The effects of deviation of Mars from its equilibrium state on the flattening of the core-mantle boundary

Details The effects of deviation of Mars from its equilibrium state on the flattening of the core-mantle boundary The effects of deviation of Mars from its equilibrium state on the flattening of the core-mantle boundary

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf...60g&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

Computer Science

Scientific paper

In a static approach the calculations for the non-hydrostatic deviations in the core-mantle boundary have been performed for a trial interior structure model of Mars with a crust of 50 km thick (Fig.1). Mars departs from hydrostatic equilibrium to significant extent. It is seen if we compare the first even gravitational moments and for the Martian models in hydrostatic equilibrium state , with gravitational moments of the planet , [1].

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