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Encyclopedia > Numbers about the solar system XVI

Masses of some asteroids and corresponding gravitational constants



Asteroids Mass (in solar mass) References Mass(1024 kg) G M (m3 s-2)
1 Ceres (4.39 ± 0.04) × 10-10 Hilton (1999) 0.000 99 6.6 × 1010
2 Pallas (1.59 ± 0.05) × 10-10 Hilton (1999) 0.000 25 1.7 × 1010
3 Juno (1.42 ± 0.06) × 10-11 Pitjeva (2004) 0.000 028 2.0 × 109
4 Vesta (1.69 ± 0.11) × 10-10 Hilton (1999) 0.000 334 2.34 × 1010
7 Iris (5.2 ± 0.8) × 10-12 Pitjeva (2004) 0.000 011 7.2 × 108
9 Metis (2.5 ± 2.3) × 10-12 - 0.000 005 3.3 × 108
10 Hygiea (4.7 ± 2.3) × 10-11 Scholl et al. (1987) 0.000 093 6.2 × 109
11 Parthenope (2.58 ± 0.10) × 10-12 Viateau & Rapaport (1997) 0.000 005 3.6 × 108
15 Eunomia (4.2 ± 1.1) × 10-12 Hilton (1997) 0.000 008 5.8 × 108
16 Psyche (8.7 ± 2.6) × 10-12 Viateau (1999) 0.000 017 12.0 × 108
20 Massalia (2.4 ± 0.4) × 10-12 Bange (1998) 0.000 005 3.3 × 108
45 Eugenia (3.05 ± 0.13) × 10-12 Merline, et al. (1999) 0.000 006 4.22 × 108
121 Hermione (4.7 ± 0.8) × 10-12 Viateau (1999) 0.000 009 6.2 × 108
216 Kleopatra (1.0 ± 0.1) × 10-12* Marchis, et al. (1999) 0.000 002 1.3 × 108
243 Ida (2.18 ± 0.32) × 10-14** Petit, et al. (1997) 0.000 00004 3.0 × 106
253 Mathilde (5.193 ± 0.022) × 10-14 Yeomans, et al. (1998) 0.000 0001 7.1 × 106
324 Bamberga (5.1 ± 0.8) × 10-12 Pitjeva (2004) 0.000 010 7.1 × 108
433 Eros (3.361 ± 0.002) × 10-15 Yeomans, et al. (2000) 0.000 00001 4.6 × 105
704 Interamnia (3.7 ± 1.7) × 10-11 Landgraff (1992) 0.000 073 5.1 × 109

* The mass of Kleopatra is deduced from its rotation assuming that the two pieces making the object are not in contact.

** The mass of Ida is deduced from the long term stability of its satellite, Dactyl.

The references are accessible on http://aa.usno.navy.mil/hilton/asteroid_masses.htm

Credit: IMCCE/J. Hilton