This image shows an exposure of the north polar layered deposits (center). The layering visible here might have been formed by recent climate variations on Mars, similar to ice ages on Earth.

While the polar layered deposits are mostly water ice, exposures such as this are typically covered by a layer of red dust, protecting the underlying ice from evaporation during the summer. This dusty layer hides the internal composition of the polar layered deposits from view, but variations in the slopes of the surfaces of the layers are still visible.

The slope of each layer is probably affected by the internal composition, so the topography of exposures like this is of interest to scientists. When this image was taken (northern spring), the surface was mostly covered by seasonal carbon dioxide frost. This white frost layer helps to highlight the surface slopes because the visible brightness variations are mainly caused by topographic variations. Therefore, this image will be useful for photoclinometric, or "shape from shading" analyses that can yield topographic maps limited only by the resolution of the image.

Written by: Ken Herkenhoff

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.