Context image for PIA10309
Old Dunes
The crater just out of frame to the left in this image is located on the floor of
Schiaparelli Crater. Within the lows of the ejecta blanket of the small crater
are old, linear dunes. These dunes do not appear to be active at this time.
Image information: VIS instrument. Latitude -2.9N, Longitude 14.5E.
18 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.