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Table A.1

Proper orbital elements (and their formal uncertainties) of the Adelaide family members.

Asteroid aP δaP eP δeP sinIP δsinIP H
[au] [au] [mag]
525 Adelaide 2.2452003 0.0000072 0.14870 0.00075 0.11703 0.00029 12.1
422 494 2014 SV342 2.2456475 0.0000186 0.14822 0.00074 0.11732 0.00030 18.2
452 322 2000 GG121 2.2462281 0.0000151 0.14904 0.00069 0.11706 0.00029 18.4
463 394 2013 GV28 2.2450021 0.0000032 0.14869 0.00075 0.11704 0.00029 18.6
475 474 2006 SZ152 2.2451926 0.0000031 0.14839 0.00076 0.11701 0.00031 18.3
486 081 2012 UX41 2.2455429 0.0000241 0.14838 0.00077 0.11712 0.00033 18.6
504 375 2007 VV73 2.2456417 0.0000167 0.14842 0.00075 0.11724 0.00032 18.5
517 580 2014 UZ170 2.2456581 0.0000198 0.14859 0.00070 0.11693 0.00030 18.5
534 611 2014 UC204 2.2455882 0.0001423 0.14862 0.00078 0.11700 0.00030 18.2
545 614 2011 SA45 2.2456659 0.0000081 0.14813 0.00074 0.11701 0.00025 18.3
2004 HU76 2.2456679 0.0000084 0.14816 0.00070 0.11703 0.00027 18.9
2004 HJ85 2.2456534 0.0000102 0.14849 0.00074 0.11745 0.00027 19.0
2005 UF193 2.2456726 0.0000105 0.14869 0.00074 0.11738 0.00030 18.5
2005 UK370 2.2456739 0.0000167 0.14907 0.00072 0.11718 0.00031 18.8
2005 VP83 2.2456279 0.0000542 0.14876 0.00076 0.11721 0.00031 18.2
2006 SK449 2.2458731 0.0000035 0.14882 0.00072 0.11697 0.00029 18.1
2007 VT345 2.2452387 0.0000008 0.14873 0.00074 0.11713 0.00029 18.5
2008 ET179 2.2457280 0.0000385 0.14891 0.00071 0.11711 0.00031 18.6
2008 US17 2.2455787 0.0000294 0.14908 0.00074 0.11716 0.00030 18.3
2008 UR182 2.2456539 0.0000181 0.14854 0.00074 0.11732 0.00030 18.2
2009 WJ157 2.2458738 0.0000013 0.14838 0.00075 0.11713 0.00031 18.7
2010 UF125 2.2456849 0.0000342 0.14888 0.00075 0.11718 0.00031 18.5
2010 VC228 2.2456836 0.0000070 0.14916 0.00067 0.11703 0.00028 18.2
2010 VF260 2.2456700 0.0000071 0.14928 0.00066 0.11710 0.00023 18.4
2010 XB115 2.2457353 0.0001025 0.14873 0.00071 0.11707 0.00030 18.7
2012 TM342 2.2450178 0.0000050 0.14879 0.00074 0.11702 0.00029 19.1
2014 AD31 2.2452038 0.0000032 0.14880 0.00074 0.11707 0.00030 18.4
2014 EM164 2.2450582 0.0000004 0.14874 0.00075 0.11705 0.00029 18.9
2014 JA2 2.2456762 0.0000122 0.14896 0.00072 0.11716 0.00030 18.0
2014 JY105 2.2461386 0.0000002 0.14852 0.00072 0.11708 0.00030 18.9
2014 WM167 2.2457519 0.0000693 0.14877 0.00073 0.11709 0.00031 18.6
2015 BE285 2.2453595 0.0000021 0.14835 0.00076 0.11718 0.00030 18.8
2015 HU72 2.2455920 0.0000978 0.14809 0.00080 0.11722 0.00032 18.6
2015 RM186 2.2461823 0.0000252 0.14901 0.00071 0.11700 0.00029 18.5
2015 TD44 2.2446159 0.0000033 0.14867 0.00077 0.11703 0.00029 19.0
2015 UR18 2.2456509 0.0000109 0.14852 0.00070 0.11740 0.00027 18.9
2015 XZ90 2.2450035 0.0000054 0.14869 0.00075 0.11704 0.00029 18.5
2016 AL322 2.2453643 0.0000108 0.14851 0.00075 0.11734 0.00029 18.7
2016 CX104 2.2446077 0.0000017 0.14872 0.00077 0.11708 0.00029 18.9
2016 FA34 2.2453296 0.0000112 0.14858 0.00075 0.11721 0.00030 18.6
2016 GO11 2.2447194 0.0000018 0.14874 0.00076 0.11707 0.00029 18.5
2016 QE71 2.2455566 0.0001558 0.14823 0.00080 0.11717 0.00031 18.4
2017 AU38 2.2456416 0.0000150 0.14890 0.00071 0.11703 0.00028 18.5
2017 HL72 2.2461432 0.0000007 0.14873 0.00072 0.11696 0.00030 18.9
2017 TG26 2.2450745 0.0000020 0.14883 0.00075 0.11708 0.00028 18.7
2017 UF65 2.2451124 0.0000014 0.14866 0.00075 0.11719 0.00029 19.1
2017 WP50 2.2449717 0.0000034 0.14873 0.00075 0.11713 0.00029 19.0
2016 UO110 2.2455685 0.0000310 0.14794 0.00079 0.11743 0.00033 18.9
2017 RS100 2.2446158 0.0000025 0.14888 0.00076 0.11699 0.00029 19.1
2019 TC62 2.2462278 0.0000033 0.14887 0.00070 0.11707 0.00030 18.9
2019 YE29 2.2460516 0.0000007 0.14870 0.00072 0.11716 0.00029 19.4

Notes.The Adelaide family membership as of February 2021. The first column lists the asteroid number (if numbered) and identification. The next six columns provide the asteroid’s proper elements (aP, eP, sinIP) and their formal uncertainties (δaP, δeP, δsinIP) determined by the methods described in the appendix. The last column gives the absolute magnitude H from the MPC database. Being a by-product of an orbit determination procedure from observations of sky surveys, the listed H values might be uncertain. The asteroids whose data are listed in roman font are multi-opposition, while the last four (in italics) are single-opposition. In the latter cases, the uncertainties on the proper elements are only formal since the uncertainty of the osculating elements may currently be higher.

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