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首页> 外文期刊>Journal of Sedimentary Research >Storm-Influenced Prodelta Turbidite Complex in the Lower Kenilworth Member at Hatch Mesa, Book Cliffs, Utah, U.S.A.: Implications for Shallow Marine Facies Models
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Storm-Influenced Prodelta Turbidite Complex in the Lower Kenilworth Member at Hatch Mesa, Book Cliffs, Utah, U.S.A.: Implications for Shallow Marine Facies Models

机译:美国犹他州书峭壁Hatch Mesa下部Kenilworth成员受风暴影响的Prodelta浊积体:对浅海相模型的影响

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摘要

Isolated sandstone bodies encased in marine mudstones have proved difficult to explain, especially those that are not easily incorporated into conventional facies models. The Hatch Mesa succession (Campanian, lower Kenilworth Member) is a marine mudstone-encased, turbiditic sandstone body, 6 to 20 m thick, that is exposed along a 7-km-long outcrop belt, approximately 15 km east of Green River, Utah, U.S.A. Various interpretations of depositional environment and regional correlation have been proposed over the past 20 years. A sedimentological analysis of the Hatch Mesa succession suggests deposition as a storm-influenced, prodelta turbidite complex on the shallow inner shelf, between fair-weather and storm wave base. This interpretation is corroborated by the high-resolution outcrop correlation and subsequent paleogeographic reconstruction, which indicates deposition 16 to 21 km basinward of the time equivalent lower-shoreface deposits, in about 20 m water depth. A variety of mechanisms are capable of generating instability in the delta front and triggering the turbid flow of sediments into deeper water, including storm events, river flooding, high rates of sedimentation, or earthquakes. This explains the complex mixture of event beds in the Hatch Mesa succession, which are dominated by wave-modified turbidites. A three-component model, consisting of delta-front, subaqueous channel, and prodelta turbidite deposits, is proposed to explain the depositional environment and setting of the Hatch Mesa succession. All three components are observed in the lower Kenilworth Member to upper Aberdeen Member stratigraphic interval. The results of this study indicate that shallow marine facies models should be revised to include marine mudstone-encased, prodelta turbidite complexes, thus adding one more possibility to the diverse suite of interpretations used to explain the generation and preservation of isolated marine sandstone bodies. These results also shed new light on the stratigraphic position and depositional setting of the Mancos Shale-encased, isolated sandstone bodies of the Prairie Canyon Member in eastern Utah and western Colorado.
机译:事实证明,包裹在海洋泥岩中的孤立砂岩体很难解释,特别是那些不易与常规相模型合并的砂岩体。哈奇·梅萨演替场(Campanian, 下肯尼尔沃思成员)是一个由海洋泥岩包裹的,浑浊的,厚度为6至20 m的砂岩体,在7公里的范围内暴露-长 露头带,位于美国犹他州格林河以东约15公里在过去的20年中,已经提出了各种沉积环境和 区域相关性的解释。 对Hatch Mesa演替的沉积学分析表明, 沉积为受风暴影响的浅层内层架上的三角洲浊积质复合物 ,在晴天和风暴波 基底之间。高分辨率 露头相关性和随后的古地理重建( )证实了这种解释,这表明距时间 相当低的时间向后沉积了16至21 km在约20 m的水深处形成海岸沉积物。 多种机制能够在三角洲前缘产生不稳定性 并触发沉积物的浑浊流 进入更深的水中,包括暴风雨事件,河水泛滥,高sups 沉积速率或地震。这就解释了Hatch Mesa演替过程中事件床的复杂 混合物,其中 主要由波变浊度组成。提出了由三角洲前缘,水下通道和前三角洲 浊石沉积物组成的三组分模型 来解释沉积 环境和环境孵化台面系列。在Kenilworth下部至Aberdeen上部地层间隔中均观察到这三个 分量。 研究的结果表明,应修改 浅海相模型,使其包含海洋泥岩包裹的三角洲浊积岩复合体, 再添加一个 各种解释的可能性,用于解释孤立的 海洋砂岩体的生成和保存。这些结果也为 草原上峡谷 成员的Mancos 页岩包裹的孤立砂岩体的地层位置和沉积环境提供了新的依据。犹他州东部和科罗拉多州西部。

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  • 来源
    《Journal of Sedimentary Research》 |2005年第3期|00000420-00000439|共20页
  • 作者

    Simon A.J. Pattison;

  • 作者单位

    Department of Geology, Brandon University, Brandon, Manitoba, R7A 6A9, Canadapattison@brandonu.ca;

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  • 正文语种 eng
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