首页> 外文期刊>Precambrian Research >Precambrian mafic dyke swarms in the Singhbhum craton (eastern India) and their links with dyke swarms of the eastern Dharwar craton (southern Cheek tot updates India)
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Precambrian mafic dyke swarms in the Singhbhum craton (eastern India) and their links with dyke swarms of the eastern Dharwar craton (southern Cheek tot updates India)

机译:Precambrian Mafic Dyke在Singhbhum Craton(印度东部)及其与东部Dharwar Craton的堤坝(南方脸颊Tot更新印度)的联系

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Based on trend, cross-cutting relationships and U-Pb dating, Precambrian mafic dykes in the Singhbhum craton, earlier collectively identified as 'Newer Dolerite Swarm', have been separated into seven distinct swarms, which are thought to be the plumbing systems for Large Igneous Provinces (LIPs). These Singhbhum swarms range in age from similar to 2.80 Ga to similar to 1.76 Ga, and include the similar to 2.80 Ga NE-SW trending Keshargaria swarm, similar to 2.75-2.76 Ga NNE-SSW to NE-SW trending Ghatgaon swarm, the similar to 2.26 Ga NE-SW to ENE-WSW trending Kaptipada swarm (based on a new U-Pb ID-TIMS age 2256 +/- 6 Ma), the similar to 1.77 Ga WNW-ESE trending Pipilia swarm, the earlyPaleoproterozoic E-W to ENE-WSW trending Keonjhar swarm, the middle-Paleoproterozoic NW-SE to NNW-SSE trending Bhagamunda swarm, and the late-Paleoproterozoic N-S to NNE-SSW trending Barigaon swarm. Two of the Singhbhum swarms, the similar to 2.26 Ga Kaptipada and 1.77 Ga Pipilia, are closely matched with the similar to 2.26-2.25 Ga Ippaguda-Dhiburahalli and similar to 1.79 Ga Pebbair swarms, respectively, of the eastern Dharwar craton. The correlations suggest that the Singhbhum and Dharwar cratons were close enough at these times to share two reconstructed LIPs, a 2.26-2.25 Ga Kaptipada Ippaguda-Dhiburahalli LIP and a 1.79-1.77 Ga PipiliaPebbair LIP, and if so, both swarms must be present in the intervening Bastar craton (candidates are proposed). Also, the 2.76-2.75 Ga Ghatgaon swarm of the Singhbhum craton can be provisionally correlated with 2.7 Ga Keshkal swarm of the Bastar craton. The 2.26-2.25 Ga Kaptipada Ippaguda-Dhiburahalli LIP of the SinghbhumBastar-Dharwar reconstruction has age matches in the Vestfold Hills of Antarctica (similar to 2.24 Ga dykes), the Kaapvaal craton (the similar to 2.25-2.23 Ga Hekpoort lavas) and perhaps the Zimbabwe craton (2.26 Ga Chimbadzi troctolite intrusions). The 1.76-1.79 Ga Pipilia-Pebbair LIP of the Singhbhum-Bastar-Dharwar reconstruction h
机译:基于趋势,跨领域关系和U-PB约会,Precambrian Mafic Dykes在Singhbhum Craton中,早些时候将被统称为“较新的Dolerite Swarm”,已被分成七个不同的群体,这被认为是大型管道系统火耳塞省(嘴唇)。这些Singhbhum群的年龄群从类似于2.80 Ga与1.76 Ga类似,并包括类似于2.80 Ga Ne-SW趋势Keshargaria Swarm,类似于2.75-2.76 Ga Nne-SSW到Ne-SW Trending Ghatgaon Sharm,类似到2.26 Ga Ne-SW到Ene-WSW Trending Kaptipada Swarm(基于新的U-PB ID-Tims 2256 +/- 6 mA),类似于1.77 Ga Wnw-ESE Pipilia Sharm,早期的BaleoProteroZoice ew to Ene -wsw ring keonjhar swarm,中古普罗佐尼的nw-se to nnw-sse趋势bhagamunda sharm,以及古地区古代Ns到Nne-SSW Trending Barigaon Swarm。两个Singhbhum Sharms,类似于2.26 Ga Kaptipada和1.77的Ga Pipilia,与2.26-2.25 Ga Ippaguda-dibulahalli相似,与东部Dharwar Craton东部的1.79 Ga Pebbair群。相关性表明,Singhbhum和Dharwar Cratons在这些时间上足够接近,分享两个重建的嘴唇,一个2.26-2.25 Ga Kaptipada Ippaguda-diburahalli嘴唇和1.79-1.77 Ga Pipiliapebair嘴唇,如果是这样,这两种群体都必须出现介入巴斯塔尔·克拉顿(提出候选人)。此外,Singhbhum Craton的2.76-2.75 Ga Ga Gahatgaon Swarm可以与Bastar Craton的2.7 Ga Keshkal Sharm临时相关。 2.26-25 Ga Kaptipada Ippaguda-diburahalli歌曲的Singhbhumbastar-Dharwar重建在南极洲Vestfold山(类似于2.24 GA Dykes),Kaapvaal Craton(类似于2.25-2.23 Ga Hekpoort Lavas),也许是津巴布韦克拉顿(2.26 Ga Chimbadzi Trocolite Intrings)。 1.76-1.79 GA Pipilia-Pebbair唇部的Singhbhum-Bastar-Dharwar重建H.

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