首页> 外文期刊>Contributions to Mineralogy and Petrology >Petrogenesis of the amphibole-rich veins from the Lherz orogenic lherzolite massif (Eastern Pyrenees, France): a case study for the origin of orthopyroxene-bearing amphibole pyroxenites in the lithospheric mantle
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Petrogenesis of the amphibole-rich veins from the Lherz orogenic lherzolite massif (Eastern Pyrenees, France): a case study for the origin of orthopyroxene-bearing amphibole pyroxenites in the lithospheric mantle

机译:来自Lherz造山形锂铁矿地块(法国东比利牛斯)的富含闪石的脉的成岩作用:以岩石圈地幔中含邻苯二甲闪石的辉石为起源的案例研究

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摘要

The Lherz orogenic lherzolite massif (Eastern French Pyrenees) displays one of the best exposures of subcontinental lithospheric mantle containing veins of amphibole pyroxenites and hornblendites. A reappraisal of the petrogenesis of these rocks has been attempted from a comprehensive study of their mutual structural relationships, their petrography and their mineral compositions. Amphibole pyroxenites comprise clinopyroxene, orthopyroxene and spinel as early cumulus phases, with garnet and late-magmatic K2O-poor pargasite replacing clinopyroxene, and subsolidus exsolution products (olivine, spinel II, garnet II, plagioclase). The original magmatic mineralogy and rock compositions were partly obscured by late-intrusive hornblendites and over a few centimetres by vein–wallrock exchange reactions which continued down to subsolidus temperatures for Mg–Fe. Thermobarometric data and liquidus parageneses indicate that amphibole pyroxenites started to crystallize at P ≥ 13 kbar and recrystallized at P < 12 kbar. The high AlVI/AlIV ratio (>1) of clinopyroxenes, the early precipitation of orthopyroxene and the late-magmatic amphibole are arguments for parental melts richer in silica but poorer in water than alkali basalts. Their modelled major element compositions are similar to transitional alkali basalt with about 1–3 wt% H2O. In contrast to amphibole pyroxenites, hornblendites only show kaersutite as liquidus phase, and phlogopite as intercumulus phase. They are interpreted as crystalline segregates from primary basanitic magmas (mg=0.6; 4–6 wt% H2O). These latter cannot be related to the parental liquids of amphibole pyroxenites by a fractional crystallization process. Rather, basanitic liquids mostly reused pre-existing pyroxenite vein conduits at a higher structural level (P ≤ 10 kbar). A continuous process of redox melting and/or alkali melt/peridotite interaction in a veined lithospheric mantle is proposed to account for the origin of the Lherz hydrous veins. The transitional basalt composition is interpreted in terms of extensive dissolution of olivine and orthopyroxene from wallrock peridotite by alkaline melts produced at the mechanical boundary layer/thermal boundary layer transition (about 45–50 km deep). Continuous fluid ingress allowed remelting of the deeper veined mantle to produce the basanitic, strongly volatiles enriched, melts that precipitated hornblendites. A similar model could be valid for the few orthopyroxene-rich hydrous pyroxenites described in basalt-hosted mantle xenoliths.
机译:Lherz造山带锂铁矿地块(法国东部比利牛斯山脉)显示出含有闪石辉石和角闪石脉的次大陆岩石圈地幔最佳暴露之一。通过对它们的相互结构关系,岩石学和矿物成分的全面研究,试图重新评估这些岩石的岩石成因。闪石的辉石岩包括早期的积云阶段的斜辉石,邻辉石和尖晶石,石榴石和后期岩浆中的贫K2 O辉石代替斜辉石和亚固相分离产物(橄榄石,尖晶石II,榴石II,斜长石)。最初的岩浆矿物学和岩石成分被晚期侵入性的角闪长岩部分遮盖,并因脉-壁岩石交换反应(持续到亚固相温度下的Mg-Fe)超过了几厘米。热压数据和液相线同源物表明,闪石辉石在P≥13 kbar时开始结晶,在P <12 kbar时重结晶。斜辉石的AlVI / AlIV 比高(> 1),邻辉石的早期析出和岩浆闪石的晚闪石是母体熔体中二氧化硅含量高而在水中比碱玄武岩中差的理由。他们模拟的主要元素组成与过渡碱式玄武岩相似,含大约1-3 wt%H2 O。与角闪石辉石岩相比,角闪石仅显示出喀苏石为液相,而金云母为积间相。它们被解释为是初级基底岩浆的结晶偏析物(mg = 0.6; 4-6 wt%H2O)。后者不能通过分步结晶过程而与闪石辉石的母液有关。相反,玄武质液体大多以较高的结构水平(P≤10 kbar)再利用预先存在的辉石岩静脉导管。提出了在脉状岩石圈地幔中氧化还原熔融和/或碱熔/橄榄岩相互作用的连续过程,以解释Lherz含水脉的起源。过渡玄武岩成分的解释是,在机械边界层/热边界层过渡(约45至50 km深)产生的碱性熔体将橄榄岩和邻苯二酚从围岩橄榄岩中大量溶解。连续不断的流体进入使得深部静脉地幔发生重熔,从而产生了玄武质,强烈挥发的富集熔体,使角闪石沉淀。类似的模型对于玄武岩质地幔异岩中描述的少量富含邻苯二酚的含水辉石也可能有效。

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    《Contributions to Mineralogy and Petrology》 |2001年第4期|383-403|共21页
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    Laboratoire de Minéralogie Muséum National d'Histoire Naturelle ESA–CNRS 7058 61 rue Buffon 75005 Paris France e-mail: lorand@mnhn.fr;

    Laboratoire de Minéralogie Muséum National d'Histoire Naturelle ESA–CNRS 7058 61 rue Buffon 75005 Paris France e-mail: lorand@mnhn.fr;

    Laboratoire de Minéralogie Muséum National d'Histoire Naturelle ESA–CNRS 7058 61 rue Buffon 75005 Paris France e-mail: lorand@mnhn.fr;

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