Scott A. Whattam , Robert J. Stern , Hossein Azizi , Keewook Yi , Haitham M. Baggazi , Abdullah Alquabalee , Fatemeh Nouri , Brian Jicha , Yanick Brice Lemdjou , Abdelhamid El Fakharani
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引用次数: 0
Abstract
The tectonic evolution of the Arabian-Nubian Shield began with formation of intra-oceanic arcs followed by collisions between these in Tonian-Cryogenian time and culminated in Ediacaran continental collision to form Gondwana. We provide new insights into the middle stage of this tectonic evolution by focusing on two Neoproterozoic dike swarms of different age in northern Arabia. The 695–700 Ma Za’am dikes were emplaced about the time of collision between the Midyan and Hijaz terranes whereas the 635 Ma Bayda dikes were emplaced ∼ 60 million years after collision. These record a shift from relatively unfractionated 695 Ma arc-type magmas in the south to fractionated 635 Ma within-plate alkaline magmas in the north. Our results document mantle source and crustal evolution beneath the Midyan terrane during and after terrane accretion, revealing a tectono-magmatic transition from SSZ-type magmas accompanying arc collision to post-terrane accretion within-plate magmatism through Cryogenian time. In addition, our results confirm the potential of dike studies for reconstructing the tectono-magmatic-metallogenic evolution of orogens.
阿拉伯地盾西北部米迪安地层南部新近新生代岩脉记录的 635 Ma 时弧状岩浆活动向板块内岩浆活动的转变
阿拉伯-努比亚地盾的构造演化始于洋内弧的形成,随后在托尼-新生代发生碰撞,最终在埃迪卡拉纪发生大陆碰撞形成冈瓦纳。我们通过重点研究阿拉伯北部两个不同时代的新新生代堤坝群,对这一构造演化的中期阶段有了新的认识。695-700Ma的Za'am堤群约在米迪扬地块和希贾兹地块碰撞时形成,而635Ma的Bayda堤群则在碰撞后6000万年左右形成。这些岩浆记录了从南部相对未分馏的 695 Ma 弧型岩浆到北部分馏的 635 Ma 板块内碱性岩浆的转变。我们的研究结果记录了地台增生过程中和增生后米德兰地台下方的地幔源和地壳演化,揭示了从伴随弧形碰撞的SSZ型岩浆到地台增生后的板内岩浆活动的构造-岩浆过渡,一直持续到冷元古代。此外,我们的研究结果证实了堤坝研究在重建造山构造-岩浆-成矿演化方面的潜力。
期刊介绍:
Precambrian Research publishes studies on all aspects of the early stages of the composition, structure and evolution of the Earth and its planetary neighbours. With a focus on process-oriented and comparative studies, it covers, but is not restricted to, subjects such as:
(1) Chemical, biological, biochemical and cosmochemical evolution; the origin of life; the evolution of the oceans and atmosphere; the early fossil record; palaeobiology;
(2) Geochronology and isotope and elemental geochemistry;
(3) Precambrian mineral deposits;
(4) Geophysical aspects of the early Earth and Precambrian terrains;
(5) Nature, formation and evolution of the Precambrian lithosphere and mantle including magmatic, depositional, metamorphic and tectonic processes.
In addition, the editors particularly welcome integrated process-oriented studies that involve a combination of the above fields and comparative studies that demonstrate the effect of Precambrian evolution on Phanerozoic earth system processes.
Regional and localised studies of Precambrian phenomena are considered appropriate only when the detail and quality allow illustration of a wider process, or when significant gaps in basic knowledge of a particular area can be filled.