. Clarke

text: coined the term in his novel

text: Rendezvous with Rama

text: (1972) where SPACEGUARD was the name of an early warning system created following a catastrophic

text: asteroid impact

text: . This name was later adopted by a number of real life efforts to discover and study near-

text: Earth

text: objects.A 1992

text: US Congressional

text: study produced a "Spaceguard Survey Report" which led to a mandate that

text: NASA

text: locate 90% of near-Earth

text: asteroid

text: s larger than 1 km within 10 years.  This is often referred to as the "Spaceguard Goal."  A number of efforts which receive money through NASA are all considered to be working on the "Spaceguard Project."

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answers: larger than 1 km

answers: NDQ_003822

answers: near-Earth objects

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answers: NDQ_003824

answers: Spaceguard Survey Report

answers: NDQ_003825

answers: near-Earth objects

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answers: catastrophic asteroid impact

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answers: catastrophic asteroid impact

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answers: SPACEGUARD

text: In 1975, an asteroid taxonomic system based on color, albedo, and spectral shape was developed by Clark R. Chapman, David Morrison, and Ben Zellner. These properties are thought to correspond to the composition of the asteroid's surface material. The original classification system had three categories: C-types for dark carbonaceous objects (75% of known asteroids), S-types for stony (silicaceous) objects (17% of known asteroids) and U for those that did not fit into either C or S. This classification has since been expanded to include many other asteroid types. The number of types continues to grow as more asteroids are studied.

text: In 1975, an asteroid

text: taxonomic

text: system based on

text: color

text: albedo

text: , and

text: spectral shape

text: was developed by

text: Clark R. Chapman

text: David Morrison

text: , and

text: Ben Zellner

text: . These properties are thought to correspond to the composition of the asteroid's surface material. The original classification system had three categories:

text: C-types

text: for dark carbonaceous objects (75% of known asteroids),

text: S-types

text: for stony (silicaceous) objects (17% of known asteroids) and U for those that did not fit into either C or S. This classification has since been expanded to include many other asteroid types. The number of types continues to grow as more asteroids are studied.

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answers: objects

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answers: 75% of known asteroids

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroid taxonomic system

answers: NDQ_003825

answers: 75% of known asteroids

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: carbonaceous

answers: NDQ_003828

answers: Mars

answers: NDQ_003829

answers: The number of types continues to grow as more asteroids are studied

answers: NDQ_003830

answers: taxonomic system

text: Asteroids are differentiated from comets and meteoroids. In the case of comets, the difference is one of composition: while asteroids are mainly composed of mineral and rock, comets are composed of dust and ice. In addition, asteroids formed closer to the sun, preventing the development of the aforementioned cometary ice. The difference between asteroids and meteoroids is mainly one of size: meteoroids have a diameter of less than one meter, whereas asteroids have a diameter of greater than one meter. Finally, meteoroids can be composed of either cometary or asteroidal materials.

text: Asteroids are differentiated from

text: comet

text: s and

text: meteoroid

text: s. In the case of comets, the difference is one of composition: while asteroids are mainly composed of mineral and rock, comets are composed of dust and ice. In addition, asteroids formed closer to the sun, preventing the development of the aforementioned cometary ice. The difference between asteroids and meteoroids is mainly one of size: meteoroids have a diameter of less than one meter, whereas asteroids have a diameter of greater than one meter. Finally, meteoroids can be composed of either cometary or asteroidal materials.

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answers: formed closer to the sun

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answers: Asteroids are different from comets and meteoroids

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answers: comets

text: There is increasing interest in identifying asteroids whose orbits cross Earth's, and that could, given enough time, collide with Earth (see Earth-crosser asteroids). The three most important groups of near-Earth asteroids are the Apollos, Amors, and Atens. Various asteroid deflection strategies have been proposed, as early as the 1960s.

text: There is increasing interest in identifying asteroids whose orbits cross

text: Earth

text: 's, and that could, given enough time, collide with Earth (see

text: Earth-crosser asteroids

text: ). The three most important groups of

text: near-Earth asteroid

text: s are the

text: Apollos

text: Amors

text: , and

text: Atens

text: . Various

text: asteroid deflection strategies

text: have been proposed, as early as the 1960s.

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answers: near-Earth

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answers: Earth-crosser asteroids

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answers: asteroids

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answers: There is increasing interest in identifying asteroids

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answers: Earth-crosser asteroids

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answers: near-Earth

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answers: collide with Earth

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answers: Earth-crosser asteroids

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answers: could, given enough time, collide with Earth

text: The only other unambiguously identified triple asteroid in the near-Earth population is (136617) 1994 CC, which was discovered to be a triple system in 2009.

text: The only other unambiguously identified triple asteroid in the near-Earth population is

text: (136617) 1994 CC

text: , which was discovered to be a triple system in 2009.

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

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answers: unambiguously identified

answers: NDQ_003822

answers: asteroid

answers: NDQ_003823

answers: (136617) 1994 CC

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answers: (136617) 1994 CC

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answers: asteroid

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answers: near-Earth population

answers: NDQ_003827

answers: triple system

answers: NDQ_003828

answers: (136617) 1994 CC

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answers: (136617) 1994 CC

answers: NDQ_003830

answers: triple system

text: NEAs survive in their orbits for just a few million years. They are eventually eliminated by planetary perturbations, causing ejection from the Solar System or a collision with the Sun or a planet. With orbital lifetimes short compared to the age of the Solar System, new asteroids must be constantly moved into near-Earth orbits to explain the observed asteroids. The accepted origin of these asteroids is that asteroid-belt asteroids are moved into the inner Solar System through orbital resonances with Jupiter. The interaction with Jupiter through the resonance perturbs the asteroid's orbit and it comes into the inner Solar System. The asteroid belt has gaps, known as Kirkwood gaps, where these resonances occur as the asteroids in these resonances have been moved onto other orbits. New asteroids migrate into these resonances, due to the Yarkovsky effect that provides a continuing supply of near-Earth asteroids. The known asteroid with the greatest known chance of impacting Earth is  with a 1 in 16 chance of impacting Earth on 5 September 2095. Its 7-meter estimated diameter ensures that an impact would cause little damage.

text: NEAs survive in their orbits for just a few million years. They are eventually eliminated by planetary

text: perturbations

text: , causing ejection from the Solar System or a

text: collision

text: with the Sun or a planet. With orbital lifetimes short compared to the age of the Solar System, new asteroids must be constantly moved into near-Earth orbits to explain the observed asteroids. The accepted origin of these asteroids is that

text: asteroid-belt asteroids

text: are moved into the inner Solar System through

text: orbital resonance

text: s with

text: Jupiter

text: . The interaction with Jupiter through the resonance

text: perturb

text: s the asteroid's orbit and it comes into the inner Solar System. The asteroid belt has gaps, known as

text: Kirkwood gap

text: s, where these resonances occur as the asteroids in these resonances have been moved onto other orbits. New asteroids migrate into these resonances, due to the

text: Yarkovsky effect

text: that provides a continuing supply of near-Earth asteroids. The known asteroid with the greatest known chance of impacting Earth is  with a 1 in 16 chance of impacting Earth on 5 September 2095. Its 7-meter estimated diameter ensures that an impact would cause little damage.

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answers: NEAs

answers: NDQ_003823

answers: An impact would cause little damage

answers: NDQ_003824

answers: With orbital lifetimes short compared to the age of the Solar System

answers: NDQ_003825

answers: NEAs

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: impacting Earth

answers: NDQ_003828

answers: Its 7-meter estimated diameter ensures that an impact would cause little damage

answers: NDQ_003829

answers: Its 7-meter estimated diameter ensures that an impact would cause little damage

answers: NDQ_003830

answers: Earth

text: 1125 China () is a main belt asteroid orbiting the Sun. It makes a revolution around the Sun once every 5 years. It was discovered at the Purple Mountain Observatory, Nanking, on October 30, 1957. Named for the country in which it was discovered, its name and number were actually taken from another asteroid that was considered a lost asteroid at the time, but was eventually rediscovered and given the new designation 3789 Zhongguo (1928 UF). What is now known as 1125 China had a provisional designation: .

text: 1125 China () is a

text: main belt asteroid

text: orbiting the

text: Sun

text: . It makes a revolution around the Sun once every 5 years. It was discovered at the

text: Purple Mountain Observatory

text: Nanking

text: , on October 30, 1957. Named for the

text: country

text: in which it was discovered, its name and number were actually taken from another asteroid that was considered a

text: lost asteroid

text: at the time, but was eventually rediscovered and given the new designation

text: 3789 Zhongguo

text: 1928 UF

text: ). What is now known as 1125 China had a provisional designation: .

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answers: main belt

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answers: orbiting the Sun

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answers: orbiting the Sun

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answers: It orbits the Sun

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answers: 1125 China

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answers: orbiting the Sun

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answers: 1125 China

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answers: NDQ_003830

answers: orbiting the Sun

text: The temperature of the asteroid belt varies with the distance from the Sun. For dust particles within the belt, typical temperatures range from 200 K (−73 °C) at 2.2 AU down to 165 K (−108 °C) at 3.2 AU However, due to rotation, the surface temperature of an asteroid can vary considerably as the sides are alternately exposed to solar radiation and then to the stellar background.

text: The temperature of the asteroid belt varies with the distance from the Sun. For dust particles within the belt, typical temperatures range from 200 K (−73 °C) at 2.2 AU down to 165 K (−108 °C) at 3.2 AU However, due to rotation, the surface temperature of an asteroid can vary considerably as the sides are alternately exposed to solar radiation and then to the stellar background.

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text: Until the advent of space travel, objects in the asteroid belt were merely pinpricks of light in even the largest telescopes, their shapes and terrain remaining a mystery.Several asteroids have now been visited by probes, the first of which was Galileo, which flew past two: 951 Gaspra in 1991, followed by 243 Ida in 1993. Both of these lay near enough to Galileos planned trajectory to Jupiter that they could be visited at acceptable cost. The first landing on an asteroid was performed by the NEAR Shoemaker probe in 2000, following an orbital survey of the object. The dwarf planet Ceres and the asteroid 4 Vesta, two of the three largest asteroids, were visited by NASA's Dawn spacecraft, launched in 2007.

text: Until the advent of

text: space travel

text: , objects in the

text: asteroid belt

text: were merely pinpricks of light in even the largest telescopes, their shapes and terrain remaining a mystery.Several asteroids have now been visited by probes, the first of which was

text: Galileo

text: , which flew past two:

text: 951 Gaspra

text: in 1991, followed by

text: 243 Ida

text: in 1993. Both of these lay near enough to Galileos planned trajectory to Jupiter that they could be visited at acceptable cost. The first landing on an asteroid was performed by the

text: NEAR Shoemaker

text: probe in 2000, following an orbital survey of the object. The dwarf planet

text: Ceres

text: and the asteroid

text: 4 Vesta

text: , two of the three largest asteroids, were visited by NASA's

text: Dawn spacecraft

text: , launched in 2007.

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answers: NASA's Dawn spacecraft, launched in 2007

answers: NDQ_003825

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answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: their shapes and terrain remaining a mystery

text: The Hungaria asteroids are thought to be the remains of the hypothetical E-belt asteroid population.  The dispersal of most of that hypothetical E-belt might have been caused by the outwards migration of the giant planets of the Solar System according to simulations done under the Nice model—and these dispersed E-Belt asteroids might in turn have been the impactors of the Late Heavy Bombardment.

text: The Hungaria asteroids are thought to be the remains of the hypothetical

text: E-belt asteroid population

text: .  The dispersal of most of that hypothetical E-belt might have been caused by the

text: outwards migration

text: of the

text: giant planet

text: s of the

text: Solar System

text: according to simulations done under the

text: Nice model

text: —and these dispersed E-Belt asteroids might in turn have been the impactors of the

text: Late Heavy Bombardment

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answers: asteroids are too small for nasa missions to visit them

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text: In the partial lists, numbered minor planets (MPs) are categorized into one of 8 distinct orbital groups. These are the near-Earth asteroids, the Mars-crossing asteroids, the inner-, middle- and outer main-belt asteroids (MBA), the Jupiter trojans, the centaurs and the trans-Neptunian objects. A minor planet's orbital group is represented by the background color of the table row . This classification is exclusively based on the body's relevant orbital elements, that is, its semi-major axis (a) and eccentricity (e). From these elements its perihelion (q) and aphelion (Q) can be derived.

text: In the partial lists, numbered minor planets (MPs) are categorized into one of 8 distinct orbital groups. These are the

text: near-Earth

text: asteroids, the

text: Mars-crossing

text: asteroids, the inner-, middle- and outer

text: main-belt

text: asteroids (MBA), the

text: Jupiter trojan

text: s, the

text: centaurs

text: and the

text: trans-Neptunian object

text: s. A minor planet's orbital group is represented by the background color of the table row . This classification is exclusively based on the body's relevant orbital elements, that is, its

text: semi-major axis

text: (a) and

text: eccentricity

text: (e). From these elements its

text: perihelion

text: (q) and

text: aphelion

text: (Q) can be derived.

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answers: minor planets

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answers: NDQ_003823

answers: Asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: This classification is exclusively based on the body's relevant orbital elements

answers: NDQ_003825

answers: minor planets

answers: NDQ_003826

answers: trans-Neptunian

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answers: NDQ_003828

answers: Mars-crossing asteroids

answers: NDQ_003829

answers: A minor planet's orbital group is represented by the background color of the table row

answers: NDQ_003830

answers: minor planets

text: In 1967, Professor Paul Sandorff at the Massachusetts Institute of Technology asked his graduate students to come up with a plan to deflect the approximately 1 km wide asteroid 1566 Icarus. An asteroid which was observed to have an orbit bringing it into a close approach pass by Earth in the coming year, curiosity however motivated Sandorff to task his students to come up with a solution to the thought experiment of, What If it-were-on-an-impact-trajectory.

text: In 1967, Professor Paul Sandorff at the

text: Massachusetts Institute of Technology

text: asked his graduate students to come up with a plan to deflect the approximately 1 km wide asteroid

text: 1566 Icarus

text: . An asteroid which was observed to have an orbit bringing it into a close approach pass by Earth in the coming year, curiosity however motivated Sandorff to task his students to come up with a solution to the thought experiment of, What If it-were-on-an-impact-trajectory.

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answers: 1 km wide

answers: NDQ_003822

answers: 1566 Icarus

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: asteroid 1566 Icarus

answers: NDQ_003825

answers: 1566 Icarus

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answers: Earth

answers: NDQ_003827

answers: impact

answers: NDQ_003828

answers: 1566 Icarus

answers: NDQ_003829

answers: 1566 Icarus

answers: NDQ_003830

answers: curiosity

text: (456938)  is a small asteroid that is a Near-Earth object and an Apollo asteroid.

text: (456938)  is a small

text: asteroid

text: that is a

text: Near-Earth object

text: and an

text: Apollo asteroid

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answers: Near-Earth

answers: NDQ_003822

answers: (456938)

answers: NDQ_003823

answers: (456938)

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answers: Near Earth

answers: NDQ_003827

answers: Apollo

answers: NDQ_003828

answers: (456938)

answers: NDQ_003829

answers: (456938) is a small asteroid

answers: NDQ_003830

answers: Apollo asteroid

text: Until the age of space travel, objects in the asteroid belt were merely pinpricks of light in even the largest telescopes and their shapes and terrain remained a mystery. The best modern ground-based telescopes and the Earth-orbiting Hubble Space Telescope can resolve a small amount of detail on the surfaces of the largest asteroids, but even these mostly remain little more than fuzzy blobs. Limited information about the shapes and compositions of asteroids can be inferred from their light curves (their variation in brightness as they rotate) and their spectral properties, and asteroid sizes can be estimated by timing the lengths of star occulations (when an asteroid passes directly in front of a star). Radar imaging can yield good information about asteroid shapes and orbital and rotational parameters, especially for near-Earth asteroids. In terms of delta-v and propellant requirements, NEOs are more easily accessible than the Moon.

text: Until the age of

text: space travel

text: , objects in the asteroid belt were merely pinpricks of light in even the largest telescopes and their shapes and terrain remained a mystery. The best modern ground-based telescopes and the Earth-orbiting

text: Hubble Space Telescope

text: can resolve a small amount of detail on the surfaces of the largest asteroids, but even these mostly remain little more than fuzzy blobs. Limited information about the shapes and compositions of asteroids can be inferred from their

text: light curve

text: s (their variation in brightness as they rotate) and their spectral properties, and asteroid sizes can be estimated by timing the lengths of star occulations (when an asteroid passes directly in front of a star).

text: Radar

text: imaging can yield good information about asteroid shapes and orbital and rotational parameters, especially for near-Earth asteroids. In terms of

text: delta-v

text: and propellant requirements, NEOs are more easily accessible than the Moon.

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answers: NEOs

answers: NDQ_003822

answers: objects in the asteroid belt

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: Until the age of space travel

answers: NDQ_003825

answers: objects in the asteroid belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Radar imaging

answers: NDQ_003828

answers: The best modern ground-based telescopes

answers: NDQ_003829

answers: The best modern ground-based telescopes

answers: NDQ_003830

answers: NEOs are more easily accessible than the Moon

text: 2014 RC is a small Apollo near-Earth asteroid that made a close approach to Earth of  (0.1 lunar distances) around 18:02 UTC on 7 September 2014. It is the fastest rotating asteroid so far discovered. The asteroid briefly brightened to about apparent magnitude 11.5, so it was not visible to the naked eye or common binoculars. At the peak brightness the asteroid had a declination of –47, and was most easily visible over New Zealand. The asteroid is approximately the diameter of the Chelyabinsk meteor, and passed almost as close to Earth as 367943 Duende (2012 DA14) did in 2013. During 2014, asteroids 2014 AA and  have come closer to Earth. 2014 RC was removed from the JPL Sentry Risk Table on 5 September 2014 and there are no known possible impact dates in the next 100 years. On 8 September 2115 the asteroid will pass about  from the moon. On 5 September 1973, the asteroid passed between  and  from Earth.

text: 2014 RC is a small

text: Apollo

text: near-Earth asteroid

text: that made a close approach to Earth of  (0.1 lunar distances) around 18:02 UTC on 7 September 2014. It is the

text: fastest rotating asteroid

text: so far discovered. The asteroid briefly brightened to about

text: apparent magnitude

text: 11.5, so it was not visible to the

text: naked eye

text: or common binoculars. At the peak brightness the asteroid had a

text: declination

text: of –47, and was most easily visible over New Zealand. The asteroid is approximately the diameter of the

text: Chelyabinsk meteor

text: , and passed almost as close to Earth as

text: 367943 Duende

text: (2012 DA14) did in 2013.

entity_name: List of asteroid close approaches to Earth in 2014

text: During 2014

text: , asteroids

text: 2014 AA

text: and  have come closer to Earth. 2014 RC was removed from the JPL

text: Sentry Risk Table

text: on 5 September 2014 and there are no known possible impact dates in the next 100 years. On 8 September 2115 the asteroid will pass about  from the moon. On 5 September 1973, the asteroid passed between  and  from Earth.

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answers: asteroid

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answers: no known possible impact dates in the next 100 years

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answers: no known possible impact dates in the next 100 years

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answers: near-Earth

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answers: come closer to Earth

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answers: On 5 September 1973, the asteroid passed between and from Earth

answers: NDQ_003829

answers: no known possible impact dates in the next 100 years

answers: NDQ_003830

answers: impact dates

text: Asteroids, or "planetoids" as Cole argued they should more properly be called, were a particular focus of his work. In the early 1960s, he surveyed what was then known about what he termed "Cis-Martian" asteroids.(These are now referred to as "near-Earth asteroids," or NEAs," a subclass of near-Earth objects" - NEOs.)

text: Asteroids

text: , or "planetoids" as Cole argued they should more properly be called, were a particular focus of his work. In the early 1960s, he surveyed what was then known about what he termed "Cis-Martian" asteroids.(These are now referred to as "near-Earth asteroids," or NEAs," a subclass of

text: near-Earth objects

text: " - NEOs.)

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text: The only object that has ever been rated at 4 on the Torino Scale (since downgraded), the Aten asteroid (99942) Apophis, has an Earth MOID of 0.0007 AU.  This is not the smallest Earth MOID in the catalogues; many bodies with a small Earth MOID are not classed as PHO's because the objects are less than roughly 140 meters in diameter (or absolute magnitude, H < 22). Earth MOID values are generally more practical for asteroids less than 140 meters in diameter as those asteroids are very dim and often have a short observation arc with a poorly determined orbit. The only objects that have been detected and had their Earth-MOID calculated before Earth impact were the small asteroids  and 2014 AA.  was listed with a MOID of 0.00001 AU in the Minor Planet Center database, and is the smallest MOID calculated for an Apollo asteroid. It is even smaller at the more precise JPL Small Body Database (0.0000078 AU).

text: The only object that has ever been rated at 4 on the

text: Torino Scale

text: (since downgraded), the

text: Aten asteroid

text: (99942) Apophis

text: , has an Earth MOID of 0.0007 AU.  This is not the smallest Earth MOID in the catalogues; many bodies with a small Earth MOID are not classed as PHO's because the objects are less than roughly 140 meters in diameter (or

text: absolute magnitude

text: , H < 22). Earth MOID values are generally more practical for asteroids less than 140 meters in diameter as those asteroids are very dim and often have a short

text: observation arc

text: with a poorly determined orbit. The only objects that have been detected and had their Earth-MOID calculated before Earth impact were the small asteroids  and

text: 2014 AA

text: .  was listed with a MOID of 0.00001 AU in the

text: Minor Planet Center

text: database, and is the smallest MOID calculated for an

text: Apollo asteroid

text: . It is even smaller at the more precise

text: JPL

text: Small Body Database (0.0000078 AU).

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answers: Small Body

answers: NDQ_003822

answers: less than 140 meters in diameter

answers: NDQ_003823

answers: asteroids are too small to have impacts

answers: NDQ_003824

answers: Earth MOID values are generally more practical for asteroids

answers: NDQ_003825

answers: less than 140 meters in diameter

answers: NDQ_003826

answers: Minor Planet Center

answers: NDQ_003827

answers: Earth MOID

answers: NDQ_003828

answers: 2014 AA

answers: NDQ_003829

answers: Earth-MOID

answers: NDQ_003830

answers: minor planets

text: 322 Phaeo is a large Main belt asteroid. It is classified as a M-type asteroid.

text: 322 Phaeo is a large

text: Main belt

text: asteroid

text: . It is classified as a

text: M-type asteroid

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answers: Main belt

answers: NDQ_003827

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answers: classified

answers: NDQ_003822

answers: M-type

answers: NDQ_003823

answers: no

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answers: 322 Phaeo

answers: NDQ_003825

answers: M-type

answers: NDQ_003826

answers: Main belt

answers: NDQ_003827

answers: M-type asteroid

answers: NDQ_003828

answers: 322 Phaeo

answers: NDQ_003829

answers: 322 Phaeo

answers: NDQ_003830

answers: M-type asteroid

text: Didymos is the target of the proposed Asteroid Impact & Deflection Assessment (AIDA) mission, a collaboration between ESA and NASA. This will be the first spacecraft to target an asteroid known to have a moon (243 Ida was visited by the Galileo spacecraft but its moon was a surprise). The mission is intended to test whether a spacecraft could successfully deflect an asteroid on a collision course with Earth; it would study Didymos from orbit, while also crashing a smaller spacecraft into Didymoon, in order to study the effect on its orbit.

text: Didymos is the target of the proposed

text: Asteroid Impact & Deflection Assessment (AIDA) mission

text: , a collaboration between

text: ESA

text: and

text: NASA

text: . This will be the first spacecraft to target an asteroid known to have a moon (

text: 243 Ida

text: was visited by the Galileo spacecraft but its moon was a surprise). The mission is intended to test whether a spacecraft could successfully deflect an asteroid on a collision course with Earth; it would study Didymos from orbit, while also crashing a smaller spacecraft into Didymoon, in order to study the effect on its orbit.

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answers: 4

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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_003821

answers: collision course with Earth

answers: NDQ_003822

answers: Didymos

answers: NDQ_003823

answers: No

answers: NDQ_003824

answers: Galileo spacecraft

answers: NDQ_003825

answers: Didymos

answers: NDQ_003826

answers: Asteroid Belt

answers: NDQ_003827

answers: collision course with Earth

answers: NDQ_003828

answers: Didymos

answers: NDQ_003829

answers: It would study Didymos from orbit

answers: NDQ_003830

answers: collision course with Earth

text: The object of the game is to destroy all the asteroids which have a set speed at which they fly through the Sector. Asteroids come in varying sizes, and when shot, larger asteroids break into multiple smaller ones. Only shooting the smallest ones will actually remove them from the Sector. Asteroids also come in different types. Normal asteroids don't contain anything, but red asteroids can contain power-ups in the form of Power Crystals that are released by completely destroying asteroids. Crystals decay over time. Popcorn Asteroids require several hits, which expands their size, and eventually makes them stop spinning. They can't be destroyed, but stopping them is enough to finish each Sector. Egg asteroids contain leeches which home in on the user's ship and suck out its energy. They can be shot and destroyed. Finally there are Seeker asteroids which home in on the player's ship after being shot.

text: The object of the game is to destroy all the asteroids which have a set speed at which they fly through the Sector. Asteroids come in varying sizes, and when shot, larger asteroids break into multiple smaller ones. Only shooting the smallest ones will actually remove them from the Sector. Asteroids also come in different types. Normal asteroids don't contain anything, but red asteroids can contain

text: power-up

text: s in the form of Power Crystals that are released by completely destroying asteroids. Crystals

text: decay

text: over time.

text: Popcorn

text: Asteroids require several hits, which expands their size, and eventually makes them stop spinning. They can't be destroyed, but stopping them is enough to finish each Sector. Egg asteroids contain

text: leech

text: es which home in on the user's ship and suck out its energy. They can be shot and destroyed. Finally there are Seeker asteroids which home in on the player's ship after being shot.

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answers: NDQ_003821

answers: fly through the Sector

answers: NDQ_003822

answers: come in varying sizes

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: Asteroids

answers: NDQ_003825

answers: come in varying sizes

answers: NDQ_003826

answers: Sector

answers: NDQ_003827

answers: Home in on the user's ship

answers: NDQ_003828

answers: Asteroids

answers: NDQ_003829

answers: It's impossible to say

answers: NDQ_003830

answers: asteroids fly through the Sector

text: The small mass of Mars the low mass asteroid belt may be the result of pebble accretion becoming less efficient as the density of gas in the protoplanetary disk decreases. The protoplanetary disk from which the Solar System formed is believed to have had a surface density that decreased with distance from the Sun and have been flared, with an increasing thickness with distance from the Sun. As a result, the density of the gas and the aerodynamic drag felt by pebbles embedded in the disk would have decreased significantly with distance. If the pebbles were large the efficiency of pebble accretion would decline with distance from the Sun as the aerodynamic drag becomes too weak for the pebbles to be captured during encounters with the largest objects. An object that grows rapidly at Earth's orbital distance would only grow slowly in Mars's orbit and very little in the asteroid belt. The formation of Jupiter's core could also reduce the mass of the asteroid belt by crating a gap in the pebble disk and halting the inward drift of pebbles from beyond the ice line. Objects in the asteroid belt would then be deprived of pebbles early while objects in the terrestrial region continued to accrete pebbles that drifted in from the asteroid region.

text: The small mass of Mars the low mass asteroid belt may be the result of pebble accretion becoming less efficient as the density of gas in the protoplanetary disk decreases. The protoplanetary disk from which the Solar System formed is believed to have had a

text: surface density

text: that decreased with distance from the

text: Sun

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answers: pebbles

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answers: pebbles

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: Objects in the asteroid belt

answers: NDQ_003825

answers: pebbles

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: grow rapidly

answers: NDQ_003828

answers: If the pebbles were large the efficiency of pebble accretion would decline with distance from the Sun

answers: NDQ_003829

answers: An object that grows rapidly at Earth's orbital distance

answers: NDQ_003830

answers: accretion

text: The asteroid 3425 Hurukawa, a main-belt asteroid of the Eos family, was named in his honor. Naming citation was published on 16 December 1986 (M.P.C. 11443).

text: The asteroid

text: 3425 Hurukawa

text: , a main-belt asteroid of the

text: Eos family

text: , was named in his honor. Naming citation was published on 16 December 1986 (

text: M.P.C.

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answers: NDQ_003821

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answers: main-belt

answers: NDQ_003822

answers: 3425 Hurukawa

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: The asteroid 3425 Hurukawa

answers: NDQ_003825

answers: 3425 Hurukawa

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: named in his honor

answers: NDQ_003828

answers: asteroid

answers: NDQ_003829

answers: The asteroid 3425 Hurukawa

answers: NDQ_003830

answers: Eos family

text: |-| 27301 Joeingalls ||  || 27301 Joeingalls Discovered 2000 Jan. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joseph Ingalls mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Saint Margaret's Episcopal School, San Juan Capistrano, California, U.S. |-id=302| 27302 Jeankobis ||  || 27302 Jeankobis Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jean A. Kobis mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Williamsville High School East, East Amherst, New York, U.S. |-id=303| 27303 Leitner ||  || 27303 Leitner Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Roxanne Leitner mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Ursuline Academy Of Dallas, Dallas, Texas, U.S. |-id=309| 27309 Serenamccalla ||  || 27309 Serenamccalla Discovered 2000 Jan. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Serena McCalla mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Jericho Senior High School, Jericho, New York, U.S. |-id=314| 27314 Janemcdonald ||  || 27314 Janemcdonald Discovered 2000 Jan. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jane McDonald mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Rickards High School, Tallahassee, Florida, U.S. |-id=320| 27320 Vellinga ||  || Joseph Vellinga (born 1938), the Flight System Manager for the OSIRIS-REx Asteroid Sample Return Mission. |-id=323| 27323 Julianewman ||  || 27323 Julianewman Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Julia Newman mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Torrey Pines High School, San Diego, California, U.S. |-id=326| 27326 Jimobrien ||  || 27326 Jimobrien Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. James O'Brien mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Venture School, San Ramon, California, U.S. |-id=327| 27327 Lindaplante ||  || 27327 Lindaplante Discovered 2000 Feb. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Linda Plante mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Woodbury High School, Woodbury, Minnesota, U.S. |-id=328| 27328 Pohlonski ||  || 27328 Pohlonski Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Emily Parker Pohlonski mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Novi High School, Novi, Michigan, U.S. |-id=330| 27330 Markporter ||  || 27330 Markporter Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mark Porter mentored a finalist in the 2011 Intel Science Talent Search (STS), a science competition for high-school seniors. He teaches at the Mira Loma High School, Sacramento, California, U.S. |-id=332| 27332 Happritchard ||  || 27332 Happritchard Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Parmely Hap Pritchard mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Oregon Episcopal School, Portland, Oregon, U.S. |-id=336| 27336 Mikequinn ||  || 27336 Mikequinn Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mike Quinn mentored a finalist in the 2011 Intel Science Talent Search (STS), a science competition for high-school seniors. He teaches at the Sunset High School, Portland, Oregon, U.S. |-id=338| 27338 Malaraghavan ||  || 27338 Malaraghavan Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mala Raghavan mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Harker School, San Jose, California, U.S. |-id=341| 27341 Fabiomuzzi ||  || Fabio Muzzi, Italian amateur astronomer |-id=342| 27342 Joescanio ||  || 27342 Joescanio Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joseph M. V. Scanio mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Choate Rosemary Hall, Wallingford, Connecticut, U.S. |-id=343| 27343 Deannashea ||  || 27343 Deannashea Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Deanna Shea mentored a finalist in the 2011 Intel Science Talent Search (STS), a science competition for high-school seniors. She teaches at the Shepton High School, Plano, Texas, U.S. |-id=344| 27344 Vesevlada ||  || Vladimír Veselý, Czech researcher in apiculture †|-id=347| 27347 Dworkin ||  || Jason Dworkin (born 1969), the Project Scientist for the OSIRIS-REx Asteroid Sample Return Mission. |-id=348| 27348 Mink ||  || Ronald Mink (born 1970), the Deputy Project Systems Engineer for the OSIRISREx Asteroid Sample Return Mission. |-id=349| 27349 Enos ||  || Heather Enos (born 1968), the Project Planning and Control Officer for the OSIRIS-REx Asteroid Sample Return mission. |-id=353| 27353 Chrisspenner ||  || Chris Spenner mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Harker School, San Jose, California, U.S. |-id=354| 27354 Stiklaitis ||  || Angela Stiklaitis mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Penn Manor High School, Millersville, Pennsylvania, U.S. |-id=356| 27356 Mattstrom ||  || Matthew Strom mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Basha High School, Chandler, Arizona, U.S. |-id=363| 27363 Alvanclark ||  || Alvan Clark (1804–1887), a noted American astronomer and telescope manufacturer. |-id=365| 27365 Henryfitz ||  || Henry Fitz (1808–1863), an amateur astronomer, early photographer and an optician best known for his high quality telescopes in an era when glass was of inferior quality. |-id=368| 27368 Raytesar ||  || 27368 Raytesar Discovered 2000 Mar. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Raymond Tesar mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Plainview-Old Bethpage John F. Kennedy High School, Plainview, New York, U.S. |-id=372| 27372 Ujifusa ||  || 27372 Ujifusa Discovered 2000 Mar. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Allannah Ujifusa mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Cupertino High School, Cupertino, California, U.S. |-id=373| 27373 Davidvernon ||  || 27373 Davidvernon Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David C. Vernon mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Western Alamance High School, Elon, North Carolina, U.S. |-id=374| 27374 Yim ||  || 27374 Yim Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. P. J. Yim mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Saratoga High School, Saratoga, California, U.S. |-id=375| 27375 Asirvatham ||  || Roshini Shreya Asirvatham (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her behavioral and social sciences project. |-id=381| 27381 Balasingam ||  || Namrata Ramya Balasingam (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her physical sciences project. |-id=382| 27382 Justinbarber ||  || Justin Alexander Barber (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his physical sciences project. |-id=383| 27383 Braebenedict ||  || Braeden Christopher Benedict (born 1996) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his physical sciences project. |-id=384| 27384 Meaganbethel ||  || Meagan Alanna Bethel (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her animal and plant sciences project. |-id=385| 27385 Andblonsky ||  || Andrew C. Blonsky (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his environmental sciences project. |-id=386| 27386 Chadcampbell ||  || Chad Robert Campbell (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his biochemistry, medicine, health science and microbiology project. |-id=387| 27387 Chhabra ||  || Chad Robert Campbell (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his biochemistry, medicine, health science and microbiology project. |-id=390| 27390 Kyledavis ||  || Kyle McKay Davis (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his animal and plant sciences project. |-id=392| 27392 Valerieding ||  || Valerie S. Ding (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her physical sciences project. |-id=396| 27396 Shuji ||  || Shuji Nakamura, Japanese-American electronics engineer, inventor of the blue LED and the violet-blue laser |-id=397| 27397 D'Souza ||  || Alicia Danielle D´Souza (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her environmental sciences project. |}

text: 27301 Joeingalls

text: ||  || 27301 Joeingalls Discovered 2000 Jan. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joseph Ingalls mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Saint Margaret's Episcopal School, San Juan Capistrano, California, U.S. |-id=302|

text: 27302 Jeankobis

text: ||  || 27302 Jeankobis Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jean A. Kobis mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Williamsville High School East, East Amherst, New York, U.S. |-id=303|

text: 27303 Leitner

text: ||  || 27303 Leitner Discovered 2000 Jan. 7 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Roxanne Leitner mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Ursuline Academy Of Dallas, Dallas, Texas, U.S. |-id=309|

text: 27309 Serenamccalla

text: ||  || 27309 Serenamccalla Discovered 2000 Jan. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Serena McCalla mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Jericho Senior High School, Jericho, New York, U.S. |-id=314|

text: 27314 Janemcdonald

text: ||  || 27314 Janemcdonald Discovered 2000 Jan. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Jane McDonald mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Rickards High School, Tallahassee, Florida, U.S. |-id=320|

text: 27320 Vellinga

text: Joseph Vellinga

text: (born 1938), the Flight System Manager for the OSIRIS-REx Asteroid Sample Return Mission. |-id=323|

text: 27323 Julianewman

text: ||  || 27323 Julianewman Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Julia Newman mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Torrey Pines High School, San Diego, California, U.S. |-id=326|

text: 27326 Jimobrien

text: ||  || 27326 Jimobrien Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. James O'Brien mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Venture School, San Ramon, California, U.S. |-id=327|

text: 27327 Lindaplante

text: ||  || 27327 Lindaplante Discovered 2000 Feb. 3 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Linda Plante mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Woodbury High School, Woodbury, Minnesota, U.S. |-id=328|

text: 27328 Pohlonski

text: ||  || 27328 Pohlonski Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Emily Parker Pohlonski mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Novi High School, Novi, Michigan, U.S. |-id=330|

text: 27330 Markporter

text: ||  || 27330 Markporter Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mark Porter mentored a finalist in the 2011 Intel Science Talent Search (STS), a science competition for high-school seniors. He teaches at the Mira Loma High School, Sacramento, California, U.S. |-id=332|

text: 27332 Happritchard

text: ||  || 27332 Happritchard Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Parmely Hap Pritchard mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Oregon Episcopal School, Portland, Oregon, U.S. |-id=336|

text: 27336 Mikequinn

text: ||  || 27336 Mikequinn Discovered 2000 Feb. 4 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mike Quinn mentored a finalist in the 2011 Intel Science Talent Search (STS), a science competition for high-school seniors. He teaches at the Sunset High School, Portland, Oregon, U.S. |-id=338|

text: 27338 Malaraghavan

text: ||  || 27338 Malaraghavan Discovered 2000 Feb. 6 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Mala Raghavan mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Harker School, San Jose, California, U.S. |-id=341|

text: 27341 Fabiomuzzi

text: ||  || Fabio Muzzi, Italian amateur astronomer |-id=342|

text: 27342 Joescanio

text: ||  || 27342 Joescanio Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Joseph M. V. Scanio mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Choate Rosemary Hall, Wallingford, Connecticut, U.S. |-id=343|

text: 27343 Deannashea

text: ||  || 27343 Deannashea Discovered 2000 Feb. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Deanna Shea mentored a finalist in the 2011 Intel Science Talent Search (STS), a science competition for high-school seniors. She teaches at the Shepton High School, Plano, Texas, U.S. |-id=344|

text: 27344 Vesevlada

text: Vladimír Veselý

text: , Czech researcher in apiculture †|-id=347|

text: 27347 Dworkin

text: ||  || Jason Dworkin (born 1969), the Project Scientist for the OSIRIS-REx Asteroid Sample Return Mission. |-id=348|

text: 27348 Mink

text: ||  || Ronald Mink (born 1970), the Deputy Project Systems Engineer for the OSIRISREx Asteroid Sample Return Mission. |-id=349|

text: 27349 Enos

text: ||  || Heather Enos (born 1968), the Project Planning and Control Officer for the OSIRIS-REx Asteroid Sample Return mission. |-id=353|

text: 27353 Chrisspenner

text: ||  || Chris Spenner mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Harker School, San Jose, California, U.S. |-id=354|

text: 27354 Stiklaitis

text: ||  || Angela Stiklaitis mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Penn Manor High School, Millersville, Pennsylvania, U.S. |-id=356|

text: 27356 Mattstrom

text: ||  || Matthew Strom mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Basha High School, Chandler, Arizona, U.S. |-id=363|

text: 27363 Alvanclark

text: ||  || Alvan Clark (1804–1887), a noted American astronomer and telescope manufacturer. |-id=365|

text: 27365 Henryfitz

text: ||  || Henry Fitz (1808–1863), an amateur astronomer, early photographer and an optician best known for his high quality telescopes in an era when glass was of inferior quality. |-id=368|

text: 27368 Raytesar

text: ||  || 27368 Raytesar Discovered 2000 Mar. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Raymond Tesar mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Plainview-Old Bethpage John F. Kennedy High School, Plainview, New York, U.S. |-id=372|

text: 27372 Ujifusa

text: ||  || 27372 Ujifusa Discovered 2000 Mar. 8 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Allannah Ujifusa mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Cupertino High School, Cupertino, California, U.S. |-id=373|

text: 27373 Davidvernon

text: ||  || 27373 Davidvernon Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. David C. Vernon mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Western Alamance High School, Elon, North Carolina, U.S. |-id=374|

text: 27374 Yim

text: ||  || 27374 Yim Discovered 2000 Mar. 9 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. P. J. Yim mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. He teaches at the Saratoga High School, Saratoga, California, U.S. |-id=375|

text: 27375 Asirvatham

text: ||  || Roshini Shreya Asirvatham (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her behavioral and social sciences project. |-id=381|

text: 27381 Balasingam

text: ||  || Namrata Ramya Balasingam (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her physical sciences project. |-id=382|

text: 27382 Justinbarber

text: ||  || Justin Alexander Barber (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his physical sciences project. |-id=383|

text: 27383 Braebenedict

text: ||  || Braeden Christopher Benedict (born 1996) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his physical sciences project. |-id=384|

text: 27384 Meaganbethel

text: ||  || Meagan Alanna Bethel (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her animal and plant sciences project. |-id=385|

text: 27385 Andblonsky

text: ||  || Andrew C. Blonsky (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his environmental sciences project. |-id=386|

text: 27386 Chadcampbell

text: ||  || Chad Robert Campbell (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his biochemistry, medicine, health science and microbiology project. |-id=387|

text: 27387 Chhabra

text: ||  || Chad Robert Campbell (born 1999) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his biochemistry, medicine, health science and microbiology project. |-id=390|

text: 27390 Kyledavis

text: ||  || Kyle McKay Davis (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for his animal and plant sciences project. |-id=392|

text: 27392 Valerieding

text: ||  || Valerie S. Ding (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her physical sciences project. |-id=396|

text: 27396 Shuji

text: ||  || Shuji Nakamura, Japanese-American electronics engineer, inventor of the blue LED and the violet-blue laser |-id=397|

text: 27397 D'Souza

text: ||  || Alicia Danielle D´Souza (born 1997) is a finalist in the 2011 Broadcom MASTERS, a math and science competition for middle-school students, for her environmental sciences project. |}

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

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answers: NDQ_003821

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answers: NDQ_003822

answers: 4

answers: NDQ_003823

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

answers: NDQ_003824

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

answers: NDQ_003825

answers: 4

answers: NDQ_003826

answers: 3

answers: NDQ_003827

answers: 0

answers: NDQ_003828

answers: 0

answers: NDQ_003829

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

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: science competition for high-school seniors

answers: NDQ_003822

answers: science competition for high-school seniors

answers: NDQ_003823

answers: Asteroids are too small to have impacts with other objects, so they don't have craters.

answers: NDQ_003824

answers: Asteroids are too small for NASA missions to visit them.

answers: NDQ_003825

answers: science competition for high-school seniors

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Talent Search

answers: NDQ_003828

answers: |-id=314| 27314 Janemcdonald Discovered 2000 Jan. 2 by the Lincoln Laboratory Near-Earth Asteroid Research Team at Socorro. Janemcdonald mentored a finalist in the 2011 Intel Science Talent Search, a science competition for high-school seniors. She teaches at the Jericho Senior High School, Jericho, New York, U.S.

answers: NDQ_003829

answers: 2011 Intel Science Talent Search, a science competition for high-school seniors.

answers: NDQ_003830

answers: Science Talent Search

text: The Apollo asteroids are a group of near-Earth asteroids named after 1862 Apollo, discovered by German astronomer Karl Reinmuth in the 1930s. They are Earth crossing asteroids that have an orbital semi-major axis greater than that of the Earth (> 1 AU) but perihelion distances less than the Earth's aphelion distance (q < 1.017 AU).

text: The Apollo asteroids are a group of

text: near-Earth asteroid

text: s named after

text: 1862 Apollo

text: , discovered by German astronomer

text: Karl Reinmuth

text: in the 1930s. They are

text: Earth crossing asteroid

text: s that have an orbital

text: semi-major axis

text: greater than that of the Earth (> 1

text: AU

text: ) but

text: perihelion

text: distances less than the Earth's

text: aphelion

text: distance (q < 1.017 AU).

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answers: NDQ_003821

answers: near-Earth

answers: NDQ_003822

answers: near-Earth

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: astronomer Karl Reinmuth

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: perihelion

answers: NDQ_003827

answers: Earth crossing

answers: NDQ_003828

answers: Earth crossing asteroids

answers: NDQ_003829

answers: An asteroid could cause humans to go extinct.

answers: NDQ_003830

answers: asteroids

text: In September 2007, a report published in Nature proposed an origin for the asteroid that created the Chicxulub Crater. The authors, William F. Bottke, David Vokrouhlický, and David Nesvorný, argued that a collision in the asteroid belt 160 million years ago resulted in the Baptistina family of asteroids, the largest surviving member of which is 298 Baptistina. They proposed that the "Chicxulub asteroid" was also a member of this group. The connection between Chicxulub and Baptistina is supported by the large amount of carbonaceous material present in microscopic fragments of the impactor, suggesting the impactor was a member of a rare class of asteroids called carbonaceous chondrites, like Baptistina. According to Bottke, the Chicxulub impactor was a fragment of a much larger parent body about  across, with the other impacting body being around  in diameter. In 2011, new data from the Wide-field Infrared Survey Explorer revised the date of the collision which created the Baptistina family to about 80 million years ago. This makes an asteroid from this family highly improbable to be the asteroid that created the Chicxulub Crater, as typically the process of resonance and collision of an asteroid takes many tens of millions of years. In 2010, another hypothesis was offered which implicated the newly discovered asteroid P/2010 A2, a member of the Flora family of asteroids, as a possible remnant cohort of the K/Pg impactor.

text: In September 2007, a report published in

text: Nature

text: proposed an origin for the asteroid that created the Chicxulub Crater. The authors,

text: William F. Bottke

text: , David Vokrouhlický, and

text: David Nesvorný

text: , argued that a collision in the asteroid belt 160 million years ago resulted in the

text: Baptistina family

text: of asteroids, the largest surviving member of which is

text: 298 Baptistina

text: . They proposed that the "Chicxulub asteroid" was also a member of this group. The connection between Chicxulub and Baptistina is supported by the large amount of carbonaceous material present in microscopic fragments of the impactor, suggesting the impactor was a member of a rare class of asteroids called

text: carbonaceous chondrite

text: s, like Baptistina. According to Bottke, the Chicxulub impactor was a fragment of a much larger parent body about  across, with the other impacting body being around  in diameter. In 2011, new data from the

text: Wide-field Infrared Survey Explorer

text: revised the date of the collision which created the

text: Baptistina family

text: to about 80 million years ago. This makes an asteroid from this family highly improbable to be the asteroid that created the Chicxulub Crater, as typically the process of resonance and collision of an asteroid takes many tens of millions of years. In 2010, another hypothesis was offered which implicated the newly discovered asteroid

text: P/2010 A2

text: , a member of the

text: Flora family

text: of asteroids, as a possible remnant cohort of the K/Pg impactor.

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answers: asteroid belt

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answers: member of the Flora family of asteroids

answers: NDQ_003822

answers: carbonaceous chondrites

answers: NDQ_003823

answers: Chicxulub Crater

answers: NDQ_003824

answers: The Chicxulub Crater

answers: NDQ_003825

answers: carbonaceous chondrites

answers: NDQ_003826

answers: the asteroid belt

answers: NDQ_003827

answers: Chicxulub Crater

answers: NDQ_003828

answers: Chicxulub Crater

answers: NDQ_003829

answers: It is highly improbable

answers: NDQ_003830

answers: asteroids

text: Most belt asteroids imaged to date have come from brief flyby opportunities by probes headed for other targets. Only the Dawn, NEAR and Hayabusa missions have studied asteroids for a protracted period in orbit and at the surface. Dawn explored Vesta from July 2011 to September 2012, and has been orbiting Ceres since March 2015.

text: Most belt asteroids imaged to date have come from brief

text: flyby

text: opportunities by probes headed for other targets. Only the Dawn, NEAR and

text: Hayabusa

text: missions have studied asteroids for a protracted period in orbit and at the surface. Dawn explored Vesta from July 2011 to September 2012, and has been orbiting

text: Ceres

text: since March 2015.

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answers: NDQ_003821

answers: orbiting

answers: NDQ_003822

answers: Belt asteroids

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: Most belt asteroids imaged to date have come from brief flyby opportunities

answers: NDQ_003825

answers: Belt asteroids

answers: NDQ_003826

answers: belt

answers: NDQ_003827

answers: flyby

answers: NDQ_003828

answers: Ceres

answers: NDQ_003829

answers: It could cause humans to go extinct.

answers: NDQ_003830

answers: orbit and at the surface

text: The upper limit is also vague. Two orbiting bodies are sometimes described as a double body rather than primary and satellite. Asteroids such as 90 Antiope are considered double asteroids, but they have not forced a clear definition of what constitutes a moon. Some authors consider the Pluto–Charon system to be a double (dwarf) planet. The most common dividing line on what is considered a moon rests upon whether the barycentre is below the surface of the larger body, though this is somewhat arbitrary, because it depends on distance as well as relative mass.

text: The upper limit is also vague. Two orbiting bodies are sometimes described as a

text: double body

text: rather than primary and satellite.

text: Asteroid

text: s such as

text: 90 Antiope

text: are considered double asteroids, but they have not forced a clear definition of what constitutes a moon. Some authors consider the Pluto–Charon system to be a double (dwarf) planet. The most common dividing line on what is considered a moon rests upon whether the

text: barycentre

text: is below the surface of the larger body, though this is somewhat arbitrary, because it depends on distance as well as relative mass.

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answers: NDQ_003821

answers: orbiting bodies

answers: NDQ_003822

answers: 90 Antiope

answers: NDQ_003823

answers: It depends on distance as well as relative mass

answers: NDQ_003824

answers: The upper limit is also vague

answers: NDQ_003825

answers: 90 Antiope

answers: NDQ_003826

answers: upper limit

answers: NDQ_003827

answers: orbiting bodies

answers: NDQ_003828

answers: 90 Antiope are considered double asteroids

answers: NDQ_003829

answers: The upper limit is also vague

answers: NDQ_003830

answers: Pluto–Charon system

text: This mission would place an asteroid in lunar orbit, rather than sending astronauts to an asteroid in deep space.The Keck Institute for Space Studies at the California Institute of Technology, in partnership with the Jet Propulsion Laboratory, estimates a mission cost of approximately $2.6 billion.  By contrast, original estimates for colonization of the Moon, as a part of the Constellation Program, reached a total cost of $150 billion.  However, the $2.6 billion estimate is solely the cost of asteroid capture.  It does not include any developmental costs, nor does it cover the costs of Orion flights to a 4 m asteroid once it is captured, so this comparison does not include the full costs of this enterprise.The Obama Administration estimates that this mission would actually cost even less than the estimated $2.6 billion and was a part of the FY2014 budget request.Steps toward accomplishing this mission would simultaneously develop advanced solar electric propulsion technology.

text: This mission would place an asteroid in

text: lunar orbit

text: , rather than sending astronauts to an asteroid in

text: deep space

text: .The

text: Keck Institute for Space Studies

text: at the

text: California Institute of Technology

text: , in partnership with the

text: Jet Propulsion Laboratory

text: , estimates a mission cost of approximately $2.6 billion.  By contrast, original estimates for

text: colonization of the Moon

text: , as a part of the

text: Constellation Program

text: , reached a total cost of $150 billion.  However, the $2.6 billion estimate is solely the cost of

text: asteroid capture

text: .  It does not include any developmental costs, nor does it cover the costs of Orion flights to a 4 m asteroid once it is captured, so this comparison does not include the full costs of this enterprise.The

text: Obama Administration

text: estimates that this mission would actually cost even less than the estimated $2.6 billion and was a part of the

text: FY2014 budget request

text: .Steps toward accomplishing this mission would simultaneously develop advanced

text: solar electric propulsion

text: technology.

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answers: deep space

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answers: 4 m

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answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: It does not include any developmental costs

answers: NDQ_003825

answers: 4 m

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answers: orbit

answers: NDQ_003827

answers: colonize the Moon

answers: NDQ_003828

answers: The Obama Administration estimates that this mission would actually cost even less than the estimated $2.6 billion

answers: NDQ_003829

answers: The Obama Administration estimates that this mission would actually cost even less than the estimated $2.6 billion

answers: NDQ_003830

answers: colonization

text: A-type asteroids are relatively uncommon inner-belt asteroids that have a strong, broad 1 µm olivine feature and a very reddish spectrum shortwards of 0.7 µm. They are thought to come from the completely differentiated mantle of an asteroid.

text: A-type asteroids are relatively uncommon inner-belt

text: asteroid

text: s that have a strong, broad 1

text: µm

text: olivine

text: feature and a very reddish spectrum shortwards of 0.7 µm. They are thought to come from the completely differentiated

text: mantle

text: of an asteroid.

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text: is a rare-type carbonaceous binary asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 1.7 kilometers in diameter. It was discovered on 24 March 1996, by Australian astronomer Robert McNaught at Siding Spring Observatory in New South Wales, Australia. The asteroid was also a target of a rejected mission-proposal for the Marco Polo spacecraft.

text: is a rare-type carbonaceous

text: binary

text: asteroid

text: , classified as

text: near-Earth object

text: and

text: potentially hazardous asteroid

text: of the

text: Apollo

text: group, approximately 1.7 kilometers in diameter. It was discovered on 24 March 1996, by Australian astronomer

text: Robert McNaught

text: at

text: Siding Spring Observatory

text: in New South Wales, Australia. The asteroid was also a target of a rejected mission-proposal for the

text: Marco Polo

text: spacecraft.

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answers: near-Earth object

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answers: carbonaceous binary

answers: NDQ_003823

answers: It was discovered on 24 March 1996

answers: NDQ_003824

answers: The asteroid was also a target of a rejected mission

answers: NDQ_003825

answers: carbonaceous binary

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answers: Apollo group

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answers: Hazardous

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answers: 1.7 kilometers

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answers: Classified as near-Earth object

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answers: spacecraft

text: Under the Morocco Oukaimeden Sky Survey (MOSS) Project, the University of Marrakesh discovered two major comets and one NEO, which resulted in the university gaining prestige by naming the asteroid 2007 NQ3 as Cadi Ayyad. The first discovery was comet P/2011 W2 (Rinner) on 25 November 2011 using a 500 mm telescope at the Oukaimeden Observatory. The second comet with the name  (MOSS) was discovered on 13 February 2011. A near-Earth asteroid was discovered on the night of 15 to 16 November 2011 using a MOSS telescope. A third comet was officially discovered in January 2013 was designated .

text: Under the Morocco Oukaimeden Sky Survey (MOSS) Project, the University of Marrakesh discovered two major

text: comets

text: and one

text: NEO

text: , which resulted in the university gaining prestige by naming the asteroid 2007 NQ3 as

text: Cadi Ayyad

text: . The first discovery was comet P/2011 W2 (Rinner) on 25 November 2011 using a 500 mm

text: telescope

text: at the Oukaimeden Observatory. The second comet with the name  (MOSS) was discovered on 13 February 2011. A

text: near-Earth

text: asteroid

text: was discovered on the night of 15 to 16 November 2011 using a MOSS telescope. A third comet was officially discovered in January 2013 was designated .

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answers: NEO

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answers: asteroids

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answers: Mars Oukaimeden Sky Survey (MOSS) Project

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answers: 2007 NQ3

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answers: near-Earth

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answers: discovered

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answers: An asteroid could cause humans to go extinct

answers: NDQ_003830

answers: comets

text: B-type asteroids are a relatively uncommon type of carbonaceous asteroid, falling into the wider C-group. In the asteroid population, B-class objects can be found in the outer asteroid belt, and also dominate the high-inclination Pallas family which includes the second-largest asteroid 2 Pallas. They are thought to be primitive,  volatile-rich remnants from the early Solar System. There are 65 known B-type asteroids in the SMASS classification, and 9 in the Tholen classification as of March 2015.

text: B-type asteroids are a relatively uncommon type of

text: carbon

text: aceous

text: asteroid

text: , falling into the wider

text: C-group

text: . In the asteroid population, B-class objects can be found in the outer

text: asteroid belt

text: , and also dominate the high-

text: inclination

text: Pallas family

text: which includes the second-largest asteroid

text: 2 Pallas

text: . They are thought to be

text: primitive

text: volatile

text: -rich remnants from the early

text: Solar System

text: . There are 65 known B-type asteroids in the SMASS classification, and 9 in the Tholen classification as of March 2015.

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answers: 4

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: 0

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answers: carbonaceous

answers: NDQ_003822

answers: carbonaceous

answers: NDQ_003823

answers: B-type asteroids

answers: NDQ_003824

answers: They are thought to be primitive, volatile-rich remnants from the early Solar System

answers: NDQ_003825

answers: carbonaceous

answers: NDQ_003826

answers: the outer asteroid belt

answers: NDQ_003827

answers: be found in the outer asteroid belt

answers: NDQ_003828

answers: B-type asteroids

answers: NDQ_003829

answers: B-class objects can be found in the outer asteroid belt

answers: NDQ_003830

answers: ancient remnants from the early Solar System

text: According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 7.4 kilometers in diameter and its surface has an albedo of 0.17, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 12.2 kilometers, as the lower the body's albedo (reflectivity), the larger its diameter, at a constant absolute magnitude (brightness).

text: According to the survey carried out by the

text: NEOWISE

text: mission of NASA's

text: Wide-field Infrared Survey Explorer

text: , the asteroid measures 7.4 kilometers in diameter and its surface has an

text: albedo

text: of 0.17, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 12.2 kilometers, as the lower the body's albedo (reflectivity), the larger its diameter, at a constant absolute magnitude (brightness).

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answers: carbonaceous

answers: NDQ_003822

answers: carbonaceous

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: The survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer

answers: NDQ_003825

answers: carbonaceous

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: carbonaceous

answers: NDQ_003828

answers: The asteroid measures 7.4 kilometers in diameter

answers: NDQ_003829

answers: The asteroid measures 7.4 kilometers in diameter

answers: NDQ_003830

answers: asteroids

text: is a small asteroid that is a near-Earth object, an Earth coorbital, and an Apollo asteroid.

text: is a small

text: asteroid

text: that is a

text: near-Earth object

text: , an

text: Earth coorbital

text: , and an

text: Apollo asteroid

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answers: NDQ_003822

answers: asteroid

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

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answers: NDQ_003829

answers: An asteroid could cause humans to go extinct

answers: NDQ_003830

answers: Earth coorbital

text: Near Earth Space Surveillance (NESS), led by Principal Investigator Alan Hildebrand of the University of Calgary, will use NEOSSat to search for and track near-Earth asteroids inside Earth's orbit around the Sun, including asteroids in the Aten and Atira classes. These asteroids are particularly difficult to detect from the surface of the Earth, as they are usually positioned in the daylit or twilit sky, when background light from the Sun makes such faint objects invisible. This form of stray light is not an issue for a telescope in orbit, making even a small-aperture telescope such as that on NEOSSat capable of detecting faint asteroids. The NESS science team expects to be able to detect many such asteroids as faint as visual magnitude 19. The NESS mission is funded by the CSA.

text: Near Earth Space Surveillance (NESS), led by Principal Investigator Alan Hildebrand of the University of Calgary, will use NEOSSat to search for and track near-Earth asteroids inside Earth's orbit around the Sun, including asteroids in the

text: Aten

text: and

text: Atira

text: classes. These asteroids are particularly difficult to detect from the surface of the Earth, as they are usually positioned in the daylit or twilit sky, when background light from the Sun makes such faint objects invisible. This form of stray light is not an issue for a telescope in orbit, making even a small-aperture telescope such as that on NEOSSat capable of detecting faint asteroids. The NESS science team expects to be able to detect many such asteroids as faint as visual magnitude 19. The NESS mission is funded by the CSA.

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answers: faint objects

answers: NDQ_003822

answers: Aten and Atira classes

answers: NDQ_003823

answers: asteroids inside Earth's orbit around the Sun

answers: NDQ_003824

answers: These asteroids are particularly difficult to detect from the surface of the Earth

answers: NDQ_003825

answers: Aten and Atira classes

answers: NDQ_003826

answers: Earth's orbit

answers: NDQ_003827

answers: twilit sky

answers: NDQ_003828

answers: The NESS mission is funded by the CSA

answers: NDQ_003829

answers: It's impossible to say

answers: NDQ_003830

answers: are particularly difficult to detect from the surface of the Earth

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2009.

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2009.

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answers: near-Earth

answers: NDQ_003822

answers: near-Earth

answers: NDQ_003823

answers: asteroids do not have craters

answers: NDQ_003824

answers: 0.00256 AU

answers: NDQ_003825

answers: near-Earth

answers: NDQ_003826

answers: AU

answers: NDQ_003827

answers: passed more than 1 lunar distance

answers: NDQ_003828

answers: 1 lunar distance

answers: NDQ_003829

answers: 0.00256 AU

answers: NDQ_003830

answers: near-Earth asteroids

text: Other situations, however, may have more direct financial application, such as an asteroid defense mechanism.  There is a minute probability of an asteroid strike large enough to destroy the planet - what should we do about this?  Clearly if we poured the entire GDP of the planet into protecting against this, we could minimize the risk, but might there be better things to spend it on?  Instead, armed with a value for the planet, we can put in place systems that provide early warning and a good measure of the probability of asteroid impact.  This knowledge itself reduces the average cost of a meteor impact to an "acceptable" level.

text: Other situations, however, may have more direct financial application, such as an

text: asteroid

text: defense mechanism.  There is a minute probability of an asteroid strike large enough to destroy the planet - what should we do about this?  Clearly if we poured the entire GDP of the planet into protecting against this, we could minimize the risk, but might there be better things to spend it on?  Instead, armed with a value for the planet, we can put in place systems that provide early warning and a good measure of the probability of asteroid impact.  This knowledge itself reduces the average cost of a meteor impact to an "acceptable" level.

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answers: NDQ_003821

answers: a meteor

answers: NDQ_003822

answers: The average cost of a meteor impact to an "acceptable" level

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects

answers: NDQ_003824

answers: The average cost of a meteor impact

answers: NDQ_003825

answers: The average cost of a meteor impact to an "acceptable" level

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: destroy the planet

answers: NDQ_003828

answers: An asteroid strike large enough to destroy the planet

answers: NDQ_003829

answers: The average cost of a meteor impact to an "acceptable" level

answers: NDQ_003830

answers: direct financial application

text: S-type asteroids, or silicaceous asteroids, are of a stony composition, hence the name. Approximately 17% of asteroids are of this type, making it the second most common after the C-type.

text: S-type asteroids, or silicaceous asteroids, are of a stony composition, hence the name. Approximately 17% of

text: asteroid

text: s are of this type, making it the second most common after the

text: C-type

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answers: stony composition

answers: NDQ_003822

answers: S-type asteroids

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: Approximately 17% of asteroids are of this type

answers: NDQ_003825

answers: S-type asteroids

answers: NDQ_003826

answers: C-type

answers: NDQ_003827

answers: silicaceous

answers: NDQ_003828

answers: C-type

answers: NDQ_003829

answers: S-type asteroids

answers: NDQ_003830

answers: are of a stony composition

text: |-id=003| 134003 Ingridgalinsky ||  || Ingrid Galinsky (b. 1962) worked on the OSIRIS-REx mission as the Science Processing and Operation Center Test Lead. |-id=008| 134008 Davidhammond ||  || Dave Hammond (b. 1983) worked on the OSIRIS-REx mission as the Science Processing Lead at the Science Processing and Operations Center. |-id=019| 134019 Nathanmogk ||  || Nathan Mogk (b. 1989) worked on the OSIRIS-REx mission as a systems engineer for the Science Processing and Operations Center. His previous planetary science work included making DTMs of Mars from HiRISE data and research on three-body-problem dynamics. |-id=027| 134027 Deanbooher ||  || Daniel "Dean" Booher (b. 1971) was the Quality Assurance Manager for the OCAMS Instrument Suite on the OSIRIS-REx Asteroid Sample Return Mission.|-id=028| 134028 Mikefitzgibbon ||  || Mike Fitzgibbon (b. 1962) worked on the OSIRIS-REx mission as an OCAMS Software Engineer and on Space Shuttle missions with the AIS, GLO and UVSTAR instruments, and a number of planetary missions including Mars Polar Lander, Mars Odyssey, Phoenix, Lunar Reconnaissance Orbiter, MESSENGER and MSL. |-id=034| 134034 Bloomenthal ||  || H. Philip Bloomenthal (b. 1981) worked as a Systems Administrator at the University of Arizona Science Processing and Operations Center for the OSIRIS-REx mission. He helped keep the little green lights blinking. |-id=036| 134036 Austincummings ||  || Austin Cummings (b. 1995) worked on the NASA's OSIRIS-REx mission as a software developer at the Science Processing and Operations Center.|-id=039| 134039 Stephaniebarnes ||  || Stephanie Barnes (b. 1984) was the SPOC Science Operations Engineer for the OSIRIS-REx mission. |-id=040| 134040 Beaubierhaus ||  || Beau Bierhaus (b. 1972) was the science team interface to the spacecraft design and development activities for the OSIRIS-REx mission. |-id=044| 134044 Chrisshinohara ||  || Chris Shinohara (b. 1965) was the Science Processing and Operations Center Manager for the OSIRIS-REx Asteroid Sample Return mission at the University of Arizona. He also worked on the Phoenix and Mars Reconnaissance Orbiter missions. |-id=050| 134050 Rebeccaghent ||  || Rebecca Ghent (b. 1971) is a Co-I on the OSIRIS-REx Asteroid Sample Return Mission. She is also a Co-I for the Diviner thermal radiometer on the Lunar Reconnaissance Orbiter mission, and has contributed to the body of knowledge of planetary impacts, regolith development and tectonics. |-id=063| 134063 Damianhammond ||  || Damian Hammond (b. 1972) was the Software Engineering Lead for OSIRIS-REx Telemetry Processing at the Science Processing and Operations Center, for the OSIRIS-REx mission. |-id=069| 134069 Miyo ||  || Miyo Itagaki, the discoverer's mother |-id=072| 134072 Sharonhooven ||  || Sharon Hooven (b. 1958) was the Senior Business Manager for the OSIRIS-REx mission at the University of Arizona. |-id=081| 134081 Johnmarshall ||  || John Marshall (b. 1948) was the Asteroid Scientist - Regolith for the OSIRIS-REx mission. |-id=087| 134087 Symeonplatts ||  || Symeon Platts (b. 1991) was the Senior Videographer for the OSIRIS-REx Mission at the University of Arizona. |-id=088| 134088 Brettperkins ||  || Brett Perkins (b. 1967) is the Launch Site Integration Manager for the OSIRIS-REx Mission. He served in a similar capacity for the JUNO Jupiter mission and multiple TDRSS missions. During the Space Shuttle Program he served as a test engineer and a NASA Test Director for missions from 1990 through 2011. |-id=091| 134091 Jaysoncowley ||  || Jayson Cowley (b. 1959) is the United Launch Alliance Mission Manager for the OSIRIS-REx Asteroid Sample Return Mission. He has supported NASA with Titan- IV, Delta-II and Atlas-V launch services for the MAVEN, LDCM, WISE, STSS-D and Cassini missions. |-id=092| 134092 Lindaleematthias ||  || Linda Lee Matthias (b. 1968) is the KSC/LSP Contamination Control Engineer for the OSIRIS-REx Asteroid Sample Return Mission. Since 1988 she has supported over 70 successful Titan IV and NASA Launch Services Program Missions as the Planetary Protection and Contamination Control Engineer. |-id=099| 134099 Rexengelhardt ||  || Rex Engelhardt (b. 1959) is the KSC Launch Services Program Mission Manager for the OSIRIS-REx Asteroid Sample Return Mission. As a Mission Manager, he has led more than 10 missions since LSP was established in 1998. He supported many payload support jobs for NASA Kennedy Space Center and the Air Force. |}

text: 134003 Ingridgalinsky

text: ||  || Ingrid Galinsky (b. 1962) worked on the OSIRIS-REx mission as the Science Processing and Operation Center Test Lead. |-id=008|

text: 134008 Davidhammond

text: ||  || Dave Hammond (b. 1983) worked on the OSIRIS-REx mission as the Science Processing Lead at the Science Processing and Operations Center. |-id=019|

text: 134019 Nathanmogk

text: ||  || Nathan Mogk (b. 1989) worked on the OSIRIS-REx mission as a systems engineer for the Science Processing and Operations Center. His previous planetary science work included making DTMs of Mars from HiRISE data and research on three-body-problem dynamics. |-id=027|

text: 134027 Deanbooher

text: ||  || Daniel "Dean" Booher (b. 1971) was the Quality Assurance Manager for the OCAMS Instrument Suite on the OSIRIS-REx Asteroid Sample Return Mission.|-id=028|

text: 134028 Mikefitzgibbon

text: ||  || Mike Fitzgibbon (b. 1962) worked on the OSIRIS-REx mission as an OCAMS Software Engineer and on Space Shuttle missions with the AIS, GLO and UVSTAR instruments, and a number of planetary missions including Mars Polar Lander, Mars Odyssey, Phoenix, Lunar Reconnaissance Orbiter, MESSENGER and MSL. |-id=034|

text: 134034 Bloomenthal

text: ||  || H. Philip Bloomenthal (b. 1981) worked as a Systems Administrator at the University of Arizona Science Processing and Operations Center for the OSIRIS-REx mission. He helped keep the little green lights blinking. |-id=036|

text: 134036 Austincummings

text: ||  || Austin Cummings (b. 1995) worked on the NASA's OSIRIS-REx mission as a software developer at the Science Processing and Operations Center.|-id=039|

text: 134039 Stephaniebarnes

text: ||  || Stephanie Barnes (b. 1984) was the SPOC Science Operations Engineer for the OSIRIS-REx mission. |-id=040|

text: 134040 Beaubierhaus

text: ||  || Beau Bierhaus (b. 1972) was the science team interface to the spacecraft design and development activities for the OSIRIS-REx mission. |-id=044|

text: 134044 Chrisshinohara

text: ||  || Chris Shinohara (b. 1965) was the Science Processing and Operations Center Manager for the OSIRIS-REx Asteroid Sample Return mission at the University of Arizona. He also worked on the Phoenix and Mars Reconnaissance Orbiter missions. |-id=050|

text: 134050 Rebeccaghent

text: ||  || Rebecca Ghent (b. 1971) is a Co-I on the OSIRIS-REx Asteroid Sample Return Mission. She is also a Co-I for the Diviner thermal radiometer on the Lunar Reconnaissance Orbiter mission, and has contributed to the body of knowledge of planetary impacts, regolith development and tectonics. |-id=063|

text: 134063 Damianhammond

text: ||  || Damian Hammond (b. 1972) was the Software Engineering Lead for OSIRIS-REx Telemetry Processing at the Science Processing and Operations Center, for the OSIRIS-REx mission. |-id=069|

text: 134069 Miyo

text: ||  || Miyo Itagaki, the discoverer's mother |-id=072|

text: 134072 Sharonhooven

text: ||  || Sharon Hooven (b. 1958) was the Senior Business Manager for the OSIRIS-REx mission at the University of Arizona. |-id=081|

text: 134081 Johnmarshall

text: ||  || John Marshall (b. 1948) was the Asteroid Scientist - Regolith for the OSIRIS-REx mission. |-id=087|

text: 134087 Symeonplatts

text: ||  || Symeon Platts (b. 1991) was the Senior Videographer for the OSIRIS-REx Mission at the University of Arizona. |-id=088|

text: 134088 Brettperkins

text: ||  || Brett Perkins (b. 1967) is the Launch Site Integration Manager for the OSIRIS-REx Mission. He served in a similar capacity for the JUNO Jupiter mission and multiple TDRSS missions. During the Space Shuttle Program he served as a test engineer and a NASA Test Director for missions from 1990 through 2011. |-id=091|

text: 134091 Jaysoncowley

text: ||  || Jayson Cowley (b. 1959) is the United Launch Alliance Mission Manager for the OSIRIS-REx Asteroid Sample Return Mission. He has supported NASA with Titan- IV, Delta-II and Atlas-V launch services for the MAVEN, LDCM, WISE, STSS-D and Cassini missions. |-id=092|

text: 134092 Lindaleematthias

text: ||  || Linda Lee Matthias (b. 1968) is the KSC/LSP Contamination Control Engineer for the OSIRIS-REx Asteroid Sample Return Mission. Since 1988 she has supported over 70 successful Titan IV and NASA Launch Services Program Missions as the Planetary Protection and Contamination Control Engineer. |-id=099|

text: 134099 Rexengelhardt

text: ||  || Rex Engelhardt (b. 1959) is the KSC Launch Services Program Mission Manager for the OSIRIS-REx Asteroid Sample Return Mission. As a Mission Manager, he has led more than 10 missions since LSP was established in 1998. He supported many payload support jobs for NASA Kennedy Space Center and the Air Force. |}

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answers: NDQ_003821

answers: || Ingrid Galinsky (b. 1962) worked on the OSIRIS-REx mission as a systems engineer for the Science Processing and Operations Center. Her previous planetary science work included making DTMs of Mars from HiRISE data and research on three-body-problem dynamics. |-id=027| 134027 Deanbooher (b. 1971) was the Quality Assurance Manager for the OCAMS Instrument Suite on the OSIRIS-REx Asteroid Sample Return Mission. |-id=028| 134028 Mikefitzgibbon (b. 1962) worked on the OSIRIS-REx mission as an OCAMS Software Engineer and on Space Shuttle missions with the AIS, GLO and UVSTAR instruments, and a number of planetary missions including Mars Polar Lander, Mars Odyssey, Phoenix, Lunar Reconnaissance Orbiter, MESSENGER, and MSL. |-id=036| 134036 Austincummings (b. 1995) worked on the OSIRIS-REx mission as a software developer at the Science Processing and Operations Center.

answers: NDQ_003822

answers: || Ingrid Galinsky (b. 1962) worked on the OSIRIS-REx mission as the Science Processing and Operation Center Test Lead. |-id=003| 134003 Davidhammond (b. 1983) worked on the OSIRIS-REx mission as the Science Processing Lead at the Science Processing and Operations Center. |-id=028| 134028 Nathanmogk (b. 1989) worked on the OSIRIS-REx mission as a systems engineer for the Science Processing and Operations Center. His previous planetary science work included making DTMs of Mars from HiRISE data and research on three-body-problem dynamics. |-id=027| 134027 Deanbooher (b. 1971) was the Quality Assurance Manager for the OCAMS Instrument Suite on the OSIRIS-REx Asteroid Sample Return Mission. |-id=028| 134028 Mikefitzgibbon (b. 1962) worked on the OSIRIS-REx mission as an OCAMS Software Engineer and on Space Shuttle missions with the AIS, GLO and UVSTAR instruments, and a number of planetary missions including Mars Polar Lander, Mars Odyssey, Phoenix, Lunar Reconnaissance Orbiter, MESSENGER, and MSL. |-id=036| 134036 Austincummings (b. 1995) worked on the OSIRIS-REx mission as a software developer at the Science Processing and Operations Center. |-id=039| 134039 Stephanie Barnes (b. 1995) worked on the OSIRIS-REx mission as a software developer at the Science Processing and Operations Center. |-id=039| 134039

answers: NDQ_003823

answers: || Ingrid Galinsky (b. 1962) worked on the NASA's OSIRIS-REx mission as the Science Processing and Operation Center Test Lead. |-id=003| 134003 Davidhammond (b. 1983) worked on the OSIRIS-REx mission as the Science Processing Lead at the Science Processing and Operations Center.

answers: NDQ_003824

answers: Operations Center.

answers: NDQ_003825

answers: || Ingrid Galinsky (b. 1962) worked on the OSIRIS-REx mission as the Science Processing and Operation Center Test Lead. |-id=003| 134003 Davidhammond (b. 1983) worked on the OSIRIS-REx mission as the Science Processing Lead at the Science Processing and Operations Center. |-id=028| 134028 Nathanmogk (b. 1989) worked on the OSIRIS-REx mission as a systems engineer for the Science Processing and Operations Center. His previous planetary science work included making DTMs of Mars from HiRISE data and research on three-body-problem dynamics. |-id=027| 134027 Deanbooher (b. 1971) was the Quality Assurance Manager for the OCAMS Instrument Suite on the OSIRIS-REx Asteroid Sample Return Mission. |-id=028| 134028 Mikefitzgibbon (b. 1962) worked on the OSIRIS-REx mission as an OCAMS Software Engineer and on Space Shuttle missions with the AIS, GLO and UVSTAR instruments, and a number of planetary missions including Mars Polar Lander, Mars Odyssey, Phoenix, Lunar Reconnaissance Orbiter, MESSENGER, and MSL. |-id=036| 134036 Austincummings (b. 1995) worked on the OSIRIS-REx mission as a software developer at the Science Processing and Operations Center. |-id=039| 134039 Stephanie Barnes (b. 1995) worked on the OSIRIS-REx mission as a software developer at the Science Processing and Operations Center. |-id=039| 134039

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: Asteroid Sample Return Mission

answers: NDQ_003828

answers: || || Ingrid Galinsky (b. 1962) worked on the OSIRIS-REx mission as the Science Processing and Operation Center Test Lead. || ||

answers: NDQ_003829

answers: 4036

answers: NDQ_003830

answers: NASA's OSIRIS-REx Asteroid Sample Return Mission

text: When they discuss children, Cole says he does not want any, and Maya reveals she is incapable.  As the asteroid grows closer, Cole asks Maya to marry him.  Maya jokingly accepts, and Cole insists that he is serious; now serious, Maya again agrees.  Although initially dismissive of the danger, scientists become increasingly worried about a collision.  Various missions to divert the asteroid end in failure, putting the world on edge.  In the flashforwards, Cole and Maya's relationship deteriorates in the face of their hardship in finding food and shelter.

text: When they discuss children, Cole says he does not want any, and Maya reveals she is incapable.  As the asteroid grows closer, Cole asks Maya to marry him.  Maya jokingly accepts, and Cole insists that he is serious; now serious, Maya again agrees.  Although initially dismissive of the danger, scientists become increasingly worried about a collision.  Various missions to divert the asteroid end in failure, putting the world on edge.  In the flashforwards, Cole and Maya's relationship deteriorates in the face of their hardship in finding food and shelter.

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answers: closer

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answers: Collision

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answers: Various missions to divert the asteroid

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answers: asteroid belt

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answers: collision

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answers: collide

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answers: putting the world on edge

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answers: collision

text: Originally, the ESA identified two near-Earth asteroids as possible targets:  and (10302) 1989 ML. Neither asteroid represents a threat to Earth. In a subsequent study, two different possibilities were selected: the Amor asteroid 2003 SM84 and 99942 Apophis; the latter is of particular significance to Earth as it will make a close approach in 2029 and 2036.

text: Originally, the ESA identified two

text: near-Earth asteroid

text: s as possible targets:  and

text: (10302) 1989 ML

text: . Neither asteroid represents a threat to Earth. In a subsequent study, two different possibilities were selected: the

text: Amor asteroid

text: 2003 SM84

text: and

text: 99942 Apophis

text: ; the latter is of particular significance to Earth as it will make a close approach in 2029 and 2036.

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answers: a threat

answers: NDQ_003822

answers: 10302) 1989 ML

answers: NDQ_003823

answers: 10302) 1989 ML

answers: NDQ_003824

answers: Neither asteroid represents a threat to Earth

answers: NDQ_003825

answers: 10302) 1989 ML

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: make a close approach

answers: NDQ_003828

answers: 10302) 1989 ML

answers: NDQ_003829

answers: 10302) 1989 ML

answers: NDQ_003830

answers: Earth

text: However, Karl Ludwig Hencke persisted, and began searching for more asteroids in 1830. Fifteen years later, he found 5 Astraea, the first new asteroid in 38 years. He also found 6 Hebe less than two years later. After this, other astronomers joined in the search and at least one new asteroid was discovered every year after that (except the wartime year 1945). Notable asteroid hunters of this early era were J. R. Hind, Annibale de Gasparis, Robert Luther, H. M. S. Goldschmidt, Jean Chacornac, James Ferguson, Norman Robert Pogson, E. W. Tempel, J. C. Watson, C. H. F. Peters, A. Borrelly, J. Palisa, the Henry brothers and Auguste Charlois.

text: However,

text: Karl Ludwig Hencke

text: persisted, and began searching for more asteroids in 1830. Fifteen years later, he found

text: 5 Astraea

text: , the first new asteroid in 38 years. He also found

text: 6 Hebe

text: less than two years later. After this, other astronomers joined in the search and at least one new asteroid was discovered every year after that (except the wartime year 1945). Notable asteroid hunters of this early era were

text: J. R. Hind

text: Annibale de Gasparis

text: Robert Luther

text: H. M. S. Goldschmidt

text: Jean Chacornac

text: James Ferguson

text: Norman Robert Pogson

text: E. W. Tempel

text: J. C. Watson

text: C. H. F. Peters

text: A. Borrelly

text: J. Palisa

text: , the

text: Henry brothers

text: and

text: Auguste Charlois

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answers: asteroids

answers: NDQ_003822

answers: At least one new asteroid was discovered every year after that

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: At least one new asteroid was discovered every year after that

answers: NDQ_003825

answers: At least one new asteroid was discovered every year after that

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: wartime

answers: NDQ_003828

answers: 1945

answers: NDQ_003829

answers: It was not found

answers: NDQ_003830

answers: new asteroid was discovered every year

text: , provisionally known as 2002 CU11, is a near-Earth asteroid and potentially hazardous object. It was discovered on 7 February 2002 by Lincoln Near-Earth Asteroid Research (LINEAR) at an apparent magnitude of 19 using a  reflecting telescope. It has an estimated diameter of . The asteroid was listed on Sentry Risk Table with a Torino Scale rating of 1 on 20 March 2002.

text: provisionally known

text: as 2002 CU11, is a

text: near-Earth asteroid

text: and

text: potentially hazardous object

text: . It was discovered on 7 February 2002 by

text: Lincoln Near-Earth Asteroid Research

text: (LINEAR) at an

text: apparent magnitude

text: of 19 using a

text: reflecting telescope

text: . It has an estimated diameter of . The asteroid was listed on

text: Sentry Risk Table

text: with a

text: Torino Scale

text: rating of 1 on 20 March 2002.

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answers: Near-Earth

answers: NDQ_003822

answers: is a near-Earth asteroid

answers: NDQ_003823

answers: It has an estimated diameter of

answers: NDQ_003824

answers: It was discovered on 7 February 2002

answers: NDQ_003825

answers: is a near-Earth asteroid

answers: NDQ_003826

answers: Near-Earth

answers: NDQ_003827

answers: potentially hazardous

answers: NDQ_003828

answers: 2002 CU11

answers: NDQ_003829

answers: The asteroid has an estimated diameter of

answers: NDQ_003830

answers: potentially hazardous object

text: 44 Nysa  is a large and very bright main-belt asteroid, and the brightest member of the Nysian asteroid family. It is classified as a rare class E asteroid and is probably the largest of this type (though 55 Pandora is only slightly smaller).

text: 44 Nysa  is a large and very bright

text: main-belt

text: asteroid

text: , and the brightest member of the

text: Nysian asteroid family

text: . It is classified as a rare

text: class E

text: asteroid and is probably the largest of this type (though

text: 55 Pandora

text: is only slightly smaller).

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answers: class E

answers: NDQ_003822

answers: 44 Nysa

answers: NDQ_003823

answers: 44 Nysa

answers: NDQ_003824

answers: 44 Nysa

answers: NDQ_003825

answers: 44 Nysa

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: class E

answers: NDQ_003828

answers: 44 Nysa

answers: NDQ_003829

answers: 44 Nysa

answers: NDQ_003830

answers: rare

text: Atira asteroids or Apohele asteroids, also known as Interior-Earth Objects (IEOs), are asteroids, whose orbits are entirely confined within Earth's orbit, that is, their orbit has an aphelion (farthest point from the Sun) smaller than Earth's perihelion (nearest point to the Sun), which is 0.983 astronomical units (AU). Atira asteroids are by far the smallest group of near-Earth objects, compared to the Aten, Apollo and Amor asteroids.

text: Atira asteroids or Apohele asteroids, also known as Interior-Earth Objects (IEOs), are

text: asteroid

text: s, whose orbits are entirely confined within

text: Earth

text: 's orbit, that is, their orbit has an

text: aphelion

text: (farthest point from the Sun) smaller than Earth's

text: perihelion

text: (nearest point to the Sun), which is 0.983

text: astronomical unit

text: s (AU). Atira asteroids are by far the smallest group of

text: near-Earth object

text: s, compared to the

text: Aten

text: Apollo

text: and

text: Amor

text: asteroids.

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answers: near-Earth objects

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answers: Asteroids do not have craters

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answers: Atira asteroids

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answers: near-Earth objects

text: Dynamical models indicate that  migrated inward across the inner asteroid belt over long timescales (i.e. the order of ~0.01–1 Gyr) until it reached a planetary gravitational resonance that drove it into the near-Earth asteroid (NEA) population over a timescale of the order of ~1 Myr. From there, gravitational interactions with both the planets and resonances allowed it to reach its current orbit within a few Myr to a few tens of Myr.

text: Dynamical models indicate that  migrated inward across the inner asteroid belt over long timescales (i.e. the order of ~0.01–1 Gyr) until it reached a planetary gravitational resonance that drove it into the near-Earth asteroid (NEA) population over a timescale of the order of ~1 Myr. From there, gravitational interactions with both the planets and resonances allowed it to reach its current orbit within a few Myr to a few tens of Myr.

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answers: NEA

answers: NDQ_003822

answers: NEA

answers: NDQ_003823

answers: Gravitational interactions

answers: NDQ_003824

answers: Dynamical models

answers: NDQ_003825

answers: NEA

answers: NDQ_003826

answers: inner asteroid belt

answers: NDQ_003827

answers: drive it into the near-Earth asteroid population

answers: NDQ_003828

answers: Gravitational interactions

answers: NDQ_003829

answers: NEA

answers: NDQ_003830

answers: NEA

text: 235 Carolina is a sizeable Main belt asteroid. It is an S-type asteroid.

text: 235 Carolina is a sizeable

text: Main belt

text: asteroid

text: . It is an

text: S-type asteroid

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answers: NDQ_003826

answers: Main belt

answers: NDQ_003827

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answers: NDQ_003828

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answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: sizeable

answers: NDQ_003822

answers: Main belt

answers: NDQ_003823

answers: no

answers: NDQ_003824

answers: 235 Carolina is a sizeable

answers: NDQ_003825

answers: Main belt

answers: NDQ_003826

answers: Main belt

answers: NDQ_003827

answers: sizeable

answers: NDQ_003828

answers: 235 Carolina

answers: NDQ_003829

answers: S-type asteroid

answers: NDQ_003830

answers: S-type asteroid

text: Sisyphus will pass  from Earth on 24 November 2071, and will peak at roughly apparent magnitude 9.3 on November 26, 2071. When it was discovered it peaked at magnitude 9.0 on 25 November 1972. It is one of the brightest near-Earth asteroids. With a measured mean diameter in the range of 5.7–8.9 kilometers, it the largest of the Earth-crossing asteroids, comparable in size to the Chicxulub object whose impact contributed to the extinction of the dinosaurs. Larger near-Earth asteroids which are neither classified as Apollos nor Earth-crossers include 1036 Ganymed (32 km), 3552 Don Quixote (19 km), 433 Eros (17 km), and 4954 Eric (10.8 km).

text: Sisyphus will pass  from Earth on 24 November 2071, and will peak at roughly

text: apparent magnitude

text: 9.3 on November 26, 2071. When it was discovered it peaked at magnitude 9.0 on 25 November 1972. It is one of the brightest near-Earth asteroids. With a measured mean diameter in the range of 5.7–8.9 kilometers, it the largest of the

text: Earth-crossing asteroids

text: , comparable in size to the

text: Chicxulub

text: object whose impact contributed to the

text: extinction

text: of the dinosaurs. Larger near-Earth asteroids which are neither classified as Apollos nor Earth-crossers include

text: 1036 Ganymed

text: (32 km),

text: 3552 Don Quixote

text: (19 km),

text: 433 Eros

text: (17 km), and

text: 4954 Eric

text: (10.8 km).

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answers: NDQ_003821

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answers: 4

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answers: NDQ_003824

answers: 0

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answers: 4

answers: NDQ_003826

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answers: 4

answers: NDQ_003828

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answers: NDQ_003829

answers: 0

answers: NDQ_003830

answers: 0

answers: NDQ_003821

answers: near-Earth

answers: NDQ_003822

answers: Sisyphus

answers: NDQ_003823

answers: Earth-crossing asteroids

answers: NDQ_003824

answers: Larger near-Earth asteroids which are neither classified as Apollos nor Earth-crossers

answers: NDQ_003825

answers: Sisyphus

answers: NDQ_003826

answers: near-Earth

answers: NDQ_003827

answers: Earth-crossing

answers: NDQ_003828

answers: Chicxulub

answers: NDQ_003829

answers: It is one of the brightest near-Earth asteroids

answers: NDQ_003830

answers: Earth-crossing asteroids

text: An asteroid in the Asteroid belt, 10102 Digerhuvud, is named after the area.

text: An

text: asteroid

text: in the

text: Asteroid belt

text: 10102 Digerhuvud

text: , is

text: named

text: after the area.

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

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answers: NDQ_003826

answers: Asteroid belt

answers: NDQ_003827

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answers: NDQ_003821

answers: named after the area

answers: NDQ_003822

answers: in the Asteroid belt

answers: NDQ_003823

answers: It does not have craters.

answers: NDQ_003824

answers: 10102 Digerhuvud

answers: NDQ_003825

answers: in the Asteroid belt

answers: NDQ_003826

answers: Asteroid belt

answers: NDQ_003827

answers: name after the area

answers: NDQ_003828

answers: 10102 Digerhuvud

answers: NDQ_003829

answers: 10102 Digerhuvud

answers: NDQ_003830

answers: Asteroid belt

text: Located in the outermost part of the main-belt, the asteroid is a member of the Hilda family, a large group of asteroids that are thought to have originated from the Kuiper belt. They orbit in a 3:2 orbital resonance with the gas giant Jupiter, meaning that for every 2 orbits Jupiter completes around the Sun, a Hildian asteroid will complete 3 orbits. The asteroid's orbit does not cross the path of any of the planets and therefore it will not be pulled out of orbit by Jupiter's gravitational field. As a result of this, it is likely that the asteroid will remain in a stable orbit for thousands of years.

text: Located in the outermost part of the main-belt, the asteroid is a member of the

text: Hilda family

text: , a large group of asteroids that are thought to have originated from the

text: Kuiper belt

text: . They orbit in a 3:2

text: orbital resonance

text: with the gas giant Jupiter, meaning that for every 2 orbits Jupiter completes around the Sun, a Hildian asteroid will complete 3 orbits. The asteroid's orbit does not cross the path of any of the planets and therefore it will not be pulled out of orbit by Jupiter's gravitational field. As a result of this, it is likely that the asteroid will remain in a stable orbit for thousands of years.

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answers: a member of the Hilda family

answers: NDQ_003822

answers: Hilda family

answers: NDQ_003823

answers: The asteroid's orbit does not cross the path of any of the planets

answers: NDQ_003824

answers: They orbit in a 3:2 orbital resonance with the gas giant Jupiter

answers: NDQ_003825

answers: Hilda family

answers: NDQ_003826

answers: main-belt

answers: NDQ_003827

answers: orbital resonance with the gas giant Jupiter

answers: NDQ_003828

answers: It orbits in a 3:2 orbital resonance

answers: NDQ_003829

answers: It is unlikely that the asteroid will remain in a stable orbit

answers: NDQ_003830

answers: Jupiter's gravitational field

text: 121 Hermione is a very large asteroid discovered in 1872. It orbits in the Cybele group in the far outer asteroid belt. As an asteroid of the dark C spectral type, it is probably composed of carbonaceous materials. In 2002, a small moon was found to be orbiting Hermione.

text: 121 Hermione is a very large

text: asteroid

text: discovered in 1872. It orbits in the

text: Cybele group

text: in the far outer

text: asteroid belt

text: . As an asteroid of the dark

text: C spectral type

text: , it is probably composed of

text: carbonaceous

text: materials. In 2002, a small

text: moon

text: was found to be orbiting Hermione.

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answers: asteroid belt

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answers: discovered

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answers: Cybele group

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answers: asteroids

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answers: asteroid

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answers: Cybele group

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answers: asteroid belt

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answers: 121 Hermione

answers: NDQ_003829

answers: 121 Hermione

answers: NDQ_003830

answers: asteroid

text: The Hygiea or Hygiean family of asteroids is a grouping of dark, carbonaceous C-type and B-type asteroids in outer asteroid belt, the largest member of which is 10 Hygiea. About 1% of all known asteroids in the asteroid belt belong to this family.

text: The Hygiea or Hygiean

text: family of asteroids

text: is a grouping of dark,

text: carbon

text: aceous

text: C-type

text: and

text: B-type

text: asteroid

text: s in outer

text: asteroid belt

text: , the largest member of which is

text: 10 Hygiea

text: . About 1% of all known asteroids in the asteroid belt belong to this family.

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answers: asteroid belt

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answers: carbonaceous

answers: NDQ_003822

answers: C-type and B-type

answers: NDQ_003823

answers: asteroids

answers: NDQ_003824

answers: about 1% of all known asteroids in the asteroid belt

answers: NDQ_003825

answers: C-type and B-type

answers: NDQ_003826

answers: outer asteroid belt

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answers: 10 Hygiea

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answers: 10 Hygiea

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answers: Hygiean family of asteroids

text: From the perspective of Earth, the only types of asteroids that can transit the Sun are those with orbits that take them between the two bodies. These include Aten asteroids (including Apohele asteroids and the hypothetical Vulcanoid asteroids) and some Apollo asteroids (perhaps including quasi-satellites of Earth). Unfortunately, observations of such transits are difficult because all of these asteroids are only a few kilometres in diameter at most, so that their angular diameter is too tiny to observe against the Sun.

text: From the perspective of Earth, the only types of asteroids that can transit the Sun are those with orbits that take them between the two bodies. These include

text: Aten asteroid

text: s (including

text: Apohele asteroid

text: s and the hypothetical

text: Vulcanoid asteroid

text: s) and some

text: Apollo asteroid

text: s (perhaps including

text: quasi-satellite

text: s of Earth). Unfortunately, observations of such transits are difficult because all of these asteroids are only a few kilometres in diameter at most, so that their

text: angular diameter

text: is too tiny to observe against the Sun.

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answers: NDQ_003821

answers: kilometres in diameter at most

answers: NDQ_003822

answers: can transit the Sun

answers: NDQ_003823

answers: asteroids are too small to have impacts

answers: NDQ_003824

answers: angular diameter is too tiny to observe against the Sun

answers: NDQ_003825

answers: can transit the Sun

answers: NDQ_003826

answers: Aten

answers: NDQ_003827

answers: transit the Sun

answers: NDQ_003828

answers: Apollo asteroids

answers: NDQ_003829

answers: Vulcanoid asteroids

answers: NDQ_003830

answers: transits

text: The Asteroid Impact and Deflection Assessment (AIDA) mission is a proposed space probe which would study and demonstrate the kinetic effects of crashing an impactor spacecraft into an asteroid moon. The mission is intended to test whether a spacecraft could successfully deflect an asteroid on a collision course with Earth. It would be composed of two spacecraft: AIM, which would orbit the asteroid, and DART, which would impact its moon. Besides the observation of the change of orbital parameters of the asteroid moon, the observation of the plume, the crater, and the freshly exposed material will provide truly unique information for asteroid deflection, science and mining communities.

text: The Asteroid Impact and Deflection Assessment (AIDA) mission is a proposed

text: space probe

text: which would study and demonstrate the kinetic effects of crashing an impactor spacecraft into an

text: asteroid moon

text: . The mission is intended to test whether a spacecraft could successfully

text: deflect an asteroid

text: on a collision course with

text: Earth

text: . It would be composed of two spacecraft: AIM, which would orbit the asteroid, and DART, which would impact its moon. Besides the observation of the change of orbital parameters of the asteroid moon, the observation of the plume, the crater, and the freshly exposed material will provide truly unique information for asteroid deflection, science and mining communities.

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answers: NDQ_003821

answers: an asteroid

answers: NDQ_003822

answers: Asteroid

answers: NDQ_003823

answers: No

answers: NDQ_003824

answers: It would be composed of two spacecraft

answers: NDQ_003825

answers: Asteroid

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: collision course with Earth

answers: NDQ_003828

answers: DART, which would impact its moon

answers: NDQ_003829

answers: The mission is intended to test whether a spacecraft could successfully deflect an asteroid

answers: NDQ_003830

answers: mining communities

text: 19383 Rolling Stones (1998 BZ32) is a main-belt asteroid discovered on January 29, 1998, by the OCA-DLR Asteroid Survey at Caussols. It has been named in honor of the English musical group The Rolling Stones.

text: 19383 Rolling Stones (1998 BZ32) is a

text: main-belt

text: asteroid

text: discovered on January 29, 1998, by the

text: OCA-DLR Asteroid Survey

text: at

text: Caussols

text: . It has been named in honor of the English musical group

text: The Rolling Stones

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answers: Asteroid Survey

text: Richey is the Deputy Science Advisor for the NASA  Science Mission Directorate (SMD), where she compiles and distributes information about the Research and Analysis (R&A) awards from the SMD Divisions, and focuses on communication with the greater communities working directly with the SMD. Additionally, she is the Deputy Program Scientist in the Planetary Science Division for the OSIRIS-REx Mission (the Origins Spectral Interpretation Resource Identification Security- Regolith Mission). OSIRIS-REx launched in 2016 and will travel to a near-Earth Asteroid, called Bennu and bring back a returned sample to Earth for study.  The mission will help scientists investigate how planets formed and how life began, as well as improve our understanding of asteroids that could impact Earth.  She is additionally a Program Officer in PSD, where she runs several R&A Programs.

text: Richey is the Deputy Science Advisor for the

text: NASA

text: Science Mission Directorate

text: (SMD), where she compiles and distributes information about the Research and Analysis (R&A) awards from the SMD Divisions, and focuses on communication with the greater communities working directly with the SMD. Additionally, she is the Deputy Program Scientist in the Planetary Science Division for the

text: OSIRIS-REx

text: Mission (the Origins Spectral Interpretation Resource Identification Security- Regolith Mission).

text: OSIRIS-REx

text: launched in 2016 and will travel to a near-Earth Asteroid, called

text: Bennu

text: and bring back a returned sample to Earth for study.  The mission will help scientists investigate how planets formed and how life began, as well as improve our understanding of asteroids that could impact Earth.  She is additionally a Program Officer in PSD, where she runs several R&A Programs.

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answers: could impact Earth

text: According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures 3.9 kilometers in diameter and its surface has an albedo of 0.075, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 4.2 kilometers.

text: According to the survey carried out by NASA's

text: Wide-field Infrared Survey Explorer

text: with its subsequent

text: NEOWISE

text: mission, the asteroid measures 3.9 kilometers in diameter and its surface has an

text: albedo

text: of 0.075, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 4.2 kilometers.

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answers: carbonaceous asteroids

text: (136617) 1994 CC is a near-Earth asteroid that was discovered on February 3, 1994, by Spacewatch's Jim Scotti. In June 2009 it was shown to be a triple system, i.e. the largest body is orbited by two satellites; only about one percent (1%) of near-Earth asteroids observed by a radar are found to be triple systems such as this one.The only other unambiguously identified triple asteroid in the near-Earth population is , which was discovered to be a triple system in 2008.

text: (136617) 1994 CC is a

text: near-Earth asteroid

text: that was discovered on February 3, 1994, by

text: Spacewatch

text: 's

text: Jim Scotti

text: . In June 2009 it was shown to be a triple system, i.e. the largest body is orbited by two

text: satellites

text: ; only about one percent (1%) of near-Earth asteroids observed by a radar are found to be triple systems such as this one.The only other unambiguously identified triple asteroid in the near-Earth population is , which was discovered to be a triple system in 2008.

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answers: orbited by two satellites

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answers: Near-Earth

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answers: (136617) 1994 CC is a near-Earth asteroid

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answers: (136617) 1994 CC is a near-Earth asteroid

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answers: Near-Earth

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answers: near-Earth

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answers: orbited by two satellite

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answers: (136617) 1994 CC

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answers: (136617) 1994 CC

answers: NDQ_003830

answers: are orbited by two satellites

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2014.

text: An example list of near-Earth asteroids that passed more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2014.

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

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text: The Asteroid Redirect Mission (ARM), also known as the Asteroid Retrieval and Utilization (ARU) mission and the Asteroid Initiative, is a potential future space mission proposed by NASA. Still in the early stages of planning and development, the Asteroid Retrieval Robotic Mission (ARRM) spacecraft would rendezvous with a large near-Earth asteroid and use robotic arms with anchoring grippers to retrieve a 4-meter boulder from the asteroid.

text: The Asteroid Redirect Mission (ARM), also known as the Asteroid Retrieval and Utilization (ARU) mission and the Asteroid Initiative, is a potential future

text: space mission

text: proposed by

text: NASA

text: . Still in the early stages of planning and development, the Asteroid Retrieval Robotic Mission (ARRM) spacecraft would rendezvous with a large

text: near-Earth asteroid

text: and use robotic arms with anchoring grippers to retrieve a 4-meter boulder from the asteroid.

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answers: retrieve a 4-meter boulder

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answers: The Asteroid Redirect Mission

answers: NDQ_003830

answers: Asteroid Initiative

text: On 12 November, Hayabusa closed in to  from the asteroid's surface.  MINERVA was released but due to an error failed to reach the surface. On 19 November, Hayabusa landed on the asteroid. There was considerable confusion during and after the maneuver about precisely what had happened, because the high-gain antenna of the probe could not be used during final phase of touch-down, as well as the blackout during handover of ground station antenna from DSN to Usuda station.  It was initially reported that Hayabusa had stopped at approximately 10 meters from the surface, hovering for 30 minutes for unknown reasons. Ground control sent a command to abort and ascend, and by the time the communication was regained, the probe had moved 100 km away from the asteroid.  The probe had entered into a safe mode, slowly spinning to stabilize attitude control. However, after regaining control and communication with the probe, the data from the landing attempt were downloaded and analyzed, and on 23 November, JAXA announced that the probe had indeed landed on the asteroid's surface. Unfortunately, the sampling sequence was not triggered since a sensor detected an obstacle during descent; the probe tried to abort the landing, but since its altitude was not appropriate for ascent, it chose instead a safe descent mode. This mode did not permit a sample to be taken, but there is a high probability that some dust may have whirled up into the sampling horn when it touched the asteroid, so the sample canister currently attached to the sampling horn was sealed.  On November 25, a second touchdown attempt was performed. It was initially thought that this time, the sampling device was activated; however, later analysis decided that this was probably another failure and that no pellets were fired. Due to a leak in the thruster system, the probe was put in a "safe hold mode".

text: On 12 November, Hayabusa closed in to  from the asteroid's surface.  MINERVA was released but due to an error failed to reach the surface. On 19 November, Hayabusa landed on the asteroid. There was considerable confusion during and after the maneuver about precisely what had happened, because the high-gain antenna of the probe could not be used during final phase of touch-down, as well as the blackout during handover of ground station antenna from

text: DSN

text: to Usuda station.  It was initially reported that Hayabusa had stopped at approximately 10 meters from the surface, hovering for 30 minutes for unknown reasons. Ground control sent a command to abort and ascend, and by the time the communication was regained, the probe had moved 100 km away from the asteroid.  The probe had entered into a

text: safe mode

text: , slowly spinning to stabilize

text: attitude control

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answers: surface

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answers: Hayabusa

answers: NDQ_003823

answers: Hayabusa landed on the asteroid

answers: NDQ_003824

answers: Hayabusa landed on the asteroid

answers: NDQ_003825

answers: Hayabusa

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: landed on the asteroid

answers: NDQ_003828

answers: MINERVA was released but due to an error failed to reach the surface

answers: NDQ_003829

answers: It was initially reported that Hayabusa had stopped at approximately 10 meters from the surface

answers: NDQ_003830

answers: asteroid

text: In its yearly trek around the sun, asteroid  spends about half of the time closer to the sun than Earth is (that is, the asteroid is inside the Earth's orbit) and passes ahead of our planet, and about half of the time farther away (crosses outside Earth's orbit), causing it to fall behind. Its orbit is also tilted a little, causing it to bob up and then down once each year through Earth's orbital plane. In effect, this small asteroid is caught in a game of leap frog with Earth that will last for hundreds of years.

text: In its yearly trek around the sun, asteroid  spends about half of the time closer to the sun than Earth is (that is, the asteroid is inside the

text: Earth's orbit

text: ) and passes ahead of our planet, and about half of the time farther away (crosses outside Earth's orbit), causing it to fall behind. Its orbit is also tilted a little, causing it to bob up and then down once each year through Earth's orbital plane. In effect, this small asteroid is caught in a game of leap frog with Earth that will last for hundreds of years.

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answers: Earth's orbit

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answers: in its yearly trek around the sun

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answers: No craters

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answers: nasa missions to visit them

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answers: in its yearly trek around the sun

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answers: passes ahead of our planet

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answers: Its orbit is also tilted a little

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answers: Its orbit is also tilted a little

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answers: Earth's orbit

text: {{Infobox video game| title       = Asteroids| image       = Asteroids-arcadegame.jpg| caption     = A promotional flyer for Asteroids, featuring the arcade cabinet over a background of floating asteroids surrounding a planet. The Asteroids logo and details about the game are seen in the bottom of the flyer.| developer   = Atari, Inc.| publisher   = Atari, Inc.| distributor =| designer    = Lyle Rains<br>Ed Logg

text: {{Infobox video game| title       = Asteroids| image       = Asteroids-arcadegame.jpg| caption     = A promotional flyer for Asteroids, featuring the arcade cabinet over a background of floating asteroids surrounding a planet. The Asteroids logo and details about the game are seen in the bottom of the flyer.| developer   =

text: Atari, Inc.

text: | publisher   = Atari, Inc.| distributor =| designer    =

text: Lyle Rains

text: <br>

text: Ed Logg

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

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answers: floating

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answers: Atari, Inc.

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answers: asteroids are too small to have impacts with other objects so they dont have craters

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answers: Asteroids is a video game developed by Atari, Inc. and published by Atari, Inc.

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answers: An asteroid could cause humans to go extinct.

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answers: asteroids orbit planets

text: Most asteroids within the asteroid belt have orbital eccentricities of less than 0.4, and an inclination of less than 30°. The orbital distribution of the asteroids reaches a maximum at an eccentricity of around 0.07 and an inclination below 4°. Thus although a typical asteroid has a relatively circular orbit and lies near the plane of the ecliptic, some asteroid orbits can be highly eccentric or travel well outside the ecliptic plane.

text: Most asteroids within the asteroid belt have orbital eccentricities of less than 0.4, and an inclination of less than 30°. The orbital distribution of the asteroids reaches a maximum at an eccentricity of around 0.07 and an inclination below 4°. Thus although a typical asteroid has a relatively circular orbit and lies near the plane of the

text: ecliptic

text: , some asteroid orbits can be highly eccentric or travel well outside the ecliptic plane.

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answers: orbital eccentricities

answers: NDQ_003822

answers: within the asteroid belt

answers: NDQ_003823

answers: asteroids are too small to have impacts with other objects so they dont have craters

answers: NDQ_003824

answers: asteroids within the asteroid belt

answers: NDQ_003825

answers: within the asteroid belt

answers: NDQ_003826

answers: asteroid belt

answers: NDQ_003827

answers: travel well outside the ecliptic plane

answers: NDQ_003828

answers: asteroid belt

answers: NDQ_003829

answers: Asteroids can be highly eccentric or travel well outside the ecliptic plane

answers: NDQ_003830

answers: orbital eccentricities of less than 0.4

text: The AIDA mission is a joint international collaboration of the European Space Agency (ESA), the German Aerospace Center (DLR), Observatoire de la Côte d'Azur (OCA), NASA, and Johns Hopkins University Applied Physics Laboratory (JHU/APL). The project was formed by joining two separate studies, called Double Asteroid Redirection Test (DART), an asteroid impactor developed by NASA, and a monitoring spacecraft - ESA's Asteroid Impact Mission (AIM).

text: The AIDA mission is a joint international collaboration of the

text: European Space Agency

text: (ESA), the

text: German Aerospace Center

text: (DLR), Observatoire de la Côte d'Azur (OCA), NASA, and Johns Hopkins University Applied Physics Laboratory (JHU/APL). The project was formed by joining two separate studies, called

text: Double Asteroid Redirection Test

text: (DART), an asteroid impactor developed by NASA, and a monitoring spacecraft - ESA's

text: Asteroid Impact Mission

text: (AIM).

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