Fractures in Cerberus Fossae
NASA/JPL/University of Arizona

Fractures in Cerberus Fossae
PSP_009913_1910  Science Theme: Tectonic Processes
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This image shows an example of "en echelon" fractures in the Cerberus Fossae region. The fractures formed tectonically, by movement of Mars' crust. En echelon means that the fractures are laterally displaced from each other in a way consistent with the lateral displacement of other fractures in the same area.

The colors in this enhanced color image result from differences in composition of the materials and do not represent how it would appear to the human eye. Note that one can make out boulders and small dunes at the bottom of these fractures and layering within the walls. Just visible at the top of the image is well-preserved impact crater ejecta. The image is 1.2 kilometer across.Written by: Kate Fishbaugh   (22 October 2008)



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Acquisition date:06 September 2008 Local Mars time: 3:28 PM
Latitude (centered):11.0 degrees Longitude (East):155.4 degrees
Range to target site:280.0 km (175.0 miles)Original image scale range:28.0 cm/pixel (with 1 x 1 binning) so objects ~84 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:EQUIRECTANGULAR
Emission angle:7.7 degrees Phase angle:57.7 degrees
Solar incidence angle:51 degrees, with the Sun about 39 degrees above the horizon Solar longitude:123.5 degrees, Northern Summer
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North azimuth:97 degrees Sub-solar azimuth:23.5 degrees
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North azimuth:270 degreesSub solar azimuth:197.8 degrees

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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.