Water and Carbon Dioxide in the Martian Magma Ocean: Early Atmospheric Growth, Subsequent Mantle Compositions, and Planetary Cooling Rates

Details Water and Carbon Dioxide in the Martian Magma Ocean: Early Atmospheric Growth, Subsequent Mantle Compositions, and Planetary Cooling Rates Water and Carbon Dioxide in the Martian Magma Ocean: Early Atmospheric Growth, Subsequent Mantle Compositions, and Planetary Cooling Rates

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2007e&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2007

Computer Science

1

Scientific paper

The volatile content of a magma ocean has significant effects on
planetary evolution. Calculations are presented for water and carbon
dioxide degassing to form a planetary atmosphere, cooling of the magma
ocean, and subsequent mantle composition.

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