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Olympus Rupes

The margin of Olympus Mons consists of a cliff-like edge where elevation changes very quickly over a very small width. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of that edge.
PIA21155
Credits: NASA/JPL-Caltech/ASU
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Context image for PIA21155
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The margin of Olympus Mons consists of a cliff-like edge where elevation changes very quickly over a very small width. This edge is called Olympus Rupes. This VIS image shows part of that edge and the lava flows that spilled over the edge to flood the surrounding plains.

Orbit Number: 65335 Latitude: 16.0811 Longitude: 221.373 Instrument: VIS Captured: 2016-09-05 12:58

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.