水活动和早期火星上生命的挑战
Nicholas J Tosca1, Andrew H Knoll, Scott M McLennan
1Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, MA 02138, USA. ntosca@fas.harvard.edu
概括
古代火星上有酸性,性液态水,但其高度可能超过已知的地球生命的极限. 这项研究探讨了火星环境中的水活动 (aH2O),发现潜在的条件对于微生物居住来说过于恶劣.
科学领域:
- 天体生物学 天体生物学
- 行星科学 行星科学
- 地质化学 地质化学
背景情况:
- 现场和轨道任务显示,古代火星拥有酸性,性液态水.
- 这种水的宜居性严重依赖于水活动 (aH2O),这是盐度的衡量标准.
- 陆地生命对水活动有明确的界限.
研究的目的:
- 为了计算古代火星表面水中的最大水活性 (aH2O).
- 根据盐度限制,评估这些水域对陆地生物的宜居性.
- 为了评估像Meridiani Planum这样的环境,盐从盐水中沉.
主要方法:
- 利用了来自火星数据的流体化学和盐酸矿物学的约束.
- 针对特定的火星环境计算的最大水活性 (aH2O).
- 将计算的aH2O水平与陆地生物的已知耐受性极限进行比较.
主要成果:
- 计算表明,有充分记录的火星地表水中的盐度往往超过了陆地生命的耐受性水平.
- 盐水矿物学和流体化学表明水活动非常低的条件.
- 像Meridiani Planum这样的环境可能经历过高盐度的条件.
结论:
- 古代火星的地表水,特别是在像Meridiani Planum这样的环境中,很可能太,无法支持已知的陆地生命.
- 这些盐水的热力学条件 (低aH2O) 挑战了与地球相似的外星生命的潜力.
- 需要进一步的研究,以了解火星上可居住性的全部范围.
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