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首页> 外文期刊>International Geology Review >Geodynamics of the Amirante Ridge and Trench Complex, Western Indian Ocean
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Geodynamics of the Amirante Ridge and Trench Complex, Western Indian Ocean

机译:西印度洋阿米兰特岭和海沟复合体的地球动力学

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摘要

The formation and evolution of the ~600 km long arcuate Amirante Ridge and Trench Complex (ARTC) is a significant geo-morphic-structural feature in the Western Indian Ocean (WIO). The WIO contains evidence of at least two major magmatic episodes followed by continental rifting within the span of a little more than 20 million years. This involved the splitting of Madagascar from India at around 85 Ma and then separation between India and the Seychelles at 64-63 Ma as a possible consequence of two powerful volcanic eruptions from the Marion and Reunion hot spots, respectively. Formation and evolution of the ARTC represents this tumultuous period in the Indian Ocean, approximately between 85 and 60 Ma (Late Cretaceous-Early Tertiary). We integrated geophysical, palaeomagnetical, and petrological data to examine three existing models that attempt to explain the formation of ARTC. In contrast, our study hints at several stages of extension and compression responsible for its formation. Our integrated data also suggest that the Carlsberg Ridge may have played a prominent role in the evolution of the ARTC that seems to have formed through a ridge-jump process after the conjugate spreading centres - Mascarene and Palitana ridges formed earlier during the India-Madagascar separation - ceased spreading because of violent eruption of the Reunion hot spot at around 65 Ma. The eruption disturbed the plumbing system of magma ascent, resulting in cessation of spreading along the conjugate spreading centres, forcing a ridge jump.A collage of seismic refraction and reflection, free-air gravity, magnetic anomaly data, and Ar dating of rocks indicates that as the Carlsberg Ridge swept the Seychelles towards south, the crust between Madagascar and the Seychelles was increasingly compressed, with the abandoned northern Mascarene spreading centre absorbing the maximum stress. With continued compression, the western limb of the abandoned spreading ridge was thrust below the eastern limb to a limited degree. This partial subduction agrees with the gravity and seismic results. Our new study also accounts for the anomalous presence of 14 km-thick oceanic crust beneath the ARTC and its characteristic difference in petrology with other established subduction zones in the world.
机译:约600公里长的弓形阿米兰特山脊和海沟复合体(ARTC)的形成和演化是西印度洋(WIO)的重要地貌构造特征。 WIO包含至少两千万年间至少两次主要岩浆事件和大陆裂谷的证据。这涉及到马达加斯加从印度约85 Ma分裂,然后在印度和塞舌尔群岛之间以64-63 Ma分开,这可能是由于分别从马里恩(Marion)和留尼汪(Reunion)热点两次强烈喷发造成的。 ARTC的形成和演化代表了印度洋这个动荡的时期,大约在85至60 Ma(晚白垩世-早第三纪)之间。我们整合了地球物理,古地磁和岩石学数据,以检验试图解释ARTC形成的三个现有模型。相比之下,我们的研究暗示了延伸和压缩的几个阶段。我们的综合数据还表明,卡尔斯伯格山脊可能在ARTC的演化中发挥了重要作用,该过程似乎是在共轭扩散中心(印度-马达加斯加分离初期形成的玛斯卡林和帕利塔纳山脊)之后通过脊跃过程形成的-由于留尼汪岛热点在65 Ma左右爆发而停止传播。火山喷发扰乱了岩浆上升的管道系统,导致沿共轭扩散中心的扩散停止,迫使山脊跳跃。地震折射和反射,自由空气重力,磁异常数据和岩石的Ar定年拼贴表明:随着嘉士伯山脊向南席卷塞舌尔,马达加斯加和塞舌尔之间的地壳越来越受挤压,废弃的北部玛斯卡林扩散中心吸收了最大的应力。随着不断的压缩,废弃的蔓延脊的西肢被有限程度地推入东肢之下。这种部分俯冲与重力和地震结果一致。我们的新研究还解释了ARTC下方14 km厚的洋壳异常存在,以及其与世界上其他已确定的俯冲带的岩石学特征差异。

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