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首页> 外文期刊>Mineralogy and Petrology >Minette mafic microgranular enclaves and their relationship to host syenites in systems formed at mantle pressures: major and trace element evidence from the Piquiri Syenite Massif, southernmost Brazil
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Minette mafic microgranular enclaves and their relationship to host syenites in systems formed at mantle pressures: major and trace element evidence from the Piquiri Syenite Massif, southernmost Brazil

机译:地幔压力下形成的Minette镁铁质微颗粒飞地及其与主体正长岩的关系:来自巴西最南端的Piquiri Syenite断层的主要和微量元素证据

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Mafic microgranular enclaves in the ultrapotassic Piquiri Syenitic Massif (611 + - 1 Ma) in southern Brazil represent a minette magma mingled with a syenitic one, both produced from similar mantle sources and emplaced in a post-collisional setting of Neo-proterozoic age. The minette magma is compositionally close to typical minettes and high-SiO_2 lamproites, with relatively high contents of LREE, Cs and Rb. It is slightly silica-undersaturated, ultrapotassic and metaluminous, with K_2O/Na_2O ratios around 2-3, and about 4-7 wt percent K_2O. The Piquiri minettes contain K-clinopyroxene and py-rope, which are interpreted to have crystallized under pressures about 5 GPa. Whole-rock and mineral chemistry indicate that the most suitable source for the minette magma is clinopyroxene-phlogopite-apatite-amphibole-sulphide + - garnet mantle veins, under pressures of about 5 GPa and melting temperatures over 1,000 deg C. Fractional melting is admitted in order to explain the extremely high Rb, Cs and LREE contents of the minette melt, and is consistent with its estimated rheological behavior. The syenitic host-rock parental magma was produced from a similar source, probably at lower pressures, and the co-mingling probably occurred still at large depth, under pressures around 3 GPa. Rheological and geochemical considerations support a model based on fractional melting of a veined mantle which had been metasomatized during previous (760-700 Ma) ocean-plate consumption. The subduction-related metasomatism in the source is indicated by low LREE/(Nb or Ta) ratios, high Nb/Ta and U/Th ratios, and low Ti contents. The compositional similarity and close spatial and temporal association of minette and syenitic magmas can be explained by their common source region. Compared to typical lamproitic magmatism, the major difference is that the Piquiri minette magmas are derived from a subduction-modified source.
机译:巴西南部超钾质的Piquiri Syenitic地块(611 +-1 Ma)中的镁铁质微细颗粒飞地代表了一种min浆岩浆,混有一种Syenitic岩浆,两者均来自相似的地幔来源,并置于新元古代的碰撞后环境中。碎浆岩浆在成分上接近典型的碎浆岩和高SiO_2的堇青石,其中LREE,Cs和Rb的含量相对较高。它是略微不足以饱和的二氧化硅,超钾和金属质,K_2O / Na_2O的比例约为2-3,K_2O约为4-7重量%。皮基里(Piquiri)碎浆机包含K-斜基吡咯和py-rope,它们被解释为在约5 GPa压力下结晶。全岩石和矿物化学表明,小成矿岩浆最合适的来源是斜辉石-金云母-磷灰石-磷灰石-闪石-硫化物+-石榴石地幔脉,在约5 GPa的压力和超过1000摄氏度的熔化温度下进行。允许部分熔化为了解释薄饼熔体中极高的Rb,Cs和LREE含量,并与其估计的流变行为相一致。共生的母岩母岩浆是由类似的来源产生的,可能是在较低的压力下发生的,并且在3 GPa左右的压力下,混合仍可能在较大的深度发生。流变学和地球化学方面的考虑支持了一种模型,该模型基于在先前(760-700 Ma)海底消耗期间已交代化的脉状地幔的部分熔融。源中与俯冲有关的交代作用由低LREE /(Nb或Ta)比,高Nb / Ta和U / Th比以及低Ti含量指示。细小岩浆和共生岩浆的成分相似性和紧密的时空联系可以通过它们共同的源区来解释。与典型的浅红岩岩浆相比,主要的不同之处在于,Piquiri薄板岩浆岩浆来自俯冲改造源。

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