Did ice streams shape the largest channels on Mars?

Kite, E. S. and Hindmarsh, R. C. A. (2007) Did ice streams shape the largest channels on Mars? Geophysical Research Letters, 34. L19202. DOI https://doi.org/10.1029/2007GL030530

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The largest channels on Mars are the Northwestern Slope Valleys (NSVs) of Tharsis, which have previously been interpreted as the probable erosional trace of catastrophic flooding. It is argued here that ice-streaming within ancient ice sheets emplaced by atmospheric precipitation at high mean obliquity may instead account for these channels, explaining similarities between the region and terrestrial Pleistocene subglacial landscapes. An ice-sheet model shows extensive basal melting in and only in the NSV region, and ice streams which have significant erosive power.

Item Type: Article
Uncontrolled Keywords: TYAREP; 2007 P; IA55; Part III
Subjects: 02 - Geodynamics, Geophysics and Tectonics
Divisions: 02 - Geodynamics, Geophysics and Tectonics
06 - Part-III Projects
Journal or Publication Title: Geophysical Research Letters
Volume: 34
Page Range: L19202
Identification Number: https://doi.org/10.1029/2007GL030530
Depositing User: Sarah Humbert
Date Deposited: 16 Feb 2009 13:02
Last Modified: 09 Jun 2014 16:25
URI: http://eprints.esc.cam.ac.uk/id/eprint/456

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