Olympus Rupes is the name of the large escarpment surrounding Olympus Mons. The escarpment is a cliff where there is a large elevation change over a short distance. The elevation change from the lower volcanic plains to the volcano flank is up to 5 miles (26,400 feet), almost the height of Mount Everest. This VIS image is located along the southeastern margin of Olympus Mons, the largest Martian volcano.
Orbit Number: 85819 Latitude: 16.3331 Longitude: 230.812 Instrument: VIS Captured: 2021-04-19 15:33
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.
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, Mountain, Thermal, Volcano | |
Acquisition Date | ||
Release Date | 2021-09-13 | |
Date in Caption | 2021-04-19 | |
Image Credit | NASA/JPL-Caltech/ASU | |
Source | photojournal.jpl.nasa.gov/catalog/PIA24876 | |
Identifier | PIA24876 |