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The Geologic History of Submarine Fans in the Deepwater Gulf of Mexico: Mesozoic to Modern

机译:墨西哥深水湾潜艇粉丝的地质史:中生代近代

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Submarine fans are among the most important reservoirs in the prolific Gulf of Mexico Basin and are known from industry drilling and seismic data to be contained within strata extending from the Mesozoic to modern. However, little has been published on how these systems evolve over this time frame, responding to extra-basinal factors like tectonics, climate, sediment discharge, etc. A comparison of Mesozoic age submarine fans with those of the most important Cenozoic fans in the Gulf reveals important new insights into the basin formation and evolution. We interpret the newly formed basin, just after termination of Callovian salt deposition, to be rather shallow but not entirely terrestrial. The initial middle-Jurassic low-dipping ramp from land to sea transitioned into a shelf-slope-basinal profile, with sea floor spreading ranging in age from Kimmeridgian to Berriasian. This in turn provided impetus for development of the earliest poorly organized submarine aprons in the late Jurassic and early Cretaceous. These eventually evolved into submarine fans but their sizes were constrained by rather short river lengths until reorganization of North American drainage systems in the mid-Cretaceous. Mapping major sand-prone fairways reveal that most of the Mesozoic slope and basin systems were fed by eastern North American source terrains. Siliciclastic delivery into the basin was also hampered by reef blocking, as large rimmed shelf reef systems of Barremanian to Albian age restricted sediment bypass to a few discrete basin entry points. The dramatic drainage reorganization in the Cenomanian ushered in the first of the large and extensive submarine fan systems, known from exploration wildcats to have extended nearly 500 km from the coeval shelf edge. Deep crustal tectonic events likely played a role in both drainage re-routing but also allowed siliciclastic systems to surmount the rimmed shelf reef systems and develop shelf-edge/slope-basin pathways over broad fairways. The Cenomanian fan systems look more like Cenozoic fan successors, with long run-outs, variable sediment gravity flow products, and tendency to respond to the para-autochthonous salt seascape and developing primary basins. The alteration of the seascape caused by the Chicxulub impact event subsequently altered deepwater transport pathways in some areas. But this event did set the stage for Paleogene and later fans that responded to continental scale drainage networks developed with the Laramide orogeny. Subsequent evolution of these fans was modulated by salt tectonics, climate-related sediment discharge variations, volcanism, and eventually the Neogene ice sheets. The Value of Information: Wilcox Play Mapping, 1998-2015 Our knowledge of submarine fan systems in the Gulf of Mexico has advanced with migration of exploration from onshore to shelf to deepwater over the last 90 years. A historical examination of the Paleogene Wilcox Play maps constructed by the Gulf Basin Depositional Synthesis (GBDS) research project at the University of Texas reveals how our expectations of size and extent of this prolific hydrocarbon reservoir play have been episodically reset with evolving regional depositional models and new drilling results. The analysis also documents the value of information in reducing risk and uncertainty for high-cost drilling targets like the deepwater Wilcox. Prior to 1998, the Wilcox was largely viewed as an economically challenged onshore deep gas play, with discoveries peaking in the early 1980s (Snedden et al., 2002; Zarra, 2007). Few wells were drilled offshore for the Wilcox and in the deep water, as strata older than Oligocene were only penetrated in salt carapaces and rafts at shallow depths (Fig. 1, top). The presence of large Paleogene fluvial and deltaic systems, documented in outcrop and onshore subsurface wells, suggested the presence of a Lower Wilcox sandy apron system in offshore areas (Fig. 1, bottom).
机译:潜艇粉丝是墨西哥盆地多产湾最重要的水库之一,并且是从工业钻井和地震数据中闻名的,以包含在从中生代到现代的地层中。然而,很少已经发表了这些系统如何在此时间框架中发展,响应构造,气候,沉积物放电等额外基底因素等。中生代潜艇粉丝与海湾中最重要的新生代粉丝的比较揭示了进入盆地形成和进化的重要新见解。我们解释新形成的盆地,刚刚在终止呼链盐沉积之后,相当浅但没有完全陆地。初始中侏罗纪低浸渍坡道从陆地到海上转变为搁板坡面剖面,海底蔓延到岁月到Berriasian。这反过来提供了在侏罗纪晚期和早期白垩纪最早的潜艇围裙的发展动力。这些最终演变为潜艇风扇,但它们的尺寸受到相当短的河流长度的限制,直到中白垩纪的北美排水系统重组。映射主要的沙易散装通道揭示了大多数中生代坡和盆地系统被东部北美来源地带喂养。通过珊瑚礁阻挡,泥石流输送到盆地中也受到阻碍的,因为巴拉斯时代的大型边缘货架礁系统到白尔翁年龄限制沉积物旁路到几个离散盆地入口点。 Cenomanian中的戏剧性排水重新组织迎来了一流的大型潜艇风扇系统中,从探索野猫队开始延伸距离科夫架边缘近500公里。深层地壳构造事件可能在排水重新路由中发挥作用,而且还允许丝状体系来超越镶边搁板礁系统,并在宽阔的球道上开发搁板边缘/坡度盆地。 Cenomanian粉丝系统看起来更像是新生代粉丝后继,随着长远,可变沉积物重力流产品,以及倾向于响应帕拉自动加持的盐海景和开发初级盆地。由肾小管冲击事件引起的海景的改变随后改变了一些区域的深水输送途径。但是,这个事件确实为古代和后来的粉丝设定了古代和后来球迷的舞台,这些舞台响应了随着LARAMIDE ORONSONY开发的大陆尺度引流网络。这些风扇的后续演变被盐构造,气候相关的沉积物排放变化,火山,最终是Neogene冰盖。信息的价值:Wilcox Play Mapping,1998 - 2015年我们对墨西哥湾潜艇风扇系统的知识已经通过陆上探索的探索到过去90年来深水。德克萨斯大学海湾盆地沉积综合(GBDS)研究项目构建的古代Wilcox Play地图的历史检查揭示了我们对这种多产的碳氢化合物储层的规模和程度的期望如何,并通过不断发展的区域沉积模型来重置这一多种碳氢化合物储层游戏。新钻探结果。分析还记录了减少高成本钻井目标的风险和不确定性的信息的价值,如深水Wilcox。在1998年之前,Wilcox在很大程度上被视为一个经济上挑战的陆上深气体发挥,在20世纪80年代初发现达到峰值(Snedden等,2002; Zarra,2007)。近距离蠕动的Wilcox和深水钻井井,因为少于少茂的地层仅在盐围巾和浅深度下渗透(图1,顶部)。在露头和陆上地下井中记录了大型古血小腺氟和德伦特系统,建议在海上地区存在下威尔科克含有较低的Wilcox砂岩系统(图1,底部)。

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