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

Authors :
Farrand, W. H
Lane, M. D
Source :
Lunar and Planetary Science XXXIII.
Publication Year :
2002
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2002.

Abstract

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

Details

Language :
English
Database :
NASA Technical Reports
Journal :
Lunar and Planetary Science XXXIII
Notes :
NAG5-10577
Publication Type :
Report
Accession number :
edsnas.20020046330
Document Type :
Report