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Aram Chaos
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Caption:
Context image
Today's VIS image shows part of Aram Chaos. Aram Chaos was initially formed by a large impact. Over time the crater interior was modified by several different processes, including liquid water. Chaos forms from erosion of the surface into mesa features. With time the valleys expand creating the jumble of hills seen in the image.
Orbit Number: 80125 Latitude: 1.19021 Longitude: 338.127 Instrument: VIS Captured: 2020-01-06 19:28
Background Info:
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Science Mission Directorate, 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.
Cataloging Keywords:
| Name | Value | Additional Values |
|---|---|---|
| Target | Mars | |
| System | ||
| Target Type | Planet | |
| Mission | 2001 Mars Odyssey | |
| Instrument Host | Mars Odyssey | |
| Host Type | Orbiter | |
| Instrument | Thermal Emission Imaging System (THEMIS) | |
| Detector | ||
| Extra Keywords | Crater, Grayscale, Impact, Thermal, Water | |
| Acquisition Date | ||
| Release Date | 2020-03-26 | |
| Date in Caption | 2020-01-06 | |
| Image Credit | NASA/JPL-Caltech/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA23814 | |
| Identifier | PIA23814 | |
