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首页> 外文期刊>Doklady Earth Sciences >Late Riphean Rifting and Breakup of Laurasia: Data on Geochronological Studies of Ultramafic Alkaline Complexes in the Southern Framing of the Siberian Craton
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Late Riphean Rifting and Breakup of Laurasia: Data on Geochronological Studies of Ultramafic Alkaline Complexes in the Southern Framing of the Siberian Craton

机译:里菲亚晚期裂谷和劳拉西亚破裂:西伯利亚克拉通南部框架中超镁铁质碱性复合物的年代学研究数据

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The origin of the Paleo-Asian Ocean and consequent formation of the Central Asian foldbelt (CAFB), which represents the largest structure of Asia and borders the Siberian Craton in the south and southwest, is one of the key problems in the geology of Asia. The CAFB is composed of Caledonian, Hercynian, and Indo-Sinian folded structures, suggesting that the pale-ocean began to form not later than 570 Ma ago (the age of the oldest ophiolites in the CAFB Caledonides). The origin of the paleocean, i.e., its oldest age, is closely related to the breakup of the supercontinent Rodinia. The southern margin (in modern coordinates) of Siberia, a constituent of this supercontinent, adjoined Laurentia and formed the giant Laurasian continental block together with Baltia and Greenland. Previously, we attempted to estimate the age of the Laurasia breakup and the time at which oceanic basins began to surround the Siberian continent. This estimate was based, first of all, on the age of rifting between Siberia and the North Canadian part of Laurentia. Processes of rifting are best reflected in structures of the giant Franklin dike belt that formed 725-615 Ma ago with the maximal activity between 723 and 718 Ma ago. In the Siberian Craton, the breakup is reflected in numerous manifestations of Late Riphean intraplate activity (grabens, dike belts, carbonatite-bearing ultramafic alkaline massifs, and others). The age of these events, usually based on the K-Ar method, has appeared to be rather ambiguous because of the substantial variations in obtained dates. We carried out more reliable U-Pb geochronological measurements in carbonatite-bearing alkaline massifs distributed along the southern margin of the Siberian Craton. The data obtained make it possible to specify the age and geological consequences of the rifting that resulted in the breakup of Laurasia and formation of the Paleo-Asian ocean.
机译:古亚洲海洋的起源以及随之而来的中亚褶皱带(CAFB)的形成是亚洲地质学中的关键问题之一,它代表了亚洲最大的结构,与西伯利亚克拉通接壤,在南部和西南部。 CAFB由加里东,海西和印度-Sinian褶皱构造组成,表明该古海洋开始形成的时间不早于570 Ma以前(CAFB加里多尼德斯最古老的蛇绿岩年龄)。古海洋的起源,即最古老的年龄,与超大陆罗丹尼亚的破裂密切相关。西伯利亚的南缘(以现代坐标表示)是该超级大陆的组成部分,毗邻劳伦西亚(Laurentia),与巴尔蒂亚(Baltia)和格陵兰(Greenland)一起形成了巨大的劳拉西亚大陆块。以前,我们试图估计劳拉西亚解体的年龄以及洋盆开始围绕西伯利亚大陆的时间。首先,这一估计是基于西伯利亚和Laurentia的北加拿大部分之间的裂谷年龄。裂谷的过程最好反映在725-615 Ma以前的富兰克林堤防地带的结构中,最大活动在723和718 Ma以前。在西伯利亚克拉通中,破裂作用反映在晚里弗期板内活动的多种表现形式(岩钉,堤防带,含碳酸盐的超镁铁质碱性地块等)中。这些事件的年龄通常基于K-Ar方法,由于获得的日期存在很大差异,因此似乎模棱两可。我们对沿西伯利亚克拉通南缘分布的含碳酸盐岩质碱块进行了更可靠的U-Pb地质年代学测量。所获得的数据使人们能够确定裂谷的年龄和地质后果,该裂谷导致了劳拉西亚破裂和古亚洲洋的形成。

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