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首页> 外文期刊>International Geology Review >Geochemical characteristics and petrogenesis of four Palaeoproterozoic mafic dike swarms and associated large igneous provinces from the eastern Dharwar craton, India
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Geochemical characteristics and petrogenesis of four Palaeoproterozoic mafic dike swarms and associated large igneous provinces from the eastern Dharwar craton, India

机译:印度东部Dharwar克拉通的四个古元古代镁铁质堤防群和相关的火成岩大省的地球化学特征和岩石成因

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摘要

Palaeoproterozoic mafic dike swarms of different ages are well exposed in the eastern Dharwar craton of India. Available U-Pb mineral ages on these dikes indicate four discrete episodes, viz. (1) ~2.37Ga Bangalore swarm, (2) ~2.21Ga Kunigal swarm, (3) ~2.18Ga Mahbubnagar swarm, and (4) ~1.89Ga Bastar-Dharwar swarm. These are mostly sub-alkaline tholeiitic suites, with ~1.89Ga samples having a slightly higher concentration of high-field strength elements than other swarms with a similar MgO contents. Mg number (Mg#) in the four swarms suggest that the two older swarms were derived from primary mantle melts, whereas the two younger swarms were derived from slightly evolved mantle melt. Trace element petrogenetic models suggest that magmas of the ~2.37Ga swarm were generated within the spinel stability field by ~15-20% melting of a depleted mantle source, whereas magmas of the other three swarms may have been generated within the garnet stability field with percentage of melting lowering from the ~2.21Ga swarm (~25%), ~2.18Ga swarm (~15-20%), to ~1.89Ga swarm (~10-12%). These observations indicate that the melting depth increased with time for mafic dike magmas. Large igneous province (LIP) records of the eastern Dharwar craton are compared to those of similar mafic events observed from other shield areas. The Dharwar and the North Atlantic cratons were probably together at ~2.37Ga, although such an episode is not found in any other craton. The ~2.21Ga mafic magmatic event is reported from the Dharwar, Superior, North Atlantic, and Slave cratons, suggesting the presence of a supercontinent, 'Superia'. It is difficult to find any match for the ~2.18Ga mafic dikes of the eastern Dharwar craton, except in the Superior Province. The ~1.88-1.90Ga mafic magmatic event is reported from many different blocks, and therefore may not be very useful for supercontinent reconstructions.
机译:在印度东部的Dharwar克拉通中,不同年龄的古元古代镁铁质堤坝群暴露无遗。这些堤坝上可用的U-Pb矿物年龄表明四个不连续的事件,即。 (1)〜2.37Ga班加罗尔群,(2)〜2.21Ga Kunigal群,(3)〜2.18Ga Mahbubnagar群和(4)〜1.89Ga Bastar-Dharwar群。这些大部分是亚碱性的韧性套件,〜1.89Ga样品中的高场强元素浓度比其他具有类似MgO含量的群体略高。四个群中的Mg数(Mg#)表明,两个较旧的群是由原始地幔熔体衍生而来的,而两个较年轻的群是由略有演化的地幔熔体衍生的。微量元素成岩模型表明,〜2.37Ga群的岩浆是由贫化地幔源的约15-20%熔化在尖晶石稳定区内产生的,而其他三个群的岩浆可能是在石榴石稳定场内产生的。熔化百分比从〜2.21Ga群(〜25%),〜2.18Ga群(〜15-20%)降低到〜1.89Ga群(〜10-12%)。这些观察结果表明,铁镁质岩浆岩浆的熔融深度随时间增加。将东部Dharwar克拉通的大火成岩省(LIP)记录与从其他盾构地区观测到的类似黑手性事件进行了比较。 Dharwar和北大西洋的克拉通大概在〜2.37Ga处,尽管在任何其他克拉通中都没有发现这种情况。 Dharwar,Superior,北大西洋和奴隶克拉通报道了〜2.21Ga镁铁质岩浆事件,表明存在超大陆“ Superia”。除了上级省以外,很难找到东达哈克拉通的〜2.18Ga黑手党堤堤的任何匹配物。 〜1.88-1.90Ga镁铁质岩浆事件据报道来自许多不同的块体,因此对于超大陆重建可能不是很有用。

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