Ab'/> U–Pb detrital zircon ages from the Paleozoic Marbella Conglomerate of the Malaguide Complex (Betic Cordilleras, Spain). Implications on Paleotethyan evolution
首页> 外文期刊>Lithos: An International Journal of Mineralogy, Petrology, and Geochemistry >U–Pb detrital zircon ages from the Paleozoic Marbella Conglomerate of the Malaguide Complex (Betic Cordilleras, Spain). Implications on Paleotethyan evolution
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U–Pb detrital zircon ages from the Paleozoic Marbella Conglomerate of the Malaguide Complex (Betic Cordilleras, Spain). Implications on Paleotethyan evolution

机译:u-pb滴乳锆石来自古生代马尔贝拉集团的马尔制氨酸综合体(Betickindillas,西班牙)。 对古石山的影响

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AbstractThe Marbella Conglomerate (Betic Cordilleras, SW Spain) is a poorly sorted and polymictic rock of vaguely constrained Late Carboniferous age interlayered within a sandy sequence. It contains variable amounts of pebbles of quartzite, gneiss, deformed granitoid, schist, aplite, dacite and other volcanic rocks among others, which makes it a potential target for detrital zircon provenance studies. In order to decipher provenance we combined U–Pb SHRIMP and LA–ICP-MS analyses on zircons obtained from single pebbles of deformed rocks (schist, granitoids) and detrital zircons from the sandy sequence, respectively. The age spectra of the detrital zircons indicates that at least the sedimentation took place soon after the start of the Permian according to the youngest detrital zircon age (≈286Ma), and it involved the denudation of terranes with rocks bearing Paleoproterozoic, Neoproterozoic, Cambro-Ordovician, Devonian and Carboniferous zircon age clusters. In contrast with the Permian age of the detrital zircons from the sandstones, igneous (ca.532 and 516Ma) and metamorphic (ca.356Ma) U–Pb SHRIMP Concordia ages were obtained from the pebbles. The different age clusters observed could be correlated to igneous, metamorphic and detrital rocks from an already eroded terrane similar to the Ossa-Morena Zone of the Iberian Variscan Belt. Therefore, we propose that most of the sedimentation of the Marbella Conglomerate took place along the western border of the Paleotethys at the north margin of Gondwana during the dismantling of the Variscan orogenic edifice and/or the Neotethys ocean opening and the birth of the Cimmerian ribbon continent.Graphical abstractDisplay OmittedHighlights?Provenance from a Cadomian terrane is deduced for the Marbella Conglomerate.?The basin was likely filled mainly with sediments provided by the Ossa-Morena Zone.?The sedimentation took place along the western border of the Paleotethys.?A maximum age of ≈286Ma is inferred for the deposition.]]>
机译:<![cdata [ 抽象 Marbella Conglomerate(Betic Cordilleras,SW Spain)是一种含糊不限约束的后期石炭系的含量差的和金属岩石在沙质序列内夹层。它含有可变量的石英岩,片状,变形的花岗岩,分泌物,消费件,达卡酮和其他火山岩等,这使其成为替代锆石种源研究的潜在目标。为了破译来源,我们将U-Pb虾和La-ICP-MS分析在含有沙质序列的单粒岩石(Schist,Granitoids)和碎屑锆石中获得的锆石分析。碎屑锆石的年龄谱表明,根据最小的替代锆石(≈286MA),在二叠纪开始后,至少沉淀得很快就会发生,并且涉及岩石岩石,古普罗佐,新蛋白古代,寒武纪,Cambro- Ordovician,Demonian和石炭系锆石年龄集群。与砂岩碎屑锆的二叠纪年龄相比,火耳塞( ca. 532和516mA)和变质( ca. 356ma )从鹅卵石中获得U-Pb虾Concordia年龄。观察到的不同年龄集群可能与来自已经侵蚀的地区的火岩,变质和碎屑岩体相关联,类似于伊比利亚·瓦森骑士的Ossa-Morena区。因此,我们建议马尔贝拉集团的大部分沉降在拆除了大景的orenatenic大厦和/或海洋开放和Cimmerian缎带的诞生期间在Gondwana的北边缘的西部地区沿着Gondwana的北边缘进行了沉积物。大陆。 图形摘要 显示省略 亮点 为马尔贝拉集团推导出来。 ?< / ce:标签> 盆地可能主要填充OSSA-MOREA区域提供的沉积物。 沉淀在古本边界的西部边界沿袭。 沉积的最大年龄为≈286mA。 ]]>

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