Unveiling Challenging Microbial Fossil Biosignatures from Rio Tinto with Micro-to-Nanoscale Chemical and Ultrastructural Imaging.

Fossil Biosignatures Geomicrobiology Mars Microfossils Multiscale Nano-X-Ray Fluorescence Ptychographic X-Ray Computed Laminography Rio Tinto X-Ray Nanoimaging

Journal

Astrobiology
ISSN: 1557-8070
Titre abrégé: Astrobiology
Pays: United States
ID NLM: 101088083

Informations de publication

Date de publication:
10 Jul 2024
Historique:
medline: 10 7 2024
pubmed: 10 7 2024
entrez: 10 7 2024
Statut: aheadofprint

Résumé

Understanding the nature and preservation of microbial traces in extreme environments is crucial for reconstructing Earth's early biosphere and for the search for life on other planets or moons. At Rio Tinto, southwestern Spain, ferric oxide and sulfate deposits similar to those discovered at Meridiani Planum, Mars, entomb a diversity of fossilized organisms, despite chemical conditions commonly thought to be challenging for life and fossil preservation. Investigating this unique fossil microbiota can elucidate ancient extremophile communities and the preservation of biosignatures in acidic environments on Earth and, potentially, Mars. In this study, we use an innovative multiscale approach that combines the state-of-the-art synchrotron X-ray nanoimaging methods of ptychographic X-ray computed laminography and nano-X-ray fluorescence to reveal Rio Tinto's microfossils at subcellular resolution. The unprecedented nanoscale views of several different specimens within their geological and geochemical contexts reveal novel intricacies of preserved microbial communities. Different morphotypes, ecological interactions, and possible taxonomic affinities were inferred based on qualitative and quantitative 3D ultrastructural information, whereas diagenetic processes and metabolic affinities were inferred from complementary chemical information. Our integrated nano-to-microscale analytical approach revealed previously invisible microbial and mineral interactions, which complemented and filled a gap of spatial resolution in conventional methods. Ultimately, this study contributes to the challenge of deciphering the faint chemical and morphological biosignatures that can indicate life's presence on the early Earth and on distant worlds.

Identifiants

pubmed: 38985734
doi: 10.1089/ast.2023.0127
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Auteurs

Lara Maldanis (L)

ISTerre, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, IFSTTAR, Grenoble, France.

David Fernandez-Remolar (D)

SKL Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China.
CNSA Macau Center for Space Exploration and Science, Macau, China.

Laurence Lemelle (L)

LGL-TPE, ENS de Lyon, Univ. de Lyon, CNRS, Lyon, France.

Andrew H Knoll (AH)

Department of Organismic and Evolutionary Biology, Harvard University, Cambridge Massachusetts, USA.

Manuel Guizar-Sicairos (M)

Paul Scherrer Institute, Villigen PSI, Switzerland.
Institute of Physics, École Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland.

Mirko Holler (M)

Paul Scherrer Institute, Villigen PSI, Switzerland.

Francisco Mateus Cirilo da Silva (FMC)

Brazilian Synchrotron Light Laboratory, LNLS, Brazilian Center for Research in Energy and Materials, CNPEM, Campinas, Brazil.
Institute of Physics, IFGW, Campinas University, UNICAMP, Campinas, Brazil.

Valérie Magnin (V)

ISTerre, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, IFSTTAR, Grenoble, France.

Michel Mermoux (M)

LEPMI, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, Grenoble INP, 38000 Grenoble, France.

Alexandre Simionovici (A)

ISTerre, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, IFSTTAR, Grenoble, France.

Classifications MeSH