id string | question string | answer string | documents list |
|---|---|---|---|
(4953)_1990_MU_31850785 | What information does the article about '(4953) 1990 MU' provide? | (4953) 1990 MU (prov. designation: ) is a large Earth-crossing asteroid (ECA) belonging to the Apollo group of near-Earth objects which also cross the orbits of Mars and Venus. At approximately 3 km in diameter, it is one of the largest known ECAs. It has been assigned a permanent number from the Minor Planet Center (4... | [
"(4953) 1990 MU — Description\n\nit approached to 0.1418 AU. The Earth MOID of has been decreasing (becoming more hazardous) during the 20th century, while the Venus MOID (0.0455) has been increasing. Besides its original discovery at Siding Spring Observatory in Australia, has also been studied by radar at Goldsto... |
(4953)_1990_MU_31850789 | What does the article about '(4953) 1990 MU' say regarding 'Description'? | figure, they state that the albedo of an NEO is not likely to be much over 0.5 and their measurement uncertainty is "around a factor of 2". The Gaia mission of the European Space Agency, launched in December 2013, has been tasked with measuring the Yarkovsky effect on near-Earth asteroids (NEAs). The Yarkovsky effect i... | [
"(4953) 1990 MU — Description\n\nit approached to 0.1418 AU. The Earth MOID of has been decreasing (becoming more hazardous) during the 20th century, while the Venus MOID (0.0455) has been increasing. Besides its original discovery at Siding Spring Observatory in Australia, has also been studied by radar at Goldsto... |
(4953)_1990_MU_31850787 | Reconstruct the content about 'Description' from the article on '(4953) 1990 MU'. | an Earth minimum orbit intersection distance (MOID) of 0.0263 AU, which is close enough to classify it as a Potentially Hazardous Asteroid (PHA). It will make a close approach to Earth on 6 June 2027 at 0.0308 AU, becoming as bright as apparent magnitude 9.7 on 8 June 2027, and even closer on 5 June 2058 at 0.0231 AU. ... | [
"(4953) 1990 MU — Description\n\nit approached to 0.1418 AU. The Earth MOID of has been decreasing (becoming more hazardous) during the 20th century, while the Venus MOID (0.0455) has been increasing. Besides its original discovery at Siding Spring Observatory in Australia, has also been studied by radar at Goldsto... |
(495603)_2015_AM281_30207985 | Summarize the 'Discovery' part of '(495603) 2015 AM281'. | The body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in April 2000, nearly 10 years prior to its official discovery observation at Haleakala Observatory. The discovery was announced in a Minor Planet Electronic Circular in July 2016, after additional observations by Pan-STARRS had be... | [
"(495603) 2015 AM281 — Discovery\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in April 2000, nearly 10 years prior to its official discovery observation at Haleakala Observatory. The discovery was announced in a Minor Planet Electronic Circular in July 2016, after addi... |
(495603)_2015_AM281_30207987 | What information does the article about '(495603) 2015 AM281' provide on 'Numbering and naming'? | This minor planet was numbered by the Minor Planet Center on 9 June 2017 and received the number in the minor planet catalog (M.P.C. 105261). As of 2018, it has not been named. | [
"(495603) 2015 AM281 — Discovery\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in April 2000, nearly 10 years prior to its official discovery observation at Haleakala Observatory. The discovery was announced in a Minor Planet Electronic Circular in July 2016, after addi... |
(495603)_2015_AM281_30207988 | Reconstruct the content about 'Physical characteristics' from the article on '(495603) 2015 AM281'. | According to the Johnston's archive and American astronomer Michael Brown, measures 468 and 479 kilometers in diameter based on an assumed albedo of 0.09 and 0.07, respectively. As of 2018, no rotational lightcurve has been obtained from photometric observations. The body's rotation period, pole and shape remain unknow... | [
"(495603) 2015 AM281 — Discovery\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in April 2000, nearly 10 years prior to its official discovery observation at Haleakala Observatory. The discovery was announced in a Minor Planet Electronic Circular in July 2016, after addi... |
(501546)_2014_JJ80_29731947 | What does the article about '(501546) 2014 JJ80' say regarding 'Numbering and naming'? | This minor planet was numbered by the Minor Planet Center on 5 October 2017 and received the number in the minor planet catalog (M.P.C. 106396). As of 2021, it has not been named. | [
"(501546) 2014 JJ80 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 5 October 2017 and received the number in the minor planet catalog (M.P.C. 106396). As of 2021, it has not been named.",
"(501546) 2014 JJ80 — Physical characteristics\n\nAccording to American astronomer Mic... |
(501546)_2014_JJ80_29731948 | What does the article about '(501546) 2014 JJ80' say regarding 'Physical characteristics'? | According to American astronomer Michael Brown and the Johnston's archive, measures 344 and 352 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-cl... | [
"(501546) 2014 JJ80 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 5 October 2017 and received the number in the minor planet catalog (M.P.C. 106396). As of 2021, it has not been named.",
"(501546) 2014 JJ80 — Physical characteristics\n\nAccording to American astronomer Mic... |
(501546)_2014_JJ80_29731945 | Describe the content of the article about '(501546) 2014 JJ80'. | , prov. designation:, is a trans-Neptunian object from the outermost region of the Solar System. It was discovered on 9 July 2013, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. It is a dwarf planet candidate, as it measures approximately 350 km in diameter. | [
"(501546) 2014 JJ80 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 5 October 2017 and received the number in the minor planet catalog (M.P.C. 106396). As of 2021, it has not been named.",
"(501546) 2014 JJ80 — Physical characteristics\n\nAccording to American astronomer Mic... |
(501546)_2014_JJ80_29731946 | Describe the 'Orbit and classification' section of the article about '(501546) 2014 JJ80'. | orbits the Sun at a distance of 31.3–55.1 AU once every 283 years and 9 months (103,645 days; semi-major axis of 43.18 AU). Its orbit has an eccentricity of 0.28 and an inclination of 19° with respect to the ecliptic. The body's observation arc begins at Haleakalā with a precovery taken in August 2010, nearly 3 years p... | [
"(501546) 2014 JJ80 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 5 October 2017 and received the number in the minor planet catalog (M.P.C. 106396). As of 2021, it has not been named.",
"(501546) 2014 JJ80 — Physical characteristics\n\nAccording to American astronomer Mic... |
(501581)_2014_OB394_29558037 | Based on the article about '(501581) 2014 OB394', describe the 'Physical characteristics' section. | According to American astronomer Michael Brown and the Johnston's archive, measures 255 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-cl... | [
"(501581) 2014 OB394 — Physical characteristics\n\nAccording to American astronomer Michael Brown and the Johnston's archive, measures 255 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a \"possible\" dwarf planet (200–400 km), wh... |
(501581)_2014_OB394_29558036 | What information does the article about '(501581) 2014 OB394' provide on 'Numbering and naming'? | This minor planet was numbered by the Minor Planet Center on 5 October 2017 and received the number in the minor planet catalog (M.P.C. 106397). As of 2018, it has not been named. | [
"(501581) 2014 OB394 — Physical characteristics\n\nAccording to American astronomer Michael Brown and the Johnston's archive, measures 255 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a \"possible\" dwarf planet (200–400 km), wh... |
(501581)_2014_OB394_29558034 | Describe the content of the article about '(501581) 2014 OB394'. | , provisional designation, is a trans-Neptunian object from the outermost region of the Solar System, approximately 260 km in diameter. It was discovered on 25 August 2012, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The weak dwarf planet candidate was numbered in 2017 and... | [
"(501581) 2014 OB394 — Physical characteristics\n\nAccording to American astronomer Michael Brown and the Johnston's archive, measures 255 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a \"possible\" dwarf planet (200–400 km), wh... |
(501581)_2014_OB394_29558035 | Reconstruct the content about 'Orbit and classification' from the article on '(501581) 2014 OB394'. | orbits the Sun at a distance of 35.0–58.2 AU once every 318 years and 5 months (116,302 days; semi-major axis of 46.63 AU). Its orbit has an eccentricity of 0.25 and an inclination of 21° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Haleakala Observatory in ... | [
"(501581) 2014 OB394 — Physical characteristics\n\nAccording to American astronomer Michael Brown and the Johnston's archive, measures 255 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a \"possible\" dwarf planet (200–400 km), wh... |
(505448)_2013_SA100_30035990 | From the article on '(505448) 2013 SA100', restate the 'Numbering and naming' content. | This minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number in the minor planet catalog (M.P.C. 107067). As of 2018, it has not been named. | [
"(505448) 2013 SA100 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number in the minor planet catalog (M.P.C. 107067). As of 2018, it has not been named.",
"(505448) 2013 SA100 — Orbit and classification\n\nIt orbits the Sun at a distance o... |
(505448)_2013_SA100_30035989 | Summarize the 'Orbit and classification' part of '(505448) 2013 SA100'. | It orbits the Sun at a distance of 38.6–53.8 AU once every 314 years and 1 month (114,732 days; semi-major axis of 46.21 AU). Its orbit has an eccentricity of 0.16 and an inclination of 8° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Mauna Kea Observatories ... | [
"(505448) 2013 SA100 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number in the minor planet catalog (M.P.C. 107067). As of 2018, it has not been named.",
"(505448) 2013 SA100 — Orbit and classification\n\nIt orbits the Sun at a distance o... |
(505448)_2013_SA100_30035988 | Summarize the following section from the article on '(505448) 2013 SA100'. | , provisional designation and also known as o3l79, is a trans-Neptunian object from the classical Kuiper belt in the outermost region of the Solar System. It was discovered on 5 August 2013, by astronomer with the Outer Solar System Origins Survey at the Mauna Kea Observatories, Hawaii, in the United States. The classi... | [
"(505448) 2013 SA100 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number in the minor planet catalog (M.P.C. 107067). As of 2018, it has not been named.",
"(505448) 2013 SA100 — Orbit and classification\n\nIt orbits the Sun at a distance o... |
(505448)_2013_SA100_30035991 | Based on the article about '(505448) 2013 SA100', describe the 'Physical characteristics' section. | According to the American astronomer Michael Brown, measures 255 kilometers in diameter based on an assumed albedo of 0.08. On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system. Similarly, Johnston's archive es... | [
"(505448) 2013 SA100 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number in the minor planet catalog (M.P.C. 107067). As of 2018, it has not been named.",
"(505448) 2013 SA100 — Orbit and classification\n\nIt orbits the Sun at a distance o... |
(505478)_2013_UT15_17507104 | Summarize the following section from the article on '(505478) 2013 UT15'. | is an extreme trans-Neptunian object from the scattered disc, located in the outermost regions of the Solar System, approximately 260 km in diameter. It was discovered on 2 August 2013, by astronomers of the Outer Solar System Origins Survey at Mauna Kea Observatory, Hawaii, United States. | [
"(505478) 2013 UT15\n\nis an extreme trans-Neptunian object from the scattered disc, located in the outermost regions of the Solar System, approximately 260 km in diameter. It was discovered on 2 August 2013, by astronomers of the Outer Solar System Origins Survey at Mauna Kea Observatory, Hawaii, United States.",
... |
(505478)_2013_UT15_17507107 | Summarize the 'Diameter' part of '(505478) 2013 UT15'. | has been estimated to measure 243 and 340 kilometers in diameter, based on an assumed albedo of 0.09 and 0.04, respectively. A generic magnitude-to-diameter conversion gives a mean-diameter of 260 kilometers, using with a typical albedo of 0.08 and a published absolute magnitude of 6.2951. | [
"(505478) 2013 UT15\n\nis an extreme trans-Neptunian object from the scattered disc, located in the outermost regions of the Solar System, approximately 260 km in diameter. It was discovered on 2 August 2013, by astronomers of the Outer Solar System Origins Survey at Mauna Kea Observatory, Hawaii, United States.",
... |
(505478)_2013_UT15_17507108 | From the article on '(505478) 2013 UT15', restate the 'Numbering and naming' content. | was numbered (505478) by the Minor Planet Center on 4 November 2017 (M.P.C. 107067). As of 2017, this minor planet has not received a name. | [
"(505478) 2013 UT15\n\nis an extreme trans-Neptunian object from the scattered disc, located in the outermost regions of the Solar System, approximately 260 km in diameter. It was discovered on 2 August 2013, by astronomers of the Outer Solar System Origins Survey at Mauna Kea Observatory, Hawaii, United States.",
... |
(505478)_2013_UT15_17507105 | What does the article about '(505478) 2013 UT15' say regarding 'Orbit'? | With a semi-major axis of 196 AU, orbits the Sun at a distance of 43.9–348 AU once every 2,742 years. Its orbit has an eccentricity of 0.78 and an inclination of 11° with respect to the ecliptic. It has a similar orbit to, except for a smaller inclination. belongs to a small number of detached objects with perihelion d... | [
"(505478) 2013 UT15\n\nis an extreme trans-Neptunian object from the scattered disc, located in the outermost regions of the Solar System, approximately 260 km in diameter. It was discovered on 2 August 2013, by astronomers of the Outer Solar System Origins Survey at Mauna Kea Observatory, Hawaii, United States.",
... |
(505624)_2014_GU53_142589 | Describe the 'Physical characteristics' section of the article about '(505624) 2014 GU53'. | According to the American astronomer Michael Brown, for an object to be considered as a "possible" dwarf planet, its diameter has to measure between 200 and 400 kilometers. With his estimated diameter of 315 kilometers, this object falls into this category, which is the one with the lowest certainty in Brown's 5-class ... | [
"(505624) 2014 GU53 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, for an object to be considered as a \"possible\" dwarf planet, its diameter has to measure between 200 and 400 kilometers. With his estimated diameter of 315 kilometers, this object falls into this category, which ... |
(505624)_2014_GU53_142586 | What information does the article about '(505624) 2014 GU53' provide? | , provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 8 April 2014, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper belt object belongs to the hot... | [
"(505624) 2014 GU53 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, for an object to be considered as a \"possible\" dwarf planet, its diameter has to measure between 200 and 400 kilometers. With his estimated diameter of 315 kilometers, this object falls into this category, which ... |
(505624)_2014_GU53_142587 | Summarize the 'Orbit and classification' part of '(505624) 2014 GU53'. | orbits the Sun at a distance of 36.1–51.6 AU once every 290 years and 6 months (106,111 days; semi-major axis of 43.86 AU). Its orbit has an eccentricity of 0.18 and an inclination of 23° with respect to the ecliptic. It has an orbital uncertainty of 2–3. The object's observation arc begins with a precovery taken by Pa... | [
"(505624) 2014 GU53 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, for an object to be considered as a \"possible\" dwarf planet, its diameter has to measure between 200 and 400 kilometers. With his estimated diameter of 315 kilometers, this object falls into this category, which ... |
(505624)_2014_GU53_142588 | Summarize the 'Numbering and naming' part of '(505624) 2014 GU53'. | This minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number in the minor planet catalog (M.P.C. 107069). As of 2018, it has not been named. | [
"(505624) 2014 GU53 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, for an object to be considered as a \"possible\" dwarf planet, its diameter has to measure between 200 and 400 kilometers. With his estimated diameter of 315 kilometers, this object falls into this category, which ... |
(505657)_2014_SR339_8249235 | Summarize the '2018 flyby' part of '(505657) 2014 SR339'. | On 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 million km on 8 February 2095. It will al... | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249234 | Summarize the 'Close approaches' part of '(505657) 2014 SR339'. | As a potentially hazardous asteroid, has a minimum orbital intersection distance (MOID) with Earth of less than 0.05 AU and a diameter of greater than 150 meters. The Earth-MOID is currently 0.0354 AU, which translates into 13.8 lunar distances (LD). | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249232 | Reconstruct the content from the article about '(505657) 2014 SR339'. | , provisional designation, is a dark and elongated asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 970 m in diameter. It was discovered on 30 September 2014, by NASA's Wide-field Infrared Survey Explorer telescope (WISE) in Earth's orbit. Closely observed ... | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249239 | Explain what '(505657) 2014 SR339' covers in the 'Numbering and naming' section. | This minor planet was numbered by the Minor Planet Center on 4 November 2017 (M.P.C. 107069). As of 2018, it has not been named. | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249237 | Describe the 'Rotation period' section of the article about '(505657) 2014 SR339'. | On 9 February, radiometric observations by the Arecibo Observatory revealed that the asteroid has an elongated, lumpy shape. The radar images also gave it a rotational period between 8 and 9 hours. A refined period of 8.7 hour agrees with (photometric) lightcurve observations by American photometrist Brian Warner at th... | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249233 | What information does the article about '(505657) 2014 SR339' provide on 'Orbit and classification'? | is a member of the Apollo asteroids, which cross the orbit of Earth. Apollo's are the largest group of near-Earth objects with nearly 10 thousand known objects. It orbits the Sun at a distance of 0.90–1.70 AU once every 18 months (541 days; semi-major axis of 1.30 AU). Its orbit has an eccentricity of 0.30 and an incli... | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249236 | From the article on '(505657) 2014 SR339', restate the 'Physical characteristics' content. | The asteroid's spectral type is unknown. Due to its unusually low albedo (see below) it is likely a carbonaceous C-type asteroid. | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(505657)_2014_SR339_8249238 | What information does the article about '(505657) 2014 SR339' provide on 'Diameter and albedo'? | According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, measures 0.971 kilometers in diameter and its surface has an albedo of 0.068. During its close approach in February 2018, radiometric observations by Arecibo Observatory determined that the object is at least 1.5 km wide. | [
"(505657) 2014 SR339 — 2018 flyby\n\nOn 7 February 2018 it passed 0.054 AU from the Earth when its apparent magnitude brightened to 14. Goldstone observed it until the following day. While this was an 8.1-million kilometer flyby, the next close flyby of 6.3 million km will occur on 5 February 2058, and another 7.6 ... |
(506479)_2003_HB57_18040019 | Explain what '(506479) 2003 HB57' covers in the 'Physical characterization' section. | has a BR-type spectrum and an estimated diameter of 147 and 200 kilometers based on an assumed albedo of 0.09 and 0.04, respectively. | [
"(506479) 2003 HB57 — Physical characterization\n\nhas a BR-type spectrum and an estimated diameter of 147 and 200 kilometers based on an assumed albedo of 0.09 and 0.04, respectively.",
"(506479) 2003 HB57\n\n, is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Sol... |
(506479)_2003_HB57_18040016 | What information does the article about '(506479) 2003 HB57' provide? | , is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Solar System, approximately 180 kilometers in diameter. It was discovered by astronomers at the Mauna Kea Observatory on 26 April 2003. | [
"(506479) 2003 HB57 — Physical characterization\n\nhas a BR-type spectrum and an estimated diameter of 147 and 200 kilometers based on an assumed albedo of 0.09 and 0.04, respectively.",
"(506479) 2003 HB57\n\n, is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Sol... |
(506479)_2003_HB57_18040017 | Describe the 'Description' section of the article about '(506479) 2003 HB57'. | orbits the Sun at a distance of 38.1–294.2 AU once every 2141 years and 10 months (782,317 days). Its orbit has an eccentricity of 0.77 and an inclination of 15° with respect to the ecliptic. | [
"(506479) 2003 HB57 — Physical characterization\n\nhas a BR-type spectrum and an estimated diameter of 147 and 200 kilometers based on an assumed albedo of 0.09 and 0.04, respectively.",
"(506479) 2003 HB57\n\n, is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Sol... |
(506479)_2003_HB57_18040018 | What information does the article about '(506479) 2003 HB57' provide on 'Extended scattered disc'? | It is one of a small group of extreme trans-Neptunian objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more. Such objects can not have reached their present-day orbits without the gravitational influence of some perturbing object, which lead to the speculation of planet nine. | [
"(506479) 2003 HB57 — Physical characterization\n\nhas a BR-type spectrum and an estimated diameter of 147 and 200 kilometers based on an assumed albedo of 0.09 and 0.04, respectively.",
"(506479) 2003 HB57\n\n, is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Sol... |
(508338)_2015_SO20_18040077 | Summarize the following section from the article on '(508338) 2015 SO20'. | is an extreme trans-Neptunian object and extended scattered disc object from the outermost region of the Solar System, approximately 220 km in diameter. | [
"(508338) 2015 SO20\n\nis an extreme trans-Neptunian object and extended scattered disc object from the outermost region of the Solar System, approximately 220 km in diameter.",
"(508338) 2015 SO20 — Description\n\nThis minor planet was first observed as on 8 October 2010, by American astronomer Megan Schwamb at ... |
(508338)_2015_SO20_18040078 | Based on the article about '(508338) 2015 SO20', describe the 'Description' section. | This minor planet was first observed as on 8 October 2010, by American astronomer Megan Schwamb at ESO's La Silla Observatory in northern Chile. It has also been observed as during the Calar Alto TNO Survey (Z79) at the Calar Alto Observatory, Spain, on 20 September 2015. It orbits the Sun at a distance of 33.2–290.1 A... | [
"(508338) 2015 SO20\n\nis an extreme trans-Neptunian object and extended scattered disc object from the outermost region of the Solar System, approximately 220 km in diameter.",
"(508338) 2015 SO20 — Description\n\nThis minor planet was first observed as on 8 October 2010, by American astronomer Megan Schwamb at ... |
(508338)_2015_SO20_18040079 | From the article on '(508338) 2015 SO20', restate the 'Extended scattered disc' content. | It is one a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more. Such objects can not reach such orbits without some perturbing object, which lead to the speculation of planet nine. | [
"(508338) 2015 SO20\n\nis an extreme trans-Neptunian object and extended scattered disc object from the outermost region of the Solar System, approximately 220 km in diameter.",
"(508338) 2015 SO20 — Description\n\nThis minor planet was first observed as on 8 October 2010, by American astronomer Megan Schwamb at ... |
(508338)_2015_SO20_18040080 | From the article on '(508338) 2015 SO20', restate the 'Physical characteristics' content. | Based on an absolute magnitude of 6.5 and an assumed albedo of 0.09, the Johnston's Archive calculated a mean-diameter of 222 kilometers. Michael Brown estimates an albedo of 0.08 with a diameter of 221 kilometers using an absolute magnitude of 6.7. He also considers it a dwarf-planet candidate with a low probability (... | [
"(508338) 2015 SO20\n\nis an extreme trans-Neptunian object and extended scattered disc object from the outermost region of the Solar System, approximately 220 km in diameter.",
"(508338) 2015 SO20 — Description\n\nThis minor planet was first observed as on 8 October 2010, by American astronomer Megan Schwamb at ... |
(511002)_2013_MZ5_14646169 | Describe the '10,000th discovered NEO' section of the article about '(511002) 2013 MZ5'. | was the 10,000th near-Earth object (NEO) ever discovered in June 2013 and considered a significant milestone in exploring the NEO population. | [
"(511002) 2013 MZ5 — 10,000th discovered NEO\n\nwas the 10,000th near-Earth object (NEO) ever discovered in June 2013 and considered a significant milestone in exploring the NEO population.",
"(511002) 2013 MZ5 — Orbit and classification\n\nis an Amor asteroid – a subgroup of near-Earth asteroids that approach th... |
(511002)_2013_MZ5_14646167 | Explain what '(511002) 2013 MZ5' covers in the 'Orbit and classification' section. | is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. It orbits the Sun at a distance of 1.3–1.8 AU once every 23 months (707 days; semi-major axis of 1.55 AU). Its orbit has an eccentricity of 0.18 and an inclination of 29° with respect to the eclip... | [
"(511002) 2013 MZ5 — 10,000th discovered NEO\n\nwas the 10,000th near-Earth object (NEO) ever discovered in June 2013 and considered a significant milestone in exploring the NEO population.",
"(511002) 2013 MZ5 — Orbit and classification\n\nis an Amor asteroid – a subgroup of near-Earth asteroids that approach th... |
(511002)_2013_MZ5_14646166 | Describe the content of the article about '(511002) 2013 MZ5'. | , provisional designation, is a sub-kilometer asteroid, classified as a near-Earth object of the Amor group, estimated to measure approximately 300 m in diameter. It was discovered on 18 June 2013, by astronomers with the Pan-STARRS survey at Haleakala Observatory on the island of Maui, Hawaii, in the United States. It... | [
"(511002) 2013 MZ5 — 10,000th discovered NEO\n\nwas the 10,000th near-Earth object (NEO) ever discovered in June 2013 and considered a significant milestone in exploring the NEO population.",
"(511002) 2013 MZ5 — Orbit and classification\n\nis an Amor asteroid – a subgroup of near-Earth asteroids that approach th... |
(511002)_2013_MZ5_14646171 | Reconstruct the content about 'Diameter and albedo' from the article on '(511002) 2013 MZ5'. | measures approximately 300 meters in diameter for an absolute magnitude of 20.1 and an assumed albedo 0.18, which is typical value for stony asteroids. A generic magnitude-to-diameter conversion on a wider range of possible albedos (0.30 to 0.05) gives a diameter between 230 and 570 meters. As of 2019, no rotational li... | [
"(511002) 2013 MZ5 — 10,000th discovered NEO\n\nwas the 10,000th near-Earth object (NEO) ever discovered in June 2013 and considered a significant milestone in exploring the NEO population.",
"(511002) 2013 MZ5 — Orbit and classification\n\nis an Amor asteroid – a subgroup of near-Earth asteroids that approach th... |
(511002)_2013_MZ5_14646168 | Reconstruct the content about 'Close approaches' from the article on '(511002) 2013 MZ5'. | The asteroid has an Earth minimum orbital intersection distance of 0.4613 AU, which translates into 180 lunar distances. It also makes close approaches to Mars. On 28 August 2125, it is projected to pass the Red Planet at a nominal distance of 0.0910 AU. With an aphelion of 1.83 AU, it is also a Mars-crossing asteroid. | [
"(511002) 2013 MZ5 — 10,000th discovered NEO\n\nwas the 10,000th near-Earth object (NEO) ever discovered in June 2013 and considered a significant milestone in exploring the NEO population.",
"(511002) 2013 MZ5 — Orbit and classification\n\nis an Amor asteroid – a subgroup of near-Earth asteroids that approach th... |
(516977)_2012_HZ84_14087084 | Summarize the 'Orbit and classification' part of '(516977) 2012 HZ84'. | of the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contrary to the much less gravitationally affected objects o... | [
"(516977) 2012 HZ84 — Orbit and classification\n\nof the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contra... |
(516977)_2012_HZ84_14087085 | Based on the article about '(516977) 2012 HZ84', describe the 'Milestone image' section. | When the New Horizons spacecraft imaged in 2017, it was the farthest from Earth ever captured by a spacecraft. The image was taken by the spacecraft's Long Range Reconnaissance Imager (LORRI) on 5 December 2017 at more than 6.12 billion kilometers (40.9 AU) away from Earth. This record was previously held by the Voyage... | [
"(516977) 2012 HZ84 — Orbit and classification\n\nof the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contra... |
(516977)_2012_HZ84_14087083 | Based on the article about '(516977) 2012 HZ84', describe the 'Orbit and classification' section. | orbits the Sun at a distance of 37.2–55.4 AU once every 315 years and 5 months (semi-major axis of 46.33 AU). Its orbit has an eccentricity of 0.20 and an inclination of 5.4° with respect to the ecliptic. As a cubewano, also known as classical Kuiper belt object, is located in between the resonant plutino and twotino p... | [
"(516977) 2012 HZ84 — Orbit and classification\n\nof the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contra... |
(516977)_2012_HZ84_14087086 | Explain what '(516977) 2012 HZ84' covers in the 'Numbering and naming' section. | This minor planet was numbered by the Minor Planet Center on 30 April 2018 and received the number in the minor planet catalog (M.P.C. 110093). As of 2020, it has not been named. | [
"(516977) 2012 HZ84 — Orbit and classification\n\nof the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contra... |
(516977)_2012_HZ84_14087082 | Describe the content of the article about '(516977) 2012 HZ84'. | , provisional designation, is a small trans-Neptunian object from the Kuiper belt located in the outermost region of the Solar System, approximately 74 km in diameter. It was discovered on 17 April 2012, by a team of astronomers using one of the Magellan Telescopes in Chile during the New Horizons KBO Search in order t... | [
"(516977) 2012 HZ84 — Orbit and classification\n\nof the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contra... |
(516977)_2012_HZ84_14087087 | Reconstruct the content about 'Physical characteristics' from the article on '(516977) 2012 HZ84'. | According to Johnston's Archive, the object measures 74 kilometers in diameter based on an assumed albedo of 0.09 and an absolute magnitude of 8.9. As of 2019, no rotational lightcurve of has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown. | [
"(516977) 2012 HZ84 — Orbit and classification\n\nof the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contra... |
(523635)_2010_DN93_18331423 | What information does the article about '(523635) 2010 DN93' provide on 'Numbering and naming'? | The body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey at Apache Point Observatory in March 2003, almost seven years prior to its official discovery observation at Haleakala. It was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been na... | [
"(523635) 2010 DN93 — Numbering and naming\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey at Apache Point Observatory in March 2003, almost seven years prior to its official discovery observation at Haleakala. It was numbered by the Minor Planet Center on 25 September 20... |
(523635)_2010_DN93_18331424 | Based on the article about '(523635) 2010 DN93', describe the 'Diameter and albedo' section. | has an absolute magnitude of 4.8. According to the Johnston's archive and astronomer Michael Brown, it measures 486 and 490 kilometers in diameter, based on an assumed albedo for the body's surface of 0.09 and 0.07, respectively. As of 2018, no physical characteristics have been determined from photometric observations... | [
"(523635) 2010 DN93 — Numbering and naming\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey at Apache Point Observatory in March 2003, almost seven years prior to its official discovery observation at Haleakala. It was numbered by the Minor Planet Center on 25 September 20... |
(523635)_2010_DN93_18331422 | Explain what '(523635) 2010 DN93' covers in the 'Orbit and classification' section. | orbits the Sun at a distance of 45.1–65.5 AU once every 411 years (150,152 days; semi-major axis of 55.29 AU). Its orbit has an eccentricity of 0.18 and an inclination of 41° with respect to the ecliptic. This distant minor planet is a trans-Neptunian object and a member of the scattered disc population. Scattered-disc... | [
"(523635) 2010 DN93 — Numbering and naming\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey at Apache Point Observatory in March 2003, almost seven years prior to its official discovery observation at Haleakala. It was numbered by the Minor Planet Center on 25 September 20... |
(523635)_2010_DN93_18331421 | Summarize the following section from the article on '(523635) 2010 DN93'. | , provisional designation, is a trans-Neptunian object from in the scattered disc located in the outermost region of the Solar System. It was discovered on 26 February 2010, by astronomers with the Pan-STARRS survey at Haleakala Observatory on the island of Maui, Hawaii, in the United States. Assuming a low albedo, the... | [
"(523635) 2010 DN93 — Numbering and naming\n\nThe body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey at Apache Point Observatory in March 2003, almost seven years prior to its official discovery observation at Haleakala. It was numbered by the Minor Planet Center on 25 September 20... |
(523639)_2010_RE64_4891120 | From the article on '(523639) 2010 RE64', restate the 'Numbering and naming' content. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named. | [
"(523639) 2010 RE64 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523639) 2010 RE64 — Classification and orbit\n\nhas an observation arc of 1774 days, and there are currently no known precovery image... |
(523639)_2010_RE64_4891119 | Describe the 'Classification and orbit' section of the article about '(523639) 2010 RE64'. | has an observation arc of 1774 days, and there are currently no known precovery images to help refine its orbit. It is currently 53.7 AU from the Sun. Based on JPL's best-fit solution for the orbit, it reached aphelion around 1829. It is estimated to come to perihelion around 2079. Although the discovery is credited to... | [
"(523639) 2010 RE64 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523639) 2010 RE64 — Classification and orbit\n\nhas an observation arc of 1774 days, and there are currently no known precovery image... |
(523639)_2010_RE64_4891118 | What information does the article about '(523639) 2010 RE64' provide? | ''', provisional designation ', is a trans-Neptunian object in the scattered disc located in the outermost region of the Solar System, approximately 570 km in diameter. It was discovered on 11 July 2010 by the Pan-STARRS-1 survey at the Haleakala Observatory, Hawaii, in the United States. | [
"(523639) 2010 RE64 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523639) 2010 RE64 — Classification and orbit\n\nhas an observation arc of 1774 days, and there are currently no known precovery image... |
(523639)_2010_RE64_4891121 | From the article on '(523639) 2010 RE64', restate the 'Physical characteristics' content. | Assuming a generic trans-Neptunian albedo of 0.09, it is about 580 kilometers in diameter. However, since the true albedo is unknown and it has an absolute magnitude of 4.4, it could easily be from about 350 to 780 km in diameter (for typical albedos of 0.05 to 0.25). Michael Brown estimates a similar diameter of 561 k... | [
"(523639) 2010 RE64 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523639) 2010 RE64 — Classification and orbit\n\nhas an observation arc of 1774 days, and there are currently no known precovery image... |
(523643)_2010_TY53_17615088 | What does the article about '(523643) 2010 TY53' say regarding 'Diameter and albedo'? | According to the Johnston's archive and to Michael Brown, measures 321 and 329 kilometers in diameter, based on an absolute magnitude of 5.7 and 5.8 and an assumed standard albedo of 0.09 and 0.08 for the body's surface, respectively. As of 2018, no physical characteristics have been determined from photometric observ... | [
"(523643) 2010 TY53 — Diameter and albedo\n\nAccording to the Johnston's archive and to Michael Brown, measures 321 and 329 kilometers in diameter, based on an absolute magnitude of 5.7 and 5.8 and an assumed standard albedo of 0.09 and 0.08 for the body's surface, respectively. As of 2018, no physical characteris... |
(523643)_2010_TY53_17615086 | Reconstruct the content about 'Orbit and classification' from the article on '(523643) 2010 TY53'. | orbits the Sun at a distance of 21.1–56.6 AU once every 241 years and 11 months (88,365 days; semi-major axis of 38.83 AU). Its orbit has an eccentricity of 0.46 and an inclination of 22° with respect to the ecliptic. The body's observation arc begins with a precovery at Palomar Observatory in October 2004, or almost s... | [
"(523643) 2010 TY53 — Diameter and albedo\n\nAccording to the Johnston's archive and to Michael Brown, measures 321 and 329 kilometers in diameter, based on an absolute magnitude of 5.7 and 5.8 and an assumed standard albedo of 0.09 and 0.08 for the body's surface, respectively. As of 2018, no physical characteris... |
(523643)_2010_TY53_17615087 | What information does the article about '(523643) 2010 TY53' provide on 'Numbering and naming'? | This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named. | [
"(523643) 2010 TY53 — Diameter and albedo\n\nAccording to the Johnston's archive and to Michael Brown, measures 321 and 329 kilometers in diameter, based on an absolute magnitude of 5.7 and 5.8 and an assumed standard albedo of 0.09 and 0.08 for the body's surface, respectively. As of 2018, no physical characteris... |
(523643)_2010_TY53_17615085 | What information does the article about '(523643) 2010 TY53' provide? | ''', provisional designation ' is a trans-Neptunian object and centaur located in the outermost region of the Solar System. With an absolute magnitude of 5.7, it approximately measures 325 km in diameter. It was discovered on 4 August 2010 by the Pan-STARRS-1 survey at the Haleakala Observatory, Hawaii, in the United S... | [
"(523643) 2010 TY53 — Diameter and albedo\n\nAccording to the Johnston's archive and to Michael Brown, measures 321 and 329 kilometers in diameter, based on an absolute magnitude of 5.7 and 5.8 and an assumed standard albedo of 0.09 and 0.08 for the body's surface, respectively. As of 2018, no physical characteris... |
(523645)_2010_VK201_56390 | Explain what '(523645) 2010 VK201' covers in the 'Numbering and naming' section. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named. | [
"(523645) 2010 VK201 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523645) 2010 VK201 — Orbit and classification\n\nLocated beyond the orbit of Neptune, is a non-resonant classical Kuiper belt objec... |
(523645)_2010_VK201_56389 | What does the article about '(523645) 2010 VK201' say regarding 'Orbit and classification'? | Located beyond the orbit of Neptune, is a non-resonant classical Kuiper belt object (cubewano) of the so-called hot population, which have higher inclinations than those of the cold population. It orbits the Sun at a distance of 38.0–48.1 AU once every 282 years and 2 months (103,060 days; semi-major axis of 43.02 AU)... | [
"(523645) 2010 VK201 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523645) 2010 VK201 — Orbit and classification\n\nLocated beyond the orbit of Neptune, is a non-resonant classical Kuiper belt objec... |
(523645)_2010_VK201_56388 | What information does the article about '(523645) 2010 VK201' provide? | ''', provisional designation ', is a trans-Neptunian object and member of the classical Kuiper belt, approximately 500 km in diameter. It was discovered on 1 November 2010, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. It has a rotation period of 7.6 hours. It was numbered in September 201... | [
"(523645) 2010 VK201 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523645) 2010 VK201 — Orbit and classification\n\nLocated beyond the orbit of Neptune, is a non-resonant classical Kuiper belt objec... |
(523645)_2010_VK201_56392 | Based on the article about '(523645) 2010 VK201', describe the 'Rotation period' section. | In 2011, a rotational lightcurve of was obtained from photometric observations in the S- and R-band by Susan Benecchi and Scott Sheppard taken with Carnegie's 2.5-meter Irénée du Pont telescope at the Las Campanas Observatory in Chile. Lightcurve analysis gave a rotation period of 7.59 hours with a brightness amplitud... | [
"(523645) 2010 VK201 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523645) 2010 VK201 — Orbit and classification\n\nLocated beyond the orbit of Neptune, is a non-resonant classical Kuiper belt objec... |
(523645)_2010_VK201_56393 | Explain what '(523645) 2010 VK201' covers in the 'Diameter and albedo' section. | According to Michael Brown and the Collaborative Asteroid Lightcurve Link, measures 501 and 505 kilometers in diameter, based on an absolute magnitude of 4.6 and 5.0, assuming an albedo of 0.07 and 0.10 for the body's surface, respectively. The Johnston's archive estimates a smaller diameter of 443 kilometers. | [
"(523645) 2010 VK201 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523645) 2010 VK201 — Orbit and classification\n\nLocated beyond the orbit of Neptune, is a non-resonant classical Kuiper belt objec... |
(523662)_2012_MU2_1400623 | From the article on '(523662) 2012 MU2', restate the 'Numbering and naming' content. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named. | [
"(523662) 2012 MU2 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523662) 2012 MU2 — Orbit and classification\n\nis a member of the Apollo asteroids, a group of near-Earth objects with an Earth-crossi... |
(523662)_2012_MU2_1400622 | From the article on '(523662) 2012 MU2', restate the 'Orbit and classification' content. | is a member of the Apollo asteroids, a group of near-Earth objects with an Earth-crossing orbit. It orbits the Sun at a distance of 1.0–3.1 AU once every 2 years and 11 months (1,076 days; semi-major axis of 2.06 AU). Its orbit has an eccentricity of 0.51 and an inclination of 11° with respect to the ecliptic. On 24 Ju... | [
"(523662) 2012 MU2 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523662) 2012 MU2 — Orbit and classification\n\nis a member of the Apollo asteroids, a group of near-Earth objects with an Earth-crossi... |
(523662)_2012_MU2_1400621 | Reconstruct the content from the article about '(523662) 2012 MU2'. | ''', provisional designation ', is a sub-kilometer asteroid on an eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group. It was discovered on 18 June 2012 by astronomers of the Catalina Sky Survey at an apparent magnitude of 19.9 using a 0.68 m Schmidt–Cassegrain telesc... | [
"(523662) 2012 MU2 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). As of 2018, it has not been named.",
"(523662) 2012 MU2 — Orbit and classification\n\nis a member of the Apollo asteroids, a group of near-Earth objects with an Earth-crossi... |
(523671)_2013_FZ27_29326391 | Summarize the 'Numbering and naming' part of '(523671) 2013 FZ27'. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). The body was given the wrong discovery credit in the initial MPC Circular and The Minor Planet Center issued an Errata on April 6, 2019 on MPC 112429 correcting the mistake and gives the discovery credit of 2013 FZ27 to Scot... | [
"(523671) 2013 FZ27 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). The body was given the wrong discovery credit in the initial MPC Circular and The Minor Planet Center issued an Errata on April 6, 2019 on MPC 112429 correcting the mistake a... |
(523671)_2013_FZ27_29326392 | Based on the article about '(523671) 2013 FZ27', describe the 'Diameter and albedo' section. | According to Michael Brown and the Johnston's archive, measures 561 and 584 kilometers in diameter, based on an absolute magnitude of 4.6 and 4.4 respectively. Both sources assume a standard albedo of 0.09 for the body's surface. As of 2018, no physical characteristics have been determined from photometric observation... | [
"(523671) 2013 FZ27 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). The body was given the wrong discovery credit in the initial MPC Circular and The Minor Planet Center issued an Errata on April 6, 2019 on MPC 112429 correcting the mistake a... |
(523671)_2013_FZ27_29326388 | Describe the content of the article about '(523671) 2013 FZ27'. | ''', provisional designation ', is a trans-Neptunian object located in the Kuiper belt in the outermost region of the Solar System, approximately 570 km in diameter. It was discovered on 16 March 2013, by American astronomers Scott Sheppard and Chad Trujillo at the CTIO in Chile. Numbered in 2018, this minor planet has... | [
"(523671) 2013 FZ27 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111778). The body was given the wrong discovery credit in the initial MPC Circular and The Minor Planet Center issued an Errata on April 6, 2019 on MPC 112429 correcting the mistake a... |
(523674)_2013_MA12_29729155 | Summarize the 'Orbit and classification' part of '(523674) 2013 MA12'. | orbits the Sun at a distance of 39.1–44.3 AU once every 269 years and 1 month (98,276 days; semi-major axis of 41.68 AU). Its orbit has an eccentricity of 0.06 and an inclination of 23° with respect to the ecliptic. As a cubewano, also known as classical Kuiper belt object, it is located in between the resonant plutino... | [
"(523674) 2013 MA12 — Orbit and classification\n\norbits the Sun at a distance of 39.1–44.3 AU once every 269 years and 1 month (98,276 days; semi-major axis of 41.68 AU). Its orbit has an eccentricity of 0.06 and an inclination of 23° with respect to the ecliptic. As a cubewano, also known as classical Kuiper belt... |
(523674)_2013_MA12_29729157 | Summarize the 'Physical characteristics' part of '(523674) 2013 MA12'. | According to the American astronomer Michael Brown, measures 343 kilometers in diameter based on an assumed albedo of 0.08. On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system. Similarly, Johnston's archive es... | [
"(523674) 2013 MA12 — Orbit and classification\n\norbits the Sun at a distance of 39.1–44.3 AU once every 269 years and 1 month (98,276 days; semi-major axis of 41.68 AU). Its orbit has an eccentricity of 0.06 and an inclination of 23° with respect to the ecliptic. As a cubewano, also known as classical Kuiper belt... |
(523674)_2013_MA12_29729154 | What information does the article about '(523674) 2013 MA12' provide? | , provisional designation, is a classical trans-Neptunian object and dwarf planet candidate from the Kuiper belt, located in the outermost region of the Solar System, approximately 340 km in diameter. The cubewano belongs to the hot population. It was discovered on 26 July 2011, by astronomers with the Pan-STARRS surve... | [
"(523674) 2013 MA12 — Orbit and classification\n\norbits the Sun at a distance of 39.1–44.3 AU once every 269 years and 1 month (98,276 days; semi-major axis of 41.68 AU). Its orbit has an eccentricity of 0.06 and an inclination of 23° with respect to the ecliptic. As a cubewano, also known as classical Kuiper belt... |
(523676)_2013_UL10_19252066 | Describe the 'Numbering and naming' section of the article about '(523676) 2013 UL10'. | This minor planet was numbered by the Minor Planet Center on 25 September 2018, receiving the number in the minor planet catalog (M.P.C. 111778). , it has not been named. According to the established naming conventions, it will be named after one of the many centaurs from Greek mythology, which are creatures with the u... | [
"(523676) 2013 UL10 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018, receiving the number in the minor planet catalog (M.P.C. 111778). , it has not been named. According to the established naming conventions, it will be named after one of the many centaurs fr... |
(523676)_2013_UL10_19252065 | Summarize the 'Orbit and classification' part of '(523676) 2013 UL10'. | This object belongs to the centaurs, a dynamically unstable population of small Solar System bodies with chaotic orbits between the classical asteroids and the trans-Neptunian objects. Centaurs are considered to be objects with short lifetimes of approximately one million years, transitioning from the inactive populati... | [
"(523676) 2013 UL10 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018, receiving the number in the minor planet catalog (M.P.C. 111778). , it has not been named. According to the established naming conventions, it will be named after one of the many centaurs fr... |
(523676)_2013_UL10_19252064 | Describe the content of the article about '(523676) 2013 UL10'. | (prov. designation: ) is a reddish centaur with cometary activity orbiting the Sun between Jupiter and Uranus. It was discovered on 18 August 2010, by a team of astronomers with the Pan-STARRS survey at the Haleakalā Observatory, Hawaii. It is the first centaur known to have both comet-like activity and red surface col... | [
"(523676) 2013 UL10 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018, receiving the number in the minor planet catalog (M.P.C. 111778). , it has not been named. According to the established naming conventions, it will be named after one of the many centaurs fr... |
(523676)_2013_UL10_19252068 | Summarize the 'Physical characteristics' part of '(523676) 2013 UL10'. | with an absolute magnitude 13.46. In December 2015, observations with the Galileo National Telescope on the Canary Islands revealed that exhibits comet-like activity. Apart from the object's dust coma, the astronomers also deduced a diameter of no more than 10 km for this centaur's nucleus, assuming an albedo of 0.12.... | [
"(523676) 2013 UL10 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018, receiving the number in the minor planet catalog (M.P.C. 111778). , it has not been named. According to the established naming conventions, it will be named after one of the many centaurs fr... |
(523676)_2013_UL10_19252067 | Reconstruct the content about 'Physical characteristics' from the article on '(523676) 2013 UL10'. | As with other populations, the centaurs show a bimodal distribution of colors: red and blue-grey. Cometary-like activity is well known among the grey centaurs, prominently represented by 2060 Chiron, which is also the namesake of the Chiron-type comets. However, outgassing activity of red centaurs (e.g. 5145 Pholus) ha... | [
"(523676) 2013 UL10 — Numbering and naming\n\nThis minor planet was numbered by the Minor Planet Center on 25 September 2018, receiving the number in the minor planet catalog (M.P.C. 111778). , it has not been named. According to the established naming conventions, it will be named after one of the many centaurs fr... |
(523683)_2014_CP23_30206440 | Based on the article about '(523683) 2014 CP23', describe the 'Orbit and classification' section. | orbits the Sun at a distance of 38.1–66.5 AU once every 378 years and 5 months (138,225 days; semi-major axis of 52.32 AU). Its orbit has an eccentricity of 0.27 and an inclination of 29° with respect to the ecliptic. It is a scattered-disc object on a moderately eccentric orbit that never comes closer than 8 AU to the... | [
"(523683) 2014 CP23 — Orbit and classification\n\norbits the Sun at a distance of 38.1–66.5 AU once every 378 years and 5 months (138,225 days; semi-major axis of 52.32 AU). Its orbit has an eccentricity of 0.27 and an inclination of 29° with respect to the ecliptic. It is a scattered-disc object on a moderately ec... |
(523683)_2014_CP23_30206442 | Describe the 'Physical characteristics' section of the article about '(523683) 2014 CP23'. | According to American astronomer Michael Brown and the Johnston's archive, measures 266 and 267 kilometers in diameter based on an assumed albedo of 0.08 and 0.09, respectively. On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-cl... | [
"(523683) 2014 CP23 — Orbit and classification\n\norbits the Sun at a distance of 38.1–66.5 AU once every 378 years and 5 months (138,225 days; semi-major axis of 52.32 AU). Its orbit has an eccentricity of 0.27 and an inclination of 29° with respect to the ecliptic. It is a scattered-disc object on a moderately ec... |
(523683)_2014_CP23_30206439 | Summarize the following section from the article on '(523683) 2014 CP23'. | , provisional designation, is a trans-Neptunian object from the scattered disc located in the outermost region of the Solar System It was discovered on 29 October 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The dwarf planet candidate measures approximately 267 km in ... | [
"(523683) 2014 CP23 — Orbit and classification\n\norbits the Sun at a distance of 38.1–66.5 AU once every 378 years and 5 months (138,225 days; semi-major axis of 52.32 AU). Its orbit has an eccentricity of 0.27 and an inclination of 29° with respect to the ecliptic. It is a scattered-disc object on a moderately ec... |
(523684)_2014_CQ23_30037688 | What information does the article about '(523684) 2014 CQ23' provide on 'Physical characteristics'? | According to the American astronomer Michael Brown, measures 343 kilometers in diameter based on an assumed albedo of 0.08. On his website, Michael Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system. Similarly, Johnston's ar... | [
"(523684) 2014 CQ23 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, measures 343 kilometers in diameter based on an assumed albedo of 0.08. On his website, Michael Brown lists this object as a \"possible\" dwarf planet (200–400 km), which is the category with the lowest certainty i... |
(523684)_2014_CQ23_30037687 | From the article on '(523684) 2014 CQ23', restate the 'Numbering and naming' content. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 and received the number in the minor planet catalog (M.P.C. 111779). As of 2018, it has not been named. | [
"(523684) 2014 CQ23 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, measures 343 kilometers in diameter based on an assumed albedo of 0.08. On his website, Michael Brown lists this object as a \"possible\" dwarf planet (200–400 km), which is the category with the lowest certainty i... |
(523684)_2014_CQ23_30037685 | Reconstruct the content from the article about '(523684) 2014 CQ23'. | , provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 13 March 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper belt object belongs to the ho... | [
"(523684) 2014 CQ23 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, measures 343 kilometers in diameter based on an assumed albedo of 0.08. On his website, Michael Brown lists this object as a \"possible\" dwarf planet (200–400 km), which is the category with the lowest certainty i... |
(523684)_2014_CQ23_30037686 | From the article on '(523684) 2014 CQ23', restate the 'Orbit and classification' content. | is a cubewano, a classical, low-eccentricity object in the Kuiper belt, located in between the two resonant plutino and twotino populations, and belongs to the "stirred" hot population rather than to the cold population with low inclinations. It orbits the Sun at a distance of 38.7–53.7 AU once every 313 years and 8 mo... | [
"(523684) 2014 CQ23 — Physical characteristics\n\nAccording to the American astronomer Michael Brown, measures 343 kilometers in diameter based on an assumed albedo of 0.08. On his website, Michael Brown lists this object as a \"possible\" dwarf planet (200–400 km), which is the category with the lowest certainty i... |
(523687)_2014_DF143_30206860 | Reconstruct the content from the article about '(523687) 2014 DF143'. | , provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 12 April 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper belt object belongs to the ho... | [
"(523687) 2014 DF143\n\n, provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 12 April 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper b... |
(523687)_2014_DF143_30206863 | Summarize the 'Physical characteristics' part of '(523687) 2014 DF143'. | According to the American astronomer Michael Brown, measures 358 kilometers in diameter based on an assumed albedo of 0.08. On his website, Michael Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system. Similarly, Johnston's ar... | [
"(523687) 2014 DF143\n\n, provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 12 April 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper b... |
(523687)_2014_DF143_30206862 | Summarize the 'Numbering and naming' part of '(523687) 2014 DF143'. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 and received the number in the minor planet catalog (M.P.C. 111779). As of 2018, it has not been named. | [
"(523687) 2014 DF143\n\n, provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 12 April 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper b... |
(523687)_2014_DF143_30206861 | Reconstruct the content about 'Orbit and classification' from the article on '(523687) 2014 DF143'. | orbits the Sun at a distance of 40.9–44.8 AU once every 280 years and 4 months (102,379 days; semi-major axis of 42.83 AU). Its orbit has an eccentricity of 0.05 and an inclination of 24° with respect to the ecliptic. It has an orbital uncertainty of 1–2. The object's observation arc begins with a precovery taken by th... | [
"(523687) 2014 DF143\n\n, provisional designation, is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 12 April 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. The classical Kuiper b... |
(523692)_2014_EZ51_24833984 | Summarize the following section from the article on '(523692) 2014 EZ51'. | , prov. designation:, is a large trans-Neptunian object in the scattered disc, approximately 700 km in diameter. It was discovered on 18 April 2010, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. | [
"(523692) 2014 EZ51\n\n, prov. designation:, is a large trans-Neptunian object in the scattered disc, approximately 700 km in diameter. It was discovered on 18 April 2010, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States.",
"(523692) 2014 EZ51 — Physical characteristics\n\nAccording to M... |
(523692)_2014_EZ51_24833987 | From the article on '(523692) 2014 EZ51', restate the 'Physical characteristics' content. | According to Michael Brown and the Johnston's archive, measures 626 and 770 kilometers in diameter, based on an absolute magnitude of 4.2 and 3.8, with an assumed albedo of 0.10 and 0.09, respectively. The MPC/JPL databases give an absolute magnitude of 3.92. On 25 February 2019, a stellar occultation by was observed i... | [
"(523692) 2014 EZ51\n\n, prov. designation:, is a large trans-Neptunian object in the scattered disc, approximately 700 km in diameter. It was discovered on 18 April 2010, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States.",
"(523692) 2014 EZ51 — Physical characteristics\n\nAccording to M... |
(523692)_2014_EZ51_24833985 | What does the article about '(523692) 2014 EZ51' say regarding 'Orbit and classification'? | orbits the Sun at a distance of 40.4–64.4 AU once every 379 years and 3 months (138,537 days; semi-major axis of 52.4 AU). Its orbit has an eccentricity of 0.23 and an inclination of 10 deg with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Haleakala in April 2010... | [
"(523692) 2014 EZ51\n\n, prov. designation:, is a large trans-Neptunian object in the scattered disc, approximately 700 km in diameter. It was discovered on 18 April 2010, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States.",
"(523692) 2014 EZ51 — Physical characteristics\n\nAccording to M... |
(523706)_2014_HF200_29894411 | Based on the article about '(523706) 2014 HF200', describe the 'Physical characteristics' section. | According to the Johnston's archive and American astronomer Michael Brown, measures 293 and 302 kilometers in diameter based on an assumed albedo of 0.09 and 0.08, respectively. On his website, Michael Brown lists this object as a "possible" dwarf planet (200–400 km) which is the category with the lowest certainty in h... | [
"(523706) 2014 HF200 — Physical characteristics\n\nAccording to the Johnston's archive and American astronomer Michael Brown, measures 293 and 302 kilometers in diameter based on an assumed albedo of 0.09 and 0.08, respectively. On his website, Michael Brown lists this object as a \"possible\" dwarf planet (200–400... |
(523706)_2014_HF200_29894410 | Summarize the 'Numbering and naming' part of '(523706) 2014 HF200'. | This minor planet was numbered by the Minor Planet Center on 25 September 2018 and received the number in the minor planet catalog (M.P.C. 111779). As of 2018, it has not been named. | [
"(523706) 2014 HF200 — Physical characteristics\n\nAccording to the Johnston's archive and American astronomer Michael Brown, measures 293 and 302 kilometers in diameter based on an assumed albedo of 0.09 and 0.08, respectively. On his website, Michael Brown lists this object as a \"possible\" dwarf planet (200–400... |
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