Gravity flow deposits in Mesozoic sediments of Chukotka microplate (North-East Russia)

IF 1.9 3区 地球科学 Q1 GEOLOGY
Marianna I. Tuchkova, Elena V. Vatrushkina, Sergey D. Sokolov
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Abstract

In the Mesozoic succession of the Anyui–Chukotka fold system (North-East Russia), five stratigraphic intervals were recognised that have an abundance of gravity flow deposits. These are the Olenekian (Lower Triassic), Upper Carnian, Upper Norian, Oxfordian–Kimmeridgian and Valanginian. The Triassic gravity flow deposits formed on the south-facing, passive margin of the Chukotka microplate and consist of greywackes and lithic arenites. Palaeocurrent data indicate that the flows were directed towards the south-east. The Olenekian gravity flow units consist of clast-rich sandstone deposited on the continental slope, and clast-poor sandstone deposited at the base of the slope. Upper Carnian mud-poor sandstones were deposited at the base of the slope and the Norian thin-bedded turbidites were upper to mid-slope deposits. The continental margin was affected by tectonism and was uplifted in the latest Triassic–earliest Jurassic, possibly due to the initiation of the southward translation of the Arctic Alaska–Chukotka microplate. Following an Early–Middle Jurassic uplift of the area, sedimentation resumed in the Late Jurassic and earliest Cretaceous. Several syn-orogenic depressions (Rauchua, Pegtymel, Pevek, Myrgovaam and Kytepveem) developed on the south-western margin of the Chukotka microplate, and deposition in these basins included gravity flow deposits at various times. In both the Oxfordian–Kimmeridgian and Valanginian successions, gravity flow deposits included arkosic and subarkosic sandstones with a northern source area of granitoid complexes and deformed Triassic strata. The intervening Tithonian–Berriasian gravity flow deposits consisted mainly of thin-bedded turbidites. These sediments had a southern source, which included a volcanic arc that had accreted to the southern margin of the Chukotka microplate.

Abstract Image

楚科奇微板块中生代沉积物中的重力流沉积(俄罗斯东北部)
在安义-丘科特卡褶皱系统(俄罗斯东北部)的中生代演替中,有五个地层区间被认为具有丰富的重力流沉积。它们分别是奥利尼克期(下三叠统)、上卡尼期、上诺尔期、牛津-基默里吉期和瓦朗基尼期。三叠纪重力流沉积形成于楚科奇微板块朝南的被动边缘,由灰岩和碎屑岩组成。古水流数据表明,这些水流流向东南。奥利尼克重力流单元由沉积在大陆坡上的富含碎屑的砂岩和沉积在坡底的贫含碎屑的砂岩组成。上卡尼期贫泥砂岩沉积于斜坡底部,诺尔纪薄层浊积岩为斜坡中上部沉积。大陆边缘受到构造运动的影响,在晚三叠世-早侏罗世发生隆起,这可能是由于北极阿拉斯加-楚科奇微板块开始向南平移所致。该地区在侏罗纪早中期隆升之后,在侏罗纪晚期和白垩纪早期恢复了沉积作用。楚科奇微板块西南边缘形成了几个同源坳陷(Rauchua、Pegtymel、Pevek、Myrgovaam 和 Kytepveem),这些盆地的沉积在不同时期包括重力流沉积。在牛津-基默里德纪和瓦朗基尼纪岩层中,重力流沉积包括弧光砂岩和亚弧光砂岩,其北部源区为花岗岩群和变形的三叠纪地层。其间的提托尼-白垩纪重力流沉积主要由薄层浊积岩组成。这些沉积物的南部来源包括楚科奇微板块南缘增生的火山弧。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
4.10
自引率
16.70%
发文量
42
审稿时长
16 weeks
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