Do Early Liquidus Phases in Olivine-Phyric Martian Basalts Reflect the Characteristics of Their Mantle Sources? Insights from NWA 1110, NWA 1195, and NWA 2046

Details Do Early Liquidus Phases in Olivine-Phyric Martian Basalts Reflect the Characteristics of Their Mantle Sources? Insights from NWA 1110, NWA 1195, and NWA 2046 Do Early Liquidus Phases in Olivine-Phyric Martian Basalts Reflect the Characteristics of Their Mantle Sources? Insights from NWA 1110, NWA 1195, and NWA 2046

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1193s&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1193

Computer Science

1

Scientific paper

Olivine in martian meteorites NWA 1110, NWA 1195, NWA 2046 reflect both
the fO2 conditions and incompatible element nature of the sources for
olivine-phyric martian basalts.

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