JavaScript is required
JPL Logo
Image

Patapsco Vallis

Jan. 8, 2014
This image captured by NASA's 2001 Mars Odyssey spacecraft shows where Patapsco Vallis enters the largest depression of Elysium Fossae. Patapsco Vallis, on the Elysium Mons volcanic complex, was likely formed by the flow of lava rather than water.
Context Image

This VIS image shows where Patapsco Vallis enters the largest depression of Elysium Fossae. Patapsco Vallis, as other valley systems on the Elysium Mons volcanic complex, was likely formed by the flow of lava rather than water.

Orbit Number: 52938 Latitude: 23.8099 Longitude: 153.968 Instrument: VIS: Captured: 2013-11-19 20:20

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.

Keep Exploring