3.9 Article

Geochronological and geochemical constraints on the petrogenesis of high-K granite from the Suffi abad area, Sanandaj-Sirjan Zone, NW Iran

Journal

CHEMIE DER ERDE-GEOCHEMISTRY
Volume 71, Issue 4, Pages 363-376

Publisher

ELSEVIER GMBH
DOI: 10.1016/j.chemer.2011.06.005

Keywords

Sanadaj-Sirjan Zone; High-K granite; I-type granite; Sr-Nd isotopes; U-Pb zircon age

Funding

  1. University of Kurdistan (UOK) at Nagoya University, Japan

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The Sanandaj-Sirjan Zone (SSZ) trends northwestward in western Iran on the Precambrian to Paleozoic basement and exposes abundant l-type granitoids and calc-alkaline volcanic rocks that were most active during the Late Jurassic to Upper Cretaceous. The petrogenesis of the granitoids and associated volcanic rocks has been widely related to Neotethyan subduction beneath the Iranian plate. We report a geochronological and geochemical study of the Suffi abad granite (SLG) body that crops outs southeast of Sanandaj within the SSZ and is mainly composed of K-feldspar + quartz + plagioclase +/- hornblende. The SLG, which shows a high-K calc-alkaline affinity, has LA-ICPMS zircon U-Pb ages ranging between 149 +/- 2 and 144 +/- 3 Ma and initial Sr-87/Sr-86 of similar to 0.7024-0.7069 and Nd-143/Nd-144 of similar to 0.5125-0.5127. These value correspond to an epsilon(Nd) (145 Ma) of +1.5 and +4.9, suggesting that the SLG originated from the juvenile crust or depleted mantle with a young T-DM (650-900 Ma) over the subduction zone beneath the SSZ. Zircon saturation temperatures suggest that crystallization of the zircons, or emplacement of the host magmas, occurred at 560-750 degrees C, consistent with an intergrowth texture of K-feldspar and quartz that implies crystallization around the K-feldspar-quartz eutectic at lower temperatures. Overall, geochemical data suggest that crystallization of the hornblende and plagioclase played a role in magma differentiation. These data allow us to conclude that the high-K SLG did not originate directly from the juvenile mantle source as do most l-type, calc-alkaline granitoids, but more likely was produced from the partial melting of pre-existing I-type granitoids in the upper continental crust under low pressure conditions. Published by Elsevier GmbH.

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