Dynamic Processes in Extensional and Compressional Settings - Mountain Building: From Earthquakes to Geological Deformation
- Creators
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Avouac, J.-P.
- Other:
- Schubert, Gerald
Abstract
Mountain ranges are the most spectacular manifestation of continental dynamics. T he fact that some mountain ranges were able to maintain their topography over tens of millions of years, while their erosion was feeding large sedimentary basins, is unambiguous evidence that tectonic forces can cause sustained uplift of subsidence of the continental crust. Geologists noticed quite early on that most mountain ranges are contractional orogens, the result of horizontal contraction of the continental crust, and that they tend to form long belts separating domains with often quite different geological history (e.g., Willis, 1891; Argand, 1924). A rapid tour of active mountain ranges on Earth today shows that contractional mountain ranges can arise in a variety of contexts. Some have formed along converging plate boundaries as the result of collisions which can involve two continents (along the Himalaya, for example, as detailed in this review), a continent and an island arc (in Taiwan) (e.g., Malavieille et al., 2002a), or a continent and an oceanic plateau (in the Southern Alps of New Zealand) (e.g., Walcott, 1998). Contractional mountain ranges can also form along subduction zones without being necessarily collisional features. In the Andes for example, the stresses transmitted across a subduction zone appear to be sufficient to cause trench-perpendicular shortening (e.g., (Lamb, 2006), probably because high heat flow in the back-arc zone weakens the continental lithosphere (Hyndman et al., 2005). Mountain ranges are thus often closely associated with converging plate boundaries. However, active mountain building can also occur far away) from plate boundaries, the Tien Shan, in Central Asia, being an outstanding example (e.g., Hendrix et al., 1992 and Avouac, et al., 1993).
Additional Information
© 2007 Elsevier B.V.Additional details
- Eprint ID
- 21705
- Resolver ID
- CaltechAUTHORS:20110111-120419364
- Created
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2011-01-25Created from EPrint's datestamp field
- Updated
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2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Caltech Tectonics Observatory, Caltech Tectonics Observatory. Indo-Asian Collision Zone, Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)