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举报邮箱：Other reports of asteroid/TNO companions
Other Reports of Asteroid/TNO Companions
compiled by Wm. Robert Johnston
last updated 29 December 2017
This listing of other reported/postulated asteroid/TNO companions may be incomplete.
It includes 293 asteroids:
269 suggested binaries, plus 17 cases where subsequent analysis and/or observations have refuted the existence of a companion, plus one object suggested to have rings, plus six confirmed binaries where an unconfirmed third component is proposed.
Note there are two distinct reports each for (2) Pallas and (146) Lucina.
Some diameter figures are triaxial dimensions from shape models which supercede the interpretations suggesting the presence of a companion.
Additional data for these asteroids/TNOs are available on .
(Note that the delineation between the most likely candidates on this list and the least likely candidates on the previo corrections are welcome.)
designationprimarya (AU)primaryeprimarydiameter (km)companionseparation (km)companiondiameter (km)notes
(2) Pallas2.7720.231570 x 525 x 482?129 May 1978 based on occulation data by R. Radick et al.
7501751980 by E. Hege, W. Cocke, E. Hubbard, J. Christou, and R. Radick based on sp refuted by 29 May 1983 occultation observations
(6) Hebe2.4260.202185900205 Mar 1977 by P. D. Maley based on occultation data (nicknamed "Jebe"); see
(9) Metis2.3860.12219111006011 Dec 1979 by V additional reports 23 Dec 1979-23 Feb 1980 by Wang S., Wu Y., Bao M., Deng L., and Wu S. at Purple Mt. Obs.; discounted by 1982 see , ,
(12) Victoria2.3340.221127??1980 by E. Hege, W. Cocke, E. Hubbard, J. Christou, and R. Radick based on sp irregular shape suggested in 1995 by D. Mitchell, S. Ostro, and K. Rosema based on radar observations
(15) Eunomia2.6440.188259300180reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi base model shown unstable in 1985
(18) Melpomene2.2960.21914111006511 Dec 1978 by R. M. Williamon based designated S/; see
(21) Lutetia2.4340.165961000??Mar 2007 by V. Busarev, V. Prokofeva, and V. Bochkov based
no satellite observed during Rosetta flyby in 2010
(29) Amphitrite2.5550.072227??suggested 1979 by E. Tedesco as interpretation of lightcurve data
(39) Laetitia2.7690.114145 x 130 x 120168120 x 70 x 70reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(43) Ariadne2.2030.169728570 x 40 x 40reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(44) Nysa2.4230.14970 x 70 x 608350 x 25 x 25reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(46) Hestia2.5260.172124??reported 1981 by F. Scaltriti, V. Zappala, and A. W. Harris based on lightcurve data
(49) Pales3.0940.228148??reported 1979 by E. Tedesco based on lightcurve data
(51) Nemausa2.3660.067143??suggested 1979 by E. Tedesco as interpretation of lightcurve data
(61) Danae2.9830.16785 x 80 x 7510155 x 30 x 30reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(63) Ausonia2.3950.12810310090 x 60 x 55reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(65) Cybele3.4280.1102379001117 Oct 1979 by V. Rakhimov and O. Najmov at Ura-Tyube based see
(82) Alkmene2.7660.21960 x 55 x 506640 x 25 x 25reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(98) Ianthe2.6880.186111??suggested in Apr 2004 by R. Venable based on occultation observations
(129) Antigone2.8700.211130??suggested 1979 by E. Tedesco as interpretation of lightcurve data by F. Scaltriti and V. Zappala
(146) Lucina2.7190.0661321600618 Apr 1982 by J. Arlot, J. Lecacheux, C. Richardson, and W. Thuillot based see ,
500?reported 2003 from
astrometric observations by Kikwaya, Thuillot, ROcher, Martins, Arlot, and Angeli
(171) Ophelia3.1300.131104??reported 1979 by E. Tedesco based on lightcurve data
(182) Elsa2.4160.18644??reported 1984 by S. Dermott, A. W. Harris, and C. Murray based on long period
(192) Nausikaa2.4030.2469315050 x 40 x 40reported 1985 by A. Cellino, R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi based on lightcurve data
(234) Barbara2.3860.2455424?21?suggested in 2009 by M. Delbo, S. Ligori, A. Matter, A. Cellino, and J. Berthier based on thermal modeling
(249) Ilse2.3780.21637??reported 1987 by R. P. Binzel based on long period
(279) Thule4.2950.010113??suggested in 2010
(280) Philia2.9430.10743??reported 1987 by R. P. Binzel based on long period
(287) Nephthys2.3530.02362140?suspected 2003
(288) Glauke2.7610.20432200?15?reported 1983 by A. W. Harris based on long period
(302) Clarissa2.4060.11134~300?5?reported based on occultation observations by P. Dombrowski on 24 Jun 2004
(324) Bamberga2.6810.340221??suggested 2015 based on lightcurve data
(349) Dembowska2.9230.092217??suggested 1979 by E. Tedesco as interpretation of lightcurve data
(354) Eleonora2.7990.115165??suggested 1979 by E. Tedesco as interpretation of lightcurve data
(361) Bononia3.9620.214152??suggested 31 Jan 2002 by R. Venable
(385) Ilmatar2.8500.12294??reported 1989 by A. W. Harris based on long period
(407) Arachne2.6250.06998??reported 1989 by S. J. Weidenschilling based on long period
(423) Diotima3.0670.039177??1982 by H. J. Schober from lightcurve data
(433) Eros1.4580.22333 x 17 x 13??reported 1901 by C. Andre base later modeled as single elongated object, shape confirmed by NEAR Shoemaker
(437) Rhodia2.3880.24716??reported 1987 by R. P. Binzel based on long period
(508) Princetonia3.1660.009120??reported 1989 by A. W. Harris based on long period
(532) Herculina2.7740.176203975457 Jun 1978 by E. Bowell and M. A'Hearn at Lowell Obs. and J. McMahon at B designated S/) 1; see
(709) Fringilla2.9140.11291??reported 1984 by S. Dermott, A. W. Harris, and C. Murray based on long period
(772) Tanete3.0000.092143??based on occultation observations by R. Sumner and R. Nolthenius in Apr 2004; see
(893) Leopoldina3.0500.15075 x 6417054 x 24reported 29 Jan 1996 by EAON based on occultation data
(911) Agamemnon5.2710.0671672785reported Sep 2013 by B. Timerson et al. based on occultation data
(944) Hidalgo5.7360.66252??suggested 1979 by E. Tedesco based on lightcurve variation with solar phase angle
(1024) Hale2.8660.22548??suggested in Apr 2004 by R. Venable based on occultation observations
(1090) Sumida2.3590.22013??suggested in Oct 2012 by B. Warner based on lightcurve observations
(1103) Sequoia1.9330.09512???suggested 23 Mar 2015 by B. Warner based on lightcurve observations
(1220) Crocus(=1932 CU)3.0030.07218?20reported 1985 by R. P. Binzel based on long period
(1271) Isergina3.1470.11947.5??suggested Sep 2016 based on lightcurve data
(1355) Magoeba1.8530.0458.1????suggested Dec 2014 by B. Warner based on lightcurve observations
(1481) Tubingia(=1938 DR)3.0160.04637??reported 1987 by R. P. Binzel based on long period
(1580) Betulia(=1950 KA)2.1970.4876??reported 1979 by E. Tedesco based on long period
(1620) Geographos(=1951 RA)1.2450.3365.1 x 1.8??1994 by L. G. Karachkina, V. V. Prokof'eva, and V. P. Tarashchuk based on lightcurve data
(1627) Ivar1.8630.3978.4??suggested by Hoffmann and Geyer in 1990 based on lig single elogated object model preferred
(1656) Suomi1.8770.1247.9??suggested 2016 based on lightcurve data
(1829) Dawson2.2520.1208.1??suggested 2015 by Oey et al. based on lightcurve data
(1857) Parchomenko2.2440.1348.5??reported 7 Jun 2006
(1876) Napolitania1.9640.0483.2???suggested Dec 2015 by B. Warner based on lightcurve data
(1943) Anteros1.4300.2562.3???suggested Jun 2017 by B. Warner et al. based on lightcurve data
(1979) Sakharov2.3740.1004.8??suggested in July 2013 based on lightcurve observations
(2006) Polonskaya2.3240.1934.6??suggested based on lightcurve data
(2048) Dwornik1.9540.0422.6??suggested Jun 2016 by B. Warner based on lightcurve data
(2060) Chiron13.6380.382230320?ring system suggested by J. L. Ortiz et al. in 2015 based on reinterpretation of occultation observations
(2063) Bacchus1.0780.3491.1 x 0.5 x 0.5??suggested by Ostro et al. in 1999 based on radar observations, but single bilobated object model preferred
(2074) Shoemaker1.8000.0826???suggested in 2009 by Warner et al. based on reanalysis of 2003 lightcurve observations by R. D. Stephens
(2083) Smither1.8720.0514.4??suggested by B. D. Warner et al. in 2010 based on lightcurve observations
(2102) Tantalus1.2900.2992.1???suggested Dec 2014 by B. Warner based on lightcurve observations
(2483) Guinevere3.9720.27835.7??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(2501) Lohja2.4220.19611.8??suggested by D. Higgins and P. Pravec in Apr 2006 based on lightcurve observations
(2658) Gingerich 3.0680.28911.8??reported in Oct 2007 by L. A. Molnar and M. J. Haegert based on lig see
(2759) Idomeneus5.1840.06653.7??suggested 2016 based on lightcurve data
(2841) Puijo2.2520.0846.8??suggested in Dec 2004 by B. Warner based on lightcurve observations
(3076) Garber2.2380.1905.3??suggested by D. Higgins et al. in 2010 based on lightcurve observations
(3145) Walter Adams2.1920.2363.8??suggested by L. E. Owings et al. in 2010 based on lightcurve observations
(3146) Dato2.4330.2016.6???suggested 2014 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(3155) Lee2.3430.10111???suggested in Nov 2004 by W. Ryan, E. Ryan, and C. Martinez based on lightcurve
(3220) Murayama2.2260.1749???suggested in Oct 2005 by A. Tsuchikawa, S. Miyasaka, and H. Hamanowa based on lightcurve
(3352) McAuliffe1.8790.3692???suggested in Jul 2012 by B. D. Warner based on lightcurve observations
(3637) O扢eara2.5560.12412.6??suggested Dec 2016 by Macias based on lightcurve data
(3665) Fitzgerald2.4180.0899???suggested by P. Pravec in Jun 2006 based on lightcurve observations
(3682) Welther2.7550.32219.333?suggested in Apr 2004 by P. Szekely et ali based on lightcurve observations
(3704) Gaoshiqi2.4100.0519.8??suggested in July 2013 based on lightcurve observations
(3800) Karayusuf1.5780.0761.62??suggested 2008 based on lightcurve data
(3854) George1.8920.1345???suggested in 2006 by B. D. Warner et al. based on lightcurve observations
(3880) Kaiserman1.9460.0838.4???suggested 23 Mar 2015 by B. Warner based on lightcurve observations
(3923) Radzievskij3.9630.22329.9??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(4149) Harrison2.6660.12410.1??suggested Sep 2015 by Papini et al. based on lightcurve data
(4179) Toutatis(=1989 AC)2.5340.6304.6 x 2.4 x 1.9??1988 based on radar observations sugge in
modeled as one double-lobed object
(4182) Mount Locke2.7980.13410.4??suggested in 2008 by Behrend based on lightcurve observations
(4197) Morpheus(=1982 TA)2.2960.7723.04.42?1996 by V. V. Prokof'eva, N. M. Gaftonyuk, and V. P. Tarashchuk from Crimean Astrophysical Obs. base binary nature not reported from 1996 radar observations
(4217) Engelhardt2.3140.2139??suggested in April 2012 by B. D. Warner based on lightcurve observations
(4230) van den Bergh3.9460.13328.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(4486) Mithra(=1987 SB)2.1990.6631.85??reported in 2000 by Ostro et ali from radar observations made July-August 2000 showing bifurcation
(4555) Josefaperez2.2570.1993.13??suggested Dec 2015 by Oey based on lightcurve data
(4605) Nikitin2.2280.1544.6??suggested Oct 2017 based on lightcurve data
(4718) Araki2.3610.1595.94??suggested 2017 based on lightcurve data
(4769) Castalia(=1989 PB)1.0630.4831.8 x 0.80.750.7522 Aug 1989 by S. J. Ostro, J. F. Chandler, A. A. Hine, K. D. Rosema, I. I. Shapiro, and D. K. Yeomans based on Arecibo radar observations sugge now modeled as one double-lobed object
(4962) Vercherka2.6060.1469.95??suggested Sep. 2016 by Tomov et al. based on lightcurve data
(4963) Kanroku2.6000.16411.3??suggested Dec. 2016 by Marchini et al. based on lightcurve data
(5175) Ables1.9670.0397.2???suggested by B. D. Warner in Jun 2014 based on lightcurve observations
(5325) Silver2.3640.2198.9??suggested by D. Higgins et al. in 2010 based on lightcurve observations
( FE2.1970.4544.8???suggested Jun 2017 by B. Warner based on lightcurve data
( EA1.2710.5851.5???suggested Jun 2017 by B. Warner based on lightcurve data
( AM1.6980.6952.2?5??suggested Sep 2013 by B. Warner based on lightcurve observations
(5968) Trauger1.9090.0264.810??suggested Dec 2013 by B. Warner based on lightcurve observations
(6063) Jason2.2130.7661.4??&
(6170) Levasseur2.3520.3197???suggested by D. Higgins et al. in 2010 based on lightcurve observations
( XR12.2970.1376.0???suggested 2015 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(6602) Gilclark1.8710.0744.1??suggested by B. D. Warner in Mar 2014 based on lightcurve observations
( VW1.6960.4841.4?3??suggested by P. Pravec et al. in Jun 2005 based on lightcurve observations
(6815) Mutchler2.4320.1904???suggested 4 Nov 2006 by Photometric Survey for Asynchronous Binary Asteroids program based on lightcurve observations
(6853) Silvanomassaglia2.2610.1183.4??suggested Mar 2016 based on lightcurve data
(6901) Roybishop1.9430.1115.8??suggested by B. D. Warner et al. in 2010 based on lightcurve observations
(6944) Elaineowens2.3160.1394.8???suggested 2014 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(7027) Toshihanda3.9660.19623.8??suggested 2017 Jun by Warner and Stephens based on lightcurve data
( WN22.2420.0444.7??reported 6 Apr 2009 as inconclusive by Photometric Survey for Asynchronous Binary Asteroids program
(7144) Dossobuono2.4150.1436.0???suggested 2015 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(7173) Sepkoski1.9570.0134.2??suggested by B. D. Warner in Mar 2014 based on lightcurve observations
(7247) Robertstirling1.9170.1183??suggested Jan 2013 by B. Warner based on lightcurve observations
(7452) Izabelyuria3.1060.2018???suggested 7 May 2014 by C.-K. Chang et al. based on lightcurve observations
(7516) Kranjc2.3130.2406.0??suggested Apr 2008 by Oey based on lig not confirmed
(7560) Spudis1.9550.1055???&
(7758) Poulanderson2.3820.1855???suggested in Oct 2012 by B. Warner based on lightcurve observations
( CS1.1230.1651.60??suggested Mar 2016 based on lightcurve data
( PS15.1260.08438??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
( HL12.3930.2764???suggested Jul 2016 based on lightcurve data
(9671) Hermera2.6910.4365.5???suggested 2017 Jun by Salvaggio et al. based on lightcurve data
( MB2.6750.1898.7???suggested 2015 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
( FX32.6460.3374.72??suggested 2015 Dec by Marchini et al. based on lightcurve data
(1 PN2.3750.5442.8???suggested 2016 Sep by Warner based on lightcurve data
(10498) Bobgent2.2870.2592.7??suggested Sep 2017 based on lightcurve data
(11001) Andrewulff2.2270.2125???reported Apr 2012 as inconclusive by Photometric Survey for Asynchronous Binary Asteroids program
(11066) Sigurd1.3920.3752.8??reported in Dec 2004 by L. Benner et ali based on radar observations indicating a contact binary shape
(1 EK2.1960.2283.120??reported in 2006 and 2009 based on lightcurve observations
(11429) Demodokus5.2720.02938??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(11829) Tuvikene2.2840.1384.2???suggested 2015 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(1 WB11.8550.1523.6?6??suggested Sep 2013 by B. D. Warner and R. D. Stephens based on lightcurve observations
(1 SQ5.1120.08923.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(13921) Sgarbini2.2930.2315.3???suggested Sep 2014 by J. Oey based on lightcurve observations
(1 DB1.7160.4020.84??suggested by P. Pravec in Feb 2000 based on lightcurve observations
(1 BE22.2590.0985.7??reported 10 Jun 2010 as inconclusive by Photometric Survey for Asynchronous Binary Asteroids program
(15350) Naganuma2.3790.2764.422??suggested Nov 2005 by D. Pray et al. based on lightcurve observations
(1 UZ235.1280.02736??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(1 VN802.8780.24310??suggested 2008 by R. Behrend based on lig not confirmed
(1 HR503.9500.11218.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(1 NH2.3040.3133.8???suggested Dec 2014 by B. Warner based on lightcurve observations
(1 YN125.1250.09616.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(1 SB342.1690.1653.71??suggested Jun 2017 by Washburn and Ditteon based on lightcurve data
(1 FX683.9800.13922.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(1 RN105.1300.03221.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(19204) Joshuatree1.7190.2525.3???suggested Jun 2016 based on lightcurve data
(20000) Varuna(=2000 WR106)43.2070.052714??suggested in 2002 based on lightcurve observations
(20037) Duke1.8840.1213.3???suggested by B. D. Warner in 2010 based on lightcurve observations
(2 WG205.2190.14527??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(20460) Rodwhiteley1.8770.1442.7??suggested Jul 2017 based on lightcurve data
(2 T-12.4620.2415.17??suggested 2016 based on lightcurve data
(21047) Hodierna3.9820.17616.0??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(2 AN1063.9770.27618.8??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(23405) Nisyros3.9520.13014.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(2 FK121.9610.1003.5??suggested Jun 2015 by B. Warner based on lightcurve observations
(2 FJ12.7910.2766.9???suggested 2015 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(2 KK61.8920.0623.3??suggested Jan 2013 by B. Warner based on lightcurve observations
(25884) Asai1.9540.0801.9??suggested by B. D. Warner et al. in July 2012 based on lightcurve observations
(2 BC765.2260.04418??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(2 KJ2.3080.1784.9??reported Sep 2011 as probable but inconclusive by Photometric Survey for Asynchronous Binary Asteroids program
(3 OR51.9260.0303.3???suggested Dec 2014 by B. Warner based on lightcurve observations
(30935) Davasobel1.9030.1182.4??suggested Jun 2015 by V. Benishek based on lightcurve observations, refuted by followup observations with B. Warner prior to report
(31097) Nucciomula3.9600.10915.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(3 QC191.8980.0702.8??suggested Jun 2015 by B. Warner based on lightcurve observations, refuted by followup observations by B. Warner prior to report
(3 QY939.7020.26466??suggested in May 2004 by S. Sheppard and D. Jewitt based on long rotation period and lightcurve amplitude
(3 UF22.2850.2393.2???suggested 2014 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(3 BU4833.4330.384213??suggested in May 2004 by S. Sheppard and D. Jewitt based on long rotation period and lightcurve amplitude
(39405) Mosigkau3.9600.22214.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(39415) Janeausten3.9250.2099.4??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(4 UQ513.9720.1628.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(4 WX291.9350.0992.01??suggested 2017 Jun by Warner based on lightcurve data
(4 DF332.7620.3526.9??suggested in April 2012 by B. D. Warner based on lightcurve observations
(4 PS383.9530.24315.7??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(4 HB31.9010.0582.62??suggested Dec 2015 by B. Warner based on lightcurve data
(4 GN17139.3750.282147??suggested in May 2004 by S. Sheppard and D. Jewitt based on long rotation period and lightcurve amplitude
(5 RM885.2010.07019.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(5 KK171.4270.5251.06??suggested Dec 2016 by B. Warner based on lightcurve data
(5 UQ101.8370.1445???suggested by B. D. Warner in 2010 based on lightcurve observations
(5 KJ332.2760.1414.06??suggested 2017 based on lightcurve data
(5 SM1123.9810.13916.1??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(5 TY2295.2800.09521??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(5 VD1.9240.1332.8???suggested 2014 based on lightcurve data
(6 AG2513.9310.14611.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(6 BJ265.2010.04922.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(6 TA1975.2040.09516.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(6 UY1493.9360.2506.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(6 EK445.2500.08116.7??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(6 RF123.9480.2609.8??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(6 TU30.7870.4843??suggested by Hicks et al. in 2010 based on lightcurve observations
(6 BA191.9040.0682.7??suggested Jan 2013 by B. Warner based on lightcurve observations
(6 LO72.1520.8424.8???suggested Dec 2014 by B. Warner based on lightcurve observations
(70030) Margaretmiller1.9530.0851.4??suggested by B. D. Warner in Jan 2012 based on lightcurve observations
(7 AE552.6730.1245???suggested 7 May 2014 by C.-K. Chang et al. based on lightcurve observations
(7 RW1055.1590.09717.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(7 SB3105.2870.09918.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(8 UN1573.9350.1017.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(8 LY1.8900.4421.9???suggested 2007 based on lightcurve data
(8 JD60.8830.6331.46??suggested in Feb 2008 by D. Polishook and N. Brosch based on lightcurve observations
(8 CK330.9680.4150.8???suggested in Feb 2008 by D. Polishook and N. Brosch based on lightcurve observations
(8 BT653.9740.15018.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(8 VS781.7870.3082.6???suggested by P. Pravec in Feb 2002 based on lightcurve observations
(90377) Sedna(=2003 VB12)532.30.857995??suggested in 2004 by M. Brown et al. based on
long rotation period since refuted
(9 DO3.9330.10010.9??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(99 CR953.1470.1316.9??suggested 2012 based on lightcurve data
(02 QG83.9350.18510.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 VX605.1640.06920.9??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(01 YN422.5840.2542.3??suggested by B. D. Warner in Mar 2014 based on lightcurve observations
(98 YM313.9320.17110.0??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(05 AD215.2420.03820.0??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(00 AG905.1310.04417.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 RO953.9590.2428.9??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(99 KX41.4570.2931.41.7??suggested Dec 2013 by A. Carbognani based on lightcurve observations
(01 AU431.8970.3772.2???suggested Dec 2017 based on lightcurve data
(02 GY693.9710.11710.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 KL62.3070.5481.1???suggested Sep 2016 by B. Warner et al. based on lightcurve data
(06 KH895.3020.08917.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(00 DJ81.4110.2531.1???suggested Jun 2015 by B. Warner based on lightcurve observations
(01 DZ35.2380.05719.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 EU1075.2300.05419.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(00 SR2825.2000.11515.1??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(01 SD305.1500.05914.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(03 TK153.9730.2898.9??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(07 RQ2785.1880.04521.4??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(96 RT295.2530.01316.1??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(00 SU2363.9600.3077.7??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(04 FL1224.0000.0848.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(04 RO23.9690.0768.1??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 MQ30.9140.2741.08??suggested Sep 2016 by B. Warner based on lightcurve data
(01 SA2273.9750.2696.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 EZ1345.1670.10013.0??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(08 TB615.1320.01817.0??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(09 TV415.1020.05913.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(09 VR283.9600.1855.1??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(241528) Tubman3.9530.1387.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 NK423.9370.2897.8??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(03 NZ60.7930.4920.37??suggested in Feb 2008 by D. Polishook and N. Brosch based on lightcurve observations
(08 SO475.1460.22315.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 CU13.9770.2366.4??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(04 AG175.2790.09815??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(09 DN693.9380.1156.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 RK683.9330.1788.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(07 EM1813.9210.1147.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(07 SJ2.0140.5341.8???suggested Sep 2014 by A. Carbognani based on lightcurve observations
(02 FW51.3150.2180.48???suggested Mar 2017 by B. Warner based on lightcurve data
(08 QE373.9390.2026.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(09 KD51.0460.2610.78??reported 30 Jun 2010 by M. Hicks et al. based on lightcurve observations
(08 FU61.3240.5691.2???suggested Sep 2014 by B. D. Warner based on lightcurve observations
(04 EU453.9550.1336.7??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(04 FH112.2560.4472.0???suggested Sep 2014 by B. D. Warner based on lightcurve observations
(02 QA1233.9230.1675.9??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(02 RC683.9490.2666.2??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(01 UC2283.9620.2167??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(09 VG585.1880.05816.0??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(08 XE32.6080.5501.8?1.5??suggested Dec 2013 by A. Carbognani based on lightcurve observations
(08 GT875.1750.13715.6??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(11 PW85.2360.20213.4??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(09 VB35.3380.05517.8??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(13 CP3.9330.2055.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(11 MD112.5010.4970.8???suggested Mar 2016 based on lightcurve data
(08 SE2683.9550.2234.7??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
(06 UY640.9320.1570.4???suggested Mar 2016 based on lightcurve data
(11 EZ782.3950.5421.2???suggested Jul 2011 based on lightcurve observations by Photometric Survey for Asynchronous Binary Asteroids program
(13 BY452.1140.4070.50???suggested Jun 2016 by B. Warner based on lightcurve data
(04 FZ11.7940.5310.73???suggested Dec 2016 by B. Warner based on lightcurve data
(09 EC1.7680.3650.58???suggested Sep 2016 by B. Warner based on lightcurve data
(03 YU32.6770.3751.9???suggested Mar 2017 by B. Warner based on lightcurve data
(09 ES1.4350.3300.25???suggested Dec 2016 by B. Warner based on lightcurve data
2002 RM3.9530.2795.3??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
2003 SQ31742.6290.080265???suggested by P. Lacerda et al. in Sep 2013 based on lightcurve observations
2004 RZ1642.5520.6140.5???suggested by P. Pravec in Dec 2004 based on lightcurve observations
2010 MJ933.9670.244??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
2010 NB1153.9790.2745.5??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
2010 NO523.9640.2524.4??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
2010 OS143.9130.2536.1??suggested 4 Dec 2014 by S. Sonnett et al. based on high amplitude lightcurve
2010 WG953.2930.648113790?70?suggested May 2013 based on long rotation period by D. Rabinowitz et al.
2012 RV162.7570.6740.4???suggested Nov 2012 based on radar observations
2014 PL511.9510.4440.3???suggested Dec 2014 by B. Warner et al. based on lightcurve observations
2015 KN202.2880.0330.9???suggested Dec 2017 based on lightcurve data
2016 BU132.1510.5460.32???suggested Sep 2016 by B. Warner based on lightcurve data
2016 EV272.6930.6470.07???suggested Jun 2016 by B. Warner based on lightcurve data
Principal sources:
Cellino, A., R. Pannunzio, V. Zappala', P. Farinella, and P. Paolicchi, "Do we observe light curves of binary asteroids?," 1984, Astronomy and Astrophysics, 144:355-362.
Denissenko, Denis, 15 Feb 2002, .
Dunham, David, 27 Feb 2002, .
Higgins, David, 2006, .
JPL, 2003, .
"A list of suspected or known binary asteroids," 2 April 2002, .
Peebles, Curtis, 2000, Asteroids:
A History, Smithsonian Institution Press, Washington, DC.
Sonnett, S., A. Mainzer, T. Grav, J. Masiero, and J. Bauer, 2014, Binary candidates in the Jovian Trojan and Hilda populations from NEOWISE lightcurves, arXiv ().
Tedesco, E., "Binary asteroids:
evidence for their existence from lightcurves," 1979, Science, 203:905-907.
Tedesco, E., et ali, Mar 1998, IRAS Minor Planet Survey, version 4, .
Weidenschilling, Stuart J., Paolo Paolicchi, and Vincenzo Zappala', 1989, "Do asteroids have satellites?," pp. 643-658 in Asteroids, ed. by R. P. Binzel, T. Gehrels, and M. S. Matthews, Univ. of Arizona Press, Tucson, AZ.
& , 2017 by Wm. Robert Johnston.
Last modified 29 December 2017.
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