A Host for Lithium in MIL03346 and Implications for Aqueous Alteration on Mars

Details A Host for Lithium in MIL03346 and Implications for Aqueous Alteration on Mars A Host for Lithium in MIL03346 and Implications for Aqueous Alteration on Mars

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2362r&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2362

Physics

Scientific paper

In nakhlites, poorly crystalline clays formed by aqueous alteration on
Mars show the highest Li contents. The finding of likewise enriched
olivine in the MIL03345 mesostasis revokes the need for sources outside
the nakhlitic flow(s) as explanation.

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