形成地球外的和它们的衍生物
Serge A Krasnokutski1, Cornelia Jäger1, Thomas Henning2
1Laboratory Astrophysics Group of the Max Planck Institute for Astronomy at the Friedrich Schiller University Jena, Helmholtzweg 3, D-07743 Jena, Germany.
Science advances
|April 17, 2024
概括
科学家们在类似太空的条件下合成了,证实了生命起源的途径. 水的存在稍微降低了的形成效率,但没有阻止它,这表明了强大的前生物化学.
科学领域:
- 天体生物学 天体生物学
- 化学进化的化学进化
- 天体化学是天体化学.
背景情况:
- 生命的起源可能涉及星际空间中有机分子的前生物合成.
- 在外星条件下了解的形成对天体生物学至关重要.
研究的目的:
- 在模拟的星际条件下通过aminoketene聚合来研究的形成.
- 为了确定水分子对这种合成途径的效率的影响.
主要方法:
- 模拟星际分子云的低温,低密度条件.
- 使用碳 (C),一氧化碳 (CO) 和氨 (NH3) 的合成实验.
- 用碳-13 (13C) 的同位素标记来追踪反应途径.
- 用水和没有水 (H2O) 的反应产物的分析.
主要成果:
- 通过氨基基分子的聚合,确认了的形成.
- 证明C + CO + NH3反应是获得前体的可行途径.
- 在水的存在下观察到聚合效率略有降低.
- 证实水不会抑制的形成.
结论:
- 在星际条件下,的形成是可能的,为生命起源提供了替代途径.
- 太空中常见的水的存在并不排除必要的生物分子的合成.
- 这项研究支持了生命构建块的外星起源假设.
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