Igneous and Aqueous Processes on Mars: Evidence from Measurements of K and Th by the Mars Odyssey Gamma Ray Spectrometer

Details Igneous and Aqueous Processes on Mars: Evidence from Measurements of K and Th by the Mars Odyssey Gamma Ray Spectrometer Igneous and Aqueous Processes on Mars: Evidence from Measurements of K and Th by the Mars Odyssey Gamma Ray Spectrometer

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3207t&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3207

Physics

4

Scientific paper

Concentrations of K and Th and the K/Th ratio vary across the surface.
Concentrations are higher than in martian meteorites, suggesting that
most of the crust formed by partial melting of enriched mantle.

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