Dry Ice and Dunes
NASA/JPL/University of Arizona

Dry Ice and Dunes
PSP_007494_2580  Science Theme: Aeolian Processes
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Mars has a vast sea of sand dunes in the high latitude region encircling its North polar cap, known as the North polar erg. These dunes are made up of basalt and gypsum sand grains.

In some regions of the North polar erg where the sand supply is limited they take on an elongated crescent shape (see PSP_009324_2650). The icy ground that the dunes are on top of has irregular polygonal patterns. In other areas with an abundant supply of sand the dunes are continuous.

The entire North polar erg is covered in the winter with a seasonal polar cap composed of carbon dioxide (dry ice). In the springtime this seasonal polar cap evaporates. This image shows the dunes mostly still covered with dry ice, but the dark spots are places where the ice has evaporated and the dark sand of the dune is visible.
Written by: Candy Hansen   (25 August 2010)



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Acquisition date:02 March 2008 Local Mars time: 1:52 PM
Latitude (centered):77.8 degrees Longitude (East):307.2 degrees
Range to target site:321.4 km (200.9 miles)Original image scale range:from 32.2 cm/pixel (with 1 x 1 binning) to 64.3 cm/pixel (with 2 x 2 binning)
Map projected scale:25 cm/pixelMap projection:POLAR STEREOGRAPHIC
Emission angle:6.4 degrees Phase angle:68.5 degrees
Solar incidence angle:64 degrees, with the Sun about 26 degrees above the horizon Solar longitude:39.5 degrees, Northern Spring
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North azimuth:106 degrees Sub-solar azimuth:315.2 degrees
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North azimuth:322.7 degreesSub solar azimuth:173.2 degrees

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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.