Tharsis Montes
| Tharsis Montes | |
|---|---|
 Three volcanoes comprise the Tharsis Montes. They include Arsia Mons (in the south), Pavonis Mons (at center) and Ascraeus Mons (in the north). |
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| Location | Tharsis Region |
| Coordinates | 1°12′N 112°30′W / 1.2°N 112.5°WCoordinates: 1°12′N 112°30′W / 1.2°N 112.5°W |
| Peak | Ascraeus Mons (18.2 km) |
| Discoverer | Mariner 9 |
The Tharsis Montes are three large shield volcanoes in the Tharsis region of the planet Mars. From north to south, the volcanoes are Ascraeus Mons, Pavonis Mons and Arsia Mons. Mons (plural montes) is the Latin word for mountain. It is a descriptor term used in astrogeology for mountainous features in the Solar System.
The three Tharsis Montes volcanoes are enormous by terrestrial standards, ranging in diameter from 375 km (Pavonis Mons) to 475 km (Arsia Mons).[1] Ascraeus Mons is the tallest with a summit elevation of over 18 km,[2] or 15 km base-to-peak. For comparison, the largest volcano on Earth, Mauna Loa in Hawaii, is about 120 km across and stands 9 km above the ocean floor.[3]
The Tharsis Montes volcanoes lie near the equator, along the crest of a vast volcanic plateau called the Tharsis region or Tharsis buldge. The Tharsis region is thousands of kilometers across and averages nearly 10 km above the mean elevation of the planet. Olympus Mons, the tallest known mountain in the Solar System, is located about 1,200 km northwest of the Tharsis Montes, at the edge of the Tharsis region.
The Tharsis Montes were discovered by the Mariner 9 spacecraft in 1971. They were among the few surface features visible as the spacecraft entered orbit during a global dust storm. Appearing as faint spots through the dusty haze, they were informally christened North Spot, Middle Spot, and South Spot. (A fourth spot corresponding to the albedo feature Nix Olympica was also visible and later named Olympus Mons.) As the dust cleared, it became obvious that the spots were the tops of enormous shield volcanoes with complex central calderas (collapse craters).[4][5]
The three Tharsis Montes volcanoes are evenly spaced about 700 km apart (from peak to peak) in a line oriented southwest-northeast.[6] This alignment is unlikely to be coincidental. Several volcanic centers northeast of the Tharsis Montes also form part of the line. The line clearly represents a major structural feature of the planet, but its origin is uncertain.[7]
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Arsia Mons, southernmost peak of Tharsis Montes. Image Credit: NASA/JPL/Arizona State University
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Pavonis Mons, the central peak of Tharsis Montes. Image Credit: NASA/JPL/Malin Space Science Systems
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The caldera of Ascraeus Mons, northernmost peak of Tharsis Montes. Image Credit: NASA/JPL/Malin Space Science Systems
[edit] References
- ^ USGS Gazetteer of Planetary Nomenclature. http://planetarynames.wr.usgs.gov/.
- ^ Plescia, J.B. (2004). Morphometric Properties of Martian Volcanoes. J. Geophys. Res. 109(E03003), Table 1.
- ^ Carr, M.H. (2006). The Surface of Mars; Cambridge University Press: Cambridge, UK, p. 46.
- ^ Masursky, H. (1973). An Overview of Geological Results from Mariner 9. J. Geophys. Res., 78(20), 4009–4030.
- ^ Carr, M.H. (1973). Volcanism on Mars. J. Geophys. Res. 78(20), p. 4049-4062.
- ^ Cattermole, P.J. (2001) Mars: the Mystery Unfolds; Oxford University Press: New York, p. 72.
- ^ Carr, M.H. (2006). The Surface of Mars; Cambridge University Press: New York, p. 70.
[edit] External links
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