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Gullies in Utopia Planitia
Gullies in Utopia Planitia
Gullies in Utopia Planitia  (PSP_006724_2165)
Credit: NASA/JPL/University of Arizona

Seen here are gullies in a northern hemisphere crater. The crater is well-preserved as indicated by its sharp rim and steep walls. Gullies are rarer in the northern hemisphere, possibly because there are fewer slopes for them to form on compared to the heavily cratered southern highlands.

This image captures a range of gully morphologies. The gullies on the north wall (south facing) are more abundant and evenly-spaced than those on the east and south walls, and they extend up to the crater rim on the northern side. These differences might occur because of differences in sunlight exposure and temperature variations.

The crater floor has a linear texture suggestive of flow. Ice-rich material might have moved off the crater walls, driven by gravity, and flowed towards the crater center.


OBSERVATION TOOLBOX
Acquisition date:02 January 2008 Local Mars time: 2:21 PM
Latitude (centered):36.4 ° Longitude (East):107.8 °
Range to target site:298.2 km (186.4 miles)Original image scale range:29.8 cm/pixel
(with 1 x 1 binning) so objects ~90 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:3.4 ° Phase angle:48.4 °
Solar incidence angle:45 °, with the Sun about 45 ° above the horizon Solar longitude:11.6 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:329.8 °
For map projected products:
North azimuth:270°Sub solar azimuth144.891°

 

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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.