PIA17713: Lava Channels
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  2001 Mars Odyssey
 Spacecraft:  2001 Mars Odyssey
 Instrument:  THEMIS
 Product Size:  1430 x 2924 pixels (w x h)
 Produced By:  Arizona State University
 Full-Res TIFF:  PIA17713.tif (4.186 MB)
 Full-Res JPEG:  PIA17713.jpg (335.9 kB)

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Original Caption Released with Image:

Context image for PIA17713
Context image

The channels and linear depression in this VIS image are located on the western margin of the Elysium Volcanic complex. The channels were created by lava flow.

Orbit Number: 52464 Latitude: 29.9196 Longitude: 139.502 Instrument: VIS Captured: 2013-10-11 20:12

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.

Image Credit:
NASA/JPL-Caltech/ASU

Image Addition Date:
2013-12-03