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Chronological and geochemical studies of granite and enclave in Baimashan pluton, Hunan, South China

机译:中国湖南白马山岩体花岗岩和飞地的年代地球化学研究

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摘要

Zircon LA-ICP-MS U-Pb dating reveals that the Baimashan Pluton is composed mainly of late Indosinian (204.5±2.8 Ma—209.2±3.8 Ma) biotite granodiorites/monzonitic granites (LIGs) and early Yanshanian (176.7±1.7 Ma) two-micas monzonitic granites (EYGs), and the coeval (203.2±4.5 Ma—205.1 ±3.9 Ma) mafic microgranular enclaves (MMEs) are generally found in the former. In addition, the ages of cores within zircons from LIGs and MMEs ranging from 221.4±4.0 Ma to 226.5±4.1Ma provide evidence of multistage magma intrusion during Indosinian in the study area. Measured 3010±20.6 Ma of inherited zircon age suggests that there may be recycling Archaean curstal material in existence in this area. LIGs and EYGs share some similar geochemical features: subalkaline and peraluminous granites, enrichment of Th, U, K, Ta, Zr, Hf and LREE but depletion of Ba, Nb, P, Ti and Eu, low ε_(Nd)(t) values but high ((~(87)Sr/~(86)Sr))_i; ratios, and old T_(2DM)(ca. 1.9—2.0 Ga). The behaviors of incompatible elements and REE are mainly dominated by fractional crystallization of plagioclase, K-feldspar, ilmenite and apatite, but that of Sr isotope mainly controlled by EC-AFC. They are crust-sourced and derived from partial melting of paleo-Proterozoic metagreywackes and related to biotite dehydration melting. LIGs are formed in post-collisional tectonic setting as crustal local extension and thinning during late Indosinian. But EYGs may be evolved products of congeneric granitic magma with LIGs formed in late Indoinian, which were emplaced again when crust underwent extensive thinning and extension in post-orogenic tectonic setting during Yanshanian in SC after undergoing EC-AFC. MMEs should be cognate enclaves and derived from liquid immiscibility of host magma.
机译:锆石LA-ICP-MS U-Pb测年表明白马山岩体主要由印度支那晚期(204.5±2.8 Ma—209.2±3.8 Ma)黑云母花岗闪长岩/单长花岗岩(LIGs)和燕山初期(176.7±1.7 Ma)组成。前者中普遍发现有-micas的单带花岗岩(EYGs)和同时代的(203.2±4.5 Ma–205.1±3.9 Ma)基性微细粒状飞地。此外,来自LIGs和MMEs的锆石核心的年龄范围从221.4±4.0 Ma到226.5±4.1Ma,提供了研究区域印度支那时期多阶段岩浆侵入的证据。测得的继承锆石年龄为3010±20.6 Ma,表明该地区可能存在回收的古生阿尔卡迪亚地壳物质。 LIGs和EYGs具有一些相似的地球化学特征:碱性和高铝质花岗岩,Th,U,K,Ta,Zr,Hf和LREE的富集,但是Ba,Nb,P,Ti和Eu的损耗,低ε_(Nd)(t)值高((〜(87)Sr /〜(86)Sr))_ i;比率和旧的T_(2DM)(约1.9-2.0 Ga)。不相容元素和稀土元素的行为主要由斜长石,钾长石,钛铁矿和磷灰石的分级结晶决定,而锶同位素的结晶主要受EC-AFC控制。它们是地壳来源的,并且来自古元古代的变质灰泥的部分熔融,并且与黑云母脱水熔融有关。 LIGs在碰撞后的构造环境中形成,是在印度支那晚期的地壳局部扩展和变薄。但EYGs可能是同质花岗岩岩浆的演化产物,形成于印度支那晚期,LIGs在燕山期南海造山带在经历EC-AFC后,在造山后构造环境中经历了广泛的变薄和伸展时,再次发生了沉积。 MME应为同源飞地,并应来自宿主岩浆的液体不溶混性。

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