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Cell proliferation at 122 degrees C and isotopically heavy CH4 production by a hyperthermophilic methanogen under high-pressure cultivation.

Authors
  • Takai, Ken
  • Nakamura, Kentaro
  • Toki, Tomohiro
  • Tsunogai, Urumu
  • Miyazaki, Masayuki
  • Miyazaki, Junichi
  • Hirayama, Hisako
  • Nakagawa, Satoshi
  • Nunoura, Takuro
  • Horikoshi, Koki
Type
Published Article
Journal
Proceedings of the National Academy of Sciences
Publisher
Proceedings of the National Academy of Sciences
Publication Date
Aug 05, 2008
Volume
105
Issue
31
Pages
10949–10954
Identifiers
DOI: 10.1073/pnas.0712334105
PMID: 18664583
Source
Medline
License
Unknown

Abstract

We have developed a technique for cultivation of chemolithoautotrophs under high hydrostatic pressures that is successfully applicable to various types of deep-sea chemolithoautotrophs, including methanogens. It is based on a glass-syringe-sealing liquid medium and gas mixture used in conjunction with a butyl rubber piston and a metallic needle stuck into butyl rubber. By using this technique, growth, survival, and methane production of a newly isolated, hyperthermophilic methanogen Methanopyrus kandleri strain 116 are characterized under high temperatures and hydrostatic pressures. Elevated hydrostatic pressures extend the temperature maximum for possible cell proliferation from 116 degrees C at 0.4 MPa to 122 degrees C at 20 MPa, providing the potential for growth even at 122 degrees C under an in situ high pressure. In addition, piezophilic growth significantly affected stable carbon isotope fractionation of methanogenesis from CO(2). Under conventional growth conditions, the isotope fractionation of methanogenesis by M. kandleri strain 116 was similar to values (-34 per thousand to -27 per thousand) previously reported for other hydrogenotrophic methanogens. However, under high hydrostatic pressures, the isotope fractionation effect became much smaller (< -12 per thousand), and the kinetic isotope effect at 122 degrees C and 40 MPa was -9.4 per thousand, which is one of the smallest effects ever reported. This observation will shed light on the sources and production mechanisms of deep-sea methane.

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