This VIS image shows a portion of the ejecta deposit of Yuty Crater. The raised edge of the ejecta is termed a rampart, and indicates that a volatile like water may have been present. The ejecta edge looks like a flow front and much different from air fall ejecta emplacement.
Orbit Number: 68736 Latitude: 22.247 Longitude: 325.213 Instrument: VIS Captured: 2017-06-12 17:57
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.
|Mission||2001 Mars Odyssey|
|Instrument Host||2001 Mars Odyssey|
|Instrument||Thermal Emission Imaging System (THEMIS)|
|Extra Keywords||Crater, Grayscale, Water|
|Date in Caption||2017-06-12|