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多年冻土中甲烷及产甲烷古菌的生物地球化学

Biogeochemistry of methane and methanogenic archaea in permafrost.

作者信息

Rivkina Elizaveta, Shcherbakova Viktoria, Laurinavichius Kestas, Petrovskaya Lada, Krivushin Kirill, Kraev Gleb, Pecheritsina Svetlana, Gilichinsky David

机构信息

Institute of Physicochemical and Biological Problems in Soil Sciences, Russian Academy of Sciences, Moscow, Russian Federation.

出版信息

FEMS Microbiol Ecol. 2007 Jul;61(1):1-15. doi: 10.1111/j.1574-6941.2007.00315.x. Epub 2007 Apr 11.

DOI:10.1111/j.1574-6941.2007.00315.x
PMID:17428301
Abstract

This study summarizes the findings of our research on the genesis of methane, its content and distribution in permafrost horizons of different age and origin. Supported by reliable data from a broad geographical sweep, these findings confirm the presence of methane in permanently frozen fine-grained sediments. In contrast to the omnipresence of carbon dioxide in permafrost, methane-containing horizons (up to 40.0 mL kg(-1)) alternate with strata free of methane. Discrete methane-containing horizons representing over tens of thousands of years are indicative of the absence of methane diffusion through the frozen layers. Along with the isotopic composition of CH(4) carbon (delta(13)C -64 per thousand to -99 per thousand), this confirms its biological origin and points to in situ formation of this biogenic gas. Using (14)C-labeled substrates, the possibility of methane formation within permafrost was experimentally shown, as confirmed by delta(13)C values. Extremely low values (near -99 per thousand) indicate that the process of CH(4) formation is accompanied by the substantial fractionation of carbon isotopes. For the first time, cultures of methane-forming archaea, Methanosarcina mazei strain JL01 VKM B-2370, Methanobacterium sp. strain M2 VKM B-2371 and Methanobacterium sp. strain MK4 VKM B-2440 from permafrost, were isolated and described.

摘要

本研究总结了我们关于甲烷的产生、其在不同年代和成因的多年冻土层面中的含量及分布的研究结果。这些结果得到了广泛地理区域可靠数据的支持,证实了在永久冻土细粒沉积物中存在甲烷。与二氧化碳在多年冻土中无处不在不同,含甲烷层(含量高达40.0 mL kg(-1))与不含甲烷的地层交替出现。代表数万年的离散含甲烷层表明甲烷没有通过冻层扩散。连同CH(4)碳的同位素组成(δ(13)C为-64‰至-99‰),这证实了其生物起源,并表明这种生物成因气是原地形成的。利用(14)C标记底物,通过δ(13)C值证实,实验证明了多年冻土内甲烷形成的可能性。极低的值(接近-99‰)表明CH(4)形成过程伴随着碳同位素的大量分馏。首次从多年冻土中分离并描述了产甲烷古菌培养物,即马氏甲烷八叠球菌JL01菌株VKM B-2370、甲烷杆菌属M2菌株VKM B-2371和甲烷杆菌属MK4菌株VKM B-2440。

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