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ORIGIN, DISTRIBUTION AND ALTERATION OF ORGANIC MATTER AND GENERATION AND MIGRATION OF HYDROCARBONS IN AUSTIN CHALK, UPPER CRETACEOUS, SOUTHEASTERN TEXAS.

机译:德克萨斯州上白垩统奥斯汀粉笔中有机物的起源,分布和交替以及烃的生成和迁移。

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摘要

The Austin Chalk is an impure "onshore" chalk that was deposited on a ramp marginal to the Gulf of Mexico during the Late Cretaceous. Basinal chalks are organic rich, commonly containing 0.5-5.0% amorphous, sapropelic kerogen derived from marine organic matter with only trace amounts of terrestial kerogen. Less organic matter was deposited and perserved in oxygenated shallow water, and fresh-water diagenesis oxidized the organic matter on outcrop. In each sample, the kerogen is concentrated in microstylolites, with organic fluids segregated in micropores in the chalk.;The Austin Chalk reservoirs petroleum sourced within the formation and petroleum that has migrated into the chalk from elsewhere in the chalk and the underlying Eagleford Formation. The hydrocarbons are reservoired in interparticulate pores and micro- and macrofractures. Migration results in an enrichment in saturated hydrocarbons and, to a lesser extent, in aromatic hydrocarbons and resins in porous, reservior chalks. Crude oil produced from fractured chalks tends to have a high API gravity and to be enriched in saturated hydrocarbons, probably due to migration. Biodegradation may lower the gravity and hydrocarbon content of crude oils reservoired in shallow chalks.;The bitumen from the Austin Chalk contains geochemical fossils characteristic of plankton and algae: steranes, triterpanes, isoprenoids (particularly pristane and phytane), and even-carbon numbered C(,15)-C(,22) n-alkanes. These geochemical fossils become less abundant with increasing burial depth, due to the generation of hydrocarbons during catagenesis. The kerogen darkens and becomes condensed and aromatic as the H/C atomic ratio decreases and hydrocarbons are liberated from the kerogen and from asphaltenes. Saturated hydrocarbons, particularly C(,12)-C(,26) n-alkanes and isoalkanes and single-ring cycloalkanes, increase more rapidly than aromatic hydrocarbons and resins. Kerogen alteration and hydrocarbon generation are unaffected by the mineral composition of the chalk, suggesting that the dominant controls on the rate of alteration and the composition of hydrocarbons generated are the type of organic matter and thermal history of the rocks. The principal zone of oil generation for the Austin Chalk occurs at the same depth as for shales of the same age.
机译:奥斯汀粉笔是一种不纯的“陆上”粉笔,在白垩纪晚期沉积在墨西哥湾边缘的斜坡上。陆生白垩富含有机物,通常含有0.5-5.0%的无定形腐泥型干酪根,其来源于海洋有机物,仅有少量陆生干酪根。较少的有机物沉积并保留在含氧浅水中,淡水成岩作用使露头的有机物氧化。在每个样品中,干酪根都集中在微苯乙烯中,而有机流体则被隔离在白垩的微孔中。奥斯汀粉笔储层中的石油来自石油,而石油则从白垩和下层的伊格福德组中迁移到白垩中。碳氢化合物储藏在颗粒间的孔隙以及微裂缝和大裂缝中。迁移导致了饱和烃的富集,而在较小程度上,多孔的储层白垩中的芳烃和树脂富集。由破裂的白垩产生的原油倾向于具有较高的API比重,并且可能由于迁移而富含饱和烃。生物降解可能会降低浅粉垩中储藏的原油的重力和碳氢化合物含量。奥斯汀粉笔中的沥青包含浮游生物和藻类的地球化学化石:甾烷,三萜,类异戊二烯(尤其是rist烷和植烷),以及碳编号为C的偶数碳(,15)-C(,22)正构烷烃。这些地球化学化石随着埋藏深度的增加而变得不那么丰富,这是由于在催化作用期间产生了碳氢化合物。随着H / C原子比的降低,干酪根变黑并凝结成芳香族,烃从干酪根和沥青质中释放出来。饱和烃,特别是C(,12)-C(,26)正构烷烃和异烷烃以及单环环烷烃,比芳烃和树脂的增长更快。干酪根的蚀变和生烃不受白垩矿物成分的影响,这表明蚀变速率和生烃成分的主要控制因素是有机质的类型和岩石的热历史。奥斯丁粉笔的主要产油区出现在与相同年龄的页岩相同的深度处。

著录项

  • 作者单位

    Rice University.;

  • 授予单位 Rice University.;
  • 学科 Geochemistry.
  • 学位 Ph.D.
  • 年度 1981
  • 页码 295 p.
  • 总页数 295
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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