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Baetis Chaos
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Caption:
Context image
Today's VIS image shows part of Baetis Chaos. This region of chaos is located north of Juventae Chasma. Juventae Chasma is a huge box canyon near Valles Marineris. Water flowed from Juventae Chasma, through Baetis Chaos and created the northward flowing channel called Maja Valles.
Orbit Number: 81212 Latitude: -0.365878 Longitude: 299.435 Instrument: VIS Captured: 2020-04-05 07:31
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 | Mariner |
| Instrument Host | Mars Odyssey | |
| Host Type | Orbiter | Flyby Spacecraft |
| Instrument | Thermal Emission Imaging System (THEMIS) | |
| Detector | ||
| Extra Keywords | Grayscale, Thermal, Water | |
| Acquisition Date | ||
| Release Date | 2020-06-09 | |
| Date in Caption | 2020-04-05 | |
| Image Credit | NASA/JPL-Caltech/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA23942 | |
| Identifier | PIA23942 | |
