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硫酸镁和氯酸钾饱和及共晶溶液中的细菌生长与火星和海洋世界的关系

Bacterial Growth in Saturated and Eutectic Solutions of Magnesium Sulphate and Potassium Chlorate with Relevance to Mars and the Ocean Worlds.

作者信息

Wilks Jonathan M, Chen Fei, Clark Benton C, Schneegurt Mark A

机构信息

Department of Biological Sciences, Wichita State University, Wichita, KS.

Planetary Protection Group, Jet Propulsion Laboratory, Pasadena CA.

出版信息

Int J Astrobiol. 2019 Dec;18(6):502-509. doi: 10.1017/s1473550418000502. Epub 2019 Jan 28.

Abstract

Liquid water on Mars might be created by deliquescence of hygroscopic salts or by permafrost melts, both potentially forming saturated brines. Freezing point depression allows these heavy brines to remain liquid in the near-surface environment for extended periods, perhaps as eutectic solutions, at the lowest temperatures and highest salt concentrations where ices and precipitates do not form. Perchlorate and chlorate salts and iron sulfate form brines with low eutectic temperatures and may persist under Mars near-surface conditions, but are chemically harsh at high concentrations and were expected to be incompatible with life, while brines of common sulfate salts on Mars may be more suitable for microbial growth. Microbial growth in saturated brines also may be relevant beyond Mars, to the oceans of Ceres, Enceladus, Europa and Pluto. We have previously shown strong growth of salinotolerant bacteria in media containing 2 M MgSO heptahydrate (~50% w/v) at 25 °C. Here we extend those observations to bacterial isolates from Basque Lake, BC and Hot Lake, WA, that grow well in saturated MgSO medium (67%) at 25 °C and in 50% MgSO medium at 4 °C (56% would be saturated). Psychrotolerant, salinotolerant microbes isolated from Basque Lake soils included and , which were identified by 16S rRNA gene sequencing and characterized phenetically. Eutectic liquid medium constituted by 43% MgSO at -4 °C supported copious growth of these psychrotolerant isolates, among others. Bacterial isolates also grew well at the eutectic for K chlorate (3% at -3 °C). Survival and growth in eutectic solutions increases the possibility that microbes contaminating spacecraft pose a contamination risk to Mars. The cold brines of sulfate and (per)chlorate salts that may form at times on Mars through deliquescence or permafrost melt have now been demonstrated to be suitable microbial habitats, should appropriate nutrients be available and dormant cells become vegetative.

摘要

火星上的液态水可能是由吸湿盐的潮解作用或永久冻土融化形成的,这两种情况都有可能形成饱和盐水。冰点降低使得这些浓盐水能够在近地表环境中长时间保持液态,也许是以共熔溶液的形式,处于不形成冰和沉淀物的最低温度和最高盐浓度条件下。高氯酸盐、氯酸盐和硫酸铁形成的盐水具有较低的共熔温度,可能在火星近地表条件下持续存在,但在高浓度时化学性质较为恶劣,预计与生命不相容,而火星上常见硫酸盐的盐水可能更适合微生物生长。饱和盐水中的微生物生长可能不仅与火星有关,还与谷神星、土卫二、木卫二和冥王星的海洋有关。我们之前已经表明,耐盐细菌在含有2 M七水硫酸镁(~50% w/v)的培养基中于25°C时生长旺盛。在此,我们将这些观察结果扩展到从加拿大不列颠哥伦比亚省的巴斯克湖和华盛顿州的霍特湖分离出的细菌菌株,它们在25°C的饱和硫酸镁培养基(67%)中以及在4°C的50%硫酸镁培养基(56%时为饱和状态)中生长良好。从巴斯克湖土壤中分离出的耐低温、耐盐微生物包括 和 ,它们通过16S rRNA基因测序进行鉴定,并进行了表型特征分析。由43%硫酸镁在-4°C构成的共熔液体培养基支持了这些耐低温 分离株以及其他一些菌株的大量生长。细菌分离株在氯酸钾的共熔温度(-3°C时为3%)下也生长良好。在共熔溶液中的存活和生长增加了污染航天器的微生物对火星构成污染风险的可能性。现在已经证明,通过潮解或永久冻土融化有时可能在火星上形成的硫酸盐和(高)氯酸盐冷盐水,如果有合适的养分且休眠细胞能够复苏,就是适合微生物生存的栖息地。

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