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Shalbatana Vallis
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Caption:
Context image
Today's VIS image shows a portion of Shalbatana Vallis. Located in Xanthe Terra, Shalbatana Vallis is an outflow channel carved by massive floods of escaping groundwater whose source lies far to the south of this image. Shalbatana Vallis is over 1300 km long (808 miles). This channel, and all others in this region, drain into Chryse Planitia.
Orbit Number: 86752 Latitude: 5.19688 Longitude: 316.501 Instrument: VIS Captured: 2021-07-05 11:12
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 | Grayscale, Thermal, Water | |
| Acquisition Date | ||
| Release Date | 2021-11-16 | |
| Date in Caption | 2021-07-05 | |
| Image Credit | NASA/JPL-Caltech/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA24992 | |
| Identifier | PIA24992 | |
