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Pinto GA, Lezcano MÁ, Sanchéz-García L, Martínez R, Parro V, Carrizo D. Higher Microbial Biomass Accumulation on El Médano 464 Meteorite Compared with Adjacent Soils in the Atacama Desert. ASTROBIOLOGY 2025; 25:115-132. [PMID: 39969489 DOI: 10.1089/ast.2024.0071] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 02/20/2025]
Abstract
Chondritic meteorites can be appropriate substrates for the colonization of terrestrial microorganisms. However, determining whether organic compounds are intrinsic to the meteorite or come from external (terrestrial) contamination is still controversial. This research explores the molecular distribution and carbon isotopic composition of three lipid families (hydrocarbons, alkanoic acids, and alcohols) as well as DNA extracted from the interior of a CO carbonaceous chondrite named El Médano 464 (EM 464), discovered in the Atacama Desert in 2019. Three soil samples from the discovery area of EM 464 were collected and used as a background control for the composition and distribution of organic compounds. Our results revealed a higher abundance of the three lipid families in EM 464 compared with the surrounding soil samples. The organic compounds in EM 464 showed a mean δ13C value of -27.8 ± 0.5 for hydrocarbons (N = 20), -27.6 ± 1.1 for alkanoic acids (N = 17), and -27.5 ± 2.2‰ for alcohols (N = 18). These δ13C-depleted values are compatible with terrestrial biosignatures and are within isotopic values produced as a result of carbon fixation due to the Calvin cycle (δ13C of ca. from -19 to -34‰) widely used by photosynthetic terrestrial microorganisms. The DNA analysis (based on the bacterial 16S rRNA gene) showed a dominance of Proteobacteria (now Pseudomonadota) and Actinobacteriota in both meteorite and soils but exhibited different bacterial composition at the family level. This suggests that the microbial material inside the meteorite may have partially come from the adjacent soils, but we cannot rule out other sources, such as windborne microbes from distant locations. In addition, the meteorite showed higher bacterial diversity (H' = 2.4-2.8) compared with the three soil samples (H' = 0.3-1.8). Based on the distribution and δ13C value of organic compounds as well as DNA analysis, we suggest that most, if not all, of the organic compounds detected in the studied CO chondrite are of terrestrial origin (i.e., contamination). The terrestrial contamination of EM 464 by a diverse microbial community indicates that Atacama chondrites can offer distinctive ecological conditions for microorganisms to thrive in the harsh desert environment, which can result in an accumulation of microbial biomass and preservation of molecular fossils over time.
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Affiliation(s)
- Gabriel A Pinto
- Institute of Natural Sciences, Geological Survey of Belgium, Brussels, Belgium
- Laboratoire G-Time, Université Libre de Bruxelles, Brussels, Belgium
- Archaeology, Environmental Changes, and Geo-Chemistry, Vrije Universiteit Brussel, Brussels, Belgium
- INCT, Universidad de Atacama, Copiapó, Chile
| | - María Ángeles Lezcano
- Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain
- IMDEA Water Institute, Madrid, Spain
| | | | | | - Víctor Parro
- Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain
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2
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Lezcano MÁ, Bornemann TLV, Sánchez-García L, Carrizo D, Adam PS, Esser SP, Cabrol NA, Probst AJ, Parro V. Hyperexpansion of genetic diversity and metabolic capacity of extremophilic bacteria and archaea in ancient Andean lake sediments. MICROBIOME 2024; 12:176. [PMID: 39300577 PMCID: PMC11411797 DOI: 10.1186/s40168-024-01878-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/24/2024] [Accepted: 07/19/2024] [Indexed: 09/22/2024]
Abstract
BACKGROUND The Andean Altiplano hosts a repertoire of high-altitude lakes with harsh conditions for life. These lakes are undergoing a process of desiccation caused by the current climate, leaving terraces exposed to extreme atmospheric conditions and serving as analogs to Martian paleolake basins. Microbiomes in Altiplano lake terraces have been poorly studied, enclosing uncultured lineages and a great opportunity to understand environmental adaptation and the limits of life on Earth. Here we examine the microbial diversity and function in ancient sediments (10.3-11 kyr BP (before present)) from a terrace profile of Laguna Lejía, a sulfur- and metal/metalloid-rich saline lake in the Chilean Altiplano. We also evaluate the physical and chemical changes of the lake over time by studying the mineralogy and geochemistry of the terrace profile. RESULTS The mineralogy and geochemistry of the terrace profile revealed large water level fluctuations in the lake, scarcity of organic carbon, and high concentration of SO42--S, Na, Cl and Mg. Lipid biomarker analysis indicated the presence of aquatic/terrestrial plant remnants preserved in the ancient sediments, and genome-resolved metagenomics unveiled a diverse prokaryotic community with still active microorganisms based on in silico growth predictions. We reconstructed 591 bacterial and archaeal metagenome-assembled genomes (MAGs), of which 98.8% belonged to previously unreported species. The most abundant and widespread metabolisms among MAGs were the reduction and oxidation of S, N, As, and halogenated compounds, as well as aerobic CO oxidation, possibly as a key metabolic trait in the organic carbon-depleted sediments. The broad redox and CO2 fixation pathways among phylogenetically distant bacteria and archaea extended the knowledge of metabolic capacities to previously unknown taxa. For instance, we identified genomic potential for dissimilatory sulfate reduction in Bacteroidota and α- and γ-Proteobacteria, predicted an enzyme for ammonia oxidation in a novel Actinobacteriota, and predicted enzymes of the Calvin-Benson-Bassham cycle in Planctomycetota, Gemmatimonadota, and Nanoarchaeota. CONCLUSIONS The high number of novel bacterial and archaeal MAGs in the Laguna Lejía indicates the wide prokaryotic diversity discovered. In addition, the detection of genes in unexpected taxonomic groups has significant implications for the expansion of microorganisms involved in the biogeochemical cycles of carbon, nitrogen, and sulfur. Video Abstract.
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Affiliation(s)
- María Ángeles Lezcano
- Centro de Astrobiología (CAB), CSIC-INTA, 28850, Torrejón de Ardoz, Madrid, Spain.
- IMDEA Water Institute, Avenida Punto Com 2, 28805, Alcalá de Henares, Madrid, Spain.
| | - Till L V Bornemann
- Environmental Metagenomics, Research Center One Health Ruhr of the University Alliance Ruhr, Faculty of Chemistry, University of Duisburg-Essen, Essen, Germany
- Centre of Water and Environmental Research (ZWU), University of Duisburg-Essen, Essen, Germany
| | - Laura Sánchez-García
- Centro de Astrobiología (CAB), CSIC-INTA, 28850, Torrejón de Ardoz, Madrid, Spain
| | - Daniel Carrizo
- Centro de Astrobiología (CAB), CSIC-INTA, 28850, Torrejón de Ardoz, Madrid, Spain
| | - Panagiotis S Adam
- Environmental Metagenomics, Research Center One Health Ruhr of the University Alliance Ruhr, Faculty of Chemistry, University of Duisburg-Essen, Essen, Germany
- Institute of General Microbiology, Kiel University, Kiel, Germany
| | - Sarah P Esser
- Environmental Metagenomics, Research Center One Health Ruhr of the University Alliance Ruhr, Faculty of Chemistry, University of Duisburg-Essen, Essen, Germany
| | - Nathalie A Cabrol
- SETI Institute, 339 Bernardo Avenue, Suite 200, Mountain View, CA, 94043, USA
| | - Alexander J Probst
- Environmental Metagenomics, Research Center One Health Ruhr of the University Alliance Ruhr, Faculty of Chemistry, University of Duisburg-Essen, Essen, Germany
- Centre of Water and Environmental Research (ZWU), University of Duisburg-Essen, Essen, Germany
| | - Víctor Parro
- Centro de Astrobiología (CAB), CSIC-INTA, 28850, Torrejón de Ardoz, Madrid, Spain
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3
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Escribano-Álvarez P, Castro MG, Pertierra LR, Olalla-Tárraga MÁ. Intra and interspecific differences in desiccation tolerance in native and alien Antarctic springtails in geothermal grounds. JOURNAL OF EXPERIMENTAL ZOOLOGY. PART A, ECOLOGICAL AND INTEGRATIVE PHYSIOLOGY 2024; 341:357-363. [PMID: 38318929 DOI: 10.1002/jez.2789] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/27/2023] [Revised: 11/10/2023] [Accepted: 01/26/2024] [Indexed: 02/07/2024]
Abstract
The extreme low humidity and temperatures in Antarctica make it one of the harsher areas for life on our planet. In a global change context, environmental barriers that prevented the arrival of alien species in Antarctica are weakening. Deception Island, one of the four active volcanoes of Antarctica, is especially vulnerable to the impacts of alien species. Geothermal areas (GA) in this Island offer unique microclimatic conditions that could differentially affect native and alien soil arthropods. Here we explore the desiccation tolerance of a native (Cryptopygus antarcticus) and an alien (Proisotoma minuta) springtail (Collembola) species to these extreme environmental conditions. GA and non-geothermal areas (NGA) were selected to evaluate intra- and interspecific variation in desiccation tolerance. Populations of P. minuta from GA had greater desiccation tolerance than populations from NGA. However, desiccation tolerance of C. antarcticus did not differ between GA and NGA. This native species had greater desiccation tolerance than the alien P. minuta, but also greater body size. Our findings show that the alien P. minuta responds differently to environmental conditions than the native C. antarcticus. Furthermore, body size may influence desiccation tolerance in these two springtail species.
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Affiliation(s)
- Pablo Escribano-Álvarez
- Dpto, Biología, Geología, Física y Química Inorgánica. Instituto de Cambio Global. Universidad Rey Juan Carlos, Mostoles, Spain
| | - Mario G Castro
- Dpto, Biología, Geología, Física y Química Inorgánica. Instituto de Cambio Global. Universidad Rey Juan Carlos, Mostoles, Spain
| | - Luis R Pertierra
- Millennium Institute Biodiversity of Antarctic and Subantarctic Ecosystems (BASE), Santiago, Chile
| | - Miguel Á Olalla-Tárraga
- Dpto, Biología, Geología, Física y Química Inorgánica. Instituto de Cambio Global. Universidad Rey Juan Carlos, Mostoles, Spain
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Maggiori C, Fernández-Martínez MA, Bourdages LJ, Sánchez-García L, Moreno-Paz M, Sobrado JM, Carrizo D, Vicente-Retortillo Á, Goordial J, Whyte LG. Biosignature Detection and MinION Sequencing of Antarctic Cryptoendoliths After Exposure to Mars Simulation Conditions. ASTROBIOLOGY 2024; 24:44-60. [PMID: 38153386 DOI: 10.1089/ast.2023.0025] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/29/2023]
Abstract
In the search for life in our Solar System, Mars remains a promising target based on its proximity and similarity to Earth. When Mars transitioned from a warmer, wetter climate to its current dry and freezing conditions, any putative extant life probably retreated into habitable refugia such as the subsurface or the interior of rocks. Terrestrial cryptoendolithic microorganisms (i.e., those inhabiting rock interiors) thus represent possible modern-day Mars analogs, particularly those from the hyperarid McMurdo Dry Valleys in Antarctica. As DNA is a strong definitive biosignature, given that there is no known abiotic chemistry that can polymerize nucleobases, we investigated DNA detection with MinION sequencing in Antarctic cryptoendoliths after an ∼58-sol exposure in MARTE, a Mars environmental chamber capable of simulating martian temperature, pressure, humidity, ultraviolet (UV) radiation, and atmospheric composition, in conjunction with protein and lipid detection. The MARTE conditions resulted in changes in community composition and DNA, proteins, and cell membrane-derived lipids remained detectable postexposure. Of the multitude of extreme environmental conditions on Mars, UV radiation (specifically UVC) is the most destructive to both cells and DNA. As such, we further investigated if a UVC exposure corresponding to ∼278 martian years would impede DNA detection via MinION sequencing. The MinION was able to successfully detect and sequence DNA after this UVC radiation exposure, suggesting its utility for life detection in future astrobiology missions focused on finding relatively recently exposed biomarkers inside possible martian refugia.
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Affiliation(s)
- Catherine Maggiori
- Department of Biology, Georgetown University, Washington, District of Columbia, USA
| | - Miguel Angel Fernández-Martínez
- Department of Natural Resource Sciences, Faculty of Agricultural and Environmental Sciences, McGill University, Ste. Anne-de-Bellevue, Quebec, Canada
- Department of Ecology, Universidad Autónoma de Madrid, Ciudad Universitaria de Cantoblanco, Madrid, Spain
| | - Louis-Jacques Bourdages
- Department of Natural Resource Sciences, Faculty of Agricultural and Environmental Sciences, McGill University, Ste. Anne-de-Bellevue, Quebec, Canada
| | | | | | | | | | | | - Jacqueline Goordial
- School of Environmental Sciences, University of Guelph, Guelph, Ontario, Canada
| | - Lyle G Whyte
- Department of Natural Resource Sciences, Faculty of Agricultural and Environmental Sciences, McGill University, Ste. Anne-de-Bellevue, Quebec, Canada
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5
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Bendia AG, Moreira JCF, Ferreira JCN, Romano RG, Ferreira IGC, Franco DC, Evangelista H, Montone RC, Pellizari VH. Insights into Antarctic microbiomes: diversity patterns for terrestrial and marine habitats. AN ACAD BRAS CIENC 2023; 95:e20211442. [PMID: 37820122 DOI: 10.1590/0001-3765202320211442] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/27/2021] [Accepted: 08/27/2022] [Indexed: 10/13/2023] Open
Abstract
Microorganisms in Antarctica are recognized for having crucial roles in ecosystems functioning and biogeochemical cycles. To explore the diversity and composition of microbial communities through different terrestrial and marine Antarctic habitats, we analyze 16S rRNA sequence datasets from fumarole and marine sediments, soil, snow and seawater environments. We obtained measures of alpha- and beta-diversities, as well as we have identified the core microbiome and the indicator microbial taxa of a particular habitat. Our results showed a unique microbial community structure according to each habitat, including specific taxa composing each microbiome. Marine sediments harbored the highest microbial diversity among the analyzed habitats. In the fumarole sediments, the core microbiome was composed mainly of thermophiles and hyperthermophilic Archaea, while in the majority of soil samples Archaea was absent. In the seawater samples, the core microbiome was mainly composed by cultured and uncultured orders usually identified on Antarctic pelagic ecosystems. Snow samples exhibited common taxa previously described for habitats of the Antarctic Peninsula, which suggests long-distance dispersal processes occurring from the Peninsula to the Continent. This study contributes as a baseline for further efforts on evaluating the microbial responses to environmental conditions and future changes.
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Affiliation(s)
- Amanda G Bendia
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Julio Cezar F Moreira
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Juliana C N Ferreira
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Renato G Romano
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Ivan G C Ferreira
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Diego C Franco
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Heitor Evangelista
- Universidade do Estado do Rio de Janeiro (UERJ), Instituto de Biologia Roberto Alcantara Gomes, Maracanã, 20550-013 Rio de Janeiro, RJ, Brazil
| | - Rosalinda C Montone
- Universidade de São Paulo (USP), Departamento de Oceanografia Física, Química e Geológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
| | - Vivian Helena Pellizari
- Universidade de São Paulo (USP), Departamento de Oceanografia Biológica, Instituto Oceanográfico, Cidade Universitária, Praça do Oceanográfico, 191, 05508-900 São Paulo, SP, Brazil
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6
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Sánchez-García L, Lezcano MÁ, Carrizo D, Severino R, García-Villadangos M, Cady SL, Warren-Rhodes K, Cabrol NA, Parro V. Assessing siliceous sinter matrices for long-term preservation of lipid biomarkers in opaline sinter deposits analogous to Mars in El Tatio (Chile). THE SCIENCE OF THE TOTAL ENVIRONMENT 2023; 870:161765. [PMID: 36702265 DOI: 10.1016/j.scitotenv.2023.161765] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/25/2022] [Revised: 01/16/2023] [Accepted: 01/18/2023] [Indexed: 06/18/2023]
Abstract
Subaerial hydrothermal systems are of great interest for paleobiology and astrobiology as plausible candidate environments to support the origin of life on Earth that offer a unique and interrelated atmosphere-hydrosphere-lithosphere interface. They harbor extensive sinter deposits of high preservation potential that are promising targets in the search for traces of possible extraterrestrial life on Hesperian Mars. However, long-term quality preservation is paramount for recognizing biosignatures in old samples and there are still significant gaps in our understanding of the impact and extent of taphonomy processes on life fingerprints. Here, we propose a study based on lipid biomarkers -highly resistant cell-membrane components- to investigate the effects of silicification on their preservation in hydrothermal opaline sinter. We explore the lipid biomarkers profile in three sinter deposits of up to ~3000 years from El Tatio, one of the best Martian analogs on Earth. The lipid profile in local living biofilms is used as a fresh counterpart of the fossil biomarkers in the centuries-old sinter deposits to qualitatively assess the taphonomy effects of silicification on the lipid's preservation. Despite the geological alteration, the preserved lipids retained a depleted stable-carbon isotopic fingerprint characteristic of biological sources, result highly relevant for astrobiology. The data allowed us to estimate for the first time the degradation rate of lipid biomarkers in sinter deposits from El Tatio, and to assess the time preservation framework of opaline silica. Auxiliary techniques of higher taxonomic resolution (DNA sequencing and metaproteomics) helped in the reconstruction of the paleobiology. The lipids were the best-preserved biomolecules, whereas the detection of DNA and proteins dropped considerably from 5 cm depth. These findings provide new insights into taphonomy processes affecting life fingerprints in hydrothermal deposits and serves as a useful baseline for assessing the time window for recovering unambiguous signs of past life on Earth and beyond.
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Affiliation(s)
| | | | - Daniel Carrizo
- Centro de Astrobiología (CAB, CSIC-INTA), 28850 Torrejón de Ardoz, Spain
| | - Rita Severino
- Centro de Astrobiología (CAB, CSIC-INTA), 28850 Torrejón de Ardoz, Spain; Dept. of Physics and Mathematics and Automatics, University of Alcalá (UAH), 28805 Alcalá de Henares, Spain
| | | | - Sherry L Cady
- Environmental Molecular Sciences Laboratory, Pacific Northwest National Laboratory, Richland, WA, United States
| | - Kim Warren-Rhodes
- Carl Sagan Center for the Study of Life in the Universe, SETI Institute, CA 94043, United States
| | - Nathalie A Cabrol
- Carl Sagan Center for the Study of Life in the Universe, SETI Institute, CA 94043, United States
| | - Víctor Parro
- Centro de Astrobiología (CAB, CSIC-INTA), 28850 Torrejón de Ardoz, Spain
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7
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Azua-Bustos A, Fairén AG, González-Silva C, Prieto-Ballesteros O, Carrizo D, Sánchez-García L, Parro V, Fernández-Martínez MÁ, Escudero C, Muñoz-Iglesias V, Fernández-Sampedro M, Molina A, Villadangos MG, Moreno-Paz M, Wierzchos J, Ascaso C, Fornaro T, Brucato JR, Poggiali G, Manrique JA, Veneranda M, López-Reyes G, Sanz-Arranz A, Rull F, Ollila AM, Wiens RC, Reyes-Newell A, Clegg SM, Millan M, Johnson SS, McIntosh O, Szopa C, Freissinet C, Sekine Y, Fukushi K, Morida K, Inoue K, Sakuma H, Rampe E. Dark microbiome and extremely low organics in Atacama fossil delta unveil Mars life detection limits. Nat Commun 2023; 14:808. [PMID: 36810853 PMCID: PMC9944251 DOI: 10.1038/s41467-023-36172-1] [Citation(s) in RCA: 12] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/28/2022] [Accepted: 01/17/2023] [Indexed: 02/24/2023] Open
Abstract
Identifying unequivocal signs of life on Mars is one of the most important objectives for sending missions to the red planet. Here we report Red Stone, a 163-100 My alluvial fan-fan delta that formed under arid conditions in the Atacama Desert, rich in hematite and mudstones containing clays such as vermiculite and smectites, and therefore geologically analogous to Mars. We show that Red Stone samples display an important number of microorganisms with an unusual high rate of phylogenetic indeterminacy, what we refer to as "dark microbiome", and a mix of biosignatures from extant and ancient microorganisms that can be barely detected with state-of-the-art laboratory equipment. Our analyses by testbed instruments that are on or will be sent to Mars unveil that although the mineralogy of Red Stone matches that detected by ground-based instruments on the red planet, similarly low levels of organics will be hard, if not impossible to detect in Martian rocks depending on the instrument and technique used. Our results stress the importance in returning samples to Earth for conclusively addressing whether life ever existed on Mars.
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Affiliation(s)
- Armando Azua-Bustos
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain. .,Instituto de Ciencias Biomédicas, Facultad de Ciencias de la Salud, Universidad Autónoma de Chile, Santiago, Chile.
| | - Alberto G Fairén
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain.,Department of Astronomy, Cornell University, Ithaca, 14853, NY, USA
| | | | | | - Daniel Carrizo
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain
| | | | - Victor Parro
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain
| | | | | | | | | | - Antonio Molina
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain
| | | | | | - Jacek Wierzchos
- Museo Nacional de Ciencias Naturales (CSIC), 28006, Madrid, Spain
| | - Carmen Ascaso
- Museo Nacional de Ciencias Naturales (CSIC), 28006, Madrid, Spain
| | - Teresa Fornaro
- INAF-Astrophysical Observatory of Arcetri, Florence, Italy
| | | | | | - Jose Antonio Manrique
- Universidad de Valladolid, Valladolid, Spain.,Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France
| | | | | | | | | | - Ann M Ollila
- Purdue University, Earth, Atmospheric, and Planetary Sciences, West Lafayette, USA
| | - Roger C Wiens
- Purdue University, Earth, Atmospheric, and Planetary Sciences, West Lafayette, USA
| | | | - Samuel M Clegg
- Purdue University, Earth, Atmospheric, and Planetary Sciences, West Lafayette, USA
| | - Maëva Millan
- Department of Biology, Georgetown University, Washington, DC, 20057, USA.,NASA Goddard Space Flight Center, Solar System Exploration Division, Greenbelt, MD, 20771, USA.,LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - Sarah Stewart Johnson
- Department of Biology, Georgetown University, Washington, DC, 20057, USA.,Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Ophélie McIntosh
- INAF-Astrophysical Observatory of Arcetri, Florence, Italy.,Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Cyril Szopa
- Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Caroline Freissinet
- Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Yasuhito Sekine
- Earth-Life Science Institute (ELSI), Tokyo Institute of Technology, Tokyo, Japan.,Institute of Nature and Environmental Technology, Kanazawa University, Kanazawa, Japan
| | - Keisuke Fukushi
- Institute of Nature and Environmental Technology, Kanazawa University, Kanazawa, Japan
| | - Koki Morida
- Division of Natural System, Kanazawa University, Kanazawa, Japan
| | - Kosuke Inoue
- Division of Natural System, Kanazawa University, Kanazawa, Japan
| | - Hiroshi Sakuma
- National Institute for Materials Science, Tsukuba, Japan
| | - Elizabeth Rampe
- Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX, USA
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8
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Ugwuanyi IR, Fogel ML, Bowden R, Steele A, De Natale G, Troise C, Somma R, Piochi M, Mormone A, Glamoclija M. Comparative metagenomics at Solfatara and Pisciarelli hydrothermal systems in Italy reveal that ecological differences across substrates are not ubiquitous. Front Microbiol 2023; 14:1066406. [PMID: 36819055 PMCID: PMC9930910 DOI: 10.3389/fmicb.2023.1066406] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/10/2022] [Accepted: 01/06/2023] [Indexed: 02/04/2023] Open
Abstract
Introduction Continental hydrothermal systems (CHSs) are geochemically complex, and they support microbial communities that vary across substrates. However, our understanding of these variations across the complete range of substrates in CHS is limited because many previous studies have focused predominantly on aqueous settings. Methods Here we used metagenomes in the context of their environmental geochemistry to investigate the ecology of different substrates (i.e., water, mud and fumarolic deposits) from Solfatara and Pisciarelli. Results and Discussion Results indicate that both locations are lithologically similar with distinct fluid geochemistry. In particular, all substrates from Solfatara have similar chemistry whereas Pisciarelli substrates have varying chemistry; with water and mud from bubbling pools exhibiting high SO4 2- and NH4 + concentrations. Species alpha diversity was found to be different between locations but not across substrates, and pH was shown to be the most important driver of both diversity and microbial community composition. Based on cluster analysis, microbial community structure differed significantly between Pisciarelli substrates but not between Solfatara substrates. Pisciarelli mud pools, were dominated by (hyper)thermophilic archaea, and on average, bacteria dominated Pisciarelli fumarolic deposits and all investigated Solfatara environments. Carbon fixation and sulfur oxidation were the most important metabolic pathways fueled by volcanic outgassing at both locations. Together, results demonstrate that ecological differences across substrates are not a widespread phenomenon but specific to the system. Therefore, this study demonstrates the importance of analyzing different substrates of a CHS to understand the full range of microbial ecology to avoid biased ecological assessments.
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Affiliation(s)
- Ifeoma R. Ugwuanyi
- Department of Earth and Environmental Sciences, Rutgers University, Newark, NJ, United States,Ifeoma R. Ugwuanyi, ✉
| | - Marilyn L. Fogel
- EDGE Institute, University of California, Riverside, Riverside, CA, United States
| | - Roxane Bowden
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, United States
| | - Andrew Steele
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, United States
| | - Giuseppe De Natale
- Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Vesuviano, Naples, Italy,Consiglio Nazionale delle Ricerche INO, Naples, Italy
| | - Claudia Troise
- Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Vesuviano, Naples, Italy,Consiglio Nazionale delle Ricerche INO, Naples, Italy
| | - Renato Somma
- Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Vesuviano, Naples, Italy,Consiglio Nazionale delle Ricerche IRISS, Naples, Italy
| | - Monica Piochi
- Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Vesuviano, Naples, Italy
| | - Angela Mormone
- Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Vesuviano, Naples, Italy
| | - Mihaela Glamoclija
- Department of Earth and Environmental Sciences, Rutgers University, Newark, NJ, United States,*Correspondence: Mihaela Glamoclija, ✉
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9
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Allioux M, Yvenou S, Merkel A, Cozannet M, Aubé J, Pommellec J, Le Romancer M, Lavastre V, Guillaume D, Alain K. A metagenomic insight into the microbiomes of geothermal springs in the Subantarctic Kerguelen Islands. Sci Rep 2022; 12:22243. [PMID: 36564496 PMCID: PMC9789041 DOI: 10.1038/s41598-022-26299-4] [Citation(s) in RCA: 7] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/05/2022] [Accepted: 12/13/2022] [Indexed: 12/24/2022] Open
Abstract
The Kerguelen Islands, located in the southern part of the Indian Ocean, are very isolated geographically. The microbial diversity and communities present on the island, especially associated to geothermal springs, have never been analyzed with high-throughput sequencing methods. In this article, we performed the first metagenomics analysis of microorganisms present in Kerguelen hot springs. From four hot springs, we assembled metagenomes and recovered 42 metagenome-assembled genomes, mostly associated with new putative taxa based on phylogenomic analyses and overall genome relatedness indices. The 42 MAGs were studied in detail and showed putative affiliations to 13 new genomic species and 6 new genera of Bacteria or Archaea according to GTDB. Functional potential of MAGs suggests the presence of thermophiles and hyperthermophiles, as well as heterotrophs and primary producers possibly involved in the sulfur cycle, notably in the oxidation of sulfur compounds. This paper focused on only four of the dozens of hot springs in the Kerguelen Islands and should be considered as a preliminary study of the microorganisms inhabiting the hot springs of these isolated islands. These results show that more efforts should be made towards characterization of Kerguelen Islands ecosystems, as they represent a reservoir of unknown microbial lineages.
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Affiliation(s)
- Maxime Allioux
- Univ Brest, CNRS, IFREMER, IRP 1211 MicrobSea, Unité Biologie et Ecologie des Ecosystèmes Marins Profonds BEEP, IUEM, Rue Dumont d'Urville, 29280, Plouzané, France
| | - Stéven Yvenou
- Univ Brest, CNRS, IFREMER, IRP 1211 MicrobSea, Unité Biologie et Ecologie des Ecosystèmes Marins Profonds BEEP, IUEM, Rue Dumont d'Urville, 29280, Plouzané, France
| | - Alexander Merkel
- , Research Center of Biotechnology of the Russian Academy of Sciences, Winogradsky Institute of Microbiology, Moscow, Russia
| | - Marc Cozannet
- Univ Brest, CNRS, IFREMER, IRP 1211 MicrobSea, Unité Biologie et Ecologie des Ecosystèmes Marins Profonds BEEP, IUEM, Rue Dumont d'Urville, 29280, Plouzané, France
| | - Johanne Aubé
- Univ Brest, CNRS, IFREMER, IRP 1211 MicrobSea, Unité Biologie et Ecologie des Ecosystèmes Marins Profonds BEEP, IUEM, Rue Dumont d'Urville, 29280, Plouzané, France
| | - Jolann Pommellec
- Univ Brest, CNRS, IFREMER, IRP 1211 MicrobSea, Unité Biologie et Ecologie des Ecosystèmes Marins Profonds BEEP, IUEM, Rue Dumont d'Urville, 29280, Plouzané, France
| | - Marc Le Romancer
- UBO, UFR Sciences et Techniques, UR 7462, Laboratoire Géoarchitecture, Territoires, Urbanisation, Biodiversité, Environnement, Rennes, France
| | | | | | - Karine Alain
- Univ Brest, CNRS, IFREMER, IRP 1211 MicrobSea, Unité Biologie et Ecologie des Ecosystèmes Marins Profonds BEEP, IUEM, Rue Dumont d'Urville, 29280, Plouzané, France.
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10
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Ren Z, Cao S, Chen T, Zhang C, Yu J. Bacterial functional redundancy and carbon metabolism potentials in soil, sediment, and water of thermokarst landscapes across the Qinghai-Tibet Plateau: Implications for the fate of permafrost carbon. THE SCIENCE OF THE TOTAL ENVIRONMENT 2022; 852:158340. [PMID: 36041614 DOI: 10.1016/j.scitotenv.2022.158340] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/10/2022] [Revised: 08/23/2022] [Accepted: 08/23/2022] [Indexed: 06/15/2023]
Abstract
Permafrost thaw create widespread thermokarst landscapes. As a result, distinct habitats are provided to harbor different bacterial communities in degraded permafrost soil (PBCs), thermokarst lake sediment (SBCs), and lake water (WBCs), driving carbon metabolism differentially. In this study, we investigated functional diversity and redundancy, and carbon metabolism potentials of PBCs, SBCs, and WBCs in thermokarst landscapes across the Qinghai-Tibet Plateau. The results showed that PBCs and SBCs had higher taxonomic and functional alpha diversity than WBCs, while WBCs had lower functional redundancy. WBCs had the highest beta diversity followed by SBCs and PBCs, suggesting strong determination of taxonomic variations on functional differences. Community assembly processes also had significant influences on beta diversity, especially for SBCs. Metabolism pathways of carbohydrate metabolism, methane metabolism, and carbon fixation were enriched differentially in PBCs, SBCs, and WBCs, suggesting different C fate in distinct habitats. Carbohydrate metabolism data suggested that PBCs might have stronger potentials to mineralize a greater diversity of organic carbon substrate than SBCs and WBCs, promoting degradation of organic carbon stocks in degraded permafrost soils. Methane metabolism data showed that SBCs had a stronger methanogenesis potential followed by PBCs and WBCs, while PBCs had a stronger methane oxidation potential. High abundance of genes involving in formaldehyde assimilation might suggested that a large proportion of produced methane might be assimilated by methanotrophs in the thermokarst landscapes. Both aerobic and anaerobic carbon fixation pathways were enriched in PBCs. The results added our understanding of functional properties and biogeochemical carbon cycles in thermokarst landscapes, improving our abilities in accurate modeling of carbon dynamics and the ultimate fate of permafrost carbon in a warming world.
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Affiliation(s)
- Ze Ren
- Research and Development Center for Watershed Environmental Eco-Engineering, Advanced Institute of Natural Sciences, Beijing Normal University, Zhuhai 519087, China; School of Environment, Beijing Normal University, Beijing 100875, China.
| | - Shengkui Cao
- School of Geographical Science, Qinghai Normal University, Xining 810008, China.
| | - Tao Chen
- Center for Grassland Microbiome, State Key Laboratory of Grassland Agro-ecosystems, Lanzhou University, Lanzhou 730020, China
| | - Cheng Zhang
- Research and Development Center for Watershed Environmental Eco-Engineering, Advanced Institute of Natural Sciences, Beijing Normal University, Zhuhai 519087, China; School of Engineering Technology, Beijing Normal University, Zhuhai 519087, China
| | - Jinlei Yu
- Key Laboratory of Geographic Information Science, Ministry of Education, East China Normal University, Shanghai 200241, China
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11
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Megevand V, Carrizo D, Lezcano MÁ, Moreno-Paz M, Cabrol NA, Parro V, Sánchez-García L. Lipid Profiles From Fresh Biofilms Along a Temperature Gradient on a Hydrothermal Stream at El Tatio (Chilean Andes), as a Proxy for the Interpretation of Past and Present Biomarkers Beyond Earth. Front Microbiol 2022; 13:811904. [PMID: 35832812 PMCID: PMC9271869 DOI: 10.3389/fmicb.2022.811904] [Citation(s) in RCA: 6] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/09/2021] [Accepted: 05/18/2022] [Indexed: 11/13/2022] Open
Abstract
Hydrothermal systems and their deposits are primary targets in the search for fossil evidence of life beyond Earth. However, to learn how to decode fossil biomarker records in ancient hydrothermal deposits, we must first be able to interpret unambiguously modern biosignatures, their distribution patterns, and their association with physicochemical factors. Here, we investigated the molecular and isotopic profile of microbial biomarkers along a thermal gradient (from 29 to 72°C) in a hot spring (labeled Cacao) from El Tatio, a geyser field in the Chilean Andes with abundant opaline silica deposits resembling the nodular and digitate structures discovered on Mars. As a molecular forensic approach, we focused on the analysis of lipid compounds bearing recognized resistance to degradation and the potential to reconstruct the paleobiology of an environment on a broader temporal scale than other, more labile, biomolecules. By exploiting the lipid biomarkers' potential to diagnose biological sources and carbon fixation pathways, we reconstructed the microbial community structure and its ecology along the Cacao hydrothermal transect. The taxonomic adscription of the lipid biomarkers was qualitatively corroborated with DNA sequencing analysis. The forensic capacity of the lipid biomarkers to identify biosources in fresh biofilms was validated down to the genus level for Roseiflexus, Chloroflexus, and Fischerella. We identified lipid biomarkers and DNA of several new cyanobacterial species in El Tatio and reported the first detection of Fischerella biomarkers at a temperature as high as 72°C. This, together with ecological peculiarities and the proportion of clades being characterized as unclassified, illustrates the ecological singularity of El Tatio and strengthens its astrobiological relevance. The Cacao hydrothermal ecosystem was defined by a succession of microbial communities and metabolic traits associated with a high- (72°C) to low-(29°C) temperature gradient that resembled the inferred metabolic sequence events from the 16S rRNA gene universal phylogenetic tree from thermophilic to anoxygenic photosynthetic species and oxygenic phototrophs. The locally calibrated DNA-validated lipidic profile in the Cacao biofilms provided a modern (molecular and isotopic) end member to facilitate the recognition of past biosources and metabolisms from altered biomarkers records in ancient silica deposits at El Tatio analogous to Martian opaline silica structures.
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Affiliation(s)
- Valentine Megevand
- Centro de Astrobiología (CAB), INTA-CSIC, Madrid, Spain
- Department of Earth Sciences, Ecole Normale Supérieure de Lyon, Université Claude Bernard Lyon, Lyon, France
| | | | | | | | - Nathalie A. Cabrol
- Carl Sagan Center for Research, The SETI Institute, Mountain View, CA, United States
| | - Víctor Parro
- Centro de Astrobiología (CAB), INTA-CSIC, Madrid, Spain
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12
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Doytchinov VV, Dimov SG. Microbial Community Composition of the Antarctic Ecosystems: Review of the Bacteria, Fungi, and Archaea Identified through an NGS-Based Metagenomics Approach. LIFE (BASEL, SWITZERLAND) 2022; 12:life12060916. [PMID: 35743947 PMCID: PMC9228076 DOI: 10.3390/life12060916] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.7] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 05/20/2022] [Revised: 06/09/2022] [Accepted: 06/16/2022] [Indexed: 11/16/2022]
Abstract
Antarctica represents a unique environment, both due to the extreme meteorological and geological conditions that govern it and the relative isolation from human influences that have kept its environment largely undisturbed. However, recent trends in climate change dictate an unavoidable change in the global biodiversity as a whole, and pristine environments, such as Antarctica, allow us to study and monitor more closely the effects of the human impact. Additionally, due to its inaccessibility, Antarctica contains a plethora of yet uncultured and unidentified microorganisms with great potential for useful biological activities and production of metabolites, such as novel antibiotics, proteins, pigments, etc. In recent years, amplicon-based next-generation sequencing (NGS) has allowed for a fast and thorough examination of microbial communities to accelerate the efforts of unknown species identification. For these reasons, in this review, we present an overview of the archaea, bacteria, and fungi present on the Antarctic continent and the surrounding area (maritime Antarctica, sub-Antarctica, Southern Sea, etc.) that have recently been identified using amplicon-based NGS methods.
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13
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Lezcano MÁ, Sánchez-García L, Quesada A, Carrizo D, Fernández-Martínez MÁ, Cavalcante-Silva E, Parro V. Comprehensive Metabolic and Taxonomic Reconstruction of an Ancient Microbial Mat From the McMurdo Ice Shelf (Antarctica) by Integrating Genetic, Metaproteomic and Lipid Biomarker Analyses. Front Microbiol 2022; 13:799360. [PMID: 35928160 PMCID: PMC9345047 DOI: 10.3389/fmicb.2022.799360] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/21/2021] [Accepted: 03/21/2022] [Indexed: 12/31/2022] Open
Abstract
Paleobiological reconstructions based on molecular fossils may be limited by degradation processes causing differential preservation of biomolecules, the distinct taxonomic specificity of each biomolecule type, and analytical biases. Here, we combined the analysis of DNA, proteins and lipid biomarkers using 16S and 18S rRNA gene metabarcoding, metaproteomics and lipid analysis to reconstruct the taxonomic composition and metabolisms of a desiccated microbial mat from the McMurdo Ice Shelf (MIS) (Antarctica) dated ~1,000 years BP. The different lability, taxonomic resolution and analytical bias of each biomolecule type led to a distinct microbial community profile. DNA analysis showed selective preservation of DNA remnants from the most resistant taxa (e.g., spore-formers). In contrast, the proteins profile revealed microorganisms missed by DNA sequencing, such as Cyanobacteria, and showed a microbial composition similar to fresh microbial mats in the MIS. Lipid hydrocarbons also confirmed Cyanobacteria and suggested the presence of mosses or vascular plant remnants from a period in Antarctica when the climate was warmer (e.g., Mid-Miocene or Eocene). The combined analysis of the three biomolecule types also revealed diverse metabolisms that operated in the microbial mat before desiccation: oxygenic and anoxygenic photosynthesis, nitrogen fixation, nitrification, denitrification, sulfur reduction and oxidation, and methanogenesis. Therefore, the joint analysis of DNA, proteins and lipids resulted in a powerful approach that improved taxonomic and metabolic reconstructions overcoming information gaps derived from using individual biomolecules types.
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Affiliation(s)
- María Ángeles Lezcano
- Centro de Astrobiología (CAB), CSIC-INTA, Carretera de Ajalvir, Madrid, Spain
- *Correspondence: María Ángeles Lezcano,
| | | | - Antonio Quesada
- Centro de Astrobiología (CAB), CSIC-INTA, Carretera de Ajalvir, Madrid, Spain
- Departamento de Biología, C. Darwin 2, Universidad Autónoma de Madrid, Madrid, Spain
| | - Daniel Carrizo
- Centro de Astrobiología (CAB), CSIC-INTA, Carretera de Ajalvir, Madrid, Spain
| | | | | | - Víctor Parro
- Centro de Astrobiología (CAB), CSIC-INTA, Carretera de Ajalvir, Madrid, Spain
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14
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Abstract
The glaciers in China have an important role as one of the most climate-sensitive constituents of the Tibetan Plateau which is known as the Asian Water Tower. Although the cryosphere is one of the most extreme environments for organisms, the soils of the glacier foreland harbor surprisingly rich microbiomes. A large amount of accelerated glacier retreat accompanied by global warming will not only raise the sea level, but it will also lead to the massive release of a considerable amount of carbon stored in these glaciers. The responses of glacier microbiomes could alter the biogeochemical cycle of carbon and have a complex impact on climate change. Thus, understanding present-day and future glacier microbiome changes is crucial to assess the feedback on climate change and the impacts on ecosystems. To this end, we discuss here the diversity and biogeochemical functions of the microbiomes in Chinese mountain glacier ecosystems.
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15
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Prokaryotic diversity and biogeochemical characteristics of benthic microbial ecosystems from James Ross Archipelago (West Antarctica). Polar Biol 2022. [DOI: 10.1007/s00300-021-02997-z] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/20/2022]
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16
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Vicente J, de Celis M, Alonso A, Marquina D, Santos A. Microbial Communities Present in Hydrothermal Sediments from Deception Island, Antarctica. Microorganisms 2021; 9:microorganisms9081631. [PMID: 34442712 PMCID: PMC8399207 DOI: 10.3390/microorganisms9081631] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/02/2021] [Revised: 07/26/2021] [Accepted: 07/27/2021] [Indexed: 12/03/2022] Open
Abstract
Deception Island is a geothermal location in Antarctica that presents active fumaroles, which confers unique characteristics to this habitat. Several studies about microbial communities in Antarctica have been carried out, nevertheless, Antarctic microbiota is still partially unknown. Here we present a multidisciplinary study about sediments obtained by deposition during 4 years in which several approaches have been considered for their characterization. First, a physicochemical characterization, using ionic chromatography and mass spectrometry for the determination of most abundant ions (chloride and sulphate) and elements (mainly silicon), was conducted. In addition, the total microbial community was studied using a metataxonomical approach, revealing a bacterial community dominated by Proteobacteria and Thaumarchaeota as the main archaeal genera and a fungal community mainly composed by Aspergillaceae. Culture-dependent studies showed low microbial diversity, only achieving the isolation of Bacillus-related species, some of them thermophilic, and the isolation of common fungi of Aspergillus or Penicillium spp. Furthermore, diatoms were detected in the sediment and characterized attending to their morphological characteristics using scanning electron microscopy. The study reveals a high influence of the physicochemical conditions in the microbial populations and their distribution, offering valuable data on the interaction between the island and water microbiota.
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17
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Bendia AG, Lemos LN, Mendes LW, Signori CN, Bohannan BJM, Pellizari VH. Metabolic potential and survival strategies of microbial communities across extreme temperature gradients on Deception Island volcano, Antarctica. Environ Microbiol 2021; 23:4054-4073. [PMID: 34245102 DOI: 10.1111/1462-2920.15649] [Citation(s) in RCA: 9] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/10/2020] [Revised: 06/16/2021] [Accepted: 06/20/2021] [Indexed: 11/27/2022]
Abstract
Active volcanoes in Antarctica have remarkable temperature and geochemical gradients that could select for a wide variety of microbial adaptive mechanisms and metabolic pathways. Deception Island is a stratovolcano flooded by the sea, resulting in contrasting ecosystems such as permanent glaciers and active fumaroles, which creates steep gradients that have been shown to affect microbial diversity. In this study, we used shotgun metagenomics and metagenome-assembled genomes to explore the metabolic potentials and survival strategies of microbial communities along an extreme temperature gradient in fumarole and glacier sediments on Deception Island. We observed that communities from a 98 °C fumarole were significantly enriched in genes related to hyperthermophilic (e.g. reverse gyrase, GroEL/GroES and thermosome) and oxidative stress responses, as well as genes related to sulfate reduction, ammonification and carbon fixation. Communities from <80 °C fumaroles possessed more genes related osmotic, cold- and heat-shock responses, and diverse metabolic potentials, such as those related to sulfur oxidation and denitrification, while glacier communities showed abundant metabolic potentials mainly related to heterotrophy. Through the reconstruction of genomes, we were able to reveal the metabolic potentials and different survival strategies of underrepresented taxonomic groups, especially those related to Nanoarchaeota, Pyrodictiaceae and thermophilic ammonia-oxidizing archaeal lineages.
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Affiliation(s)
- Amanda Gonçalves Bendia
- Departamento de Oceanografia Biológica, Instituto Oceanográfico, Universidade de São Paulo (USP), Praça do Oceanográfico, 191, São Paulo, SP, CEP 05508-120, Brazil
| | - Leandro Nascimento Lemos
- Laboratório de Biologia Celular e Molecular, Centro de Energia Nuclear na Agricultura, Universidade de São Paulo, Avenida Centenário 303, Piracicaba, SP, CEP 13416-00, Brazil
| | - Lucas William Mendes
- Laboratório de Biologia Celular e Molecular, Centro de Energia Nuclear na Agricultura, Universidade de São Paulo, Avenida Centenário 303, Piracicaba, SP, CEP 13416-00, Brazil
| | - Camila Negrão Signori
- Departamento de Oceanografia Biológica, Instituto Oceanográfico, Universidade de São Paulo (USP), Praça do Oceanográfico, 191, São Paulo, SP, CEP 05508-120, Brazil
| | - Brendan J M Bohannan
- Department of Biology, Institute of Ecology and Evolution, University of Oregon, Eugene, OR, USA
| | - Vivian Helena Pellizari
- Departamento de Oceanografia Biológica, Instituto Oceanográfico, Universidade de São Paulo (USP), Praça do Oceanográfico, 191, São Paulo, SP, CEP 05508-120, Brazil
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18
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Fernández-Martínez MÁ, García-Villadangos M, Moreno-Paz M, Gangloff V, Carrizo D, Blanco Y, González S, Sánchez-García L, Prieto-Ballesteros O, Altshuler I, Whyte LG, Parro V, Fairén AG. Geomicrobiological Heterogeneity of Lithic Habitats in the Extreme Environment of Antarctic Nunataks: A Potential Early Mars Analog. Front Microbiol 2021; 12:670982. [PMID: 34276605 PMCID: PMC8284421 DOI: 10.3389/fmicb.2021.670982] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/22/2021] [Accepted: 05/21/2021] [Indexed: 11/13/2022] Open
Abstract
Nunataks are permanent ice-free rocky peaks that project above ice caps in polar regions, thus being exposed to extreme climatic conditions throughout the year. They undergo extremely low temperatures and scarcity of liquid water in winter, while receiving high incident and reflected (albedo) UVA-B radiation in summer. Here, we investigate the geomicrobiology of the permanently exposed lithic substrates of nunataks from Livingston Island (South Shetlands, Antarctic Peninsula), with focus on prokaryotic community structure and their main metabolic traits. Contrarily to first hypothesis, an extensive sampling based on different gradients and multianalytical approaches demonstrated significant differences for most geomicrobiological parameters between the bedrock, soil, and loose rock substrates, which overlapped any other regional variation. Brevibacillus genus dominated on bedrock and soil substrates, while loose rocks contained a diverse microbial community, including Actinobacteria, Alphaproteobacteria and abundant Cyanobacteria inhabiting the milder and diverse microhabitats within. Archaea, a domain never described before in similar Antarctic environments, were also consistently found in the three substrates, but being more abundant and potentially more active in soils. Stable isotopic ratios of total carbon (δ 13C) and nitrogen (δ 15N), soluble anions concentrations, and the detection of proteins involved in key metabolisms via the Life Detector Chip (LDChip), suggest that microbial primary production has a pivotal role in nutrient cycling at these exposed areas with limited deposition of nutrients. Detection of stress-resistance proteins, such as molecular chaperons, suggests microbial molecular adaptation mechanisms to cope with these harsh conditions. Since early Mars may have encompassed analogous environmental conditions as the ones found in these Antarctic nunataks, our study also contributes to the understanding of the metabolic features and biomarker profiles of a potential Martian microbiota, as well as the use of LDChip in future life detection missions.
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Affiliation(s)
- Miguel Ángel Fernández-Martínez
- Centro de Astrobiología, CSIC-INTA, Madrid, Spain.,Department of Natural Resource Sciences, Faculty of Agricultural and Environmental Sciences, McGill University, Sainte-Anne-de-Bellevue, QC, Canada
| | | | | | | | | | | | - Sergi González
- Antarctic Group, Agencia Estatal de Meteorología, Barcelona, Spain
| | | | | | - Ianina Altshuler
- Department of Natural Resource Sciences, Faculty of Agricultural and Environmental Sciences, McGill University, Sainte-Anne-de-Bellevue, QC, Canada
| | - Lyle G Whyte
- Department of Natural Resource Sciences, Faculty of Agricultural and Environmental Sciences, McGill University, Sainte-Anne-de-Bellevue, QC, Canada
| | - Victor Parro
- Centro de Astrobiología, CSIC-INTA, Madrid, Spain
| | - Alberto G Fairén
- Centro de Astrobiología, CSIC-INTA, Madrid, Spain.,Department of Astronomy, Cornell University, Ithaca, NY, United States
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19
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Reed PA, Lagasse BA, Garcia CD. Fast Degradation of Hydrogen Peroxide by Immobilized Catalase to Enable the Use of Biosensors in Extraterrestrial Bodies. ASTROBIOLOGY 2021; 21:191-198. [PMID: 33052719 DOI: 10.1089/ast.2020.2263] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/11/2023]
Abstract
Hydrogen peroxide has been postulated to be present on the surface of Europa and Enceladus. While it could represent a potential source of energy for possible life-forms, H2O2 may also interfere with a number of current detection technologies, including biosensors. To take advantage of the selectivity and portability of these devices, simple and reliable routes to degrade the potential H2O2 present should be developed and implemented to prepare for this possibility. Unfortunately, most of the current approaches for removing H2O2 are slow, may affect the sample, or could interfere with the performance of biosensors. To address these limitations, catalase was immobilized onto silica particles and used as a means to selectively decompose H2O2 prior to the analysis of common biomarkers with a biosensor. For these experiments, glucose, l-leucine, and lactic acid were used as representative examples of biomolecules such as carbohydrates, amino acids, and organic acids, respectively, which could be used as biomarkers on extraterrestrial bodies. While the decomposition reaction between catalase and H2O2 is well known, to our knowledge this is the first instance where catalase has been used in combination with a microfluidic paper-based analytical device (μPAD) to implement selective sample pretreatment.
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Affiliation(s)
- Paige A Reed
- Department of Chemistry, Clemson University, Clemson, South Carolina, USA
| | - Bryan A Lagasse
- Department of Chemistry, Clemson University, Clemson, South Carolina, USA
- Department of Chemistry and Life Science, United States Military Academy, West Point, New York, USA
| | - Carlos D Garcia
- Department of Chemistry, Clemson University, Clemson, South Carolina, USA
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20
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Sánchez-García L, Carrizo D, Molina A, Muñoz-Iglesias V, Lezcano MÁ, Fernández-Sampedro M, Parro V, Prieto-Ballesteros O. Fingerprinting molecular and isotopic biosignatures on different hydrothermal scenarios of Iceland, an acidic and sulfur-rich Mars analog. Sci Rep 2020; 10:21196. [PMID: 33273669 PMCID: PMC7712778 DOI: 10.1038/s41598-020-78240-2] [Citation(s) in RCA: 12] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/15/2020] [Accepted: 11/23/2020] [Indexed: 11/09/2022] Open
Abstract
Detecting signs of potential extant/extinct life on Mars is challenging because the presence of organics on that planet is expected to be very low and most likely linked to radiation-protected refugia and/or preservative strategies (e.g., organo-mineral complexes). With scarcity of organics, accounting for biomineralization and potential relationships between biomarkers, mineralogy, and geochemistry is key in the search for extraterrestrial life. Here we explored microbial fingerprints and their associated mineralogy in Icelandic hydrothermal systems analog to Mars (i.e., high sulfur content, or amorphous silica), to identify potentially habitable locations on that planet. The mineralogical assemblage of four hydrothermal substrates (hot springs biofilms, mud pots, and steaming and inactive fumaroles) was analyzed concerning the distribution of biomarkers. Molecular and isotopic composition of lipids revealed quantitative and compositional differences apparently impacted by surface geothermal alteration and environmental factors. pH and water showed an influence (i.e., greatest biomass in circumneutral settings with highest supply and turnover of water), whereas temperature conditioned the mineralogy that supported specific microbial metabolisms related with sulfur. Raman spectra suggested the possible coexistence of abiotic and biomediated sources of minerals (i.e., sulfur or hematite). These findings may help to interpret future Raman or GC-MS signals in forthcoming Martian missions.
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Affiliation(s)
| | - Daniel Carrizo
- Centro de Astrobiología (CSIC-INTA), Carretera de Ajalvir km 4, Madrid, Spain
| | - Antonio Molina
- Centro de Astrobiología (CSIC-INTA), Carretera de Ajalvir km 4, Madrid, Spain
| | | | | | | | - Victor Parro
- Centro de Astrobiología (CSIC-INTA), Carretera de Ajalvir km 4, Madrid, Spain
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Fairén AG, Gómez-Elvira J, Briones C, Prieto-Ballesteros O, Rodríguez-Manfredi JA, López Heredero R, Belenguer T, Moral AG, Moreno-Paz M, Parro V. The Complex Molecules Detector (CMOLD): A Fluidic-Based Instrument Suite to Search for (Bio)chemical Complexity on Mars and Icy Moons. ASTROBIOLOGY 2020; 20:1076-1096. [PMID: 32856927 PMCID: PMC7116096 DOI: 10.1089/ast.2019.2167] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 09/13/2019] [Accepted: 06/01/2020] [Indexed: 06/11/2023]
Abstract
Organic chemistry is ubiquitous in the Solar System, and both Mars and a number of icy satellites of the outer Solar System show substantial promise for having hosted or hosting life. Here, we propose a novel astrobiologically focused instrument suite that could be included as scientific payload in future missions to Mars or the icy moons: the Complex Molecules Detector, or CMOLD. CMOLD is devoted to determining different levels of prebiotic/biotic chemical and structural targets following a chemically general approach (i.e., valid for both terrestrial and nonterrestrial life), as well as their compatibility with terrestrial life. CMOLD is based on a microfluidic block that distributes a liquid suspension sample to three instruments by using complementary technologies: (1) novel microscopic techniques for identifying ultrastructures and cell-like morphologies, (2) Raman spectroscopy for detecting universal intramolecular complexity that leads to biochemical functionality, and (3) bioaffinity-based systems (including antibodies and aptamers as capture probes) for finding life-related and nonlife-related molecular structures. We highlight our current developments to make this type of instruments flight-ready for upcoming Mars missions: the Raman spectrometer included in the science payload of the ESAs Rosalind Franklin rover (Raman Laser Spectrometer instrument) to be launched in 2022, and the biomarker detector that was included as payload in the NASA Icebreaker lander mission proposal (SOLID instrument). CMOLD is a robust solution that builds on the combination of three complementary, existing techniques to cover a wide spectrum of targets in the search for (bio)chemical complexity in the Solar System.
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Affiliation(s)
- Alberto G. Fairén
- Centro de Astrobiología (CSIC-INTA), Madrid, Spain
- Department of Astronomy, Cornell University, Ithaca New York, USA
| | - Javier Gómez-Elvira
- Payload & Space Science Department, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | | | | | | | - Raquel López Heredero
- Payload & Space Science Department, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | - Tomás Belenguer
- Payload & Space Science Department, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | - Andoni G. Moral
- Payload & Space Science Department, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | | | - Víctor Parro
- Centro de Astrobiología (CSIC-INTA), Madrid, Spain
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