Status Report

Mars Odyssey THEMIS Image: Volcano Vents

By SpaceRef Editor
May 5, 2003
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Medium image for 20030505a

Image Context:

Context image for 20030505a
Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team
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This low-relief shield volcano imaged with the THEMIS visible camera has two
large vents which have erupted several individual lava flows. The positions
of the orgins of many of the flows indicate that it is probable that the
vents are secondary structures that formed only after the shield was built up
by eruptions from a central caldera.


[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


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ParameterValue ParameterValue
Latitude17.6 &nbsp InstrumentVIS
Longitude243.6E (116.4W) &nbsp Resolution (m)19
Image Size (pixels)3025×1228 &nbsp Image Size (km)57.5×23.3

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