HiRISE: High Resolution Imaging Science Experiment          The University of Arizona
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Clustered Impact Features
Clustered Impact Features
Clustered Impact Features  (PSP_008571_1995)
Credit: NASA/JPL/University of Arizona

Nili Fossae is a region that is thought to be approximately 3.5 billion years in age and, based on results from Omega, is the largest exposure of olivine (a common dark colored rock forming mineral found in igneous rocks) on the surface of Mars. The many fractures and grabens (depressed blocks of crust resulting from extension) that make up the region are believed to be the result of the Isidis impact basin.

Of particular interest are the two impact clusters found midway down this image. Each cluster is approximately 100 meters in diameter. The exact origin of such features is not known. It is thought that they are the result of a loosely conglomerated, stony meteoroid that broke apart during descent through the Martian atmosphere.


OBSERVATION TOOLBOX
Acquisition date:25 May 2008 Local Mars time: 3:09 PM
Latitude (centered):19.4 ° Longitude (East):75.6 °
Range to target site:283.5 km (177.2 miles)Original image scale range:28.4 cm/pixel
(with 1 x 1 binning) so objects ~85 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:9.0 ° Phase angle:52.3 °
Solar incidence angle:44 °, with the Sun about 46 ° above the horizon Solar longitude:76.5 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:21.3 °
For map projected products:
North azimuth:270°Sub solar azimuth195.171°

 

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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.