FeO and Refractory Elements of Lunar Magma Ocean Constrained by Condition of Anorthosite Crust Formation

Details FeO and Refractory Elements of Lunar Magma Ocean Constrained by Condition of Anorthosite Crust Formation FeO and Refractory Elements of Lunar Magma Ocean Constrained by Condition of Anorthosite Crust Formation

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1636s&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1636

Physics

Scientific paper

The bulk composition of the lunar magma ocean was constrained by
developing a new model to satisfy the physics and chemistry of the magma
ocean that formed the upper crust exclusively consisting of anorthosite
with the thickness of several tens km.

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