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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Linking collisional and accretionary orogens during Rodinia assembly and breakup: Implications for models of supercontinent cycles
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Linking collisional and accretionary orogens during Rodinia assembly and breakup: Implications for models of supercontinent cycles

机译:在Rodinia组装和分裂过程中链接碰撞和增生造山带:对超大陆周期模型的启示

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Periodic assembly and dispersal of continental fragments has been a characteristic of the solid Earth for much of its history. Geodynamic drivers of this cyclic activity are inferred to be either top-down processes related to near surface lithospheric stresses at plate boundaries or bottom-up processes related to mantle convection and, in particular, mantle plumes, or some combination of the two. Analysis of the geological history of Rodinian crustal blocks suggests that internal rifting and breakup of the supercontinent were linked to the initiation of subduction and development of accretionary orogens around its periphery. Thus, breakup was a top-down instigated process. The locus of convergence was initially around northeastern and northern Laurentia in the early Neoproterozoic before extending to outboard of Amazonia and Africa, including Avalonia-Cadomia, and arcs outboard of Siberia and eastern to northern Baltica in the mid-Neoproterozoic (similar to 760 Ma). The duration of subduction around the periphery of Rodinia coincides with the interval of lithospheric extension within the supercontinent, including the opening of the proto-Pacific at ca. 760 Ma and the commencement of rifting in east Laurentia. Final development of passive margin successions around Laurentia, Baltica and Siberia was not completed until the late Neoproterozoic to early Paleozoic (ca. 570-530 Ma), which corresponds with the termination of convergent plate interactions that gave rise to Gondwana and the consequent relocation of subduction zones to the periphery of this supercontinent. The temporal link between external subduction and internal extension suggests that breakup was initiated by a top-down process driven by accretionary tectonics along the periphery of the supercontinent. Plume-related magmatism may be present at specific times and in specific places during breakup but is not the prime driving force. Comparison of the Rodinia record of continental assembly and dispersal with that for Nuna, Gondwana and Pangea suggests grouping into two supercycles in which Nuna and Gondwana underwent only partial or no break-up phase prior to their incorporation into Rodinia and Pangea respectively. It was only after this final phase of assembly that the supercontinents then underwent full dispersal. (C) 2016 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
机译:大陆碎片的定期组装和散布是固体地球历史上的一大特征。推论这种循环活动的地球动力是与板块边界近地表岩石圈应力有关的自上而下的过程,或是与地幔对流,特别是与地幔柱有关的自下而上的过程,或两者的某种组合。对罗迪尼地壳块的地质历史的分析表明,超大陆的内部裂谷和破裂与周围俯冲的开始和增生造山带的发育有关。因此,分手是自上而下的激励过程。收敛的地点最初是在新元古代早期的东北和北部劳伦西亚附近,然后延伸到亚马孙地区和非洲的外围,包括阿瓦隆-卡多维亚,并在新生代中期(类似于760 Ma)延伸到西伯利亚外侧和波罗的海北部至北部。 。围绕罗迪尼亚外围的俯冲持续时间与超大陆内部岩石圈伸展的时间间隔相吻合,包括原始太平洋在1998年的开放。 760 Ma和东部Laurentia的裂谷开始。直到新元古代晚期至古生代早期(约570-530 Ma)之前,劳伦西亚,波罗的海和西伯利亚周围的被动边缘演替的最终开发才完成,这对应于会聚板块相互作用的终止,从而导致冈瓦纳和随后的重新定位。该超大陆外围的俯冲带。外部俯冲和内部扩展之间的时间联系表明,破裂是由超大陆外围增生构造驱动的自上而下的过程引发的。与羽状岩浆有关的岩浆作用可能在破裂过程中的特定时间和特定位置出现,但不是主要驱动力。 Rodinia与大陆纳努,冈瓦纳和Pangea的大陆集会和散布记录的比较表明,将努纳和冈瓦纳分成两个超级周期,其中纳纳和冈瓦纳分别进入罗迪尼亚和Pangea之前仅经历了部分或没有破碎阶段。只有在组装的最后阶段之后,超大陆才进行完全分散。 (C)2016作者。由Elsevier B.V.发布。这是CC BY许可下的开放获取文章(http://creativecommons.org/licenses/by/4.0/)。

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