PIA26025: Oti Fossae
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  2001 Mars Odyssey
 Spacecraft:  2001 Mars Odyssey
 Instrument:  THEMIS
 Product Size:  601 x 2706 pixels (w x h)
 Produced By:  Arizona State University
 Full-Res TIFF:  PIA26025.tif (770.8 kB)
 Full-Res JPEG:  PIA26025.jpg (115 kB)

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The linear features in the bottom half of this VIS image are called Oti Fossae. Oti Fossae is located on the eastern flank of Arsia Mons and aligns with the regional northeast/southwest trend of the major Tharsis volcanoes. Fossae are typically tectonic features termed graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. The crustal deformation in this region was from the inflation of the surface by the rise of magma that created the Tharsis volcanoes.

Arsia Mons is the southernmost and youngest of the three large, aligned Tharsis volcanoes [Arsia Mons, Pavonis Mons and Ascreaus Mons, from south to north]. This alignment may indicate a large fracture/vent system was responsible for the eruptions that formed all three volcanoes. Arsia Mons is 270 miles (450km) in diameter, almost 12 miles (20km) high, and the summit caldera is 72 miles (120km) wide. For comparison, the largest volcano on Earth is Mauna Loa. From its base on the sea floor, Mauna Loa measures only 6.3 miles high and 75 miles in diameter.

Orbit Number: 94404 Latitude: -8.85515 Longitude: 242.188 Instrument: VIS Captured: 2023-03-27 12:39

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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