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Spectral Differences Between Palagonite Tuffs Formed in Sub-Glacial Versus Liquid Water Environments: Relevance to MarsThe 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.
Document ID
20020046330
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Farrand, W. H. (Space Science Inst. Boulder, CO United States)
Lane, M. D. (Planetary Science Inst. Tucson, AZ United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
CONTRACT_GRANT: NAG5-10577
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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