Baetis Chasma is a chasmata near but not directly connected to Valles Marineris. Dunes are prevalent on the floor of this portion of Juventae Chasma in this image taken by NASA's 2001 Mars Odyssey.
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Juventae Chasma

Context image for PIA13071
Context image

Baetis Chasma is a chasmata near Valles Marineris. It is not directly connected to Valles Marineris, but contains some of the same features seen in the larger chasmata. Dunes are prevalent on the floor of this portion of Juventae Chasma.

Orbit Number: 36444 Latitude: -4.68844 Longitude: 297.159 Instrument: VIS Captured: 2010-03-03 01:41

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.

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2001 Mars Odyssey

2001 Mars Odyssey

Thermal Emission Imaging System



Full-Res TIFF:
PIA13071.tif (3.7 MB)

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PIA13071.jpg (0.26 MB)

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