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Palynological, palynofacies, paleoenvironmental and organic geochemical studies on the Upper Cretaceous succession of the GPTSW-7 well, North Western Desert, Egypt

机译:埃及西北沙漠GPTSW-7井上白垩纪演替的孢粉,孢粉,古环境和有机地球化学研究

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The present study of the Abu Roash and Bahariya formations in well GPTSW-7 refines our understanding of the subsurface Cretaceous of the north Western Desert of Egypt. Our investigations are based on the palynological analyses of 71 cuttings samples, of which 24 have also been analyzed for geochemistry, in addition to 3 sidewall cores analyzed for vitrinite reflectance (R_o). Four palynological zones and three subzones in addition to a poorly fossiliferous interval ranging in age from Coniacian-Santonian to early Cenomanian are proposed. These include a poorly fossiliferous interval (Coniacian-Santonian), Dinogymnium vozzhennikovae Interval Zone (late to middle Turanian), Ephedripites ambiguus-Ephedripites multicostatus-Foveotricolpites giganteus-Foveotricolpites gigantor-eticultus Assemblage Zone (early Turanian), Classopollis brasiliensis Interval Zone (late to middle Cenomanian), and Afropollis jardinus Interval Zone (early Cenomanian). The succeeding subzones are; Afropollis kahramanensis Interval Subzone, Elaterosporites klaszii Interval Subzone and Cretacaeiporites densimurus Interval Subzone, all of early Cenomanian age. Total organic carbon (TOC) and Rock-Eval pyrolysis and palynofacies analyses indicate that the Bahariya Formation and the Abu Roash G Member are primarily of kerogen III type and hence gas prone, suggesting a strong influence of hydrogen-enriched organic matter. The Abu Roash A, C-E Members may also be gas prone (type III kerogen) and appear to contain highly oxidized terrestrial organic matter. In contrast, the Abu Roash F Member has very high TOC and HI values and contains a very high proportion of amorphous organic matter (AOM) indicating a highly oil-prone fades. While this finding is not unexpected for anoxic black shale, it contrasts with earlier studies that suggest a gas prone nature. R_o measurements show that the Bahariya Formation represents an immature-early genesis dry gas phase. This is also true for all investigated samples from the Abu Roash and Bahariya formations, based on their low thermal alteration index (TAI). Quantitative and qualitative analyses of both the palynoflora and palynofacies show that the Abu Roash A and C Members (B is missing), both of Coniacian-Santonian age, represent oxic proximal and distal shelf environment. The Abu Roash D and E Members, dated as Turanian, represent oxic (proximal) shelf, whereas the Cenomanian Abu Roash F Member was deposited in a distal suboxic-anoxic basin. The Cenomanian Abu Roash G Member and the Bahariya Formation were deposited in a shallow marine and shallow marine to fluvio-deltaic setting, respectively. The Senonian Palmae Province is recognized in the palynoflora by the presence of Proteacidites, Auric-uliidites reticulatus, Ariadnaesporites, Gabonisporis vigourouxii. On the other hand the Albian-Cenomanian Elaterates Province is characterized by the presence of Steevesipollenites, Gnetaceaepollenites, Elaterocolpites, Elaterosporites, Elateroplicites, Senegalosporites, Sofrepites, Afropollis and Cretacaeiporites.
机译:对GPTSW-7井中Abu Roash和Bahariya地层的当前研究进一步完善了我们对埃及西北沙漠地下白垩纪的认识。我们的研究基于71个岩屑样品的孢粉学分析,此外,还分析了3个侧壁岩心的镜质反射率(R_o),其中24个也进行了地球化学分析。除了从柯尼西亚-桑托尼时代到早西诺曼尼时代的年龄范围内的化石间隔差外,还提出了四个孢粉学区和三个亚区。这些包括化石差的地区(Coniacian-Santonian),Dinogymnium v​​ozzhennikovae间隔区(晚至Turanian中部),Ephedripites ambiguus-Ephedripites multicostatus-Foveotricolpites giganteus-Foveotricolpites gigantor-eticultus组合带(早期Turanoplatelate)中西诺曼尼亚)和Afropollis jardinus间隔区(西诺曼尼亚早期)。后续分区是; Afropollis kahramanensis区间子区,Elaterosporites klaszii区间子区和Cretacaeiporites densimurus区间子区,都属于早西诺曼时代。总有机碳(TOC)以及岩石评估热解和古岩相分析表明,Bahariya组和Abu Roash G成员主要为干酪根III型,因此容易产生天然气,表明富氢有机物的影响很大。 Abu Roash A,C-E成员也可能是易燃气体(III型干酪根),并且似乎含有高度氧化的陆地有机物。相比之下,Abu Roash F会员的TOC和HI值非常高,并且含有很高比例的无定形有机物(AOM),表明容易产生油污。虽然这一发现对于缺氧的黑色页岩并不意外,但它与早期的研究相反,后者表明天然气易生。 R_o测量表明,Bahariya组代表了一个未成熟的早成因的干气相。基于低热蚀变指数(TAI),对于所有来自阿布鲁阿什(Abu Roash)和巴哈里亚(Bahariya)地层的调查样品也是如此。 ly粉和孢粉的定量和定性分析表明,科尼亚—桑顿时期的阿布·罗什A和C成员(B缺失)代表了近端和远端的有氧环境。日期为Turanian的Abu Roash D和E成员代表有氧(近端)层架,而Cenomanian Abu Roash F成员则沉积在远缺氧-缺氧盆地中。 Cenomanian Abu Roash G成员和Bahariya组分别沉积在浅海和浅海至潮三角地区。芦苇科的帕诺科省被认为存在于蛋白酸岩,金乌利特岩,网纹岩藻,加蓬孢霉。另一方面,阿尔比亚-西奥马尼埃拉特省的特征是存在硬脂硅粉,鹅毛藻粉,Elaterocolpites,Elaterosporites,Elateroplicites,Senegalosporites,Sofrepites,Afropollis和Cretacaeiporites。

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