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Forearc basin detrital zircon provenance of Mesozoic terrane accretion and translation, Talkeetna Mountains-Matanuska Valley, south-central Alaska

机译:Forearc盆地碎屑锆石物种的中生代地体增生和翻译,Talkeetna山脉 - 马塔努斯卡谷,阿拉斯加中南部

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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 (εHf(t)=4.5-14.7). 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 (εHf(t)=6.0-18.8). 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 (εHf(t)=4.5-14.7). 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 (εHf(t)=-1.5-14.9) and Paleozoic-Precambrian grains (εHf(t)=-23.7-16.3).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:该Wrangellia复合地体加入到中生代以来时间北美大陆的新生地壳的最大的片段之一,并完善其增生的历史有重要的影响为了解大陆如何成长。从Wrangellia复合地块的弧前晚侏罗世,晚白垩世地层碎屑锆石的新的U-Pb同位素年代学和Hf同位素允许在terrane.Our的构造和古地理历史,从晚侏罗世地层纳克内克最古老的地层样本有更多的了解一碎屑锆石签名通过早期和晚期侏罗纪晶粒(195-190马; 153-147 Ma)的支配。这些颗粒的Hf同位素组合物是少年至中间体(εHf(T)= 4.5-14.7)。 Disconformably的纳克内克形成上述两种知之甚少单位Ks的和KC。对KS单元由早期为主到晚侏晶粒(159-154马)与几个古生界的晶粒(347-340马)。 HF石炭 - 侏罗纪晶粒的同位素组成少年至中间体(εHf(T)= 6.0-18.8)。覆的Kc单位有晚来早侏罗世锆石(198-161马),并在古生代年龄的增加(374-323马)。这些颗粒的Hf同位素组合物是少年至中间体(εHf(T)= 4.5-14.7)。从马塔努斯卡组样品有重大的晚白垩世谷物(90-71马),和次要早白垩世(137-106马),晚至早侏罗世(200-153马),古生代(367-277马),和前寒武纪谷物(1097至37年马)。 HF的组合物具有从两晚白垩颗粒更宽范围(εHf(T)= - 1.5-14.9)和古生界 - 前寒武纪的晶粒(εHf(T)= - 23.7-16.3)。我们的结果表明一个演变出处晚侏罗晚白垩世时间Wrangellia复合地块弧前盆地。晚侏纳克内克形成样品显性从少年到中间侏罗纪火成岩沉积物来源。在早白垩时间,存在对KS和KC单元样品中古生代晶粒的数量略有增加。早白垩沉积物具有提示的侏罗纪和古生界少年火成岩沉积物源折返一个大多正Hf同位素组合物。到晚白垩世的时候,我们的数据说明了在古生代粮丰度再次增加,除了引进前寒武纪粒,全部用大范围变化的Hf同位素组成。我们解释这反映了从阿拉斯加的内部,其中更进化的那个时代的火成岩中发现较大的泥沙通量。

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    Mattie Morgan Reid;

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