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Swirls of Rock in Candor Chasma (PSP_001984_1735)

Swirls of Rock in Candor Chasma
Swirls of Rock in Candor Chasma (PSP_001984_1735)
Credit: NASA/JPL/University of Arizona

This image shows spectacular layers exposed on the bottom of Candor Chasma, which is a large canyon in the Valles Marineris system.

The floor here is approximately 4 kilometers below the canyon rim. The layers are made of sand- and dust-sized particles that were transported here by either wind or water. This canyon may have been filled to its rim by these sedimentary layers, subsequently eroded away, most likely by the wind. The elongate hills may represent areas of rock that are stronger due to differences in the size of the sedimentary particles, chemical alteration, or both.

One of the most eye-catching aspects of this scene are the intricate swirls that these layers form. Sedimentary rock generally accumulates in horizontal layers. These layers, however, have been folded into the patterns that we see today. Folding of the layers that are exposed here may have occurred due to the weight of overlying sediments.

Understanding the geologic history of this region may provide clues into the history of water on Mars, because these layers may have accumulated in shallow lakes and may have undergone chemical reactions with this water. The presence of certain kinds of chemical reactions between water and rock can release energy that could have sustained habitable oases in these areas.
Written by: Chris O

OBSERVATION TOOLBOX
Acquisition date:29 December 2006 Local Mars time: 3:39 PM
Latitude (centered):-6.5 ° Longitude (East):283.1 °
Range to target site:261.6 km (163.5 miles)Original image scale range:26.2 cm/pixel
(with 1 x 1 binning) so objects ~79 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:0.9 ° Phase angle:56.1 °
Solar incidence angle:57 °, with the Sun about 33 ° above the horizon Solar longitude:157.8 °, Northern Summer
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:20.7 °
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 azimuth195.4°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_001918_1735Convergence angle24.7°

 

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SCIENCE THEME
Sedimentary/Layering Processes

STEREO PAIR
PSP_001918_1735

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All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible: Image: NASA/JPL/University of Arizona


P O S T S C R I P T

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.