Orbital Spectral Mapping of Surface Compositions in the Antarctic Dry Valleys: Regional Distributions of Secondary Mineral-Phases as Climate Indicators and Implications for Mars

Details Orbital Spectral Mapping of Surface Compositions in the Antarctic Dry Valleys: Regional Distributions of Secondary Mineral-Phases as Climate Indicators and Implications for Mars Orbital Spectral Mapping of Surface Compositions in the Antarctic Dry Valleys: Regional Distributions of Secondary Mineral-Phases as Climate Indicators and Implications for Mars

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2275w&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2275

Computer Science

Scientific paper

The Antarctic Dry Valleys are an ideal location to examine links between
surface compositions and climate variables in a Mars-like, hyper-arid,
cold-polar desert. We report results from ongoing field work and
laboratory and orbital spectroscopy.

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