首页> 外文期刊>Organic Geochemistry: A Publication of the International Association of Geochemistry and Cosmochemistry >The organic geochemistry of oil seeps from the Sierra de Perijá eastern foothills, Lake Maracaibo Basin, Venezuela
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The organic geochemistry of oil seeps from the Sierra de Perijá eastern foothills, Lake Maracaibo Basin, Venezuela

机译:委内瑞拉马拉开波湖盆地塞拉利昂德佩里哈东部山麓油渗流的有机地球化学

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摘要

The organic geochemistry of samples from 11 oil seeps was studied. The samples were collected from the Cachirí area, Carboniferous Region of Tulé (Lake Maracaibo Basin, Venezuela), associated with the Tigre Fault. Biomarkers (hopanes, steranes, n-alkanes, acyclic isoprenoids, and aromatic steroids) were analyzed using gas chromatography-mass spectrometry (GC-MS). These hydrocarbon rich fluids have undergone biodegradation (2-6 on the Peters and Moldowan scale), showing both the partial loss of n-alkanes and the microbial degradation of isoprenoids and steranes. These oil seeps were generated from a mature calcareous source rock that was deposited in a marine paleoenvironment under reducing conditions. Moreover, these seeps are likely derived from the Cretaceous La Luna Formation that reached a level of maturity near the peak of oil generation in the study area. The nature of the studied oil seeps, together with the oil generation models reported for this rock unit in the study area, suggests that these oils are a mixture of an initially heavy, altered oil and a second migrated light crude oil resulting from two generation pulses from the La Luna Formation. Evidence for the presence of light oil trapped in the study area should prompt re-exploration in the northwestern coast of Lake Maracaibo in shallow reservoirs, previously discarded because they usually demonstrated a lack of light oils.
机译:研究了11个渗油样品的有机地球化学特征。样品是从与蒂格雷断层有关的图莱石炭纪地区卡奇里地区(委内瑞拉湖马拉开波盆地)采集的。使用气相色谱-质谱(GC-MS)分析了生物标志物(庚烷,甾烷,正构烷烃,无环类异戊二烯和芳香族类固醇)。这些富含烃的流体经历了生物降解(在Peters和Moldowan规模上为2-6),既显示了正构烷烃的部分损失,又显示了类异戊二烯和甾烷的微生物降解。这些油渗出物是由成熟的钙质烃源岩产生的,该烃源岩在还原条件下沉积在海洋古环境中。此外,这些渗漏很可能来自白垩纪La Luna地层,在研究区的采油高峰附近达到了成熟水平。所研究的油渗漏的性质以及研究区域内该岩石单元所报告的生油模型表明,这些油是由两次重生脉冲产生的初始重质,蚀变油和第二种轻质原油的混合物。来自La Luna组。研究区域中存在轻油的证据应促使马拉开波湖西北海岸浅层储层中的勘探活动重新进行,这些浅水库以前被丢弃,是因为它们通常表明缺乏轻质油而被丢弃。

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