Origin of heavy oil in Cretaceous petroleum reservoirs

Q3 Earth and Planetary Sciences Bullentin of Canadian Petroleum Geology Pub Date : 2016-06-01 DOI:10.2113/GSCPGBULL.64.2.106
Timothy P. Bata, J. Parnell, S. Bowden, A. Boyce
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引用次数: 13

Abstract

Abstract Much of the world’s heavy oil is found in Cretaceous reservoir rocks due to a combination of tectonic, climatic, geological, and biological factors. Here we study Cretaceous oil sands from the Neuquen Basin (Argentina), Sergipe-Alagoas Basin (Brazil), Alberta (Canada), Dahomey Basin (Nigeria), Uinta Basin (USA), Western Moray Firth Basin (United Kingdom), and Wessex Basin (United Kingdom) to improve our understanding of the origin of the heavy oils. Our results indicate that the oils were generated as conventional light oil, which later degraded into heavy oils, rather than thermally cracked oils from over matured source rocks. All the studied Cretaceous oil sands are enriched in the polar fraction, and the total ion current (TIC) fragmentogram of the saturate fractions show unresolved complex mixture (UCM) humps indicating that the oils have undergone biodegradation. Sterane data for the Cretaceous oil sands show a selective increase in the C29 regular steranes relative to C27 and C28 regular sterane, which is also consistent with biodegradation. There is also evidence for diasterane degradation in some samples which are related, suggesting severe biodegradation. The trisnorhopane thermal maturity indicator showed that the Cretaceous oil sands have thermal maturity levels equivalent to 0.66–1.32% Ro, consistent with an early to late oil window. 25-norhopanes were not detected in any of the studied Cretaceous oil sands despite sterane degradation. This strongly suggests that biodegradation in the Cretaceous oil sands occurred at shallow depths rather than at greater depths. Pyrite associated with the Cretaceous oil sands was found to be consistently isotopically light. The isotopic fractionation between these pyrites and contemporary seawater sulfate was calculated using the mean δ34S values and the established seawater composition curve. This fractionation exceeded the maximum known kinetic isotope fractionation of approximately 20‰ that is possible from non-biogenic mechanisms, such as thermochemical sulfate reduction. This strongly suggests that the pyrite precipitated from an open system by means of microbial sulfate reduction as part of the biodegradation process.
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白垩系油藏稠油成因
由于构造、气候、地质和生物等多种因素的综合作用,世界上大部分稠油都分布在白垩纪储层中。本文研究了阿根廷Neuquen盆地、巴西Sergipe-Alagoas盆地、加拿大Alberta盆地、尼日利亚Dahomey盆地、美国unta盆地、英国Western Moray Firth盆地和英国Wessex盆地的白垩系油砂,以提高对稠油成因的认识。我们的研究结果表明,这些油是作为常规轻油生成的,然后降解为重油,而不是来自过成熟烃源岩的热裂解油。研究的白垩系油砂均富含极性组分,饱和组分的总离子电流(TIC)碎片图显示未解决的复杂混合物(UCM)峰,表明油砂经历了生物降解。白垩纪油砂甾烷数据显示,C29规则甾烷相对于C27和C28规则甾烷选择性增加,这也与生物降解相一致。也有证据表明,在一些相关的样品中,二甾烷降解,表明严重的生物降解。三去藿烷热成熟度指标表明,白垩系油砂热成熟度水平为0.66 ~ 1.32% Ro,符合早、晚含油窗;白垩纪油砂中除甾烷降解外未检出25-去藿烷。这有力地表明白垩纪油砂的生物降解发生在较浅的深度,而不是更深的深度。与白垩纪油砂伴生的黄铁矿同位素一致较轻。利用平均δ34S值和建立的海水成分曲线计算了这些黄铁矿与当代海水硫酸盐之间的同位素分馏。这种分馏超过了已知的最大动力学同位素分馏值约20‰,这可能来自非生物成因机制,如热化学硫酸盐还原。这强烈表明,黄铁矿沉淀从一个开放的系统通过微生物硫酸盐还原作为生物降解过程的一部分。
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来源期刊
Bullentin of Canadian Petroleum Geology
Bullentin of Canadian Petroleum Geology Earth and Planetary Sciences-Geochemistry and Petrology
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期刊介绍: The Bulletin of Canadian Petroleum Geology is a peer-reviewed scientific journal published four times a year. Founded in 1953, the BCPG aims to be the journal of record for papers dealing with all aspects of petroleum geology, broadly conceived, with a particularly (though not exclusively) Canadian focus. International submissions are encouraged, especially where a connection can be made to Canadian examples.
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