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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Sedimentary halogens and noble gases within Western Antarctic xenoliths: Implications of extensive volatile recycling to the sub continental lithospheric mantle
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Sedimentary halogens and noble gases within Western Antarctic xenoliths: Implications of extensive volatile recycling to the sub continental lithospheric mantle

机译:南极西部异种岩中的沉积卤素和稀有气体:对亚大陆岩石圈地幔的大量挥发物再循环的影响

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摘要

Recycling of marine volatiles back into the mantle at subduction zones has a profound, yet poorly constrained impact on the geochemical evolution of the Earth's mantle. Here we present a combined noble gas and halogen study on mantle xenoliths from the Western Antarctic Rift System (WARS) to better understand the flux of subducted volatiles to the sub continental lithospheric mantle (SCLM) and assess the impact this has on mantle chemistry. The xenoliths are extremely enriched in the heavy halogens (Br and I), with I concentrations up to 1 ppm and maximum measured I/C1 ratios (85.2 x 10(-3)) being similar to 2000 times greater than mid ocean ridge basalts (MORB). The Br/C1 and I/C1 ratios of the xenoliths span a range from MORB-like ratios to values similar to marine pore fluids and serpentinites, whilst the Kr-84/Ar-36 and Xe-136/Ar-36 ratios range from modern atmosphere to oceanic sediments. This indicates that marine derived volatiles have been incorporated into the SCLM during an episode of subduction related metasomatism. Helium isotopic analysis of the xenoliths show average He-3/He-4 ratios of 7.5 +/- 0.5 R-A (where R-A is the He-3/He-4 ratio of air = 1.39 x 10(-6)), similar to that of MORB. The He-3/He-4 ratios within the xenoliths are higher than expected for the xenoliths originating from the SCLM which has been extensively modified by the addition of subducted volatiles, indicating that the SCLM beneath the WARS must have seen a secondary alteration from the infiltration and rise of asthenospheric fluids/melts as a consequence of rifting and lithospheric thinning. Noble gases and halogens within these xenoliths have recorded past episodes of volatile interaction within the SCLM and can be used to reconstruct a tectonic history of the WARS. Marine halogen and noble gas signatures within the SCLM xenoliths provide evidence for the introduction and retention of recycled volatiles within the SCLM by subduction related metasomatism, signifying that not all volatiles that survive subduction are mixed efficiently through the convecting mantle. The global SCLM therefore represents a potentially important reservoir for the long term residence of subducted volatiles. (C) 2016 Published by Elsevier Ltd.
机译:在俯冲带将海洋挥发物再循环回地幔对地球地幔的地球化学演化具有深远但受约束的影响。在这里,我们对来自南极裂谷系统(WARS)的地幔异种岩进行稀有气体和卤素的组合研究,以更好地了解俯冲挥发物通向亚大陆岩石圈地幔(SCLM)的流量,并评估其对地幔化学的影响。异种岩中的重卤素(Br和I)极为丰富,I浓度高达1 ppm,最大测得的I / C1比(85.2 x 10(-3))约为中海脊玄武岩的2000倍( MORB)。异岩的Br / C1和I / C1比值范围从MORB类比值到类似于海洋孔隙流体和蛇纹岩的值,而Kr-84 / Ar-36和Xe-136 / Ar-36比值范围从现代大气到海洋沉积物。这表明在与俯冲有关的交代作用期间,海洋衍生的挥发物已被纳入SCLM。异种石的氦同位素分析显示,平均He-3 / He-4比率为7.5 +/- 0.5 RA(其中RA是空气的He-3 / He-4比率= 1.39 x 10(-6)),与MORB。异种岩中的He-3 / He-4比率高于源自SCLM的异种岩的预期值,该物质已通过添加俯冲挥发物进行了广泛修改,这表明WARS下的SCLM必须经历了次生变化。裂谷和岩石圈变薄的结果是软流圈流体/熔体的渗透和上升。这些异质岩中的稀有气体和卤素已记录了SCLM内过去的挥发性相互作用,可用于重建WARS的构造历史。 SCLM异种岩中的海洋卤素和稀有气体特征通过俯冲相关的交代作用为SCLM内引入和保留循环挥发物提供了证据,这表明并非所有在俯冲中幸存的挥发物都通过对流地幔有效混合。因此,全球SCLM代表着潜入挥发物长期驻留的潜在重要储量。 (C)2016由Elsevier Ltd.出版

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