PIA18753: Faults and Flows
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  2001 Mars Odyssey
 Spacecraft:  2001 Mars Odyssey
 Instrument:  THEMIS
 Product Size:  1391 x 2954 pixels (w x h)
 Produced By:  Arizona State University
 Full-Res TIFF:  PIA18753.tif (4.114 MB)
 Full-Res JPEG:  PIA18753.jpg (367.7 kB)

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Original Caption Released with Image:

Context image for PIA18753
Context image

Lava flows of Daedalia Planum can be seen at the top and bottom portions of this VIS image. The ridge and linear depression in the central part of the image are part of Mangala Fossa, a fault bounded graben.

Orbit Number: 56476 Latitude: -15.1511 Longitude: 219.447 Instrument: VIS Captured: 2014-09-06 23:36

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:
2014-10-20