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dc.contributor.advisorKip V. Hodges and Leigh H. Royden.en_US
dc.contributor.authorHuerta Audrey Dean, 1960-en_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.en_US
dc.date.accessioned2010-04-28T15:33:04Z
dc.date.available2010-04-28T15:33:04Z
dc.date.copyright1999en_US
dc.date.issued1999en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/54441
dc.descriptionThesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, February 1999.en_US
dc.descriptionIncludes bibliographical references.en_US
dc.description.abstractSimple thermal models of collisional orogenesis generally predict metamorphic temperatures that are much cooler than those revealed by thermo barometric studies of real metamorphic terrains. This thesis focuses on a more realistic model that accounts for the redistribution of crust enriched in heat-producing elements by accretion and erosion. In collisional settings, these processes lead to the development and growth of a wedge of heat producing crust within the overriding plate. Maximum temperatures in an orogenic setting occur within this wedge, and inverted thermal gradients occur beneath the zone of maximum temperatures, a characteristic not displayed by simple models that ignore the combined effects of accretion and erosion. Synthetic metamorphic field gradients generated by tracking the pressure temperature history of rocks advected through a model orogen are generally similar to those observed in the field. Specific aspects of these metamorphic patterns can be related to the relative rates of accretion, erosion, and plate convergence. In particular, peak metamorphic temperatures within the core of an orogen are related to ratios of accretion rate to convergence velocity; and the distance from the toe of an orogen to the metamorphic core is controlled by the ratio of erosion rate to accretion rate. In addition, results of this model challenge two prevailing paradigms in metamorphic petrology: 1) that the metamorphic record does not closely reflect the geothermal gradients within an orogen; and 2) that metamorphic pressure-temperature paths characterized by isothermal decompression require rapid un roofing. Under special (but nonetheless realistic) conditions, metamorphic field gradients closely mimic actual geotherms. The model predicts that pressure-temperature paths for rocks from the metamorphic cores of mountain ranges will display a component of isothermal decompression, even at low exhumation rates. The sensitivity of the metamorphic history of a synthetic collisional orogen to the rate and geometry of accretionary and erosional processes implies that it should be possible to use the metamorphic record of a real orogen to extract information about rates of deformation and denudation. Tests of this hypothesis with data from the Himalayan orogen confirm that most critical parameters can be constrained to within about 30%.en_US
dc.description.statementofresponsibilityby Audrey Dean Huerta.en_US
dc.format.extent140 p.en_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectEarth, Atmospheric, and Planetary Sciences.en_US
dc.titleThe thermal and metamorphic evolution of mountain belts as a response to erosion, accretion, and radiogenic heatingen_US
dc.typeThesisen_US
dc.description.degreePh.D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.oclc48172569en_US


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