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Recent aeolian dune change on Mars

Authors :
Bourke, M.C.
Edgett, K.S.
Cantor, B.A.
Source :
Geomorphology. Feb2008, Vol. 94 Issue 1/2, p247-255. 9p.
Publication Year :
2008

Abstract

Abstract: Previous comparisons of Martian aeolian dunes in satellite images have not detected any change in dune form or position. Here, we show dome dunes in the north polar region that shrank and then disappeared over a period of 3.04 Mars years (5.7 Earth years), while larger, neighboring dunes showed no erosion or movement. The removal of sand from these dunes indicates that not only is the threshold wind speed for saltation exceeded under present conditions on Mars, but that any sand that is available for transport is likely to be moved. Dunes that show no evidence of change could be crusted, indurated, or subject to infrequent episodes of movement. [Copyright &y& Elsevier]

Details

Language :
English
ISSN :
0169555X
Volume :
94
Issue :
1/2
Database :
Academic Search Index
Journal :
Geomorphology
Publication Type :
Academic Journal
Accession number :
28010873
Full Text :
https://doi.org/10.1016/j.geomorph.2007.05.012