PIA24462: Eroding Sediments
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Reconnaissance Orbiter (MRO)
 Spacecraft:  Mars Reconnaissance Orbiter (MRO)
 Instrument:  HiRISE
 Product Size:  2880 x 1800 pixels (w x h)
 Produced By:  University of Arizona/HiRISE-LPL
Other products from ESP_067690_1860
 Full-Res TIFF:  PIA24462.tif (5.191 MB)
 Full-Res JPEG:  PIA24462.jpg (816.1 kB)

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Map Projected Browse Image
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This image shows evidence of a complex cycle of cratering and erosion. The center of the image covers an old impact crater, roughly 6 to 7 kilometers in diameter. This can actually be easier to see in lower-resolution images that cover more area, like those from MRO's Context Camera. The crater was later filled by sediments.

Erosion then occurred across the region. The crater rim was left high-standing even though material outside the rim was eroded down to the level of the crater floor. The sediments filling the crater also eroded from the rim inwards, leaving a circular pancake of sedimentary rock. Similar "rim-inwards" erosion has been hypothesized for the (much larger) Gale Crater where the Curiosity rover is operating.

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. (The original image scale is 27.4 centimeters [10.8 inches] per pixel [with 1 x 1 binning]; objects on the order of 82 centimeters [32.3 inches] across are resolved.) North is up.

The University of Arizona, in Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Image Credit:
NASA/JPL-Caltech/University of Arizona

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