Bains William, Petkowski Janusz J, Seager Sara
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA.
School of Physics & Astronomy, Cardiff University, Cardiff, UK.
Astrobiology. 2024 Dec;24(12):1231-1256. doi: 10.1089/ast.2024.0004. Epub 2024 Dec 2.
Life is a complex, dynamic chemical system that requires a dense fluid solvent in which to take place. A common assumption is that the most likely solvent for life is liquid water, and some researchers argue that water is the only plausible solvent. However, a persistent theme in astrobiological research postulates that other liquids might be cosmically common and could be solvents for the chemistry of life. In this article, we present a new framework for the analysis of candidate solvents for life, and we deploy this framework to review substances that have been suggested as solvent candidates. We categorize each solvent candidate through the following four criteria: occurrence, solvation, solute stability, and solvent chemical functionality. Our semiquantitative approach addresses all the requirements for a solvent not only from the point of view of its chemical properties but also from the standpoint of its biochemical function. Only the protonating solvents fulfill all the chemical requirements to be a solvent for life, and of those only water and concentrated sulfuric acid are also likely to be abundant in a rocky planetary context. Among the nonprotonating solvents, liquid CO stands out as a planetary solvent, and its potential as a solvent for life should be explored. We conclude with a discussion of whether it is possible for a biochemistry to change solvents as an adaptation to radical changes in a planet's environment. Our analysis provides the basis for prioritizing future experimental work to explore potential complex chemistry on other planets. Key Words: Habitability-Alternative solvents for life-Alternative biochemistry. Astrobiology 24, 1231-1256.
生命是一个复杂、动态的化学系统,其发生需要一种稠密的流体溶剂。一个普遍的假设是,生命最可能的溶剂是液态水,一些研究人员认为水是唯一合理的溶剂。然而,天体生物学研究中一个持续的观点假定,其他液体可能在宇宙中很常见,并且可能是生命化学过程的溶剂。在本文中,我们提出了一个分析生命候选溶剂的新框架,并运用这个框架来审视那些被提议作为候选溶剂的物质。我们通过以下四个标准对每个候选溶剂进行分类:存在情况、溶剂化作用、溶质稳定性和溶剂化学功能。我们的半定量方法不仅从化学性质的角度,而且从生化功能的角度满足了对一种溶剂的所有要求。只有质子化溶剂满足作为生命溶剂的所有化学要求,而在这些溶剂中,只有水和浓硫酸在岩石行星环境中也可能大量存在。在非质子化溶剂中,液态CO作为一种行星溶剂脱颖而出,其作为生命溶剂的潜力值得探索。我们最后讨论了生物化学是否有可能改变溶剂以适应行星环境的剧烈变化。我们的分析为优先开展未来实验工作以探索其他行星上潜在的复杂化学过程提供了基础。关键词:宜居性-生命的替代溶剂-替代生物化学。《天体生物学》24卷,1231 - 1256页