首页> 外文期刊>GSA Bulletin >Provenance, detrital zircon U-Pb geochronometry, and tectonic significance of Permian to Lower Triassic sandstone in southeastern Quesnellia, British Columbia and Washington
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Provenance, detrital zircon U-Pb geochronometry, and tectonic significance of Permian to Lower Triassic sandstone in southeastern Quesnellia, British Columbia and Washington

机译:昆士兰州东南部,不列颠哥伦比亚省和华盛顿州的二叠系至下三叠统砂岩的物源,碎屑锆石U-Pb年代学和构造意义

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摘要

U-Pb ages of Permian detrital zircons within eastern Quesnellia are similar to ages of western and southwestern Laurentian basement provinces, suggesting sedimentologic ties between the Quesnellian arc terrane and the Laurentian continental margin. The Permian to Lower Triassic Mount Roberts Formation forms the easternmost exposures of the Harper Ranch subterrane of Quesnellia. The formation consists of interbedded lithic graywacke, argillite, limestone, and volcanic rocks deposited within an ensimatic arc environment. Petrology of Mount Roberts Formation sandstones indicate derivation from lithologically diverse sources that consisted predominantly of volcanic rocks but also included significant amounts of sedimentary, metamorphic, and plutonic rocks. U-Pb ages of 27 individual detrital zircons from a single Permian to lower Triassic sandstone of the Mount Roberts Formation indicate that detritus was derived from source terranes with ages of approximately 0.37–0.40 Ga, 1.0–1.3 Ga, 1.50 Ga, 1.61–1.66 Ga, 1.8–2.1 Ga, 2.36 Ga, 2.48 Ga, and 2.5–2.7 Ga. Devonian zircons are interpreted to represent first-cycle detritus derived from an igneous source terrane that may make up local basement to the Mount Roberts Formation. Most Precambrian zircons are well rounded by sedimentary abrasion and thus were probably derived from older sedimentary rocks. The ultimate sources of 1.0–1.66 Ga detrital zircons are unknown, but it is unlikely that they were derived from the presently adjacent craton. Zircons 1.0–1.66 Ga may represent detritus ultimately derived from southwestern Laurentia. Zircons 1.8–2.7 Ga are similar in age to geologic provinces within western Laurentia, suggesting presently adjacent provinces within the Laurentian craton as ultimate sources of some Precambrian detritus within the Mount Roberts Formation. Although Laurentia may have been the ultimate source of Precambrian detritus within the Mount Roberts Formation, sedimentologic and petrologic data and regional geologic considerations strongly suggest that most of this detritus was recycled from craton-derived sedimentary and metasedimentary rocks that composed part of Quesnellia.
机译:东部Quesnellia 内的二叠纪碎屑锆石的U-Pb年龄与西部和西南Laurentian地下室 的年龄相似,表明Quesnellian 之间的沉积学联系弧地带和劳伦山脉大陆边缘。下三叠纪罗伯茨山组的二叠系 形成了Quesnellia的Harper Ranch地下最东侧的 暴露。 地层由互层的岩灰质,泥质, 石灰石和火山岩沉积在火山岩 环境中。罗伯茨山组砂岩的岩石学 表示源自岩性多样的来源,这些来源主要由火山岩组成,但还包括大量的沉积,变质和plutonic 从单个 二叠纪到较低的三叠系砂岩的27个碎屑锆石的U-Pb年龄 表示碎屑来自具有 1.50 Ga,1.61–1.66 Ga,1.8–2.1 Ga,2.36 Ga,2.48 Ga和2.5的年龄–2.7 Ga。 泥盆纪锆石被解释为代表来自火成岩源地的第一周期碎屑 ,其可能构成了Mount的局部 基底。罗伯茨编队。多数前寒武纪锆石 由于沉积作用而被很好地环绕,因此 可能源自较老的沉积岩。 1.0–1.66 Ga碎屑锆石的最终来源是未知的,但 不太可能来自当前相邻的克拉通。 Zircons 1.0–1.66 Ga可能代表碎屑,这些碎屑最终从西南劳伦西亚(Laurentia)衍生而来。锆石1.8–2.7 Ga的年龄与Laurentia西部的地质省份相似,表明Laurentian克拉通内的当前相邻省份是某些地区的最终来源 Roberts组中的前寒武纪碎屑。尽管Laurentia可能是罗伯茨山组内前寒武纪碎屑的最终 来源,但 沉积学和岩石学数据以及区域地质考虑因素 强烈建议碎屑的一部分从 克拉通来源的沉积岩和准沉积岩中回收,这些岩石构成了Quesnellia的 部分。

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  • 来源
    《GSA Bulletin》 |1995年第6期|665-675|共11页
  • 作者单位

    Department of Geological Sciences, University of Texas at Austin, Austin, Texas 78713-7909;

    Department of Geological Sciences, University of Texas at Austin, Austin, Texas 78713-7909;

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