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Tectonic controls on post-subduction granite genesis and emplacement: The late Caledonian suite of Britain and Ireland

机译:俯冲后花岗岩成因和构造的构造控制:英国和爱尔兰的晚喀里多尼亚时期

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摘要

Rates of magma emplacement commonly vary as a function of tectonic setting. The late Caledonian granites of Britain and Ireland are associated with closure of the Iapetus Ocean and were emplaced into a varying regime of transpression and transtension throughout the Silurian and into the early Devonian. Here we evaluate a new approach for examining how magma volumes vary as a function of tectonic setting. Available radiometric ages from the late Caledonian granites are used to calculate probability density functions (age spectra), with each pluton weighted by outcrop area as a proxy for its volume. These spectra confirm an absence of magmatic activity during Iapetus subduction between c. 455 Ma and 425 Ma and a dominance of post-subduction magmas between c. 425 Ma and 380 Ma. We review possible reasons why, despite the widespread outcrop of the late Caledonian granites, magmatism appears absent during Iapetus subduction. These include shallow angle subduction or extensive erosion and tectonic removal of the arc.\ud\udIn contrast to previous work, we find no strong difference in the age or major element chemistry of post-subduction granites across all terranes. We propose a common causal mechanism in which the down-going Iapetus oceanic slab peeled back and detached beneath the suture following final Iapetus closure. The lithospheric mantle was delaminated beneath the suture and for about 100 km back beneath the Avalonian margin. While magma generation is largely a function of gravitationally driven lithosphere delamination, strike slip dominated kinematics in the overlying continental crust is what modulated granitic magma emplacement. Early Devonian (419–404 Ma) transtension permitted large volumes of granite emplacement, whereas the subsequent Acadian (late Early Devonian, 404–394 Ma) transpression reduced and eventually suppressed magma emplacement.
机译:岩浆的沉积速率通常随构造背景而变化。英国和爱尔兰的晚喀里多尼亚花岗岩与伊帕图斯海的封闭有关,并在志留纪时期和泥盆纪早期进入了不同的压迫和变迁体系。在这里,我们评估了一种检查岩浆体积如何随构造环境变化的新方法。来自加里东晚期花岗岩的可用辐射年龄被用于计算概率密度函数(年龄谱),每个岩体均以露头面积加权作为其体积的代用品。这些光谱证实了在伊塔皮图斯俯冲过程中在c之间没有岩浆活动。 455 Ma和425 Ma以及俯冲后岩浆之间的优势c。 425马和380马。我们回顾了可能的原因,尽管晚喀里多尼亚花岗岩广泛露头,但伊帕特斯俯冲过程中似乎没有岩浆作用。这些包括浅角度俯冲或弧的大范围侵蚀和构造去除。与以前的工作相比,我们发现在所有地形中俯冲后花岗岩的年龄或主要元素化学性质均无明显差异。我们提出了一种常见的因果机制,其中,在最终的Iapetus闭合后,下降的Iapetus大洋板剥离并在缝合线下方脱离。岩石圈地幔在缝合线之下分层,并在阿瓦隆边缘之下回退约100公里。尽管岩浆的产生主要是重力驱动的岩石圈分层的作用,但上覆大陆壳中以走滑为主的运动学是调节花岗岩岩浆位置的原因。早期泥盆纪(419-404 Ma)的压变允许大量花岗岩的沉积,而随后的阿卡迪亚期(404-394 Ma的早期泥盆纪晚期)的压降减少并最终抑制了岩浆的沉积。

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