Metasomatising the Lunar Mantle with TiO2-rich Melts: A Disequilibrium Porous Flow Model

Details Metasomatising the Lunar Mantle with TiO2-rich Melts: A Disequilibrium Porous Flow Model Metasomatising the Lunar Mantle with TiO2-rich Melts: A Disequilibrium Porous Flow Model

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1040b&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1040

Physics

Scientific paper

Our model investigates the ability of a TiO2-rich melt to fertilize
lunar mantle cumulates via disequilibrium porous flow. We found that
partial melts of these metasomatised cumulates display chemical
signatures unlike those of the picritic glasses.

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