File:Pavonis Mons (PIA25768).tiff

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This VIS image shows a cross section of the upper elevations of Pavonis Mons, including part of the summit caldera (circular region near the center of the image). Pavonis Mons is the central volcano of the three large Tharsis volcanoes.

Summary[edit]

Description
English:


Context image

This VIS image shows a cross section of the upper elevations of Pavonis Mons, including part of the summit caldera (circular region near the center of the image). Pavonis Mons is the central volcano of the three large Tharsis volcanoes. In order from north to south the volcanoes are Ascreaus Mons, Pavonis Mons and Arsia Mons. All three volcanoes form a line located along a tectonic bulge caused by extensional forces in the region. Along this trend there are increased tectonic features and additional lava flows that arose from the flanks of the volcanoes rather than just the summit. Like the other large volcanoes in the region, Pavonis Mons is a shield volcano. Shield volcanoes are formed by lava flows originating near or at the summit, building up layers upon layers of lava. In shield volcanoes summit calderas are typically formed where the surface collapses into the void formed by an emptied magma chamber. Pavonis Mons is the smallest of the three volcanoes with a summit of only 14km (8.7 miles) and a width of 375 km (233 miles). Like most shield volcanoes the surface has a low profile. In the case of Pavonis Mons the average slope is only 4 degrees. Pavonis means peacock in Latin, making it's name peacock mountain.

Orbit Number: 92650 Latitude: 0.705474 Longitude: 247.87 Instrument: VIS Captured: 2022-11-03 03:34

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.

Date (published)
Source Catalog page · Full-res (JPEG · TIFF) · Full-res ([ MP4]) · Full-res ([ GIF])
Author NASA/JPL-Caltech/ASU
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This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA25768.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
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This media is a product of the
2001 Mars Odyssey mission
Credit and attribution belongs to the Thermal Emission Imaging System (THEMIS) team, NASA/JPL-Caltech/ASU

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Courtesy NASA/JPL-Caltech

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current13:46, 8 August 2023Thumbnail for version as of 13:46, 8 August 2023603 × 2,700 (750 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://photojournal.jpl.nasa.gov/tiff/PIA25768.tif via Commons:Spacemedia

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