首页> 外文期刊>Geosphere >Detrital zircons from crystalline rocks along the Southern Oklahoma fault system, Wichita and Arbuckle Mountains, USA
【24h】

Detrital zircons from crystalline rocks along the Southern Oklahoma fault system, Wichita and Arbuckle Mountains, USA

机译:美国俄克拉荷马州南部断层系统,威奇托和阿巴克勒山脉的结晶岩碎屑锆石

获取原文
       

摘要

Detrital zircons with ages of 535 ?± 10 Ma in many North American Midcontinent sandstones are commonly attributed to sources in Cambrian synrift igneous rocks along the Southern Oklahoma fault system. New analyses are designed to test the characteristics of proximal detritus from the Wichita and Arbuckle uplifts. Detrital zircons from a sandstone (Lower Permian Post Oak Conglomerate) directly above an unconformable contact with the Wichita Granite Group in the Wichita Mountains have strongly unimodal U-Pb ages of 540a€“520 Ma and ?μHft values of +4.7 to +10.1. In contrast, two sandstone samples (Upper Pennsylvanian Vanoss Conglomerate) in the onlapping succession above an angular unconformity on Paleozoic strata on the flank of the Arbuckle anticline have detrital zircons with U-Pb ages that correspond dominantly to the Superior (a??2700 Ma) and secondarily to the Granite-Rhyolite (1480a€“1320 Ma) and Grenville (1300a€“970 Ma) provinces of the Laurentian craton. The Vanoss zircons indicate recycling from quartzose sandstones within the Middle Ordovician platform carbonates in the Arbuckle passive-margin cover succession. A stratigraphically higher sandstone (Permian Wellington Formation) above the onlapping conglomerates has a more diverse detrital-zircon population, indicating that sediment dispersal from external sources overwhelmed the proximal detritus in the immediate cover of the Wichita and Arbuckle uplifts. The distinctive ?μHft values of the proximal detritus from the Cambrian synrift igneous rocks offer potential discrimination from zircons of the same age from Gondwanan accreted terranes, which are represented in the Wellington sample.
机译:在许多北美中大陆砂岩中,年龄为535±10 Ma的碎屑锆石通常归因于沿俄克拉荷马州南部断裂系统的寒武纪同生火成岩中的来源。设计了新的分析方法,以测试Wichita和Arbuckle隆起的近端碎屑的特征。在与威奇托山的威奇托花岗岩集团不整合接触的正上方的砂岩(下二叠纪橡树后砾岩)中的碎屑锆石具有很强的单峰U-Pb年龄,为540a-520520 Ma,?μHft值介于+4.7至+10.1之间。相反,在Arbuckle背斜侧面上的古生界地层上,在一个角度不整合面之上的重叠演替中的两个砂岩样品(宾夕法尼亚州上瓦努斯砾岩上部)具有U-Pb年龄的碎屑锆石,主要对应于上层(a ?? 2700 Ma)。 ),其次是Laurentian克拉通的Granite-Rhoolite(1480a€“ 1320 Ma”)和Grenville(1300a€“ 970 Ma)省。 Vanoss锆石表明从Arbuckle被动边缘覆盖层中段的奥陶系中层碳酸盐岩中的石英砂岩中回收。重叠砾岩上方的地层较高的砂岩(二叠纪惠灵顿组)具有更多的碎屑锆石种群,这表明来自外部资源的沉积物扩散使威奇托和阿尔巴克勒隆起的直接覆盖层中的近端碎屑不堪重负。寒武纪同火成岩火成岩近端碎屑的独特的?μHft值可以区分来自冈瓦南增生的地层的同年龄的锆石,这在惠灵顿样品中得到了体现。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号