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Exposure of Layers and Minerals in Candor Chasma (PSP_007166_1740)

Exposure of Layers and Minerals in Candor Chasma
Exposure of Layers and Minerals in Candor Chasma (PSP_007166_1740)
Credit: NASA/JPL/University of Arizona

Scanning across several kilometers of relief, this image shows a cliff along a light-toned layered deposit in Valles Marineris. This particular cliff was targeted because of the excellent exposure of layering and the identification of the minerals kieserite (a mineral containing magnesium) and hematite (an iron oxide).

The hematite appears in the darker low-lying region near the lower left of the image and the kieserite is associated with the light-toned layers. The fact that these minerals are found here with a layered deposit suggests that water may have been involved in the deposition of these minerals and the layers.

Erosion by wind has carved V-shaped patterns along the edges of many of the layers. The layers appear friable (easy to erode) so this is why wind can carve deep grooves along a steep cliff such as visible here. The top of the layered deposit (upper part of image) is smooth and relatively dark because it is covered by debris laid down by the wind, dust and other fine materials.

The cliff has stronger winds flowing up and down it, plus the effects of gravity, so airborne debris can be shed downslope to expose the fresh brighter layered deposit.
Written by: Cathy

OBSERVATION TOOLBOX
Acquisition date:05 February 2008 Local Mars time: 2:47 PM
Latitude (centered):-5.9 ° Longitude (East):286.1 °
Range to target site:265.6 km (166.0 miles)Original image scale range:26.6 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:9.7 ° Phase angle:36.9 °
Solar incidence angle:45 °, with the Sun about 45 ° above the horizon Solar longitude:27.9 °, Northern Spring
For non-map projected products:
North azimuth:100 ° Sub-solar azimuth:28.0 °
F O R   M A P   P R O J E C T E D   P R O D U C T S
North azimuth:270°Sub solar azimuth202.6°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_007456_1740Convergence angle15.2°

 

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For information about NASA and agency programs on the Web, visit: http://www.nasa.gov. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona. The image data were processed using the U.S. Geological Survey’s ISIS3 software.