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 | | Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team | [ Find on map: Javascript version ]
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This somewhat cloudy THEMIS visible image shows a stunning example of
layered deposits in Terby crater, just north of the Hellas impact basin.
Some researchers argue that layered terrain in craters were deposited by
water. However, in some places, layered deposits will extend for up to a
kilometer above the crater rim, leading others to conclude that they must
be volcanic airfall deposits.
[Source: ASU THEMIS Science Team]
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 Credit: NASA/JPL/Arizona State University |
