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Cryptic Terrain on Mars
Cryptic Terrain on Mars
Cryptic Terrain on Mars  (PSP_003179_0945)
Credit: NASA/JPL/University of Arizona

This caption is part of a December 2007 AGU presentation "Spring at the South Pole of Mars."

There is an enigmatic region near the south pole of Mars known as the "cryptic" terrain. It stays cold in the spring, even as its albedo darkens and the sun rises in the sky.

This region is covered by a layer of translucent seasonal carbon dioxide ice that warms and evaporates from below. As carbon dioxide gas escapes from below the slab of seasonal ice it scours dust from the surface. The gas vents to the surface, where the dust is carried downwind by the prevailing wind.

The channels carved by the escaping gas are often radially organized and are known informally as "spiders."


OBSERVATION TOOLBOX
Acquisition date:01 April 2007 Local Mars time: 6:19 PM
Latitude (centered):-85.4 ° Longitude (East):104.0 °
Range to target site:245.9 km (153.7 miles)Original image scale range:49.2 cm/pixel
(with 2 x 2 binning) so objects ~148 cm across are resolved
Map projected scale:50 cm/pixelMap projection:POLAR STEREOGRAPHIC
Emission angle:3.8 ° Phase angle:74.7 °
Solar incidence angle:78 °, with the Sun about 12 ° above the horizon Solar longitude:210.8 °, Northern Autumn
For non-map projected products:
North azimuth:147 ° Sub-solar azimuth:33.9 °
For map projected products:
North azimuth:14.0878°Sub solar azimuth278.169°

 

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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.