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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Microbial hydrocarbon gases in the Witwatersrand Basin, South Africa: Implications for the deep biosphere
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Microbial hydrocarbon gases in the Witwatersrand Basin, South Africa: Implications for the deep biosphere

机译:南非Witwatersrand盆地中的微生物碳氢化合物气体:对深层生物圈的影响

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摘要

In this study, compositions and delta(13)C and delta(2)H isotopic values of hydrocarbon gases from 5 mines in the Witwatersrand basin, South Africa, support the widespread occurrence of microbially produced methane in millions of years-old fissure waters. The presence of microbial methane is, to a large extent, controlled by the geologic formations in which the gases are found. Samples from the Witwatersand Supergroup have the largest microbial component based on delta(13)C and delta(2)H signatures and CH4/C-2+ values. Based on mixing between a microbial CH, component and a more C-13-enriched and H-2-depleted C-2+-rich end member, conservative estimates of the % contribution of microbial CH4 to the gas samples range from >90% microbial CH4 at Beatrix, Masimong, and Merriespruit, to between 5 and 80% microbial CH4 at Evander, and <18% microbial CH4 at Kloof. The Witwatersrand basin's history of thermal alteration of organic-rich ancient sedimentary units suggests a thermogenic origin for this C-13-enriched end member. Alternatively, the potential for an abiogenic origin similar to hydrocarbon gases produced by water-rock interaction at other Precambrian Shield mines is discussed. Microbial methane is predominantly found in paleo-meteoric fissure waters with delta(18)O and delta(2)H values that fall on the meteoric waterline, and have temperatures between 30 to 40degreesC. In contrast, fissure waters with a larger component of nonmicrobial hydrocarbon gases show a trend towards more enriched delta(18)O and delta(2)H values that fall well above the meteoric waterline, and temperatures of 45 to 60degreesC. The enrichment in O-18 and H-2 in these samples, and their high salinity, are similar to the isotopic and compositional characteristics of saline groundwaters and brines produced by water-rock interaction at Precambrian Shield sites elsewhere. The reported 100 Ma ages of fissure waters from the Witwatersrand and Ventersdorp, formations suggest that these microbial hydrocarbon gases are the product of in situ methanogenic communities in the deep subsurface of the Witswaterand basin. Small subunit ribosomal RNA genes were amplified using archaeal-specific primer sets from DNA extracts derived from several of these waters. Fissure waters with a high proportion of microbial methane also contained sequences resembling those of known methanogens. Copyright (C) 2004 Elsevier Ltd.
机译:在这项研究中,来自南非维特沃特斯兰德盆地5个矿山的烃类气体的组成以及δ(13)C和δ(2)H同位素值支持了数百万年前的裂隙水中微生物产生的甲烷的广泛存在。微生物甲烷的存在在很大程度上受到发现气体的地质构造的控制。基于delta(13)C和delta(2)H签名以及CH4 / C-2 +值,威特沃特和超级集团的样本具有最大的微生物成分。根据微生物CH,组分与更富C-13且富H-2的富C-2 +端基之间的混合,保守估计微生物CH4对气体样品贡献的百分比范围为> 90% Beatrix,Masimong和Merriespruit的微生物CH4,Evander的微生物CH4在5%至80%之间,Kloof的微生物CH4在18%以下。威特沃特斯兰德盆地对富含有机物的古代沉积单元进行热变质的历史表明,这种富含C-13的末段成员具有热成因。或者,讨论了与其他前寒武纪盾构矿山的水-岩相互作用产生的烃类气体类似的生物成因起源的可能性。微生物甲烷主要存在于古金属裂隙水中,其δ(18)O和δ(2)H值落在陨石水线上,温度在30至40摄氏度之间。相比之下,具有非微生物碳氢化合物成分较大的裂隙水显示出趋势,即δ(18)O和delta(2)H值更富集,且该值远低于流线水线,温度为45至60摄氏度。这些样品中O-18和H-2的富集及其高盐度与其他地方的前寒武纪盾构站点中水-岩相互作用产生的盐分地下水和盐水的同位素和组成特征相似。据报道,维特沃特斯兰德和温特斯多普地层的裂隙水年龄为100 Ma,这表明这些微生物碳氢化合物气体是Witswaterand盆地深部地下原位产甲烷菌的产物。使用古细菌特异的引物组从这些水中的几种提取的DNA提取物中扩增出小的亚基核糖体RNA基因。含有高比例微生物甲烷的裂隙水还含有与已知产甲烷菌相似的序列。版权所有(C)2004 Elsevier Ltd.

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