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The nature, origin and significance of luminescent layers in the Bazhenov Shale Formation of West Siberia, Russia

机译:俄罗斯西西伯利亚Bazhenov Shale形成的发光层的性质,起源和意义

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Argillites that strongly luminesce under UV radiation were detected in the Bazhenov Shale Formation (BSF) of the West Siberian Basin during routine core examination and found to be persistent over a wide lateral area. The mineralogy and fabric of these luminescent layers were characterized by optical and fluorescence microscopy, SEM, TEM, XRD and IR methods. Optical and fluorescence microscopy showed that the luminescent layers were to a large extent derived from volcanic ash falls and could be described as meta-tuffites, although normal detrital sedimentation continued at the same time. The layers have a thickness of several mm to a maximum of 3-4 cm and can be defined as a clay-rich regional horizons extending for over 500 km. XRD showed that two principal clay minerals were predominant, namely a kaolinite group minerals, (kaolinite-rich) and a mixed-layer illite-smectite (WS) similar to that found in K-bentonite. Total organic matter in the luminescent layers is much lower than that in the enclosing BSF clayey-silty siliceous sediments above and below as shown by pyrolytic analyses. Evidence is presented that the luminescent characteristic of the argillites is related to their clay mineralogy, specifically to their content of kaolin minerals, although a contribution from nitrogenous organic matter cannot be entirely discounted. In some ways the luminescent argillites can be compared with bentonites associated with ash transformations or with tonsteins in coal beds, which are also derived from volcanic ash falls and contain highly crystalline kaolinite. However, tonsteins originate at or near land surface whereas the argillites were apparently formed in the deep ocean. But just as tonsteins can be used for detailed stratigraphic studies and are valuable in the context of coal exploration, so may the luminescent argillites prove to be significant both stratigraphically and in the search for economic hydrocarbon deposits, bearing in mind that their clay mineralogy may be sensitive to temperature and depth of burial and related to their placement in the oil and gas window.
机译:在常规核心检查期间在西西伯利亚盆地的Bazhenov页岩形成(BSF)中检测到紫外线辐射下的颗粒状物,发现在宽阔的侧积上持续存在。这些发光层的矿物学和织物的特征在于光学和荧光显微镜,SEM,TEM,XRD和IR方法。光学和荧光显微镜表明,发光层在很大程度上衍生自火山灰落下,并且可以描述为元胶合物,尽管正常滴乳沉降同时持续。该层的厚度为几毫米至最大3-4厘米,可以定义为富含富含粘土的区域视野,延伸超过500公里。 XRD表明,两个主要粘土矿物是主要的,即高岭石矿物质,(富高岭石)和类似于K-膨润土中的混合层硅灰石 - 蒙脱石(WS)。如热解析分析所示,发光层中的总有机物质远低于封闭的BSF粘土 - 粉质沉积物中的封闭BSF粘土淤泥沉积物。提出了证据表明,颗粒状物的发光特性与其粘土矿物学相关,特别是对其高岭土矿物质的含量有关,尽管含氮有机物质的贡献不能完全折扣。在某种程度上,发光颗粒可以与与灰分转化相关的膨润土或煤层中的粉末,其衍生自火山灰落下并含有高度结晶的高岭石。然而,TONSTEINS起源于陆地表面或附近,而肉骨显然形成在深海中。但正如Tonsteins可用于详细的地层研究,并且在煤炭勘探的背景下都是有价值的,所以可能的发光armillits在地层和寻找经济碳氢化合物存款中,考虑到他们的粘土矿物质,所以可能是他们的粘土矿物质对埋葬温度和深度敏感,与它们在油气窗口中的放置相关。

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