Consequences of High Crystallinity for the Evolution of the Lunar Magma Ocean: Trapped Plagioclase

Details Consequences of High Crystallinity for the Evolution of the Lunar Magma Ocean: Trapped Plagioclase Consequences of High Crystallinity for the Evolution of the Lunar Magma Ocean: Trapped Plagioclase

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1678e&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1678

Physics

Scientific paper

Large-scale lunar plagioclase flotation may have been impossible. The
temperature profile lies below the liquidus for most of crystallization,
creating crystal networks. Partial melting during cumulate overturn may
be able to create crustal suites.

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