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Table A.2

Results from the previous solutions available in the literature.

Sidereal Pole 1 Pole 2 D Reference


period [h] λp βp λp βp km
(3) Juno
7.20953 105° 21° 248 ± 5 Viikinkoski et al. (2015)
             
(14) Irene
15.02987 91° − 15° 153 ± 6 Viikinkoski et al. (2017)
             
(20) Massalia
8.09902 179° 39° 360° 40° 131.56∕145.5∕− (*) Kaasalainen et al. (2002)
             
(64) Angelina
8.75033 138° 14° 317° 17° 52 ± 10 Ďurech et al. (2011)
             
(68) Leto
14.84547 103° 43° 290° 23° 112 ± 14 Hanuš et al. (2013)
             
(89) Julia
11.388332 14° − 24° 140 ± 3 Vernazza et al. (2018)
             
(114) Kassandra
10.74358 196° − 55° − 58° 93.91∕99.65∕100 (*) Ďurech et al. (2018b)
             
(145) Adeona
141.39∕151.14∕151 (*)
             
(297) Caecilia
4.151388 47° − 33° 223° − 53° 42.28∕39.48∕− (*) Hanuš et al. (2013)
             
(308) Polyxo
135.25∕140.69∕144.4 (*)
             
(381) Myrrha
6.57198 48° 160° 77° 117.12∕120.58∕129 (*) Hanuš et al. (2016)
             
(441) Bathilde
10.44313 122° 43° 285° 55° 59.42∕70.32∕70.81 (*) Hanuš et al. (2013)
             
(721) Tabora
7.98121 172° 53° 343° 38° 81.95∕76.07∕86.309 (*) Ďurech et al. (2018a)

Notes. Mirror pole solutions are labeled “pole 1” and “pole 2”. Scaled sizes are given in kilometers as the diameters of the equivalent volume spheres. For objects marked with(*)we have taken the sizes from the AKARI, SIMPS, and WISE (Usui et al. 2011; Tedesco et al. 2005; Mainzer et al. 2016) missions, respectively, for which the sizes were often calculated with an STM approximation of the spherical shape, and often without a known pole solution.

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