Petrogenesis of Lunar High-Titanium Liquids: The Importance of fO2 on the Depth of Origin and Melt Structure

Details Petrogenesis of Lunar High-Titanium Liquids: The Importance of fO2 on the Depth of Origin and Melt Structure Petrogenesis of Lunar High-Titanium Liquids: The Importance of fO2 on the Depth of Origin and Melt Structure

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2333k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2333

Physics

Scientific paper

High-Ti glasses are remelts of lunar magma ocean cumulates. We present
our experimental data on how the depth of origin for these magmas
depends on fO2 as well as discuss their melt structure and possible
relation to the high-Ti mare basalt suite.

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