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Knobs, Bright Deposits, and Inverted Channels in Eberswalde Crater (PSP_010052_1560)

Knobs, Bright Deposits, and Inverted Channels in Eberswalde Crater
Credit: NASA/JPL/University of Arizona

Eberswalde Crater is an approximately 65-kilometer diameter, closed basin crater. It contains a delta, which indicates that flowing water was present for an extended period of time in the past.

Parts of the crater have inverted channels that have higher relief because a more resistant material was deposited in the channel and therefore it was less susceptible to erosion than the surrounding area. The image also shows resistant knobs and mounds as well as a scoured surface.

The CRISM instrument on-board MRO has detected phyllosilicates (clays) in some of the bright layers here. On Earth, clays form in the presence of water, so this is more evidence that there was a persistent flow of water in Eberswalde.


OBSERVATION TOOLBOX
Acquisition date:17 September 2008 Local Mars time: 3:43 PM
Latitude (centered):-23.9 ° Longitude (East):326.6 °
Range to target site:266.3 km (166.4 miles)Original image scale range:26.6 cm/pixel
(with 1 x 1 binning) so objects ~80 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:12.9 ° Phase angle:60.2 °
Solar incidence angle:69 °, with the Sun about 21 ° above the horizon Solar longitude:128.6 °, Northern Summer
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:39.9 °
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 azimuth212.9°

 

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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.