PIA24470: Sinuous Ridges in Elysium Planitia
 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_068041_1845
 Full-Res TIFF:  PIA24470.tif (15.56 MB)
 Full-Res JPEG:  PIA24470.jpg (1.098 MB)

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A sinuous ridge is a thin and meandering formation that gives the appearance of a stream channel, but stays raised above the surface rather than incised into it. It is believed that these ridges were once stream channels that cut down into the surface.

Flowing water can have a number of effects on a channel bed, such as sorting grains and depositing rocks, all while removing loose material. The water can also carry a number of dissolved minerals that become deposited and cement the remaining grains together. The result is a stream bed that has become "armored."

Once the stream stops flowing and dries up, this armored layer can resist future erosion. Over the millions of years that follow, forces such as wind can gradually remove the original material of the surrounding terrain, but the stream bed can remain. Examining the characteristics of the ridge can reveal clues about the amount of water and the flow speed that existed long ago.

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. (The original image scale is 27.2 centimeters [10.7 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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