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Mantled Craters in Terra Cimmeria
Mantled Craters in Terra Cimmeria
Mantled Craters in Terra Cimmeria  (PSP_006736_1325)
Credit: NASA/JPL/University of Arizona

This image shows the intersection of two overlapping craters, although it is unknown which of the two formed first.

The two craters are covered in a mantling material, which gives them a smooth appearance. The mantling unit is thought to be water ice-rich. Concentric circles are visible on the floor of one crater. It is likely that these circles are evidence of ice-rich material that flowed off the crater wall, driven by gravity, onto the crater floor.

Outside of the craters, the plains have a pitted or dissected texture. Both of these textures are suggestive of material that once held ice that has since disappeared allowing the remaining soil to collapse into the subsurface. There are also dark dust devil tracks across the scene.


OBSERVATION TOOLBOX
Acquisition date:03 January 2008 Local Mars time: 2:42 PM
Latitude (centered):-47.4 ° Longitude (East):151.5 °
Range to target site:249.8 km (156.1 miles)Original image scale range:25.0 cm/pixel
(with 1 x 1 binning) so objects ~75 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:0.7 ° Phase angle:64.1 °
Solar incidence angle:63 °, with the Sun about 27 ° above the horizon Solar longitude:12.1 °, Northern Spring
For non-map projected products:
North azimuth:96 ° Sub-solar azimuth:48.9 °
For map projected products:
North azimuth:270°Sub solar azimuth222.407°
 

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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.