Abstract
The Yilgarn Craton in Australia has a large number of naturally occurring shallow ephemeral lakes underlain by a dendritic system of paleodrainage channels. Processes like evaporation, flooding, erosion, as well as inflow of saline, often acidic and ion-rich groundwater contribute to the (dynamic) nature of the lakes and the composition of the sediments. The region has previously been described as an analog environment for early Mars due to its geological and geophysical similarities. Here, we investigated sediment samples of four lake environments aimed at getting a fundamental understanding of the native microbial communities and the mineralogical and (bio)chemical composition of the sediments they are associated with. The dominant mineral phases in the sediments were quartz, feldspars and amphiboles, while halite and gypsum were the only evaporites detected. Element analysis revealed a rich and complex image, in which silicon, iron, and aluminum were the dominant ions, but relative high concentrations of trace elements such as strontium, chromium, zirconium, and barium were also found. The concentrations of organic carbon, nitrogen, and phosphorus were generally low. 16S amplicon sequencing on the Illumina platform showed the presence of diverse microbial communities in all four lake environments. We found that most of the communities were dominated by extremely halophilic Archaea of the Halobacteriaceae family. The dynamic nature of these lakes appears to influence the biological, biochemical, and geological components of the ecosystem to a large effect. Inter-and intra-lake variations in the distributions of microbial communities were significant, and could only to a minor degree be explained by underlying environmental conditions. The communities are likely significantly influenced by small scale local effects caused by variations in geological settings and dynamic interactions caused by aeolian transport and flooding and evaporation events.
Original language | English |
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Article number | 779 |
Pages (from-to) | 1-19 |
Number of pages | 19 |
Journal | Frontiers in Microbiology |
Volume | 10 |
Issue number | MAY |
DOIs | |
Publication status | Published - 6 May 2019 |
Funding
This study was supported by the User Support Programme Space Research (Grant ALW-GO/13-09) of the Netherlands Organisation for Scientific Research (NWO), STFC (Grant ST/J001260/1) and by a Royal Society International Exchanges grant (IE121318). This work was financed by FEDER ? Fundo Europeu de Desenvolvimento Regional funds through the COMPETE 2020 ? Operacional Programme for Competitiveness and Internationalisation (POCI), and by Portuguese funds through FCT ? Funda??o para a Ci?ncia e a Tecnologia in the framework of the project POCI-01-0145-FEDER-029932 (PTDC/FIS-AST/29932/2017).
Funders | Funder number |
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Science and Technology Facilities Council | ST/J001260/1 |
Royal Society | IE121318 |
Fundação para a Ciência e a Tecnologia | PTDC/FIS-AST/29932/2017, POCI-01-0145-FEDER-029932 |
Nederlandse Organisatie voor Wetenschappelijk Onderzoek | |
European Regional Development Fund |
Keywords
- 16S sequencing
- Geology
- Halophiles
- Mars
- Microbial communities
- Yilgarn Craton