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Cratered Dunes and Yardangs in the Medusae Fossae Formation (PSP_010453_1675)

Cratered Dunes and Yardangs in the Medusae Fossae Formation
Cratered Dunes and Yardangs in the Medusae Fossae Formation (PSP_010453_1675)
Credit: NASA/JPL/University of Arizona

This image shows cratered dunes and yardangs in the Medusae Fossae Formation, located in the Martian mid-latitudes and is characterized by wind-sculpted landforms. The composition of the Medusae Fossae is unclear but may include indurated (hardened) volcanic ash deposits or remnant dust-ice mixtures that formed during a different Martian climate.

The bottom half of the image reveals dunes that have apparently become cemented. The dune field is heavily cratered and both the dunes and craters exhibit much erosion and degradation indicating that they are relatively old in age. Most craters do not have visible ejecta deposits (most likely due to erosion and/or mantling (being covered)) and have superposed smaller dunes and ripples that also indicate that the craters and thus the dunes on which they lie are old in age.

Sharp ridges formed from wind abrasion, or yardangs, are visible in the upper half of the image. Yardangs typically form in dry, desert environments with strong prevailing winds that are unidirectional and carry an abrasive sediment load. Abrasive winds erode the surface into parallel elongate landforms, or ridges, that are often three or more times longer than they are wide.

When viewed from above, these landforms often resemble the hull of a boat. Yardangs typically form in easily-eroded material, most likely sedimentary rock or volcanic ash deposits that contain some amount of sand. Yardangs are found on both Earth and Mars.


Written by: Maria Banks

OBSERVATION TOOLBOX
Acquisition date:19 October 2008 Local Mars time: 3:48 PM
Latitude (centered):-12.6 ° Longitude (East):178.1 °
Range to target site:280.2 km (175.1 miles)Original image scale range:28.0 cm/pixel
(with 1 x 1 binning) so objects ~84 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:20.6 ° Phase angle:45.8 °
Solar incidence angle:63 °, with the Sun about 27 ° above the horizon Solar longitude:144.0 °, Northern Summer
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:31.2 °
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 azimuth203.6°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_009609_1675Convergence angle26.2°

 

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STEREO PAIR
PSP_009609_1675

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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.