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NASA Mars Odyssey THEMIS Image: Overlapping Flows

Status Report From: Mars Odyssey THEMIS
Posted: Thursday, December 23, 2004

Medium image for 20041223A
Image Context:
Context image for 20041223A
Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team
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ParameterValue ParameterValue
Latitude-6.4   InstrumentIR
Longitude229.6E (130.4W)   Resolution (m)100
Image Size (pixels)2870x320   Image Size (km)287x32

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. Toward the top of the image a set of dark-toned overlapping flows can be identified by the darker margins where dust/sand has been trapped against the flow margin.

[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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