Variations in Light Lithophile Elements (Li, B, Be) and Lithium Isotopes in Martian Pyroxenes and Olivines: Roles of Degassing and Diffusion

Details Variations in Light Lithophile Elements (Li, B, Be) and Lithium Isotopes in Martian Pyroxenes and Olivines: Roles of Degassing and Diffusion Variations in Light Lithophile Elements (Li, B, Be) and Lithium Isotopes in Martian Pyroxenes and Olivines: Roles of Degassing and Diffusion

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2362a&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2362

Computer Science

Scientific paper

We have measured and modelled light lithophile elements and Li isotopic
composition in pyroxenes and olivines from newly discovered martian
meteorites to assess the roles of various processes involved in martian
magmatic history.

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