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The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of the floor of Danielson Crater. This crater has deposits of material on the floor that have the appearance of wind erosion. The ridges and elongate hills are indications of wind direction. The dark blue material in this image is sand, most likely basaltic. The sand has formed dunes, but also can be seen filling small valleys to the upper right of the main dune.

Orbit Number: 13206 Latitude: 7.82772 Longitude: 353.071 Instrument: VIS Captured: 2004-12-05 18:35

Please see the THEMIS Data Citation Note for details on crediting THEMIS images.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Science Mission Directorate, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.