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Olympus Rupes is the name of the large escarpment surrounding Olympus Mons. The escarpment is a cliff where there is a large elevation change over a short distance. The elevation change from the lower volcanic plains to the volcano flank is up to 8km (5 miles), almost the height of Mount Everest. This VIS image is located along the northern margin of Olympus Mons, the largest Martian volcano. The brighter toned material in the central part of this image is the escarpment, with the lower elevation surface at the top of the image.

Orbit Number: 89625 Latitude: 21.7334 Longitude: 229.57 Instrument: VIS Captured: 2022-02-27 00:48

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.