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The Gravina Sequence: Remnants of a Mid-Mesozoic oceanic arc in southern southeast Alaska

机译:Gravina序列:阿拉斯加东南部南部中生代洋弧的残余

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摘要

Fragments of Upper Jurassic to Lower Cretaceous volcanic and basinal strata constitute the Gravina belt in southeast Alaska. In the Ketchikan area the Gravina belt is made up of two lithotectonic units. The lower unit consists of coarse marine pyroclastic and volcaniclastic strata, mafic flows, breccia, and fine-grained tuff which are locally intruded by hypabyssal bodies of diorite and quartz diorite. The volcanic rocks are characterized by tholeiitic arc basalts, lack felsic volcanic strata, and overlie Upper Triassic and older strata of the Alexander terrane. Augite and/or hornblende-bearing porphyritic rocks are common and locally intrude the Alexander terrane basement, where they are thought to represent the intrusive equivalents of lavas within the section. Age constraints for the volcanic unit, based on structural and stratigraphic relations with adjacent units, are late Middle to Late Jurassic. The Gravina belt upper unit consists of fine- to coarse-grained turbidites and related conglomeratic channel-fill deposits. The basinal rocks unconformably overlie Permian and Triassic rocks of the Taku terrane and remnants of the lower volcanic part of the Gravina sequence which overlie the Alexander terrane. The conglomerate units contain mostly volcanic and plutonic lithic clasts, some of which yield Pb-U zircon ages of 154–158 Ma. The predominance of pyroclastic deposits interbedded with massive flows, tuff, breccia, and argillaceous turbidites, and the lithologic and chemical composition of the volcanic rocks indicate a submarine volcanic arc setting for the Gravina sequence. The basinal pyroclastic rocks are inferred to have been shed from submarine stratovolcanos during the Late Jurassic. Epiclastic rocks were deposited as submarine fans, derived in part from erosion of a magmatic arc. The presence of fine-grained tuffaceous turbidites implies ongoing, but distant, volcanism. The pyroclastic and volcaniclastic rocks represent remnants of a Late Jurassic oceanic arc constructed on a composite basement consisting of the Alexander and Taku terranes. The strata accumulated in an intra-arc basin on the eastern edge of the Alexander terrane. The volcanic and basinal rocks were deformed during a major mid-Cretaceous intra-arc contractional event, in conjunction with the emplacement of a distinctly younger, arc-related plutonic suite.
机译:从上侏罗纪到下白垩纪的火山岩和盆地地层构成了阿拉斯加东南部的格拉维纳带。在凯奇坎地区,格拉维纳带由两个岩石构造单元组成。下层单元由海相碎屑岩和火山碎屑岩,镁铁矿流,角砾岩和细密的凝灰岩组成,它们被闪长岩和石英闪长岩的下伏体局部侵入。火山岩的特征为高生质弧形玄武岩,缺乏长英质火山岩地层,并覆盖上三叠纪和亚历山大山地的较旧地层。附有奥古石和/或角闪石的斑岩岩很常见,并局部侵入亚历山大山脉的地下室,据认为它们代表了该断面内熔岩的侵入性等价物。基于与相邻单元的结构和地层关系,该火山单元的年龄限制是中侏罗世晚期。 Gravina带上部单元由细粒至粗粒状浊石和相关的砾岩状河道沉积物组成。塔库山脉的二叠纪和三叠纪岩石以及格拉维纳层序的下火山部分的残余物不整合地覆盖在亚历山大山脉之上。砾岩单元主要包含火山岩和深成岩碎屑,其中一些碎屑生成的Pb-U锆石年龄为154-158 Ma。火山碎屑沉积物以大量流动,凝灰岩,角砾岩和泥质浊积岩夹层为主,火山岩的岩性和化学成分表明格拉维纳序列的海底火山弧环境。推断侏罗纪晚期,盆地的火山碎屑岩是从海底平流层火山中脱落的。表观岩石是作为海底扇沉积的,部分源于岩浆弧的侵蚀。细颗粒的凝灰质浊度的存在意味着正在进行的但遥远的火山活动。火山碎屑岩和火山碎屑岩代表了侏罗纪晚期海洋弧的残余物,该弧构造在由亚历山大和塔库(Taku)地层组成的复合基底上。地层聚集在亚历山大地层东缘的弧内盆地中。火山岩和盆地岩石在大型白垩纪弧内收缩事件中变形,同时还伴有明显年轻的与弧有关的岩溶套件。

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