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Eastern Hebes Chasma
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Caption:
Context image
Today's VIS image shows part of eastern Hebes Chasma. The floor of the chasma is covered with chaotic materials, some from landslides and other layered deposits of unknown origin. Hebes Chasma is a closed basin north of Valles Marineris. It measures 126km wide north/south (78 miles), 315 km long east/west (196 miles), and 8 km (5 miles) at its deepest point.
Orbit Number: 88001 Latitude: -1.32567 Longitude: 284.971 Instrument: VIS Captured: 2021-10-16 07:20
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 | 2022-01-14 | |
| Date in Caption | 2021-10-16 | |
| Image Credit | NASA/JPL-Caltech/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA25105 | |
| Identifier | PIA25105 | |
