This observation crosses over a part of the hemispheric dichotomy boundary on Mars which separates low-lying northern plains from older southern highlands.

In the northern part of the scene, much of the surface is covered with small boulders, most only 1 to 2 meters wide (1 meter is approximately 1 yard). In other areas, it appears that sand or dust has accumulated in depressions, forming light patches. These areas also show short sinuous or linear features, likely ripples formed from wind-blown material. The southern part contains an old valley, now mantled by later deposits, and has a pitted texture due to erosion.

It has been proposed that the lowland was once filled by an ocean. In this case several arcuate or linear features along the boundary slope could be old shorelines, but this interpretation is still debated. The features have been modified by erosion, and in some cases appear to slope towards the highlands.

Written by: Colin Dundas

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

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.