Low-FeO Silicates and Abundant Fe,Mg,Ti-Oxides: Indications from MELTS Modeling for a Complex Igneous History for Mercury

Details Low-FeO Silicates and Abundant Fe,Mg,Ti-Oxides: Indications from MELTS Modeling for a Complex Igneous History for Mercury Low-FeO Silicates and Abundant Fe,Mg,Ti-Oxides: Indications from MELTS Modeling for a Complex Igneous History for Mercury

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2339s&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2339

Physics

Scientific paper

Equilibrium and fractional crystallization MELTS models of potential
parental magmas for the surface of Mercury were run. Results suggest
that no single-stage melting of a chondritic precursor could have
produced the surface of Mercury.

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