Layered Mesa in Coprates Chasma
NASA/JPL/University of Arizona

Layered Mesa in Coprates Chasma
PSP_002036_1655  Science Theme: Sedimentary/Layering Processes


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This observation shows a mesa within Coprates Chasma, a large trough in the Valles Marineris canyon system. Multiple layers, some only a few meters in thickness, are visible on the slopes descending from the edges of the flat-topped mesa.

The layered rocks could have formed from volcanic, lacustrine, or aeolian sediments that were deposited in portions of the Valles Marineris trough. Variations in the brightness of the layers may represent compositional differences. In particular, the slopes contain a prominent layer of dark material that is seemingly composed of materials more resistant to erosion than the overlying brighter layers.

Dunes and ripples can also visible on the top of the mesa.
Written by: Maria Banks   (21 July 2010)

This is a stereo pair with PSP_003104_1655.



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Acquisition date:02 January 2007 Local Mars time: 3:40 PM
Latitude (centered):-14.4 degrees Longitude (East):304.2 degrees
Range to target site:258.8 km (161.7 miles)Original image scale range:from 25.9 cm/pixel (with 1 x 1 binning) to 51.8 cm/pixel (with 2 x 2 binning)
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Solar incidence angle:59 degrees, with the Sun about 31 degrees above the horizon Solar longitude:160.0 degrees, Northern Summer
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