The lava flows from Arsia Mons are some of the youngest flows in the region, as seen in this image from NASA's Mars Odyssey spacecraft. The flows are long, fairly narrow, overlapping, and with various surface features and textures.
figure 1 for PIA03963

The lava flows from Arsia Mons are some of the youngest flows in the region. The region of flows south of the volcano have had little modification and appear very similar in appearance to Hawaiian lava flows. This VIS image shows typical flows for the region. The flows are long, fairly narrow, overlapping, and with various surface features and textures.

Image information: VIS instrument. Latitude -19.5, Longitude 240.1 East (119.9 West). 17 meter/pixel resolution.

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.

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