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Palaeoproterozoic accretion processes of Australia and comparisons with Laurentia

机译:澳大利亚古元古代的增生过程及其与劳伦西亚的比较

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The Palaeoproterozoic rocks of Australia and Laurentia preserve an excellent record of the accretionary tectonics associated with transitions between the Columbia (Nuna) and Rodinia supercontinents. The geologic records of Australia and Laurentia suggest that the dominant tectonic driver was one or more subduction zones in which several episodes of crustal accretion occurred between ca. 1790 Ma and 1620 Ma. Correlated orogenic events include the ca. 1800–1780 Ma Yapungku–Yambah (Australia)–Medicine Bow (Laurentia) orogenies, ca. 1740–1690 Ma Strangways–Kimban (Australia)–Nimrod (Antarctica)–Yavapai (Laurentia) orogenies, and the ca. 1650–1620 Ma Leibig–Ooldea (Australia)–Mazatzal (Laurentia) orogenies. There are major differences in the style of accretion: Laurentia is characterized by accretion of dominantly juvenile arc terranes, whereas accreted Australian terranes are more evolved and are isotopically similar to the continental nucleus. Adjacent to its plate margin, the Australian continent contained regions of elevated heat production compared with the Laurentian margin. Brace-Goetze lithospheric strength models for ca. 1700 Ma indicate that the Australian plate margin was significantly weaker than that of Laurentia. This variation in lithospheric strength is interpreted to impact the behaviour of the overriding plate during subduction roll back. Attenuation of the Australian lithosphere during ductile extension caused rifting of large continental fragments from the plate margin. Their subsequent accretion resulted in the re-amalgamation of pre-existing continental lithosphere similar to the lithosphere in the overriding plate. Subduction roll back adjacent to the cold and rigid Laurentian margin (e.g. the Wyoming Craton) had relatively little impact on the overriding plate, with oceanic back-arc basins and juvenile arc terranes developing outboard of the plate margin. Inversion of these arc and oceanic back-arc terranes resulted in episodic continental growth.
机译:澳大利亚和Laurentia的古元古代岩石保存了与哥伦比亚(努纳)和罗迪尼亚超大陆之间的过渡有关的增生构造的优良记录。澳大利亚和劳伦西亚的地质记录表明,主要的构造动因是一个或多个俯冲带,在这些俯冲带之间约有数次地壳增生发生。 1790年和1620年。相关的造山事件包括大约在1800年至1780年之间的Ma Yapungku-Yambah(澳大利亚)-Medicine Bow(Laurentia)造山带。 1740–1690年Ma Strangways–Kimban(澳大利亚)–Nimrod(南极洲)–Yavapai(Laurentia)造山运动,以及约1650–1620年马雷比格–奥尔德亚(澳大利亚)–马萨兹尔(劳伦西亚)造山运动。增生方式存在主要差异:Laurentia的特征是主要为幼年弧形弧面增生,而增生的澳大利亚地貌则演化得更多,并且在同位素上与大陆核相似。与板块边缘相邻,与劳伦边缘相比,澳大利亚大陆的热量产生区域较高。 Brace-Goetze岩石圈强度模型约。 1700 Ma指示澳大利亚板块余量明显低于Laurentia。岩石圈强度的这种变化被解释为在俯冲回滚期间影响上覆板的行为。延性伸展过程中澳大利亚岩石圈的衰减导致板块边缘的大块大陆碎裂。他们随后的增生导致先前存在的大陆岩石圈重新融合,类似于上覆板块的岩石圈。俯冲在冷而刚性的劳伦山脉边缘(如怀俄明州克拉顿)附近回滚,对上覆板块的影响相对较小,在板块边缘外侧发育了海洋背弧盆地和幼年弧面。这些弧形和海洋弧形地表的倒转导致了大陆的间歇性生长。

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