Petrogenesis of Olivine-Phyric Shergottites Sayh Al Uhaymir 005 and Elephant Moraine A79001 Lithology A

Details Petrogenesis of Olivine-Phyric Shergottites Sayh Al Uhaymir 005 and Elephant Moraine A79001 Lithology A Petrogenesis of Olivine-Phyric Shergottites Sayh Al Uhaymir 005 and Elephant Moraine A79001 Lithology A

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002usnc.conf...17g&link_type=abstract

Unmixing the SNCs: Chemical, Isotopic, and Petrologic Components of the Martian Meteorites, p. 17-18

Mathematics

Logic

Lithology, Olivine, Petrogenesis, Shergottites, Glacial Drift, Basalt, Abundance, Magma, Crystallization

Scientific paper

Martian meteorites Sayh al Uhaymir (SaU) 005 and lithology A of EETA79001 (EET-A) belong to a newly emerging group of olivine-phyric shergottites. Previous models for the origin of such shergottites have focused on mixing between basaltic shergottite-like magmas and lherzolitic shergottite-like material. Results of this work, however, suggest that SaU 005 and EET-A formed from olivine-saturated magmas that may have been parental to basaltic shergottites.

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