Scarp-Fed Dark Dunes
NASA/JPL/University of Arizona

Scarp-Fed Dark Dunes
PSP_010344_2655  Science Theme: Polar Geology


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Multiple levels within the north polar layered deposits are visible in this HiRISE image.

The north polar layered deposits (NPLD) are a stack of dusty water-ice layers that are thought to record information about past Martian climates in the same way that ice-caps on the Earth record variations in our climate. These Martian layers are visible in the walls of troughs and scarps eroded into the stack. One such scarp-face is visible on the far left of the full image and decreases in height from left to right.

Scientists continue to debate the length of time required to accumulate this stack of layers with estimates ranging from a few million years to about a billion years. Although we don’t yet know which layer corresponds to which time in Mars’ history, we can still use these layers to try to understand how the climate has changed over this period.

The topmost layers, which are the most recent (far left of the image), are brighter and appear brownish in this false-color view. They are interpreted to be a mixture of water ice and dust. The lower layering is more complex and appears to be a mixture of bright whiteiish layers (that we think are ice) and dark blue-ish layers (which we think are mostly sand). A large pit in the center of the image penetrates deeply into this stack of layers and shows these alternating sandy and icy layers extending to depths of hundreds of meters (about 1000 feet).

Erosion of the dark sandy layers releases sandy material which collects into dunes such as the linear example that stretches across the middle of this image.
Written by: Shane Byrne   (19 August 2009)

This is a stereo pair with PSP_009885_2655.



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Acquisition date:10 October 2008 Local Mars time: 9:59 AM
Latitude (centered):85.7 degrees Longitude (East):179.4 degrees
Range to target site:330.6 km (206.6 miles)Original image scale range:66.1 cm/pixel (with 2 x 2 binning) so objects ~198 cm across are resolved
Map projected scale:50 cm/pixelMap projection:POLAR STEREOGRAPHIC
Emission angle:17.5 degrees Phase angle:84.7 degrees
Solar incidence angle:70 degrees, with the Sun about 20 degrees above the horizon Solar longitude:139.7 degrees, Northern Summer
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North azimuth:175 degrees Sub-solar azimuth:321.6 degrees
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North azimuth:90.59 degreesSub solar azimuth:239.8 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.