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Paleogeography of the Congo/Sao Francisco craton at 1.5 Ga: Expanding the core of Nuna supercontinent

机译:1.5 Ga的刚果/圣弗朗西斯科克拉通古地理:扩展努纳超大陆的核心

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The Congo/Sao Francisco (C/SF) craton, one of the largest cratons in Proterozoic paleogeography, has been lacking reliable paleomagnetic data for the supercontinent Nuna interval (ca. 1600-1300 Ma). Here we provide a new paleomagnetic key pole for this craton from recently dated mafic dykes in the Curaca (1506.7 +/- 6.9 Ma) region of Brazil. The characteristic remanent magnetization (ChRM) direction D = 070.6 degrees, I = 54.0 degrees (k = 22.1 and a(95) = 13.1 degrees) corresponds with a paleomagnetic pole at 10.1 degrees N, 009.6 degrees E (K = 15.6, A(95) 15.8 degrees), which places C/SF craton in moderate paleolatitudes at the time of remanence acquisition. Primary nature of the paleomagnetic remanence is supported by a baked-contact test. A similar ChRM direction was obtained for four Mesoproterozoic mafic intrusions in Chapada Diamantina region. The new pole, only from Curaca, for C/SF allows us to reconstruct the extended core of the supercontinent Nuna at 1.5 Ga. Based on coeval 1.5 Ga and 1.38 Ga magmatism in Baltica, Siberia and C/SF, we favor the position where Southwest Congo is reconstructed against present South -Southeast (S-SE) Baltica. We explore two alternative 1.5 Ga reconstructions of Nuna's core. In both of them Baltica and Laurentia are shown in the well-defined NENA (Northern Europe North America) fit, together with Siberia in a tight fit to northern Laurentia. In reconstruction option A, more traditional fit of Amazonia with Baltica is shown, modified from the geologically based SAMBA (South AMerica BAltica) model to accommodate paleomagnetic data. In this option, however, West Africa must be extricated from SAMBA because C/SF has taken its place. For reconstruction option B, Amazonia is shifted to lie adjacent to NE Laurentia and West Baltica. In both options SW Congo is reconstructed against S-SE Baltica, but in option B there is a tighter fit between them, and there is a better match with our new paleomagnetic data for C/SF. In either option, separation of C/SF from Baltica and Siberia probably occurred at 1.38 Ga, the age of pronounced mafic magmatism throughout this sector of Nuna. (C) 2016 Elsevier B.V. All rights reserved.
机译:刚果/圣弗朗西斯科(C / SF)克拉通是元古代古地理中最大的克拉通之一,在超大陆Nuna区间(约1600-1300 Ma)一直缺乏可靠的古磁数据。在这里,我们从巴西库拉卡(1506.7 +/- 6.9毫安)地区新近出现的铁镁质岩堤为这个克拉通提供了一个新的古磁钥匙极。特征剩磁(ChRM)方向D = 070.6度,I = 54.0度(k = 22.1和a(95)= 13.1度)对应于在10.1度N,009.6度E(K = 15.6,A( 95)15.8度),在获得剩磁时将C / SF克拉通置于中古纬度。烘烤接触测试支持了古磁性剩磁的主要性质。 Chapada Diamantina地区的四个中元古代镁铁质侵入体获得了相似的ChRM方向。仅来自库拉卡(Curaca)的C / SF新极点使我们能够重建1.5 Ga的超大陆努纳的延伸核。基于波罗的海,西伯利亚和C / SF的同期1.5 Ga和1.38 Ga岩浆作用,我们倾向于以下位置相对于目前的东南(S-SE)波罗的海,重建了西南刚果。我们探索了努纳核心的两个备选1.5 Ga重建。波罗的海(Baltica)和劳伦蒂亚(Laurentia)均以明确的NENA(北欧北美)搭配,西伯利亚则与劳伦蒂亚北部紧密配合。在重建方案A中,显示了Amazonia与Baltica的更传统拟合,并从基于地质的SAMBA(南美洲BAltica)模型进行了修改,以适应古磁数据。但是,在这种选择下,因为C / SF已经取代了西非,所以必须从SAMBA中解脱出来。对于重建方案B,将Amazonia移至NE Laurentia和West Baltica附近。在这两个选项中,SW Congo都是针对S-SE Baltica重建的,但在选项B中,两者之间的拟合度更高,并且与我们针对C / SF的新古地磁数据更好地匹配。在这两种选择中,C / SF与波罗的海和西伯利亚的分离可能发生在1.38 Ga,这是整个努纳地区明显的铁镁质岩浆作用年龄。 (C)2016 Elsevier B.V.保留所有权利。

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