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Frost Covered Gullies (PSP_001552_1410)

Frost Covered Gullies
Frost Covered Gullies (PSP_001552_1410)
Credit: NASA/JPL/University of Arizona

PSP_001552_1410 shows gullies in a crater in Terra Sirenum in the southern hemisphere of Mars.

This image was acquired during the winter, which explains the abundant frost (the bright material) seen throughout the image. The frost is likely water frost, as opposed to carbon dioxide, because temperatures at this latitude probably do not get cold enough for carbon dioxide to condense.

The formation mechanism of gullies is much debated. Several theories support erosion by liquid water, while others favor dry debris flows or carbon dioxide. A major unknown is, if the gullies are formed by liquid water, does the water originate from the surface or subsurface? Dendritic structures, such as those seen in the alcove displayed in the subimage (approximately 1.3 km across; 2560 x 3000, 7MB), form from surface runoff on Earth. Water originating in the subsurface would not produce a structure like this. This alcove is evidence for a surface source for the water possibly required to form gullies.

Also interesting about this scene is the fact that the gullies occur at multiple elevations along the same crater wall. This is uncommon on Mars. Gullies, whether or not they are found in conjunction with an obvious horizontal layer, usually form at the same elevation on a given slope. It is unknown what caused these gullies to form at multiple elevations. Their locations are suggestive of a distributed water source, which also favors a surface, rather than a confined subsurface origin of water, such as an aquifer.
Written by: Kelly Kolb

OBSERVATION TOOLBOX
Acquisition date:25 November 2006 Local Mars time: 3:40 PM
Latitude (centered):-38.9 ° Longitude (East):195.9 °
Range to target site:250.5 km (156.6 miles)Original image scale range:50.1 cm/pixel
(with 2 x 2 binning) so objects ~150 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:2.4 ° Phase angle:76.9 °
Solar incidence angle:75 °, with the Sun about 15 ° above the horizon Solar longitude:140.6 °, Northern Summer
For non-map projected products:
North azimuth:96 ° Sub-solar azimuth:41.0 °
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 azimuth213.8°
A N A G L Y P H   P R O D U C T S
Left observation:PSP_002172_1410Convergence angle16.4°

 

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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


P O S T S C R I P T

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.