At the Summit of Arsia Mons Volcano
NASA/JPL/University of Arizona

At the Summit of Arsia Mons Volcano
PSP_002157_1715  Science Theme: Volcanic Processes


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Like the other major shield volcanoes on Mars, Arsia Mons has a caldera (large volcanic crater) at its summit.

Calderas form when magma (molten rock) is removed from the magma chamber in the volcano, and the roof of the magma chamber collapses into the resulting void. In the case of Arsia Mons, there are relatively young lava flows that overtop the northeast rim of the caldera.

This HiRISE image samples some of these lava flows. The long elliptical depression is the summit crater of a small shield volcano that fed some of these lava flows. At HiRISE resolution, we see that even these younger lavas are covered by a thick layer of dust. The small dark-rayed crater in the southwest edge of the image shows that the rock under the dust is dark, as expected of lava.
Written by: Laszlo P. Keszthelyi   (10 March 2010)



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Acquisition date:11 January 2007 Local Mars time: 3:41 PM
Latitude (centered):-8.5 degrees Longitude (East):240.1 degrees
Range to target site:244.7 km (153.0 miles)Original image scale range:49.0 cm/pixel (with 2 x 2 binning) so objects ~147 cm across are resolved
Map projected scale:50 cm/pixel and North is upMap projection:EQUIRECTANGULAR
Emission angle:0.1 degrees Phase angle:57.1 degrees
Solar incidence angle:57 degrees, with the Sun about 33 degrees above the horizon Solar longitude:165.0 degrees, Northern Summer
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North azimuth:97 degrees Sub-solar azimuth:19.4 degrees
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North azimuth:270 degreesSub solar azimuth:193.1 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.