首页> 外文期刊>Journal of South American earth sciences >Petrogenesis of mica-amphibole-bearing lamprophyres associated with the Paleoproterozoic Morro do Afonso syenite intrusion, eastern Brazil
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Petrogenesis of mica-amphibole-bearing lamprophyres associated with the Paleoproterozoic Morro do Afonso syenite intrusion, eastern Brazil

机译:巴西东元古元古代Morro do Afonso绢云母侵入带云母-含闪石斑岩的成岩作用

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摘要

Mica-amphibole-lamprophyres, identified as vogesites, are associated with the Paleoproterozoic Morro do Afonso syenite intrusion in northeastern Brazil. The lamprophyres occur mainly as dykes that crosscut the syenitic rocks and occasionally as enclaves. Lamprophy-ric rocks are formed by the early magmatic paragenesis amphibole-clinopyroxene-apatite-phlogopite-ilmenite; feldspars are found in the groundmass. Near liquidus amphibole is edenite, close to the boundary with pargasite, which is enriched in alkalis relative to the other amphiboles (Mg-hornblende and actinolite). Clinopyroxene is diopside, and inclusions of phlogopite are analyzed in both clinopyroxene and amphibole phenocrysts. The chemical evolution of the mafic minerals is consistent with increasing oxygen fugacity during late magmatic stages. Whole-rock geochemical data suggest a metaluminous, ultrapotassic parental liquid, with silica saturation close to the limit of undersaturation. Trace element concentrations, such as enrichment in large ion lithophile and strong depletion of some high field-strength elements, indicate a mantle source that was partially modified by a subduction event. In this metasomatic mantle, it is important to emphasize the strong enrichment of light rare-earth elements, which is higher than those typically associated with basaltic rocks from active continental margins, and corresponding concentrations similar to those determined in lamproitic rocks. Major element modeling shows that fractional crystallization and magma flow segregation are the main petrogenetic processes involved in the magmatic evolution of lamprophyre magma, and it is possible to generate syenite magma by these mechanisms.
机译:云母-闪石-斑岩藻被认为是辉石,与巴西东北部的古元古代莫罗-阿方索正长岩侵入有关。煌斑岩主要以横穿蛇纹岩的堤坝为主,偶尔也有飞地。早古岩浆共生闪石-斜辉石-磷灰石-金云母-钛铁矿形成了火山岩。长石存在于地下。液相线闪石附近的辉石是辉石,靠近辉石的边界,相对于其他闪石(镁角闪石和阳起石),辉石富含碱。 Clinopyroxene是透辉石,并在clinopyroxene和角闪石phenocrysts中分析了金云母的夹杂物。镁铁质矿物的化学演化与岩浆后期后期的氧气逸度增加是一致的。整个岩石的地球化学数据表明,它是一种金属的,超钾的母液,二氧化硅的饱和度接近饱和度的极限。痕量元素的浓度,例如大量离子亲石物质的富集和某些高场强元素的强耗尽,表明地幔源已被俯冲事件部分修饰。在这种变质作用地幔中,重要的是要强调轻稀土元素的强富集,这要比活跃大陆边缘的玄武岩通常所富集的那些富集的高,并且相应的浓度类似于在黄铁矿中确定的那些。主要元素模拟表明,部分结晶和岩浆流偏析是与煌斑岩岩浆岩浆演化有关的主要成岩过程,并有可能通过这些机制生成正长岩浆岩。

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