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Natural and experimental constraints on formation of the continental crust based on niobium-tantalum fractionation

机译:基于铌-钽分离的大陆壳形成的自然和实验约束

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摘要

Fractionation between Nb and Ta, elements generally regarded as geochemical 'identical twins', is a key to deciphering the formation of the continental crust (CC). Here we show that Nb/Ta of rutile grains in eclogitic rocks from the Chinese Continental Scientific Drilling (CCSD) project are remarkably heterogeneous but overall subchondritic at core depths of 100-700 m, and are less variable and mainly suprachondritic at core depths of 700-3025 m, indicating clear Nb/Ta fractionation across a subducted slab. To understand the potential mechanism of Nb/Ta fractionation within the subducted plate, we analysed by laser ablation ICPMS a thermal migration experiment in which a wet andesite was placed in a large thermal gradient (300 deg C/cm with ends ranging from 950-350 deg C) at 0.5Gpa. Results show that Nb, Ta and Ti, driven by the thermal gradient, preferentially migrate by diffusion through supercritical fluids into the cooler end of the experiment (at approx 650-350 deg C). Due to contrasting Nb and Ta thermal migration patterns, dramatic fractionation between Nb, Ta, and Ti took place in the cooler end. Experimental results are consistent with the measured Nb, Ta in rutile from CCSD drillhole samples. We consider that major fractionation between Nb, Ta must occur before rutile appears, most likely during the prograde blueschist to amphibole-eclogite transformation, when Ti is also mobile. Before rutile appears, partitioning between Ti-rich dominant minerals such as amphiboles and fluids in the hotter region where dehydration preferentially occurs, produces Nb-Ta-Ti-rich fluids with subchondritic Nb/Ta, and dehydration residues with suprachondritic Nb/Ta. Meanwhile, owing to evolution of the thermal gradient within the subducting slab, thermal migration of Nb, Ta, and Ti in aqueous fluids result in Nb, Ta, and Ti enrichment in the cooler region and depletion in the hotter region. As a result of high-pressure metamorphism, hydrous rutile-rich eclogites with overall subchondritic Nb/Ta form in the cooler region, whereas relatively anhydrous rutile-poor eclogites with suprachondritic Nb/Ta form in the hotter region. Subsequently, partial melting of hydrous rutile-rich eclogites with initial subchondritic Nb/Ta at deeper levels transfers overall subchondritic Nb/Ta coupled with Nb, Ta, and Ti depletion characteristics to the CC, leaving dry rutile-poor eclogites with suprachondritic Nb/Ta and rutile-rich residual eclogites with overall, heterogeneous subchondritic Nb/Ta as a complementary reservoir to the CC.
机译:Nb和Ta之间的分离(通常被认为是地球化学“同卵双生”的元素)是解密大陆壳(CC)形成的关键。在这里,我们显示了中国大陆科学钻探(CCSD)项目的闪长岩中金红石晶粒的Nb / Ta明显非均质,但总体呈细软骨状,岩心深度为100-700 m,变化较小,并且主要在岩心深度700处是超单晶的-3025 m,表明整个俯冲板块都有清晰的Nb / Ta分馏。为了了解俯冲板内Nb / Ta分级分离的潜在机理,我们通过激光烧蚀ICPMS分析了热迁移实验,其中将湿安山岩放置在较大的热梯度(300℃/ cm,末端范围为950-350)之间℃)在0.5Gpa。结果表明,由热梯度驱动的Nb,Ta和Ti优先通过扩散通过超临界流体迁移到实验的较冷端(约650-350℃)。由于Nb和Ta的热迁移模式相反,Nb,Ta和Ti之间的较明显的分离发生在较冷的一端。实验结果与CCSD钻孔样品中金红石中Nb,Ta的测定结果一致。我们认为,Nb,Ta之间的主要分馏必须在金红石出现之前发生,最有可能是在Ti也是可移动的时,从蓝晶转变为闪石-榴辉岩转变。在金红石出现之前,富含钛的主要矿物(如闪石)与优先发生脱水的较热区域的流体之间的分配,产生了具有亚软骨状Nb / Ta的富含Nb-Ta-Ti的流体和具有超软骨状Nb / Ta的脱水残留物。同时,由于俯冲板中温度梯度的演化,Nb,Ta和Ti在水性流体中的热迁移导致Nb,Ta和Ti在较冷的区域富集而在较热的区域耗尽。高压变质作用的结果是,较凉爽的区域形成了总体呈亚软骨状Nb / Ta的含水富金红石的榴辉岩,而较热的地区形成了具有超单晶的Nb / Ta相对较无水的金红石的榴辉岩。随后,含水的金红石型富水榴辉岩与初始亚软骨状Nb / Ta的更深部分融化,将总体亚软骨状Nb / Ta以及Nb,Ta和Ti的损耗特征转移至CC,剩下干金红石型榴辉岩和超单晶Nb / Ta富含金红石的残留榴辉岩,整体呈异质亚软骨状Nb / Ta作为CC的补充储层。

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