Tharsis 3d

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Mosaic/ topography image with 10:1 vertical exaggeration, showing the massive side lobes on the southwest (top) and northeast (bottom) sides of the volcanoCoordinates:Peak20 km/ 63,360 ftEponymLatin – Arsia Silva – classical albedo feature nameArsia Mons is the southernmost of three (collectively known as ) on the bulge near the of the. To its north is, and north of that is. The tallest volcano in the, is to its northwest. Its name comes from a corresponding on a map by, which he named in turn after the legendary Roman forest of. Topographic map of Arsia MonsThe volcano is 435 kilometres (270 mi) in diameter, almost 20 kilometres (12 mi) high (more than 9 kilometers (5.6 mi) higher than the surrounding plains ), and the summit is 110 km (72 miles) wide. It experiences lower than 107 at the summit.

Excluding Olympus Mons, it is the largest known volcano in terms of volume. Arsia Mons has 30 times the volume of in, the largest volcano on the Earth.The caldera of Arsia Mons was formed when the mountain collapsed in on itself after its reservoir of was exhausted. There are many other geologic collapse features on the mountain's flanks. The caldera floor formed around 150 Mya ago.The shield is transected roughly northeast to southwest by a set of collapse features. The collapse features on the shield are connected by a line of small shield volcanoes on the floor of the caldera.

It is possible that this line represents a significant fault similar to others found on the Tharsis bulge. This fault may represent the source of the Arsia lavas.The rift area to the southwest has been imaged in significant detail by the European Space Agency probe. In 2004, a 3D map of this region was created at high resolution. Cliffs, landslides, and numerous collapse features can be seen. Combined with the extensive lava flows at the termination of the rift, this may reveal areas that drained the caldera lavas and contributed to the collapse.The northwest flank of the volcano is significantly different and rougher than the southeast flank, and the features may represent evidence of glaciers. Possible plate tectonics.

Carr`, Michael (2006). Cambridge, UK:. March 11, 2007, at the NASA MGS data 9.2 degrees S 238.2 degrees E 17757 meters 1.07 mbar. Carr`, Michael (2006). Cambridge, UK: Cambridge University Press. Carr`, Michael (2006). Cambridge, UK: Cambridge University Press.

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A.; Wilson, J. A.; Connor, C. B.; Bleacher, J. E.; Kiyosugi, K. 'Recurrence rate and magma effusion rate for the latest volcanism on Arsia Mons, Mars'. Earth and Planetary Science Letters.

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8 (1). ESA, October 2018. Kerber, L.; et al. 'The disporsal of pyroclasts from ancient explosive volcanoes on Mars: Implications for the friable layered deposits'. 219: 358–381. Shean, David E.; Head III, James W.; Fastook, James L.; Marchant, David R. (21 March 2007).

Journal of Geophysical Research. 112 (E03004): 1–23.:. Retrieved 1 April 2012. Scanlon,K., J. REMNANT BURIED ICE IN THE ARSIA MONS FAN-SHAPED DEPOSIT, MARS. 46th Lunar and Planetary Science Conference.

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