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