在地球早期的益生菌环境中的紫外线传播
Zoe R Todd1,2, Gabriella G Lozano3, Corinna L Kufner3
1Department of Earth and Space Sciences, University of Washington, Seattle, Washington, USA.
Astrobiology
|May 20, 2024
概括
紫外线 (UV) 光影响了生命早期的化学反应. 研究人员测量了益生菌分子的紫外线吸收,发现更简单的分子吸收的紫外线比核基如腺因少,影响紫外线透到早期的地球水域.
科学领域:
- 天体生物学 天体生物学
- 生命的起源研究 生命的起源研究
- 摄影化学的使用.
背景情况:
- 紫外线 (UV) 辐射是生命起源的关键因素.
- 紫外线可以驱动益生菌化学,但其通过早期地球水域的传播受到很小的约束.
- 要了解紫外线的作用,就需要了解紫外线被益生菌分子吸收的情况.
研究的目的:
- 实验性地确定与前生物合成相关的分子的紫外线吸收特性.
- 提供数据来建模UV光子透在可信的早期地球水生环境中的数据.
- 改进对生命起源的条件和化学途径的限制.
主要方法:
- 测量小微生物原料分子的摩尔十年灭绝系数.
- 对紫外线吸收光谱的实验性确定.
- 简单分子的吸收光谱与核基 (例如,腺因) 的吸收光谱的比较.
主要成果:
- 许多小的益生菌原料分子在短波长 (~200 nm) 时表现出最大的紫外线吸收.
- 紫外线的吸收通常会随着这些分子的波长的增加而减少.
- 与更简单的益生菌分子相比,核基腺因显示显著更高的紫外线吸收.
结论:
- 测量的灭绝系数允许计算紫外线光子透深度在前生物水中.
- 结果有助于限制生命场景起源的可信性和自我一致性.
- 对益生菌紫外线环境的更好理解有助于定义早期生命形成所必需的化学和环境条件.
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