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SPACE-MARS-WIND-SEDIMENTS
This NASA image obtained September 26, 2013 shows a scene situated in the Noctis Labyrinthus region of Mars, perched high on the Tharsis rise in the upper reaches of the Valles Marineris canyon system. Targeting the bright rimmed bedrock knobs, the image also captures the interaction of two distinct types of windblown sediments. Surrounding the bedrock knobs is a network of pale reddish ridges with a complex interlinked morphology. These pale ridges resemble the simpler “transverse aeolian ridges” (called TARs) that are common in the equatorial regions of Mars. Dark sand dunes comprise the second type of windblown sediment visible in this image. The original image was acquired on August 31, 2013, by the HiRISE (High Resolution Imaging Science Experiment) instrument aboard NASA's Mars Reconnaissance Orbiter (MRO). HiRISE is operated by the University of Arizona, Tucson. AFP PHOTO / NASA/JPL/UNIVERSITY OF ARIZONA/ == RESTRICTED TO EDITORIAL USE / MANDATORY CREDIT: "AFP PHOTO / NASA/JPL/UNIVERSITY OF ARIZONA/ NO MARKETING / NO ADVERTISING CAMPAIGNS / DISTRIBUTED AS A SERVICE TO CLIENTS ==
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Detalii fotografie |
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-, SPACE |
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AFP / Mediafax Foto |
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Fotograf: |
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HO |
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Data: |
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26 Septembrie 2013 |
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Dimensiuni: |
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2880 x 1800 (1.08 MB) |
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