Matches in DBpedia 2015-10 for { ?s <http://www.w3.org/2000/01/rdf-schema#comment> ?o }
- (153591)_2001_SN263 comment "(153591) 2001 SN263 is a small near-Earth asteroid discovered by the LINEAR project in 2001. In 2008, scientists using the planetary radar at Arecibo Observatory discovered that the object is orbited by two satellites, when the triple asteroid made a close approach to Earth of 0.066 AU (nearly 10 million kilometers).".
- (153814)_2001_WN5 comment "(153814) 2001 WN5 is a near-Earth Asteroid belonging to the Apollo family. It was first discovered by the LONEOS Project at Anderson Mesa on November 20, 2001, and was later classified as a Potentially Hazardous Asteroid (PHA). It was removed from the Sentry Risk Table on January 30, 2002. There are precovery images dating back to February 10, 1996. The orbit is well determined with an observation arc of 14.9 years using two radar delay observations, and has an Uncertainty Parameter of 0.".
- (15430)_1998_UR31 comment "(15430) 1998 UR31 is a main-belt binary asteroid. It was discovered through the Beijing Schmidt CCD Asteroid Program at the Xinglong Station in the Chinese province of Hebei on October 22, 1998. A moon was discovered orbiting the asteroid in 2010. The moon has an orbital period of almost exactly a day, and is tidally locked with the asteroid.".
- (15760)_1992_QB1 comment "(15760) 1992 QB1, also written (15760) 1992 QB1, was the first trans-Neptunian object to be discovered after Pluto and Charon. It was discovered in 1992 by David C. Jewitt and Jane X. Luu at the Mauna Kea Observatory, Hawaii. It is a classical Kuiper belt object and gave rise to the name cubewano for this kind of object, after the "QB1" portion of its designation. Decoding its provisional designation, "QB1" reveals that it was the 27th object found in the second half of August of that year.".
- (15788)_1993_SB comment "(15788) 1993 SB is a trans-Neptunian object of the plutino class. Apart from Pluto, it was one of the first such objects discovered (beaten by two days by (385185) 1993 RO and by one day by 1993 RP), and the first to have an orbit calculated well enough to receive a number. The discovery was made in 1993 at the La Palma Observatory with the Isaac Newton Telescope.Very little is known about the object. Even the diameter estimate of ~130 km is based on an assumed albedo of 0.09.".
- (15789)_1993_SC comment "(15789) 1993 SC is a trans-Neptunian object of the plutino class. The discovery was made in 1993 at the La Palma Observatory with the Isaac Newton Telescope. It was the second plutino to receive an MPC number.".
- (15807)_1994_GV9 comment "(15807) 1994 GV9, also written (15807) 1994 GV9, is a trans-Neptunian object of the cubewano class.It was discovered on April 15, 1994, by David C. Jewitt and Jun Chen at the Observatories at Mauna Kea near Hilo, Hawaii. Very little is known about the object.(15807) 1994 GV9 is the second cubewano to be given an official Minor Planet Center catalog number. The first cubewano is (15760) 1992 QB1.".
- (15809)_1994_JS comment "(15809) 1994 JS is a trans-Neptunian object that resides in the Kuiper belt beyond Pluto. It is in a 3:5 orbital resonance with Neptune.".
- (15810)_1994_JR1 comment "(15810) 1994 JR1, also written (15810) 1994 JR1, is a minor planet that moves around the Sun in an orbit entirely located beyond Neptune. It is the first object that was confirmed to be a quasi-satellite of Pluto.".
- (15820)_1994_TB comment "(15820) 1994 TB is a trans-Neptunian object residing in the Kuiper belt. It is in a 3:2 orbital resonance with Neptune similar to Pluto. It was discovered on October 2, 1994, by David C. Jewitt and Jun Chen at the Mauna Kea Observatory, Hawaii.".
- (15836)_1995_DA2 comment "(15836) 1995 DA2, also written as (15836) 1995 DA2, is a trans-Neptunian object. It was discovered on February 24, 1995, by David C. Jewitt and Jane X. Luu at the Mauna Kea Observatory, Hawaii.".
- (15874)_1996_TL66 comment "(15874) 1996 TL66 (also written (15874) 1996 TL66) is a trans-Neptunian object (TNO) that resides in the scattered disc. The Spitzer Space Telescope has estimated this object to be about 575 kilometres (357 mi) in diameter, but 2012 estimates from the Herschel Space Observatory estimate the diameter as closer to 339 kilometres (211 mi). It is not a detached object, since its perihelion (closest approach to the Sun) is under the influence of Neptune.".
- (15875)_1996_TP66 comment "(15875) 1996 TP66, also written as (15875) 1996 TP66, is a resonant trans-Neptunian object in 2:3 resonance with Neptune, like Pluto (plutino). It was discovered on 11 October 1996 by Chad Trujillo, David C. Jewitt, and Jane X. Luu at the Mauna Kea Observatory, Hawaii.".
- (15883)_1997_CR29 comment "(15883) 1997 CR29, also written as (15883) 1997 CR29, is a trans-Neptunian object. It was discovered on February 3, 1997, by Chad Trujillo, Jun Chen, and David C. Jewitt at the Mauna Kea Observatory, Hawaii.".
- (162173)_1999_JU3 comment "(162173) 1999 JU3 is an Apollo asteroid. It is planned that the Japanese space probe Hayabusa 2 returns samples from this asteroid by December 2020. It is the rare spectral type Cg, having qualities of both a C-type asteroid and a G-type asteroid.".
- (163132)_2002_CU11 comment "(163132) 2002 CU11, provisionally known as 2002 CU11, is a near-Earth asteroid and potentially hazardous object. It was discovered on 7 February 2002 by Lincoln Near-Earth Asteroid Research (LINEAR) at an apparent magnitude of 19 using a 1.0-meter (39 in) reflecting telescope. It has an estimated diameter of 730 meters (2,400 ft).".
- (163189)_2002_EU6 comment "(163189) 2002 EU6 is a Jupiter Trojan minor planet, located in the L4 Lagrangian point. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on March 6, 2002.".
- (163249)_2002_GT comment "(163249) 2002 GT is an Apollo asteroid with an absolute magnitude of 18.26. It is a potentially hazardous asteroid as its orbit crosses that of Earth.In 2011, NASA considered sending the unmanned spacecraft Deep Impact toward the asteroid with the aim of performing a flyby in 2020.".
- (163364)_2002_OD20 comment "(163364) 2002 OD20 is a near-Earth object that is classified as a potentially hazardous asteroid (PHA). It was scheduled to be observed by Goldstone radar in May 2013. It has a well determined orbit and will make a close approach to Earth on 23 May 2013, at a distance of 0.0387 AU (5,790,000 km; 3,600,000 mi). It is due to make another close pass on 23 May 2131, coming as close as 0.0248 AU. It was discoverded on 21 July 2002 by Near-Earth Asteroid Tracking (NEAT).".
- (164207)_2004_GU9 comment "(164207) 2004 GU9 is a small near-Earth asteroid in the Apollo asteroid family. It will be a quasi-satellite of Earth until around 2600.On 14 April 2004 (with less than a 1-day observation arc), the Sentry Risk Table showed 180 virtual impactors. It was removed from the Sentry Risk Table 2 days later on 16 April 2004. 2004 GU9 now has a well determined orbit with an observation arc of 12 years.".
- (16684)_1994_JQ1 comment "(16684) 1994 JQ1, also written as (16684) 1994 JQ1, is a trans-Neptunian object of the cubewano class. It was discovered on May 11, 1994, by Michael J. Irwin and Anna N. Zytkow.(16684) 1994 JQ1 is the third cubewano to be given an official Minor Planet Center catalog number. The first two official cubewanos are (15760) 1992 QB1 and (15807) 1994 GV9.".
- (17246)_2000_GL74 comment "(17246) 2000 GL74 is a main belt asteroid. It was discovered by the LINEAR program on April 5, 2000. It is known to possess a moon: S/2004 (17246) 1.".
- (175113)_2004_PF115 comment "(175113) 2004 PF115 (also written 2004 PF115) is a trans-Neptunian object (TNO). It was discovered in 2006 by M. Brown, C. Trujillo, D. Rabinowitz. The object is a plutino (in 2:3 resonance with Neptune).".
- (175706)_1996_FG3 comment "(175706) 1996 FG3 is a near-Earth binary asteroid in the Apollo group. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on March 24, 1996. It is listed as a potentially hazardous object. A moon was discovered orbiting the asteroid in 1998.".
- (177049)_2003_EE16 comment "(177049) 2003 EE16, provisionally known as 2003 EE16, is a near-Earth asteroid and potentially hazardous object. It was discovered on 8 March 2003 by LPL/Spacewatch II at an apparent magnitude of 20 using a 1.8-meter (71 in) reflecting telescope. It has an estimated diameter of 320 meters (1,050 ft).".
- (179806)_2002_TD66 comment "2002 TD66 (also written 2002 TD66) is a near-Earth asteroid, discovered on October 5, 2002, by the LINEAR project. It was announced on October 7, 2002, and appeared later that day on the JPL current risk page.Due to the proximity of its orbit to Earth and its estimated size, this object has been classified as a potentially hazardous asteroid (PHA) by the Minor Planet Center in Cambridge, Massachusetts. In November 2006 there were 823 PHAs known. As of October 2011, there are 1261 PHAs known.".
- (181708)_1993_FW comment "(181708) 1993 FW was the second trans-Neptunian object to be discovered after Pluto and Charon. It was discovered in 1993 by David C. Jewitt and Jane X. Luu at the Mauna Kea Observatory, Hawaii. Mike Brown lists it as possibly a dwarf planet on his website.".
- (181902)_1999_RD215 comment "(181902) 1999 RD215 is a scattered disc object with a diameter of about 175 kilometers (110 miles.) It was discovered on September 6, 1999, by Chad Trujillo, Jane Luu, and David Jewitt. The orbit of the asteroid regularly takes it from the center of the Kuiper belt to well beyond, into the Scattered disc.".
- (182294)_2001_KU76 comment "(182294) 2001 KU76, provisionally known as 2001 KU76, is a trans-Neptunian object (TNO) that has a 6:11 resonance with Neptune. This is the same resonance that dwarf planet Makemake is either near or in.It will come to perihelion in 2021.Assuming a generic TNO albedo of 0.09, it is about 211 km in diameter. The assumed diameter of this object makes it a possible dwarf planet.".
- (18412)_1993_LX comment "(18412) 1993 LX is a main-belt minor planet. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on June 13, 1993.In 2012, Asteroid 18412 was named in honour of Dr Karl Kruszelnicki, an Australian Science Broadcaster and author.".
- (18413)_1993_LD1 comment "(18413) 1993 LD1 is a main-belt minor planet. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on June 13, 1993.In 2012, Asteroid 18413 was named in honour of Adam Spencer, an Australian broadcaster, mathematician and stand up comedian.".
- (184212)_2004_PB112 comment "(184212) 2004 PB112, also written as 2004 PB112, is a scattered-disc object with a semi-major axis of about 110 AU.2004 PB112 reached perihelion on 2011-10-05 (JD 2455839.806).".
- (185105)_2006_SV23 comment "2006 SV23 is a Ceres trojan asteroid discovered in 2006.".
- (185851)_2000_DP107 comment "2000 DP107 is a near-Earth asteroid that is notable because it provided evidence for binary asteroids in the near-Earth population.".
- (19255)_1994_VK8 comment "(19255) 1994 VK8, also written as (19255) 1994 VK8, is a trans-Neptunian object (TNO) of the cubewano class. It was discovered on November 8, 1994, by Alan Fitzsimmons, Donal O'Ceallaigh, and Iwan P. Williams.(19255) 1994 VK8 is the fourth cubewano to be given an official Minor Planet Center catalog number. The first three official cubewanos are (15760) 1992 QB1, (15807) 1994 GV9, and (16684) 1994 JQ1.".
- (192642)_1999_RD32 comment "(192642) 1999 RD32, provisionally known as 1999 RD32, is a near-Earth asteroid and potentially hazardous object. It was discovered on 8 September 1999 by Lincoln Near-Earth Asteroid Research (LINEAR) at an apparent magnitude of 18 using a 1.0-meter (39 in) reflecting telescope.With two precovery images from January 1995, the asteroid has a very well determined orbit with an observation arc of 17 years.".
- (19299)_1996_SZ4 comment "(19299) 1996 SZ4 (also written (19299) 1996 SZ4) is a trans-Neptunian object (TNO) that resides in the Kuiper belt. It is in a 3:2 orbital resonance with Neptune similar to Pluto.".
- (19308)_1996_TO66 comment "(19308) 1996 TO66 (also written (19308) 1996 TO66) is a trans-Neptunian object that was discovered in 1996 by Chadwick Trujillo, David Jewitt and Jane Luu.".
- (196256)_2003_EH1 comment "(196256) 2003 EH1 is a small Solar System body discovered in March 2003. Peter Jenniskens (2003–2004) proposed that it is the parent body of the Quadrantid meteor shower. 2003 EH1 is likely an extinct comet and may even be related to the comet C/1490 Y1. 2003 EH1 came to perihelion on 12 March 2014.".
- (2,3,7)_triangle_group comment "In the theory of Riemann surfaces and hyperbolic geometry, the triangle group (2,3,7) is particularly important.".
- (2,4,6-Trimethylphenyl)gold comment "(2,4,6-Trimethylphenyl)gold is a member of a special group of compounds where an aryl carbon atom acts as a bridge between two gold atoms. This compound is formed in a reaction between Au(CO)Cl and mesityl Grignard. It crystallizes as a cyclical pentamer.".
- (2-Chlorophenyl)thiourea comment "(2-Chlorophenyl)thiourea is a chemical compound used as an herbicide. As of 1998, the Environmental Protection Agency did not have it registered as a pesticide in the United States.".
- (20026)_1992_EP11 comment "(20026) 1992 EP11 is an asteroid in the asteroid belt that was discovered by UESAC on March 6, 1992 at La Silla Observatory.It has an orbital eccentricity of 0.03500560 and an orbital inclination of 2.72994°.".
- (202421)_2005_UQ513 comment "(202421) 2005 UQ513, also written as 2005 UQ513, is a cubewano with an absolute magnitude of 3.4. Mike Brown's website lists it as a highly likely dwarf planet. 2005 UQ513 shows signs of weak water ice. Like Quaoar, it has a very red spectrum, which indicates that its surface probably contains a lot of complex, processed organic molecules. Its light curve shows variations of Δm=0.3 mag, but no period has been determined.".
- (208996)_2003_AZ84 comment "(208996) 2003 AZ84, also written as 2003 AZ84, is a plutino, like Pluto, in a 2:3 resonance with Neptune. Its light-curve amplitude deviates little from that of an ellipsoid, which suggests that it is likely one with small albedo spots. Tancredi (2010) considers 2003 AZ84 to very probably be a dwarf planet, although the International Astronomical Union does not currently classify it as such. It was discovered on January 13, 2003 by C. Trujillo and M.".
- (21083)_1991_TH14 comment "The asteroid (21083) 1991 TH14 is a main belt asteroid discovered by Charles de Saint-Aignan at Lowell Observatory, examining films taken at Palomar.".
- (214869)_2007_PA8 comment "(214869) 2007 PA8 is an asteroid roughly 1.6 km in diameter and that came within 6.5 million km (4 million miles, 17 lunar distances) to Earth on November 5, 2012. It was discovered on August 9, 2007 by LINEAR. It was studied by the Goldstone radar as it came near Earth, which resulted in images and other data about the asteroid, such as its rotation rate.".
- (225088)_2007_OR10 comment "(225088) 2007 OR10 is a very large planetoid located in the scattered disc. It is the largest known body in the Solar System without a name. It is approximately the size of Makemake and Haumea, and appears to be a dwarf planet.".
- (225312)_1996_XB27 comment "1996 XB27, also written as 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.".
- (229762)_2007_UK126 comment "(229762) 2007 UK126, also written as (229762) 2007 UK126, is a scattered disc object (SDO) with a bright absolute magnitude of 3.7. This makes it probably a dwarf planet. As of August 2011, Mike Brown lists it as highly likely a dwarf planet. Its light-curve amplitude is estimated to be Δm=0.111 mag.Its orbital eccentricity of 0.49 suggests that it was gravitationally scattered onto its eccentric orbit.".
- (230965)_2004_XA192 comment "(230965) 2004 XA192 is a Kuiper-belt object with a diameter of 7005339000000000000♠339+120−95 km. It has an absolute magnitude of 4.11. It was discovered on 12 December 2004 at Palomar Observatory.It is currently at 35.8 AU from the Sun, near its perihelion.".
- (23624)_1996_UX3 comment "(23624) 1996 UX3 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 October 29, 1996.".
- (237442)_1999_TA10 comment "(237442) 1999 TA10, provisionally known as 1999 TA10, is a near-Earth object (NEO) from the Amor asteroid group. It is suspected of being an inner fragment of the differentiated asteroid 4 Vesta.Given an absolute magnitude (H) of 17.9, and that the albedo is unknown, this NEO could vary from 500 to 1500 meters in diameter.1999 TA10 was discovered on 5 October 1999 at apparent magnitude 17.7, when it was only 0.39 AU from Earth. In 2010, it came within 0.3 AU of Earth.".
- (242450)_2004_QY2 comment "(242450) 2004 QY2 is a large near-Earth asteroid and potentially hazardous object. It has a well determined orbit with an observation arc of 7 years and an uncertainty parameter of 0. It was discovered on 20 August 2004 by the Siding Spring Survey at an apparent magnitude of 16.5 using the 0.5-metre (20 in) Uppsala Southern Schmidt Telescope.Based on an absolute magnitude of 15, the asteroid has an estimated diameter of 3.5 to 7.7 km.".
- (24835)_1995_SM55 comment "(24835) 1995 SM55, also written (24835) 1995 SM55, is a trans-Neptunian object (TNO) that resides in the Kuiper belt that was discovered on September 19, 1995, by Nichole M. Danzl.".
- (248835)_2006_SX368 comment "(248835) 2006 SX368 /əˈkɪroʊ.iː/, also known as 2006 SX368, is a centaur orbiting in the outer Solar System between Saturn and Neptune. It was discovered on September 16, 2006 by Andrew Becker, Andrew Puckett and Jeremy Kubica at Apache Point Observatory in Sunspot, New Mexico.".
- (24952)_1997_QJ4 comment "(24952) 1997 QJ4, also written as 1997 QJ4, is a plutino and as such it is trapped in a 2:3 mean-motion resonance with Neptune. It was discovered on 28 August 1997 by Jane X. Luu, Chad Trujillo, David C. Jewitt and K. Berney. This object has a perihelion (closest approach to the Sun) at 30.463 AU and an aphelion (farthest approach from the Sun) at 48.038 AU, so it moves in a relatively eccentric orbit (0.224).".
- (24978)_1998_HJ151 comment "(24978) 1998 HJ151, also written as (24978) 1998 HJ151, is a cubewano. It has a perihelion (closest approach to the Sun) at 41.339 AU and an aphelion (farthest approach to the Sun) at 45.889 AU. It has a diameter of about 139 km. It was discovered on April 28, 1998, by Jane X. Luu, Chadwick A. Trujillo, David J. Tholen and David C. Jewitt.".
- (251732)_1998_HG49 comment "1998 HG49, also written as 1998 HG49, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach to Earth is more than 0.14 AU.".
- (26181)_1996_GQ21 comment "(26181) 1996 GQ21, also written as (26181) 1996 GQ21, is a trans-Neptunian object (TNO) that resides in the scattered disc region of the Solar System. It was discovered on 12 April 1996 by Nichole M. Danzl.".
- (26308)_1998_SM165 comment "(26308) 1998 SM165, also written as (26308) 1998 SM165, is a binary trans-Neptunian object (TNO) that resides in the Kuiper belt. It was discovered on September 16, 1998, by Nichole Danzl. It is in a 1:2 orbital resonance with the planet Neptune.".
- (26375)_1999_DE9 comment "(26375) 1999 DE9 (also written (26375) 1999 DE9) is a trans-Neptunian object. Light-curve-amplitude analysis shows only small deviations, suggesting 1999 DE9 is a spheroid with small albedo spots. Measurements by the Spitzer Space Telescope estimate that it is 461 ± 45 km in diameter. It was discovered in 1999 by Chad Trujillo and Jane X. Luu. It is possibly a dwarf planet.1999 DE9 orbit is in 2:5 resonance with Neptune's. Spectral analysis has shown traces of ice.".
- (276033)_2002_AJ129 comment "(276033) 2002 AJ129, also written as 2002 AJ129, is a Mercury-crossing asteroid. It has the fourth-smallest perihelion of all numbered asteroids, after (137924) 2000 BD19, (374158) 2004 UL, and (386454) 2008 XM.It is classified as an Apollo asteroid because it is a near-Earth asteroid with a semi-major axis larger than Earth's.".
- (277475)_2005_WK4 comment "(277475) 2005 WK4 is a near-Earth asteroid that passed within 8.2 Lunar distances on August 8, 2013. It was radar-imaged by the Deep Space Network dish at Goldstone, USA. The asteroid is between 660 and 980 feet (200 and 300 meters) in diameter, and rotated 2.5 times in 6.5 hours. It had been observed by the Arecibo radar in July 2012 (this was not a close approach though), and is also classified as a Potentially Hazardous Object (PHA).".
- (277810)_2006_FV35 comment "(277810) 2006 FV35 is a small near-Earth asteroid in the Apollo asteroid family. It is a quasi-satellite of Earth. It is also notable for having a low delta-v requirement for rendezvous. Although its orbital period is almost exactly 1 year, the orbit of 2006 FV35 has a high eccentricity which causes it to cross the paths of both Venus and Mars.".
- (278361)_2007_JJ43 comment "(268361) 2007 JJ43 is a trans-Neptunian object (TNO) orbiting the Sun near the outer edge of the Kuiper belt. Based on how bright it appears, it is a possible dwarf planet.Its discovery images were taken in 2007, and its absolute magnitude of 4.4 is one of the twenty brightest exhibited by TNOs. Assuming it has a typical albedo, this would make it roughly the same size as Ixion (about 650–800 km diameter).".
- (27981)_1997_UK21 comment "(27981) 1997 UK21 is a main-belt minor planet. It was discovered through the Beijing Schmidt CCD Asteroid Program at the Xinglong Station in the Chinese province of Hebei on October 20, 1997. It is usually about 2.72 AU away from Earth and has an orbital period of 14.6 Julian years.".
- (280244)_2002_WP11 comment "(280244) 2002 WP11 is an asteroid, discovered on November 27, 2002 by CINEOS.".
- (285263)_1998_QE2 comment "(285263) 1998 QE2 is a near-Earth asteroid 2.75 kilometers (1.71 mi) in diameter. It was discovered on August 19, 1998, by the Lincoln Near Earth Asteroid Research (LINEAR) program located near Socorro, New Mexico. 1998 QE2 has an observation arc of 14 years and a well-determined orbit.".
- (29075)_1950_DA comment "(29075) 1950 DA is a near-Earth asteroid. Among asteroids more than 1 km in diameter, it is notable for having the highest known probability of impacting Earth. In 2002, it had the highest Palermo rating with a value of 0.17 for a possible collision in 2880. In 2013, the odds of an Earth impact in 2880 were estimated as 1 in 4,000 (0.025%) with a Palermo rating of −0.83. In 2014, the odds of an Earth impact were further reduced to only 1 in 20,000 (0.005%) with a Palermo rating of −1.81.".
- (292220)_2006_SU49 comment "(292220) 2006 SU49 (also written 2006 SU49) is a near-Earth asteroid that had a 1 in 42000 chance of impacting Earth on January 22, 2029. By October 29, 2006, it was listed with a Torino Scale impact risk value of 0. It was removed from the Sentry Risk Table on November 23, 2006.".
- (2E,6E)-farnesyl-diphosphate:isopentenyl-diphosphate_farnesyltranstransferase comment "(2E,6E)-farnesyl-diphosphate:isopentenyl-diphosphate farnesyltranstransferase may refer to: Hexaprenyl-diphosphate synthase ((2E,6E)-farnesyl-diphosphate specific), an enzyme All-trans-octaprenyl-diphosphate synthase, an enzyme All-trans-decaprenyl-diphosphate synthase, an enzyme".
- (2E,6E)-farnesyl-diphosphate_diphosphate-lyase comment "(2E,6E)-farnesyl-diphosphate diphosphate-lyase may refer to:Enzymes".
- (2Z,6E)-farnesyl-diphosphate_diphosphate-lyase comment "(2Z,6E)-farnesyl-diphosphate diphosphate-lyase may refer to: (-)-gamma-cadinene synthase ((2Z,6E)-farnesyl diphosphate cyclizing), an enzyme Alpha-guaiene synthase, an enzyme 5-epi-alpha-selinene synthase, an enzyme".
- (2Z,6Z)-farnesyl_diphosphate_lyase comment "(2Z,6Z)-farnesyl diphosphate lyase may refer to: (+)-alpha-santalene synthase ((2Z,6Z)-farnesyl diphosphate cyclizing), an enzyme (+)-endo-beta-bergamotene synthase ((2Z,6Z)-farnesyl diphosphate cyclizing), an enzyme (-)-endo-alpha-bergamotene synthase ((2Z,6Z)-farnesyl diphosphate cyclizing), an enzyme".
- (3-Aminopropyl)triethoxysilane comment "(3-Aminopropyl)triethoxysilane (APTES) is an aminosilane frequently used in the process of silanization, the functionalization of surfaces with alkoxysilane molecules.".
- (303775)_2005_QU182 comment "(303775) 2005 QU182, also written as (303775) 2005 QU182, is a trans-Neptunian object with a bright absolute magnitude of 3.8. Mike Brown lists it as probably a dwarf planet.".
- (307261)_2002_MS4 comment "(307261) 2002 MS4 is a large classical Kuiper belt object, the second-largest known object in the Solar System without a name, after 2007 OR10. It was discovered in 2002 by Chad Trujillo and Michael Brown.Brown's website lists it as nearly certain to be a dwarf planet. The Spitzer Space Telescope estimated it to have a diameter of 7005726000000000000♠726±123 km.".
- (307463)_2002_VU130 comment "(307463) 2002 VU130 (also written (307463) 2002 VU130) is a trans-Neptunian object (TNO). It was discovered in 2002 by Marc W. Buie at Kitt Peak Observatory. The object is classified as a plutino (in 2:3 resonance with Neptune).".
- (307616)_2003_QW90 comment "(307616) 2003 QW90 is a classical Kuiper belt object that was discovered on August 23, 2003, by Marc W. Buie. In 2008, it's diameter was listed as 440 kilometres (270 mi).".
- (308193)_2005_CB79 comment "(308193) 2005 CB79 is a trans-Neptunian object that is a member of the Haumea family.As a member of the Haumea family, (308193) 2005 CB79 is suspected of being an icy mantle collisional fragment from dwarf planet Haumea. With an absolute magnitude (H) of 4.7, and a Haumea-family albedo of 0.7, this object would have a diameter of 158 km.Observations by Mike Brown in 2012 using the W. M. Keck Observatory suggest that (308193) 2005 CB79 does not have a companion.".
- (308242)_2005_GO21 comment "(308242) 2005 GO21 is a large near-Earth asteroid and potentially hazardous object. It has a well determined orbit with an observation arc of 7 years and an uncertainty parameter of 0. It was discovered on 1 April 2005 by the Siding Spring Survey at an apparent magnitude of 18.1 using the 0.5-metre (20 in) Uppsala Southern Schmidt Telescope.Based on an absolute magnitude of 16.4, the asteroid has an estimated diameter of 1.6 km (within a factor of two).".
- (308635)_2005_YU55 comment "(308635) 2005 YU55, provisionally known as 2005 YU55, is a potentially hazardous asteroid 360±40 meters in diameter, as measured after its Earth flyby. Previously it was estimated at 310 meters or about 400 m (1,300 feet) in diameter. It was discovered on 28 December 2005 by Robert S. McMillan at Steward Observatory, Kitt Peak. On 8 November 2011 it passed 0.85 lunar distances (324,900 kilometers; 201,900 miles) from Earth.".
- (308933)_2006_SQ372 comment "(308933) 2006 SQ372 is a small trans-Neptunian object discovered through the Sloan Digital Sky Survey by Andrew Becker, Andrew Puckett, and Jeremy Kubica on images first taken on September 27, 2006 (with precovery images dated to September 13, 2005).It has a strongly eccentric orbit, crossing that of Neptune near perihelion but bringing it more than 1,500 AU from the Sun at aphelion. It takes about 22,500 years to orbit the barycenter of the Solar System.".
- (309239)_2007_RW10 comment "(309239) 2007 RW10, also written (309239) 2007 RW10, is a temporary quasi-satellite of Neptune. Observed from Neptune, it would appear to go around it during one Neptunian year but it actually orbits the Sun, not Neptune.".
- (310071)_2010_KR59 comment "(310071) 2010 KR59, also written as 2010 KR59, is a minor planet classified by the Minor Planet Center as a centaur. The object is trapped in a 1:1 mean motion resonance with Neptune.".
- (311999)_2007_NS2 comment "2007 NS2 is an asteroid orbiting near the L5 point of Mars.".
- (31345)_1998_PG comment "(31345) 1998 PG is a near-earth object discovered by the LONEOS program on August 3, 1998. It is known to have a moon, S/2001 (31345) 1.".
- (315898)_2008_QD4 comment "(315898) 2008 QD4, also written as (315898) 2008 QD4, is a centaur with a perihelion greater than Jupiter and a semi-major axis less than Saturn.".
- (316179)_2010_EN65 comment "(316179) 2010 EN65, also written as 2010 EN65, is a minor body (as of October 2012) classified by the Minor Planet Center as a centaur. However, the object is actually a jumping trojan, is jumping from the Lagrangian point L4 into L5 via L3.".
- (31669)_1999_JT6 comment "(31669) 1999 JT6 is an Earth-crossing asteroid belonging to the Apollo family of asteroids which also crosses the orbit of Mars. 1999 JT6 is the asteroid's temporary discovery name. It has now been assigned a permanent number from the Minor Planet Center (31669) indicating that its orbit has been confirmed, but has not (at least so far) been assigned a name.".
- (322756)_2001_CK32 comment "2001 CK32, also written 2001 CK32, is a transient Venus co-orbital, but also a Mercury grazer and an Earth crosser. It is an Aten asteroid that is included in the Minor Planet Center list of Potentially Hazardous Asteroids (PHAs) as it comes to within 0.05 AU of Earth periodically.".
- (33001)_1997_CU29 comment "(33001) 1997 CU29, also written as (33001) 1997 CU29 is a cubewano. It has a perihelion (closest approach to the Sun) at 41.660 AU and an aphelion (farthest approach from the Sun) of 45.134 AU. 1997 CU29 is about 211 km in diameter. It was discovered on February 6, 1997, by David C. Jewitt, Jane X. Luu, Chad Trujillo, and Jun Chen at the Mauna Kea Observatory, Hawaii.".
- (332446)_2008_AF4 comment "(332446) 2008 AF4 is an asteroid which was listed on the Sentry Risk Table in January 2008 with a Torino Scale rating of 1. The asteroid showed a 1 in 71,000 chance of impact on 9 January 2089. It was briefly downgraded to Torino Scale 0 in February 2008, but still showed a cumulative 1 in 53,000 chance of an impact. In March it was back at Torino Scale 1 with a 1 in 28,000 chance of impact on 9 January 2089. By mid April 2008, it was back to Torino Scale 0.".
- (33340)_1998_VG44 comment "(33340) 1998 VG44, also written as (33340) 1998 VG44, is a trans-Neptunian object. It has a 2:3 orbital resonance with the planet Neptune, similar to Pluto, classifying it as a plutino. Its average distance from the Sun is 39.083 AU with a perihelion of 29.354 AU and an aphelion at 48.813 AU. Its orbit has an eccentricity of 0.249, and is inclined by 3°. It is about 221 km in diameter, so it is unlikely to be classified as a dwarf planet. It was discovered on November 14, 1998, by J. A.".
- (33342)_1998_WT24 comment "(33342) 1998 WT24 (also written (33342) 1998 WT24) is an Aten asteroid located in Venus' zone of influence that has frequent close encounters with Mercury, Venus, and Earth. It is also one of the best studied potentially hazardous asteroids and was the 10th Aten to be numbered.".
- (341843)_2008_EV5 comment "(341843) 2008 EV5 (or 2008 EV5) is a near-Earth, potentially hazardous, Aten asteroid. It was discovered by the Mount Lemmon Survey in Tucson, Arizona, United States, on 4 March 2008.".
- (343158)_2009_HC82 comment "(343158) 2009 HC82, also written as (343158) 2009 HC82 is a near-Earth asteroid, initially listed as a potentially hazardous object. It was removed from the Sentry Risk Table on 6 May 2009. It has a retrograde orbit and makes many close approaches to Earth, Venus, and Mars at a very high relative velocity.".
- (350462)_1998_KG3 comment "(350462) 1998 KG3, also written as (350462) 1998 KG3, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach to Earth is more than 0.12 AU.".
- (35144)_1992_YE1 comment "(35144) 1992 YE1 is a minor planet, discovered on December 18, 1992, at the CERGA Observatory in Caussols, France by Eric Walter Elst.".