Abstract
Windy Mars: A dynamic planet as seen by the HiRISE camera
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
U.S. Geological Survey, Flagstaff, Arizona, USA
Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
Planetary Science Institute, Tucson, Arizona, USA
U.S. Geological Survey, Flagstaff, Arizona, USA
U.S. Geological Survey, Flagstaff, Arizona, USA
Department of Geological Sciences, University of Colorado, Boulder, Colorado, USA
With a dynamic atmosphere and a large supply of particulate material, the surface of Mars is heavily influenced by wind-driven, or aeolian, processes. The High Resolution Imaging Science Experiment (HiRISE) camera on the Mars Reconnaissance Orbiter (MRO) provides a new view of Martian geology, with the ability to see decimeter-size features. Current sand movement, and evidence for recent bedform development, is observed. Dunes and ripples generally exhibit complex surfaces down to the limits of resolution. Yardangs have diverse textures, with some being massive at HiRISE scale, others having horizontal and cross-cutting layers of variable character, and some exhibiting blocky and polygonal morphologies. “Reticulate” (fine polygonal texture) bedforms are ubiquitous in the thick mantle at the highest elevations.
Received 7 August 2007; accepted 23 October 2007; published 15 December 2007.
Citation: (2007), Windy Mars: A dynamic planet as seen by the HiRISE camera, Geophys. Res. Lett., 34, L23205, doi:10.1029/2007GL031445.
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