Astrometric asteroid masses: a simultaneous determination
arXiv:1402.4241 · doi:10.1051/0004-6361/201322766
Abstract
Using over 89 million astrometric observations of 349,737 numbered minor planets, an attempt was made to determine the masses of 230 of them by simultaneously solving for corrections to all orbital elements and the masses. For 132 minor planets an acceptable result was obtained, 50 of which appear to be new.
17 pages, 1 figure, submitted to A&A
References in corpus (7)
- Main Belt Binary Asteroidal Systems With Eccentric Mutual Orbits
- New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses
- Main Belt Binary Asteroidal Systems With Circular Mutual Orbits
- INPOP new release: INPOP10e
- Statistical and Numerical Study of Asteroid Orbital Uncertainty
- Orbits, masses, and evolution of main belt triple (87) Sylvia
- The Resolved Asteroid Program - Size, shape, and pole of (52) Europa
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