Surface Abundances of K, Th, and U on Mercury and Implications for Planet Formation and Evolution

Details Surface Abundances of K, Th, and U on Mercury and Implications for Planet Formation and Evolution Surface Abundances of K, Th, and U on Mercury and Implications for Planet Formation and Evolution

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2290p&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2290

Computer Science

1

Scientific paper

Measurements made by the MESSENGER gamma-ray spectrometer during the
Mercury flybys were used to calculate the surface K, Th, and U
abundances. Comparisons to compositional models illustrate the ability
of gamma-ray spectroscopy to contribute to geochemical analysis.

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