PIA20379: Inverted Terrain in Eridania
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Reconnaissance Orbiter (MRO)
 Spacecraft:  Mars Reconnaissance Orbiter (MRO)
 Instrument:  HiRISE
 Product Size:  2880 x 1800 pixels (w x h)
 Produced By:  University of Arizona/HiRISE-LPL
 Other  
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 Full-Res TIFF:  PIA20379.tif (15.56 MB)
 Full-Res JPEG:  PIA20379.jpg (768 kB)

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The Eridania Basin is thought to have once contained a large sea. This image shows the Gorgonum Basin, which lies along the eastern edge of Eridania.

Along this eastern boundary, the terrain is being eroded away to expose light-toned altered material, including clays. There are also linear ridges and inverted channels. The channels and ridges are now inverted because they are composed of material that is harder than their surroundings (e.g., cements) so as erosion removes the softer materials, the harder rocks within the channels and ridges remain.

The ridges and channels are interpreted to have formed by water flow, either along the surface (channels) or in the subsurface (ridges), providing clues to the water history of Eridania.

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Image Credit:
NASA/JPL-Caltech/Univ. of Arizona

Image Addition Date:
2016-02-11