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Slipping and Sliding in Coprates Chasma (PSP_001970_1655)

Slipping and Sliding in Coprates Chasma
Slipping and Sliding in Coprates Chasma (PSP_001970_1655)
Credit: NASA/JPL/University of Arizona

This image shows a landslide in the Coprates Chasma region of Valles Marineris that occurred when a large unstable area of rock broke away from the cliffs along the top of the image.

This mass of falling rock broke into many small pieces as it slid downhill and came to rest at the base of the cliff, forming the lobate (curved) mound in the lower part of the image.

The smooth textured ripples that are in the central part of the image are sand dunes. Sand dunes form as wind-blown particles roll across the surface and accumulate. Since the air on Mars is very thin, sand dunes take much longer to form on Mars than they do on Earth. The presence of large sand dunes, along with many small impact craters, on top of this landslide indicates that movement of the slide occurred a very long time ago, perhaps hundreds of millions of years.

This landslide was probably caused by a strong earthquake. A nearby meteorite impact may have generated an earthquake that was sufficiently strong to cause this landslide. Alternatively, movement along nearby faults may have triggered the landslide.

The Valles Marineris region is cut by many faults and in fact contains many more landslides such as this one. Some scientists believe that these landslides represent a record of earthquake activity in this area. Understanding the history of earthquake activity in the region may help scientists to predict the likelihood that such earthquakes occur on Mars today.
Written by: Chris O

OBSERVATION TOOLBOX
Acquisition date:27 December 2006 Local Mars time: 3:42 PM
Latitude (centered):-14.2 ° Longitude (East):306.7 °
Range to target site:266.1 km (166.3 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:7.0 ° Phase angle:53.9 °
Solar incidence angle:60 °, with the Sun about 30 ° above the horizon Solar longitude:157.3 °, Northern Summer
For non-map projected products:
North azimuth:98 ° Sub-solar azimuth:25.5 °
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 azimuth199.7°

 

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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


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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.