Valley West of Ganges Chasma
NASA/JPL/University of Arizona

Valley West of Ganges Chasma
PSP_009011_1705  Science Theme: Geologic Contacts/Stratigraphy
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This image shows an apparent valley north of a 37-kilometer long pit called Ophir Cavus.This valley is just west of another 155-km long valley system called Allegheny Vallis that also emanates from the pit.

The association of valleys with the pit suggests that water was released when the pit formed, perhaps when volcanic eruptions melted ice in the surface or subsurface. The HiRISE image reveals light-toned units along portions of the plains and these could be minerals deposited by the flowing water or alteration of the plains by the water that once flowed here.

Written by: Cathy   (12 August 2008)



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Acquisition date:28 June 2008 Local Mars time: 3:24 PM
Latitude (centered):-9.6 degrees Longitude (East):304.8 degrees
Range to target site:258.8 km (161.7 miles)Original image scale range:25.9 cm/pixel (with 1 x 1 binning) so objects ~78 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:EQUIRECTANGULAR
Emission angle:2.2 degrees Phase angle:59.2 degrees
Solar incidence angle:61 degrees, with the Sun about 29 degrees above the horizon Solar longitude:91.5 degrees, Northern Summer
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North azimuth:97 degrees Sub-solar azimuth:41.6 degrees
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North azimuth:270 degreesSub solar azimuth:215.8 degrees

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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.