New Constraints on the Formation of Shergottite EET 79001 Lithology

Details New Constraints on the Formation of Shergottite EET 79001 Lithology New Constraints on the Formation of Shergottite EET 79001 Lithology

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2456t&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2456

Physics

Scientific paper

Since the martian meteorite EET 79001 contains two lithologies, an
olivine-phyric portion and a basaltic portion, in an apparent igneous
contact, several models have been proposed for the formation of EET
79001.

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