日本地球惑星科学連合2016年大会

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インターナショナルセッション(口頭発表)

セッション記号 B (地球生命科学) » B-AO 宇宙生物学・生命起源

[B-AO01] Astrobiology: Origins, Evolution, Distribution of Life

2016年5月24日(火) 15:30 〜 17:00 A01 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*小林 憲正(横浜国立大学大学院工学研究院)、山岸 明彦(東京薬科大学生命科学部)、大石 雅寿(国立天文台天文データセンター)、田近 英一(東京大学大学院新領域創成科学研究科複雑理工学専攻)、掛川 武(東北大学大学院理学研究科地学専攻)、井田 茂(東京工業大学大学院理工学研究科地球惑星科学専攻)、Voytek Mary(NASA Headquarter)、Kirschvink Joseph(Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA)、座長:田近 英一(東京大学大学院新領域創成科学研究科複雑理工学専攻)、掛川 武(東北大学大学院理学研究科地学専攻)

15:45 〜 16:00

[BAO01-08] Pressure-induced formation of alanine oligopeptides at 25 °C

*藤本 千賀子1篠崎 彩子2三村 耕一2西田 民人2後藤 弘匡3小松 一生1鍵 裕之1 (1.東京大学大学院理学系研究科附属地殻化学実験施設、2.名古屋大学環境科学研究科、3.東京大学物性研究所)

キーワード:amino acids, high pressure, oligomerization

Introduction
Oligomerization of amino acids can provide a clue to the origin of life because it is a fundamental step of protein synthesis. Under high pressure, increases of intermolecular interactions result in chemical reaction which cannot proceed under ambient condition. Oligomerization of amino acids was reported from experiments under high pressure and high temperature conditions simulating impact of comets, hydrothermal vents, diagenesis in sub-seafloor sedimentary environments (e.g., Sugahara and Mimura, 2015; Imai and Honda, 2010; Otake et al., 2011). In these experiments, both high pressure and high temperature are the important factors for amino acids oligomerization. However, it is unknown which factor is more efficient for forming oligomers. In this study, we focus on exclusive effect of high pressure on oligomerization reaction. We tested oligomerization of L-alanine under a room temperature and high-pressure condition. Fujimoto et al. (2015) reported pressure-induced oligomerization of L-alanine up to the trimer using GC-MS analysis (Fig 1). In the present study, we used LC-MSMS to detect higher oligomers.
Experimental procedures
All high-pressure experiments were carried out at 25 °C. Starting material was loaded in a high-pressure cell with three different conditions: wet, dry and solution (wet: L-Alanine powder with its saturated aqueous solution. dry: L-alanine powder. solution: saturated L-alanine aqueous solution.). Sample was compressed using a large-volume opposed-anvil apparatus or a “Kawai-type” multi-anvil apparatus. Experimental runs were conducted at pressures of approximately 5 GPa, 7 GPa, 9 GPa, 11 GPa, and 16 GPa using an opposed-anvil apparatus and 18 GPa and 23 GPa using a multi-anvil apparatus. After decompression to ambient pressure, run products were dissolved in pure water and analyzed using LC-MSMS.
Results and discussion
Alanine dimer was detected from all the run products. With increasing pressure, the yields of alanylalanine increased for each experimental condition (wet, dry, and solution). At pressures higher than 9 GPa, formation of alanine trimer was detected and the yield increased with pressure. These results are consistent with the results of Fujimoto et al. (2015). It is noteworthy that oligomerization of alanine occurred under water-coexisting conditions. In the pressure and temperature conditions applied in this study, water in the samples existed as ice VII, the oligomerization observed here was a solid-phase reaction. Higher oligomers were detected from the samples recovered from high pressure. Under the wet condition, the formed oligomers decreased with increasing the oligomer size and the largest oligomer detected was 8-mer.
This study revealed that oligomerization of amino acids occurs under high pressure at room temperature with existence of water as ice VII which is known to exist in the interiors of icy planets. This study proposes an interior of an icy planet as a new abiotic condition for oligomerization of amino acids.