寻找脉冲:加尔瓦尔-喜马拉雅地区的熔体形成和时间

Charlie Oldman, C. Warren, C. Spencer, T. Argles, N. Harris, S. Hammond
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引用次数: 0

摘要

进阶变质作用对造山演化最重要的影响是高变质岩的熔融作用,导致其机械强度急剧下降,剪切带的激活和随后的掘出。花岗岩体位于喜马拉雅造山带最高变质等级内,是由角闪岩级泥质岩石熔融形成的,或者是由于含水流体的存在,或者是由于白云母等含水相的脱水。这些花岗岩和部分熔融的源混辉岩分布在大喜马拉雅层序(GHS)中,以中央逆冲构造(MCT)和藏南分离构造(STD)为界。其中许多花岗岩形成于中新世,在快速挖掘过程中,该单元的减压引发了融化;然而,确切的时间和反应途径似乎在造山带的横向上有所不同。深融、合并、迁移和侵位的时间尺度是目前研究的热点,对造山带构造发育具有重要意义。最近对花岗岩岩体形成的研究表明,在低熔体分数条件下,一系列脉冲熔融事件具有长时间的结晶。这些研究表明,年龄的粒度变化可以与独居石和锆石中的微量元素数据联系起来,这些数据跨越了数百万年的结晶。因此,重要的是要认识到这些过程在花岗岩、混杂岩和熔融提取的矿石中留下的地球化学特征,并更准确地描绘导致岩浆成因的相关过程和时间尺度。我们提出了一个初步的数据集,旨在限制形成GHS上部混辉岩和浅花岗岩的熔融事件的来源、熔融反应和时间尺度。我们在印度喜马拉雅的加尔瓦尔地区沿Rishi Ganga (Badrinath)和Alaknanda山谷取样了浅花岗岩、杂岩及其寄主变质沉积岩。利用LA-ICPMS分析了这些样品中的锆石的结晶年龄(U-Pb)、hf同位素比、氧同位素和微量元素组成。利用阴极发光(CL)成像确定的边缘域是优先目标,目的是收集与喜马拉雅融化过程相关的数据。初步结果表明,浅花岗岩的结晶时间为22 ~13 Ma,锆石的结晶在这段时间内发生了间断。混合岩的锆石边缘年龄普遍较老,在34 ~15 Ma之间。hf同位素和微量元素数据与岩石学观测相结合,可以将矿物年龄数据与地质过程的变化联系起来。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Finding a Pulse: Melt Formation and Timing in the Garhwal Himalaya

The most significant consequence of prograde metamorphism for orogenic evolution is the melting of high-grade metamorphic rocks, resulting in a dramatic decrease in their mechanical strength, the activation of shear zones and consequent exhumation. Granitic bodies emplaced within the highest metamorphic grades of the Himalayan orogen form by the melting of amphibolite-grade pelitic rocks, either due to the presence of aqueous fluid or through the dehydration of hydrous phases such as muscovite. Across the Himalayas, these granites, and partially melted source migmatites, are found in the Greater Himalayan Sequence (GHS), bounded by the Main Central Thrust (MCT) and the South Tibetan Detachment (STD). Many of these granites formed during the Miocene when decompression of the unit during rapid exhumation triggered melting; however, exact timings and reaction pathways appear to vary laterally across the orogen. The timescales of anatexis, amalgamation, migration, and emplacement are the focus of active research and have implications for orogenic tectonic development. Recent studies of granite pluton formation suggest a series of pulsed melting events with protracted periods of crystallisation under low melt-fraction conditions. These studies show that grain-scale variations in age can be linked with trace element data in both monazite and zircon, spanning millions of years of crystallisation. It is, therefore, important to recognise the geochemical signatures that these processes leave in granites, migmatites, and melt-extracted restite and to delineate more precisely the relevant processes and timescales leading to magma genesis. We present a preliminary dataset that aims to constrain the source, melt reactions, and timescales of melting episodes that form the migmatites and leucogranites of the upper GHS. We sampled leucogranites, migmatites, and their host metasediments along the Rishi Ganga (Badrinath) and Alaknanda valleys in the Garhwal region of the Indian Himalaya. Zircon from these samples were analysed for their crystallisation age (U-Pb), Hf-isotopic ratios, oxygen isotope and trace element composition using LA-ICPMS.  Rim domains identified using cathodoluminescence (CL) imaging were preferentially targeted, with the aim of collecting data that related to Himalayan melting processes. Preliminary findings suggest that the leucogranites crystallised from 22 Ma to ~13 Ma, with punctuated zircon crystallisation occurring throughout this timespan. Zircon rim ages from migmatites are generally older, ranging from 34 Ma to ~15 Ma. Integration of Hf-isotopic and trace elemental data, combined with petrographic observations allow mineral age data to be linked to changes in geological processes.

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