Origin of Low-Ca Pyroxene Megacrysts in Martian Basalts. Comparisons Among the Composition of Minerals in RBT 04262

Details Origin of Low-Ca Pyroxene Megacrysts in Martian Basalts. Comparisons Among the Composition of Minerals in RBT 04262 Origin of Low-Ca Pyroxene Megacrysts in Martian Basalts. Comparisons Among the Composition of Minerals in RBT 04262

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2053b&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2053

Computer Science

Scientific paper

We compare mineral compositions in three textures observed in martian
meteorite RBT 04262 to gain a better understanding of the origin of
megacrysts in shergottites, the petrogenesis of martian basalts, and the
nature of the martian crust.

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