Volume 465, Number 3, April III 2007
|Page(s)||1075 - 1084|
|Section||Celestial mechanics and astrometry|
|Published online||29 January 2007|
First numerical ephemerides of the Martian moons
Royal Observatory of Belgium, 3 avenue Circulaire, 1180 Bruxelles, Belgium e-mail: Lainey@oma.be
2 Institut de Mécanique Céleste et de Calcul des Ephémérides-Observatoire de Paris, UMR 8028 du CNRS, 77 avenue Denfert-Rochereau, 75014 Paris, France
3 Institut für Geophysik und Meteorologie, Universität zu Köln, Albertus-Magnus-Platz, 50923 Cologne, Germany
Accepted: 22 December 2006
We present new ephemerides of Phobos and Deimos that are fit to observations from 1877 to 2005 and include recent spacecraft observations by Mars Global Surveyor and Mars Express. In contrast to earlier models, this is the first completely numerical one. In particular, the tidal effects have been modeled by the tidal bulge raised by each moon on the planet, instead of fitting secular accelerations in the satellite longitudes. This partly avoids absorbing the Deimos observational errors in its related tidal acceleration. Moreover, applying this model to other systems will be easier. Our estimate of the Martian dissipation is Q = 79.91±0.69 (1σ-formal error) when assuming for the Martian Love number and = 0.68106 m3/s2 for the Phobos mass. We also report the possibility of fitting the Phobos oblateness gravity field. We suspect a non-uniform density for Phobos or a bias in either the observations or the Martian gravity field. A FORTRAN subroutine that computes the Martian moons' ephemerides is available on request.
Key words: planets and satellites: general / ephemerides / celestial mechanics / astrometry
© ESO, 2007
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