日本地球惑星科学連合2016年大会

講演情報

ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS33] 地球惑星科学と微生物生態学の接点

2016年5月23日(月) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*砂村 倫成(東京大学大学院理学系研究科地球惑星科学専攻)、高井 研(海洋研究開発機構極限環境生物圏研究センター)、濱村 奈津子(九州大学)、諸野 祐樹(海洋研究開発機構高知コア研究所)

17:15 〜 18:30

[MIS33-P02] 巨大地震後の深海底におけるメタン生成ホットスポットの出現

*田角 栄二1野牧 秀隆1柳川 勝紀2今野 祐多酒井 早苗1平井 美穂1藤倉 克則1布浦 拓郎1高井 研1 (1.国立研究開発法人 海洋研究開発機構、2.九州大学)

キーワード:深海、メタン生成、巨大地震

We investigated the deep-sea microbial ecosystem after the 2011 Off Tohoku Earthquake and tsunami. In the series of study, we found several "hot spot of methanogeneis" on the deep-seafloor after the mega-earthquake and demonstrated the methylotrophic methanegenesis in the deep-sea surface sentiment.
On the 2011 cruise, we found a lot of large microbial mats on the 5,000 m-depth deep-seafloor. The surface sediment cores (< 25 cm) were collected from microbial mats and analyzed their chemical and microbial profiles. On the top of the cores (a few centimeters), decomposing dead body of maline lives such as echinoderms that contains trimethylamine N-oxide, a precursor of trimetylamine (TMA), in the body were accumulated. In the surface layer (< 15 cm), high concentration of ammonium, TMA, and isotopically light methane was detected. In this layer, heterotrophic microbes such as Bacteroides, Firmicutes, and Spirochaeta were dominated. These results suggests that huge amount of organic matter had been recently supplied on the deep-seafloor. In addition, a large number of mcrA gene were also detected. Most of which were identified as those of Methanococcoides sp. that can grow on methyl compounds as the sole energy source. From the results of investigation in 2011, we hypothesized that high concentration of methane in the microbial mat sediments were generated by methylotrophic methanogen.
On the 2012 cruise, we conducted in-situ incubation to prove our hypothesis. In-situ incubation cores with 13C substrate, 13C-bicarbonate, 13C-acetate, 13C-monomethylamine (MMA) were set on the deep-seafloor where a large microbial mat had been found in 2011 and measured methanogenesis activity. During three days of incubation, significant activity was detected only in the incubation core supplied MMA.
We hope that our results provide important hints to understand the ecology and evolution of methanogenic/methanotrophic archaea in deep-sea environments.