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首页> 外文期刊>Contributions to Mineralogy and Petrology >Aluminous websterite and granulite xenoliths from the Chyulu Hills volcanic field, Kenya: gabbro-troctolitic cumulates subjected to lithospheric foundering
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Aluminous websterite and granulite xenoliths from the Chyulu Hills volcanic field, Kenya: gabbro-troctolitic cumulates subjected to lithospheric foundering

机译:肯尼亚Chyulu Hills火山田的铝镁铝榴石和花岗石异岩:岩石圈下沉的辉长岩-微晶石堆积物

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Whole rock major and trace element abundances in aluminous garnet-spinel websterite, sapphi-rine-bearing Mg-Al granulite and hibonite-bearing Ca-Al granulite xenoliths from the Chyulu Hills volcanic field, Kenya, suggest that the samples represent a meta-igneous suite linked by fractionation. The incompatible major element contents increase from the websterites to the Mg-Al granulites and further to the Ca-Al granu-lites. High bulk rock Mg#s and very low concentrations of most incompatible trace elements indicate that the rocks are cumulates rather than crystallized melts. Elevated Ni abundances, impoverishment in Cr and HFSE and high contents of normative plagioclase and olivine in the granulites indicate that their protoliths were similar to troctolite. The textures and metamorphic reaction paths recorded in the granulites suggest igneous emplacement in the crust and cooling from igneous to ambient crustal temperatures accompanied or followed by compression. For the websterite xenoliths, there is an apparent contradiction between the results of P-T calculations that suggest high P and T of crystallization of early generation pyroxenes and elevated P-T conditions during final equilibration (1.4-2.2 GPa/740-980 deg C) on the one hand and the positive Eu anomaly that suggests shallow-level plagioclase accumulation on the other hand. This contradiction can be reconciled by a model of compression of a plagioclase-bearing (gab-broic) protolith to mantle depths where it recrystallized to an ultramafic assemblage, which requires foundering of dense lower crustal material into the mantle.
机译:肯尼亚丘尤鲁山火山场中的铝石榴石-尖晶石型韦斯特石,含蓝宝石-碱的Mg-Al花岗岩和含钙铝石的Ca-Al花岗岩异岩中的整个岩石主要元素和痕量元素丰度表明,这些样品代表了亚火成岩套件通过分数链接。不相容的主要元素含量从韦氏体到Mg-Al颗粒,再到Ca-Al颗粒,增加。大量Mg#s和极低浓度的大多数不相容的痕量元素表明,岩石是堆积而不是结晶的熔体。镍中镍的含量增加,Cr和HFSE的贫化以及规范性斜长石和橄榄石的含量较高,这表明它们的原生石与滑石类似。粒状岩中记录的质地和变质反应路径表明,火成岩在地壳中存在,并伴随着或紧随压缩而从火成岩降温到周围的地壳温度。对于维氏异种石,PT计算结果之间存在明显矛盾,这表明早期辉石的结晶的高P和T和最终平衡(1.4-2.2 GPa / 740-980℃)期间的PT条件升高。另一方面,正Eu异常则表明浅层斜长石堆积。可以通过将斜长石(gab-bric)原生岩压缩到地幔深度的模型来调解这种矛盾,在那里将其重结晶成超镁铁质的组合,这需要将密集的下地壳物质沉入地幔中。

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