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首页> 外文期刊>Contributions to Mineralogy and Petrology >Nb–Ta fractionation by partial melting at the titanite–rutile transition
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Nb–Ta fractionation by partial melting at the titanite–rutile transition

机译:通过在钛铁矿-金红石相变过程中部分熔融而分离出Nb-Ta

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摘要

During the evolution of the Earth, distinct geochemical reservoirs with different Nb/Ta ratios have developed. Archean granitoids of the tonalite–trondhjemite– granodiorite (TTG) suite, which represent the Earth’s early continental crust, show larger Nb/Ta variations than any other Earth reservoir. This implies that significant Nb–Ta fractionation must have occurred during early crust formation, while the underlying mechanism behind is still unclear. Here, we present a new model on how Nb may be fractionated from Ta during partial melting of subducted oceanic crust. Our data show that Nb/Ta ratios in meltsderived from rutile- and titanite-bearing eclogite are largely controlled by the modal relative abundances of rutile and titanite in the source. High modal ratios of titanite over rutile generate melts with very high Nb/Ta (>60), whereas low modal titanite/rutile produces melts with much lower Nb/Ta (≤30). Very low Nb/Ta (>16) occur when all Ti-phases are consumed at very high degrees of melting. As the modal ratio of titanite to rutile is a function of pressure, the Nb/Ta of melts is a function of melting depth. Our new model helps to explain the extreme variation of Nb/Ta observed in many TTGs and thus how Nb and Ta were fractionated during the early evolution of the Earth. Furthermore, the model also indicates that simple one-stage melting models for mafic crust are not sufficient to explain the formation of TTGs.
机译:在地球演化过程中,已开发出具有不同Nb / Ta比的独特地球化学储层。斜方晶石-长生硬岩-花岗闪长岩(TTG)组的太古代花岗岩,代表了地球早期的地壳,其Nb / Ta的变化比其他任何地球储层都大。这意味着在早期地壳形成过程中必须发生大量的Nb-Ta分馏,而其背后的潜在机制仍不清楚。在这里,我们提出了一个新的模型,说明在俯冲的洋壳部分融化过程中,如何从Ta中分离出Nb。我们的数据表明,来自金红石和钛矿的榴辉岩衍生的熔体中的Nb / Ta比在很大程度上受源中金红石和钛矿的模态相对丰度的控制。钛铁矿对金红石的高模态比产生的熔体具有很高的Nb / Ta(> 60),而低模态的钛铁矿/金红石产生的熔体具有低得多的Nb / Ta(≤30)。当所有钛相都以非常高的熔化度消耗时,就会产生非常低的Nb / Ta(> 16)。由于钛矿与金红石的模态比是压力的函数,因此熔体的Nb / Ta是熔化深度的函数。我们的新模型有助于解释在许多TTG中观察到的Nb / Ta的极端变化,从而解释了地球早期演化过程中Nb和Ta的分离方式。此外,该模型还表明,简单的一阶镁铁质地壳熔融模型不足以解释TTG的形成。

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