Matches in DBpedia 2015-10 for { ?s <http://dbpedia.org/ontology/abstract> ?o }
- (145452)_2005_RN43 abstract "(145452) 2005 RN43, also written as (145452) 2005 RN43, is a classical Kuiper belt object. It has an estimated diameter of 7005679000000000000♠679+55−73 km. It was discovered by by Andrew Becker, Andrew Puckett and Jeremy Kubica on 10 September 2005 at Apache Point Observatory in Sunspot, New Mexico. It is possibly a dwarf planet.".
- (145453)_2005_RR43 abstract "(145453) 2005 RR43, also written as (145453) 2005 RR43, is a trans-Neptunian object (TNO) estimated to be about 250 km in diameter. It was discovered on 9 September 2005 by Andrew Becker, Andrew Puckett and Jeremy Kubica at Apache Point Observatory in Sunspot, New Mexico. It is possibly a dwarf planet.".
- (145480)_2005_TB190 abstract "(145480) 2005 TB190, provisionally known as 2005 TB190, is a trans-Neptunian object (TNO) with an absolute magnitude of 4.4, making it a likely dwarf planet.".
- (148209)_2000_CR105 abstract "(148209) 2000 CR105, also written as (148209) 2000 CR105, is roughly the seventh-most-distant known object in the Solar System. Considered a detached object, it orbits the Sun in a highly eccentric orbit every 3345 years at an average distance of 223 astronomical units (AU).Mike Brown's website lists it as a possible dwarf planet with a diameter of 328 kilometres (204 mi) based on an assumed albedo of 0.04. The albedo is expected to be low because the object has a blue (neutral) color. However, if the albedo is higher, the object could easily be half that size.2000 CR105 and Sedna differ from scattered-disc objects in that they are not within the gravitational influence of the planet Neptune even at their perihelion distances (closest approaches to the Sun). It is something of a mystery as to how these objects came to be in their current, far-flung orbits. Several hypotheses have been put forward: They were pulled from their original positions by a passing star. They were pulled from their original positions by a very distant, and as-yet-undiscovered (albeit unlikely), giant planet. They were pulled from their original positions by an undiscovered companion star orbiting the Sun. They were captured from another planetary system during a close encounter early in the Sun's history. According to Kenyon and Bromley, there is a 15% probability that a star like the Sun had an early close encounter and a 1% probability that outer planetary exchanges would have happened. 2000 CR105 is estimated to be 2–3 times more likely to be a captured planetary object than Sedna.2000 CR105 is the first object discovered in the Solar System to have a semi-major axis exceeding 150 AU, a perihelion beyond Neptune, and an argument of perihelion of 340 ± 55°.".
- (148975)_2001_XA255 abstract "(148975) 2001 XA255, also written as 2001 XA255, is a minor body classified as centaur by the Minor Planet Center. The object is currently trapped in a 1:1 mean-motion resonance with Neptune following a path of the horseshoe type.".
- (152680)_1998_KJ9 abstract "(152680) 1998 KJ9 is a near-Earth asteroid and potentially hazardous object. It has a well determined orbit with an excellent observation arc of 21 years and an Uncertainty Parameter of 0.It was discovered on 27 May 1998 by the Lincoln Near-Earth Asteroid Research (LINEAR) at an apparent magnitude of 17.6 using a 1.0-meter (39 in) reflector. It was tracked through 9 June 1998. It was recovered on 28 December 2003 which extended the observation arc by 5 years. Two precovery images from January 1990 extended the observation arc by 8 years.Based on an absolute magnitude of 19.4, the asteroid has an estimated diameter of about 500 metres (1,600 ft). 1998 KJ9 is noted for a close approach to the Earth on 31 December 1914 at a distance of 0.00155 AU (232,000 km; 144,000 mi). It is one of the largest objects known to have come inside the orbit of the moon. During the 1914 close approach the asteroid reached about apparent magnitude 7.7.".
- (153201)_2000_WO107 abstract "(153201) 2000 WO107 is a small asteroid that is a Near-Earth object and an Aten asteroid.".
- (153591)_2001_SN263 abstract "(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). The largest body is called Alpha and is spheroid in shape, with principal axes of 2.8±.1 km, 2.7±.1 km, and 2.5±.2 km and a density of nearly 1.3±0.6 g cm−3, and the satellites, named Beta and Gamma, are several times smaller in size.Beta is 1.1 km in diameter and Gamma 0.4 km.The only other unambiguously identified triple asteroid in the near-Earth population is (136617) 1994 CC, which was discovered to be a triple system in 2009.".
- (153814)_2001_WN5 abstract "(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. The asteroid will pass within 250,000 km (0.65 lunar distances) from the Earth on June 26, 2028. During the close approach, the asteroid should peak at about apparent magnitude 6.7, and will be visible in binoculars. It has an absolute magnitude (H) of 18.2. Depending on its characteristics and albedo, it is estimated to be 700 to 1,500 meters in diameter.".
- (15430)_1998_UR31 abstract "(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 abstract "(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. Over 1,500 further objects have been found beyond Neptune, a good number of which are classical Kuiper belt objects.The discoverers suggested the name "Smiley" for (15760) 1992 QB1, but the name was already used for an asteroid 1613 Smiley, named after the American astronomer Charles Hugh Smiley. It has received the number 15760 and remains unnamed; it is normally referred to simply as "QB1", even though this is technically ambiguous without the year of discovery.".
- (15788)_1993_SB abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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. Light-curve-amplitude analysis suggests it is a spheroid. Tancredi presents "in the form of a decision tree, the set of questions to be considered in order to classify an object as an icy 'dwarf planet'." They find that 1996 TL66 is very probably a dwarf planet. Mike Brown's website, using a radiometrically determined diameter of 344 kilometres (214 mi), lists it as a possible dwarf planet.".
- (15875)_1996_TP66 abstract "(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 abstract "(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 abstract "(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 abstract "(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). The asteroid was listed on Sentry Risk Table with a Torino Scale rating of 1 on 20 March 2002.With an observation arc of 44 days, 2002 CU11 showed a 1 in 9,300 chance of impacting Earth in 2049. It was removed from the Sentry Risk Table on 26 April 2002. It is now known that on 3 September 2049 the asteroid will be 0.0843 AU (12,610,000 km; 7,840,000 mi) from Earth.".
- (163189)_2002_EU6 abstract "(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 abstract "(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. It was uncertain whether Deep Impact carried sufficient fuel for this operation.On November 24, 2011 and October 4, 2012, the space probe's thrusters were fired briefly for two trajectory correction maneuvers that targeted Deep Impact for an encounter with 2002 GT in 2020, possibly within a distance of no more than 400 kilometers. However, funding for the flyby mission was not guaranteed. In June 2013 the asteroid was observed in radar by the Arecibo Observatory.However, on August 8, 2013 NASA lost communication with the spacecraft, and on September 20, 2013, NASA abandoned further attempts to contact the craft. According to A'Hearn, the most probable reason of software malfunction was a Y2K-like problem (at 11 August 2013 0:38:49 it was 232 deciseconds from 1 January 2000).".
- (163364)_2002_OD20 abstract "(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). With an absolute magnitude (H) of 18.8, the diameter is estimated to be 460–1030 meters.".
- (164207)_2004_GU9 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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. The moon is 0.49 ± 0.08 km in diameter, and orbits the asteroid every 16 hours, 9 minutes, and 3 seconds.Prior to late 2012, (175706) 1996 FG3 was the preliminary baseline target of the European Space Agency's MarcoPolo-R mission, which was selected for the assessment study phase of ESA's M3 mission.".
- (177049)_2003_EE16 abstract "(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). The asteroid was listed on Sentry Risk Table with a Torino Scale rating of 1 on 2 April 2003.Many of the virtual impactors were located near the nominal orbital solution and the asteroid has a low inclination relative to Earth's orbit. Observation by the Very Large Telescope (VLT) 8 meter facilities on 22 May and 19 June 2003 when 2003 EE16 was very dim with an apparent magnitude between 24–25 refined the orbit. It was removed from the Sentry Risk Table on 28 May 2003.2003 EE16 has the smallest Earth Minimum orbit intersection distance (MOID) of any known potentially hazardous asteroid. The Earth MOID is 0.0000475 AU (7,110 km; 4,420 mi). Asteroids with a smaller Earth MOID are less than ~100 meters in diameter such as 2013 XY8 and 2010 TD54. Earth impactors 2008 TC3 and 2014 AA had small Earth MOID values as they were on their impact approach when discovered.".
- (179806)_2002_TD66 abstract "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. 2002 TD66 was removed from the Sentry Risk Table on October 10, 2002. A Doppler observation has helped produce a well known trajectory with a condition code (Uncertainty Parameter U) of 0.Based on an absolute magnitude (H) of 20.2, the asteroid is estimated to be between 270 and 590 meters in diameter. Radar astronomy shows it is a contact binary asteroid with a diameter of 300 meters and a rotation period of 9.5 hours.On February 26, 2008, 2002 TD66 passed 0.04282 AU (6,406,000 km; 3,980,000 mi) from Earth. The asteroid also comes close to Venus, Mars, and dwarf planet Ceres.".
- (181708)_1993_FW abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "2006 SV23 is a Ceres trojan asteroid discovered in 2006.".
- (185851)_2000_DP107 abstract "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 abstract "(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 abstract "(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. It is known that 1999 RD32 passed 0.0093 AU (1,390,000 km; 860,000 mi) from Earth on 27 August 1969. During the 1969 close approach the asteroid reached about apparent magnitude 8.8. The similarly-sized 4179 Toutatis also reached that brightness in September 2004. 1999 RD32 passed less than 0.007 AU (1,000,000 km; 650,000 mi) from asteroid 29 Amphitrite on 17 January 1939.Arecibo radar observations on 5–6 March 2012 showed that 1999 RD32 is approximately 5 kilometers (3 mi) in diameter and has an albedo of only a few percent. The two visible lobes suggest that 1999 RD32 is a tight binary asteroid or contact binary. About 10–15% of near-Earth asteroids larger than 200 meters are expected to be contact binary asteroids with two lobes in mutual contact.".
- (19299)_1996_SZ4 abstract "(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 abstract "(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 abstract "(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 abstract "In the theory of Riemann surfaces and hyperbolic geometry, the triangle group (2,3,7) is particularly important. This importance stems from its connection to Hurwitz surfaces, namely Riemann surfaces of genus g with the largest possible order, 84(g − 1), of its automorphism group.A note on terminology – the "(2,3,7) triangle group" most often refers, not to the full triangle group Δ(2,3,7) (the Coxeter group with Schwarz triangle (2,3,7) or a realization as a hyperbolic reflection group), but rather to the ordinary triangle group (the von Dyck group) D(2,3,7) of orientation-preserving maps (the rotation group), which is index 2.Torsion-free normal subgroups of the (2,3,7) triangle group are Fuchsian groups associated with Hurwitz surfaces, such as the Klein quartic, Macbeath surface and First Hurwitz triplet.".
- (2,4,6-Trimethylphenyl)gold abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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. Brown using the Samuel Oschin telescope in the Palomar Observatory.".
- (21083)_1991_TH14 abstract "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 abstract "(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. It has an Apollo type orbit and is classified as a potentially hazardous asteroid (PHA).2007 PA8 may be a dormant comet related to the November γ Pegasids meteor shower.".
- (225088)_2007_OR10 abstract "(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 abstract "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 abstract "(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. It will come to perihelion in February 2046.It has been observed 73 times over 11 oppositions with precovery images back to 1982.".
- (230965)_2004_XA192 abstract "(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 abstract "(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 abstract "(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. During the 2010 close approach, NASA Infrared Telescope Facility (NASA IRTF) studies suggested that 1999 TA10 originated from the interior of Vesta. The next close approach will be in 2023. In 2086, it will come within 0.017 AU (2,500,000 km; 1,600,000 mi) of Mars.".
- (242450)_2004_QY2 abstract "(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. 2004 QY2 is one of the largest potentially hazardous asteroids (PHA) discovered. As of 2013 it has the brightest absolute magnitude of any PHA since its discovery. On 29 July 2012 it passed Earth at a distance of 0.4314 AU (64,540,000 km; 40,100,000 mi).Given the estimated size of roughly 5km, 2004 QY2 is one of the largest objects to appear on the Sentry Risk Table. It was removed from the Sentry Risk Table on 25 August 2004.".
- (24835)_1995_SM55 abstract "(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 abstract "(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 abstract "(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). It has an estimated diameter of 139 km; therefore, it is unlikely to be classified as a dwarf planet.".
- (24978)_1998_HJ151 abstract "(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 abstract "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 abstract "(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 abstract "(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 abstract "(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 abstract "(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 abstract "(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). The asteroid was discovered November 27, 2005 by the Siding Spring Survey.".
- (277810)_2006_FV35 abstract "(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 abstract "(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). Mike Brown's website lists it as a "highly likely" dwarf planet, but its diameter has never been measured.Observations by Brown in 2012, using the W. M. Keck Observatory, suggest that 2007 JJ43 does not have a companion.As of 2014, it is about 41.3 AU from the Sun.".
- (27981)_1997_UK21 abstract "(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 abstract "(280244) 2002 WP11 is an asteroid, discovered on November 27, 2002 by CINEOS.".
- (285263)_1998_QE2 abstract "(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 abstract "(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. 1950 DA is not assigned a Torino scale rating, because the 2880 date is over 100 years in the future.".
- (292220)_2006_SU49 abstract "(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. It is now known that on January 28, 2029, the asteroid will be 0.00818 AU (1,224,000 km; 760,000 mi) from Earth.It is a near-Earth asteroid that received minor attention in late September and early October 2006 because initial observations indicated a higher than usual probability that it would strike the Earth in 2029. However, the Near-Earth Object (NEO) Office at NASA's Jet Propulsion Laboratory (JPL) removed 2006 SU49 from its risk list as additional observations provided improved predictions that eliminated the possibility of an impact on Earth or the Moon through 2106. Similarly, NEODyS estimates show a zero impact probability through 2080.(292220) 2006 SU49 briefly led the Earth-impact hazard list from September 27, 2006, through October 4, 2006, temporarily displacing 2004 VD17 from the number one position. At the time, both held a Torino scale of level 1 and were the only asteroids to hold a Torino value greater than 0.Even though 2006 SU49 has an Earth MOID of 0.0003 AU (45,000 km; 28,000 mi), the orbit and future close approaches are well determined with an orbital uncertainty of 0.2006 SU49 was discovered on September 20, 2006, by the Spacewatch project at the University of Arizona. The object is estimated at 380 meters in diameter with a mass of about 7.3×1010 kg.".
- (2E,6E)-farnesyl-diphosphate:isopentenyl-diphosphate_farnesyltranstransferase abstract "(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 abstract "(2E,6E)-farnesyl-diphosphate diphosphate-lyase may refer to:Enzymes".
- (2Z,6E)-farnesyl-diphosphate_diphosphate-lyase abstract "(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 abstract "(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 abstract "(3-Aminopropyl)triethoxysilane (APTES) is an aminosilane frequently used in the process of silanization, the functionalization of surfaces with alkoxysilane molecules.".
- (303775)_2005_QU182 abstract "(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 abstract "(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. The Herschel team estimates it to be 7005934000000000000♠934±47 km, which would make it one of the 10 largest TNOs currently known and large enough to be considered a dwarf planet under the 2006 draft proposal of the IAU. It is currently 47.2 AU from the Sun and will come to perihelion in 2123.It has been observed 46 times, with precovery images back to 1954.".
- (307463)_2002_VU130 abstract "(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 abstract "(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 abstract "(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 abstract "(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). 2005 GO21 is the largest potentially hazardous asteroid (PHA) discovered in 2005. On 21 June 2012 it passed Earth at a distance of 0.043963 AU (6,576,800 km; 4,086,600 mi). The 2012 passage was studied with radar using Goldstone and Arecibo.".
- (308635)_2005_YU55 abstract "(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 abstract "(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. The large semi-major axis makes it similar to (87269) 2000 OO67 and 90377 Sedna. With an absolute magnitude (H) of 8.1, it is estimated to be about 60 to 140 km in diameter. Michael Brown estimates that it has an albedo of 0.08 which would give a diameter of around 110 km.The object could possibly be a comet. The discoverers hypothesize that the object could come from the inner Oort cloud, but other scientists like California Institute of Technology's Michael Brown also consider other possibilities, as "it may have formed from debris just beyond Neptune [in the Kuiper belt] and been 'kicked' into its distant orbit by a planet like Neptune or Uranus".".
- (309239)_2007_RW10 abstract "(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 abstract "(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 abstract "2007 NS2 is an asteroid orbiting near the L5 point of Mars.".
- (31345)_1998_PG abstract "(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 abstract "(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 abstract "(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 abstract "(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. Only a small fraction of asteroids have been named.It has an Earth minimum orbit intersection distance of 0.00354 AU (328,978 miles), which is close enough to classify it as a Potentially Hazardous Asteroid (PHA). It will make a close approach to Earth on 14 December 2076 at 0.0260 AU (2,506,321 miles) and an even closer approach to the minor planet Ceres on 16 Feb 2084 at 0.0171 AU (1,587,064 miles).".
- (322756)_2001_CK32 abstract "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 abstract "(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.".