Publikace na Matematicko-fyzikální fakulta |
2020
Abstrakt
In this paper, we present masses of 103 asteroids deduced from their perturbations on the orbits of the inner planets, in particular Mars and the Earth. These determinations and the INPOP19a planetary ephemerides are improved by the recent Mars orbiter navigation data and the updated orbit of Jupiter based on the Juno mission data.
More realistic mass estimates are computed by a new method based on random Monte Carlo sampling that uses up-to-date knowledge of asteroid bulk densities. We provide masses with uncertainties better than 33 per cent for 103 asteroids.
Deduced bulk densities are consistent with those observed within the main spectroscopic complexes.