Did subduction in the western Mediterranean drive Neogene alpine dynamics? Insights from analogue modeling

J. Martinod, Ayend-Christ Daou, Laurent Métral, Christian Sue
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Abstract

We present analogue models simulating the Neogene subduction that occurred in the Western Mediterranean region, in order to understand how it impacted the regional tectonics. Although models do not include the lithospheric plate overriding the subduction zone, their surface deformations share many similarities with the Neogene tectonics of Western Europe and Iberia. We observe that the tectonic evolution is largely controlled by the roll-back of the slab, that occurred much faster than the Africa-Eurasia convergence. Models reproduce the opening of the Western Mediterranean Basins and the dispersion of the AlKaPeCa continental fragments. They also show that oceanic subduction favors the counterclockwise rotation of Adria. In more elaborated models, we introduced a pre-existing weakness along the Africa and Adria margins, to reproduce the break-off of the oceanic slab that followed the beginning of continental subduction both in Northern Africa and Italia. Slab break-off is followed by the exhumation of the subducted continent. We observe that the influence of subduction on the kinematics of Adria largely decreases following slab break-off. In models, the total counterclockwise rotation of Adria varies between 7° and more than 30°, depending on the timing of slab break-off. Since the process of subduction modifies the displacement of Adria, it also impacts the tectonic evolution of the regions that bound this plate, especially in the Alpine belt: in the Western Alps, an older Late Cretaceous to Eocene “Pyrenean-Provençal” tectonic phase accommodating N-S shortening is classically described resulting from the convergence between Africa and Eurasia. It is followed by the Neogene “Alpine phase” accommodating E-W shortening. Since this major tectonic change is not explained by a modification of the global Africa-Eurasia convergence, it should be explained instead by more local causes. Our models show that during slab-roll back and before slab break-off, the azimuth of convergence between Adria and Europe shifts from ~N-S to ~ENE-WSW. Hence, they suggest that the oceanic subduction in the Western Mediterranean may explain the “Oligocene revolution” described by Dumont et al. (2011), leading to E-W shortening in the Western Alps and to the activation of the Periadriatic right-lateral shear zones in the Central Alps. We conclude that the western Mediterranean region is a spectacular example showing how the tectonics of mountain ranges and plate boundaries may be controlled by distant subduction processes.
地中海西部的俯冲是否驱动了新纪高山动力学?模拟模型的启示
我们提出了模拟发生在西地中海地区的新近纪俯冲的模拟模型,以了解它是如何影响区域构造的。虽然模型不包括俯冲带上方的岩石圈板块,但其地表变形与西欧和伊比利亚的新近纪构造有许多相似之处。我们观察到,构造演化在很大程度上受板块后退的控制,而板块后退的速度远远快于非洲-欧亚大陆辐合的速度。模型再现了西地中海盆地的打开和 AlKaPeCa 大陆碎片的分散。模型还显示,大洋俯冲有利于阿德里亚的逆时针旋转。在更详尽的模型中,我们沿非洲和阿德里亚边缘引入了一个预先存在的薄弱环节,以再现北非和意大利大陆俯冲开始后大洋板块的断裂。板块断裂之后是俯冲大陆的掘起。我们观察到,板块断裂后,俯冲对阿德里亚运动学的影响在很大程度上减弱了。在模型中,根据板块断裂的时间,阿德里亚的总逆时针旋转角度在7°到30°之间变化。由于俯冲过程改变了阿德里亚板块的位移,因此也影响了与该板块相联系地区的构造演化,尤其是阿尔卑斯山带:在西阿尔卑斯山,人们通常描述了一个较早的晚白垩世至始新世 "比利牛斯-普罗旺斯 "构造阶段,该阶段因非洲和欧亚大陆的汇聚而导致南北向缩短。随后是新近纪的 "阿尔卑斯山阶段",它是东西向的缩短。由于这一重大构造变化无法用全球非洲-欧亚大陆辐合的改变来解释,因此应该用更多的局部原因来解释。我们的模型显示,在板块回滚期间和板块断裂之前,阿德里亚和欧洲之间的辐合方位角从 ~N-S 转向 ~ENE-WSW。 因此,这些模型表明,地中海西部的大洋俯冲可以解释 Dumont 等人(2011 年)所描述的 "渐新世革命",导致西阿尔卑斯山的东西向缩短和中阿尔卑斯山的 Periadriatic 右侧剪切带的激活。我们的结论是,地中海西部地区是一个壮观的例子,显示了山脉和板块边界的构造是如何受遥远的俯冲过程控制的。
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