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Geochemical and Microbiological Evidence for Microbial Methane Production in Deep Aquifers of the Cretaceous Accretionary Prism

机译:白垩纪增生棱镜深层含水层中微生物甲烷产生的地球化学和微生物证据。

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摘要

Accretionary prisms are thick layers of sedimentary material piled up at convergent plate boundaries. Large amounts of anaerobic groundwater and methane (CH4) are contained in the deep aquifers associated with accretionary prisms. In order to identify microbial activity and CH4 production processes in the deep aquifers associated with the Cretaceous accretionary prism in Okinawa Island, Japan, we performed geochemical and microbiological studies using anaerobic groundwater and natural gas (mainly CH4) samples collected through four deep wells. Chemical and stable hydrogen and oxygen isotope analyses of groundwater samples indicated that the groundwater samples obtained from each site originated from ancient seawater and a mixture of rainwater and seawater, respectively. Additionally, the chemical and stable carbon isotopic signatures of groundwater and natural gas samples suggested that CH4 in the natural gas samples was of a biogenic origin or a mixture of biogenic and thermogenic origins. Microscopic observations and a 16S rRNA gene analysis targeting microbial communities in groundwater samples revealed the predominance of dihydrogen (H2)-producing fermentative bacteria and H2-utilizing methanogenic archaea. Moreover, anaerobic cultures using groundwater samples suggested a high potential for CH4 production by a syntrophic consortium of H2-producing fermentative bacteria and H2-utilizing methanogenic archaea through the biodegradation of organic substrates. Collectively, our geochemical and microbiological data support the conclusion that the ongoing biodegradation of organic matter widely contributes to CH4 production in the deep aquifers associated with the Cretaceous accretionary prism.
机译:增生棱镜是堆积在会聚板边界处的厚厚沉积物质层。与增生棱镜相关的深层含水层中含有大量的厌氧地下水和甲烷(CH4)。为了确定与日本冲绳岛白垩纪增生棱镜相关的深层含水层中的微生物活性和CH4的生产过程,我们使用通过四个深井收集的厌氧地下水和天然气(主要为CH4)样品进行了地球化学和微生物学研究。地下水样品的化学和稳定氢,氧同位素分析表明,从每个站点获得的地下水样品分别来自古代海水以及雨水和海水的混合物。此外,地下水和天然气样品的化学和稳定碳同位素特征表明,天然气样品中的CH4是生物成因或生物成因和热成因的混合物。显微镜观察和针对地下水样品中微生物群落的16S rRNA基因分析揭示了产生二氢(H2)的发酵细菌和利用H2的产甲烷古细菌的优势。此外,使用地下水样品进行的厌氧培养表明,由产H2的发酵细菌的同养联合体和通过H2利用产甲烷的古细菌通过有机底物的生物降解而产生CH4的潜力很大。总的来说,我们的地球化学和微生物学数据支持这样的结论,即正在进行的有机物生物降解广泛地促进了与白垩纪增生棱镜相关的深层含水层中CH4的产生。

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