日本地球惑星科学連合2021年大会

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[J] ポスター発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS06] 惑星科学

2021年6月4日(金) 17:15 〜 18:30 Ch.03

コンビーナ:仲内 悠祐(宇宙航空研究開発機構)、菊地 紘(宇宙航空研究開発機構)

17:15 〜 18:30

[PPS06-P05] 行列表示を用いた有機物反応のモンテカルロ計算:星間粒子を模擬した糖合成実験の再現に向けて

*竹原 仁1、庄司 大悟2、井田 茂3 (1.東京工業大学、2.宇宙航空研究開発機構、3.地球生命研究所)

Because organic molecules are essential materials for life, their synthesis in a prebiotic environment is an important topic for the origin of life. Of the many organic molecules, because ribose is the component of RNA, sugar is a key prebiotic material. Meinert et al. (2016) reported that many kinds of sugar, including ribose, were detected from interstellar ice analogs radiating UV in a high vacuum chamber. They suggested that formose reaction may have occurred to form ribose and related sugars. However, it is not easy from laboratory experiments to know what kind of synthesis path actually occurred and when sugars were formed.
In order to know the details of sugar synthesis reaction in Meinert’s experiment, we performed numerical simulations based on the classical Dugundji–Ugi algebraic model.
We started the simulations from H2O and CH3OH, corresponding to the condition of Meinert’s experiment. For simplicity, we simulated the condition of UV irradiation by setting the temperature at T=105 K, which corresponds to ~10 eV of UV energy.
From the simulation results, we found that the amount of sugar production increased when we warmed up to room temperature. In addition, we got some different reaction paths from formose reaction and we can suggest that sugar may be produced by a different kind of reaction in Meinert’s experiment.