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首页> 外文期刊>Basin research >Testing long-term patterns of basin sedimentation by detrital zircon geochronology, Centralian Superbasin, Australia
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Testing long-term patterns of basin sedimentation by detrital zircon geochronology, Centralian Superbasin, Australia

机译:通过碎屑锆石年代学测试盆地沉积的长期模式,澳大利亚中部超级盆地

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Detrital zircon geochronology of Neoproterozoic to Devonian sedimentary rocks from the Georgina and Amadeus basins has been used to track changes in provenance that reflect the development and inversion of the former Australian Superbasin. Through much of the Neoproterozoic, sediments appear to have been predominantly derived from local sources in the Arunta and Musgrave inliers. Close similarities between the detrital age signatures of late Neoproterozoic sedimentary rocks in the two basins suggests that they were contiguous at this time. A dominant population of 1.2-1.0 Ga zircon in Early Cambrian sediments of the Amadeus Basin reflects the uplift of the Musgrave Inlier during the Petermann Orogeny between 560 and 520 Ma, which shed a large volume of detritus northwards into the Amadeus Basin. Early Cambrian sedimentary rocks in the Georgina Basin have a much smaller proportion of 1.2-1.0 Ga detritus, possibly due to the formation of sub-basins along the northern margin of the Amadeus Basin which might have acted as a barrier to sediment transfer. An influx of 0.6-0.5 Ga zircon towards the end of the Cambrian coincides with the transgression of the Larapintine Sea across central Australia, possibly as a result of intracratonic rifting. Detrital zircon age spectra of sedimentary rocks deposited within this epicontinental sea are very similar to those of coeval sedimentary rocks from the Pacific Gondwana margin, implying that sediment was transported into central Australia from the eastern continental margin. The remarkably consistent 'Pacific Gondwana' signature of Cambro-Ordovician sediments in central and eastern Australia reflects a distal source, possibly from east Antarctica or the East African Orogen. The peak of the marine incursion into central Australia in the early to mid Ordovician coincides with granulite-facies metamorphism at mid-crustal depths between the Amadeus and Georgina basins (the Larapinta Event). The presence of the epicontinental sea, the relative lack of a local basement zircon component in Cambro-Ordovician sedimentary rocks and their maturity suggest that metamorphism was not accompanied by mountain building, consistent with an extensional or transtensional setting for this tectonism. Sediments deposited at similar to 435-405 and similar to 365 Ma during the Alice Springs Orogeny have detrital age signatures similar to those of Cambro-Ordovician sedimentary rocks, reflecting uplift and reworking of the older succession into narrow foreland basins adjacent to the orogen.
机译:来自格奥尔基纳和阿玛迪斯盆地的新元古代至泥盆纪沉积岩的碎屑锆石年代学已被用来追踪物源的变化,这些变化反映了前澳大利亚超级盆地的发展和反演。在许多新元古代,沉积物似乎主要来自阿伦塔和穆斯格雷夫内陆地区的本地资源。两个盆地中新元古代晚期沉积岩的碎屑年龄特征之间的相似性相似,表明它们此时是连续的。阿玛迪斯盆地早期寒武纪沉积物中1.2-1.0 Ga锆石占主导地位,这反映了彼得曼造山运动在560-520 Ma期间Musgrave Inlier的隆升,这向北向阿玛迪斯盆地内注入了大量碎屑。乔治娜盆地早期的寒武纪沉积岩中碎屑占1.2-1.0 Ga的比例要小得多,这可能是由于在Amadeus盆地北缘沿亚盆地的形成,这可能成为沉积物转移的障碍。寒武纪末期涌入的0.6-0.5 Ga锆石与拉腊汀海跨澳大利亚中部的侵袭相吻合,可能是克拉通内裂谷的结果。沉积在这个大陆海中的沉积岩的碎屑锆石年龄谱与来自太平洋冈瓦纳太平洋边缘的同期沉积岩的谱非常相似,这意味着沉积物是从东部大陆边缘运到澳大利亚中部的。澳大利亚中部和东部Cambro-Ordovician沉积物的“太平洋冈瓦纳”特征非常一致,反映了一个远端源,可能来自南极东部或东非造山带。奥陶纪早期至中期,海洋侵入澳大利亚中部的高峰与Amadeus盆地和Georgina盆地之间的中地壳深度的花岗岩相变质相吻合(Larapinta事件)。上陆大陆海的存在,坎布罗-奥陶纪沉积岩中相对缺乏局部基底锆石成分以及它们的成熟度表明,变质作用并没有伴有高山造物,这与这种构造学上的伸展或伸展构造一致。在爱丽斯泉造山运动期间,沉积物沉积在类似于435-405且近似于365 Ma的沉积物上,其碎屑年龄特征与坎布罗-奥陶纪沉积岩的沉积特征相似,反映了较早的演替过程向邻近造山带的狭窄前陆盆地中隆升和返工。

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