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Silicon isotopes reveal recycled altered oceanic crust in the mantle sources of Ocean Island Basalts

机译:硅同位素揭示了大洋洲玄武岩地幔源中的再生蚀变海洋壳

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摘要

The study of silicon (Si) isotopes in Ocean Island Basalts (OIB) has the potential to discern between different models for the origins of geochemical heterogeneities in the mantle. Relatively large (similar to several per mil per atomic mass unit) Si isotope fractionation occurs in low-temperature environments during biochemical and geochemical precipitation of dissolved Si, where the precipitate is preferentially enriched in the lighter isotopes relative to the dissolved Si. In contrast, only a limited range (similar to tenths of a per mil) of Si isotope fractionation has been observed from high-temperature igneous processes. Therefore, Si isotopes may be useful as tracers for the presence of crustal material within OIB mantle source regions that experienced relatively low-temperature surface processes in a manner similar to other stable isotope systems, such as oxygen. Characterizing the isotopic composition of the mantle is also of central importance to the use of the Si isotope system as a basis for comparisons with other planetary bodies (e.g., Moon, Mars, asteroids).
机译:对大洋洲玄武岩(OIB)中硅(Si)同位素的研究有可能区分地幔中地球化学非均质性起源的不同模型。相对较大的(类似于每原子质量单位每密耳数个)Si同位素分馏发生在溶解的Si的生化和地球化学沉淀过程中的低温环境中,相对于溶解的Si,该沉淀优先富集于较轻的同位素中。相反,从高温火成过程仅观察到有限范围的Si同位素分馏(类似于每密耳的十分之一)。因此,Si同位素可用作示踪剂,用于以类似于其他稳定同位素系统(例如氧气)的方式经历相对低温表面过程的OIB地幔源区中地壳物质的存在。表征地幔的同位素组成对于使用Si同位素系统作为与其他行星体(例如,月亮,火星,小行星)进行比较的基础也至关重要。

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