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Table 6

Derived rotation periods, P (h), longitudes, λ(°), and latitudes, β(°), with their 1σ uncertainties,using convex inversion on a selection of asteroids.

Asteroid Tholen P σP λ σλ β σβ
(55) Pandora M 4.8041 4.8201(−7) 232.31234 1.1456 16.1836 1.5651
(95) Arethusa C 8.7022 1.2844(−6) 152.5368 1.8668 36.1837 3.8230
(97) Klotho M 35.2509 3.2543(−5) 14.2453 1.1257 36.2228 3.4284
(122) Gerda ST 10.6872 5.6964(−6) 201.1882 1.1676 22.1027 0.8569
(245) Vera S 14.3565 1.6794(−5) 272.6310 2.6323 –26.9151 5.7514
(246) Asporina A 16.2522 5.2870(−6) 37.2638 1.4536 –53.8884 2.9806
(376) Geometria S 7.7110 2.0245(−6) 69.9931 1.0059 67.5346 1.6809
(377) Campania PD 11.6644 2.5663(−6) 198.1173 0.6087 74.0972 1.6156
(404) Arsinoe C 8.8877 8.0200(−7) 19.5283 1.8797 60.6531 0.7748
(596) Scheila PCD 15.8663 3.0715(−5) 101.0779 1.0453 –24.5333 3.5072
(731) Sorga CD 8.1863 1.7122(−6) 82.8032 1.5318 40.1433 1.1077
(1251) Hedera E 19.9019 1.6678(−5) 110.0033 3.0122 –71.7336 2.1488

Notes. In the fourth column, for example, (−7) denotes ×10−7. All the parameters represent the means from MCMC sampling.

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