Constraints on the Interior Structure and Composition of Mars from Geodesy

Details Constraints on the Interior Structure and Composition of Mars from Geodesy Constraints on the Interior Structure and Composition of Mars from Geodesy

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2178r&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2178

Computer Science

Scientific paper

We use the recent geodesy data of Konopliv et al. 2010 to constrain the
composition and interior structure of Mars. The data is consistent with
Mars having a molten core of radius 1794±65km and a core sulfur
concentration of 16±2 wt%.

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