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Negative and Positive Relief Valley Feature (PSP_005355_2125)

Negative and Positive Relief Valley Feature
Negative and Positive Relief Valley Feature (PSP_005355_2125)
Credit: NASA/JPL/University of Arizona

How could a valley with flowing water become a high-standing ridge?

When rivers flow, they carry sediment or particles with them. The heavier and larger particles are deposited on the bottom as characteristics of the flow, such as a decrease in speed. The sediments build up and, over time, can fill in a river completely. This would typically occur on a flat plain, so that the filled-in river would be level with the surrounding banks.

As more time passes, wind erosion affects the landscape. The sediment in the valley could be more resistant to erosion, which would allow it to exist while its banks erode.

The sinuous ridge in this image, in eastern Arabia Terra in the northern hemisphere, might have been a valley with flowing water in ancient times. At the north (top) end of the image, the ridge transitions to a depression as opposed to being raised. This depression (not imaged by HiRISE) extends into a valley. The Martian valley networks are thought to have formed by flowing water billions of years ago. At the center of the right side of the image (see subimage, approximately 350 meters across) there is a branch in the ridge, which supports the valley network theory.

(A sinuous feature is one that winds about in a snake-like pattern, and a ridge is a high-standing feature.)
Written by: Kelly Kolb

OBSERVATION TOOLBOX
Acquisition date:17 September 2007 Local Mars time: 2:07 PM
Latitude (centered):32.2 ° Longitude (East):46.0 °
Range to target site:290.6 km (181.6 miles)Original image scale range:29.1 cm/pixel
(with 1 x 1 binning) so objects ~87 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:2.0 ° Phase angle:59.7 °
Solar incidence angle:58 °, with the Sun about 32 ° above the horizon Solar longitude:315.5 °, Northern Winter
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:312.1 °
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 azimuth126.9°

 

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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.