PIA19859: A Possible Landing Site for the ExoMars Rover in Aram Dorsum
 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 products from image ESP_040881_1880
 Full-Res TIFF:  PIA19859.tif (15.56 MB)
 Full-Res JPEG:  PIA19859.jpg (1.177 MB)

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This image is part of a proposed landing site for the ExoMars Rover, planned for launch in 2018.

We can see how an upper layers of light toned sediments have been eroded, leaving a lower surface which appears dark. The retreating sediment scarp slopes would be an important target for the rover if it ends up going to Aram Dorsum.

The retreating scarps will be relatively recent compared to the ancient age of the terrain. That means that organic compounds-which is what ExoMars is designed to drill to 2 meters depth and analyze-will not have been exposed to the full effects of solar and galactic radiation for their entire history. Such radiation can break down organic compounds. Prior to this later erosion, the rocks formed in the ancient, Noachian era as alluvial deposits of fine grained sediment.

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. 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

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