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Ancient Martian valley genesis and paleoclimatic inference: The present as a key to the pastI offer here the speculative genetic hypothesis that the flat-floored landforms represent episodically active, sediment-laden valley glaciers formed by localized geothermal melting of abundant interstitial ice (permafrost) in a fine-grained sedimentary terrain. Geothermal melting may also localize spring heads for the narrow deep, high-gradient valleys, or the collapse process itself may result in the generation of decanted, relatively sediment-poor overland water flows (some local evidence of fluid overtopping of the localized depressions exists). Whatever the generic mechanisms for the suite of valley landforms, perhaps the most interesting observation is simply their youth. In aggregate, the morphologies are similar to the ancient valley systems cited as evidence for a previously much denser atmosphere on Mars.
Document ID
19940017188
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Brakenridge, G. R.
(Dartmouth Coll. Hanover, NH, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Workshop on Early Mars: How Warm and How Wet?, Part 1
Subject Category
Lunar And Planetary Exploration
Accession Number
94N21661
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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