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Small Cones North of Olympus Mons (PSP_006667_2150)

Small Cones North of Olympus Mons
Small Cones North of Olympus Mons (PSP_006667_2150)
Credit: NASA/JPL/University of Arizona

Olympus Mons is the largest volcano in the Solar System and is thought to have been active in the relatively recent past (which on Mars means many millions of years ago). While this towering giant gets a lot of the attention, it is surrounded by a vast field of other volcanic features. This HiRISE image takes a close look at one set of intriguing landforms: small cones.

Cones similar to these are found atop the freshest lava flows on Mars in Athabasca Valles. In that location, HiRISE found proof that they formed by steam exploding through the lava flow. The steam was produced by boiling water (or ice) in the ground underneath the lava flow. Could the same thing have happened here?

Unfortunately, HiRISE finds that this area north of Olympus Mons is covered in a thick layer of dust. While the wonderful resolution of HiRISE reveals details of the ripples in the dust, it cannot show us what is underneath the dust. Therefore we cannot prove that these cones formed the same was as the Athabasca Valles cones. They could be small volcanic vents, but it is unlikely that so many small eruptions would have taken place so close together.

However, since we cannot show that the ground under the dust is lava, we cannot rule out non-volcanic processes. Still, the similarity in the shapes and sizes of these cones to the ones in Athabasca Valles leaves open the possibility that water and lava interacted explosively here.

Written by: Laszlo P. Keszthelyi

OBSERVATION TOOLBOX
Acquisition date:28 December 2007 Local Mars time: 2:23 PM
Latitude (centered):34.4 ° Longitude (East):225.1 °
Range to target site:293.9 km (183.7 miles)Original image scale range:29.4 cm/pixel
(with 1 x 1 binning) so objects ~88 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:4.0 ° Phase angle:41.7 °
Solar incidence angle:45 °, with the Sun about 45 ° above the horizon Solar longitude:9.5 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:330.7 °
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 azimuth146.9°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_006957_2150Convergence angle19.2°

 

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SCIENCE THEME
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STEREO PAIR
PSP_006957_2150

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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


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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.