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Early cretaceous granitoids and their implications for the collapse of the Dabie orogen, eastern China: SHRIMP zircon U-Pb dating and geochemistry

机译:早期白垩纪花岗岩类及其对中国东部大别造山带垮塌的影响:SHRIMP锆石U-Pb测年和地球化学

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Two stages of early Cretaceous post-orogenic granitoids are recognized in the Dabie orogen, eastern China, which recorded processes of extensional collapse of the orogen. The early stage granitoids (similar to 132 Ma) are foliated hornblende quartz monzonites and porphyritic monzogranites. They are of high-K calc-alkaline series and metaluminous to weakly peraluminous, with high KO and low MgO contents (Mg-# values: 32.0-46.0), they contain high Sr, low Y and heavy rare earth elements (HREE), and have high Sr/Y and (La/Yb)(N) ratios, without clear negative Eu, Sr and Ti anomalies. The early stage deformed granitoids have adakitic geochemical compositions and are equilibrated with residues rich in garnet and poor in anorthite-rich plagioclase, and thus indicate the existence of an over-thickened (>50 km) crustal root beneath the orogen at similar to 132 Ma. The later stage granitoids (similar to 128 Ma) are undeformed fine-grained monzogranites, fine-grained K-feldspar granites and coarse-grained K-feldspar granite-porphyry. They belong to a peraluminous and high-K calc-alkaline to shoshonite series, and display a flat HREE pattern and have strong negative Eu, Sr and Ti anomalies, with low Sr/Y and (La/Yb)N ratios. The late stage granitoids are equilibrated with residues rich in anorthite-rich plagioclase, hornblende, ilmenite/titanite and poor in garnet, indicating that the crust of the Dabie orogen became thinner (<35 km) at similar to 128 Ma. SHRIMP zircon U-Pb ages and changing compositional trends for these two stages of granitoids indicate that the over-thickened crust formed by the Triassic continental subduction/collision under the Dabie orogen remained until the early Cretaceous, and collapsed quickly in a few million years during the early Cretaceous. (C) 2007 Elsevier B.V. All rights reserved.
机译:在中国东部的大别造山带中,早白垩世造山后花岗岩有两个阶段,记录了造山带的伸展塌陷过程。早期花岗岩(类似于132 Ma)是叶状角闪石石英辉石和斑状辉石辉石。它们是高K钙碱性系列,金属含量至弱高铝含量,具有高KO和低MgO含量(Mg-#值:32.0-46.0),它们含有高Sr,低Y和重稀土元素(HREE),并且具有很高的Sr / Y和(La / Yb)(N)比,并且没有明显的负Eu,Sr和Ti异常。早期变形的类花岗岩具有adakitic地球化学成分,并与富含石榴石和贫富钙长石斜长石的残渣平衡,因此表明造山带下方存在一个超厚(> 50 km)的地壳根,类似于132 Ma 。后期花岗岩(近似于128 Ma)是未变形的细粒辉长花岗岩,细粒的钾长石花岗岩和粗粒的钾长石花岗岩斑岩。它们属于高铝钙钙盐-钾长石钙铁矿系列,显示出扁平的HREE模式,具有强的Eu,Sr和Ti负异常,Sr / Y和(La / Yb)N比率低。晚期花岗岩类物质富含富钙长石斜长石,角闪石,钛铁矿/钛铁矿和石榴石含量低的残留物,表明大别造山带的地壳在约128 Ma处变薄(<35 km)。这两个阶段花岗岩的SHRIMP锆石U-Pb年龄和不断变化的组成趋势表明,由大别造山带下的三叠纪大陆俯冲/碰撞形成的超厚地壳一直保留到白垩纪早期,并在此期间的几百万年中迅速崩塌。白垩纪早期。 (C)2007 Elsevier B.V.保留所有权利。

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