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Noachian-Hesperian Transition and a Possible Climatic Optimum: Evidence from LandformsA climatic optimum? The often strong contrast between the pristine and degraded Noachian channels and craters might be due to a gradual climatic change superimposed upon an episode of mantling associated with early Hesperian volcanism. On the other hand, one or more episodes of volcanism or large impacts could have induced global warming and produced a relatively short-lived optimum for precipitation and runoff. The rapid cutoff of fluvial activity following the development of the later pristine fluvial features is consistent with this scenario. We discuss the changing style of erosion in the highlands during the Noachian and early Hesperian in a companion abstract to this workshop. Here we review the some of the morphologic evidence for a possible Noachian-Hesperian (N-H) climate optimum.
Document ID
20040191787
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Moore, J. M.
(NASA Ames Research Center Moffett Field, CA, United States)
Howard, A. D.
(Virginia Univ. Charlottesville, VA, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2004
Publication Information
Publication: Second Conference on Early Mars: Geologic, Hydrologic, and Climatic Evolution and the Implications for Life
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Public Use Permitted.
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