Spectral Differences Between Palagonite Tuffs Formed in Sub-Glacial Versus Liquid Water Environments: Relevance to Mars

Details Spectral Differences Between Palagonite Tuffs Formed in Sub-Glacial Versus Liquid Water Environments: Relevance to Mars Spectral Differences Between Palagonite Tuffs Formed in Sub-Glacial Versus Liquid Water Environments: Relevance to Mars

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1804f&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1804

Computer Science

Scientific paper

The reflectance and emissivity spectra of palagonite tuffs formed in
sub-glacial enviroments are compared with those formed in liquid water
environments. The relevance to palagonites produced by water-magma
interactions on Mars is discussed.

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