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dc.contributor.authorAnderson, R. B.
dc.contributor.authorLong, S. P.
dc.contributor.authorHorton, B. K.
dc.contributor.authorThomson, S. N.
dc.contributor.authorCalle, A. Z.
dc.contributor.authorStockli, D. F.
dc.date.accessioned2019-05-13T17:03:59Z
dc.date.available2019-05-13T17:03:59Z
dc.date.issued2018-10
dc.identifier.citationAnderson, R. B., Long, S. P., Horton, B. K., Thomson, S. N., Calle, A. Z., & Stockli, D. F. ( 2018). Orogenic wedge evolution of the central Andes, Bolivia (21°S): Implications for Cordilleran cyclicity. Tectonics, 37, 3577– 3609. https://doi.org/10.1029/2018TC005132en_US
dc.identifier.issn02787407
dc.identifier.doi10.1029/2018TC005132
dc.identifier.urihttp://hdl.handle.net/10150/632235
dc.description.abstractThe Andes are an ideal setting to explore orogenic wedge evolution and the cyclical tectonic processes in Cordilleran convergent-margin systems. Paleoaltimetry data suggest that the hinterland plateau in southern Bolivia underwent rapid surface uplift at similar to 16-9 Ma, which is predicted to have induced rapid thrust belt propagation. We integrate fission track and (U-Th)/He ages from zircon and apatite with a sequentially restored cross section to quantify the timing and rates of thrust belt propagation in southern Bolivia for the last similar to 43 Myr. These data show that retroarc shortening in the Eastern Cordillera propagated westward from similar to 43 to 27 Ma as the wedge grew to attain critical taper and steady state. The thrust front then advanced rapidly eastward from similar to 25 to 17 Ma across the western Interandean zone, where a weak decollement modified the critical taper angle. The thrust front stalled for similar to 6 Myr but resumed eastward advance into the eastern Interandean zone and Subandean zone by similar to 11-8 Ma, which we interpret as a response to increased accretionary influx and rapid orogenic wedge expansion induced by eclogitic delamination and corresponding hinterland surface uplift at similar to 13 Ma. Development of an orographic barrier and wetter climatic conditions resulted in relatively steady state wedge conditions from similar to 8.5 to 1.5 Ma. Rapid wedge growth after similar to 1.5 Ma may be attributed to mass accumulation in the orogen interior or a weakened decollement. Our data reveal space-time variations in orogenic wedge evolution consistent with models of Cordilleran cyclicity and lithospheric removal, with important additional influences of erosion, climate, and rock rheology.en_US
dc.description.sponsorshipNational Science Foundation [EAR-1250510]; Repsol Bolivia S.A.en_US
dc.language.isoenen_US
dc.publisherAMER GEOPHYSICAL UNIONen_US
dc.relation.urlhttp://doi.wiley.com/10.1029/2018TC005132en_US
dc.rights© 2018. American Geophysical Union. All Rights Reserved.en_US
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.titleOrogenic Wedge Evolution of the Central Andes, Bolivia (21°S): Implications for Cordilleran Cyclicityen_US
dc.typeArticleen_US
dc.contributor.departmentUniv Arizona, Dept Geoscien_US
dc.identifier.journalTECTONICSen_US
dc.description.note6 month embargo; published online: 28 August 2018en_US
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en_US
dc.eprint.versionFinal published versionen_US
dc.source.journaltitleTectonics
dc.source.volume37
dc.source.issue10
dc.source.beginpage3577
dc.source.endpage3609
refterms.dateFOA2019-02-28T00:00:00Z


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