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Probing the composition of unexposed basement, South Portuguese Zone, southern Iberia: Implications for the connections between the Appalachian and Variscan orogens

机译:探索南伊比利亚南部葡萄牙地区未暴露的地下室组成:对阿巴拉契亚造山带和瓦里斯卡造山带之间联系的启示

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Geochemistry and Sm-Nd and U-Pb (magmatic zircon) isotope data from a postcollisional batholith that crosscuts the allochthonous South Portuguese Zone (SPZ) of southern Iberia suggest that the basement is compositionally more juvenile than the exposed upper crust. The SPZ is an allochthonous terrane of the late Paleozoic Variscan orogen. The oldest exposed units in the SPZ are Late Devonian continental clastics, and as a result, the origins of the SPZ are unknown. Multifaceted inherited zircon cores from a granitoid batholith (Sierra Norte Batholith, SNB) reveal Neoproterozoic (ca. 561- 647 Ma) and Mesoproterozoic ages (ca. 1075 - ca. 1116 Ma). Granitoid samples are characterized by εNd values ranging from +1.4 to -9.6 and model ages ca. 0.76-1.8 Ga. Conversely, the exposed Late Devonian clastics of the SPZ are characterized by more negative εNd values (-7.5 to -10.4). Taken together, U-Pb and Sm-Nd data indicate the lower crust that melted to yield the SNB was (i) Neoproterozoic (ca. 560-650 Ma) to Mesoproterozoic (ca. 1.0-1.2 Ga) in age, (ii) was not compositionally similar to the overlying Devono-Carboniferous continental detritus but was instead more juvenile, with model ages between ca. 0.9-1.2 Ga. This unusual relationship is similar to the relationship between the relatively juvenile basement and ancient upper crust documented in the exposed portion of the Meguma terrane in the northern Appalachians, which paleogeographic reconstructions show was immediately outboard of southern Iberia in the Late Devonian.
机译:地球化学以及来自碰撞后岩基的Sm-Nd和U-Pb(岩浆锆石)同位素数据横切了伊比利亚南部的异源南葡萄牙带(SPZ),表明该地下层的成分比裸露的上地壳更为幼稚。 SPZ是晚古生代Variscan造山带的异质地层。 SPZ中最古老的裸露单元是泥盆纪晚期大陆碎屑,因此SPZ的起源是未知的。花岗岩类岩基(Sierra Norte Batholith,SNB)的多面继承锆石岩心显示了新元古代(约561-647 Ma)和中元古代(约1075-约1116 Ma)。花岗岩样品的特征是εNd值介于+1.4到-9.6之间,模型年龄约为。相反,0.76-1.8Ga。SPZ暴露的晚泥盆纪碎屑岩的特征是εNd值更负(-7.5至-10.4)。两者合计,U-Pb和Sm-Nd数据表明,熔化生成SNB的下地壳年龄为(i)新元古代(约560-650 Ma)至中元古代(约1.0-1.2 Ga),(ii)在组成上与上覆的泥盆纪-石炭纪大陆碎屑并不相似,但更幼稚,模型年龄在大约。 0.9-1.2 Ga。这种不寻常的关系类似于阿巴拉契亚北部Meguma地表裸露部分记载的相对较幼稚的地下室与古代上地壳之间的关系,古地理重建表明,该区域立即位于泥盆纪晚期的伊比利亚南部外侧。

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