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Geology; October 2003; v. 31; no. 10; p. 849-852; DOI: 10.1130/G19707.1
© 2003 Geological Society of America
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Building the Pamirs: The view from the underside

Mihai N. Ducea*,1, Valery Lutkov*,2, Vladislav T. Minaev*,2, Bradley Hacker*,3, Lothar Ratschbacher*,4, Peter Luffi*,5, Martina Schwab*,6, George E. Gehrels*,7, Michael McWilliams*,8, Jeffrey Vervoort*,9 and James Metcalf*,10

1 Department of Geosciences, University of Arizona, Tucson, Arizona 85721, USA
2 Geological Institute of the Tajik Academy of Science, 734063, Dushanbe, Tajikistan
3 Department of Geological Sciences, University of California, Santa Barbara, California 93106-9630, USA
4 Institut für Geowissenschaften, Technische Universität Bergakademie Freiberg, 09599 Freiberg, Germany
5 Department of Geology and Geophysics, University of Bucharest, Bucharest 70139, Romania
6 Institut für Geowissenschaften, Universität Tübingen, 72076 Tübingen, Germany
7 Department of Geosciences, University of Arizona, Tucson, Arizona 85721, USA
8 Department of Geological and Environmental Sciences, Stanford University, Stanford, California 94305-2115, USA
9 Department of Geology, Washington State University, Pullman, Washington 99164, USA
10 Department of Geological and Environmental Sciences, Stanford University, Stanford, California 94305-2115, USA

The Pamir mountains are an outstanding example of extreme crustal shortening during continental collision that may have been accommodated by formation of a thick crust—much thicker than is currently thought—and/or by continental subduction. We present new petrologic data and radiometric ages from xenoliths in Miocene volcanic rocks in the southeastern Pamir mountains that suggest that Gondwanan igneous and sedimentary assemblages were underthrust northward, buried to >50–80 km during the early stage of the India-Asia collision, and then heated and partly melted during subsequent thermal relaxation before finally being blasted to the surface. These xenoliths, the deepest crustal samples recovered from under any active collisional belt, provide direct evidence for early Cenozoic thickening of the Pamirs and lower-crustal melting during collision; the xenoliths also suggest that the present mountain range was a steady-state elevated plateau for most of the Cenozoic.

Key Words: Pamir region • continental collision • subduction • partial melting • orogenic plateaus




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