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The subsurface hydrologic response of Mars to the thermal evolution of its early crustThe Martian valley networks and outflow channels provide persuasive evidence that large bodies of groundwater were present on Mars throughout much of its early geologic history. However, little attention was focused on how these volatile reservoirs may have responded to the thermal evolution of the early Martian crust. In this regard, one process that has likely been of critical importance to the subsurface hydrologic evolution of Mars is thermal vapor diffusion. Various aspects of the thermal vapor diffusion process on Mars are discussed.
Document ID
19920019763
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Clifford, S. M.
(Lunar and Planetary Inst. Houston, TX, United States)
Carr, M. H.
(Geological Survey Menlo Park, CA., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Workshop on the Martian Surface and Atmosphere Through Time
Subject Category
Lunar And Planetary Exploration
Accession Number
92N29006
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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