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Large Polygons in Deuteronilus Mensae (PSP_007492_2265)

Large Polygons in Deuteronilus Mensae
Large Polygons in Deuteronilus Mensae (PSP_007492_2265)
Credit: NASA/JPL/University of Arizona

This image reveals hexagonal and polygonal patterns formed by networks of soil troughs on the floor of a valley in the Deuteronilus Mensae region, located on the northern edge of Arabia Terra and borders the Martian southern highlands and northern lowlands.

The polygonal patterns indicate that the surface has undergone stress, potentially caused by subsidence (sinking), desiccation (drying out), or thermal contraction. These polygon features are similar to permafrost thermal-contraction polygons that form in polar and high alpine regions on Earth by seasonal-to-annual contraction of the subsoil. On Earth, such polygon features are indicative of the presence of ground ice and are commonly referred to as “patterned ground.” The patterns are the result of thermal contraction in ice-cemented soil or permafrost that forms a honeycomb network of small fractures below the surface. The network of fractures is eventually manifested as shallow troughs at the surface, forming the hexagonal and polygonal patterns visible in this image.

The polygons in this scene average approximately 100 meters (110 yards) in size and appear to be higher in elevation in the center than in the surrounding troughs. Boulders are accumulated in the center of the polygons and dunes are visible in several of the troughs.

The landforms we observe here most likely indicate that ice-rich permafrost is present or has been present in the past.

Written by: Maria Banks

OBSERVATION TOOLBOX
Acquisition date:02 March 2008 Local Mars time: 2:37 PM
Latitude (centered):46.1 ° Longitude (East):15.5 °
Range to target site:307.4 km (192.1 miles)Original image scale range:30.8 cm/pixel
(with 1 x 1 binning) so objects ~92 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:8.7 ° Phase angle:52.9 °
Solar incidence angle:45 °, with the Sun about 45 ° above the horizon Solar longitude:39.4 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:335.9 °
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 azimuth150.7°
A N A G L Y P H   P R O D U C T S
Left observation:PSP_007703_2265Convergence angle13.5°

 

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SCIENCE THEME
Glacial/Periglacial Processes

STEREO PAIR
PSP_007703_2265

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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.