This image taken by NASA's 2001 Mars Odyssey spacecraft shows a portion of Scamander Vallis. Dark slope streaks are also visible on the west-facing wall of the channel.
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Scamander Vallis

Context image for PIA12405
Context image
Credit: NASA/JPL/MOLA

This VIS image shows a portion of Scamander Vallis. Dark slope streaks are also visible on the west-facing wall of the channel.

Image information: VIS instrument. Latitude 14.7N, Longitude 29.0E. 21 meter/pixel resolution.

Please see the THEMIS Data Citation Note for details on crediting THEMIS images.

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.

Image details

ID#:
PIA12405

Date added:
2009-12-16

Target:
Mars

Mission:
2001 Mars Odyssey

Spacecraft:
2001 Mars Odyssey

Instruments:
Thermal Emission Imaging System

Rating:



Views:
5,396

Full-Res TIFF:
PIA12405.tif (4.01 MB)

Full-Res JPG:
PIA12405.jpg (0.44 MB)

Image credit:
NASA/JPL/ASU