Microbial Gas in the Mohe Permafrost, Northeast China and its Significance to Gas Hydrate Accumulation in Permafrost across China
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This study was entirely supported by Prospecting and Testing Production Project of Gas Hydrate resources, Ministry of Land and Resources of China (grants No. GZHL20110317, GZHL20110320, GZHL20110322). The authors thank Guo Wei and Ji Shengli for their assistance in the field, as well as Chen Liu (gas chromatograph) and Wang Guang (mass spectrometry) for their analytical expertise.

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    Abstract:

    The Mohe permafrost in northeast China possesses favorable subsurface ambient temperature, salinity, Eh values and pH levels of groundwater for the formation of microbial gas, and the Mohe Basin contains rich organic matter in the Middle Jurassic dark mudstones. This work conducted gas chromatography and isotope mass spectrometry analyses of nearly 90 core gas samples from the Mk-2 well in the Mohe Basin. The results show that the dryness coefficient (C1/C1–5) of core hydrocarbon gas from approximately 900 m intervals below the surface is larger than 98%, over 70% of the δ13C values of methane are smaller than ?55‰, and almost all δD values of methane are smaller than ?250‰, indicative of a microbial origin of the gas from almost 900 m of the upper intervals in the Mohe permafrost. Moreover, the biomarker analyses of 72 mudstone samples from the Mohe area indicate that all of them contain 25-norhopane series compounds, thereby suggesting widely distributed microbial activities in the permafrost. This work has confirmed the prevailing existence of microbial gas in the Mohe area, which may be a potential gas source of gas hydrate formation in the Mohe permafrost. This result is of great significance to gas hydrate accumulation in the permafrost across China.

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ZHAO Xingmin, SUN Youhong, DENG Jian, RAO Zhu, Lü Cheng, SONG Jian, Li Lixia.2018. Microbial Gas in the Mohe Permafrost, Northeast China and its Significance to Gas Hydrate Accumulation in Permafrost across China[J]. Acta Geologica Sinica(),92(6):2251-2266

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History
  • Received:April 11,2018
  • Revised:July 27,2018
  • Adopted:
  • Online: December 19,2018
  • Published: