Mars Odyssey THEMIS Image: Oympus Mons Flows
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| Like drippings from a candle, these lava flows on the flank of Olympus Mons volcano demonstrate how it became the largest volcano in the solar system. Multiple flows from an unknowable number of eruptions have piled one on top of another until the mountain of lava reached a height of 27 km above the average Martian elevation. The change in texture seen in the bottom 1/3 of the image marks a break in slope from the flank of the volcano to the north (top) and the flat plain surrounding it. The direction of flows changes from roughly N-S to E-W, suggesting another source for the flows on the plain. [Questions? Email images@themis.asu.edu] [Source: ASU THEMIS Science Team] |
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
| Parameter | Value | Parameter | Value | |
|---|---|---|---|---|
| Latitude | 12.9 |   | Instrument | VIS |
| Longitude | 223.6E (136.4W) |   | Resolution (m) | 19 |
| Image Size (pixels) | 3025×1233 |   | Image Size (km) | 57.5×23.4 |

