1 Jet Propulsion Laboratory, California Institute of Technology , Pasadena, California.
2 Cooperative Institute for Research in Environmental Sciences, University of Colorado , Boulder, Colorado.
Astrobiology. 2017 Oct;17(10):997-1008. doi: 10.1089/ast.2016.1545.
Observed features such as recurring slope lineae suggest that liquid water may exist on the surface and near-subsurface of Mars today. The presence of this liquid water, likely in the form of a brine, has important implications for the present-day water cycle, habitability, and planetary protection policies. It is possible that this water is formed, at least partially, by deliquescence of salts, a process during which hygroscopic salts absorb water vapor from the atmosphere and form a saturated liquid brine. We performed laboratory experiments to examine the ability of Bacillus subtilis (B-168) spores, alone or mixed with calcium perchlorate salt (Ca(ClO)), to form liquid water via deliquescence under Mars-relevant conditions. Spore survival after exposure to these conditions was examined. An environmental chamber was used to expose the samples to temperature and relative humidity (RH) values similar to those found on Mars, and Raman microscopy was used to identify the phases of water and salt that were present and to confirm the presence of spores. We found that B-168 spores did not condense any detectable water vapor on their own during the diurnal cycle, even at 100% RH. However, when spores were mixed with perchlorate salt, the entire sample deliquesced at low RH values, immersing the spores in a brine solution during the majority of the simulated martian temperature and humidity cycle. After exposure to the simulated diurnal cycles and, in some cases, perchlorate brine, the impact of each environmental scenario on spore survival was estimated by standard plate assay. We found that, if there are deliquescent salts in contact with spores, there is a mechanism for the spores to acquire liquid water starting with only atmospheric water vapor as the HO source. Also, neither crystalline nor liquid Ca(ClO) is sporicidal despite the low water activity. Key Words: Raman microscopy-Mars-Planetary protection-Salts-Water activity. Astrobiology 17, 997-1008.
观察到的特征,如反复出现的斜坡条纹,表明液态水可能存在于火星表面和近表面。这种液态水的存在,可能是以盐水的形式存在,这对当今的水循环、可居住性和行星保护政策具有重要意义。这种水可能是由盐的潮解形成的,至少部分是这样,在这个过程中,吸湿盐从大气中吸收水蒸气并形成饱和液态盐水。我们进行了实验室实验,以研究枯草芽孢杆菌(B-168)孢子单独或与高氯酸盐(Ca(ClO ) )混合在火星相关条件下通过潮解形成液态水的能力。检查了暴露于这些条件后的孢子存活率。使用环境室使样品暴露于类似于火星上发现的温度和相对湿度(RH)值,并使用拉曼显微镜来识别存在的水相和盐相,并确认孢子的存在。我们发现,B-168 孢子在白天的循环中即使在 100%的 RH 下也不能自行凝结任何可检测到的水蒸气。但是,当孢子与高氯酸盐混合时,整个样品在低 RH 值下潮解,在模拟火星温度和湿度循环的大部分时间里将孢子浸泡在盐水中。暴露于模拟的昼夜循环后,在某些情况下暴露于高氯酸盐盐水后,通过标准平板测定法估计了每种环境情况对孢子存活率的影响。我们发现,如果有潮解盐与孢子接触,则存在一种机制,使孢子可以从仅大气水蒸气作为 HO 源开始获得液态水。此外,尽管水活度低,但无论是结晶态还是液态 Ca(ClO )都没有杀菌作用。关键词:拉曼显微镜-火星-行星保护-盐-水活度。天体生物学 17,997-1008。