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首页> 外文期刊>Icarus: International Journal of Solar System Studies >Biotoxicity of Mars soils: 2. Survival of Bacillus subtilis and Enterococcus faecalis in aqueous extracts derived from six Mars analog soils
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Biotoxicity of Mars soils: 2. Survival of Bacillus subtilis and Enterococcus faecalis in aqueous extracts derived from six Mars analog soils

机译:火星土壤的生物毒性:2。枯草芽孢杆菌和肠球菌粪便中患有六个火星模拟土壤的水提取物的粪便

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The search for an extant microbiota on Mars depends on exploring sites that contain transient or permanent liquid water near the surface. Examples of possible sites for liquid water may be active recurring slope lineae (RSL) and fluid inclusions in ice or salt deposits. The presence of saline fluids on Mars will act to depress the freezing points of liquid water to as low as -60 degrees C, potentially permitting the metabolism and growth of halophilic microorganisms to temperatures significantly below the freezing point of pure water at 0 degrees C. In order to predict the potential risks of forward contamination by Earth microorganisms to subsurface sites on Mars with liquid brines, experiments were designed to characterize the short-term survival of two bacteria in aqueous soil solutions from six analog soils. The term "soil" is used here to denote any loose, unconsolidated matrix with no implications for the presence or absence of organics or biology. The analog soils were previously described (Schuerger et al., 2012, Planetary Space Sci., 72, 91-101), and represented crushed Basalt (benign control), Salt, Acid, Alkaline, Aeolian, and Phoenix analogs on Mars. The survival rates of spores of Bacillus subtilis and vegetative cells of Enterococcus faecalis were tested in soil solutions from each analog at 24, 0, or -70 degrees C for time periods up to 28 d. Survival of dormant spores of B. subtilis were mostly unaffected by incubation in the aqueous extracts of all six Mars analogs. In contrast, survival rates of E. faecalis cells were suppressed by all soil solutions when incubated at 24 degrees C but improved at 0 and -70 degrees C, except for assays in the Salt and Acid soil solutions in which most cells were killed. Results suggest that Earth microorganisms that form spores may persist in liquid brines on Mars better than non-spore forming species, and thus, spore-forming species may pose a potential forward contamination risk to sites with liquid brines. (C) 2017 Elsevier Inc. All rights reserved.
机译:搜索MAR上的现存微生物群取决于探索含有瞬态或永久性液体水的遗址。液态水的可能位点的实例可以是活性重复的斜率线eae(RSL)和冰或盐沉积物中的流体夹杂物。火星上的盐水液体的存在将使液态水的冷冻点压得低至-60℃,可能允许嗜盐微生物的代谢和生长在0摄氏度下显着低于纯水的冷冻点的温度。为了预测地球微生物向地下污染的潜在风险,用液体盐水对火星的地下部位进行潜在风险,设计实验以表征来自六种模拟土壤的两种细菌的​​短期存活。这里使用术语“土壤”来表示任何松散,未溶胀的基质,对有机物或生物学的存在或不存在没有任何影响。先前描述了模拟土壤(Schuerger等,2012年,行星空间SCI。,72,91-101),并代表粉碎的玄武岩(良性控制),盐,酸,碱性,风暴和火星上的凤凰类似物。在24,0或-70℃下的各种模拟中,在24,0或-70℃下的土壤溶液中测试胚芽芽孢杆菌孢子和肠杆菌植物和植物细胞的存活率。休眠孢子孢子的生存枯草芽孢杆菌主要不受所有六个火星类似物的含水提取物中的孵育。相反,当在24℃下孵育时,所有土壤溶液抑制E.粪便细胞的存活率,但在0和-70℃下改善,除了盐和酸性土壤溶液中的测定,其中大多数细胞被杀死。结果表明,形成孢子的地球微生物可能比非孢子成形物种更好地持续在火星上的液体盐水,因此,孢子形成物种可能对液体盐水的遗址造成潜在的前瞻性污染风险。 (c)2017年Elsevier Inc.保留所有权利。

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