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Gullies in Dao Vallis
Gullies in Dao Vallis
Gullies in Dao Vallis  (PSP_006659_1460)
Credit: NASA/JPL/University of Arizona

Gullies on the northwest side of Dao Vallis, a Martian outflow channel, are the focus of this observation. The outflow channels are thought to have been carved by gigantic, ancient floods.

Gullies are largely thought to be the result of water flow, but the origin of the water is much debated. One theory proposes that melting snowpack, or a mantling (blanketing) unit, forms gullies. Such a mantling unit is visible here between some of the gullies, in the full high-resolution image. Some alcove-shaped features appear to have mantling material in them. If the mantling unit is indeed related to gully formation, then gullies are potentially forming here.


OBSERVATION TOOLBOX
Acquisition date:28 December 2007 Local Mars time: 2:36 PM
Latitude (centered):-33.9 ° Longitude (East):92.1 °
Range to target site:255.4 km (159.6 miles)Original image scale range:25.5 cm/pixel
(with 1 x 1 binning) so objects ~77 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:0.7 ° Phase angle:52.6 °
Solar incidence angle:53 °, with the Sun about 37 ° above the horizon Solar longitude:9.2 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:43.4 °
For map projected products:
North azimuth:270°Sub solar azimuth216.602°

 

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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.