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Rasmussen B, Muhling JR, Fischer WW. Ancient Oil as a Source of Carbonaceous Matter in 1.88-Billion-Year-Old Gunflint Stromatolites and Microfossils. ASTROBIOLOGY 2021; 21:655-672. [PMID: 33684328 DOI: 10.1089/ast.2020.2376] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/12/2023]
Abstract
The 1.88-billion-year-old Gunflint carbonaceous microfossils are renowned for their exceptional morphological and chemical preservation, attributed to early and rapid entombment in amorphous silica. The carbonaceous matter lining and partly filling filamentous and spherical structures is interpreted to be indigenous, representing thermally altered relicts of cellular material (i.e., kerogen). Here we show that stromatolitic black cherts from the Gunflint Formation, Schreiber Beach, Ontario, Canada, were saturated in syn-sedimentary oil. The thermally altered oil (pyrobitumen), which occurs in the stromatolites and intercolumn sediments, fills pores and fractures, and coats detrital and diagenetic grain surfaces. The occurrence of detrital bitumen grains in the stromatolites points to the proximity of shallow seafloor oil seeps and hence the possible existence of chemosynthetic microbes degrading hydrocarbons. We suggest that hydrocarbons that migrated through the silicifying stromatolites infiltrated semi-hollow microbial molds that formed following silica nucleation on the walls or sheaths of decayed cells. Upon heating, the hydrocarbons were transformed to nanoporous pyrobitumen, retarding silica recrystallization and enhancing detailed preservation of the carbon-rich microfossils. Hydrocarbon infiltration of silicified microbes offers a new explanation for the preservation of the Gunflint microfossils and may have played a role in the formation of some of Earth's oldest microfossils.
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Affiliation(s)
- B Rasmussen
- School of Earth Sciences, The University of Western Australia, Perth, Australia
| | - J R Muhling
- School of Earth Sciences, The University of Western Australia, Perth, Australia
| | - W W Fischer
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA
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2
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The search for organic compounds with TMAH thermochemolysis: From Earth analyses to space exploration experiments. Trends Analyt Chem 2020. [DOI: 10.1016/j.trac.2020.115896] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/12/2022]
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Jacquemot P, Viennet JC, Bernard S, Le Guillou C, Rigaud B, Delbes L, Georgelin T, Jaber M. The degradation of organic compounds impacts the crystallization of clay minerals and vice versa. Sci Rep 2019; 9:20251. [PMID: 31882914 PMCID: PMC6934458 DOI: 10.1038/s41598-019-56756-6] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/19/2019] [Accepted: 11/28/2019] [Indexed: 12/03/2022] Open
Abstract
Expanding our capabilities to unambiguously identify ancient traces of life in ancient rocks requires laboratory experiments to better constrain the evolution of biomolecules during advanced fossilization processes. Here, we submitted RNA to hydrothermal conditions in the presence of a gel of Al-smectite stoichiometry at 200 °C for 20 days. NMR and STXM-XANES investigations revealed that the organic fraction of the residues is no longer RNA, nor the quite homogeneous aromatic-rich residue obtained in the absence of clays, but rather consists of particles of various chemical composition including amide-rich compounds. Rather than the pure clays obtained in the absence of RNA, electron microscopy (SEM and TEM) and diffraction (XRD) data showed that the mineralogy of the experimental residues includes amorphous silica and aluminosilicates mixed together with nanoscales phosphates and clay minerals. In addition to the influence of clay minerals on the degradation of organic compounds, these results evidence the influence of the presence of organic compounds on the nature of the mineral assemblage, highlighting the importance of fine-scale mineralogical investigations when discussing the nature/origin of organo-mineral microstructures found in ancient rocks.
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Affiliation(s)
- Pierre Jacquemot
- National Museum of Natural History (MNHN), Sorbonne University, CNRS, Institute of Mineralogy, Material Physics and Cosmochemistry (IMPMC - UMR 7590), F-75005, Paris, France
- Sorbonne University, CNRS, Laboratory of Molecular and Structural Archeology (LAMS - UMR 8220), F-75005, Paris, France
| | - Jean-Christophe Viennet
- National Museum of Natural History (MNHN), Sorbonne University, CNRS, Institute of Mineralogy, Material Physics and Cosmochemistry (IMPMC - UMR 7590), F-75005, Paris, France
- Sorbonne University, CNRS, Laboratory of Molecular and Structural Archeology (LAMS - UMR 8220), F-75005, Paris, France
| | - Sylvain Bernard
- National Museum of Natural History (MNHN), Sorbonne University, CNRS, Institute of Mineralogy, Material Physics and Cosmochemistry (IMPMC - UMR 7590), F-75005, Paris, France.
| | | | | | - Ludovic Delbes
- National Museum of Natural History (MNHN), Sorbonne University, CNRS, Institute of Mineralogy, Material Physics and Cosmochemistry (IMPMC - UMR 7590), F-75005, Paris, France
| | | | - Maguy Jaber
- Sorbonne University, CNRS, Laboratory of Molecular and Structural Archeology (LAMS - UMR 8220), F-75005, Paris, France
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Mechanistic Morphogenesis of Organo-Sedimentary Structures Growing Under Geochemically Stressed Conditions: Keystone to Proving the Biogenicity of Some Archaean Stromatolites? GEOSCIENCES 2019. [DOI: 10.3390/geosciences9080359] [Citation(s) in RCA: 13] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Morphologically diverse organo-sedimentary structures (including microbial mats and stromatolites) provide a palaeobiological record through more than three billion years of Earth history. Since understanding much of the Archaean fossil record is contingent upon proving the biogenicity of such structures, mechanistic interpretations of well-preserved fossil microbialites can reinforce our understanding of their biogeochemistry and distinguish unambiguous biological characteristics in these structures, which represent some of the earliest records of life. Mechanistic morphogenetic understanding relies upon the analysis of geomicrobiological experiments. Herein, we report morphological-biogeochemical comparisons between micromorphologies observed in growth experiments using photosynthetic mats built by the cyanobacterium Coleofasciculus chthonoplastes (formerly Microcoleus) and green anoxygenic phototrophic Chloroflexus spp. (i.e., Coleofasciculus–Chloroflexus mats), and Precambrian organo-sedimentary structures, demonstrating parallels between them. In elevated ambient concentrations of Cu (toxic to Coleofasciculus), Coleofasciculus–Chloroflexus mats respond by forming centimetre-scale pinnacle-like structures (supra-lamina complexities) associated with large quantities of EPS at their surfaces. µPIXE mapping shows that Cu and other metals become concentrated within surficial sheath-EPS-Chloroflexus-rich layers, producing density-differential micromorphologies with distinct fabric orientations that are detectable using X-ray computed micro-tomography (X-ray µCT). Similar micromorphologies are also detectable in stromatolites from the 3.481 Ga Dresser Formation (Pilbara, Western Australia). The cause and response link between the presence of toxic elements (geochemical stress) and the development of multi-layered topographical complexities in organo-sedimentary structures may thus be considered an indicator of biogenicity, being an indisputably biological and predictable morphogenetic response reflecting, in this case, the differential responses of Coleofasciculus and Chloroflexus to Cu. Growth models for microbialite morphogenesis rely upon linking morphology to intrinsic (biological) and extrinsic (environmental) influences. Since the pinnacles of Coleofasciculus–Chloroflexus mats have an unambiguously biological origin linked to extrinsic geochemistry, we suggest that similar micromorphologies observed in ancient organo-sedimentary structures are indicative of biogenesis. An identical Coleofasciculus–Chloroflexus community subjected to salinity stress also produced supra-lamina complexities (tufts) but did not produce identifiable micromorphologies in three dimensions since salinity seems not to negatively impact either organism, and therefore cannot be used as a morphogenetic tool for the interpretation of density-homogeneous micro-tufted mats—for example, those of the 3.472 Ga Middle Marker horizon. Thus, although correlative microscopy is the keystone to confirming the biogenicity of certain Precambrian stromatolites, it remains crucial to separately interrogate each putative trace of ancient life, ideally using three-dimensional analyses, to determine, where possible, palaeoenvironmental influences on morphologies. Widespread volcanism and hydrothermal effusion into the early oceans likely concentrated toxic elements in early biomes. Morphological diversity in fossil microbialites could, therefore, reflect either (or both of) differential exposure to ambient fluids enriched in toxic elements and/or changing ecosystem structure and tolerance to elements through evolutionary time—for example, after incorporation into enzymes. Proof of biogenicity by deducing morphogenesis (i.e., a process preserved in the fossil record) overcomes many of the shortcomings inherent to the proof of biogenicity by descriptions of morphology alone.
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McMahon S, Ivarsson M. A New Frontier for Palaeobiology: Earth's Vast Deep Biosphere. Bioessays 2019; 41:e1900052. [PMID: 31241200 DOI: 10.1002/bies.201900052] [Citation(s) in RCA: 10] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/16/2019] [Revised: 04/29/2019] [Indexed: 11/11/2022]
Abstract
Diverse micro-organisms populate a global deep biosphere hosted by rocks and sediments beneath land and sea, containing more biomass than any other biome except forests. This paper reviews an emerging palaeobiological archive of these dark habitats: microfossils preserved in ancient pores and fractures in the crust. This archive, seemingly dominated by mineralized filaments (although rods and coccoids are also reported), is presently far too sparsely sampled and poorly understood to reveal trends in the abundance, distribution, or diversity of deep life through time. New research is called for to establish the nature and extent of the fossil record of Earth's deep biosphere by combining systematic exploration, rigorous microanalysis, and experimental studies of both microbial preservation and the formation of abiotic pseudofossils within the crust. It is concluded that the fossil record of Earth's largest microbial habitat may still have much to tell us about the history of life, the evolution of biogeochemical cycles, and the search for life on Mars.
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Affiliation(s)
- Sean McMahon
- School of Geosciences, University of Edinburgh, Edinburgh, EH8 9XP, UK.,UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, UK
| | - Magnus Ivarsson
- Department of Biology, University of Southern Denmark, DK-5230, Odense, Denmark.,Department of Palaeobiology, Swedish Museum of Natural History, Stockholm, SE-104 05, Sweden
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Gaboyer F, Le Milbeau C, Bohmeier M, Schwendner P, Vannier P, Beblo-Vranesevic K, Rabbow E, Foucher F, Gautret P, Guégan R, Richard A, Sauldubois A, Richmann P, Perras AK, Moissl-Eichinger C, Cockell CS, Rettberg P, Marteinsson, Monaghan E, Ehrenfreund P, Garcia-Descalzo L, Gomez F, Malki M, Amils R, Cabezas P, Walter N, Westall F. Mineralization and Preservation of an extremotolerant Bacterium Isolated from an Early Mars Analog Environment. Sci Rep 2017; 7:8775. [PMID: 28821776 PMCID: PMC5562696 DOI: 10.1038/s41598-017-08929-4] [Citation(s) in RCA: 12] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/12/2017] [Accepted: 07/14/2017] [Indexed: 11/09/2022] Open
Abstract
The artificial mineralization of a polyresistant bacterial strain isolated from an acidic, oligotrophic lake was carried out to better understand microbial (i) early mineralization and (ii) potential for further fossilisation. Mineralization was conducted in mineral matrixes commonly found on Mars and Early-Earth, silica and gypsum, for 6 months. Samples were analyzed using microbiological (survival rates), morphological (electron microscopy), biochemical (GC-MS, Microarray immunoassay, Rock-Eval) and spectroscopic (EDX, FTIR, RAMAN spectroscopy) methods. We also investigated the impact of physiological status on mineralization and long-term fossilisation by exposing cells or not to Mars-related stresses (desiccation and radiation). Bacterial populations remained viable after 6 months although the kinetics of mineralization and cell-mineral interactions depended on the nature of minerals. Detection of biosignatures strongly depended on analytical methods, successful with FTIR and EDX but not with RAMAN and immunoassays. Neither influence of stress exposure, nor qualitative and quantitative changes of detected molecules were observed as a function of mineralization time and matrix. Rock-Eval analysis suggests that potential for preservation on geological times may be possible only with moderate diagenetic and metamorphic conditions. The implications of our results for microfossil preservation in the geological record of Earth as well as on Mars are discussed.
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Affiliation(s)
- F Gaboyer
- Centre de Biophysique Moléculaire, CNRS, Orléans, France.
| | - C Le Milbeau
- Institut des Sciences de la Terre d'Orléans, UMR 7327, CNRS-Université d'Orléans, 1A Rue de la Férollerie, 45071, Orléans Cedex 2, France
| | - M Bohmeier
- Institute of Aerospace Medicine, Radiation Biology Department, German Aerospace Center (DLR), Cologne, Germany
| | - P Schwendner
- UK Center for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - P Vannier
- MATIS - Prokaria, Reykjavík, Iceland
| | - K Beblo-Vranesevic
- Institute of Aerospace Medicine, Radiation Biology Department, German Aerospace Center (DLR), Cologne, Germany
| | - E Rabbow
- Institute of Aerospace Medicine, Radiation Biology Department, German Aerospace Center (DLR), Cologne, Germany
| | - F Foucher
- Centre de Biophysique Moléculaire, CNRS, Orléans, France
| | - P Gautret
- Institut des Sciences de la Terre d'Orléans, UMR 7327, CNRS-Université d'Orléans, 1A Rue de la Férollerie, 45071, Orléans Cedex 2, France
| | - R Guégan
- Institut des Sciences de la Terre d'Orléans, UMR 7327, CNRS-Université d'Orléans, 1A Rue de la Férollerie, 45071, Orléans Cedex 2, France
| | - A Richard
- Centre de Microscopie Electronique, Université d'Orléans, Orléans, France
| | - A Sauldubois
- Centre de Microscopie Electronique, Université d'Orléans, Orléans, France
| | - P Richmann
- Institut des Sciences de la Terre d'Orléans, UMR 7327, CNRS-Université d'Orléans, 1A Rue de la Férollerie, 45071, Orléans Cedex 2, France
| | - A K Perras
- University Regensburg, Department of Microbiology, Regensburg, Germany.,Medical University of Graz, Department of Internal Medicine, Graz, Austria
| | | | - C S Cockell
- UK Center for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - P Rettberg
- Institute of Aerospace Medicine, Radiation Biology Department, German Aerospace Center (DLR), Cologne, Germany
| | | | - E Monaghan
- Leiden Observatory, Universiteit Leiden, Leiden, Netherlands
| | - P Ehrenfreund
- Leiden Observatory, Universiteit Leiden, Leiden, Netherlands
| | - L Garcia-Descalzo
- Instituto Nacional de Técnica Aeroespacial - Centro de Astrobiología (INTA-CAB), Madrid, Spain
| | - F Gomez
- Instituto Nacional de Técnica Aeroespacial - Centro de Astrobiología (INTA-CAB), Madrid, Spain
| | - M Malki
- Universidad Autónoma de Madrid (UAM), Madrid, Spain
| | - R Amils
- Universidad Autónoma de Madrid (UAM), Madrid, Spain
| | - P Cabezas
- European Science Foundation (ESF), Strasbourg, France
| | - N Walter
- European Science Foundation (ESF), Strasbourg, France
| | - F Westall
- Centre de Biophysique Moléculaire, CNRS, Orléans, France
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7
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Picard A, Obst M, Schmid G, Zeitvogel F, Kappler A. Limited influence of Si on the preservation of Fe mineral-encrusted microbial cells during experimental diagenesis. GEOBIOLOGY 2016; 14:276-292. [PMID: 26695194 DOI: 10.1111/gbi.12171] [Citation(s) in RCA: 13] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/22/2015] [Accepted: 11/10/2015] [Indexed: 06/05/2023]
Abstract
The reconstruction of the history of microbial life since its emergence on early Earth is impaired by the difficulty to prove the biogenicity of putative microfossils in the rock record. While most of the oldest rocks on Earth have been exposed to different grades of diagenetic alterations, little is known about how the remains of micro-organisms evolve when exposed to pressure (P) and temperature (T) conditions typical of diagenesis. Using spectroscopy and microscopy, we compared morphological, mineralogical, and chemical biosignatures exhibited by Fe mineral-encrusted cells of the bacterium Acidovorax sp. BoFeN1 after long-term incubation under ambient conditions and after experimental diagenesis. We also evaluated the effects of Si on the preservation of microbial cells during the whole process. At ambient conditions, Si affected the morphology but not the identity (goethite) of Fe minerals that formed around cells. Fe-encrusted cells were morphologically well preserved after 1 week at 250 °C-140 MPa and after 16 weeks at 170 °C-120 MPa in the presence or in the absence of Si. Some goethite transformed to hematite and magnetite at 250 °C-140 MPa, but in the presence of Si more goethite was preserved. Proteins-the most abundant cellular components-were preserved over several months at ambient conditions but disappeared after incubations at high temperature and pressure conditions, both in the presence and in the absence of Si. Other organic compounds, such as lipids and extracellular polysaccharides seemed well preserved after exposure to diagenetic conditions. This study provides insights about the composition and potential preservation of microfossils that could have formed in Fe- and Si-rich Precambrian oceans.
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Affiliation(s)
- A Picard
- Center for Applied Geoscience, Eberhard Karls University Tübingen, Tübingen, Germany
| | - M Obst
- Center for Applied Geoscience, Eberhard Karls University Tübingen, Tübingen, Germany
| | - G Schmid
- Center for Applied Geoscience, Eberhard Karls University Tübingen, Tübingen, Germany
| | - F Zeitvogel
- Center for Applied Geoscience, Eberhard Karls University Tübingen, Tübingen, Germany
| | - A Kappler
- Center for Applied Geoscience, Eberhard Karls University Tübingen, Tübingen, Germany
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8
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Experimental diagenesis of organo-mineral structures formed by microaerophilic Fe(II)-oxidizing bacteria. Nat Commun 2015; 6:6277. [DOI: 10.1038/ncomms7277] [Citation(s) in RCA: 70] [Impact Index Per Article: 7.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/01/2014] [Accepted: 01/13/2015] [Indexed: 11/08/2022] Open
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