Faulting in Amazonis Planitia
NASA/JPL/University of Arizona

Faulting in Amazonis Planitia
PSP_001578_2000  Science Theme: Tectonic Processes


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This HiRISE image is centered on a long "strike-slip" fault on the young plains in the Amazonis region of Mars.

The most famous example of a strike-slip fault on the Earth is probably the San Andreas Fault in California. The smooth plains here have few large craters, indicating that it has been resurfaced relatively recently.

The fact that the faults have cut these plains indicates that tectonic processes (and Marsquakes) have occurred even more recently. Of course, "recently" on Mars is a relative term; it is likely that both the surfaces and the faulting are more than a billion years old.

Other interesting features are the moats around knobs and craters in the plains (most prominently near the southern edge of the image) and convoluted depressions that might mark a channel along the western edge of the image.
Written by: Laszlo P. Keszthelyi   (11 December 2009)



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Acquisition date:27 November 2006 Local Mars time: 3:26 PM
Latitude (centered):19.7 degrees Longitude (East):198.7 degrees
Range to target site:286.9 km (179.3 miles)Original image scale range:57.4 cm/pixel (with 2 x 2 binning) so objects ~172 cm across are resolved
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Emission angle:8.1 degrees Phase angle:57.2 degrees
Solar incidence angle:49 degrees, with the Sun about 41 degrees above the horizon Solar longitude:141.6 degrees, Northern Summer
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North azimuth:97 degrees Sub-solar azimuth:9.9 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.