首页> 外文会议>Meeting of the Gulf Coast Section of the Society of Economic Paleontologists and Mineralogists >New Insights into the Eastern Margin of the Tuxpan Platform and its Influence on Deepwater Plays of the Gulf of Mexico
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New Insights into the Eastern Margin of the Tuxpan Platform and its Influence on Deepwater Plays of the Gulf of Mexico

机译:新洞察燕苏平台东部边缘及其对墨西哥湾深水剧的影响

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Geological and geophysical studies were carried out with the main objective being the updating of the depositional model for the Tamabra Formation of Cretaceous (Albian-Cenomanian) age, on the eastern (offshore) side of the Tuxpan Platform, located on the southeastern side of the Tampico Misantla Basin, México. For many decades, productive fields in this formation are known to lie in a belt located on the western (onshore) side of the Tuxpan Platform, of which the Poza Rica Field is the best known example and demonstrates a combination (stratigraphic/structural) trap mechanism. Along the onshore Tamabra Formation trend, facies of carbonate debris flows form the primary reservoir facies. By contrast, the "Tamabra Formation" off the eastern (marine) side of the platform has only been penetrated by two non-commercial wells, well A and well B. In particular, the reservoir rock is thin, but it shows acceptable reservoir quality even at depths of more than 5200 m. Nevertheless, recently undertaken specialist studies, including petrography, cathpdoluminescence, fluid inclusion analysis of material from the two wells, plus seismic facies mapping have provided evidence that the Tuxpan Platform, its former slope and sometimes underlying basinal facies, have suffered significant erosion. This was due to significant structural uplift of a zone running just to the east of the present-day Marine Tuxpan Platform; this uplift and erosion combined with eustatic influences and resulted in a very notably different present-day limit to the Tuxpan Platform, to that which was present in the Albian-Cenomanian. The "Tamabra" encountered in well A and well B has emerged as a Late Cretaceous (Late Cenomanian/Turonian and younger) deposit which was largely derived from erosion of the eastern margin of the Tuxpan Platform and its slope. Because of this, true Tamabra facies of Albian-Cenomanian age in this area, have not been tested.
机译:正在进行地质和地球物理研究的主要目标是更新Tamabra形成的白垩纪(白葡萄球菌)年龄,东部(近海)的燕尾服平台,位于东南部坦克米塔拉盆地,墨西哥。多十年来,已知这种形成的生产领域是位于燕苏平台的西部(陆上)侧的皮带中,其中Poza Rica领域是最着名的示例,并演示了组合(地层/结构)陷阱机制。沿着陆上Tamabra形成趋势,碳酸盐碎片流动的面部形成主要水库相。相比之下,平台的东部(海洋)一侧的“Tamabra形成”只有两个非商用井,井A和良好的B.特别地,水库岩石薄而薄,但它显示了可接受的储层质量即使在超过5200米的深度。尽管如此,最近进行了专业研究,包括透镜,壳致发光,从两个井中的材料流体包容性分析,加上地震相形图已经提供了证据表明,燕苏平台,其前坡和有时底层面部遭受了显着的侵蚀。这是由于距离当今海洋燕尾服平台以东的一个区域的重要结构隆起;这种隆起和侵蚀结合了突然影响,导致了对Tuxpan平台的一个非常不同的当前限制,到了Albian-Cenomanian中存在的那些。众所周知的“Tamabra”遇到了一个,b良好的是作为一个晚餐(晚年康马尼亚/涡轮和较年轻)矿床,这主要来自燕尾服平台的东部边缘的侵蚀及其坡度。因此,在这一领域的Albian-Cenomanian年龄的真正Tamabra相片尚未进行测试。

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