星际模拟冰中基硫酸的非生物形成及其对瑞古古探测的含义
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Updated: Jun 25, 2025

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Conducting Miller-Urey Experiments
Published on: January 21, 2014
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Mason McAnally1,2, Jana Bocková3, Ashanie Herath1,2
1Department of Chemistry, University of Hawaii at Mānoa, Honolulu, HI, USA.
Nature communications
|May 23, 2024
概括
早期生活 早期生活
科学领域:
- 天体生物学 天体生物学
- 有机地化学 有机地化学
- 宇宙化学 宇宙化学
背景情况:
- 硫在生命早期的起源仍然是一个关键的未解决的问题.
- 在S(+VI) 氧化状态 (硫酸盐) 中的硫是必不可少的,但在早期地球上很可能很少.
- 更容易溶解的S(+IV) 化合物可能是原始微生物的初始硫源.
研究的目的:
- 为了研究S(+IV) 有机硫化合物的外星合成.
- 探索早期生命中硫的结合的潜在益生菌途径.
主要方法:
- 实验室模拟实验使用硫化冰.
- 将冰暴露在银河系宇宙射线中,以模仿星际条件.
主要成果:
- 实现了简单基硫酸 (有机S(+IV) 化合物) 的高效生产.
- 这些化合物是水溶性和生物相关的.
- 合成发生在通过宇宙射线相互作用模拟的星际冰中.
结论:
- 银河系宇宙射线可以在地球外的冰中合成必需的S(+IV) 有机硫化合物.
- 这提供了一个可信的非生物途径,通过石和彗星将硫输送到早期的地球.
- 这些发现提供了关于硫在第一批陆地生物中的起源的见解.
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