Schuerger Andrew C, Mickol Rebecca L, Schwendner Petra
Space Life Sciences Laboratory, Department of Plant Pathology, University of Florida, 505 Odyssey Way, Exploration Park, Merritt Island, FL 32953, USA.
American Society for Engineering Education, 1818 N St NW #600, Washington, DC 20036, USA.
Life (Basel). 2020 May 26;10(6):77. doi: 10.3390/life10060077.
The search for life on Mars is predicated on the idea that Earth and Mars life (if present) should be both carbon- and water-based with similar forms of evolution. However, the astrobiology community can currently only investigate plausible Martian microbial ecosystems by using Terran life-forms as proxies. In order to examine how life might persist on Mars, we used a hypopiezotolerant bacterium (def., able to grow at 7-10 hPa)--in growth assays with four Mars analog soils conducted under a subset of simulated Martian conditions including 7 hPa, 0 °C, and a CO-enriched anoxic atmosphere (called conditions). The four Mars analog soils included an dust analog, the Mars analog, a lander-site simulant, and a high- analog. cells were able to grow at 30 °C in a liquid minimal basal medium (MBM) supplemented with 10- or 20-mM sucrose, Spizizen salts, and micronutrients. When the four analog soils were doped with both MBM and cells of , and subsequently incubated at 30 °C for 72 h, cell densities increased between 2-logs ( analog) and 4-logs ( and analogs); the analog led to complete inactivation of within 24 h. In contrast, when the experiment was repeated, but incubated under conditions, cells were either killed immediately by the analog, or decreased by > 5 logs over 28 d by the , , and analogs. The failure of to grow in the analog soils under conditions was attributed to the synergistic interactions among six factors (i.e., low pressure, low temperature, anoxic atmosphere (i.e., the conditions), low-pH in the soil, dissolved salts in all analogs, and oligotrophic conditions) that increased the biocidal or inhibitory conditions within the analog soils. Results suggest that even if a hypopiezotolerant Terran microbe is displaced from a spacecraft surface on Mars, and lands in a hydrated and nutrient-rich niche, growth in the Martian regolith is not automatically assured.
对火星生命的探索基于这样一种观点,即地球和火星上的生命(如果存在的话)都应以碳和水为基础,且具有相似的进化形式。然而,目前天体生物学界只能通过将地球生命形式作为替代物来研究可能存在的火星微生物生态系统。为了研究生命如何在火星上存续,我们使用了一种耐低压细菌(定义为能够在7 - 10百帕压力下生长),在包括7百帕、0°C和富含一氧化碳的缺氧大气(称为条件)的部分模拟火星条件下,与四种火星模拟土壤进行生长试验。这四种火星模拟土壤包括一种沙尘模拟物、火星模拟物、一个着陆器站点模拟物和一个高模拟物。细胞能够在补充有10或20毫摩尔蔗糖、斯皮兹森盐和微量营养素的液体基本培养基(MBM)中于30°C下生长。当四种模拟土壤中加入MBM和细胞,随后在30°C下孵育72小时时,细胞密度增加了2个对数(模拟物)到4个对数(模拟物和模拟物);模拟物在24小时内导致完全失活。相比之下,当重复该实验但在条件下孵育时,细胞要么立即被模拟物杀死,要么在28天内被模拟物、模拟物和模拟物减少超过5个对数。在条件下模拟土壤中无法生长归因于六个因素之间的协同相互作用(即低压、低温、缺氧大气(即条件)、土壤中的低pH值、所有模拟物中的溶解盐和贫营养条件),这些因素增加了模拟土壤中的杀菌或抑制条件。结果表明,即使一种耐低压的地球微生物从火星上的航天器表面被转移,并落在一个有水合作用且营养丰富的生态位中,也不能自动确保其在火星风化层中生长。