Article ID Journal Published Year Pages File Type
1774579 Icarus 2011 21 Pages PDF
Abstract
► We present a model of megaflooding on Mars, with thermal and mechanical erosion. ► We apply the model to floods in two, well-documented outflow channels. ► We examine variations in the erosive distance and erosion rate of the floods. ► Increasing initial water depth increases erosive distance given other model inputs. ► Thermal erosion dominates mechanical erosion and can explain present channel depths.
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
Authors
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