NASA's Mars Odyssey spacecraft captured this image in August 2003, showing a large outflow channel, split and diverted around an obstacle just north of Memnonia Fossae on Mars.

Released 8 August 2003

A large outflow channel was split and diverted around an obstacle just north of Memnonia Fossae. Images released on 11/06/02) and 05/28/03) may be a continuation of this channel and offer additional insight to the ancient flow of water and geologic history of this region.

Image information: VIS instrument. Latitude -13.6, Longitude 210.4 East (149.6 West). 19 meter/pixel resolution.

Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, 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.

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