Sedimentary Layers in West Candor Chasma
NASA/JPL/University of Arizona
Sedimentary Layers in West Candor Chasma
ESP_026378_1730  Science Theme: Sedimentary/Layering Processes
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West Candor Chasma in central Valles Marineris contains some of the thickest of the fine-grained layered deposits on Mars.

We can't see the grain sizes with HiRISE, but as the material erodes in the wind it disappears--apparently carried away by the wind--so the grains must be small. The layers may have been deposited from windblown materials, fall of volcanic sediments, or carried in by water, or all of the above.

Subsequently the layers may have been altered by groundwater, producing hydrated minerals such as sulfates. The enhanced colors in the subimage are related to the minerals or to overlying dust or sand. The dark blue sharp-crested ridges are sand dunes.

Written by: Alfred McEwen (audio recording by Tre Gibbs)   (25 April 2012)

This is a stereo pair with ESP_028422_1730.

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Acquisition date:12 March 2012 Local Mars time:15:13
Latitude (centered):-6.733° Longitude (East):284.485°
Range to target site:266.6 km (166.6 miles)Original image scale range:26.7 cm/pixel (with 1 x 1 binning) so objects ~80 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:Equirectangular
Emission angle:9.8° Phase angle:50.0°
Solar incidence angle:57°, with the Sun about 33° above the horizon Solar longitude:82.4°, Northern Spring

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