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Hydaspis Chaos
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Caption:
Context image
Today's VIS image shows a small section of Hydaspis Chaos, one of many regions of chaos in Margaritifer Terra. The term chaos is applied to regions where the surface is being eroded to form mesas. As the surface processes continue individual mesas become more isolated and take on the appearance of regions of hills. Hydaspis Chaos is is part of the huge outflow system flowing from Valles Marineris to Chryse Planitia.
Orbit Number: 79027 Latitude: 2.3043 Longitude: 335.049 Instrument: VIS Captured: 2019-10-08 09:37
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 | |
| Acquisition Date | ||
| Release Date | 2019-11-14 | |
| Date in Caption | 2019-10-08 | |
| Image Credit | NASA/JPL-Caltech/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA23544 | |
| Identifier | PIA23544 | |
