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hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorRODIER, C.
hal.structure.identifierOrganisation moléculaire (évolution et matériaux fluores) [OMEMF]
dc.contributor.authorVANDENABEELE-TRAMBOUZE, O.
hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorSTERNBERG, R.
hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorCOSCIA, David
hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorCOLL, Patrice
hal.structure.identifierService d'aéronomie [SA]
dc.contributor.authorSZOPA, Cyril
hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorRAULIN, François
hal.structure.identifierLaboratoire de recherches sur les polymères [LRP]
dc.contributor.authorVIDAL-MADJAR, C.
hal.structure.identifierService d'aéronomie [SA]
dc.contributor.authorCABANE, Michel
hal.structure.identifierService d'aéronomie [SA]
dc.contributor.authorISRAEL, Guy
hal.structure.identifierService Central d'Analyse [SCA]
dc.contributor.authorGRENIER-LOUSTALOT, M.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDOBRIJEVIC, M.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDESPOIS, D.
dc.date.issued2001-01
dc.identifier.issn0273-1177
dc.description.abstractEnIf there is, or ever was, life in our solar system beyond the Earth, Mars is the most likely place to search for. Future space missions will have then to take into account the detection of prebiotic molecules or molecules of biological significance such as amino acids. Techniques of analysis used for returned samples have to be very sensitive and avoid any chemical or biological contamination whereas in situ techniques have to be automated, fast and low energy consuming. Several possible methods could be used for in situ amino acid analyses on Mars, but gas chromatography would likely be the most suitable. Returned samples could be analyzed by any method in routine laboratory use such as gas chromatography, already successfully performed for analyses of organic matter including amino acids from martian meteorites. The derivatization step, which volatilizes amino acids to perform both in situ and laboratory analysis by gas chromatography, is discussed here.
dc.language.isoen
dc.publisherElsevier
dc.title.enDetection of martian amino acids by chemical derivatization coupled to gas chromatography: In situ and laboratory analysis
dc.typeArticle de revue
dc.identifier.doi10.1016/S0273-1177(01)00047-3
dc.subject.halPlanète et Univers [physics]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalAdvances in Space Research
bordeaux.page195 - 199
bordeaux.volume27
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-01680599
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01680599v1
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