EXTREMOPHILES as Astrobiological Models. Группа авторов

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EXTREMOPHILES as Astrobiological Models - Группа авторов

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alt="Photos depict the comparison between ferruginous deposits of the Burns Formation (a) cropping up in the Endurance Crater and those formed by acidic fluvial activity (b) in Rio Tinto. In the fluvial deposits of Rio Tinto, jarosite and hematite were detected using different techniques such as X-ray diffraction (c), which form as a consequence of the low pH. "/>

      Considering the geomicrobiological characteristics of the Tinto ecosystem we propose that Rio Tinto is mainly under the control of iron [2.7]. Iron oxidizing microorganisms are responsible for the solubilization of the massive metal sulfides of the IPB and the associated high concentrations of iron and sulfate measured in the river. Iron has diverse properties of biological interest, which make the Rio Tinto basin an attractive astrobiological precedent [2.11]. Reduced iron is a good electron donor for respiration (both aerobic and anaerobic). Oxidized iron is a useful electron acceptor for anaerobic respiration. Oxidized iron is also a good buffer for controlling the pH of the system. Moreover, it has been shown that soluble ferric iron can protect sensitive organisms from damaging UV radiation [2.54] [2.55].

      This iron-controlled environment appears to be adequate for the chemolithotrophic microorganisms detected in the Tinto basin. Nonetheless, taking into consideration that eukaryotic diversity seems to be much greater than prokaryotic [2.72] [2.5] [2.3], and that most of the primary production in the system depends on eukaryotic photosynthesis, how do eukaryotes benefit from adapting to an extreme acidic environment with high concentration of toxic heavy metals? One possible answer to this question might be related to free access to an indispensable element for life, iron. Iron is difficult to obtain at neutral pH, due to its meager solubility in this condition [2.14] [2.77] [2.19] [2.18]. A reliable advantage for the eukaryotes growing in the Tinto basin is an unrestricted iron supply provided by the chemolithotrophy promoted by the extremely high concentration of IPB iron sulfides [2.53] [2.7] [2.11].

      As discussed above, we favor the hypothesis that the extreme conditions of pH and the high concentration of heavy metals detected along the Tinto basin is the result of an underground bioreactor in which interaction of metal sulfides, underground water and chemolithoautotrophic microorganisms generates the metabolic products, mainly iron and sulfuric acid, detected in the river. To demonstrate this hypothesis two devoted drilling projects to intersect this subsurface bioreactor and obtain information on the oxidation of metal sulfides in anaerobic conditions were carried out.

      The central objective of the first, the Mars Astrobiology Research and Technology Experiment (MARTE project), a joint effort between the Centro de Astrobiología (CAB, CSIC-INTA) and the NASA Astrobiology Institute (NAI), was to gather information about the microbial activity operating in the subsurface of the IPB. Peña de Hierro (Iron Mountain, a recurrent name associated with mining operations), on the north flank of Rio Tinto anticline, was selected for drilling. Complex massive sulfide lenses or stockwork veins of pyrite and quartz generated by hydrothermal activity can be found at the upper part of the IPB volcanic sequence [2.69]. Faults intersect the Early Carboniferous volcanic tuff-hosted pyrite bodies.

      Water from upslope springs was used to characterize the groundwater before contacting the ore body. The water from these springs had a neutral pH, a low ionic content and was saturated with O2. The environmental conditions within the ore body were obtained from the analysis of the core samples of two drilling boreholes, BH4 and BH8, at a depth of 165 mbs, separated by a distance of 10 m. The water table was detected at 90 mbs in both boreholes.

Photo depicts the process of the selected cores for the generation of samples in an anaerobic chamber in the Museo Minero laboratory.

      Twice a year the MLDS were analyzed to follow the evolution of fluid formation in the boreholes. Similar patterns were observed for both boreholes. The average pH was ca. 3.5 and remained acidic for two years after drilling. Sulfate concentrations were lower than in rock leachates. The dissolved, oxidized and reduced iron ratios were variable along the length of the borehole, underlying the functional activity of the iron cycle. The highest concentration of dissolved H2 was found in the upper part of the water table and dissolved methane was detected in many samples, indicating methanogenic activity in the subsurface of the IPB [2.40] [2.9].

      Core samples from both boreholes were examined with an antibody microarray (LDCHIP200) [2.85] and an oligonucleotide hybridization microarray [2.50], giving positive signals for sulfur and iron oxidizers, methanogenic archaea, sulfate reducers and Gram-positive bacteria. Denitrifying and hydrogenotrophic bacteria were identified by 16S rRNA cloning and sequencing. Enrichment cultures showed the presence of aerobic pyrite and iron oxidizers, anaerobic respiration of thiosulfate using nitrate, sulfate reducers and methanogens at different depths [2.87] [2.11].

      The environment down-gradient from the metal sulfide ore body was sampled by drilling borehole BH1. Compared to BH4 and BH8 boreholes, BH1 showed lower iron and sulfate concentrations in the leachates while sulfate concentrations in the MLDS were much higher, indicating that the groundwater had a strong interaction with the ore. Dissolved hydrogen had lower concentrations and dissolved methane had higher concentration in BH1 than in BH4 and BH8. Enrichment cultures with samples from this borehole showed mainly methanogenic and sulfate-reducing activities [2.40] [2.9].

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