Programa de Pós-Graduação Em Química, Institute of Chemistry, University of São Paulo, São Paulo, Brazil.
Programa de Pós-Graduação Em Bioquímica E Biologia Molecular, Institute of Chemistry, University of São Paulo, São Paulo, Brazil.
Sci Rep. 2024 Jun 27;14(1):14885. doi: 10.1038/s41598-024-64246-7.
Past and present habitability of Mars have been intensely studied in the context of the search for signals of life. Despite the harsh conditions observed today on the planet, some ancient Mars environments could have harbored specific characteristics able to mitigate several challenges for the development of microbial life. In such environments, Fe minerals like siderite (already identified on Mars), and vivianite (proposed, but not confirmed) could sustain a chemolithoautotrophic community. In this study, we investigate the ability of the acidophilic iron-oxidizing chemolithoautotrophic bacterium Acidithiobacillus ferrooxidans to use these minerals as its sole energy source. A. ferrooxidans was grown in media containing siderite or vivianite under different conditions and compared to abiotic controls. Our experiments demonstrated that this microorganism was able to grow, obtaining its energy from the oxidation of Fe that came from the solubilization of these minerals under low pH. Additionally, in sealed flasks without CO, A. ferrooxidans was able to fix carbon directly from the carbonate ion released from siderite for biomass production, indicating that it could be able to colonize subsurface environments with little or no contact with an atmosphere. These previously unexplored abilities broaden our knowledge on the variety of minerals able to sustain life. In the context of astrobiology, this expands the list of geomicrobiological processes that should be taken into account when considering the habitability of environments beyond Earth, and opens for investigation the possible biological traces left on these substrates as biosignatures.
过去和现在火星的可居住性在寻找生命迹象的背景下得到了深入研究。尽管今天在火星上观察到了恶劣的条件,但一些古老的火星环境可能具有特定的特征,能够减轻微生物生命发展的一些挑战。在这样的环境中,像菱铁矿(已经在火星上被识别)和磷铁石(已提出,但尚未被证实)这样的铁矿物可以维持化能自养生物群落。在这项研究中,我们研究了嗜酸氧化铁化细菌嗜酸氧化亚铁硫杆菌利用这些矿物质作为其唯一能源的能力。在不同条件下,将 A. ferrooxidans 在含有菱铁矿或磷铁石的培养基中生长,并与非生物对照进行比较。我们的实验表明,这种微生物能够生长,从这些矿物质在低 pH 值下溶解所产生的铁的氧化中获得能量。此外,在没有 CO 的密封烧瓶中,A. ferrooxidans 能够直接从菱铁矿释放的碳酸盐离子中固定碳用于生物量生产,这表明它能够在与大气几乎没有或没有接触的地下环境中定殖。这些以前未被探索的能力拓宽了我们对能够维持生命的各种矿物质的认识。在天体生物学方面,这扩大了在考虑地球以外环境的可居住性时应考虑的地质微生物过程列表,并为研究这些基质上可能留下的作为生物特征的生物痕迹开辟了道路。