Definition
Domical-shaped central vent shield volcano.
Category
A type of shield volcano
Synonyms
Plural
Tholi
Description
Tholi on Mars are central vent volcanoes with well-defined summit calderas (BVSP 1981) of up to 10 km in diameter and basal dimensions between 50 and 200 km and a height of 4–10 km (Plescia 2004). They have relatively steep peripheral flanks. Most are asymmetric with a multi-stage caldera, which appear large compared to the edifice itself. Their flanks are often buried under surrounding plains of lava flows, so that their full dimensions are indeterminable (Werner 2009). In structure they resemble shield volcanoes; some, such as Ceraunius Tholus, have numerous radial channel, and others show flow features (BVSP 1981). Most have concentric grabens similar to the large shield volcanoes (BVSP 1981). The distribution named tholi on Mars is shown in Fig. 1.
References
Basaltic Volcanism Study Project, Kaula WM, Head JW III, Merrill RB, Pepin RO, Solomon SC, Walker D, Wood CA (eds) (1981) Basaltic volcanism on the terrestrial planets. Pergamon Press, Oxford/New York/Frankfurt/Paris/Sydney/Tokyo/Toronto
Mouginis-Mark PJ, Wilson L, Zuber MT (1992) The physical volcanology of Mars. In: Kieffer HH, Jakosky BM, Snyder CW, Matthews MS (eds) Mars. Arizona Press, Tucson
Plescia JB (2004) Morphometric properties of Martian volcanoes. J Geophys Res 109:3003
Robbins S, Achille GD, Hynek BM (2011) The volcanic history of Mars: high-resolution crater-based studies of the calderas of 20 volcanoes. Icarus 211:1179–1203
Tanaka KL, Scott DH, Greeley R, Guest JE (1986) Geological map of the polar, western and eastern equatorial regions of Mars (1:15,000,000). USGS: US Geological Survey. USGS Numbered Series M(200) I no.1802–A, B, C
Werner SC (2009) The global Martian volcanic evolutionary history. Icarus 201:44–68
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Werner, S.C. (2014). Tholus (Mars). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_372-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_372-1
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