This VIS image shows a small portion of the boundary region between Terra Sabaea and Utopia Planitia. The ridges and valleys in this image were likely created by tectonic faulting. There is a small channel entering from the right side of the image. Material from this channel has been deposited in a circular region, which may be an impact crater, and then down one of the valleys.
Orbit Number: 61922 Latitude: 32.2155 Longitude: 72.2938 Instrument: VIS Captured: 2015-11-29 10:19
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 | Crater, Grayscale, Impact, Thermal | |
Acquisition Date | ||
Release Date | 2016-02-09 | |
Date in Caption | 2015-11-29 | |
Image Credit | NASA/JPL-Caltech/ASU | |
Source | photojournal.jpl.nasa.gov/catalog/PIA20255 | |
Identifier | PIA20255 |