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非嗜盐细菌在钠-镁-硫酸盐-氯化物离子体系中的生长:揭示陆地和地外水相环境中离子相互作用的复杂性。

Growth of Non-Halophilic Bacteria in the Sodium-Magnesium-Sulfate-Chloride Ion System: Unravelling the Complexities of Ion Interactions in Terrestrial and Extraterrestrial Aqueous Environments.

机构信息

UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom.

出版信息

Astrobiology. 2020 Aug;20(8):944-955. doi: 10.1089/ast.2019.2092. Epub 2020 May 20.

DOI:10.1089/ast.2019.2092
PMID:32434375
Abstract

Motivated by an interest in understanding the habitability of aqueous environments on Earth and in extraterrestrial settings, this study investigated the influence of ions in an artificial sodium-magnesium-sulfate-chloride ion system on the growth parameters (lag phase, growth rate, and final cell concentration) of bacteria. These four ions, in different combinations, are key components of many aqueous environments on Earth and elsewhere. We investigated non-halophilic bacteria deliberately to remove the bias of prior adaptations to high concentrations of selected ions so that we could compare the effects of different ions. We tested the hypothesis that water activity determined the growth parameters independent of the ion types. Neither water activity or ionic strength alone could predict growth. However, when ionic strengths were matched, many differences in growth parameters could be explained by the water activity. We suggest that species-specific effects (caused by differences in biochemical and physiological influences), the role of individual ions in cellular processes, and potentially the chaotropicity and kosmotropicity of solutions influenced the growth. Our data show that although extreme combinations of these ions allow for general predictions on the habitability of extraterrestrial aqueous environments, a complex interplay of ionic effects influences the growth and thus the adaptations required for given ion combinations. The data also show that an accurate quantification of the habitability of ocean worlds, such as Europa and Enceladus, can only be made when samples are obtained from these water bodies and the ion combinations are determined.

摘要

受研究地球和外星环境中水生环境宜居性的兴趣所驱动,本研究调查了人工钠离子-镁离子-硫酸盐-氯离子体系中离子对细菌生长参数(迟滞期、生长速率和最终细胞浓度)的影响。这四种离子以不同组合形式存在于地球上和其他地方的许多水生环境中,是关键组成部分。我们特意研究了非嗜盐细菌,以消除先前对高浓度选定离子适应的偏见,从而可以比较不同离子的影响。我们检验了这样一个假设,即水活度独立于离子类型决定了生长参数。水活度或离子强度单独都不能预测生长。然而,当离子强度相匹配时,许多生长参数的差异可以用水活度来解释。我们认为,物种特异性影响(由生化和生理影响的差异引起)、离子在细胞过程中的作用,以及溶液的离液性和反离液性可能影响了生长。我们的数据表明,尽管这些离子的极端组合允许对外星水生环境的宜居性进行一般预测,但离子效应的复杂相互作用影响了生长,从而影响了给定离子组合所需的适应性。数据还表明,只有当从这些水体中获得样本并确定离子组合时,才能准确量化欧罗巴和恩克拉多斯等海洋世界的宜居性。

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