id string | question string | answer string | documents list |
|---|---|---|---|
(+)-Naloxone_16265674 | What information does the article about '(+)-Naloxone' provide? | (+)-Naloxone (dextro-naloxone) is a drug which is the "unnatural" enantiomer of the opioid antagonist drug (β)-naloxone. Unlike "normal" naloxone, (+)-naloxone has no significant affinity for opioid receptors, but instead has been discovered to act as a selective antagonist of Toll-like receptor 4. This receptor is inv... | [
"(+)-Naloxone β Relation with opioids\n\nBoth \"normal\" and \"unnatural\" enantiomers of various opioid analgesic drugs including morphine, meperidine, fentanyl, methadone and buprenorphine, as well as some otherwise inactive metabolites like morphine-3-glucuronide, have been found to act as agonists of TLR4, and ... |
(10115)_1992_SK_15802780 | Based on the article about '(10115) 1992 SK', describe the 'Rotation period' section. | Several rotational lightcurves form photometric observations have been obtained for this body. In 1999, Czech astronomer Petr Pravec constructed a lightcurve, that rendered a rotation period of 7.328 hours and a brightness variation of 0.72 in magnitude (U=n/a). In March 2006, observations by astronomer David Polishook... | [
"(10115) 1992 SK β Rotation period\n\nSeveral rotational lightcurves form photometric observations have been obtained for this body. In 1999, Czech astronomer Petr Pravec constructed a lightcurve, that rendered a rotation period of 7.328 hours and a brightness variation of 0.72 in magnitude (U=n/a). In March 2006, ... |
(10115)_1992_SK_15802781 | What does the article about '(10115) 1992 SK' say regarding 'Diameter and albedo'? | According to the surveys carried out by NASA's space-based Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures 1.0 and 0.94 kilometers in diameter and its surface has an albedo of 0.28 ot 0.32, respectively. The ExploreNEOs project finds an albedo of 0.34, with an diameter of ... | [
"(10115) 1992 SK β Rotation period\n\nSeveral rotational lightcurves form photometric observations have been obtained for this body. In 1999, Czech astronomer Petr Pravec constructed a lightcurve, that rendered a rotation period of 7.328 hours and a brightness variation of 0.72 in magnitude (U=n/a). In March 2006, ... |
(10115)_1992_SK_15802778 | Based on the article about '(10115) 1992 SK', describe the 'Classification and orbit' section. | The asteroid orbits the Sun at a distance of 0.8β1.7 AU once every 17 months (509 days). Its orbit has an eccentricity of 0.32 and an inclination of 15Β° with respect to the ecliptic. Its Earth minimum orbit intersection distance is 0.0449 AU. This makes the body a potentially hazardous asteroid, because its MOID is les... | [
"(10115) 1992 SK β Rotation period\n\nSeveral rotational lightcurves form photometric observations have been obtained for this body. In 1999, Czech astronomer Petr Pravec constructed a lightcurve, that rendered a rotation period of 7.328 hours and a brightness variation of 0.72 in magnitude (U=n/a). In March 2006, ... |
(10115)_1992_SK_15802782 | What information does the article about '(10115) 1992 SK' provide on 'Numbering and naming'? | This minor planet was numbered by the Minor Planet Center on 2 March 1999. , it has not been named. | [
"(10115) 1992 SK β Rotation period\n\nSeveral rotational lightcurves form photometric observations have been obtained for this body. In 1999, Czech astronomer Petr Pravec constructed a lightcurve, that rendered a rotation period of 7.328 hours and a brightness variation of 0.72 in magnitude (U=n/a). In March 2006, ... |
(101869)_1999_MM_18920878 | Summarize the 'Physical characteristics' part of '(101869) 1999 MM'. | Based on its absolute magnitude of 19.3, its mean-diameter is between 370 and 830 meters, assuming an albedo in the range of 0.05 to 0.25. | [
"(101869) 1999 MM β Physical characteristics\n\nBased on its absolute magnitude of 19.3, its mean-diameter is between 370 and 830 meters, assuming an albedo in the range of 0.05 to 0.25.",
"(101869) 1999 MM β Orbit and classification\n\nThe asteroid orbits the Sun at a distance of 0.6β2.6 AU once every 2 years an... |
(101869)_1999_MM_18920877 | Reconstruct the content about 'Orbit and classification' from the article on '(101869) 1999 MM'. | The asteroid orbits the Sun at a distance of 0.6β2.6 AU once every 2 years and 1 month (756 days). Its orbit has an eccentricity of 0.61 and an inclination of 5Β° with respect to the ecliptic. It has a notably low Earth minimum orbit intersection distance of 0.0016 AU, which is less than one lunar distance, and also app... | [
"(101869) 1999 MM β Physical characteristics\n\nBased on its absolute magnitude of 19.3, its mean-diameter is between 370 and 830 meters, assuming an albedo in the range of 0.05 to 0.25.",
"(101869) 1999 MM β Orbit and classification\n\nThe asteroid orbits the Sun at a distance of 0.6β2.6 AU once every 2 years an... |
(101869)_1999_MM_18920876 | Summarize the following section from the article on '(101869) 1999 MM'. | , provisional designation is a sub-kilometer asteroid on an eccentric orbit, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group. It was discovered on 20 June 1999, by the Lowell Observatory Near-Earth-Object Search (LONEOS) at its U.S. Anderson Mesa Station in Flagstaff, Arizona. T... | [
"(101869) 1999 MM β Physical characteristics\n\nBased on its absolute magnitude of 19.3, its mean-diameter is between 370 and 830 meters, assuming an albedo in the range of 0.05 to 0.25.",
"(101869) 1999 MM β Orbit and classification\n\nThe asteroid orbits the Sun at a distance of 0.6β2.6 AU once every 2 years an... |
(111253)_2001_XU10_1388129 | What does the article about '(111253) 2001 XU10' say regarding 'Close approaches'? | With an absolute magnitude of 15.2, is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of 0.0293 AU, which translates into 11.4 lunar distances (LD). On 29 July 2054, this asteroid will make its closest near-Earth enc... | [
"(111253) 2001 XU10 β Close approaches\n\nWith an absolute magnitude of 15.2, is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of 0.0293 AU, which translates into 11.4 lunar distances (LD). On 29 July 2054, this... |
(111253)_2001_XU10_1388128 | What does the article about '(111253) 2001 XU10' say regarding 'Orbit and classification'? | orbits the Sun at a distance of 0.98β2.52 AU once every 2 years and 4 months (848 days; semi-major axis of 1.75 AU). Its orbit has an eccentricity of 0.44 and an inclination of 42Β° with respect to the ecliptic. The body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in February 2000. is... | [
"(111253) 2001 XU10 β Close approaches\n\nWith an absolute magnitude of 15.2, is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of 0.0293 AU, which translates into 11.4 lunar distances (LD). On 29 July 2054, this... |
(111253)_2001_XU10_1388127 | Reconstruct the content from the article about '(111253) 2001 XU10'. | , provisional designation, is an asteroid on an eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 3 kilometers in diameter. It was discovered on 9 December 2001, by astronomers of the LINEAR program at Lincoln Laboratory's Experimental Test Site near ... | [
"(111253) 2001 XU10 β Close approaches\n\nWith an absolute magnitude of 15.2, is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of 0.0293 AU, which translates into 11.4 lunar distances (LD). On 29 July 2054, this... |
(111253)_2001_XU10_1388130 | Based on the article about '(111253) 2001 XU10', describe the 'Physical characteristics' section. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 3.006 kilometers in diameter and its surface has an albedo of 0.178. As of 2018, no rotational lightcurve of has been obtained from photometric observations. The asteroid's rotation period, spin axis and s... | [
"(111253) 2001 XU10 β Close approaches\n\nWith an absolute magnitude of 15.2, is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of 0.0293 AU, which translates into 11.4 lunar distances (LD). On 29 July 2054, this... |
(111253)_2001_XU10_1388131 | Explain what '(111253) 2001 XU10' covers in the 'Numbering and naming' section. | This minor planet was numbered by the Minor Planet Center on 19 October 2005. As of 2018, it has not been named. | [
"(111253) 2001 XU10 β Close approaches\n\nWith an absolute magnitude of 15.2, is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of 0.0293 AU, which translates into 11.4 lunar distances (LD). On 29 July 2054, this... |
(11436)_1969_QR_18150330 | Reconstruct the content from the article about '(11436) 1969 QR'. | , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 3.7 kilometers in diameter. It was discovered on 22 August 1969, by Czech astronomer LuboΕ‘ Kohoutek at Bergedorf Observatory in Hamburg, Germany. | [
"(11436) 1969 QR\n\n, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 3.7 kilometers in diameter. It was discovered on 22 August 1969, by Czech astronomer LuboΕ‘ Kohoutek at Bergedorf Observatory in Hamburg, Germany.",
"(11436) 1969 QR β Description\n\nThe S-type asteroid is ... |
(11436)_1969_QR_18150331 | Describe the 'Description' section of the article about '(11436) 1969 QR'. | 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 1.9β2.5 AU once every 3 years and 4 months (1,212 days). Its orbit has an eccentricity of 0.14 and an inclination of 7Β° with respect to the ecliptic. As no precoveries w... | [
"(11436) 1969 QR\n\n, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 3.7 kilometers in diameter. It was discovered on 22 August 1969, by Czech astronomer LuboΕ‘ Kohoutek at Bergedorf Observatory in Hamburg, Germany.",
"(11436) 1969 QR β Description\n\nThe S-type asteroid is ... |
(11436)_1969_QR_18150332 | Based on the article about '(11436) 1969 QR', describe the 'Numbering and naming' section. | This minor planet was numbered by the Minor Planet Center on 28 September 1999. As of 2018, it has not been named. | [
"(11436) 1969 QR\n\n, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 3.7 kilometers in diameter. It was discovered on 22 August 1969, by Czech astronomer LuboΕ‘ Kohoutek at Bergedorf Observatory in Hamburg, Germany.",
"(11436) 1969 QR β Description\n\nThe S-type asteroid is ... |
(11474)_1982_SM2_30764173 | Summarize the 'Numbering and naming' part of '(11474) 1982 SM2'. | This minor planet was numbered by the Minor Planet Center on 28 September 1999. As of 2018, it has not been named. | [
"(11474) 1982 SM2 β Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 28 September 1999. As of 2018, it has not been named.",
"(11474) 1982 SM2 β Physical characteristics\n\nIn September 2013, a rotational lightcurve of this asteroid was obtained from photometric observations in... |
(11474)_1982_SM2_30764172 | Summarize the 'Physical characteristics' part of '(11474) 1982 SM2'. | In September 2013, a rotational lightcurve of this asteroid was obtained from photometric observations in the R-band at the Palomar Transient Factory in California. It gave an exceptionally long rotation period of 1917 hours with a brightness amplitude of 0.04 magnitude (U=1). However, the fragmentary light-curve has r... | [
"(11474) 1982 SM2 β Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 28 September 1999. As of 2018, it has not been named.",
"(11474) 1982 SM2 β Physical characteristics\n\nIn September 2013, a rotational lightcurve of this asteroid was obtained from photometric observations in... |
(11474)_1982_SM2_30764170 | Describe the content of the article about '(11474) 1982 SM2'. | is a carbonaceous Baptistina asteroid and potentially slow rotator from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 18 September 1982, by Belgian astronomer Henri Debehogne at ESO La Silla Observatory in northern Chile. | [
"(11474) 1982 SM2 β Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 28 September 1999. As of 2018, it has not been named.",
"(11474) 1982 SM2 β Physical characteristics\n\nIn September 2013, a rotational lightcurve of this asteroid was obtained from photometric observations in... |
(118228)_1996_TQ66_6922091 | What does the article about '(118228) 1996 TQ66' say regarding 'Rotation period'? | In 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotational lightcurve for this object has been obtaine... | [
"(118228) 1996 TQ66 β Rotation period\n\nIn 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotationa... |
(118228)_1996_TQ66_6922087 | Summarize the following section from the article on '(118228) 1996 TQ66'. | , prov. designation:, is a resonant trans-Neptunian object of the plutino population in the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 8 October 1996, by American astronomers Jun Chen, David Jewitt, Chad Trujillo and Jane Luu, using the UH88 telescope at the Mauna Kea Observa... | [
"(118228) 1996 TQ66 β Rotation period\n\nIn 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotationa... |
(118228)_1996_TQ66_6922092 | Explain what '(118228) 1996 TQ66' covers in the 'Diameter and albedo' section. | Based on a generic magnitude-to-diameter conversion, measures approximately 185 km in diameter, for an assumed albedo of 0.9 and an magnitude of 7. According to Mike Brown, who estimates a mean-diameter of 186 km, the object is too small for being considered a dwarf planet candidate ("probably not"). | [
"(118228) 1996 TQ66 β Rotation period\n\nIn 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotationa... |
(118228)_1996_TQ66_6922088 | Based on the article about '(118228) 1996 TQ66', describe the 'Orbit and classification' section. | orbits the Sun at a distance of 34.5β44.2 AU once every 247 years and 1 month (90,254 days; semi-major axis of 39.38 AU). Its orbit has an eccentricity of 0.12 and an inclination of 15Β° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at the Mauna Kea Observatories... | [
"(118228) 1996 TQ66 β Rotation period\n\nIn 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotationa... |
(118228)_1996_TQ66_6922089 | Reconstruct the content about 'Numbering and naming' from the article on '(118228) 1996 TQ66'. | This minor planet was numbered by the Minor Planet Center on 16 November 2005, receiving the number in the minor planet catalog (M.P.C. 55524). , it has not been named. According to the established naming conventions, it will be given a mythological name associated with the underworld. | [
"(118228) 1996 TQ66 β Rotation period\n\nIn 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotationa... |
(118228)_1996_TQ66_6922090 | Based on the article about '(118228) 1996 TQ66', describe the 'Physical characteristics' section. | has a very red surface color (RR) in the visible part of the spectrum, with BβV and VβR color indices of 1.19 and 0.66, respectively, for a combined BβR magnitude of 1.85. A red surface color is typically associated with the presence of tholins, polymer-like organic compounds, formed by long exposures to solar and cosm... | [
"(118228) 1996 TQ66 β Rotation period\n\nIn 1999, results of a photometric survey of Kuiper belt objects by Romanishin and Tegler were published in the Journal Nature. For, a brightness variation of no more than 0.22 in magnitude could be determined, which is indicative of a modestly irregular shape. , no rotationa... |
(118378)_1999_HT11_8701861 | Reconstruct the content from the article about '(118378) 1999 HT11'. | , provisional designation:, is a trans-Neptunian object from the outermost region of the Solar System, locked in a 4:7 orbital resonance with Neptune. It was discovered on 17 April 1999, by astronomers at the Kitt Peak Observatory, Arizona, in the United States. The very red object measures approximately 134 km in diam... | [
"(118378) 1999 HT11\n\n, provisional designation:, is a trans-Neptunian object from the outermost region of the Solar System, locked in a 4:7 orbital resonance with Neptune. It was discovered on 17 April 1999, by astronomers at the Kitt Peak Observatory, Arizona, in the United States. The very red object measures a... |
(118378)_1999_HT11_8701862 | Describe the 'Discovery' section of the article about '(118378) 1999 HT11'. | was first observed on the night of 17 April 1999, by astronomers using the 4-meter Nicholas U. Mayall Telescope at Kitt Peak National Observatory in Arizona. Five additional objects were discovered on the same weekend:, List of unnumbered minor planets: 1999 AβR, 53311 Deucalion (Deucalion), List of unnumbered minor pl... | [
"(118378) 1999 HT11\n\n, provisional designation:, is a trans-Neptunian object from the outermost region of the Solar System, locked in a 4:7 orbital resonance with Neptune. It was discovered on 17 April 1999, by astronomers at the Kitt Peak Observatory, Arizona, in the United States. The very red object measures a... |
(118378)_1999_HT11_8701863 | Summarize the 'Orbit and classification' part of '(118378) 1999 HT11'. | This minor planet orbits the Sun at a distance of 38.7β49.0 AU once every 290 years and 7 months (106,124 days; semi-major axis of 43.87 AU). Its orbit has an eccentricity of 0.12 and an inclination of 5Β° with respect to the ecliptic. , it is at 39.7 AU from the Sun with an apparent magnitude of 23.42, and will come to... | [
"(118378) 1999 HT11\n\n, provisional designation:, is a trans-Neptunian object from the outermost region of the Solar System, locked in a 4:7 orbital resonance with Neptune. It was discovered on 17 April 1999, by astronomers at the Kitt Peak Observatory, Arizona, in the United States. The very red object measures a... |
(118378)_1999_HT11_8701864 | Reconstruct the content about 'Numbering and naming' from the article on '(118378) 1999 HT11'. | This minor planet was numbered by the Minor Planet Center on 16 November 2005, receiving the number in the minor planet catalog (M.P.C. 55526). , it has not been named. According to the established naming conventions, it will be given a mythological name associated with the underworld or with creation. | [
"(118378) 1999 HT11\n\n, provisional designation:, is a trans-Neptunian object from the outermost region of the Solar System, locked in a 4:7 orbital resonance with Neptune. It was discovered on 17 April 1999, by astronomers at the Kitt Peak Observatory, Arizona, in the United States. The very red object measures a... |
(118378)_1999_HT11_8701865 | Based on the article about '(118378) 1999 HT11', describe the 'Physical characteristics' section. | has a very red surface color (RR) in the visible part of the spectrum, with BβV and VβR color indices of 1.15 and 0.67, respectively, for a combined BβR magnitude of 1.82. A red surface color is typically associated with the presence of tholins, polymer-like organic compounds, formed by long exposures to solar and cosm... | [
"(118378) 1999 HT11\n\n, provisional designation:, is a trans-Neptunian object from the outermost region of the Solar System, locked in a 4:7 orbital resonance with Neptune. It was discovered on 17 April 1999, by astronomers at the Kitt Peak Observatory, Arizona, in the United States. The very red object measures a... |
(119070)_2001_KP77_11425365 | Reconstruct the content from the article about '(119070) 2001 KP77'. | , provisional designation:, is a resonant trans-Neptunian object in the Kuiper belt, a circumstellar disc located in the outermost region of the Solar System. It was discovered on 23 May 2001, by American astronomer Marc Buie at the Cerro Tololo Observatory in Chile. The object is locked in a 4:7 orbital resonance with... | [
"(119070) 2001 KP77\n\n, provisional designation:, is a resonant trans-Neptunian object in the Kuiper belt, a circumstellar disc located in the outermost region of the Solar System. It was discovered on 23 May 2001, by American astronomer Marc Buie at the Cerro Tololo Observatory in Chile. The object is locked in a... |
(119070)_2001_KP77_11425366 | Describe the 'Discovery' section of the article about '(119070) 2001 KP77'. | was first observed near its perihelion on 23 May 2001, using the 4-meter Blanco Telescope at Cerro Tololo Inter-American Observatory in Chile. During the same night,, List of unnumbered minor planets: 2001 GβO, were also discovered. Besides Marc Buie, who is solely credited with the discovery of this object, the Minor ... | [
"(119070) 2001 KP77\n\n, provisional designation:, is a resonant trans-Neptunian object in the Kuiper belt, a circumstellar disc located in the outermost region of the Solar System. It was discovered on 23 May 2001, by American astronomer Marc Buie at the Cerro Tololo Observatory in Chile. The object is locked in a... |
(119070)_2001_KP77_11425367 | Based on the article about '(119070) 2001 KP77', describe the 'Orbit and classification' section. | This minor planet orbits the Sun at a distance of 36.1β51.9 AU once every 291 years and 7 months (106,514 days; semi-major axis of 43.98 AU). Its orbit has an eccentricity of 0.18 and an inclination of 3Β° with respect to the ecliptic. The object came to perihelion in 2002. , it is 37.0 AU from the Sun and has an appare... | [
"(119070) 2001 KP77\n\n, provisional designation:, is a resonant trans-Neptunian object in the Kuiper belt, a circumstellar disc located in the outermost region of the Solar System. It was discovered on 23 May 2001, by American astronomer Marc Buie at the Cerro Tololo Observatory in Chile. The object is locked in a... |
(119070)_2001_KP77_11425368 | Explain what '(119070) 2001 KP77' covers in the 'Numbering and naming' section. | This minor planet was numbered by the Minor Planet Center on 16 November 2005, receiving the number in the minor planet catalog (M.P.C. 55533). , it has not been named. According to the established naming conventions, it will be given a mythological name associated with the underworld or with creation. | [
"(119070) 2001 KP77\n\n, provisional designation:, is a resonant trans-Neptunian object in the Kuiper belt, a circumstellar disc located in the outermost region of the Solar System. It was discovered on 23 May 2001, by American astronomer Marc Buie at the Cerro Tololo Observatory in Chile. The object is locked in a... |
(119070)_2001_KP77_11425369 | What information does the article about '(119070) 2001 KP77' provide on 'Physical characteristics'? | This object has a red surface color, with a high BβR color index of 1.72 in the visible part of the spectrum. A red surface color is typically associated with the presence of tholins, polymer-like organic compounds, formed by long exposures to solar and cosmic radiation. A higher BβR magnitude of 1.98 including BβV and... | [
"(119070) 2001 KP77\n\n, provisional designation:, is a resonant trans-Neptunian object in the Kuiper belt, a circumstellar disc located in the outermost region of the Solar System. It was discovered on 23 May 2001, by American astronomer Marc Buie at the Cerro Tololo Observatory in Chile. The object is locked in a... |
(120216)_2004_EW95_11388798 | Reconstruct the content from the article about '(120216) 2004 EW95'. | , provisionally known as, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in this region of space. It is t... | [
"(120216) 2004 EW95\n\n, provisionally known as, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in th... |
(120216)_2004_EW95_11388800 | Reconstruct the content about 'Physical characteristics' from the article on '(120216) 2004 EW95'. | has a dark albedo of 0.04, giving it a diameter of about 291 km. Its reflectance spectrum bears striking resemblance to those of some hydrated C-type asteroids, indicating that this object possibly formed in the same environment as the C-type asteroids found today in the outer asteroid belt. Unlike the majority of smal... | [
"(120216) 2004 EW95\n\n, provisionally known as, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in th... |
(120216)_2004_EW95_11388799 | Explain what '(120216) 2004 EW95' covers in the 'Orbit' section. | Like Pluto, is classified as a plutino. It stays in a 2:3 resonance with Neptune. For every 2 orbits that a plutino makes, Neptune orbits 3 times. is currently 27.0 AU from the Sun, and came to perihelion (q=26.98 AU) in April 2018. This means that this object is currently inside the orbit of the planet Neptune. Like P... | [
"(120216) 2004 EW95\n\n, provisionally known as, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in th... |
(120216)_2004_EW95_11388801 | Describe the 'Physical characteristics' section of the article about '(120216) 2004 EW95'. | energy would have been required. While this energy could have been delivered by a very large chance collision, the strong overall similarity between the modern C-type asteroids in the outer asteroid belt and suggests that these objects formed in the same region of the early Sun's protoplanetary disk, much closer to the... | [
"(120216) 2004 EW95\n\n, provisionally known as, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in th... |
(12538)_1998_OH_28176112 | Reconstruct the content about 'Rotation period' from the article on '(12538) 1998 OH'. | In 2014, several rotational lightcurves of were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcurve analysis gave a rotation period of 5.1... | [
"(12538) 1998 OH β Rotation period\n\nIn 2014, several rotational lightcurves of were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcu... |
(12538)_1998_OH_28176109 | Reconstruct the content about 'Orbit and classification' from the article on '(12538) 1998 OH'. | is a member of the Apollo group of asteroids, which are Earth-crossing asteroids. They are the largest group of near-Earth objects with approximately 10 thousand known members. It orbits the Sun at a distance of 0.9β2.2 AU in 1 year and 11 months (699 days). Its orbit has an eccentricity of 0.41 and an inclination of 2... | [
"(12538) 1998 OH β Rotation period\n\nIn 2014, several rotational lightcurves of were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcu... |
(12538)_1998_OH_28176107 | Summarize the following section from the article on '(12538) 1998 OH'. | (12538) 1998 OH is a stony asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 1.8 kilometers (1.1 miles) in diameter. It was discovered on 19 July 1998, by astronomers of the Near-Earth Asteroid Tracking program at the Haleakala Observatory in Hawaii, United ... | [
"(12538) 1998 OH β Rotation period\n\nIn 2014, several rotational lightcurves of were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcu... |
(12538)_1998_OH_28176108 | From the article on '(12538) 1998 OH', restate the 'Numbering and naming' content. | This minor planet was numbered by the Minor Planet Center on 23 November 1999. As of 2018, it has not been named. | [
"(12538) 1998 OH β Rotation period\n\nIn 2014, several rotational lightcurves of were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcu... |
(12538)_1998_OH_28176110 | What does the article about '(12538) 1998 OH' say regarding 'Close approaches'? | The asteroid has an Earth minimum orbital intersection distance of 0.0280 AU, which corresponds to 10.9 lunar distances and makes it a potentially hazardous asteroid due to its sufficiently large size. It will pass close to Earth in 2042 and 2132, at a distance of 0.0292 AU and 0.0317 AU, respectively. | [
"(12538) 1998 OH β Rotation period\n\nIn 2014, several rotational lightcurves of were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcu... |
(127546)_2002_XU93_9624455 | What information does the article about '(127546) 2002 XU93' provide on 'Orbit and classification'? | orbits the Sun at a distance of 21β114 AU once every 552 years and 1 month (201,654 days; semi-major axis of 67.3 AU). Its orbit has an eccentricity of 0.69 and an inclination of 78Β° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Kitt Peak in December 2002. Th... | [
"(127546) 2002 XU93 β Orbit and classification\n\norbits the Sun at a distance of 21β114 AU once every 552 years and 1 month (201,654 days; semi-major axis of 67.3 AU). Its orbit has an eccentricity of 0.69 and an inclination of 78Β° with respect to the ecliptic. The body's observation arc begins with its official d... |
(127546)_2002_XU93_9624458 | Summarize the 'Rotation period' part of '(127546) 2002 XU93'. | As of 2018, no rotational lightcurve of this object has been obtained from photometric observations. The object's rotation period, pole and shape remain unknown. | [
"(127546) 2002 XU93 β Orbit and classification\n\norbits the Sun at a distance of 21β114 AU once every 552 years and 1 month (201,654 days; semi-major axis of 67.3 AU). Its orbit has an eccentricity of 0.69 and an inclination of 78Β° with respect to the ecliptic. The body's observation arc begins with its official d... |
(127546)_2002_XU93_9624457 | Reconstruct the content about 'Diameter and albedo' from the article on '(127546) 2002 XU93'. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 170 kilometers in diameter and its surface has an low albedo of 0.04. The Johnston archive gives a mean-diameter of 164 km and albedo of 0.038 from various measurement, while astronomer Michael Brown gives... | [
"(127546) 2002 XU93 β Orbit and classification\n\norbits the Sun at a distance of 21β114 AU once every 552 years and 1 month (201,654 days; semi-major axis of 67.3 AU). Its orbit has an eccentricity of 0.69 and an inclination of 78Β° with respect to the ecliptic. The body's observation arc begins with its official d... |
(127546)_2002_XU93_9624454 | Reconstruct the content from the article about '(127546) 2002 XU93'. | , provisional designation, is a trans-Neptunian object and centaur on highly inclined and eccentric orbit in the outer region of the Solar System. It measures approximately 170 km in diameter and is one of few objects with such an unusual orbit. It was discovered on 4 December 2002, by American astronomer Marc Buie at ... | [
"(127546) 2002 XU93 β Orbit and classification\n\norbits the Sun at a distance of 21β114 AU once every 552 years and 1 month (201,654 days; semi-major axis of 67.3 AU). Its orbit has an eccentricity of 0.69 and an inclination of 78Β° with respect to the ecliptic. The body's observation arc begins with its official d... |
(127546)_2002_XU93_9624456 | Explain what '(127546) 2002 XU93' covers in the 'Physical characteristics' section. | has a BBβBR taxonomy type. It shows only a moderately red surface with a spectral gradient similar to the known comets, extinct comets, Jupiter trojans, Neptune trojans, irregular satellites and damocloids. With a BβR magnitude of 1.2, the difference between the blue and red filter magnitude, it is still redder than th... | [
"(127546) 2002 XU93 β Orbit and classification\n\norbits the Sun at a distance of 21β114 AU once every 552 years and 1 month (201,654 days; semi-major axis of 67.3 AU). Its orbit has an eccentricity of 0.69 and an inclination of 78Β° with respect to the ecliptic. The body's observation arc begins with its official d... |
(131697)_2001_XH255_22227933 | Reconstruct the content from the article about '(131697) 2001 XH255'. | , provisionally known as 2001 XH255, is a trans-Neptunian object (TNO) that has a 4:5 resonance with Neptune. It will come to perihelion in 2041. Assuming a generic TNO albedo of 0.09, it is about 100 km in diameter. | [
"(131697) 2001 XH255\n\n, provisionally known as 2001 XH255, is a trans-Neptunian object (TNO) that has a 4:5 resonance with Neptune. It will come to perihelion in 2041. Assuming a generic TNO albedo of 0.09, it is about 100 km in diameter.",
"(131697) 2001 XH255 β Resonance\n\nAccording to the Deep Ecliptic Surv... |
(131697)_2001_XH255_22227934 | What does the article about '(131697) 2001 XH255' say regarding 'Resonance'? | According to the Deep Ecliptic Survey and Minor Planet Center, has a 4:5 resonance with Neptune. It comes as close as 32.2 AU from the Sun and has a fairly low orbital eccentricity of 0.07 with an inclination of only 2.86 degrees. The Neptune 4:5 resonance keeps it more than 7 AU from Neptune over a 14000-year period. ... | [
"(131697) 2001 XH255\n\n, provisionally known as 2001 XH255, is a trans-Neptunian object (TNO) that has a 4:5 resonance with Neptune. It will come to perihelion in 2041. Assuming a generic TNO albedo of 0.09, it is about 100 km in diameter.",
"(131697) 2001 XH255 β Resonance\n\nAccording to the Deep Ecliptic Surv... |
(131697)_2001_XH255_22227935 | What information does the article about '(131697) 2001 XH255' provide on 'Potential for Exploration'? | A NASA study in 2019 that confirmed the viability of using small radioisotope or nuclear fission power systems combined with xenon electric propulsion for deep space exploration, used 2001 XH255 as a representative Kuiper Belt Object as the mission's destination to orbit. | [
"(131697) 2001 XH255\n\n, provisionally known as 2001 XH255, is a trans-Neptunian object (TNO) that has a 4:5 resonance with Neptune. It will come to perihelion in 2041. Assuming a generic TNO albedo of 0.09, it is about 100 km in diameter.",
"(131697) 2001 XH255 β Resonance\n\nAccording to the Deep Ecliptic Surv... |
(13366)_1998_US24_15688167 | Based on the article about '(13366) 1998 US24', describe the 'Diameter and albedo' section. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 33.30 kilometers in diameter and its surface has an albedo of 0.058, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diamet... | [
"(13366) 1998 US24 β Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 33.30 kilometers in diameter and its surface has an albedo of 0.058, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbon... |
(13366)_1998_US24_15688164 | From the article on '(13366) 1998 US24', restate the 'Numbering and naming' content. | This minor planet was numbered by the MPC on 24 January 2000 (M.P.C. 37586). As of 2018, it has not been named. | [
"(13366) 1998 US24 β Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 33.30 kilometers in diameter and its surface has an albedo of 0.058, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbon... |
(13366)_1998_US24_15688163 | Explain what '(13366) 1998 US24' covers in the 'Orbit and classification' section. | is a dark Jovian asteroid in a 1:1 orbital resonance with Jupiter. It is located in the leading Greek camp at the Gas Giant's Lagrangian point, 60Β° ahead of its orbit. It is also a non-family asteroid in the Jovian background population. It orbits the Sun at a distance of 4.7β5.8 AU once every 11 years and 12 months (4... | [
"(13366) 1998 US24 β Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 33.30 kilometers in diameter and its surface has an albedo of 0.058, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbon... |
(13366)_1998_US24_15688162 | Describe the content of the article about '(13366) 1998 US24'. | ''', provisional designation ', is a Jupiter trojan from the Greek camp, approximately 33 km in diameter. It was discovered on 18 October 1998, by astronomers with the Lowell Observatory Near-Earth-Object Search at the Anderson Mesa Station near Flagstaff, Arizona, in the United States. The dark Jovian asteroid is a sl... | [
"(13366) 1998 US24 β Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 33.30 kilometers in diameter and its surface has an albedo of 0.058, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbon... |
(136617)_1994_CC_13763669 | Summarize the 'Observations' part of '(136617) 1994 CC'. | diameter that has two moons revolving around it. Scientists' preliminary analysis of the system suggests that the moons are at least 50 meters in diameter. In a similar study, the radar observations at Arecibo Observatory in Puerto Rico, led by the Mike Nolan, also confirmed the detection of all three objects. The scie... | [
"(136617) 1994 CC β Observations\n\ndiameter that has two moons revolving around it. Scientists' preliminary analysis of the system suggests that the moons are at least 50 meters in diameter. In a similar study, the radar observations at Arecibo Observatory in Puerto Rico, led by the Mike Nolan, also confirmed the ... |
(136617)_1994_CC_13763671 | What does the article about '(136617) 1994 CC' say regarding 'Numbering and naming'? | This minor planet was numbered by the Minor Planet Center on 5 December 2006. , it has not been named. | [
"(136617) 1994 CC β Observations\n\ndiameter that has two moons revolving around it. Scientists' preliminary analysis of the system suggests that the moons are at least 50 meters in diameter. In a similar study, the radar observations at Arecibo Observatory in Puerto Rico, led by the Mike Nolan, also confirmed the ... |
(136617)_1994_CC_13763668 | Reconstruct the content about 'Observations' from the article on '(136617) 1994 CC'. | A team of NASA's Jet Propulsion Laboratory (JPL) (Pasadena, California) scientists led by Marina Brozovic and Lance Benner, made the discovery using radar imaging at NASA's Goldstone Solar System Radar on June 12 and June 14, 2009. They showed that the near-Earth asteroid is a triple system, which encountered Earth wit... | [
"(136617) 1994 CC β Observations\n\ndiameter that has two moons revolving around it. Scientists' preliminary analysis of the system suggests that the moons are at least 50 meters in diameter. In a similar study, the radar observations at Arecibo Observatory in Puerto Rico, led by the Mike Nolan, also confirmed the ... |
(136617)_1994_CC_13763667 | Based on the article about '(136617) 1994 CC', describe the 'Discovery' section. | was discovered by Spacewatch's Jim Scotti at Kitt Peak National Observatory on 3 February 1994. 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. Th... | [
"(136617) 1994 CC β Observations\n\ndiameter that has two moons revolving around it. Scientists' preliminary analysis of the system suggests that the moons are at least 50 meters in diameter. In a similar study, the radar observations at Arecibo Observatory in Puerto Rico, led by the Mike Nolan, also confirmed the ... |
(143649)_2003_QQ47_19546688 | Describe the 'Preliminary reports' section of the article about '(143649) 2003 QQ47'. | of TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; "The odds are very, very low ... We have to keep some kind of perspective", she said. As a result of the press covera... | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143649)_2003_QQ47_19546685 | Summarize the 'Description' part of '(143649) 2003 QQ47'. | was discovered on 24 August 2003. It was added to the Sentry Risk Table on 30 August 2003. By 31 August 2003 (with an observation arc of 7 days) the odds of an impact on 21 March 2014 were already reduced to 1 in 1.7 million. The asteroid was removed from the Sentry Risk Table on 14 September 2003, indicating there is ... | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143649)_2003_QQ47_19546687 | What information does the article about '(143649) 2003 QQ47' provide on 'Preliminary reports'? | by astronomers, but these events do not warrant public concern. In fact, each year several newly discovered asteroids reach Torino Scale 1 for a brief period after discovery; is the fourth such case this year. On September 2, 2003, new measurements of 's position allowed us to narrow our prediction of its path in 2014,... | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143649)_2003_QQ47_19546686 | What information does the article about '(143649) 2003 QQ47' provide on 'Preliminary reports'? | On 3 September 2003 a NASA press release wrote, "Newly discovered asteroid has received considerable media attention over the last few days because it had a small chance of colliding with the Earth in the year 2014 and was rated a "1" on the Torino Impact Hazard Scale, which goes from 0 to 10. The odds of collision in ... | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143649)_2003_QQ47_19546684 | Describe the content of the article about '(143649) 2003 QQ47'. | , provisionally designated:, is a kilometer-sized asteroid and synchronous binary system, classified as near-Earth object and potentially hazardous asteroid of the Apollo group. It became briefly notable upon its discovery in late August 2003, when media outlets played up a very preliminary report that it had a 1 in 25... | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143649)_2003_QQ47_19546689 | What information does the article about '(143649) 2003 QQ47' provide on 'Binary system'? | A minor-planet moon, provisionally designated, was first detected on 29 August 2021, by Petr Pravec, Peter KuΕ‘nirΓ‘k, Kamil Hornoch, and others using photometric data from ESO's La Silla Observatory in Chile. The discovery was announced on 17 September 2021. The secondary measures a third the size of its primary (Ds/Dp-... | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143649)_2003_QQ47_19546690 | Describe the 'In fiction' section of the article about '(143649) 2003 QQ47'. | The asteroid was mentioned in Anonymous Rex (Les Reptilians) (2004) as the asteroid which the dinosaurs were counting on to destroy human civilization. ; The Korean drama My Love from the Star also mentions it as the asteroid that will allow Do Min-joon to travel back to his home planet. | [
"(143649) 2003 QQ47 β Preliminary reports\n\nof TNT (1.5 ZJ), enough to cause global damage. Sara Russell, a meteorite researcher at London's Natural History Museum, told the BBC on 2 September 2003 that she was not worried that would be a danger; \"The odds are very, very low ... We have to keep some kind of persp... |
(143651)_2003_QO104_26066005 | Summarize the following section from the article on '(143651) 2003 QO104'. | , provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Amor and Apollo group, respectively. It was discovered on 31 August 2003, by astronomers of the Near-Earth Asteroid Tracking program a... | [
"(143651) 2003 QO104 β Physical characteristics\n\nhas been characterized as an uncommon Q-type asteroid, that falls into the larger stony S-complex.",
"(143651) 2003 QO104\n\n, provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth o... |
(143651)_2003_QO104_26066006 | What information does the article about '(143651) 2003 QO104' provide on 'Orbit and classification'? | is a member of the Apollo group of asteroids, which are Earth-crossing asteroids. They are the largest group of near-Earth objects with approximately 10 thousand known members. As it just grazes the orbit of Earth, the Minor Planet Center (MPC), groups it to the non-Earth crossing Amor asteroids. It orbits the Sun at a... | [
"(143651) 2003 QO104 β Physical characteristics\n\nhas been characterized as an uncommon Q-type asteroid, that falls into the larger stony S-complex.",
"(143651) 2003 QO104\n\n, provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth o... |
(143651)_2003_QO104_26066011 | Reconstruct the content about 'Naming' from the article on '(143651) 2003 QO104'. | This minor planet was numbered by the MPC on 5 December 2006 (M.P.C. 58189). As of 2018, it has not been named. | [
"(143651) 2003 QO104 β Physical characteristics\n\nhas been characterized as an uncommon Q-type asteroid, that falls into the larger stony S-complex.",
"(143651) 2003 QO104\n\n, provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth o... |
(143651)_2003_QO104_26066007 | Explain what '(143651) 2003 QO104' covers in the 'Close approaches' section. | The asteroid has an Earth minimum orbital intersection distance of 0.0042 AU, which corresponds to 1.6 lunar distances and makes it a potentially hazardous asteroid due to its sufficiently large size. On the Torino Scale, this object was rated level 1 in early October 2003, and removed on 13 October 2003. On 18 May 198... | [
"(143651) 2003 QO104 β Physical characteristics\n\nhas been characterized as an uncommon Q-type asteroid, that falls into the larger stony S-complex.",
"(143651) 2003 QO104\n\n, provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth o... |
(143651)_2003_QO104_26066010 | From the article on '(143651) 2003 QO104', restate the 'Diameter and albedo' content. | According to post-cryogenic observations made by the Spitzer Telescope during the ExploreNEOs survey, this asteroid measures 2.29 and 2.31 kilometers in diameter and its surface has an albedo between 0.13 and 0.14, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 a... | [
"(143651) 2003 QO104 β Physical characteristics\n\nhas been characterized as an uncommon Q-type asteroid, that falls into the larger stony S-complex.",
"(143651) 2003 QO104\n\n, provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth o... |
(143651)_2003_QO104_26066009 | Based on the article about '(143651) 2003 QO104', describe the 'Slow rotator and tumbler' section. | Several rotational lightcurve of this asteroid were obtained from photometric observations during its close approach to the Earth in 2009. Analysis of the best-rated lightcurve β obtained by Brian Warner at his Palmer Divide Observatory in collaboration with Robert Stephens and Albino Carbognani β gave a well-defined r... | [
"(143651) 2003 QO104 β Physical characteristics\n\nhas been characterized as an uncommon Q-type asteroid, that falls into the larger stony S-complex.",
"(143651) 2003 QO104\n\n, provisional designation, is a stony asteroid, slow rotator and suspected tumbler on a highly eccentric orbit, classified as near-Earth o... |
(144897)_2004_UX10_9368929 | What does the article about '(144897) 2004 UX10' say regarding 'Orbit and rotation'? | Based on an integration of its motion over 10 million years, has been classified as a classical Kuiper belt object (cubewano). It is near a 2:3 resonance with Neptune. The object is currently at 39 AU from the Sun. The rotational period of is 5.68 h. | [
"(144897) 2004 UX10 β Orbit and rotation\n\nBased on an integration of its motion over 10 million years, has been classified as a classical Kuiper belt object (cubewano). It is near a 2:3 resonance with Neptune. The object is currently at 39 AU from the Sun. The rotational period of is 5.68 h.",
"(144897) 2004 UX... |
(144897)_2004_UX10_9368930 | Describe the 'Physical properties' section of the article about '(144897) 2004 UX10'. | The size of was measured by the Herschel Space Telescope to be 361 km. The mass of the object is currently unknown but should be greater than about 3 kg. has a moderately red slope in the visible spectral range. Its visible spectrum does not show any features, although there is a small departure from the linearity near... | [
"(144897) 2004 UX10 β Orbit and rotation\n\nBased on an integration of its motion over 10 million years, has been classified as a classical Kuiper belt object (cubewano). It is near a 2:3 resonance with Neptune. The object is currently at 39 AU from the Sun. The rotational period of is 5.68 h.",
"(144897) 2004 UX... |
(144897)_2004_UX10_9368928 | What information does the article about '(144897) 2004 UX10' provide? | is a Kuiper-belt object. It has a diameter of about 360 km and was discovered by Andrew Becker, Andrew Puckett and Jeremy Kubica on 20 October 2004 at Apache Point Observatory in Sunspot, New Mexico. The object is classified as a cubewano. It is near a 2:3 resonance with Neptune. Brown estimates it is likely a dwarf pl... | [
"(144897) 2004 UX10 β Orbit and rotation\n\nBased on an integration of its motion over 10 million years, has been classified as a classical Kuiper belt object (cubewano). It is near a 2:3 resonance with Neptune. The object is currently at 39 AU from the Sun. The rotational period of is 5.68 h.",
"(144897) 2004 UX... |
(144898)_2004_VD17_3107801 | From the article on '(144898) 2004 VD17', restate the '2008 observations' content. | As of 4 January 2008, the Sentry Risk Table assigned a Torino value of 0 and an impact probability of 1 in 58.8 million for 4 May 2102. This value was far below the background impact rate of objects this size. Further observations allowed it to be removed from the Sentry Risk Table on 14 February 2008. It will pass 0.0... | [
"(144898) 2004 VD17 β 2008 observations\n\nAs of 4 January 2008, the Sentry Risk Table assigned a Torino value of 0 and an impact probability of 1 in 58.8 million for 4 May 2102. This value was far below the background impact rate of objects this size. Further observations allowed it to be removed from the Sentry R... |
(144898)_2004_VD17_3107798 | What information does the article about '(144898) 2004 VD17' provide? | (144898) , provisional designation, is a sub-kilometer asteroid, classified as near-Earth object of the Apollo group once thought to have a low probability of impacting Earth on 4 May 2102. With an observation arc of 17 years it is known that closest Earth approach will occur two days earlier on 2 May 2102 at a distanc... | [
"(144898) 2004 VD17 β 2008 observations\n\nAs of 4 January 2008, the Sentry Risk Table assigned a Torino value of 0 and an impact probability of 1 in 58.8 million for 4 May 2102. This value was far below the background impact rate of objects this size. Further observations allowed it to be removed from the Sentry R... |
(144898)_2004_VD17_3107799 | From the article on '(144898) 2004 VD17', restate the 'History' content. | was discovered on 7 November 2004, by the NASA-funded LINEAR asteroid survey. The object is estimated by NASA's Near Earth Object Program Office to be 580 meters in diameter with an approximate mass of 260,000,000,000 kg. Being approximately 580 meters in diameter, if were to impact land, it would create an impact crat... | [
"(144898) 2004 VD17 β 2008 observations\n\nAs of 4 January 2008, the Sentry Risk Table assigned a Torino value of 0 and an impact probability of 1 in 58.8 million for 4 May 2102. This value was far below the background impact rate of objects this size. Further observations allowed it to be removed from the Sentry R... |
(144898)_2004_VD17_3107802 | Explain what '(144898) 2004 VD17' covers in the 'Properties' section. | It has a spectral type of E. This suggests that the asteroid has a high albedo and is on the smaller size range for an object with an absolute magnitude of 18.8. | [
"(144898) 2004 VD17 β 2008 observations\n\nAs of 4 January 2008, the Sentry Risk Table assigned a Torino value of 0 and an impact probability of 1 in 58.8 million for 4 May 2102. This value was far below the background impact rate of objects this size. Further observations allowed it to be removed from the Sentry R... |
(144898)_2004_VD17_3107800 | Explain what '(144898) 2004 VD17' covers in the 'Elevated risk estimate in 2006' section. | From February to May 2006, was listed with a Torino Scale impact risk value of 2, only the second asteroid in risk-monitoring history to be rated above value 1. With an observation arc of 1511 days, it was estimated to have a 1 in 1320 chance of impacting on 4 May 2102. The Torino rating was lowered to 1 after addition... | [
"(144898) 2004 VD17 β 2008 observations\n\nAs of 4 January 2008, the Sentry Risk Table assigned a Torino value of 0 and an impact probability of 1 in 58.8 million for 4 May 2102. This value was far below the background impact rate of objects this size. Further observations allowed it to be removed from the Sentry R... |
(148975)_2001_XA255_30505857 | Reconstruct the content about 'Orbit and classification' from the article on '(148975) 2001 XA255'. | follows a very eccentric orbit (0.68) with perihelion just inside the orbit of Saturn, aphelion in the trans-Neptunian belt and a semi-major axis of 28.9 AU. The orbital inclination of this object is moderate at 12.6ΒΊ. | [
"(148975) 2001 XA255 β Orbit and classification\n\nfollows a very eccentric orbit (0.68) with perihelion just inside the orbit of Saturn, aphelion in the trans-Neptunian belt and a semi-major axis of 28.9 AU. The orbital inclination of this object is moderate at 12.6ΒΊ.",
"(148975) 2001 XA255 β Physical characteri... |
(148975)_2001_XA255_30505859 | What does the article about '(148975) 2001 XA255' say regarding 'Physical characteristics'? | The object has an estimated diameter of 12.5 km and it was classified as an inactive centaur by David Jewitt. Observations by the NEOWISE mission gave a larger diameter of 37.7 kilometers and an albedo of 0.041. It has an absolute magnitude is 11.1. | [
"(148975) 2001 XA255 β Orbit and classification\n\nfollows a very eccentric orbit (0.68) with perihelion just inside the orbit of Saturn, aphelion in the trans-Neptunian belt and a semi-major axis of 28.9 AU. The orbital inclination of this object is moderate at 12.6ΒΊ.",
"(148975) 2001 XA255 β Physical characteri... |
(148975)_2001_XA255_30505858 | Reconstruct the content about 'Resonance with Neptune' from the article on '(148975) 2001 XA255'. | was identified as trapped in a 1:1 mean-motion resonance with Neptune and 1:2 with Uranus by T. Gallardo in 2006. The object is dynamically unstable and it entered the region of the giant planets relatively recently, perhaps 50,000 years ago, from the scattered disk. It follows a short-lived horseshoe orbit around Nept... | [
"(148975) 2001 XA255 β Orbit and classification\n\nfollows a very eccentric orbit (0.68) with perihelion just inside the orbit of Saturn, aphelion in the trans-Neptunian belt and a semi-major axis of 28.9 AU. The orbital inclination of this object is moderate at 12.6ΒΊ.",
"(148975) 2001 XA255 β Physical characteri... |
(153201)_2000_WO107_25126699 | Describe the content of the article about '(153201) 2000 WO107'. | is a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experimental Test Site near Socorro,... | [
"(153201) 2000 WO107\n\nis a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experime... |
(153201)_2000_WO107_25126704 | Summarize the 'Numbering and naming' part of '(153201) 2000 WO107'. | This minor planet was numbered by the Minor Planet Center on 2 April 2007. As of 2018, it has not been named. | [
"(153201) 2000 WO107\n\nis a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experime... |
(153201)_2000_WO107_25126702 | What information does the article about '(153201) 2000 WO107' provide on '2140'? | This asteroid will pass 0.00162 AU from Earth on 1 December 2140. The 2140 close approach distance is known with an accuracy of roughly Β±1000 km. For comparison, the distance to the Moon is about 0.0026 AU (384,400 km). The Jupiter Tisserand invariant, used to distinguish different kinds of orbits, is 6.228. | [
"(153201) 2000 WO107\n\nis a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experime... |
(153201)_2000_WO107_25126703 | What information does the article about '(153201) 2000 WO107' provide on 'Physical characteristics'? | In the SMASS classification, the object's spectral type is that of an X-type. According to the space-based survey by NASA's NEOWISE mission, the asteroid measures 510 meters in diameter and its surface has an albedo of 0.129. | [
"(153201) 2000 WO107\n\nis a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experime... |
(153201)_2000_WO107_25126701 | What information does the article about '(153201) 2000 WO107' provide on '2020'? | The asteroid came to perihelion on 13 October 2020 when it passed the Sun going 88 km/s. The asteroid was not more than 60 degrees from the Sun until 26 November 2020 and was observed by Goldstone radar on 27 November 2020. On 29 November 2020 the asteroid passed 0.02876 AU from Earth. Even the 2018 orbit solution had ... | [
"(153201) 2000 WO107\n\nis a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experime... |
(153201)_2000_WO107_25126700 | What information does the article about '(153201) 2000 WO107' provide on 'Orbit'? | The orbit of this potentially hazardous asteroid (PHA) has been well-established with 20 years of observations. It orbits from inside the orbit of Mercury out to the orbit of Mars. It makes close approaches to all of the inner planets. | [
"(153201) 2000 WO107\n\nis a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experime... |
(153591)_2001_SN263_12534764 | Based on the article about '(153591) 2001 SN263', describe the 'Primary' section. | , the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of 7Β° with respect to the ecliptic. A fir... | [
"(153591) 2001 SN263 β Primary\n\n, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of ... |
(153591)_2001_SN263_12534763 | Describe the 'Numbering and naming' section of the article about '(153591) 2001 SN263'. | This minor planet was numbered by the Minor Planet Center on 2 April 2007. As of 2018, the primary and its moons have not been named. In the scientific literature, the components of the trinary system are generically referred to as Alpha, Beta and Gamma, but these labels are not recognized by the IAU. | [
"(153591) 2001 SN263 β Primary\n\n, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of ... |
(153591)_2001_SN263_12534765 | Describe the 'Primary' section of the article about '(153591) 2001 SN263'. | 20.3 lunar distances. With an Earth MOID above 0.05 AU, is no longer a potentially hazardous asteroid, but it was classified as such by the MPC until early 2017. Radar observations show that it measures 2.5 kilometers in diameter. Its surface has a low albedo of 0.048. Rotational lightcurves obtained from photometric o... | [
"(153591) 2001 SN263 β Primary\n\n, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of ... |
(153591)_2001_SN263_12534767 | From the article on '(153591) 2001 SN263', restate the 'Orbital characteristics of satellites' content. | The orbital properties of the satellites are listed in this table. The orbital planes of both satellites are inclined relative to each other; the relative inclination is about 14 degrees. Such a large inclination is suggestive of past evolutionary events (e.g. close encounter with a terrestrial planet, mean-motion-reso... | [
"(153591) 2001 SN263 β Primary\n\n, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of ... |
(153591)_2001_SN263_12534762 | What information does the article about '(153591) 2001 SN263' provide? | is a carbonaceous trinary asteroid, classified as near-Earth object and former potentially hazardous asteroid of the Amor group, approximately 2.6 km in diameter. It was discovered by the Lincoln Near-Earth Asteroid Research project at Lincoln Lab's Experimental Test Site in Socorro, New Mexico, on 20 September 2001. T... | [
"(153591) 2001 SN263 β Primary\n\n, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of ... |
(153591)_2001_SN263_12534766 | Summarize the 'Trinary system' part of '(153591) 2001 SN263'. | In 2008, scientists using the planetary radar at Arecibo Observatory discovered that the object is orbited by two satellites, when the triple asteroid made a close approach to Earth of 0.066 AU (nearly 10 million kilometers). The largest body (preliminarily called Alpha) is spheroid in shape, with principal axes of 2.8... | [
"(153591) 2001 SN263 β Primary\n\n, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type. It orbits the Sun at a distance of 1.0β2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of ... |
(154276)_2002_SY50_26180815 | Describe the 'Physical characteristics' section of the article about '(154276) 2002 SY50'. | Photometry by the Sloan Digital Sky Survey has characterized as an uncommon K-type asteroid, which is typically seen among members of the Eos family in the asteroid belt. | [
"(154276) 2002 SY50 β Physical characteristics\n\nPhotometry by the Sloan Digital Sky Survey has characterized as an uncommon K-type asteroid, which is typically seen among members of the Eos family in the asteroid belt.",
"(154276) 2002 SY50\n\n, provisional designation, is a stony asteroid on a highly eccentric... |
(154276)_2002_SY50_26180812 | What information does the article about '(154276) 2002 SY50' provide? | , provisional designation, is a stony asteroid on a highly eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 1.1 km in diameter. It was discovered on 30 September 2002, by astronomers with the Lincoln Near-Earth Asteroid Research at the Lincoln Labora... | [
"(154276) 2002 SY50 β Physical characteristics\n\nPhotometry by the Sloan Digital Sky Survey has characterized as an uncommon K-type asteroid, which is typically seen among members of the Eos family in the asteroid belt.",
"(154276) 2002 SY50\n\n, provisional designation, is a stony asteroid on a highly eccentric... |
(154276)_2002_SY50_26180817 | Reconstruct the content about 'Diameter and albedo' from the article on '(154276) 2002 SY50'. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, this asteroid measures 1.06 kilometers in diameter and its surface has an albedo of 0.14, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diam... | [
"(154276) 2002 SY50 β Physical characteristics\n\nPhotometry by the Sloan Digital Sky Survey has characterized as an uncommon K-type asteroid, which is typically seen among members of the Eos family in the asteroid belt.",
"(154276) 2002 SY50\n\n, provisional designation, is a stony asteroid on a highly eccentric... |
(154276)_2002_SY50_26180813 | Reconstruct the content about 'Orbit and classification' from the article on '(154276) 2002 SY50'. | is a member of the Earth-crossing group of Apollo asteroids, the largest group of near-Earth objects with approximately 10 thousand known members. It orbits the Sun at a distance of 0.53β2.88 AU once every 2 years and 3 months (813 days; semi-major axis of 1.7 AU). Its orbit has an eccentricity of 0.69 and an inclinati... | [
"(154276) 2002 SY50 β Physical characteristics\n\nPhotometry by the Sloan Digital Sky Survey has characterized as an uncommon K-type asteroid, which is typically seen among members of the Eos family in the asteroid belt.",
"(154276) 2002 SY50\n\n, provisional designation, is a stony asteroid on a highly eccentric... |
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