埃及西贝尼苏埃夫盆地阿扎尔油田白垩系演替的地球化学评价和盆地建模

IF 1.4 4区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY Geological Journal Pub Date : 2024-05-19 DOI:10.1002/gj.4979
Sherif Farouk, Saada Ahmed Saada, Mohamed Fagelnour, Ahmed Y. Tawfik, Mohamed Arafat, Khaled El-Kahtany
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引用次数: 0

摘要

利用总有机碳(TOC)、角质成分、玻璃光泽反射率(Ro%)和岩石-评价热解数据,对埃及西部沙漠西贝尼苏埃夫盆地(WBSB)Azhar-A-2 井白垩系序列进行了地球化学分析。此外,还建立了一维盆地模型,以研究该研究区域的埋藏和温度历史。据报道,最重要的白垩纪源岩主要位于白垩系的哈里塔地层(Kharita Formation)和晚仙人掌-山童系的阿布-罗阿什地层(Abu Roash Formation)中。根据目视角质测试和岩石热解评价,阿布鲁阿什地层(A、E、F 和 G)属于油气混合型源岩,角质类型从 II 型到 III 型不等,其中 A/R 'A 和 F' 组主要为油气混合型角质,具有最高的生成潜力,而 A/R 'E 和 G' 组则为天然气混合型角质。Kh地层下部的大部分样本被解释为生成潜力较低的易燃气角质岩 III 型。另一方面,可视角岩岩浆中大量的锂辉石是一个强有力的指标,表明下石油层是一个易生油而不是易生气的源岩。研究对象的热成熟度随深度的增加而增加,从 AR 地层顶部的不成熟到下 Kharita 地层底部的主要/峰值油窗,该地层是 WBSB 产生碳氢化合物的活性源岩。贝尼苏伊夫盆地的高热流值(57 和 60 mW/m2)很好地说明了活动源岩深度极限深度的变浅。从盆地建模研究来看,在晚白垩世中期(84.3-82.5 Ma),9811 至 11,090 ft 之间的主要成熟区穿过 L. Kharita 地层,根据转化率的不同,油气生成分为三个阶段,其中第二阶段为主要阶段,TR 为 5%-50%,显示出石油开始排出(Ro:0.73%-0.78%,可能为 0.81%)。
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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Geochemical evaluation and basin modelling of the Cretaceous succession in the Azhar Oil field, West Beni Suef Basin, Egypt

Geochemical analysis was performed on the Cretaceous sequence of the Azhar-A-2 well in the West Beni Suef Basin (WBSB), Western Desert, Egypt, utilizing data on total organic carbon (TOC), kerogen composition, vitrinite reflectance (Ro%) and Rock-Eval pyrolysis. In addition, a 1D basin model was built to investigate the burial and temperature history of the study area. The most important Cretaceous source rocks are predominantly reported within the Albian Kharita Formation and Late Cenomanian-Santonian Abu Roash (AR) Formation. Based on visual kerogen tests and Rock-Eval pyrolysis, AR Formation (A, E, F, and G) are mixed oil- and gas-prone source rocks with kerogens ranging from type II to type III, where A/R ‘A and F’ Members show dominant oil-prone kerogen with the highest generative potential, while A/R ‘E and G’ Members are more gas-prone kerogen. Most samples of the lower Kh Formation were interpreted as gas-prone kerogen type III with low generative potential. On the other hand, the high amount of liptinite in the visual kerogen macerals is a strong indicator that the lower Petroleum Formation is an oil-prone rather than gas-prone source rock. The thermal maturity of the studied members increases consistently with depth, ranging from immature at the top of the AR Formation to the main/peak oil window at the base of the Lower Kharita Formation, which served as an active source rock for the hydrocarbons generated in the WBSB. The high value of the heat flow in the Beni Suef Basin (57 and 60 mW/m2) is a good indicator for the shallowing of the active source rock depth limit depth. From the study of the basin modeling, the main mature zone reached between 9811 and 11,090 ft in the middle of the Late Cretaceous (84.3–82.5 Ma) is through the L. Kharita Formation with three phases of hydrocarbon generation according to transformation ratio, where the second phase is the main stage in which TR is 5%–50%, showing the beginning of oil expulsion (Ro: 0.73%–0.78%, possibly 0.81%).

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来源期刊
Geological Journal
Geological Journal 地学-地球科学综合
CiteScore
4.20
自引率
11.10%
发文量
269
审稿时长
3 months
期刊介绍: In recent years there has been a growth of specialist journals within geological sciences. Nevertheless, there is an important role for a journal of an interdisciplinary kind. Traditionally, GEOLOGICAL JOURNAL has been such a journal and continues in its aim of promoting interest in all branches of the Geological Sciences, through publication of original research papers and review articles. The journal publishes Special Issues with a common theme or regional coverage e.g. Chinese Dinosaurs; Tectonics of the Eastern Mediterranean, Triassic basins of the Central and North Atlantic Borderlands). These are extensively cited. The Journal has a particular interest in publishing papers on regional case studies from any global locality which have conclusions of general interest. Such papers may emphasize aspects across the full spectrum of geological sciences.
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