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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Os, Pb, and Nd isotope geochemistry of the Permian Emeishan continental flood basalts: Insights into the source of a large igneous province
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Os, Pb, and Nd isotope geochemistry of the Permian Emeishan continental flood basalts: Insights into the source of a large igneous province

机译:二叠纪峨眉山大陆性洪水玄武岩的Os,Pb和Nd同位素地球化学:对火成岩大省起源的认识

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摘要

The nature of the source of continental flood basalts (CFB) is a highly debated topic. Proposed mantle sources for CFBs, including both high- and low-Ti basalts, include subcontinental lithospheric mantle (SCLM), asthenospheric mantle, and deep, plume-related mantle. Re-Os isotope systematics can offer important constraints on the sources of both ocean island basalts (OIB) and CFB, and may be applied to distinguish different possible melt sources. This paper reports the first Re-Os isotope data for the Late Permian Emeishan large igneous province (LIP) in Southwest China. Twenty one CFB samples including both low- and high-Ti basalts from five representative sites within the Emeishan LIP have been analyzed for Os, Nd, and Pb isotopic compositions. The obtained Os data demonstrate that crustal assimilation affected Os isotopic compositions of some Emeishan basalt samples with low Os concentrations but not all of the samples, and the Emeishan basalts with high Os contents likely experienced the least crustal contamination. The low and high-Ti basalts yield distinct Os signatures in terms Of Os-187/Os-188 and Os content. The low-Ti basalt with the highest Os concentration (400 ppt) has a radiogenic Os isotopic composition (gamma Os(t), +6.5), similar to that of plume-derived OIB. Because the Os isotopic composition of basalts with relatively high Os concentrations (typically > 50 ppt) likely represents that of their mantle source, this result implies a plume-derived origin for the low-Ti basalts. On the other hand, the high-Ti basalts with high Os concentration (over 50 ppt) have unradiogenic Os isotopic signatures (gamma Os(t) values range from -0.8 to -1.4), suggesting that a subcontinental lithosphere mantle (SCLM) component most likely contributed to the generation of these magmas. Combining Pb and Nd isotopic tracers with the Os data, we demonstrate that the low-Ti basaltic magmas in the Emeishan CFB were mainly sourced from a mantle plume reservoir, whereas the high-Ti basaltic magmas were most likely derived from a SCLM reservoir or were contaminated by a significant amount of lithospheric mantle material during plume-related magma ascent through the SCLM. (c) 2007 Elsevier Ltd. All rights reserved.
机译:大陆洪水玄武岩(CFB)的来源性质是一个备受争议的话题。 CFB的提议地幔来源,包括高钛玄武岩和低钛玄武岩,都包括次大陆岩石圈地幔(SCLM),软流圈地幔以及与羽流有关的深部地幔。 Re-Os同位素系统可以对海洋玄武岩(OIB)和CFB的来源提供重要的限制,并且可以用于区分不同的可能熔体来源。本文报道了中国西南地区晚二叠世峨眉山大火成岩省(LIP)的第一个Re-Os同位素数据。分析了21个来自峨眉山LIP内五个代表性地点的低钛和高钛玄武岩的CFB样品的Os,Nd和Pb同位素组成。所获得的Os数据表明,地壳同化影响了一些Os浓度低但并非全部样品的峨眉山玄武岩样品的Os同位素组成,而高Os含量的峨眉山玄武岩可能经历了最小的地壳污染。低钛和高钛玄武岩在Os-187 / Os-188和Os含量方面产生明显的Os签名。 Os浓度最高(400 ppt)的低钛玄武岩具有放射源性Os同位素组成(γOs(t),+ 6.5),类似于烟羽来源的OIB。由于具有较高Os浓度(通常> 50 ppt)的玄武岩的Os同位素组成可能代表了其地幔来源,因此该结果暗示了低Ti玄武岩的羽状来源。另一方面,具有高Os浓度(超过50 ppt)的高Ti玄武岩具有非放射源性Os同位素特征(γOs(t)值范围从-0.8到-1.4),这表明该大陆次岩石圈地幔(SCLM)成分最有可能促成了这些岩浆的产生。结合Pb和Nd同位素示踪剂与Os数据,我们证明峨眉山CFB中的低Ti玄武岩浆主要来自地幔柱储层,而高Ti玄武岩浆最有可能来自SCLM储层或在通过SCLM与羽有关的岩浆上升过程中,被大量岩石圈地幔物质污染。 (c)2007 Elsevier Ltd.保留所有权利。

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