Aonia Terra Periglacial Sample
NASA/JPL/University of Arizona

Aonia Terra Periglacial Sample
ESP_013958_1170  Science Theme: Glacial/Periglacial Processes
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Throughout this entire image in Aonia Terra, it is possible to make out regular polygonally shaped patterns. Here on Earth, wherever ice-rich permafrost occurs (soil which stays frozen throughout the year), the ground may crack and form similar patterns to those we see on Mars.

Despite remaining below freezing, changes in seasons and ground temperature cause significant thermal-contraction stress, enough so that the terrain fractures into a honeycomb network of subsurface cracks.

Criss-crossed dark paths wind throughout this region. Dust devils, turbulent whirlwinds fueled by rising ground-warmed atmosphere, track across the surface, stripping the ground of bright surface dust as they go. Comparable to miniature tornadoes, they efficiently transport surface materials on Mars. Left in their passing is the darker coarse-grained soil underneath.

In this image, the sun is low on the horizon; the shadows make it easier to see the scattered rocks and boulders. Sometimes, these boulders occur in rings, the remnants of an ancient impact whose crater has since eroded to a flat surface. The boulders are left behind, illustrating where the form of the crater once stood.

Written by: Albert Ortiz/Michael Mellon   (2 September 2009)



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Acquisition date:19 July 2009 Local Mars time: 2:43 PM
Latitude (centered):-62.6 degrees Longitude (East):252.9 degrees
Range to target site:246.1 km (153.8 miles)Original image scale range:24.6 cm/pixel (with 1 x 1 binning) so objects ~74 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:EQUIRECTANGULAR
Emission angle:0.3 degrees Phase angle:50.9 degrees
Solar incidence angle:51 degrees, with the Sun about 39 degrees above the horizon Solar longitude:305.9 degrees, Northern Winter
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North azimuth:98 degrees Sub-solar azimuth:44.1 degrees
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North azimuth:270 degreesSub solar azimuth:215.3 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.