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Possible Cinder Cone on the Southern Flank of Pavonis Mons (PSP_002671_1790)

Possible Cinder Cone on the Southern Flank of Pavonis Mons
Possible Cinder Cone on the Southern Flank of Pavonis Mons (PSP_002671_1790)
Credit: NASA/JPL/University of Arizona

This image is centered on a small cone on the side of one of Mars' giant shield volcanoes. The cone shows some layers of hard rock but most of it is made of relatively soft material. This appears to be an example of a "cinder" cone composed of pieces of lava thrown into the air during a small volcanic eruption.

Typically, such eruptions produce fountains of molten lava. Most of the lava would have cooled in this fountain, producing a loose pile of lava rocks. However, it appears that some pulses of the eruption allowed the lava to land without cooling much. These pieces were hot enough to weld together to make the hard layers we see today. The cone is 700 x 1100 m (2300 x 3600 feet) in size, similar to many cinder cones on Earth.

In other parts of the image, we see channels carved by lava. It is sometimes difficult to tell if a channel was formed by flowing water or lava; in this case, it is possible to see that lava flows feed out of these channels.
Written by: Laszlo P. Keszthelyi

OBSERVATION TOOLBOX
Acquisition date:20 February 2007 Local Mars time: 3:43 PM
Latitude (centered):-1.1 ° Longitude (East):246.6 °
Range to target site:254.5 km (159.1 miles)Original image scale range:50.9 cm/pixel
(with 2 x 2 binning) so objects ~153 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:2.5 ° Phase angle:53.3 °
Solar incidence angle:56 °, with the Sun about 34 ° above the horizon Solar longitude:187.3 °, Northern Autumn
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:3.2 °
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 azimuth177.0°
A N A G L Y P H   P R O D U C T S
Left observation:ESP_011413_1790Convergence angle17.1°

 

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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.