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dc.contributor.authorJaramillo, Elizabeth A.
dc.contributor.authorRoyle, Samuel H.
dc.contributor.authorClaire, Mark W.
dc.contributor.authorKounaves, Samuel P.
dc.contributor.authorSephton, Mark A.
dc.date.accessioned2019-03-22T14:30:06Z
dc.date.available2019-03-22T14:30:06Z
dc.date.issued2019-03-28
dc.identifier258223374
dc.identifier58348456-0896-4ba8-8b71-c616e8e889ab
dc.identifier85064233023
dc.identifier000464650400009
dc.identifier.citationJaramillo , E A , Royle , S H , Claire , M W , Kounaves , S P & Sephton , M A 2019 , ' Indigenous organic-oxidized fluid interactions in the Tissint Mars meteorite ' , Geophysical Research Letters , vol. 46 , no. 6 , pp. 3090-3098 . https://doi.org/10.1029/2018GL081335en
dc.identifier.issn0094-8276
dc.identifier.otherRIS: urn:C8FC8F6683153B914C968296400FFF96
dc.identifier.otherORCID: /0000-0001-9518-089X/work/55643821
dc.identifier.urihttps://hdl.handle.net/10023/17349
dc.descriptionPart of this work was supported by UK Space Agency Grant ST/N000560/1 and by internal funding by Tufts University and the School of Earth and Environmental Sciences at the University of St Andrews.en
dc.description.abstractThe observed fall and rapid recovery of the Tissint Mars meteorite has provided minimally contaminated samples of the Martian surface. We report analyses of Tissint for organic compounds by pyrolysis-gas chromatography-mass spectrometry and for soluble salts by ion chromatography. Pyrolysis-gas chromatography-mass spectrometry analysis shows the presence of organic compounds similar to those in the Mars EETA79001 and Nakhla meteorites. The organic profile is dominated by aromatic hydrocarbons, including oxygen and nitrogen-containing aromatics, and sulfur-containing species including thiophenes. The soluble salts in Tissint are dominated by sulfate and various oxidation states of chlorine, including perchlorate. The organic compounds and salts in the soils from the Tissint recovery strewn field differ significantly from those found in Tissint suggesting minimal terrestrial contamination. Our results support the hypothesis that the soluble inorganic components of Tissint are most likely a result of indigenous fluid inclusion, thus providing a glimpse into the composition of early Martian fluids.
dc.format.extent629018
dc.language.isoeng
dc.relation.ispartofGeophysical Research Lettersen
dc.subjectMarsen
dc.subjectMeteoriteen
dc.subjectOrganicsen
dc.subjectSaltsen
dc.subjectFluidsen
dc.subjectGE Environmental Sciencesen
dc.subjectNDASen
dc.subject.lccGEen
dc.titleIndigenous organic-oxidized fluid interactions in the Tissint Mars meteoriteen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews. St Andrews Isotope Geochemistryen
dc.identifier.doihttps://doi.org/10.1029/2018GL081335
dc.description.statusPeer revieweden


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