THE KOSHRABAD GRANITE MASSIF IN UZBEKISTAN: PETROGENESIS, METALLOGENY, AND GEODYNAMIC SETTING
D.L. Konopel'koa, Yu.S. Biskea, K. Kullerudb, R. Seltmannc, and F.K. Divaevd
aSt. Petersburg State University, Universitetskaya nab. 7/9, St. Petersburg, 199034, Russia
bDepartment of Geology, University of Tromso, N-9037 Tromso, Norway
cCERCAMS, Department of Mineralogy, NHM, Cromwell Road, London SW7 5BD, UK
dSE "Tsentral'naya Geological and Geophysical Expedition" of the Uzbekistan State Geology Committee, ul. Gagarina 148, Samarkand, 103030, Uzbekistan
Keywords: Geochemistry, tectonics, metallogeny, Koshrabad massif, Tien Shan
Pages: 1563-1573
Abstract
The Koshrabad massif, referred to as the Hercynian postcollisional intrusions of the Tien Shan, is composed of two rock series: (1) mafic and quartz monzonites and (2) granites of the main phase. Porphyritic granitoids of the main phase contain ovoids of alkali feldspar, often rimmed with plagioclase. Mafic rocks developed locally in the massif core resulted from the injections of mafic magma into the still unconsolidated rocks of the main phase, which produced hybrid rocks and various dike series. All rocks of the massif are characterized by high f (Fe/(Fe + Mg)) values and contain fayalite, which points to the reducing conditions of their formation. Mafic rocks are the product of fractional crystallization of alkali-basaltic mantle melt, and granitoids of the main phase show signs of crustal-substance contamination. In high f values and HFSE contents the massif rocks are similar to A -type granites. Data on the geochemical evolution of the massif rocks confirm the genetic relationship of the massif gold deposits with magmatic processes and suggest the accumulation of gold in residual acid melts and the rapid formation of ore quartz veins in the same structures that controlled the intrusion of late dikes. The simultaneous intrusion of compositionally different postcollisional granitoids of the North Nuratau Ridge, including the Koshrabad granitoids, is due to the synchronous melting of different crustal protoliths in the zone of transcrustal shear, which was caused by the ascent of the hot asthenospheric matter in the dilatation setting. The resulting circulation of fluids led to the mobilization of ore elements from the crustal rocks and their accumulation in commercial concentrations.
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