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The Distribution of Crystalline Hematite on Mars from the Thermal Emission Spectrometer: Evidence for Liquid WaterCrystalline hematite on Mars has been mapped using the MGS TES. Two major, and several minor areas of significant accumulation are identified. We favor precipitation models involving Fe-rich water, providing direct mineralogic evidence for large-scale water interactions.
Document ID
20000081077
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Christensen, P. R. (Arizona State Univ. Tempe, AZ United States)
Malin, M. (Malin Space Science Systems San Diego, CA United States)
Morris, D. (NASA Johnson Space Center Houston, TX United States)
Bandfield, J. (Arizona State Univ. Tempe, AZ United States)
Lane, M. (Arizona State Univ. Tempe, AZ United States)
Edgett, K. (Malin Space Science Systems San Diego, CA United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Collected WorksLunar and Planetary Science XXXI
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