Present-day formation and seasonal evolution of linear dune gullies on Mars

Present-day formation and seasonal evolution of linear dune gullies on Mars •First systematic survey of linear dune gullies in the southern hemisphere of Mars.•Linear dune gullies are found between 36.3°S and 54.3°S and 64.6°S and 70.4°S.•Linear dune gullies are forming and evolving seasonally at the present-day.•Linear dune gullies often evolve together with recurrent diffusing flows (RDF).•CO₂ sublimation and flow of water/brine are both possible formation processes. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Icarus Elsevier

Present-day formation and seasonal evolution of linear dune gullies on Mars

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Publisher
Elsevier
Copyright
Copyright © 2016 Elsevier Inc.
ISSN
0019-1035
eISSN
1090-2643
D.O.I.
10.1016/j.icarus.2016.03.024
Publisher site
See Article on Publisher Site

Abstract

•First systematic survey of linear dune gullies in the southern hemisphere of Mars.•Linear dune gullies are found between 36.3°S and 54.3°S and 64.6°S and 70.4°S.•Linear dune gullies are forming and evolving seasonally at the present-day.•Linear dune gullies often evolve together with recurrent diffusing flows (RDF).•CO₂ sublimation and flow of water/brine are both possible formation processes.

Journal

IcarusElsevier

Published: Aug 1, 2016

References

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