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Lava-Filled Crater in Elysium Planitia (PSP_008753_1880)

Lava-Filled Crater in Elysium Planitia
Lava-Filled Crater in Elysium Planitia (PSP_008753_1880)
Credit: NASA/JPL/University of Arizona

Elysium Planitia is a part of the Martian lowlands that has been repeatedly covered by vast floods of lava. This image shows an older impact crater that has been filled by one of the youngest of those lava floods.

Only sections of the circular rim of the crater remain uncovered. The lava surface consists of ridged plates that have rafted apart with smoother lava filling between the plates. The ridges formed as the solidifying lava crust was crumpled by compression, and the gaps between the plates formed as the crust was pulled apart. Similar compression and extension of lava crust has been observed in the largest lava flows in Iceland.

The most puzzling aspect of this image is that the lava in the floor of the crater appears to have sunk down compared to its surroundings. This happened after a thick crust had formed on the lava. The most likely explanation is that the last molten lava inside the flow drained away through a now buried gap in the crater rim.

A final point of interest are the small circular cones visible near the center of the crater. These formed when ground water (or ice) was turned to steam by the heat of the lava flow. This steam exploded through the flow, producing the small cratered cones.
Written by: Laszlo P. Keszthelyi

OBSERVATION TOOLBOX
Acquisition date:08 June 2008 Local Mars time: 3:20 PM
Latitude (centered):7.9 ° Longitude (East):148.5 °
Range to target site:281.3 km (175.8 miles)Original image scale range:56.3 cm/pixel
(with 2 x 2 binning) so objects ~169 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:10.9 ° Phase angle:41.8 °
Solar incidence angle:51 °, with the Sun about 39 ° above the horizon Solar longitude:82.7 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:32.5 °
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 azimuth205.7°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_009610_1880Convergence angle12.6°

 

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PSP_009610_1880

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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.