日本地球惑星科学連合2024年大会

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[J] ポスター発表

セッション記号 U (ユニオン) » ユニオン

[U-11] CO環境の生命惑星化学

2024年5月26日(日) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:上野 雄一郎(東京工業大学大学院地球惑星科学専攻)、北台 紀夫(海洋研究開発機構)、鈴木 志野(国立研究開発法人宇宙航空研究開発機構)、尾崎 和海(東京工業大学)

17:15 〜 18:45

[U11-P14] COとCO2を基質とした微生物酢酸生成の分子内炭素同位体分別

*佐藤 悠太1鈴木 志野2、加藤 創一郎3、笠井 拓哉3、山田 桂大1上野 雄一郎1,5,4、Alexis Gilbert1 (1.東京工業大学、2.宇宙航空研究開発機構、3.産業技術総合研究所、4.海洋研究開発機構、5.東京工業大学地球生命研究所)

キーワード:酢酸生成菌、CO固定、分子内同位体分析

Position-Specific Isotope Analysis (PSIA) has been utilized in a wide range of fields to tracing the sources and sink processes of molecules in environment. In this research, we focus on intramolecular carbon isotope distribution of acetic acid, which is often produced by microbial acetogenesis and plays an important role in the biogeochemical carbon cycle. The carbon isotopic relationship between methyl and carboxyl positions of acetate, which are through different pathways in acetogenic metabolisms, could be important to interpret the mechanisms of acetate production. We have incubated acetogenic bacteria and methanogenic archaea, both of which are capable of converting both CO2 and CO into acetic acid. The results showed that the acetate exhibited significant differences between carboxyl and methyl positions in acetic acid (Δcar-met >30‰) when the carbon source was CO, whereas Δcar-met value was much smaller (< 9‰) when the acetic acid was produced from CO2. Based on the experimental results, we provide a new interpretation of the carbon flows in the metabolism (i.e., Wood-Ljungdal pathway). The observed large Δcar-met can be explained by a shortage of energy and CO2 pool under CO condition. The results also demonstrated the possibility that the PSIA of acetic acid could be utilized for distinguishing carbon sources for microbial acetogenesis in the environment.