Experimental clues for detecting biosignatures on Mars

Viennet, J.-C.; Bernard, S.; Le Guillou, C.; Jacquemot, P.; Balan, E.; Delbes, L.; Rigaud, B.; Georgelin, T.; Jaber, M.

Type de document :

Article dans une revue scientifique: Article original

DOI :

10.7185/geochemlet.1931

URL permanente :

http://hdl.handle.net/20.500.12210/16660

Titre :

Experimental clues for detecting biosignatures on Mars

Auteur(s) :

Viennet, J.-C. [Auteur]
Bernard, S. [Auteur]
Le Guillou, C. [Auteur]
Jacquemot, P. [Auteur]
Balan, E. [Auteur]
Delbes, L. [Auteur]
Rigaud, B. [Auteur]
Georgelin, T. [Auteur]
Jaber, M. [Auteur]

Titre de la revue :

Geochemical Perspectives Letters

Nom court de la revue :

Geochem. Persp. Let.

Pagination :

28-33

Éditeur :

European Association of Geochemistry

Date de publication :

2019-11

ISSN :

2410-3403

Résumé en anglais : [en]

Forthcoming exploration of Mars aims at identifying fossil biosignatures within ancient clay-rich formations. The subsurface of Mars has mostly acted as a giant freezer for the last 4 Gyr, thereby preserving potential ...
Lire la suite >Forthcoming exploration of Mars aims at identifying fossil biosignatures within ancient clay-rich formations. The subsurface of Mars has mostly acted as a giant freezer for the last 4 Gyr, thereby preserving potential remains of martian life. Yet, volcanism and impactors have periodically triggered the circulation of hydrothermal fluids, inevitably causing alteration of potentially fossilised biogenic organic materials. It thus appears crucial to quantify the impact of hydrothermal processes on organic biogeochemical signals in the presence of clay minerals. Here, we submitted RNA to hydrothermal conditions in the presence of Mg-smectites. Results show heterogeneous organo-mineral residues, with sub-micrometric phosphates, carbonates and amorphous silica particles together with Mg-smectites with interlayer spaces saturated by N-rich organic compounds. Although the chemical structure of RNA did not withstand hydrothermal conditions, clay minerals efficiently trapped organic carbon, confirming the relevance of drilling for organic carbon in ancient martian sediments. In addition, the degradation of RNA in the presence of Mg-smectites led to the precipitation of a quite uncommon mineral assemblage that could be seen as a biosignature per se. Martian targets exhibiting this mineral assemblage will thus constitute high priority and highly relevant candidates for sample return.Lire moins >

Langue :

Anglais

Comité de lecture :

Oui

Audience :

Non spécifiée

Établissement(s) :

Université de Lille
CNRS
INRA
ENSCL

Collections :

Unité Matériaux et Transformations (UMET) - UMR 8207

Équipe(s) de recherche :

Matériaux Terrestres et Planétaires

Date de dépôt :

2019-11-29T14:53:44Z

Historique des modifications

Numéro de version	Lien	Date de modification
4	20.500.12210/16660	2020-07-18T13:26:14Z
3	20.500.12210/16660.3	2019-12-17T08:57:01Z
1	20.500.12210/16660.1*	2019-11-29T14:53:44Z

*Version sélectionnée

Experimental clues for detecting biosignatures ...

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Experimental clues for detecting biosignatures ... BibTeX CSV Excel RIS

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Experimental clues for detecting biosignatures ...

BibTeX

CSV

Excel

RIS