Table A.1
Athor Family: Complete and partial asteroid models.
Asteroid | λ1 | β1 | ϵ1 | λ2 | β2 | ϵ2 | P | Reference | |
---|---|---|---|---|---|---|---|---|---|
Number | Name/Designation | (deg) | (deg) | (deg) | (deg) | (deg) | (deg) | (h) | |
Complete asteroid models | |||||||||
161 | Athor | 174 | −4 | 92 | 356 | −9 | 101 | 7.2801 | This work |
757 | Portlandia | 269 | −46 | 142 | − | − | − | 6.5811 | This work |
1490 | Limpopo | 137 | 13 | 72 | 314 | 33 | 64 | 6.6516 | This work |
1998 | Titius | 54 | 16 | 81 | 236 | 2 | 81 | 6.126051 | Stephens et al. (2021) |
2194 | Arpola | 29 | −77 | 161 | 179 | −51 | 140 | 110.98 | This work |
3427 | Szentmartoni | 65 | −78 | 165 | 280 | −78 | 168 | 235.5 | This work |
3704 | Gaoshiqi | 60 | 48 | 41 | 225 | 49 | 44 | 9.778 | This work |
3865 | Lindbloom | 141 | −5 | 102 | 321 | 8 | 75 | 26.019 | This work |
4353 | Onizaki | 140 | −60 | 142 | 243 | −82 | 173 | 4.4297 | This work |
4760 | Jia–xiang | 102 | 67 | 24 | 284 | 82 | 13 | 14.962 | This work |
4839 | Daisetsuzan | 95 | 42 | 53 | 264 | 56 | 56 | 3.38381 | This work |
5160 | Camoes | 134 | 53 | 31 | 341 | 44 | 51 | 97.97 | This work |
6123 | Aristoteles | 90 | 19 | 62 | 271 | 40 | 59 | 5.745 | This work |
6247 | Amanogawa | 30 | −77 | 174 | 208 | −64 | 146 | 12.3657 | This work |
7111 | 1985QA1 | 146 | 26 | 71 | 332 | 42 | 41 | 11.2212 | This work |
8069 | Benweiss | 147 | 63 | 25 | 345 | 61 | 33 | 277.6 | This work |
8381 | Hauptmann | 147 | 48 | 34 | 344 | 62 | 36 | 4.69561 | This work |
10073 | Peterhiscocks | 72 | 65 | 19 | 232 | 68 | 28 | 442 | This work |
10368 | Kozuki | 331 | −81 | 170 | – | – | – | 4.09904 | Ďurech & Hanuš (2023) |
11977 | Leonrisoldi | 107 | 28 | 59 | 279 | 29 | 63 | 7.7904 | This work |
12425 | 1995VG2 | 26 | −82 | 164 | 147 | −60 | 152 | 8.32032 | This work |
20544 | Kimhansell | 158 | −67 | 165 | 286 | −63 | 147 | 477 | This work |
20566 | Laurielee | 121 | 47 | 48 | 284 | 44 | 40 | 14.774 | This work |
22761 | 1998YH4 | 132 | 20 | 76 | 318 | 14 | 70 | 167.9 | This work |
26660 | Samahalpern | 43 | −67 | 150 | 102 | −57 | 140 | 149.5 | This work |
33486 | 1999GN8 | 228 | 31 | 67 | 50 | 20 | 62 | 10.2325 | Ďurech & Hanuš (2023) |
36398 | 2000OQ45 | 22 | 66 | 25 | – | – | – | 10.9644 | Ďurech & Hanuš (2023) |
38233 | 1999NS57 | 136 | 44 | 36 | 327 | 54 | 50 | 5.3973 | This work |
42633 | 1998FW58 | 106 | −69 | 160 | 331 | −90 | 172 | 5.2415 | This work |
43120 | 1999XB49 | 283 | 81 | 16 | – | – | – | 118.94 | Ďurech & Hanuš (2023) |
56674 | 2000KS77 | 168 | −41 | 136 | 322 | −47 | 129 | 65.65 | This work |
82121 | 2001FQ77 | 166 | 65 | 31 | – | − | – | 6.4548 | Ďurech & Hanuš (2023) |
92599 | 2000PR19 | 49 | 56 | 28 | – | – | – | 9.7185 | Ďurech & Hanuš (2023) |
Asteroid | βP | δβ | P | Reference | |||||
---|---|---|---|---|---|---|---|---|---|
Number | Name/Designation | (deg) | (deg) | (h) | |||||
Partial asteroid models | |||||||||
2419 | Moldavia | −11 | 10 | 2.4114 | This work | ||||
4838 | Billmclaughlin | −5 | 12 | 5.2126 | This work | ||||
4845 | Tsubetsu | 25 | 13 | 3.03707 | This work | ||||
5343 | Ryzhov | −16 | 11 | 2.28943 | This work | ||||
6245 | Ikufumi | −1 | 9 | 2.92231 | This work | ||||
6855 | Armellini | −6 | 10 | 4.5725 | This work | ||||
15705 | Hautot | 35 | 15 | 2.78823 | This work | ||||
15909 | 1997TM17 | −1 | 6 | 5.2687 | This work | ||||
16258 | Willhayes | 39 | 7 | 3.17561 | This work | ||||
29750 | Chleborad | −12 | 22 | 41.82 | This work | ||||
40694 | 1999RY230 | 17 | 10 | 9.8659 | This work | ||||
42920 | 1999SA8 | 24 | 10 | 4.9068 | This work | ||||
74119 | 1998QH52 | −7 | 11 | 7.5375 | This work | ||||
92949 | 2000RS41 | 4 | 10 | 2.70517 | This work |
Notes. Listed are the physical properties: ecliptic longitudes and latitudes of the spin axis directions λ and β for one or two possible solutions; the sidereal rotation period P; the mean value of the ecliptic latitude βP and 1/2 of the range in latitude within the multiple pole solutions δβ (for partial models). The uncertainty of the pole direction is usually about 10° and of the period is of the order of the last decimal digit. This table contains new, revised and literature models used for the final analysis, for more details see Tables C.1, E.1 and E.2.
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