Aqueous Alteration Pathways for K, Th, and U on Mars

Details Aqueous Alteration Pathways for K, Th, and U on Mars Aqueous Alteration Pathways for K, Th, and U on Mars

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1429s&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1429

Computer Science

1

Scientific paper

We used dissolution rate and residence time calculations of component
minerals in Shergotty to determine the K/Th/U ratios as a martian basalt
is dissolved in water. Some variation in K/Th/U ratios may be due to
aqueous alteration processes.

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