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Viennet JC, Bernard S, Le Guillou C, Sautter V, Grégoire B, Jambon A, Pont S, Beyssac O, Zanda B, Hewins R, Remusat L. Martian Magmatic Clay Minerals Forming Vesicles: Perfect Niches for Emerging Life? Astrobiology 2021; 21:605-612. [PMID: 33684326 DOI: 10.1089/ast.2020.2345] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/12/2023]
Abstract
Mars was habitable in its early history, but the consensus is that it is quite inhospitable today, in particular because its modern climate cannot support stable liquid water at the surface. Here, we report the presence of magmatic Fe/Mg clay minerals within the mesostasis of the martian meteorite NWA 5790, an unaltered 1.3 Ga nakhlite archetypal of the martian crust. These magmatic clay minerals exhibit a vesicular texture that forms a network of microcavities or pockets, which could serve as microreactors and allow molecular crowding, a necessary step for the emergence of life. Because their formation does not depend on climate, such niches for emerging life may have been generated on Mars at many periods throughout its history, regardless of the stability or availability of liquid water at the surface.
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Affiliation(s)
- Jean-Christophe Viennet
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Sylvain Bernard
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Corentin Le Guillou
- Université Lille, CNRS, INRA, ENSCL, UMR 8207 - UMET - Unité Matériaux et Transformations, Lille, France
| | - Violaine Sautter
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Brian Grégoire
- Centre National de la Recherche Scientifique (CNRS), Université de Poitiers, UMR 7285 IC2MP-Hydrasa, Poitiers, France
| | - Albert Jambon
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Sylvain Pont
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Olivier Beyssac
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Brigitte Zanda
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Roger Hewins
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
| | - Laurent Remusat
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, Paris, France
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Megevand V, Viennet JC, Balan E, Gauthier M, Rosier P, Morand M, Garino Y, Guillaumet M, Pont S, Beyssac O, Bernard S. Impact of UV Radiation on the Raman Signal of Cystine: Implications for the Detection of S-rich Organics on Mars. Astrobiology 2021; 21:566-574. [PMID: 33691484 DOI: 10.1089/ast.2020.2340] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/12/2023]
Abstract
Traces of life may have been preserved in ancient martian rocks in the form of molecular fossils. Yet the surface of Mars is continuously exposed to intense UV radiation detrimental to the preservation of organics. Because the payload of the next rovers going to Mars to seek traces of life will comprise Raman spectroscopy tools, laboratory simulations that document the effect of UV radiation on the Raman signal of organics appear critically needed. The experiments conducted here evidence that UV radiation is directly responsible for the increase of disorder and for the creation of electronic defects and radicals within the molecular structure of S-rich organics such as cystine, enhancing the contribution of light diffusion processes to the Raman signal. The present results suggest that long exposure to UV radiation would ultimately be responsible for the total degradation of the Raman signal of cystine. Yet because the degradation induced by UV is not instantaneous, it should be possible to detect freshly excavated S-rich organics with the Raman instruments on board the rovers. Alternatively, given the very short lifetime of organic fluorescence (nanoseconds) compared to most mineral luminescence (micro- to milliseconds), exploiting fluorescence signals might allow the detection of S-rich organics on Mars. In any case, as illustrated here, we should not expect to detect pristine S-rich organic compounds on Mars, but rather by-products of their degradation.
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Affiliation(s)
- V Megevand
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
- Ecole Normale Supérieure de Lyon, Université Claude Bernard Lyon 1, Lyon, France
| | - J C Viennet
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - E Balan
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - M Gauthier
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - P Rosier
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - M Morand
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - Y Garino
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - M Guillaumet
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - S Pont
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - O Beyssac
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
| | - S Bernard
- Muséum National d'Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, Paris, France
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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] [What about the content of this article? (0)] [Affiliation(s)] [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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