Influence of the nature of the gas phase ...
Document type :
Article dans une revue scientifique: Article original
Permalink :
Title :
Influence of the nature of the gas phase on the degradation of RNA during fossilization processes
Author(s) :
Viennet, J.-C. [Auteur]
Bernard, S. [Auteur]
Le Guillou, Corentin [Auteur]
Unité Matériaux et Transformations - UMR 8207 [UMET]
Jacquemot, P. [Auteur]
Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC]
Delbes, L. [Auteur]
Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC]
Balan, E. [Auteur]
Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC]
Jaber, M. [Auteur]
Bernard, S. [Auteur]
Le Guillou, Corentin [Auteur]
Unité Matériaux et Transformations - UMR 8207 [UMET]
Jacquemot, P. [Auteur]
Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC]
Delbes, L. [Auteur]
Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC]
Balan, E. [Auteur]
Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC]
Jaber, M. [Auteur]
Journal title :
Applied Clay Science
Abbreviated title :
Applied Clay Science
Volume number :
191
Pages :
105616
Publisher :
Elsevier BV
Publication date :
2020-06
ISSN :
0169-1317
English keyword(s) :
Biosignatures
Fossilization
RNA world
Clay minerals
Gas phase
Fossilization
RNA world
Clay minerals
Gas phase
HAL domain(s) :
Chimie/Matériaux
Physique [physics]/Matière Condensée [cond-mat]/Science des matériaux [cond-mat.mtrl-sci]
Physique [physics]/Physique [physics]/Géophysique [physics.geo-ph]
Physique [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Sciences de la Terre
Physique [physics]/Matière Condensée [cond-mat]/Science des matériaux [cond-mat.mtrl-sci]
Physique [physics]/Physique [physics]/Géophysique [physics.geo-ph]
Physique [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Sciences de la Terre
English abstract : [en]
The search for the most ancient traces of life on Earth has always been fraught with controversies because of the inevitable degradation undergone by fossilized biomolecules. Laboratory experiments may provide unique clues ...
Show more >The search for the most ancient traces of life on Earth has always been fraught with controversies because of the inevitable degradation undergone by fossilized biomolecules. Laboratory experiments may provide unique clues to achieve a better mechanistic understanding of the key processes involving (biogenic or abiotic) organic carbon during a geological history. The Earth atmosphere has changed over geological times, from a CO2-rich atmosphere during the Hadean and Archean to the O2-rich atmosphere of the present day, with a direct impact on the nature of the gas phase trapped within the sediment porosity. Yet, the influence of the nature of this gas phase on fossilization processes has almost never been investigated. Here, we conducted a series of fossilization experiments using an emblematic biomolecule (i.e. RNA) and clay minerals at 200 °C for 7 days in closed systems in equilibrium with two different gas phases (e.g. CO2 versus N2/O2). The multiscale characterization of experimental residues using a suite of advanced microscopy and spectroscopy techniques showed that the final organo-mineral assemblages strongly depend on the nature of the gas phase. In addition to the nature of the mineral phases, results showed that the nature of the gas phase impacts the chemistry of the residual N-rich organic compounds trapped within the interlayer spaces of Mg-smectites (e.g. mainly aliphatic-rich under CO2 vs dominated by heterocycles under N2/O2). Altogether, the present study demonstrates the necessity to take into account the nature of the gas phase composition when experimentally simulating fossilization processes aiming at better constraining which biosignatures may be preserved in ancient rocks. Finally, the experimental results reported here may serve to identify the potential biosignatures that should be searched for on other planetary bodies.Show less >
Show more >The search for the most ancient traces of life on Earth has always been fraught with controversies because of the inevitable degradation undergone by fossilized biomolecules. Laboratory experiments may provide unique clues to achieve a better mechanistic understanding of the key processes involving (biogenic or abiotic) organic carbon during a geological history. The Earth atmosphere has changed over geological times, from a CO2-rich atmosphere during the Hadean and Archean to the O2-rich atmosphere of the present day, with a direct impact on the nature of the gas phase trapped within the sediment porosity. Yet, the influence of the nature of this gas phase on fossilization processes has almost never been investigated. Here, we conducted a series of fossilization experiments using an emblematic biomolecule (i.e. RNA) and clay minerals at 200 °C for 7 days in closed systems in equilibrium with two different gas phases (e.g. CO2 versus N2/O2). The multiscale characterization of experimental residues using a suite of advanced microscopy and spectroscopy techniques showed that the final organo-mineral assemblages strongly depend on the nature of the gas phase. In addition to the nature of the mineral phases, results showed that the nature of the gas phase impacts the chemistry of the residual N-rich organic compounds trapped within the interlayer spaces of Mg-smectites (e.g. mainly aliphatic-rich under CO2 vs dominated by heterocycles under N2/O2). Altogether, the present study demonstrates the necessity to take into account the nature of the gas phase composition when experimentally simulating fossilization processes aiming at better constraining which biosignatures may be preserved in ancient rocks. Finally, the experimental results reported here may serve to identify the potential biosignatures that should be searched for on other planetary bodies.Show less >
Language :
Anglais
Peer reviewed article :
Oui
Audience :
Internationale
Popular science :
Non
Administrative institution(s) :
Université de Lille
CNRS
INRA
ENSCL
CNRS
INRA
ENSCL
Collections :
Research team(s) :
Matériaux Terrestres et Planétaires
Submission date :
2021-11-18T15:10:37Z
2021-11-22T09:39:38Z
2021-11-22T09:39:38Z