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Tinto Vallis

Oct. 11, 2021
This image from NASA's Mars Odyssey shows a wide channel called Tinto Vallis. This northward flowing channel is 180 km (112 miles) long and is located in northern Hesperia Planum.
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The wide channel in the center of this VIS image is Tinto Vallis. This northward flowing channel is 180 km (112 miles) long and is located in northern Hesperia Planum. Tinto Vallis arises in the plains of Herperia Planum and empties into Palos Crater. In this image Tinto Vallis doglegs to the north, entering Palos Crater, and then exiting again into the northern lowland of Amenthes Planum.

Orbit Number: 85973 Latitude: -3.08676 Longitude: 110.715 Instrument: VIS Captured: 2021-05-02 07:46

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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