Study of the Yarkovsky diurnal effect on planetary satellites: application to the satellites of Mars

Details Study of the Yarkovsky diurnal effect on planetary satellites: application to the satellites of Mars Study of the Yarkovsky diurnal effect on planetary satellites: application to the satellites of Mars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..859t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.859

Computer Science

Scientific paper

We study here the perturbation caused by the Yarkovsky diurnal effect on the long-term evolution of Phobos' and Deimos' orbits. In particular, the past evolution of the Mars satellites is still not completely understood. While tidal effects may have played the most important role in the past evolution of their orbits, it is still important to verify that all relevant perturbations required to compute accurately the moon orbits have been considered. Moreover, due to their proximity to the sun, Mars moons are expected to be the most concerned of planetary moons by Yarkovsky effect.

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