Near-Infrared Spectral Diversity of the Ferrar Dolerite in Beacon Valley, Antarctica: Implications for Martian Climate & Surface Compositions

Details Near-Infrared Spectral Diversity of the Ferrar Dolerite in Beacon Valley, Antarctica: Implications for Martian Climate & Surface Compositions Near-Infrared Spectral Diversity of the Ferrar Dolerite in Beacon Valley, Antarctica: Implications for Martian Climate & Surface Compositions

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2290s&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2290

Physics

2

Scientific paper

Spectroscopic studies of Beacon Valley, Antarctica, reveal a range of
secondary alteration minerals that have developed in a cold, dry, and
stable environment. These results have implications for the development
of similar minerals on Mars.

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