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首页> 外文期刊>Geological Magazine >Caledonian terrane amalgamation of Svalbard: Detrital zircon provenance of mesoproterozoic to carboniferous strata from oscar II Land, western spitsbergen
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Caledonian terrane amalgamation of Svalbard: Detrital zircon provenance of mesoproterozoic to carboniferous strata from oscar II Land, western spitsbergen

机译:斯瓦尔巴群岛的古苏格兰地层合并:西斯匹次卑尔根奥斯卡二世地中元古代至石炭纪地层的碎屑锆石物源

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The tectonic origin of pre-Devonian rocks of Svalbard has long been a matter of debate. In particular, the origin and assemblage of pre-Devonian rocks of western Spitsbergen, including a blueschist-eclogite complex in Oscar II Land, are enigmatic. We present detrital zircon U-Pb LA-ICP-MS data from six Mesoproterozoic to Carboniferous samples and one U-Pb TIMS zircon age from an orthogneiss from Oscar II Land in order to discuss tectonic models for this region. Variable proportions of Palaeo- to Neoproterozoic detritus dominate the metasedimentary samples. The orthogneiss has an intrusion age of 927 ± 3 Ma. Comparison with detrital zircon age spectra from other units of similar depositional age within the North Atlantic region indicates that Oscar II Land experienced the following tectonic history: (1) the latest Mesoproterozoic sequence was part of a successor basin which originated close to the Grenvillian-Sveconorwegian orogen, and which was intruded by c. 980-920 Ma plutons; (2) the Neoproterozoic sediments were deposited in a large-scale basin which stretched along the Baltoscandian margin; (3) the eclogite-blueschist complex and the overlying Ordovician-Silurian sediments probably formed to the north of the Grampian/Taconian arc; (4) strike-slip movements assembled the western coast of Spitsbergen outside of, and prior to, the main Scandian collision; and (5) the remaining parts of Svalbard were assembled by strike-slip movements during the Devonian. Our study confirms previous models of complex Caledonian terrane amalgamation with contrasting tectonic histories for the different pre-Devonian terranes of Svalbard and particularly highlights the non-Laurentian origin of Oscar II Land.
机译:斯瓦尔巴特群岛前泥盆纪岩石的构造起源长期以来一直是一个争论的问题。尤其是,斯匹次卑尔根西部的前泥盆纪岩石的起源和组合,包括奥斯卡二世土地上的蓝片岩-榴辉岩复合体,都是令人费解的。我们提供了从6个中元古代到石炭纪样品的碎屑锆石U-Pb LA-ICP-MS数据,以及来自Oscar II Land的一条片麻岩的一个U-Pb TIMS锆石年龄,以讨论该地区的构造模型。古生代碎屑至新元古代碎屑的比例各异。直生片岩的侵入年龄为927±3 Ma。与北大西洋区域内其他具有相似沉积年龄的单元的碎屑锆石年龄谱进行比较表明,奥斯卡二世土地经历了以下构造历史:(1)最新的中元古代层序是一个后继盆地的一部分,该盆地起源于格伦维利安-斯韦科诺维格附近造山带,并被c。侵入。 980-920 Ma重子; (2)新元古代沉积物沉积在一个大型的盆地中,该盆地沿巴尔托斯堪的边缘伸展。 (3)榴辉岩-蓝胶岩复合体和上覆的奥陶纪-西陆纪沉积物可能形成于格兰屏/塔科尼亚弧的北部; (4)走滑运动将斯匹次卑尔根州的西海岸聚集在斯堪的纳维亚主要碰撞之前和之前。 (5)泥盆纪时期,斯瓦尔巴群岛的其余部分是通过走滑运动组装的。我们的研究证实了先前复杂的加里东地层合并模型,以及斯瓦尔巴德群岛德文阶前不同地块的构造历史形成对比,并特别强调了奥斯卡二世土地的非劳伦斯起源。

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