印度东部Rajmahal圈闭的古地磁和地球化学特征

G.V.S. Poornachandra Rao, J. Mallikharjuna Rao, M.V. Subba Rao
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引用次数: 7

摘要

早白垩世(117±1 Ma)的Rajmahal圈闭是石英拉斑玄武岩成分的中/细粒岩石。玄武岩中的斜长石斑晶显示出从An53到An68的成分分区,而基质斜长石的成分范围从An50到An58。斜辉石斑晶的组成范围为En46–48Wo35–39Fs14–19,而基质斜辉石的组成范围则为En32–46Wo33–37Fs18–34。钛磁铁矿以小斑点、棱柱状颗粒和细长针状物的形式出现。次生矿物包括取代基质斜长石和辉石的蒙脱石-绿泥石,这表明玄武岩在侵位后经历了热液蚀变。主要元素、微量元素和稀土元素数据表明玄武岩有两个不同的类别;I族,以高MgO、K2O、Sr、Rb、Cr、Ba和Nb为特征;和第II族,其特征在于高Fe2O3、TiO2和稀土元素含量。这两个玄武岩群似乎都是由同一地幔源的熔融形成的。从三个地点采集的Rajmahal玄武岩在其自然剩余磁矢量中显示出非常好的分组,具有正极性和反极性。这些岩石的详细AF和热消磁处理揭示了所有三个地点的特征成分。位点A和B表现出正磁化,位点C同时表现出正磁和反磁。这些结果与冈瓦纳大陆东部裂解期间广泛玄武岩岩浆作用的模型有关,得到了严格的评估。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Palaeomagnetic and geochemical characteristics of the Rajmahal Traps, eastern India

The Rajmahal Traps of Early Cretaceous age (117 ± 1 Ma) are medium/fine-grained rocks of quartz-tholeiitic composition. Plagioclase phenocrysts in the basalts show compositional zoning from An53 to An68, whereas groundmass plagioclase compositions range from An50 to An58. Clinopyroxene phenocrysts range in composition from En46–48Wo35–39Fs14–19, with groundmass clinopyroxene compositions in the range En32–46Wo33–37Fs18–34. Titanomagnetite occurs as small specks, prismatic grains and elongate needles. Secondary minerals include smectite-chlorite replacing groundmass plagioclase and augite, suggesting that the basalts have undergone hydrothermal alteration subsequent to their emplacement. Major, trace and rare-earth element data suggest two distinct catergories of basalts; Group I, characterised by high MgO, K2O, Sr, Rb, Cr, Ba and Nb; and Group II, characterised by high Fe2O3, TiO2 and rare-earth element contents. Both basalt groups appear to have been derived by melting of the same mantle source. Rajmahal basalts collected from three sites show very good grouping in their natural remanent magnetic vectors, with normal and reverce polarities. Detailed AF and thermal demagnetisation treatment of these rocks reveals characteristic components at all three sites. Sites A and B exhibit normal magnetisation, and site C exhibits both normal and reverse magnetisations. These results are critically evaluated in relation to models for widespread basaltic magmatism during the break-up of eastern Gondwana.

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