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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >On the overabundance of light rare earth elements in terrestrial zircons and its implication for Earth's earliest magmatic differentiation
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On the overabundance of light rare earth elements in terrestrial zircons and its implication for Earth's earliest magmatic differentiation

机译:陆地锆石中轻稀土元素的丰度及其对地球最早岩浆分异的意义

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摘要

We present whole-rock and zircon rare earth element (REE) data from two early Archaean gneisses (3.81 Ga and 3.64 Ga) from the Itsaq gneiss complex, south-west Greenland. Both gneisses represent extremely rare examples of unaltered, fresh and relatively undeformed igneous rocks of such antiquity. Cathodoluminescence imaging of their zircon indicates a single crystallisation episode with no evidence for either later metamorphic and/or anatectic reworking or inheritance of earlier grains. Uniform, single-population U/Pb age data confirm the structural simplicity of these zircons. One sample, a 3.64 Ga grandoioritic gneiss from the Gothabsfjord, yields a chondrite-normalised REE pattern with a positive slipe from La to Lu as well as substantial positive Ce and slight negative Eu anomalies, features generally considered to be typical of igneous zircon. In contrast, the second sample, a 3.81 Ga tonalite from south of the Isua Greenstone Belt, has variable but generally much higher light REE abundances, with similar middle to heavy REE. Calculation of zircon/melt distribution coefficients (D_(REE)~(zircon/melt)) from each sample yields markedly different values for the trivalent REE (i.e. Ce and Eu omitted) and simple application of one set of D_(REE)~(zircon/melt) to model the melt composition for the other sample yields concentrations that are in error by up to two orders of magnitude for the light REE (La-Nd). The observed light REE overabundance in the 3.8 Ga tonalite is a commonly observed feature in terrestrial zircons for which a number of explanations ranging from lattice strain to disequilibrium crystallisation have been proposed and are further investigated herein. Regardless of the cause of light REE overabundance, our study shows that simple application of zircon/melt distribution coefficients is not an unambiguous method of ascertaining original melt composition. In this context, recent studies that use REE data to claim that >4.3 Ga Hadean detrital zircons originally crystallised from an evolved magma, in turn suggesting the operation of geological processes in the early Earth analogous to those of the present day (e.g. subduction and melting of hydrated oceanic crust), must be regarded with caution. Indeed, comparison of terrestrial Hadean and >3.9 Ga lunar highland zircons shows remarkable similarities in the light REE, even though subduction processes that have.
机译:我们提供了来自格陵兰西南部的Itsaq片麻岩群的两个早期古生片麻岩(3.81 Ga和3.64 Ga)的全岩石和锆石稀土元素(REE)数据。这两个片麻岩都代表了极少见的古代等未变,新鲜和相对未变形的火成岩的例子。锆石的阴极发光成像表明发生了一次结晶,没有证据表明后来发生了变质和/或返水的返工或早期晶粒的遗传。统一的单种群U / Pb年龄数据证实了这些锆石的结构简单性。一个样品是来自哥德堡峡湾的3.64 Ga大球状片麻岩,产生的球粒陨石归一化REE模式具有从La到Lu的正滑移,以及大量的Ce和正的负Eu异常,通常被认为是火成锆石的典型特征。相比之下,第二个样品是Isua绿岩带以南的3.81 Ga斜长石,其轻稀土元素丰度可变,但通常要高得多,中重稀土元素相似。从每个样品计算锆石/熔体分布系数(D_(REE)〜(锆石/熔体))得出三价REE(即Ce和Eu省略)的值明显不同,并且简单应用一组D_(REE)〜(锆石/熔体)来模拟其他样品的熔体成分,得出的浓度对于轻稀土(La-Nd)的误差最高可达两个数量级。在3.8 Ga角质石中观察到的轻稀土元素过量是陆地锆石中普遍观察到的特征,对此提出了许多解释,从晶格应变到不平衡结晶,并在本文中进行了进一步研究。不管轻稀土过量存在的原因,我们的研究表明,简单应用锆石/熔体分布系数并不是确定原始熔体成分的明确方法。在这种情况下,最近的研究使用REE数据声称> 4.3 Ga Hadean碎屑锆石最初是从演化的岩浆中结晶出来的,这反过来又暗示了地球早期的地质过程类似于当今的地质过程(例如俯冲和熔化)。的水合大洋壳),必须谨慎对待。的确,即使有俯冲过程,陆地哈德族和> 3.9 Ga月球高地锆石的比较也显示出轻稀土具有显着相似性。

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