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Sapping Channel Originating from a Fissure (PSP_010689_2025)

Sapping Channel Originating from a Fissure
Sapping Channel Originating from a Fissure (PSP_010689_2025)
Credit: NASA/JPL/University of Arizona

This image of a region east of Tooting Crater is centered on a tectonic fissure west of the Olympus Mons Aureole. Three other channel systems formed along it.

The feature of note is a broad shallow channel system exhibiting a braided pattern that abruptly changes to a steep walled channel system near the fissure. These steep walled channel systems are thought to be formed when ground water flowing out along a cliff undermines the slope resulting in collapse of overlying materials. Erosion then typically moves in a headward direction along the pre-existing shallow channel system. This process is known as groundwater sapping. There are other places on Mars (such as Cerberus Fossae), where these fissures appear to have flood channels associated with them.

Within this channel there is a more resistant, cliff-forming layer near the surface with some defined horizontal strata (layers). Multiple dark streaks known as slope streaks originate from the base of this hard layer. Slope streaks are generally dark when first formed and then gradually fade over time. The origin of these slope streaks is still under debate, but they are thought to be dry dust avalanches.


Written by: Shawn D Hart

OBSERVATION TOOLBOX
Acquisition date:06 November 2008 Local Mars time: 3:38 PM
Latitude (centered):22.1 ° Longitude (East):208.7 °
Range to target site:286.2 km (178.9 miles)Original image scale range:57.3 cm/pixel
(with 2 x 2 binning) so objects ~172 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:0.8 ° Phase angle:53.9 °
Solar incidence angle:53 °, with the Sun about 37 ° above the horizon Solar longitude:153.3 °, Northern Summer
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:3.4 °
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 azimuth177.3°
A N A G L Y P H   P R O D U C T S
Left observation:PSP_010333_2025Convergence angle5.11°

 

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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.