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Dusty Lava Flows on Ascreaus Mons (PSP_002209_1865)

Dusty Lava Flows on Ascreaus Mons
Dusty Lava Flows on Ascreaus Mons (PSP_002209_1865)
Credit: NASA/JPL/University of Arizona

Ascreaus Mons is one of the giant shield volcanoes in the Tharsis region of Mars. Based on earlier lower resolution images, this location seemed to be ideal for examining how different types of lava flows interacted.

The smoother ground on the northwest side of the image is probably a lava flow with a relatively smooth crust much like "pahoehoe" lava flows in Hawaii.

The rugged terrain in the southwestern part of the image is indicative of a highly disrupted crust, possibly like what Hawaiians call an "aa" flow. Instead of confirming these hypotheses, HiRISE shows that the lava flow details are obscured by dust. The dust is carved into a curious network of scallops that are too small to have been seen by previous cameras.
Written by: Laszlo P. Keszthelyi

OBSERVATION TOOLBOX
Acquisition date:15 January 2007 Local Mars time: 3:38 PM
Latitude (centered):6.6 ° Longitude (East):258.5 °
Range to target site:265.5 km (165.9 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:1.1 ° Phase angle:55.3 °
Solar incidence angle:54 °, with the Sun about 36 ° above the horizon Solar longitude:167.2 °, Northern Summer
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:7.3 °
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 azimuth181.9°

 

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All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible: Image: NASA/JPL/University of Arizona


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.