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NASA Mars Odyssey THEMIS Image: Lava Flows and Fault In IR

Status Report From: Mars Odyssey THEMIS
Posted: Wednesday, December 22, 2004

Medium image for 20041222A
Image Context:
Context image for 20041222A
Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team
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ParameterValue ParameterValue
Latitude-19.1   InstrumentIR
Longitude239.7E (120.3W)   Resolution (m)100
Image Size (pixels)3043x320   Image Size (km)304.3x32

Full data on this image has now been released via the THEMIS Data Releases website.

This is a nighttime IR image of lava flows from Arsia Mons. Arsia Mons flows cover an extensive region, and appear to be some of the youngest flows from the Tharsis Montes. The linear feature at the bottom of the images is a fault.

[Source: ASU THEMIS Science Team]

Note: this THEMIS infrared 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


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