一个富含硫生物分子的古老大气
Nathan W Reed1,2, Cade M Christensen3, Jason D Surratt3,4
1Department of Chemistry, University of Colorado Boulder, Boulder, CO 80309.
概括
星球上的有机雾化工学可以创造必要的硫生物分子,如非生物的氨酸. 这一发现弥合了早期生活之间的差距.
科学领域:
- 益生菌化学 益生菌化学
- 天体生物学 天体生物学
- 生命的起源研究 生命的起源研究
背景情况:
- 在温和条件下对硫生物分子的非生物合成仍然是一个挑战.
- 在硫独立的早期生命和硫依赖的后来的进化之间存在一个差距.
- 硫生物分子对现代生物学至关重要,但它们的前生物起源尚不清楚.
研究的目的:
- 研究含硫生物分子的非生物生产.
- 探索行星有机雾化学在产生这些分子中的作用.
- 挑战硫生物分子仅仅是生物发明的观念.
主要方法:
- 模拟行星有机雾化学.
- 分析由此产生的化学产品,寻找含硫生物分子.
- 评估大气沉积到早期地球环境中的潜力.
主要成果:
- 证明了氨酸,M辅酶和氨酸的产生.
- 确定了 metionin 和 homocysteine 的潜在形成途径.
- 展示了在高大气条件下形成的硫生物分子.
结论:
- 星球上的有机雾化学是前生物硫生物分子的可行来源.
- 这些分子可能已经可用于早期生命.
- 硫生物分子可能不需要生物发明.
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