Primitive Olivine-Phyric Shergottite NWA 5789: Petrography, Mineral Chemistry and Cooling History Imply a Magma Similar to Yamato 980459

Details Primitive Olivine-Phyric Shergottite NWA 5789: Petrography, Mineral Chemistry and Cooling History Imply a Magma Similar to Yamato 980459 Primitive Olivine-Phyric Shergottite NWA 5789: Petrography, Mineral Chemistry and Cooling History Imply a Magma Similar to Yamato 980459

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1813g&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1813

Computer Science

Scientific paper

Petrography, mineral chemistry and cooling history of NWA 5789 and
comparison to Yamato 980459 imply that both meteorites are primitive and
crystallized from the same type of magma. Primitive melts help elucidate
the geology and geochemistry of Mars.

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