Hypothesis for Petrogenesis of Wishstone-Class Rocks in Gusev Crater: Implications for CO2 Inventory in the Martian Mantle

Details Hypothesis for Petrogenesis of Wishstone-Class Rocks in Gusev Crater: Implications for CO2 Inventory in the Martian Mantle Hypothesis for Petrogenesis of Wishstone-Class Rocks in Gusev Crater: Implications for CO2 Inventory in the Martian Mantle

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1272u&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Computer Science

1

Scientific paper

Here we propose that the Wishstone-class originates in an alkaline suite
related to a carbonatite-bearing alkaline complex. This implies that, at
least under Gusev crater, CO2 resided in the Mars mantle.

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