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首页> 外文期刊>Journal of Petrology >Metasomatism in the Lithospheric Mantle beneath Middle Atlas (Morocco) and the Origin of Fe- and Mg-rich Wehrlites
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Metasomatism in the Lithospheric Mantle beneath Middle Atlas (Morocco) and the Origin of Fe- and Mg-rich Wehrlites

机译:中阿特拉斯(摩洛哥)下岩石圈地幔的交代作用和富含铁和镁的辉绿岩的成因

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Mantle xenoliths enclosed in the Plio-Quaternary alkaline basalts from Bou Ibalrhatene, Middle Atlas, Morocco, are characterized by a wide range of lithological and chemical heterogeneity, consistent with metasomatism of their lithospheric mantle source. Subordinate porphyroclastic to protogranular spinel-lherzolites associated with websterites exhibit major and trace element signatures, along with a depleted mantle isotopic affinity, that testify to ancient melt extraction processes, possibly during Neo- to Paleoproterozoic times. These samples show large ion lithophile element (LILE) enrichments that have been imparted a long time after the accretion of their protoliths to the lithosphere, induced by alkaline melts rising from upwelling HIMU-like asthenosphere since the late Cretaceous or Eocene. Extensive sectors of the percolated lherzolite and harzburgite mantle progressively approached chemical equilibrium with the migrating melts, forming porphyroblastic amphibole-rich ultramafic rocks with strong LILE enrichment, highly variable (enriched to strongly depleted) high field strength element (HFSE) abundances and HIMU-like isotopic signatures. As a result, the older depleted lithosphere was progressively refertilized. The presence among the Bou Ibalrhatene ultramafic xenoliths of both Fe- and Mg-rich wehrlites is a rare occurrence in xenolith suites. The Fe-rich wehrlites formed by the migration through dunitic channels, which opened during earlier reactive porous flow, of larger and larger volumes of rising alkaline melts, becoming progressively less evolved in composition and more similar to the erupted lavas. In contrast, subordinate Mg-rich wehrlites characterized by the presence of apatite, extreme LILE enrichment and HFSE depletion testify to the localized chemical effects of either carbonatite melts related to the oldest (i.e. Eocene) volcanic activity in the area or, more probably, to highly evolved SiO2-saturated silicate melts that vanished through interaction with the lithosphere. As a whole, the textural, petrographic and chemical characteristics of the Bou Ibalrhatene xenoliths suggest prolonged thermo-chemical erosion of an originally heterogeneous lithosphere with a dominant depleted mantle isotopic signature by melts rising from a HIMU-like asthenospheric mantle source in response to intraplate tectonic reactivation and rifting of the Pan-African basement. The overall scenario envisaged for lithosphere–asthenosphere interaction beneath the Middle Atlas is similar to that inferred for other Cenozoic Central–Northern African volcanic centres, such as Hoggar (Algeria) and Gharyan (Libya). The majority of the mantle sectors beneath the NE–SW volcanic alignment associated with the Trans-Moroccan fault system consist of rejuvenated lithosphere formed by small-scale, shallow-mantle upwelling and accretion of asthenospheric material since late Cretaceous or Eocene times.
机译:摩洛哥中阿特拉斯的布·伊巴拉雷塔内的上新统第四纪碱性玄武岩中包裹的地幔异岩具有广泛的岩性和化学非均质性,与其岩石圈地幔源的交代作用相一致。与维斯特岩相关的下成岩碎屑状至原粒尖晶石-斜纹岩显示出主要和微量元素特征,以及地幔同位素亲和力降低,这证明了古老的熔体提取过程,可能是在新元古代到古元古代。这些样品显示出大量的离子亲石元素(LILE)富集,这是由于自晚白垩纪或始新世以来从上升HIMU样软流圈上升的碱性熔体引起的,其原石积聚到岩石圈后很长时间才被赋予。大量渗出的锂铁矿和harzburgite地幔随着迁移的熔体逐渐接近化学平衡,形成了富含利勃生质,高度可变(富集到强烈耗尽)高场强元素(HFSE)丰度和类似HIMU的富卟啉弹状闪石的超镁铁质岩石。同位素签名。结果,较老的枯竭的岩石圈逐渐被溶化。富含铁和镁的辉绿岩在Bou Ibalrhatene超镁铁质异质岩中的存在在异质岩组中很少见。富铁辉绿岩是通过在早期的反应性多孔流中打开的,通过二元通道迁移而形成的,越来越多的上升的碱性熔体在组成上逐渐减少,而与喷出的熔岩越来越相似。相反,特征在于存在磷灰石,极端LILE富集和HFSE耗尽的富镁次生辉石岩证明了该地区最古老(即始新世)火山活动有关的碳酸盐熔岩的局部化学作用。高度演化的SiO 2 -饱和硅酸盐熔体通过与岩石圈的相互作用而消失。总体而言,Bou Ibalrhatene异岩的质地,岩石学和化学特征表明,对原板岩岩石圈的长期热化学侵蚀作用是通过响应于板内构造的类似HIMU的软流圈地幔源的熔体上升而形成的,地幔同位素特征明显减少泛非地下室的重新活化和裂谷。中图集下方岩石圈-软流圈相互作用的总体设想与其他新生代中北部-北非火山中心(如霍加尔(阿尔及利亚)和加里扬(利比亚))的设想相似。与白垩纪或始新世晚期相比,与跨摩洛哥断裂系统有关的NE-SW火山线之下的大部分地幔部分由年轻的岩石圈组成,这些岩石圈由小规模的浅地幔隆升和软流圈物质的堆积形成。

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    《Journal of Petrology 》 |2009年第2期| p.197-249| 共53页
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    1CNR–Istituto di Geoscienze E Georisorse, Sezione di Pavia, Via Ferrata 1, I-27100 Pavia, Italy 2Dipartimento di Scienze Della Terra, Università di Pavia, Via Ferrata 1, I-27100 Pavia, Italy 3Institut Universitaire Européen de La Mer, UniversitÉ de Bretagne Occidentale, UMR 6538, Place Copernic, F-29280, Plouzane, France 4Laboratoire de Géologie—UMR 6524, Université Blaise Pascal, 5 Rue Kessler, F-63038, Clermont-Ferrand Cedex, France;

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