Unusual minor planet

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In planetary science, the term unusual minor planet, or unusual object, is used for a minor planet that possesses an unusual physical or orbital characteristic. For the Minor Planet Center (MPC), which operates under the auspices of the International Astronomical Union, any non-classical main-belt asteroid, which account for the vast majority of all minor planets, is an unusual minor planet. These include the near-Earth objects and Trojans as well as the distant minor planets such as centaurs and trans-Neptunian objects. [1] In a narrower sense, the term is used for a group of bodies – including main-belt asteroids, Mars-crossers, centaurs and otherwise non-classifiable minor planets – that show a high orbital eccentricity, typically above 0.5 and/or a perihelion of less than 6  AU. [2] Similarly, an unusual asteroid (UA) is an inner Solar System object with a high eccentricity and/or inclination but with a perihelion larger than 1.3 AU, which does exclude the near-Earth objects. [3]

Contents

Other unusual objects

According to the MPC, other unusual minor planets are objects, which orbital characteristics do not fit those of the near-Earth and distant populations. [2] These objects typically have high eccentricities, and inclinations often more than 90 degrees (retrograde orbits), a criterion that is common among the members of the damocloid population. Object in this list have a TJupiter of less than 3 and a perihelion between 1.67 and 5.5  AU, that is, they do not cross the orbit of Mars but cross or at least come close to Jupiter's orbit at 5.2 AU. According to the SSBN07 classification, such objects have cometary dynamics. [4] :44As of August 2021, the list contains 211 objects, most of which remain unnumbered. A bold designation links to an object's stand-alone article.

Designation Discovery D est.Orbital descriptionRemarksRefs
Year Place Discoverer LoMP
class
a
(AU)
e i
(°)
q
(AU)
Q
(AU)
TJupiter
(15504) 1999 RG33 1999( 703 ) CSS 17 km CEN 9.40.77352.1216.61.95Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid; BR-mag: 1.21

MPC
JPL
20461 Dioretsa 1999( 704 ) LINEAR 7.7 kmCEN23.90.901602.4045.4-1.54Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid; albedo: 0.030
catalog
MPC
JPL
37117 Narcissus 2000( 919 ) W. K. Y. Yeung 9.7 kmCEN6.90.55143.0710.72.62Obs: 10 opposition(s)
Johnston's Archive: unusual; albedo: 0.088

MPC
JPL
(65407) 2002 RP120 2002( 699 ) LONEOS 15 km TNO 53.90.951192.45105-0.84Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid; albedo: 0.098; BR-mag: 1.37
catalog
MPC
JPL
(144908) 2004 YH32 2004( E12 ) SSS 12 km CEN 8.20.57793.5512.81.03Obs: 3 opposition(s)
Johnston's Archive: damocloid;
catalog
MPC
JPL
(145627) 2006 RY102 2006( 644 ) NEAT 27 kmCEN6.30.28194.588.12.83Obs: 19 opposition(s)
Johnston's Archive: unusual; albedo: 0.051

MPC
JPL
(154783) 2004 PA44 2004(644)NEAT8.4 kmCEN14.20.7633.4125.02.51Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid;

MPC
JPL
(308607) 2005 WY3 2005( 291 ) Spacewatch 8.8 kmCEN6.70.73291.7911.72.12Obs: 4 opposition(s)
Johnston's Archive: unusual;

MPC
JPL
(330759) 2008 SO218 2008( G96 ) MLS 12 kmCEN8.10.561703.5412.7-1.39Listed in damocloid
Obs: 8 opposition(s)
Johnston's Archive: damocloid; albedo: 0.076; BR-mag: 1.44

MPC
JPL
(347449) 2012 TW236 1998( 704 ) LINEAR 15 kmCEN7.00.57123.0011.02.61Obs: 9 opposition(s)
Johnston's Archive: unusual;

MPC
JPL
(433873) 2015 BQ311 2006( G96 ) MLS 16 kmCEN7.10.29255.039.22.77Obs: 13 opposition(s)
Johnston's Archive: centaur; BR-mag: 1.25

MPC
JPL
(434620) 2005 VD 2005(G96)MLS6.3 kmCEN6.70.251735.008.3-1.39Listed in damocloid
Obs: 6 opposition(s)
Johnston's Archive: damocloid; BR-mag: 1.05
catalog
MPC
JPL
(540205) 2017 RS17 2016( F51 ) Pan-STARRS 15.4 kmCEN6.20.45433.418.92.27Obs: 5 opposition(s)
Johnston's Archive: unusual;

MPC
JPL
1996 PW 1996( 566 ) NEAT 7.4 km TNO 2530.99302.495041.73Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
1998 QJ1 1998( 704 ) LINEAR 2.2 km CEN 11.20.81242.0920.42.03Listed in damocloid
Obs: ( 62d)
Johnston's Archive: damocloid;
MPC
JPL
2000 AB229 2000(704)LINEAR7.0 km TNO 52.90.96682.321030.79Listed in damocloid
Obs: ( 64d)
Johnston's Archive: damocloid;
MPC
JPL
2000 DG8 2000(704)LINEAR11 km CEN 10.80.791292.2219.3-0.62Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.053
MPC
JPL
2000 HE46 2000( 699 ) LONEOS 4.9 kmCEN23.60.901592.3944.9-1.52Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.045; BR-mag: 1.42
MPC
JPL
2000 KP65 2000(699)LONEOS35 km TNO 90.20.96463.311771.63Listed in damocloid
Obs: ( 58d)
Johnston's Archive: damocloid;
MPC
JPL
2001 QF6 2001( 704 ) LINEAR 4.0 km CEN 7.30.69242.2712.32.28Obs: 4 opposition(s)
Johnston's Archive: unusual; albedo: 0.040
MPC
JPL
2001 YK61 2001(704)LINEAR8.1 kmCEN10.60.69123.2917.92.51Obs: ( 61d)
Johnston's Archive: unusual;
MPC
JPL
2002 AR91 2002( 807 ) DLS 2.9 km TNO 75.20.97182.621481.97Listed in damocloid
Obs: ( 4d)
MPC
JPL
2002 RN109 2002( 704 ) LINEAR 3.9 kmTNO5551.00582.6911071.10Listed in damocloid
Obs: ( 80d)
Johnston's Archive: damocloid;
MPC
JPL
2003 CC22 2003( 568 ) D. C. Jewitt
S. S. Sheppard
13 km CEN 7.30.4364.1710.42.84Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2003 WN188 2003( 703 ) CSS 7.0 kmCEN14.40.85272.2126.61.94Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.050; BR-mag: 1.26
MPC
JPL
2004 DA62 2004( 704 ) LINEAR 11 kmCEN7.70.47524.0911.21.99Obs: 3 opposition(s)
Johnston's Archive: damocloid; BR-mag: 1.37
MPC
JPL
2004 NN8 2004( E12 ) SSS 3.9 km TNO 98.40.981662.36194-1.78Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2005 HL32005(E12)SSS5.8 km CEN 11.30.83361.8920.71.79Listed in damocloid
Obs: (157d)
Johnston's Archive: damocloid;
MPC
JPL
2005 OE2005( 703 ) CSS 8.1 km TNO 62.90.95683.031230.90Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2005 SB2232005( E12 ) SSS 6.4 km CEN 29.40.91912.7856.10.13Listed in damocloid
Obs: (244d)
Johnston's Archive: damocloid;
MPC
JPL
2005 TJ502005( 691 ) Spacewatch 3.9 kmCEN9.10.581103.8114.5-0.17Listed in damocloid
Obs: ( 62d)
Johnston's Archive: damocloid;
MPC
JPL
2005 VX3 2005( G96 ) MLS 6.7 km TNO 9531.001124.111902-0.91Listed in damocloid
Obs: ( 81d)
Johnston's Archive: damocloid;
MPC
JPL
2006 BZ8 2006( 703 ) CSS 6.4 km CEN 9.60.801651.8917.3-1.02Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2006 EX522006(703)CSS5.3 km TNO 42.50.941502.5682.5-1.57Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2006 FV42006( 704 ) LINEAR 11 km CEN 10.80.70323.2318.32.22Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2006 JG572006( 644 ) NEAT 15 kmCEN9.60.51574.7314.51.82Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2006 RG12006( E12 ) SSS 3.4 kmCEN25.60.921342.0349.2-0.99Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2006 RJ2 2006( 703 ) CSS 2.9 kmCEN9.80.761652.3117.3-1.17Listed in damocloid
Obs: ( 37d)
Johnston's Archive: damocloid;
MPC
JPL
2006 SO1342006( 691 ) Spacewatch 2.3 kmCEN19.50.8343.3035.72.42Listed in damocloid
Obs: ( 36d)
Johnston's Archive: damocloid;
MPC
JPL
2007 DA612007( G96 ) MLS 4.6 km TNO 4470.99772.668900.48Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2007 DP502007( 691 ) Spacewatch 5.3 km CEN 6.20.3833.838.62.85Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2007 HU452007( G96 ) MLS 3.1 kmCEN6.80.5063.3910.22.73Obs: ( 28d)
Johnston's Archive: unusual;
MPC
JPL
2007 SA242007(G96)MLS4.2 kmCEN6.30.57172.729.92.56Obs: (156d)
Johnston's Archive: unusual;
MPC
JPL
2008 BN182008( 291 ) Spacewatch 7.7 km TNO 35.30.93292.6467.91.88Listed in damocloid
Obs: ( 14d)
Johnston's Archive: damocloid;
MPC
JPL
2008 JS142008( E12 ) SSS 10 km CEN 11.60.74262.9720.12.24Obs: 2 opposition(s)
Johnston's Archive: unusual; albedo: 0.044
MPC
JPL
2008 SE822008( G96 ) MLS 4.9 kmCEN19.30.84173.1835.42.29Listed in damocloid
Obs: ( 61d)
Johnston's Archive: damocloid;
MPC
JPL
2008 WA952008( 704 ) LINEAR 1.9 kmCEN14.10.88601.7226.41.16Listed in damocloid
Obs: ( 27d)
Johnston's Archive: damocloid;
MPC
JPL
2008 WT112008( 703 ) CSS 7.0 kmCEN9.90.6273.7816.02.68Obs: ( 38d)
Johnston's Archive: unusual;
MPC
JPL
2009 AU162009( E12 ) SSS 2.7 kmCEN23.60.92701.9545.30.81Listed in damocloid
Obs: (125d)
Johnston's Archive: damocloid;
MPC
JPL
2009 BL802009( 704 ) LINEAR 2.4 kmCEN6.10.6492.2010.12.49Obs: (119d)
Johnston's Archive: unusual;
MPC
JPL
2009 FW232009( E12 ) SSS 3.7 kmCEN11.50.86871.6721.40.54Listed in damocloid
Obs: ( 55d)
Johnston's Archive: damocloid;
MPC
JPL
2009 QY62009( 704 ) LINEAR 4.9 kmCEN12.50.831382.0722.9-0.85Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.015
MPC
JPL
2010 CG552010( 703 ) CSS 6.4 km TNO 32.00.911462.8861.1-1.55Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid; albedo: 0.048
MPC
JPL
2010 DC392010( G96 ) MLS 1.7 kmTNO1090.98111.832161.70Listed in damocloid
Obs: ( 2d)
MPC
JPL
2010 EE212010( C51 ) WISE 2.7 km CEN 8.50.62363.2013.72.23Obs: ( 19d)
Johnston's Archive: unusual;
MPC
JPL
2010 EX1752010(C51)WISE0 m TNO 49.40.95292.6596.11.85Listed in damocloid
Obs: ( 1d)
MPC
JPL
2010 GW642010(C51)WISE4.6 kmTNO63.30.941053.72123-0.54Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.047
MPC
JPL
2010 GW1472010(C51)WISE10 kmTNO1670.971005.39330-0.45Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: centaur; albedo: 0.037
MPC
JPL
2010 JB1842010(C51)WISE0 mTNO44.80.93193.0786.62.13Listed in damocloid
Obs: ( 1d)
MPC
JPL
2010 JC1472010(C51)WISE5.1 km CEN 14.60.76423.4725.81.97Listed in damocloid
Obs: (123d)
Johnston's Archive: damocloid; albedo: 0.064
MPC
JPL
2010 JH1242010(C51)WISE5.3 km TNO 69.10.96532.601361.26Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.052
MPC
JPL
2010 LN1352010( I41 ) PTF 7.8 kmTNO21691.00651.7243370.78Listed in damocloid
Obs: ( 32d)
MPC
JPL
2010 OM1012010( C51 ) WISE 1.8 km CEN 26.00.921192.1350.0-0.66Listed in damocloid
Obs: (101d)
Johnston's Archive: damocloid; albedo: 0.036; BR-mag: 1.34
MPC
JPL
2010 OR12010(C51)WISE2.5 kmCEN26.90.921442.0451.8-1.21Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; albedo: 0.110; BR-mag: 1.32
MPC
JPL
2010 PO582010(C51)WISE5.6 kmCEN11.80.751212.9320.6-0.59Listed in damocloid
Obs: ( 6d)
Johnston's Archive: damocloid; albedo: 0.035
MPC
JPL
2011 OR172011( E12 ) SSS 11 km TNO 2680.991113.11532-0.76Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2011 RC172011( H15 ) ISON-NM 3.1 km CEN 6.30.54112.929.72.65Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2011 SP252011( F51 ) Pan-STARRS 12.0 kmCEN19.50.881092.2736.8-0.33Listed in damocloid
Obs: ( 58d)
Johnston's Archive: damocloid;
MPC
JPL
2011 SQ2492011(F51)Pan-STARRS 15.8 kmCEN6.60.45173.619.62.71Obs: 3 opposition(s)
Johnston's Archive: unusual; albedo: 0.054
MPC
JPL
2011 UR4022011(F51)Pan-STARRS 120 kmCEN18.70.78254.1233.22.44Listed in damocloid
Obs: 7 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2011 WS412011(F51)Pan-STARRS 11.4 km TNO 37.80.951422.0773.5-1.24Listed in damocloid
Obs: ( 20d)
Johnston's Archive: damocloid;
MPC
JPL
2011 YU752011( 691 ) Spacewatch 1.8 km CEN 7.50.77171.7613.32.17Obs: (121d)
Johnston's Archive: unusual;
MPC
JPL
2012 CN292012( G96 ) MLS 4.9 kmCEN6.40.31204.438.42.79Obs: ( 67d) MPC
JPL
2012 DD612012( 703 ) CSS 9.7 kmCEN7.50.50193.7711.22.67Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2012 HD22012( 691 ) Spacewatch 3.9 km TNO 62.80.961472.56123-1.57Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2012 KA512012( I41 ) PTF 14 kmTNO4930.99714.909820.91Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2012 UN1382012( F51 ) Pan-STARRS 13.5 km CEN 10.00.66163.4516.62.53Obs: ( 31d)
Johnston's Archive: unusual;
MPC
JPL
2012 YE82012( G96 ) MLS 4.2 kmCEN9.30.591363.8314.8-0.99Listed in damocloid
Obs: ( 78d)
Johnston's Archive: damocloid;
MPC
JPL
2012 YO62012( F51 ) Pan-STARRS 15.1 kmCEN6.30.481073.309.30.26Listed in damocloid
Obs: (142d)
Johnston's Archive: damocloid; BR-mag: 1.32
MPC
JPL
2013 CM772013( 703 ) CSS 2.8 kmCEN7.40.5992.9911.82.60Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2013 GY542013( F51 ) Pan-STARRS 16.1 kmCEN13.60.6684.6122.62.78Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2013 HS1502013( W84 ) DECam-NEO 1.9 km TNO 62.80.96972.82123-0.18Listed in damocloid
Obs: ( 23d)
Johnston's Archive: damocloid;
MPC
JPL
2013 LD162013( G96 ) MLS 2.7 kmTNO81.00.971552.55159-1.73Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid; BR-mag: 1.30
MPC
JPL
2013 LG292013( F51 ) Pan-STARRS 14.6 km CEN 17.00.79153.5530.42.44Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2013 NS112013(F51)Pan-STARRS 18.4 kmCEN12.60.791302.6922.6-0.83Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid; albedo: 0.030; BR-mag: 1.30
MPC
JPL
2013 PJ442013(F51)Pan-STARRS 15.6 kmCEN12.10.68223.9120.32.52Obs: ( 32d)
Johnston's Archive: unusual;
MPC
JPL
2013 SV992013( W84 ) DECam 2.2 kmCEN6.90.26175.128.72.88Obs: ( 16d)
Johnston's Archive: centaur;
MPC
JPL
2013 WK642013( F51 ) Pan-STARRS 13.4 kmCEN7.90.63632.9512.91.54Obs: (118d)
Johnston's Archive: damocloid;
MPC
JPL
2013 YF482013( G96 ) MLS 7.0 kmCEN9.30.52784.4314.11.05Obs: ( 94d)
Johnston's Archive: damocloid;
MPC
JPL
2013 YG482013( 703 ) CSS 1.6 kmCEN8.20.75612.0314.31.43Listed in damocloid
Obs: (110d)
Johnston's Archive: damocloid; BR-mag: 1.32
MPC
JPL
2014 EY2472014( W84 ) DECam 4.4 kmCEN6.10.2864.367.82.92Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2014 JJ572014( F51 ) Pan-STARRS 113 kmCEN7.00.29964.949.00.52Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2014 KM1222014(F51)Pan-STARRS 17.0 kmCEN6.30.43283.598.92.59Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2014 MH552014(F51)Pan-STARRS 18.4 km TNO 44.80.90924.5085.10.01Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2014 ON572014(F51)Pan-STARRS 18.8 km CEN 15.30.69104.7825.72.79Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2014 RE122014(F51)Pan-STARRS 115 kmCEN14.20.64325.0823.42.52Obs: 8 opposition(s)
Johnston's Archive: centaur;
MPC
JPL
2014 SQ3392014(F51)Pan-STARRS 11.5 kmCEN27.90.901292.7853.1-1.07Listed in damocloid
Obs: ( 30d)
Johnston's Archive: damocloid;
MPC
JPL
2014 SQ3692014(F51)Pan-STARRS 11.5 kmCEN6.00.67122.0110.12.43Obs: (134d)
Johnston's Archive: unusual;
MPC
JPL
2014 TK342014(F51)Pan-STARRS 15.8 kmCEN13.90.70134.1423.62.64Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2014 UV1142014( G96 ) MLS 3.1 kmCEN13.00.691714.0222.0-1.86Listed in damocloid
Obs: ( 41d)
Johnston's Archive: damocloid;
MPC
JPL
2014 XS32014( F51 ) Pan-STARRS 14.6 km TNO 73.60.961013.25144-0.37Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 AO442015( 703 ) CSS 8.4 km CEN 22.00.841403.6240.5-1.49Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 BH3112015( G96 ) MLS 3.4 kmCEN9.20.73942.4615.80.44Listed in damocloid
Obs: ( 3d)
Johnston's Archive: damocloid;
MPC
JPL
2015 BW5242015( 568 ) Mauna Kea Obs. 6.1 kmCEN6.90.3194.769.02.92Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2015 BX5142015( F51 ) Pan-STARRS 15.1 kmCEN12.20.6254.5919.82.81Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2015 DB1982015(F51)Pan-STARRS 19.7 kmCEN8.30.42224.7511.72.75Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2015 FK372015(F51)Pan-STARRS 15.6 km TNO 4410.991564.96877-2.48Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 JH12015(F51)Pan-STARRS 19.3 km CEN 12.30.71353.5821.02.19Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2015 KJ1532015( F52 ) Pan-STARRS 23.1 kmCEN6.40.58182.6810.02.54Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2015 RE2772015( 568 ) OSSOS 2.2 kmCEN20.30.7724.7735.82.80Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 RK2452015( 703 ) CSS 5.6 km TNO 80.60.97922.761580.01Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 RL2772015( 568 ) OSSOS 2.3 kmTNO34.40.8535.1963.72.87Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: centaur;
MPC
JPL
2015 TN1782015( F51 ) Pan-STARRS 13.9 kmTNO54.60.96912.381070.06Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 TS3502015(F51)Pan-STARRS 110 kmTNO1410.96585.052761.50Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: centaur;
MPC
JPL
2015 XQ3842015(F51)Pan-STARRS 12.9 km CEN 12.70.65224.4720.92.62Obs: ( 31d)
Johnston's Archive: unusual;
MPC
JPL
2015 XR3842015(F51)Pan-STARRS 12.7 km TNO 36.90.901583.5770.3-1.97Listed in damocloid
Obs: (124d)
Johnston's Archive: damocloid;
MPC
JPL
2015 XX3512015(F51)Pan-STARRS 12.9 km CEN 14.60.851592.1327.0-1.27Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2015 YY182015(F51)Pan-STARRS 14.6 kmCEN19.50.831183.2935.6-0.75Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2016 AC2822016( G96 ) MLS 3.1 kmCEN6.10.43263.528.82.61Obs: ( 61d)
Johnston's Archive: unusual;
MPC
JPL
2016 AT2812016( F51 ) Pan-STARRS 14.2 km TNO 63.40.96222.681241.94Listed in damocloid
Obs: (134d)
Johnston's Archive: damocloid;
MPC
JPL
2016 BJ812016( G96 ) MLS 8.8 km CEN 9.70.48134.9914.32.86Obs: 5 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2016 CO2642016( F51 ) Pan-STARRS 12.5 km TNO 48.40.941303.0293.7-1.25Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2016 DF22016(F51)Pan-STARRS 11.8 km CEN 6.20.471673.299.2-1.04Listed in damocloid
Obs: ( 2d)
Johnston's Archive: damocloid;
MPC
JPL
2016 EJ2032016( G96 ) MLS 1.1 km TNO 67.80.961712.74133-1.92Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2016 KX42016( F51 ) Pan-STARRS 14.9 km CEN 7.00.68382.2811.82.10Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2016 LS2016(F51)Pan-STARRS 19.7 kmCEN13.30.611145.2421.4-0.66Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: centaur;
MPC
JPL
2016 ND212016( T05 ) ATLAS-HKO 15 kmCEN8.50.56223.7613.22.59Obs: 7 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2016 NL1002016( F51 ) Pan-STARRS 12.4 kmCEN13.90.76223.3324.42.34Listed in damocloid
Obs: ( 65d)
Johnston's Archive: damocloid;
MPC
JPL
2016 PN662016( 106 ) Črni Vrh Obs. 9.3 km TNO 31.00.911052.9059.1-0.37Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2016 TK22016( F51 ) Pan-STARRS 14.6 km CEN 9.20.55924.1214.20.48Listed in damocloid
Obs: (135d)
Johnston's Archive: damocloid;
MPC
JPL
2016 TP932016(F51)Pan-STARRS 13.2 kmCEN7.40.561383.2911.5-0.78Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2016 TT1002016( 691 ) Spacewatch 4.4 kmCEN8.90.59103.6714.22.67Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2016 VY172016( G96 ) MLS 3.2 kmCEN11.20.851481.6720.7-0.85Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2016 WS12016( C51 ) WISE 1.5 kmCEN14.40.88531.7027.21.31Listed in damocloid
Obs: ( 53d)
Johnston's Archive: damocloid;
MPC
JPL
2017 AO192017( G96 ) MLS 1.3 kmCEN6.60.69242.0411.32.28Obs: (135d)
Johnston's Archive: unusual;
MPC
JPL
2017 AX132017( F51 ) Pan-STARRS 14.2 kmCEN28.60.881373.3553.9-1.43Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2017 BA942017(F51)Pan-STARRS 11.5 kmCEN6.50.65192.2910.72.41Obs: ( 31d)
Johnston's Archive: unusual;
MPC
JPL
2017 CW322017( G96 ) MLS 3.4 km TNO 1930.991522.96382-1.83Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2017 FM992017( F51 ) Pan-STARRS 13.4 km CEN 8.20.66202.7813.72.41Obs: (106d)
Johnston's Archive: unusual;
MPC
JPL
2017 GC82017(F51)Pan-STARRS 11.1 kmCEN10.30.7472.6418.02.37Obs: ( 31d)
Johnston's Archive: unusual;
MPC
JPL
2017 GD82017(F51)Pan-STARRS 11.4 km TNO 43.50.95752.2884.70.60Listed in damocloid
Obs: ( 62d)
Johnston's Archive: damocloid;
MPC
JPL
2017 GZ82017( G96 ) MLS 5.8 km CEN 7.60.4863.9611.22.80Obs: 3 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2017 JB62017( F51 ) Pan-STARRS 14.0 km TNO 32.90.881613.8262.0-2.06Listed in damocloid
Obs: (116d)
Johnston's Archive: damocloid;
MPC
JPL
2017 MB7 2017(F51)Pan-STARRS 16.4 kmTNO35491.00564.4570941.32Listed in damocloid
Obs: (174d)
Johnston's Archive: damocloid;
MPC
JPL
2017 MZ42017(F51)Pan-STARRS 19.7 kmTNO66.40.95663.181300.97Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2017 OX682017(F51)Pan-STARRS 11.2 kmTNO59.00.97951.74116-0.04Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2017 QO332017(F51)Pan-STARRS 18.1 kmTNO34.40.861494.9463.9-2.12Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2017 RR22017(F51)Pan-STARRS 11.5 km CEN 11.60.78872.5320.70.54Listed in damocloid
Obs: ( 96d)
Johnston's Archive: damocloid;
MPC
JPL
2017 SN332017(F51)Pan-STARRS 11.2 km TNO 2490.991521.84497-1.42Listed in damocloid
Obs: ( 67d)
Johnston's Archive: damocloid;
MPC
JPL
2017 SV13 2017(F51)Pan-STARRS 11.0 km CEN 9.60.791132.0117.3-0.12Listed in damocloid
Obs: ( 42d)
Johnston's Archive: damocloid;
MPC
JPL
2017 SW112017(F51)Pan-STARRS 112 kmCEN9.80.52164.7014.82.78Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2017 UW512017( G96 ) MLS 3.9 km TNO 1300.981443.14257-1.73Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2017 YL22017( C51 ) WISE 2.4 km CEN 9.00.77282.0915.92.07Listed in damocloid
Obs: (114d)
Johnston's Archive: damocloid;
MPC
JPL
2017 YL42017( F51 ) Pan-STARRS 15.1 km TNO 1530.97894.263030.08Listed in damocloid
Obs: ( 63d)
MPC
JPL
2018 DE42018( G96 ) MLS 1.6 kmTNO32.50.93812.3962.60.44Listed in damocloid
Obs: (125d)
Johnston's Archive: damocloid;
MPC
JPL
2018 EG42018( F51 ) Pan-STARRS 13.5 km CEN 13.20.67184.3922.02.66Obs: ( 9d)
Johnston's Archive: unusual;
MPC
JPL
2018 KH32018( G96 ) MLS 8.1 km TNO 93.80.96473.711841.68Listed in damocloid
Obs: (211d)
Johnston's Archive: damocloid;
MPC
JPL
2018 MO82018( F51 ) Pan-STARRS 18.8 km CEN 15.10.67524.9925.21.92Obs: 4 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2018 MP82018(F51)Pan-STARRS 13.9 km TNO 3570.99683.837110.92Listed in damocloid
Obs: (184d)
Johnston's Archive: damocloid;
MPC
JPL
2018 PL282018(F51)Pan-STARRS 14.9 km CEN 19.50.86742.6936.40.80Listed in damocloid
Obs: 3 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2018 SQ132018( G96 ) MLS 3.4 km TNO 1540.98912.973050.00Listed in damocloid
Obs: (135d)
Johnston's Archive: damocloid;
MPC
JPL
2018 TL62018(G96)MLS460 m CEN 8.30.791711.7214.8-0.89Listed in damocloid
Obs: ( 10d)
Johnston's Archive: damocloid;
MPC
JPL
2018 UB12018( F52 ) Pan-STARRS 26.4 kmCEN7.70.52193.7111.62.64Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2018 WB12018( G96 ) MLS 1.5 kmCEN7.30.691522.2212.3-0.79Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2019 AH542019( F51 ) Pan-STARRS 14.9 kmCEN10.10.67113.3516.92.54Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2019 GG232019( W93 ) KMT-CTIO 1.4 kmCEN6.10.2914.397.92.93Obs: ( 7d) MPC
JPL
2019 HC42019( G96 ) MLS 4.4 kmCEN8.80.551343.9113.6-0.92Listed in damocloid
Obs: 5 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
C/2019 JU6 (ATLAS)
(2019 JU6)
2019( T05 ) ATLAS-HKO 4.9 km comet 1930.991482.04383-1.50Listed in damocloid
Obs: ( 2d)
MPC
JPL
2019 KE72019( G96 ) MLS 4.6 km CEN 11.70.701083.4819.9-0.22Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2019 KF72019( I41 ) ZTF 4.4 kmCEN6.10.5352.909.42.68Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2019 KV422019( F51 ) Pan-STARRS 16.4 kmCEN11.30.57204.8217.82.72Obs: ( 29d) MPC
JPL
2019 NN102019(F51)Pan-STARRS 14.4 kmCEN6.10.4263.558.72.81Obs: ( 54d)
Johnston's Archive: unusual;
MPC
JPL
2019 PN22019(F51)Pan-STARRS 12.3 kmCEN25.20.921132.0148.3-0.47Listed in damocloid
Obs: (165d)
Johnston's Archive: damocloid;
MPC
JPL
2019 RJ22019( G96 ) MLS 8.4 kmCEN9.80.48235.0714.52.74Obs: 3 opposition(s)
Johnston's Archive: centaur;
MPC
JPL
2019 RZ162019( F51 ) Pan-STARRS 12.3 kmCEN6.70.6552.3311.02.49Obs: (106d)
Johnston's Archive: unusual;
MPC
JPL
2019 UL142019(F51)Pan-STARRS 12.9 kmCEN10.00.51194.8915.22.77Obs: ( 35d)
Johnston's Archive: unusual;
MPC
JPL
2019 UT752019(F51)Pan-STARRS 1670 mCEN7.60.7851.6713.52.19Obs: ( 5d) MPC
JPL
2019 YJ62019(F51)Pan-STARRS 11.8 km TNO 37.70.93222.5672.81.95Listed in damocloid
Obs: (189d)
Johnston's Archive: damocloid;
MPC
JPL
2020 BF132020(F51)Pan-STARRS 19.4 km CEN 7.80.46364.2511.32.43Obs: 2 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2020 BV642020( G96 ) MLS 3.2 kmCEN12.00.69103.7920.32.61Obs: ( 27d) MPC
JPL
2020 DN22020( I41 ) ZTF 4.2 kmCEN6.10.46193.318.92.68Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2020 EP2020( G96 ) MLS 2.8 kmCEN10.50.76762.4818.50.93Listed in damocloid
Obs: ( 74d)
Johnston's Archive: damocloid;
MPC
JPL
2020 FH242020(G96)MLS3.5 kmCEN14.30.77293.2725.32.22Listed in damocloid
Obs: ( 57d)
MPC
JPL
2020 HB112020(G96)MLS4.5 kmCEN16.50.711474.8428.2-1.81Listed in damocloid
Obs: ( 37d)
Johnston's Archive: damocloid;
MPC
JPL
2020 HK932020( F52 ) Pan-STARRS 22.1 kmCEN7.20.57173.1411.32.58Obs: ( 29d) MPC
JPL
2020 KD62020( F51 ) Pan-STARRS 1500 mCEN13.10.87391.6824.51.61Listed in damocloid
Obs: ( 39d)
Johnston's Archive: damocloid;
MPC
JPL
2020 KH72020(F51)Pan-STARRS 14.2 kmCEN7.90.501063.9511.90.06Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2020 KU72020(F51)Pan-STARRS 14.0 km TNO 34.80.881044.2065.4-0.44Listed in damocloid
Obs: 2 opposition(s)
Johnston's Archive: damocloid;
MPC
JPL
2020 ML12020(F51)Pan-STARRS 11.3 kmTNO55.10.95832.541080.35Listed in damocloid
Obs: ( 31d)
Johnston's Archive: damocloid;
MPC
JPL
2020 OP72020(F51)Pan-STARRS 11.8 km CEN 28.70.90803.0054.40.56Listed in damocloid
Obs: ( 53d)
MPC
JPL
2020 OP82020(F51)Pan-STARRS 16.1 kmCEN14.10.72303.9424.32.34Obs: (142d) MPC
JPL
2020 OR52020(F51)Pan-STARRS 13.2 kmCEN6.20.381673.898.6-1.14Listed in damocloid
Obs: 4 opposition(s)
Johnston's Archive: unusual;
MPC
JPL
2020 OS52020(F51)Pan-STARRS 11.5 kmCEN6.80.681562.1811.4-0.76Listed in damocloid
Obs: ( 8d)
Johnston's Archive: unusual;
MPC
JPL
2020 OS862020(F51)Pan-STARRS 14.0 kmCEN8.30.6173.2313.32.61Obs: ( 29d) MPC
JPL
2020 QN62020(F51)Pan-STARRS 15.0 km TNO 6730.99774.8213410.62Listed in damocloid
Obs: (501d)
MPC
JPL
2020 QP422020(F51)Pan-STARRS 14.0 km CEN 7.90.50203.9611.92.66Obs: ( 60d) MPC
JPL
2020 SJ52020(F51)Pan-STARRS 11.9 kmCEN18.20.86772.6233.70.71Listed in damocloid
Obs: ( 52d)
MPC
JPL
2020 SL192020( F52 ) Pan-STARRS 23.2 kmCEN7.50.62222.8212.22.44Obs: (165d) MPC
JPL
2020 SV792020( G96 ) MLS 810 mCEN17.70.8962.0333.32.00Listed in damocloid
Obs: ( 26d)
MPC
JPL
2020 SW72020( F52 ) Pan-STARRS 27.0 kmCEN8.90.48154.6913.22.81Obs: 2 opposition(s) MPC
JPL
2020 TK92020( G96 ) MLS 1.5 kmCEN20.90.881062.4939.3-0.26Listed in damocloid
Obs: ( 30d)
MPC
JPL
2020 TQ142020(G96)MLS1.3 kmCEN6.00.62272.279.72.37Obs: ( 67d) MPC
JPL
2020 TU82020( F52 ) Pan-STARRS 21.5 kmCEN6.50.65472.3110.71.97Obs: ( 6d) MPC
JPL
2020 VS62020( G96 ) MLS 610 mCEN9.60.821611.7617.5-0.95Listed in damocloid
Obs: ( 5d)
MPC
JPL
2021 AD32021( F51 ) Pan-STARRS 14.2 kmCEN8.40.54293.9213.02.50Obs: ( 3d) MPC
JPL
2021 AE32021(F51)Pan-STARRS 14.6 kmCEN8.30.43324.7711.92.57Obs: ( 3d) MPC
JPL
2021 CE222021( F52 ) Pan-STARRS 2770 mCEN7.30.7771.6912.82.22Obs: ( 57d) MPC
JPL
2021 CT32021( F51 ) Pan-STARRS 13.4 kmCEN7.40.421604.2910.6-1.34Listed in damocloid
Obs: ( 26d)
MPC
JPL
2021 DL12021( G96 ) MLS 6.4 km TNO 35.30.891493.9366.7-1.89Listed in damocloid
Obs: 3 opposition(s)
MPC
JPL
2021 DN22021( F51 ) Pan-STARRS 14.2 km CEN 22.20.82113.9940.32.56Listed in damocloid
Obs: (135d)
MPC
JPL
2021 GQ572021(F51)Pan-STARRS 12.5 km TNO 86.30.961253.46169-1.25Listed in damocloid
Obs: (112d)
MPC
JPL
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Characteristics

Examples


See also

Related Research Articles

<span class="mw-page-title-main">Centaur (small Solar System body)</span> Type of solar system object

In planetary astronomy, a centaur is a small Solar System body that orbits the Sun between Jupiter and Neptune and crosses the orbits of one or more of the giant planets. Centaurs generally have unstable orbits because they cross or have crossed the orbits of the giant planets; almost all their orbits have dynamic lifetimes of only a few million years, but there is one known centaur, 514107 Kaʻepaokaʻawela, which may be in a stable orbit. Centaurs typically exhibit the characteristics of both asteroids and comets. They are named after the mythological centaurs that were a mixture of horse and human. Observational bias toward large objects makes determination of the total centaur population difficult. Estimates for the number of centaurs in the Solar System more than 1 km in diameter range from as low as 44,000 to more than 10,000,000.

Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-type or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet, but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Jupiter Tisserand invariant (TJ) of 2 or less, while Akimasa Nakamura defines this group with the following orbital elements:

(65407) 2002 RP120, provisional designation 2002 RP120, is a trans-Neptunian object and damocloid from the outer Solar System. Its orbit is retrograde and comet-like, and has a high eccentricity. It was discovered on 4 September 2002 by astronomers with the LONEOS survey at Anderson Mesa Station, Arizona, in the United States. The unusual object measures approximately 14.6 kilometers (9.1 miles) in diameter and is likely elongated in shape. It is a slow rotator and potentially a tumbler as well. The object was probably ejected from the ecliptic by Neptune.

20461 Dioretsa is a centaur and damocloid on a retrograde, cometary-like orbit from the outer Solar System. It was discovered on 8 June 1999, by members of the LINEAR team at the Lincoln Laboratory Experimental Test Site near Socorro, New Mexico, United States. The highly eccentric unusual object measures approximately 14 kilometers in diameter. It was named Dioretsa, the word "asteroid" spelled backwards.

<span class="nowrap">(528219) 2008 KV<sub>42</sub></span>

(528219) 2008 KV42 (provisional designation:2008 KV42; nicknamed Drac) is a trans-Neptunian object and the first one with a retrograde orbit to be discovered. This retrograde motion with an orbital inclination of 103° suggests that it is the missing link between its source in the Hills cloud and Halley-type comets, thus providing further insight into the evolution of the outer Solar System. The object measures approximately 77 kilometers (48 miles) in diameter. With a semi-major axis of 42 AU, it takes about 269 years to complete an orbit around the Sun.

(434620) 2005 VD, provisional designation 2005 VD, is a centaur and damocloid on a retrograde orbit from the outer Solar System, known for having the second most highly inclined orbit of any small Solar System body, behind 2013 LA2. It was the most highly inclined known object between 2005 and 2013. The unusual object measures approximately 6 kilometers in diameter.

<span class="nowrap">(612093) 1999 LE<sub>31</sub></span>

(612093) 1999 LE31, prov. designation: 1999 LE31, is a centaur and damocloid on a retrograde and eccentric orbit from the outer region of the Solar System. It was first observed on 12 June 1999, by astronomers with the LINEAR program at the Lincoln Lab's ETS near Socorro, New Mexico, in the United States. The unusual object measures approximately 17 kilometers (11 miles) in diameter.

2005 VX3 is trans-Neptunian object and retrograde damocloid on a highly eccentric, cometary-like orbit. It was first observed on 1 November 2005, by astronomers with the Mount Lemmon Survey at the Mount Lemmon Observatory in Arizona, United States. The unusual object measures approximately 7 kilometers (4 miles) in diameter. It has the 3rd largest known heliocentric semi-major axis and aphelion. Additionally its perihelion lies within the orbit of Jupiter, which means it also has the largest orbital eccentricity of any known minor planet.

2000 DG8 is a dark centaur and damocloid on a retrograde and highly eccentric orbit from the outer region of the Solar System. It was first observed on 25 February 2000, by astronomers with the LINEAR program at the Lincoln Lab's ETS near Socorro, New Mexico, United States. It has not been observed since 2001. The unusual object measures approximately 16 kilometers (9.9 miles) in diameter.

<span class="mw-page-title-main">1996 PW</span>

1996 PW is an exceptionally eccentric trans-Neptunian object and damocloid on an orbit typical of long-period comets but one that showed no sign of cometary activity around the time it was discovered. The unusual object measures approximately 10 kilometers in diameter and has a rotation period of 35.4 hours and likely an elongated shape.

2013 LA2 is a centaur and damocloid on a cometary-like and retrograde orbit from the outer Solar System, suggesting that it is an extinct comet. It was first observed on 1 June 2013 by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, in the United States. The object measures approximately 1.8 kilometers (1.1 miles) in diameter. It holds the record for having the highest orbital inclination of any known minor planet.

(336756) 2010 NV1, prov. designation: 2010 NV1, is a highly eccentric planet crossing trans-Neptunian object, also classified as centaur and damocloid, approximately 52 kilometers (32 miles) in diameter. It is on a retrograde cometary orbit. It has a barycentric semi-major axis (average distance from the Sun) of approximately 286 AU.

<span class="nowrap">(127546) 2002 XU<sub>93</sub></span>

(127546) 2002 XU93, provisional designation 2002 XU93, is a trans-Neptunian object and centaur on highly inclined and eccentric orbit in the outer region of the Solar System. It measures approximately 170 kilometers (110 mi) in diameter and is one of few objects with such an unusual orbit. It was discovered on 4 December 2002, by American astronomer Marc Buie at the Kitt Peak National Observatory in Arizona, United States.

2017 MB7 is a trans-Neptunian object and damocloid on a cometary-like orbit from the outer Solar System, approximately 6 kilometers (4 miles) in diameter. It was first observed on 22 June 2017 by the Pan-STARRS survey at Haleakala Observatory in Hawaii, United States. This unusual object has the largest heliocentric aphelion, semi-major axis, orbital eccentricity and orbital period of any known periodic minor planet, even larger than that of 2014 FE72; it is calculated to reach several thousand AU (Earth-Sun) distances at the farthest extent of its orbit.

(342842) 2008 YB3, provisional designation: 2008 YB3, is a sizable centaur and retrograde damocloid from the outer Solar System, approximately 67 kilometers (42 miles) in diameter. It was discovered on 18 December 2008, by astronomers with the Siding Spring Survey at the Siding Spring Observatory in Australia. The minor planet was numbered in 2012 and has since not been named.

(468861) 2013 LU28, provisional designation 2013 LU28 is a highly eccentric trans-Neptunian object, retrograde centaur and damocloid from the outer regions of the Solar System. It was discovered on 8 June 2013 by astronomers with the Mount Lemmon Survey at the Mount Lemmon Observatory in Arizona, United States. The object is unlikely a dwarf planet as it measures approximately 110 kilometers (68 miles) in diameter. It was numbered in 2016 and has not been named since.

(523635) 2010 DN93, provisional designation 2010 DN93, is a trans-Neptunian object from in the scattered disc located in the outermost region of the Solar System. It was discovered on 26 February 2010, by astronomers with the Pan-STARRS survey at Haleakala Observatory on the island of Maui, Hawaii, in the United States. Assuming a low albedo, the object is estimated at approximately 490 kilometers (300 miles) in diameter. It was numbered in 2018 and remains unnamed.

2011 MM4, provisional designation: 2011 MM4, is a sizable centaur and retrograde damocloid from the outer Solar System, approximately 64 kilometers (40 miles) in diameter. It was discovered on 24 June 2011, by astronomers with the Pan-STARRS 1 at the Haleakala Obs. in Hawaii.

(523676) 2013 UL10 (prov. designation:2013 UL10) is a reddish centaur with cometary activity orbiting the Sun between Jupiter and Uranus. It was discovered on 18 August 2010, by a team of astronomers with the Pan-STARRS survey at the Haleakalā Observatory, Hawaii. It is the first centaur known to have both comet-like activity and red surface colors. It is also one of the smallest centaurs, with a nucleus of no more than 10 kilometers (6.2 miles) in diameter. As of 2021, it has not been named.

References

  1. "Unusual Minor Planets". Minor Planet Center. Retrieved 14 November 2018.
  2. 1 2 "List Of Other Unusual Objects". Minor Planet Center. Retrieved 19 August 2021.
  3. Fernández, Yanga R.; Jewitt, David C.; Sheppard, Scott S. (July 2005). "Albedos of Asteroids in Comet-Like Orbits". The Astronomical Journal. 130 (1): 308–318. Bibcode:2005AJ....130..308F. CiteSeerX   10.1.1.507.2206 . doi:10.1086/430802.
  4. Gladman, B.; Marsden, B. G.; Vanlaerhoven, C. (2008). "Nomenclature in the Outer Solar System" (PDF). The Solar System Beyond Neptune: 43. Bibcode:2008ssbn.book...43G.}
  5. Davies, John K.; Tholen, David J.; Whiteley, Robert J.; Green, Simon F.; Hillier, Jon K.; Foster, Michael J.; et al. (March 2001). "The Lightcurve and Colors of Unusual Minor Planet 1998 WU 24". Icarus. 150 (1): 69–77. Bibcode:2001Icar..150...69D. doi:10.1006/icar.2000.6554.