Schirmack Janosch, Alawi Mashal, Wagner Dirk
Alfred Wegener Institute, Helmholtz Center for Polar and Marine Research - Research Unit Potsdam, Potsdam Germany.
GFZ German Research Centre for Geosciences, Section 4.5 Geomicrobiology, Potsdam Germany.
Front Microbiol. 2015 Mar 20;6:210. doi: 10.3389/fmicb.2015.00210. eCollection 2015.
Methanogenic archaea have been studied as model organisms for possible life on Mars for several reasons: they can grow lithoautotrophically by using hydrogen and carbon dioxide as energy and carbon sources, respectively; they are anaerobes; and they evolved at a time when conditions on early Earth are believed to have looked similar to those of early Mars. As Mars is currently dry and cold and as water might be available only at certain time intervals, any organism living on this planet would need to cope with desiccation. On Earth there are several regions with low water availability as well, e.g., permafrost environments, desert soils, and salt pans. Here, we present the results of a set of experiments investigating the influence of different Martian regolith analogs (MRAs) on the metabolic activity and growth of three methanogenic strains exposed to culture conditions as well as long-term desiccation. In most cases, concentrations below 1 wt% of regolith in the media resulted in an increase of methane production rates, whereas higher concentrations decreased the rates, thus prolonging the lag phase. Further experiments showed that methanogenic archaea are capable of producing methane when incubated on a water-saturated sedimentary matrix of regolith lacking nutrients. Survival of methanogens under these conditions was analyzed with a 400 day desiccation experiment in the presence of regolith analogs. All tested strains of methanogens survived the desiccation period as it was determined through reincubation on fresh medium and via qPCR following propidium monoazide treatment to identify viable cells. The survival of long-term desiccation and the ability of active metabolism on water-saturated MRAs strengthens the possibility of methanogenic archaea or physiologically similar organisms to exist in environmental niches on Mars. The best results were achieved in presence of a phyllosilicate, which provides insights of possible positive effects in habitats on Earth as well.
它们可以分别利用氢气和二氧化碳作为能量和碳源进行化能自养生长;它们是厌氧菌;并且它们在早期地球条件被认为与早期火星条件相似的时期进化而来。由于火星目前干燥寒冷,且水可能仅在特定时间间隔出现,任何生活在这个星球上的生物都需要应对干燥环境。在地球上也有一些水资源匮乏的地区,例如永久冻土环境、沙漠土壤和盐田。在此,我们展示了一组实验的结果,该实验研究了不同火星风化层模拟物(MRA)对三种产甲烷菌株在培养条件以及长期干燥环境下的代谢活性和生长的影响。在大多数情况下,培养基中低于1 wt%的风化层浓度会导致甲烷产生速率增加,而较高浓度则会降低速率,从而延长延迟期。进一步的实验表明,产甲烷古菌在缺乏营养物质的风化层水饱和沉积基质上培养时能够产生甲烷。在存在风化层模拟物的情况下,通过400天的干燥实验分析了产甲烷菌在这些条件下的存活情况。所有测试的产甲烷菌菌株都在干燥期存活了下来,这是通过在新鲜培养基上重新培养以及在单叠氮化丙锭处理后通过qPCR来鉴定活细胞确定的。长期干燥下的存活能力以及在水饱和MRA上的活跃代谢能力增强了产甲烷古菌或生理上相似的生物存在于火星环境生态位中的可能性。在存在层状硅酸盐的情况下取得了最佳结果,这也为地球上栖息地可能产生的积极影响提供了见解。