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Petrogenesis of the Mesoproterozoic Lamproites from the Krishna Valley, Eastern Dharwar Craton, Southern India

机译:印度南部东部达沃克拉通的克里希纳河谷中元古界镍铁矿的成岩作用

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Petrology and geochemistry of eleven Mesoproterozoic lamproites from the Krishna valley, Eastern Dharwar craton, are presented. The Krishna lamproites show wide variation in their petrography and modal mineralogy and constitute excellent examples of rare phenomenon of heteromorphism. Ti-phlogopite, clinopyroxene, richterite, Fe-rich sanidine, sphene, F-rich apatite, ilmenite, and rutile are the major minerals present in varying proportions. Their mineral compositions overlap with those present in world-wide Phanerozoic lamproites and casts doubt on recent suggestions regarding the absence of archetypal lamproites and kimberlites from the Indian cratons. Incompatible trace element ratios (i) rule out the Krishna lamproites to be products of direct plume- (asthenospheric) derived mantle as well as subduction-related components and (ii) demonstrate their derivation from sources similar to those of the co-spatial Cuddapah basin lamproites and Wajrakarur- and Narayanpet-kimberlites from the Eastern Dharwar craton. The source enrichment of the Krishna lamproites is related to the period of global-scale mantle upwelling at ~1.9 Ga that included the emplacement of Large igneous provinces of similar age and magmatism in the Dharwar and Bastar cratons (India), the Superior Craton (Canada) and the Kaapvaal craton (southern Africa). We find that the observed petrological and geochemical characteristics of the Krishna lamproites can be best explained by the vein-plus-wall-rock model involving phlogopite + amphibole + rutile + clinopyroxene + apatite + titanite occuring as metasomatic veins in a depleted lithospheric mantle, within the garnet stability field. Our study illustrates the significant role of the lithospheric thickness and its attendant metasomatism in influencing petrogenesis of the co-spatial Mesoproterozoic lamproites and kimberlites from the Eastern Dharwar craton.
机译:介绍了来自东达荷克拉通克里希纳河谷的11个中元古代红岩的岩石学和地球化学。克里希纳陨石在岩石学和模态矿物学上表现出很大的差异,并且是罕见的异质现象的极好例子。钛金云母,斜辉石,富钛矿,富铁的山铁矿,蝶粉,富氟磷灰石,钛铁矿和金红石是不同比例的主要矿物质。它们的矿物成分与世界范围的生代代镍铁矿中存在的矿物成分重叠,并对最近有关印度克拉通不存在原型代铁矿和金伯利岩的建议表示怀疑。不相容的微量元素比率(i)排除了克里希纳(Krishna)铅矿是直接羽流(软流层)地幔以及与俯冲有关的成分的产物,并且(ii)证明了它们的来源与同空间Cuddapah盆地的来源相似东部Dharwar克拉通的白云岩以及Wajrakarur和Narayanpet-金伯利岩。克里希纳红陨石的来源富集与全球地幔隆升时期有关,即〜1.9 Ga,其中包括Dharwar和Bastar克拉通(印度),Superior Craton(加拿大)进入了类似年龄和岩浆的大型火成岩省。 )和Kaapvaal克拉通(非洲南部)。我们发现,克里希纳斑岩的观测岩石学和地球化学特征可以最好地解释为:金矿+斜闪石+金红石+斜辉石+磷灰石+磷灰石+钛铁矿作为变质脉出现在枯竭的岩石圈地幔中,通过脉加壁-岩石模型来解释。石榴石稳定性场。我们的研究表明,岩石圈厚度及其伴随的交代作用在影响东达里克拉通的同空间中元古代红铁矿和金伯岩的成岩作用中具有重要作用。

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