Matches in DBpedia 2015-10 for { ?s <http://www.w3.org/2000/01/rdf-schema#comment> ?o }
- (35396)_1997_XF11 comment "(35396) 1997 XF11, also written (35396) 1997 XF11, is a near-Earth and Mars-crosser asteroid which, 3 months after its discovery on December 6, 1997, by James V. Scotti of the University of Arizona's Spacewatch Project, was predicted to make an exceptionally close approach to Earth on 28 October 2028.".
- (35671)_1998_SN165 comment "(35671) 1998 SN165 is a trans-Neptunian object. It was discovered on 23 September 1998, by A. Gleason at Steward Observatory.It was originally classified as a plutino with a 2:3 mean-motion resonance with Neptune, but further observations have established that it is a cubewano—a member of the classical Kuiper belt.With an estimated size of 7005393000000000000♠393+39−38 km, 1998 SN165 is a possible dwarf planet.".
- (357439)_2004_BL86 comment "(357439) 2004 BL86, provisionally known as 2004 BL86, is a near-Earth asteroid estimated to be about 325 meters (1,066 feet) in diameter. It was discovered on 30 January 2004 by LINEAR. It passed 1,199,600 km (745,400 mi), or 3.1 lunar distances, from Earth on 26 January 2015 at 16:20 UTC. During the 2015 approach it was determined to have a satellite.".
- (367789)_2011_AG5 comment "(367789) 2011 AG5 (also written 2011 AG5) is a near-Earth asteroid and potentially hazardous object. It has a diameter of about 140 meters (460 ft). It was removed from the Sentry Risk Table on 21 December 2012 and as such it now has a rating of 0 on the Torino Scale.It was discovered on 8 January 2011 by the Mt. Lemmon Survey at an apparent magnitude of 19.6 using a 1.52-meter (60 in) reflecting telescope.".
- (3708)_1974_FV1 comment "(3708) 1974 FV1 is a Jupiter trojan approximately 80 kilometers in diameter. It completes one orbit around the Sun in just under 12 years. It was discovered on 21 March 1974 at Cerro El Roble observatory in Chile. Its number is the lowest of all unnamed minor planets.".
- (374158)_2004_UL comment "(374158) 2004 UL is a Mercury-crosser, Venus-crosser, Apollo, and Mars-crosser asteroid. It has the second-smallest perihelion of any known asteroid, after (137924) 2000 BD19.".
- (38084)_1999_HB12 comment "(38084) 1999 HB12, also written as (38084) 1999 HB12, is a trans-Neptunian object that resides in the Kuiper belt region of the Solar System. It was discovered on 18 April 1999 by Marc W. Buie and Robert L. Millis.It is in a 2:5 orbital resonance with Neptune.".
- (385185)_1993_RO comment "(385185) 1993 RO is a plutino. It was the first plutino discovered after Pluto itself, with 1993 RP and (15788) 1993 SB a day and two days later, respectively. The discovery was made in 1993 at the Mauna Kea Observatory with a 2.2-meter telescope. Very little is known about 1993 RO. Even the diameter estimate of ~90 km is based on the assumed albedo of 0.09.".
- (385250)_2001_DH47 comment "2001 DH47, also written as 2001 DH47, is a small asteroid orbiting near the L5 point of Mars (60 degrees behind Mars on its orbit).".
- (385571)_2004_UP10 comment "(7005385571000000000♠385571) 2004 UP10 (also written 2004 UP10) is a Neptune trojan discovered by Scott S. Sheppard and Chadwick A. Trujillo in 2004. It was the second such body to be discovered. It has the same orbital period as Neptune and orbits at the L4 Lagrangian point about 60 degrees ahead of Neptune.".
- (385695)_2005_TO74 comment "(7005385695000000000♠385695) 2005 TO74 (also written 2005 TO74) is the fourth Neptune trojan discovered. It orbits near Neptune's L4 Lagrangian point about 60 degrees ahead of Neptune and thus has the about same orbital period as Neptune. It was discovered by Scott S. Sheppard and Chadwick A. Trujillo in 2005.".
- (386454)_2008_XM comment "(386454) 2008 XM is an asteroid with a highly eccentric orbit that crosses the orbits of Mercury, Venus, Earth, and Mars. It has the third-smallest perihelion of any numbered asteroid behind (137924) 2000 BD19 and (374158) 2004 UL.".
- (386723)_2009_YE7 comment "(386723) 2009 YE7 is a trans-Neptunian object with an absolute magnitude (H) of 4.25. However, it only qualifies as a weak dwarf-planet candidate, since it is also suspected of being a highly reflective icy member of the Haumea family. It was discovered by David Rabinowitz on December 17, 2009 at the La Silla Observatory in Chile.".
- (388188)_2006_DP14 comment "2006 DP14 is a Near-Earth object that passed about 6.2 lunar distances from Earth on 10 February 2014. On the night of February 11, 2014 NASA scientists conducted a radar imaging session using the Goldstone 70 m (230 feet) dish. These observations revealed its basic shape and size; it appears to be about 400 × 200 m. Amateur and professional astronomers helped track the asteroid in the preceding days, so they would know just where to point the large antenna.".
- (391211)_2006_HZ51 comment "(391211) 2006 HZ51 is an 800 meter in diameter asteroid discovered on 27 April 2006 by the Catalina Sky Survey that with a 1.1 day observation arc was thought to have a 1 in 6 million chance of hitting Earth on 21 June 2008. Further refinement of the orbit quickly eliminated the risk. The preliminary orbit solution was at first thought to have a period of 7 years and a perihelion of ~1.1 AU. [MPEC 2006-H58, 28 April 2006, 2-day orbit].".
- (392741)_2012_SQ31 comment "(392741) 2012 SQ31, also known as 2004 PR107, 2009 YS20 and 2012 SQ31 is an asteroid in the asteroid belt with an absolute magnitude (H) of 17.8. It was discovered on August 11, 2004 by Cerro Tololo Inter-American Observatory, and then lost due to a lack of follow-up observations.With an observation arc of only 1 day (consisting of only 2 images), 2004 PR107 was thought to be a trans-Neptunian object with a semi-major axis (a) of 46 AU.".
- (394130)_2006_HY51 comment "(394130) 2006 HY51 is the asteroid with the third-smallest known perihelion of any known object orbiting the Sun. Its extreme orbital eccentricity brings it within 0.081 AU of the Sun (26% of Mercury's perihelion) and as far as 5.118 AU from the Sun (making it a Jupiter-grazer).".
- (39544)_1991_TN14 comment "The asteroid (39544) 1991 TN14 is a main belt asteroid discovered by Charles de Saint-Aignan at Lowell Observatory, examining films taken at Palomar.".
- (39797)_1997_TK18 comment "(39797) 1997 TK18 is a Jupiter Trojan minor planet, located in the L4 Lagrangian point. It was discovered through the Beijing Schmidt CCD Asteroid Program at the Xinglong Station in the Chinese province of Hebei on 3 October 1997.".
- (3S)-2,3-epoxy-2,3-dihydrosqualene_mutase comment "(3S)-2,3-epoxy-2,3-dihydrosqualene mutase may refer to: Thalianol synthase, an enzyme Protostadienol synthase, an enzyme Cucurbitadienol synthase, an enzyme Alpha-amyrin synthase, an enzyme Lupeol synthase, an enzyme Shionone synthase, an enzyme Parkeol synthase, an enzyme Achilleol B synthase, an enzyme Glutinol synthase, an enzyme Friedelin synthase, an enzyme Baccharis oxide synthase, an enzyme Alpha-seco-amyrin synthase, an enzyme Marneral synthase, an enzyme Beta-seco-amyrin synthase, an enzyme Delta-amyrin synthase, an enzyme Tirucalladienol synthase, an enzyme Baruol synthase, an enzyme".
- (40237)_1998_VM6 comment "(40237) 1998 VM6 is a Jupiter Trojan minor planet, located in the L4 Lagrangian point. It was discovered by Yoshisada Shimizu and Takeshi Urata at the Nachi-Katsuura Observatory in Nachikatsuura, Wakayama, Japan, on November 11, 1998.".
- (40314)_1999_KR16 comment "(40314) 1999 KR16, also written as (40314) 1999 KR16, is a trans-Neptunian object (TNO) that was discovered on May 16, 1999, by Audrey C. Delsanti and Oliver R. Hainaut at La Silla Observatory in Chile.".
- (4035)_1986_WD comment "(4035) 1986 WD is a Trojan asteroid approximately 70 kilometers in diameter. It completes a revolution around the Sun once every 12 years. It was discovered by Kenzo Suzuki and Takeshi Urata in Toyota, Japan on November 22, 1986. Alternate designations for it include 1973 SR4 and 1973 UF6.".
- (410777)_2009_FD comment "(410777) 2009 FD (also written as 2009 FD) is an Apollo asteroid (a class of near-Earth asteroid) with an orbit that places it at risk of a possible future collision with Earth. It has the highest impact threat on the Palermo Technical Impact Hazard Scale now that it is estimated to be 470 meters in diameter. 2009 FD was initially announced as discovered on 16 March 2009 by La Sagra Sky Survey.".
- (415029)_2011_UL21 comment "(415029) 2011 UL21 (former is 2011 UL21) is an Apollo class potentially hazardous asteroid (PHA) discovered on October 17, 2011 by the Catalina Sky Survey project. The asteroid is estimated to have a diameter of 2.5 kilometres (1.6 mi). It was rated at Torino Scale 1 on October 27, 2011 with an observation arc of 9.6 days. (415029) 2011 UL21 briefly had about a 1 in a million chance of impacting in 2029.".
- (415713)_1998_XX2 comment "(415713) 1998 XX2 is a small asteroid that is a Near-Earth object, a Potentially Hazardous Asteroid (PHA), and an Aten asteroid. This asteroid was discovered December 8, 1998, by Lincoln Near-Earth Asteroid Research (LINEAR), and was found to have frequent approaches to the Earth, Venus, and Mercury.".
- (416151)_2002_RQ25 comment "(416151) 2002 RQ25 is an Apollo asteroid and Near-Earth Object (NEO) that frequently makes close approaches to the Earth, Venus, and Mars. It was discovered on September 3, 2002 by CINEOS. On February 20, 2015, 2002 RQ25 will make a close approach of 0.05137 AU, peaking in brightness at 16.83 on February 14.".
- (417634)_2006_XG1 comment "(417634) 2006 XG1 (also written 2006 XG1) is a near-Earth asteroid that had a low but non-zero probability of impacting Earth on October 31, 2041. Originally listed with a Torino Scale hazard rating of 0, this was raised to a rating of 1 on December 22, 2006 as a result of additional observations and refinement of the orbital calculations. However, on January 9, 2007 it was returned to a rating of 0. It was removed from the Sentry Risk Table on February 7, 2007.".
- (420356)_2012_BX85 comment "(420356) 2012 BX85 is a trans-Neptunian object (TNO) and possibly a dwarf planet lying in the Kuiper Belt. It has the second lowest eccentricity of any TNO, after 2003 YN179. 2012 BX85 orbits near the 3:5 resonance to Neptune, but takes about 160 Neptune orbits (26,500 years) to make an orbit less than would be expected of an object in a true 3:5 resonance.".
- (42301)_2001_UR163 comment "(42301) 2001 UR163, also written as (42301) 2001 UR163, is likely a dwarf planet that resides in the scattered disc. It was discovered on October 21, 2001 by the Deep Ecliptic Survey (DES) program at Kitt Peak. Light-curve-amplitude analysis shows only small deviations, suggesting that 2001 UR163 is a spheroid with small albedo spots.".
- (42493)_1991_TG14 comment "The asteroid (42493) 1991 TG14 is a main belt asteroid discovered by Charles de Saint-Aignan at Lowell Observatory, examining films taken at Palomar.".
- (432949)_2012_HH2 comment "(432949) 2012 HH2 is a trans-Neptunian object (TNO) and weak dwarf planet candidate. It was discovered by T. Vorobjov from images taken on the night of April 19, 2012 at the Astronomical Research Observatory (H21). The object has been observed forty-two times over two oppositions. It is currently 29.8 AU from the Sun.".
- (433953)_1997_XR2 comment "(433953) 1997 XR2 (also written 1997 XR2) is an asteroid discovered on December 4, 1997.".
- (434326)_2004_JG6 comment "(434326) 2004 JG6 (also written 2004 JG6) is one of the closest orbiting objects to the Sun.It is the second known Apohele asteroid (the first being 163693 Atira), which means its entire orbit lies within that of the Earth. Its orbital period is less than that of Venus, making it one of the closest known objects to the Sun, after Mercury.2004 JG6 has an eccentric orbit that crosses the orbits of both Mercury and Venus.It was discovered by Brian A. Skiff of the LONEOS project.".
- (434620)_2005_VD comment "(434620) 2005 VD is a centaur and damocloid. It has the second most highly inclined orbit of any known object in the solar system, second to 2013 LA2. It was the most highly inclined known object between 2005 and 2013.".
- (436724)_2011_UW158 comment "(436724) 2011 UW158, provisionally known as 2011 UW158, is a near-Earth asteroid and potentially hazardous object. It was discovered in 2011 from the Pan-STARRS observatory at Haleakala, Hawaii, U.S.A.The asteroid was listed as level 1 in the Torino Scale on 4 November 2011, 9 days after its discovery, but was removed two weeks later.On July, 2015 it made a close approach to Earth, attracting the interest of astronomers.".
- (44594)_1999_OX3 comment "(44594) 1999 OX3 is a trans-Neptunian object with a centaur-like orbit.".
- (4489)_1988_AK comment "(4489) 1988 AK is a Jupiter trojan minor planet. It was discovered by Edward L. G. Bowell at Anderson Mesa on January 15, 1988.On December 18, 2012, 4489 has occulted the star TYC 2467-00054-1 over parts of the United States. 1988 AK's level of brightness equals magnitude 16.1 and the star's 11.1.Photometric observations of this asteroid during 2010 were used to build a light curve showing a rotation period of 12.582 ± 0.004 hours with a brightness variation of 0.22 ± 0.01 magnitude.".
- (4715)_1989_TS1 comment "(4715) 1989 TS1 is a Jupiter Trojan minor planet. It was discovered by Yoshiaki Oshima at the Gekko Observatory in Shizuoka Prefecture, Japan, on October 9, 1989.Photometric observations of this asteroid during 1991 were used to build a light curve showing a rotation period of 8.8129 ± 0.0025 hours with a brightness variation of 0.46 ± 0.01 magnitude.".
- (47171)_1999_TC36 comment "(47171) 1999 TC36 (also written: (47171) 1999 TC36) is a system comprising three trans-Neptunian objects (TNOs). It was discovered in 1999, by Eric P. Rubenstein and Louis-Gregory Strolger during an observing run at Kitt Peak National Observatory (KPNO). Dr. Rubenstein was searching images taken by Dr. Strolger as part of the Low-Z Supernova Search program.".
- (48438)_1989_WJ2 comment "(48438) 1989 WJ2 is a Jupiter Trojan minor planet, located in the L5 Lagrangian point. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on November 21, 1989.".
- (48639)_1995_TL8 comment "(48639) 1995 TL8 (also written (48639) 1995 TL8) is a classical Kuiper belt object possessing a relatively large satellite.The assumed diameter of 352 kilometres (219 mi) is derived from an albedo guess of 0.09, being typical for trans-Neptunian objects.".
- (4953)_1990_MU comment "(4953) 1990 MU is a large Earth-crossing asteroid (ECA) belonging to the Apollo family of asteroids which also cross the orbits of Mars and Venus. At approximately 3 km in diameter, it is one of the largest known ECAs. 1990 MU is the asteroid's temporary discovery name. It has now been assigned a permanent number from the Minor Planet Center (4953) indicating that its orbit has been confirmed, but has not (at least so far) been assigned a name.".
- (5025)_1986_TS6 comment "(5025) 1986 TS6 is a 58 km Jupiter Trojan with a potentially long 250 hour rotation period. It was discovered by Milan Antal at the Piwnice Obserwatorium Astronomiczne in on October 5, 1986.".
- (5119)_1988_RA1 comment "(5119) 1988 RA1 is a Jupiter Trojan minor planet. A part of the Trojan camp, it is orbiting at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 12.807 ± 0.016 hours with a brightness variation of 0.31 ± 0.01 magnitude.".
- (52747)_1998_HM151 comment "(52747) 1998 HM151, also written as (52747) 1998 HM151, is a cubewano. It has a perihelion (closest approach to the Sun) at 41.902 AU and an aphelion (farthest approach from the Sun) at 47.500 AU. It is 116 km in diameter. It was discovered on April 29, 1998, at the Mauna Kea Observatory, Hawaii.".
- (52760)_1998_ML14 comment "(52760) 1998 ML14 (also written (52760) 1998 ML14) is an as unnamed near-Earth and Mars-crosser asteroid. It was discovered by LINEAR in 1998. It is approximately 1.5 km in diameter.Shortly after its discovery, 1998 ML14 was imaged by radar at Goldstone and Arecibo.The study showed that the asteroid has a rotation period of 15 hours, and a shape that is roughly spherical, with some steep protrusions and large craters.On August 24, 2013 it passed at a distance of 21.9 Lunar distances.".
- (53319)_1999_JM8 comment "(53319) 1999 JM8 (also written (53319) 1999 JM8) is a near-Earth asteroid and Mars-crosser asteroid discovered by LINEAR. Radar imaging by Goldstone and Arecibo has revealed the asteroid to have an effective diameter of 7 km. Like the asteroid 4179 Toutatis, its rotation speed is unusually slow and possibly chaotic.It passed closer than 0.20 AU to the Earth five times in the last century (0.033 AU in 1990), but its closest approach in the 21st century will be in 2075 at 0.256 AU.".
- (53550)_2000_BF19 comment "The Earth-crossing asteroid (53550) 2000 BF19 was discovered on 28 January 2000. Its diameter is between 300 and 700 m. It will pass close to Earth in 2022, seven years before (99942) Apophis ; the risk of collision is minimal.".
- (5407)_1992_AX comment "(5407) 1992 AX is a Mars-crossing minor planet. It was discovered by Seiji Ueda and Hiroshi Kaneda in Kushiro, Hokkaidō, on January 4, 1992.".
- (5476)_1989_TO11 comment "(5476) 1989 TO11 is a Jupiter Trojan minor planet. It was discovered by Schelte J. Bus at the Cerro Tololo Inter-American Observatory in Chile, on October 2, 1989.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 5.780 ± 0.001 hours with a brightness variation of 0.30 ± 0.01 magnitude.".
- (5496)_1973_NA comment "(5496) 1973 NA is an Apollo-type near-Earth minor planet. It was discovered by Eleanor F. Helin at the Palomar Observatory in San Diego County, California, on July 4, 1973. This was two days after the asteroid had passed 0.07984 AU (11,944,000 km; 7,422,000 mi) from Earth. It was tracked for more than a month, but was not seen again until 1992 when it was recovered as 1992 OA by Siding Spring Observatory. It is one of the first near-Earth asteroids ever discovered.".
- (55565)_2002_AW197 comment "(55565) 2002 AW197 is a classical Kuiper belt object (cubewano). Measurements with the Spitzer Space Telescope have confirmed 2002 AW197 as a probable dwarf planet, although it has not been officially classified as such by the IAU. Light-curve-amplitude analysis shows only small deviations, which suggests that 2002 AW197 is a spheroid with small albedo spots. Tancredi (2010) accepts it as a dwarf planet.".
- (55636)_2002_TX300 comment "(55636) 2002 TX300 is a bright Kuiper belt object in the outer Solar System estimated to be about 286 kilometres (178 mi) in diameter.".
- (55637)_2002_UX25 comment "(55637) 2002 UX25 is a possible dwarf planet that orbits the Sun in the Kuiper belt beyond Neptune. Its orbit takes roughly 280 years, and it has one known moon. This moon makes it much easier to calculate mass, and when the size is known, also a density. The low density of about 0.82 g/cm3 has been a surprise to astronomers.It is a trans-Neptunian object with an absolute magnitude of 3.6, making it highly likely to be a dwarf planet.".
- (55638)_2002_VE95 comment "(55638) 2002 VE95, also written as 2002 VE95, is a trans-Neptunian object (TNO) with an absolute magnitude of 5.7. A 2:3 orbital resonance with Neptune makes it a plutino.".
- (5590)_1990_VA comment "(5590) 1990 VA is an Aten-type near-Earth minor planet. It was discovered by the Spacewatch project at the Kitt Peak National Observatory in Arizona on November 9, 1990.On September 29, 2067 it will pass about 0.004 AU (600,000 km; 370,000 mi) from Venus.".
- (5604)_1992_FE comment "(5604) 1992 FE is an Aten-type near-Earth minor planet. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Canberra, Australia, on March 26, 1992. The asteroid is 550 meters (1,800 ft) in diameter.The asteroid has a Venus minimum orbit intersection distance (Venus–MOID) of 0.0059 AU (880,000 km; 550,000 mi). On April 7, 2015 the asteroid will pass 0.00717 AU (1,073,000 km; 666,000 mi) from Venus.".
- (5645)_1990_SP comment "(5645) 1990 SP is an Apollo-type near-Earth minor planet. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Canberra, Australia, on September 20, 1990.Further observations of it was made by amateur astronomer Mohammed Alsunni of Sudan, that led to the refinement of its orbital calculations. (5645) 1990 SP makes close approaches to Mars and Earth. On 1969-Apr-14 the asteroid passed 0.0133 AU (1,990,000 km; 1,240,000 mi) from Mars.".
- (5646)_1990_TR comment "(5646) 1990 TR is an Amor-type near-Earth minor planet. It was discovered by Seiji Ueda and Hiroshi Kaneda in Kushiro, Hokkaidō, Japan, on October 11, 1990.It is a binary asteroid.".
- (5648)_1990_VU1 comment "(5648) 1990 VU1 is a Jupiter Trojan minor planet. It was discovered by Kin Endate and Kazuro Watanabe at the Kitami Observatory in Hokkaidō, Japan, on November 11, 1990.Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 37.56 ± 0.05 hours with a brightness variation of 0.20 ± 0.03 magnitude.".
- (58173)_1990_SS10 comment "(58173) 1990 SS10 is a main-belt minor planet. It was discovered by Henry E. Holt at the Palomar Observatory in San Diego County, California, on September 16, 1990.".
- (58295)_1994_JJ9 comment "The asteroid (58295) 1994 JJ9 is a main belt asteroid discovered by Charles de Saint-Aignan at Lowell Observatory, examining films taken at Palomar.".
- (5836)_1993_MF comment "(5836) 1993 MF is an Amor-type near-Earth minor planet. It was discovered by Eleanor F. Helin and Kenneth J. Lawrence at the Palomar Observatory in San Diego County, California, on June 22, 1993.With an absolute magnitude of 14.7, the asteroid is about 3–7 km in diameter. On 2023-Nov-28 the asteroid will pass 0.02535 AU (3,792,000 km; 2,356,000 mi) from Mars.".
- (59358)_1999_CL158 comment "(59358) 1999 CL158, also written as (59358) 1999 CL158, is a trans-Neptunian object that resides in the Kuiper belt. It was discovered on February 11, 1999, by Jane X. Luu, Chad Trujillo, and David C. Jewitt at the Mauna Kea Observatory, Hawaii.".
- (6002)_1988_RO comment "(6002) 1988 RO is a Jupiter Trojan minor planet. A part of the Trojan camp, it lies at the L5 Lagrangian point. It was discovered by Poul Jensen at the Brorfelde Observatory near Holbæk, Denmark, on September 8, 1988.Photometric observations of this asteroid during 1993 were used to build a light curve showing a rotation period of 12.918 ± 0.022 hours with a brightness variation of 0.18 ± 0.01 magnitude.".
- (6037)_1988_EG comment "(6037) 1988 EG is an Apollo-type near-Earth minor planet. It was discovered by Jeff T. Alu at the Palomar Observatory in San Diego County, California, on March 12, 1988. It is listed as a potentially hazardous object and also makes close approaches to Mars and Venus. With an absolute magnitude of 18.7, the asteroid is about 500–1100 meters in diameter. On 2041-Feb-27 the asteroid will pass 0.02437 AU (3,646,000 km; 2,265,000 mi) from Earth.".
- (60621)_2000_FE8 comment "(60621) 2000 FE8 is a scattered-disk object that resides in a distant, eccentric orbit that brings it 1.1 to 2.6 times farther than Neptune. This object is locked in a 2:5 orbital resonance with Neptune. It is known to have a single moon, S/2007 (60621) 1.".
- (6090)_1989_DJ comment "(6090) 1989 DJ is a Jupiter Trojan minor planet. A part of the Greek camp, it lies at the L4 Lagrangian point. It was discovered by Henri Debehogne at the La Silla Observatory in Chile on February 27, 1989.Photometric observations of this asteroid during 2009 were used to build a light curve showing a rotation period of 18.476 ± 0.007 hours with a brightness variation of 0.16 ± 0.01 magnitude.".
- (6178)_1986_DA comment "(6178) 1986 DA is a 2.3-kilometre-diameter M-type Mars-crosser and near-Earth asteroid, notable for being significantly more radar-reflective than other asteroids. It is an Amor asteroid, which means it approaches the orbit of Earth from the outside but does not cross it.Radar measurements suggest it is composed of nickel and iron and that it was derived from the center of a much larger object that experienced melting and differentiation.".
- (6265)_1985_TW3 comment "(6265) 1985 TW3 is a main-belt binary asteroid. It was discovered by T. F. Fric and Richard J. Gilbrech at the Palomar Observatory in San Diego County, California, on October 11, 1985. A moon was discovered orbiting the asteroid in 2007, separated by 8 km and orbiting once every 15 hours and 52 minutes.".
- (6382)_1988_EL comment "(6382) 1988 EL is an inner main-belt minor planet. It was discovered by Jeff T. Alu at the Palomar Observatory in San Diego County, California, on March 14, 1988.With an absolute magnitude of 13.7, the asteroid is about 5–11 km in diameter. The asteroid will pass 0.086 AU (12,900,000 km; 8,000,000 mi) from Mars on 2042-Apr-13 and 0.092 AU (13,800,000 km; 8,600,000 mi) from Mars on 2113-Oct-03.".
- (6491)_1991_OA comment "(6491) 1991 OA is an Amor-type near-Earth minor planet. It was discovered by Henry E. Holt at the Palomar Observatory in San Diego County, California, on July 16, 1991. It is listed as a potentially hazardous object.On 2086-Aug-01 it will pass about 0.09 AU (13,000,000 km; 8,400,000 mi) from the Earth.".
- (65407)_2002_RP120 comment "(65407) 2002 RP120 (also written (65407) 2002 RP120) is a damocloid, which means it is also a member of a small group of retrograde minor planets. Aside from being a damocloid, it is also a scattered-disc object – a trans-Neptunian object with a very eccentric orbit, probably ejected from the ecliptic by Neptune.".
- (66063)_1998_RO1 comment "(66063) 1998 RO1 is an Aten asteroid with a very eccentric orbit that was discovered September 14, 1998, by the LINEAR program. It is known to have a moon, S/2001 (66063) 1.".
- (66391)_1999_KW4 comment "(66391) 1999 KW4 (also written (66391) 1999 KW4) is an Aten and Mercury-crossing binary asteroid discovered by LINEAR in 1999.1999 KW4 has a moon orbiting it. The moon, designated S/2001 (66391) 1 or "1999 KW4 Beta", is ~360 m in diameter, and orbits 1999 KW4 'Alpha' in 0.758 d (16 hours) at a distance of 2.6 km.".
- (68950)_2002_QF15 comment "(68950) 2002 QF15 (also written (68950) 2002 QF15) is a near-Earth object that will come as near as 7.5 Gm (.05 AU) to the Earth on May 18, 2044. It is classed as a potentially dangerous asteroid.".
- (6940)_1972_HL1 comment "(6940) 1972 HL 1 is an asteroid discovered in April 19, 1972, of the Chilean Astronomer Carlos Torres in the Cerro El Roble Observatory in Chile. According to its absolute magnitude of 14.7, its diameter can be roughly estimated between 3 and 7 km.".
- (69437)_1996_KW2 comment "(69437) 1996 KW2 is a Jupiter Trojan minor planet, located in the L5 Lagrangian point. It was discovered through the Beijing Schmidt CCD Asteroid Program at the Xinglong Station in the Chinese province of Hebei on May 21, 1996.".
- (69986)_1998_WW24 comment "(69986) 1998 WW24, also written as (69986) 1998 WW24, is a Trans-Neptunian object that resides in the Kuiper Belt. Since it is in a 2:3 orbital resonance with the planet Neptune, it is classified as a plutino.It was discovered on November 18, 1998, by Marc W. Buie at the Kitt Peak National Observatory.".
- (69987)_1998_WA25 comment "(69987) 1998 WA25, also written as (69987) 1998 WA25, is a cubewano. It has a perihelion (closest approach to the Sun) at 41.457 AU and an aphelion (farthest approach from the Sun) at 43.217 AU. It is about 160 km in diameter. It was discovered on November 19, 1998, by Marc W. Buie.".
- (69988)_1998_WA31 comment "(69988) 1998 WA31, also written as (69988) 1998 WA31, is a trans-Neptunian object that resides in the Kuiper belt. It was discovered on 18 November 1998 by Marc W. Buie at the Kitt Peak National Observatory.It is in a 2:5 orbital resonance with the planet Neptune.".
- (69990)_1998_WU31 comment "(69990) 1998 WU31, also written as (69990) 1998 WU31 is a TNO that resides in the Kuiper belt. It was discovered on November 18, 1998, by Marc W. Buie at Kitt Peak National ObservatorySince it is in a 2:3 orbital resonance with the planet Neptune, it has been classified as a plutino.".
- (6S)-6-Fluoroshikimic_acid comment "(6S)-6-Fluoroshikimic acid is an antibacterial agent acting on the aromatic biosynthetic pathway. It may be used against Plasmodium falciparum, the causative agent of malaria. The molecule is targeting the enzymes of the shikimate pathway. This metabolic pathway is not present in mammals.".
- (718)_Live_Farewell_Extravaganza comment "(718) Live Farewell Extravaganza is the CD complement of 2 Skinnee J's DVD of the same name.".
- (7335)_1989_JA comment "(7335) 1989 JA is a near-Earth minor planet in the Apollo group; it is listed as a potentially hazardous object. It was discovered by Eleanor F. Helin at the Palomar Observatory in San Diego County, California, on May 1, 1989. It is approximately 1.8 kilometres (1.1 mi) in diameter.".
- (7341)_1991_VK comment "(7341) 1991 VK is a near-Earth minor planet in the Apollo group. It was discovered by Eleanor F. Helin and Kenneth J. Lawrence at the Palomar Observatory in San Diego County, California, on November 1, 1991. It is listed as a potentially hazardous object. Every 5 years (from 1946 through 2091) the asteroid makes a close approach to the Earth. The next close approach to the Earth will be on 2017-Jan-25 at a distance of 0.0647091 AU (9,680,340 km; 6,015,090 mi).".
- (7352)_1994_CO comment "(7352) 1994 CO is a Jupiter Trojan minor planet, located in the L5 Lagrangian point. It was discovered by Seiji Ueda and Hiroshi Kaneda in Kushiro, Hokkaidō, Japan, on February 4, 1994. It takes 648 hours to rotate.".
- (7474)_1992_TC comment "7474 (1992 TC) is a moderate sized M-type asteroid discovered by Robert H. McNaught in 1992. It is notably one of a few similar M-type asteroids, including the named asteroids 4660 Nereus and 65803 Didymos, which can be reached easily by spacecraft from Earth. The delta-V required to reach 7474 (1992 TC) would be about 5.6 kilometres per second (3.5 mi/s), which is less than is needed to reach the moon.".
- (7482)_1994_PC1 comment "(7482) 1994 PC1 is a near-Earth minor planet in the Apollo group. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on August 9, 1994. It is listed as a potentially hazardous object with a well determined orbit. With an absolute magnitude (H) of 16.8, the asteroid is estimated to be 1–2.5 km in diameter.On 1933-Jan-17 it passed 0.00752 AU (1,125,000 km; 699,000 mi) from Earth.".
- (7641)_1986_TT6 comment "(7641) 1986 TT6 is a Jupiter Trojan asteroid in the Greek camp (L4 Lagrangian Point). It was discovered on October 5, 1986, at the Piwince Observatory by Milan Antal.".
- (78799)_2002_XW93 comment "(78799) 2002 XW93 is a trans-Neptunian object discovered by the Palomar observatory on December 10, 2002. Michael Brown lists it as a likely dwarf planet on his website. It most recently reached perihelion on August 10, 1926. Prior to its discovery, it was observed 29 times between December 17, 1989, and September 20, 2008.".
- (7888)_1993_UC comment "(7888) 1993 UC is a near-Earth minor planet in the Apollo group. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on October 20, 1993. The asteroid has an observation arc of 23 years and has a well determined orbit. Its estimated size is 2.3 to 5.2 km.On March 20, 2013, the asteroid passed 49 lunar distances or 0.12598 AU (18,846,000 km; 11,711,000 mi) from Earth at a relative velocity of 21.8 km/s (49,000 mph).".
- (7949)_1992_SU comment "(7949) 1992 SU is a main-belt minor planet, approximately 18.45 kilometres (11.46 mi) in diameter. It was discovered by Eleanor F. Helin at the Palomar Observatory in San Diego County, California, on September 23, 1992.".
- (79969)_1999_CP133 comment "(79969) 1999 CP133, also written as (79969) 1999 CP133, is a trans-Neptunian object. It was discovered on 11 February 1999 by Chad Trujillo, Jane X. Luu, and David C. Jewitt at the Mauna Kea Observatory, Hawaii.It is in a 4:5 orbital resonance with the planet Neptune.".
- (79978)_1999_CC158 comment "(79978) 1999 CC158, also written as (79978) 1999 CC158, is a trans-Neptunian object orbiting in the Kuiper belt of the Solar System. It was discovered on 15 February 1999 at the Mauna Kea Observatory, Hawaii. It has a 5:12 resonance with Neptune.".
- (79983)_1999_DF9 comment "(79983) 1999 DF9, also written as (79983) 1999 DF9, is a cubewano. It travels in a highly eccentric orbit which has a perihelion (closest approach to the Sun) at 39.797 AU and an aphelion (farthest approach from the Sun) at 53.264 AU. It is about 265 km in diameter. It was discovered on February 20, 1999, by Jane X. Luu, Chadwick A. Trujillo and David C. Jewitt.Due to its small size, it is unlikely to be classified as a dwarf planet.".
- (8014)_1990_MF comment "(8014) 1990 MF is a near-Earth minor planet in the Apollo group. It was discovered by Eleanor F. Helin at the Palomar Observatory in San Diego County, California, on June 26, 1990. This object is approximately 0.7 kilometres (0.43 mi) in diameter, and listed as a potentially hazardous object. On July 23, 2020, it will come within 0.055 au of the Earth—about 21.3 times the Moon's distance.".
- (8035)_1992_TB comment "(8035) 1992 TB is an Apollo asteroid, a type of Near-Earth Object. It is also a Venus-crosser and a Mars-crosser, although it doesn't make close approaches to Mars.".
- (8148)_1985_CR2 comment "(8148) 1985 CR2 is a main-belt minor planet. It was discovered by Henri Debehogne at the La Silla Observatory in Chile on February 15, 1985.".