Oliver James A W, Kelbrick Matthew, Ramkissoon Nisha K, Dugdale Amy, Stephens Ben P, Kucukkilic-Stephens Ezgi, Fox-Powell Mark G, Schwenzer Susanne P, Antunes André, Macey Michael C
Biology Department, Edge Hill University, Ormskirk L39 4QP, UK.
Department of Evolution, Ecology and Behaviour, Institute of Infection, Veterinary and Ecological Sciences, University of Liverpool, Liverpool L69 3GJ, UK.
Life (Basel). 2022 Apr 1;12(4):523. doi: 10.3390/life12040523.
Water present on the surface of early Mars (>3.0 Ga) may have been habitable. Characterising analogue environments and investigating the aspects of their microbiome best suited for growth under simulated martian chemical conditions is key to understanding potential habitability. Experiments were conducted to investigate the viability of microbes from a Mars analogue environment, Colour Peak Springs (Axel Heiberg Island, Canadian High Arctic), under simulated martian chemistries. The fluid was designed to emulate waters thought to be typical of the late Noachian, in combination with regolith simulant material based on two distinct martian geologies. These experiments were performed with a microbial community from Colour Peak Springs sediment. The impact on the microbes was assessed by cell counting and 16S rRNA gene amplicon sequencing. Changes in fluid chemistries were tested using ICP-OES. Both chemistries were shown to be habitable, with growth in both chemistries. Microbial communities exhibited distinct growth dynamics and taxonomic composition, comprised of sulfur-cycling bacteria, represented by either sulfate-reducing or sulfur-oxidising bacteria, and additional heterotrophic halophiles. Our data support the identification of Colour Peak Springs as an analogue for former martian environments, with a specific subsection of the biota able to survive under more accurate proxies for martian chemistries.
早期火星(>30亿年前)表面存在的水可能适宜居住。对类似环境进行特征描述,并研究其微生物群落中最适合在模拟火星化学条件下生长的方面,是理解潜在宜居性的关键。开展了实验,以研究来自火星类似环境——彩色峰泉(加拿大北极地区阿克塞尔·海伯格岛)的微生物在模拟火星化学条件下的生存能力。该流体旨在模拟被认为是晚诺亚纪典型的水,并结合基于两种不同火星地质的风化层模拟材料。这些实验是用来自彩色峰泉沉积物的微生物群落进行的。通过细胞计数和16S rRNA基因扩增子测序评估对微生物的影响。使用电感耦合等离子体发射光谱仪(ICP-OES)测试流体化学性质的变化。两种化学条件都显示出适宜居住,两种条件下微生物都有生长。微生物群落表现出不同的生长动态和分类组成,由硫循环细菌组成,以硫酸盐还原菌或硫氧化菌为代表,还有其他异养嗜盐菌。我们的数据支持将彩色峰泉确定为古代火星环境的类似物,其生物群的一个特定子部分能够在更精确的火星化学模拟条件下存活。