File:Ganges chasma closeup.jpg

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English: HiRise looked at a small section of Ganges Chasma, which is a trough that makes up part of Valles Marineris. The image is just stunning. Long ago, the surface of Mars in this region was flooded by lava flows. After that, time and wind began changing the surface. Windblown dust and sand covered up everything. If you click on the image and examine the larger version more closely, particularly the region near the edge of this chasm, it looks brighter and smoother than the lava flows underneath. Could this be sediments put in place by flowing water? Or did an explosive v0lcanic event layer the region with fine dust? Or, was it the work of the incessantly blowing Martian winds depositing layer upon layer of fine dust? A combination of all these factors?
Date Unknown date
Source http://thespacewriter.com/wp/2009/04/13/visiting-mars/
Author NASA HiRISE camera, Mars Reconnaissance Orbiter.
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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current01:20, 26 January 2014Thumbnail for version as of 01:20, 26 January 20141,920 × 1,440 (2.41 MB)Tillman{{Information |Description ={{en|1=HiRise looked at a small section of Ganges Chasma, which is a trough that makes up part of Valles Marineris. The image is just stunning. Long ago, the surface of Mars in this region was flooded by lava flows. Af...

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