Table A.1
Data on new asteroid pairs.
𝒩o | Primary component | Secondary component | H1 | ΔH | dphase | est.age | P1/2 | P2/Np | note |
---|---|---|---|---|---|---|---|---|---|
[mag] | [mag] | (m/s) | [kyr] | ||||||
1 | 14191 (1998 XR28) | 574338 (2010 JY46) | 13.97 | 4.42 | 9.6 | ![]() |
0.006 | 0.041 | p |
2 | 14593 Everett | 2005 WQ213 | 15.44 | 2.83 | 9.11 | ![]() |
0.793 | 0.041 | pb |
3 | 44599 (1999 RA2) | 614882 (2000 WS11) | 15.95 | 2.35 | 23.73 | ![]() |
0.055 | 0.234 | fb |
4 | 44670 (1999 RQ183) | 2015 RW129 | 16.6 | 3.35 | 0.97 | ![]() |
0.022 | 0 | p |
5 | 44938 (1999 VV50) | 2009 SF406 | 15.25 | 3.64 | 3.66 | ![]() |
0.013 | 0 | c |
6 | 70150 (1999 NS31) | 2016 JC48 | 16.39 | 2.22 | 10.14 | ![]() |
0.004 | 0.016 | c |
7 | 81069 (2000 EW77) | 2014 WL523 | 15.82 | 2.72 | 14.92 | ![]() |
0.168 | 0.016 | pb |
8 | 96658 (1999 JC6) | 637279 (2015 EA16) | 15.74 | 2.33 | 23.39 | ![]() |
1 | 0.091 | b |
9 | 107438 (2001 DK16) | 2009 HL15 | 16.4 | 2.23 | 13.17 | ![]() |
0.438 | 0.036 | b |
10 | 111632 (2002 AB142) | 2018 QX15 | 16.6 | 2.37 | 6.52 | ![]() |
0 | 0.006 | pc |
11 | 136924 (1998 KX5) | 2009 TL53 | 16.28 | 2.49 | 23.39 | ![]() |
0.838 | 0.392 | b |
12 | 142377 (2002 RW249) | 2016 GV293 | 16.82 | 1.97 | 16.34 | ![]() |
0.910 | 0.023 | pb |
13 | 148265 (2000 FQ37) | 2015 FY305 | 16.29 | 2.36 | 20.1 | ![]() |
0 | 0.165 | pc |
14 | 156163 (2001 TF112) | 2012 TJ110 | 16.16 | 2.04 | 10.5 | ![]() |
0.162 | 0.042 | pb |
15 | 178457 (1999 RS29) | 531019 (2012 BM159) | 15.91 | 1.97 | 9.68 | ![]() |
0.207 | 0.009 | fb |
16 | 189428 (1998 HB2) | 2004 RU235 | 18.13 | 1.69 | 21.54 | ![]() |
0.290 | 0.033 | pb |
17 | 200973 (2002 CM95) | 2017 BX191 | 17.06 | 2.04 | 8.11 | ![]() |
0 | 0.010 | c |
18 | 202035 (2004 RK77) | 2018 SG19 | 16.89 | 1.91 | 10.79 | ![]() |
0.010 | 0.024 | c |
19 | 208497 (2001 VH105) | 2019 SG147 | 17.86 | 1.94 | 5.79 | ![]() |
0.007 | 0.001 | c |
20 | 211512 (2003 QW43) | 2014 PG94 | 17.3 | 2.2 | 9.27 | ![]() |
0.009 | 0.006 | pc |
21 | 215512 (2002 UF14) | 2019 RS75 | 15.92 | 3.98 | 14.91 | ![]() |
0.497 | 0.003 | pb |
22 | 220222 (2002 VQ107) | 2020 TT67 | 16.63 | 2.57 | 17.74 | ![]() |
0 | 0.145 | fc |
23 | 220241 (2002 XF25) | 2018 AH65 | 16.88 | 2.05 | 3.34 | ![]() |
0 | 0 | pc |
24 | 231407 (2006 YU10) | 2015 XN498 | 16.98 | 2.02 | 8.04 | ![]() |
0 | 0.007 | pc |
25 | 237761 (2001 YN148) | 2019 JZ137 | 17.05 | 2.07 | 16.03 | ![]() |
0 | 0.050 | fc |
26 | 269964 (2000 SC291) | 628959 (2017 XQ19) | 18.11 | 1.17 | 2.43 | ![]() |
0.424 | 0.000 | b |
27 | 288902 (2004 RR320) | 2015 OU175 | 16.89 | 1.72 | 4.24 | ![]() |
0.185 | 0.001 | fpb |
28 | 304000 (2006 BV229) | 2011 BB69 | 17.89 | 0.98 | 12.85 | ![]() |
0.024 | 0.023 | c |
29 | 312647 (2010 GM101) | 558611 (2015 BC34) | 17.3 | 1.22 | 7.68 | ![]() |
0 | 0.009 | c |
30 | 329278 (1999 VA107) | 2014 HC250 | 17.49 | 1.81 | 6.74 | ![]() |
1 | 0 | pb |
31 | 333128 (2011 WD76) | 2021 VX9 | 17.35 | 2.75 | 6.66 | ![]() |
0.017 | 0.002 | p |
32 | 408807 (2000 SU248) | 2009 QZ67 | 17.57 | 1.19 | 21.87 | ![]() |
0.065 | 0.159 | p |
33 | 418156 (2008 AW97) | 2008 CR98 | 17.77 | 1.13 | 12.55 | ![]() |
0.017 | 0.034 | fc |
34 | 451414 (2011 QR46) | 2019 RP93 | 17.13 | 2.03 | 22.06 | ![]() |
0 | 0.034 | c |
35 | 461548 (2003 VN3) | 612428 (2002 QU107) | 18.09 | 1.02 | 21 | ![]() |
0 | 0.067 | pc |
36 | 469759 (2005 QM29) | 2016 QZ123 | 18.25 | 2.18 | 6.71 | ![]() |
1 | 0 | pb |
37 | 487651 (2015 OY71) | 2021 VA24 | 18.05 | 1.61 | 10.4 | ![]() |
0 | 0.007 | pc |
38 | 565005 (2017 BZ4) | 2021 VW78 | 18.0 | 1.05 | 11.78 | ![]() |
1 | 0.001 | b |
39 | 2002 QN32 | 2021 TQ46 | 18.01 | 2.82 | 14.37 | ![]() |
1 | 0.016 | b |
40 | 2005 SK228 | 2019 RW47 | 18.88 | 1.5 | 13.28 | ![]() |
0.048 | 0.039 | fpc |
Notes. The uncertainties of the age estimates are the 5th and 95th percentiles of the formation age distribution. Values of P1/2 larger than 0.01 for dphase ≤ 10 m/s, and 0.05 for pairs with greater dphase indicate that the pair is in a region of uniform orbit density. Lower values indicate the possibility of a cluster. The ratio P2/Np indicates the probability coincidental nature of a pair with P2/Np > 0.1. Note: p - has data available on physical properties, c-nonuniform density region, possibly clusterization, f - family member, b-uniform density region, clearly an asteroid pair.
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