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Table 1

Positions of Kleopatra’s satellites with respect to its photocenter.

AlexHelios

Date UT u [arcsec] v [arcsec]
1980-10-10 07:00 0.2711 0.4564
2008-09-19 11:38:00 − 0.18 0.35
2008-09-19 11:51:00 − 0.20 0.36
2008-10-05 09:13:00 − 0.27 0.37
2008-10-05 09:49:00 − 0.29 0.39
2008-10-05 10:03:00 − 0.32 0.39
2008-10-09 05:46:00 − 0.32 0.29
2017-07-14 05:00:59 − 0.4158 0.2952
2017-07-22 04:18:07 − 0.4262 0.2444
2017-07-22 05:00:55 − 0.4291 0.2614
2017-08-22 01:42:34 0.1843 − 0.3150
2018-12-10 06:47:17 − 0.4894 − 0.0958
2018-12-19 06:45:02 0.1871 − 0.2869
2018-12-22 05:58:43 − 0.2540 − 0.3438
2018-12-26 08:14:42 − 0.4973 − 0.0428
2019-01-14 04:57:43 − 0.5319 − 0.1177
CleoSelene

2008-09-19 06:17:00 − 0.25 0.50
2008-09-19 08:44:00 − 0.34 0.54
2008-09-19 11:38:00 − 0.44 0.57
2008-09-19 11:51:00 − 0.44 0.57
2008-09-19 12:02:00 − 0.44 0.58
2008-10-05 09:13:00 − 0.29 0.46
2008-10-05 09:49:00 − 0.31 0.47
2008-10-05 10:03:00 − 0.32 0.46
2008-10-09 09:36:00 0.28 − 0.44
2017-07-14 05:01:00 0.3070 − 0.2600
2017-07-22 04:18:07 − 0.2714 0.2941
2017-07-22 05:00:55 − 0.2621 0.2963
2017-08-22 01:42:34 0.4423 − 0.2401
2018-12-10 06:47:17 0.1949 − 0.1505
2018-12-19 06:45:02 0.3763 0.0929
2018-12-22 05:58:43 0.4555 − 0.0119
2018-12-26 08:14:42 0.3937 0.1271
2019-01-14 04:57:43 − 0.1008 − 0.3298

Notes. Uncertainties are approximately 0.01 arcsec. The position from 1980 is based on the stellar occultation and those from 2008 are taken from Descamps et al. (2011).

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