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Forearc Basin Detrital Zircon Provenance of Mesozoic Terrane Accretion and Translation, Talkeetna Mountains-Matanuska Valley, South-Central Alaska

机译:阿拉斯加中部塔基特纳山-马塔努斯卡河谷中生代地层增生和转化的前陆盆地碎屑锆石种源

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摘要

The Wrangellia composite terrane is one of the largest fragments of juvenile crust added to the North American continent since Mesozoic time, and refining its accretionary history has important implications for understanding how continents grow. New U-Pb geochronology and Hf isotopes of detrital zircons from Late Jurassic-Late Cretaceous strata from the forearc of the Wrangellia composite terrane allows more insight on the tectonic and paleogeographic history of the terrane.;Our stratigraphically oldest samples from the Late Jurassic Naknek Formation have a detrital zircon U-Pb signature dominated by Early and Late Jurassic grains (195-190 Ma; 153-147 Ma). Hf isotopic compositions of these grains are juvenile to intermediate (epsilonHf(t)=+4.5 to +14.7). Disconformably above the Naknek Formation are two poorly understood units Ks and Kc. The Ks unit is dominated by Early to Late Jurassic grains (159-154 Ma) with a few Paleozoic grains (347-340 Ma). Hf isotopic compositions of Carboniferous-Jurassic grains are juvenile to intermediate (epsilonHf(t)=+6.0 to +18.8). The overlying Kc unit has Late to Early Jurassic zircons (198-161 Ma), and an increase in Paleozoic ages (374-323 Ma). Hf isotopic compositions of these grains are juvenile to intermediate (epsilonHf(t)=4.5 to +14.7). Samples from the Matanuska Formation have major Late Cretaceous grains (90-71 Ma), and minor Early Cretaceous (137-106 Ma), Late to Early Jurassic (200-153 Ma), Paleozoic (367-277 Ma), and Precambrian grains (2597-1037 Ma). Hf compositions have a wider range from both the Late Cretaceous grains (epsilonHf(t)=-1.5 to +14.9) and Paleozoic-Precambrian grains (epsilonHf (t)=-23.7 to +16.3).;Our results suggest an evolving provenance from Late Jurassic to Late Cretaceous time for the Wrangellia composite terrane forearc basin. The Late Jurassic Naknek Formation samples were dominantly derived from a juvenile to intermediate Jurassic igneous sediment source. During Early Cretaceous time, there is a slight increase in the number of Paleozoic grains in the Ks and Kc unit samples. The Early Cretaceous sediments have a mostly positive Hf isotopic compositions suggesting exhumation of Jurassic and Paleozoic juvenile igneous sediment sources. By Late Cretaceous time, our data illustrates another increase in Paleozoic grain abundances, in addition to the introduction of Precambrian grains, all with widely variable Hf isotopic compositions. We interpret this to reflect a larger sediment flux from the interior of Alaska where more evolved igneous rocks of that age are found.
机译:自中生代以来,Wrangellia复合地层是添加到北美大陆的最大的幼年壳碎片之一,并且对其增生历史进行改良对于理解各大陆的生长方式具有重要意义。来自Wrangellia复合地层前缘的晚侏罗世-晚白垩世地层碎屑锆石的新的U-Pb地质年代学和Hf同位素,使人们可以更深入地了解该地层的构造和古地理历史。具有由早期和晚期侏罗纪颗粒(195-190 Ma; 153-147 Ma)控制的碎屑锆石U-Pb签名。这些晶粒的Hf同位素组成从幼年到中等(εHf(t)= + 4.5至+14.7)。 Naknek地层上方不一致地是两个认识不清的单元Ks和Kc。 Ks单元以侏罗纪早期至晚期(159-154 Ma)和少量古生代(347-340 Ma)为主。石炭纪-侏罗纪谷物的f同位素组成从幼年到中等(εHf(t)= + 6.0至+18.8)。上覆的Kc单元具有晚至早侏罗世锆石(198-161 Ma),古生代年龄增加(374-323 Ma)。这些晶粒的Hf同位素组成从幼年到中等(εHf(t)= 4.5至+14.7)。马塔努斯卡组的样品具有主要的晚白垩纪颗粒(90-71 Ma)和次要的早白垩纪(137-106 Ma),晚侏罗纪至早侏罗纪(200-153 Ma),古生代(367-277 Ma)和前寒武纪颗粒(2597-1037马)。 Hf成分的分布范围较晚白垩纪颗粒(epsilonHf(t)=-1.5至+14.9)和古生代前寒武纪颗粒(epsilonHf(t)=-23.7至+16.3).;我们的结果表明Wrangellia复合地层前臂盆地的侏罗纪晚期至白垩纪晚期。侏罗纪晚期的Naknek组样本主要来自侏罗纪至中期的侏罗纪火成岩沉积物源。在白垩纪早期,Ks和Kc单位样品中的古生代晶粒数量略有增加。早白垩世沉积物的f同位素主要为正,表明侏罗纪和古生代火成岩沉积物的掘出。到白垩纪晚期,我们的数据表明,除了引入前寒武纪晶粒外,古生代谷物丰度又有了增加,所有这些元素的H同位素组成都变化很大。我们将其解释为反映了来自阿拉斯加内部更大的沉积物通量,在那里发现了该年龄的更多演化的火成岩。

著录项

  • 作者

    Reid, Mattie Morgan.;

  • 作者单位

    The University of Iowa.;

  • 授予单位 The University of Iowa.;
  • 学科 Geology.
  • 学位 M.S.
  • 年度 2017
  • 页码 70 p.
  • 总页数 70
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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