Table A.3.
Physical properties of asteroids with revised shape model determinations based on the V-band ASAS-SN data and comparison with the DAMIT database.
Asteroid | λ1 | β1 | λ2 | β2 | P | M | NA | PLCDB | D | λD1 | βD1 | λD2 | βD2 | PD | ||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[deg] | [deg] | [deg] | [deg] | [hours] | [hours] | [km] | [deg] | [deg] | [deg] | [deg] | [hours] | |||||
5 | Astraea | 84 | 52 | 270 | 44 | 16.8006 | CE | 312 | 16.81 | 3 | 108.3 | 124 | 39 | 16.8006 | ||
12 | Victoria | 170 | 37 | 8.6604 | C | 347 | 8.66 | 3 | 115.1 | 178 | −28 | 8.6603 | ||||
13 | Egeria | 34 | 46 | 7.04664 | C | 262 | 7.04 | 3 | 227.0 | 54 | 34 | 233 | 6 | 7.04667 | ||
16 | Psyche | 35 | −11 | 215 | 16 | 4.19597 | C | 377 | 4.20 | 3 | 207.2 | 36 | −10 | 4.19595 | ||
17 | Thetis | 55 | 12 | 237 | 21 | 12.2660 | CE | 290 | 12.27 | 3 | 84.9 | 236 | 19 | 12.2660 | ||
19 | Fortuna | 102 | 51 | 283 | 59 | 7.4432 | CE | 252 | 7.44 | 3 | 196.4 | 97 | 69 | 7.4432 | ||
20 | Massalia | 122 | 46 | 302 | 47 | 8.0976 | CE | 312 | 8.10 | 3 | 131.6 | 179 | 39 | 360 | 40 | 8.0990 |
21 | Lutetia | 52 | −3 | 232 | −0 | 8.1683 | CE | 300 | 8.17 | 3 | 108.4 | 52 | −6 | 8.1683 | ||
23 | Thalia | 340 | −70 | 12.3122 | CE | 304 | 12.31 | 3 | 106.2 | 158 | −46 | 343 | −74 | 12.3124 | ||
25 | Phocaea | 342 | 9 | 9.9353 | CE | 334 | 9.93 | 3 | 83.2 | 347 | 10 | 9.9354 | ||||
28 | Bellona | 103 | −10 | 282 | 4 | 15.7078 | CE | 362 | 15.71 | 3 | 97.4 | 98 | −10 | 15.7079 |
Notes. We provide ecliptic coordinates λ and β of up to two pole solutions, sidereal rotational period P (its uncertainty is of the order of the last digit). The method (M) column indicates whether the rotation period was derived by the convex inversion (C), ellipsoid (E) approach, or both (CE) approaches. The final columns are the number of ASAS-SN measurements NA, the LCDB period with its reliability flag (Warner et al. 2009) and the size D from the MP3C database3. The full table is available at the CDS.
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