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They’re alive! present-day evolution of Martian dunes

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dc.contributor.author Diniega, S.
dc.contributor.author Bridges, N.
dc.contributor.author Hansen, C.
dc.date.accessioned 2013-10-28T19:56:56Z
dc.date.available 2013-10-28T19:56:56Z
dc.date.issued 2011-10-02
dc.identifier.citation European Planetary Science Congress (EPSC) Joint Meeting 2011 La Cité Internationale des Congrès Nantes Métropole, Nantes, France, October 2-7, 2011 en_US
dc.identifier.clearanceno 11-2120
dc.identifier.uri http://hdl.handle.net/2014/43944
dc.description.abstract The sharp brinks and margins, smooth and steep lee slopes, and lack of superimposed landforms (such as small impact craters) on many Martian sand dunes suggests that these features are geologically young clean brinks and smooth/steep lee slopes (HiRISE image PSP_010413_1920; 20°N,79°E; image width is about 500m). Within the last decade, and often primarily through the detailed inspection of high-resolution (HiRISE) images, we have finally found clear evidence that many dunes of Mars are active -- through both aeolian and seasonal (frost) processes. However, it is yet unclear if active dune formation does occur or if we are observing surficial modification of dunes which formed under different climate conditions. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011. en_US
dc.subject Mars en_US
dc.subject dunes en_US
dc.subject activity en_US
dc.title They’re alive! present-day evolution of Martian dunes en_US
dc.type Preprint en_US


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