Mars conformant planetary interior models

Details Mars conformant planetary interior models Mars conformant planetary interior models

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufm.g43a0798r&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #G43A-0798

Physics

8147 Planetary Interiors (5430, 5724), 5430 Interiors (8147), 6225 Mars

Scientific paper

We propose a set of planetary interior models in agreement with the present knowledge of the planet Mars. Our spherical, hydrostatic and non-rotating planet is constituted by a crust, parameterized by its mean density, a mantle with variable mineralogy, dependent on pressure and temperature and a partially fluid core composed of iron and sulfur. The crust thickness, the location of the core mantle boundary, the size and state of the inner-core and the concentration of sulfur in the core are adjusted to agree with the total mass and mean moment of inertia.

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