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Meteorological Control on the Formation of Martian PaleolakesWe find that an ocean-driven hydrological cycle and/or the mobilization of polar ice at high obliquity can produce conditions favorable for paleolake formation.
Document ID
20000080595
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Haberle, R. M. (NASA Ames Research Center Moffett Field, CA United States)
McKay, C. P. (NASA Ames Research Center Moffett Field, CA United States)
Schaeffer, J. (Raytheon Co. Palo Alto, CA United States)
Joshi, M. (Reading Univ. United Kingdom)
Cabrol, N. A. (NASA Ames Research Center Moffett Field, CA United States)
Grin, E. A. (NASA Ames Research Center Moffett Field, 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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