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Proctor Crater Dune Field (PSP_002455_1320)

Proctor Crater Dune Field
Proctor Crater Dune Field (PSP_002455_1320)
Credit: NASA/JPL/University of Arizona

Image PSP_002455_1320 shows the edge of a dark dune field on the floor of Proctor crater, a 150 kilometer diameter crater in the southern highlands of Mars.

The subimage (1261 x 603, 2.2 MB) is a close-up view of the dark dunes. These dunes are most likely composed of basaltic sand that has collected on the bottom of the crater. Superimposed on their surface are smaller secondary dunes which are commonly seen on terrestrial dunes of this size. Near the crests of the dark dunes are bright patches of frost. Dark spots within the frost patches are areas where defrosting is occurring.

Many smaller and brighter bed forms, most likely small dunes or granule ripples, cover the substrate between the larger dark dunes as well as most of the floor of Proctor Crater. In many locations, large boulders are seen on the same surfaces as the bright bed forms. The dark dunes stratigraphically overlie the small bright bed forms indicating that the darker dunes formed more recently.

However in several areas, the dark dunes appear to influence the orientation of the small bright dunes, possibly by wind flowing around the larger dunes, suggesting that both dark and bright bed forms are coeval.


Written by: Maria Banks

OBSERVATION TOOLBOX
Acquisition date:03 February 2007 Local Mars time: 3:56 PM
Latitude (centered):-47.8 ° Longitude (East):30.7 °
Range to target site:253.5 km (158.4 miles)Original image scale range:25.4 cm/pixel
(with 1 x 1 binning) so objects ~76 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:6.7 ° Phase angle:65.1 °
Solar incidence angle:71 °, with the Sun about 19 ° above the horizon Solar longitude:177.7 °, Northern Summer
For non-map projected products:
North azimuth:98 ° Sub-solar azimuth:30.4 °
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 azimuth203.4°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_003101_1320Convergence angle31.1°

 

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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


P O S T S C R I P T

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.