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dc.contributor.authorYeşiltaş, Mehmet
dc.contributor.authorGlotch, Timothy D.
dc.contributor.authorSava, Boğdan
dc.date.accessioned2021-12-12T17:03:21Z
dc.date.available2021-12-12T17:03:21Z
dc.date.issued2021
dc.identifier.issn2045-2322
dc.identifier.urihttps://doi.org/10.1038/s41598-021-91200-8
dc.identifier.urihttps://hdl.handle.net/20.500.11857/3660
dc.description.abstractMeteorites contain organic matter that may have contributed to the origin of life on Earth. Carbonyl compounds such as aldehydes and carboxylic acids, which occur in meteorites, may be precursors of biologically necessary organic materials in the solar system. Therefore, such organic matter is of astrobiological importance and their detection and characterization can contribute to the understanding of the early solar system as well as the origin of life. Most organic matter is typically sub-micrometer in size, and organic nanoglobules are even smaller (50-300 nm). Novel analytical techniques with nanoscale spatial resolution are required to detect and characterize organic matter within extraterrestrial materials. Most techniques require powdered samples, consume the material, and lose petrographic context of organics. Here, we report the detection of nanoglobular aldehyde and carboxylic acids in a highly primitive carbonaceous chondrite (DOM 08006) with similar to 20 nm spatial resolution using nano-FTIR spectroscopy. Such organic matter is found within the matrix of DOM 08006 and is typically 50-300 nm in size. We also show petrographic context and nanoscale morphologic/topographic features of the organic matter. Our results indicate that prebiotic carbonyl nanoglobules can form in a less aqueous and relatively elevated temperature-environment (220-230 degrees C) in a carbonaceous parent body.en_US
dc.description.sponsorshipRISE2 node of NASA's Solar System Exploration Research Virtual Institute (SSERVI)en_US
dc.description.sponsorshipWe thank the associate editor and the reviewers for their constructive comments, which significantly improved this manuscript. We thank NASA-JSC for providing the meteorite samples. This work was also supported in part by the RISE2 node of NASA's Solar System Exploration Research Virtual Institute (SSERVI; PI: T.D. Glotch).en_US
dc.language.isoengen_US
dc.publisherNature Portfolioen_US
dc.relation.ispartofScientific Reportsen_US
dc.identifier.doi10.1038/s41598-021-91200-8
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectInsoluble Organic-Matteren_US
dc.subjectTagish Lake Meteoriteen_US
dc.subjectInfrared-Spectroscopyen_US
dc.subjectCarboxylic-Acidsen_US
dc.subjectSolar-Systemen_US
dc.subjectSpectraen_US
dc.subjectMetamorphismen_US
dc.subjectAldehydesen_US
dc.subjectMineralsen_US
dc.subjectGrainsen_US
dc.titleNano-FTIR spectroscopic identification of prebiotic carbonyl compounds in Dominion Range 08006 carbonaceous chondriteen_US
dc.typearticle
dc.departmentFakülteler, Lüleburgaz Havacılık ve Uzay Bilimleri Fakültesi, Havacılık ve Uzay Mühendisliği Bölümü
dc.identifier.volume11en_US
dc.identifier.issue1en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.authorscopusid23020484700
dc.authorscopusid6507290607
dc.authorscopusid57224165810
dc.identifier.wosWOS:000687322500079en_US
dc.identifier.scopus2-s2.0-85107118526en_US
dc.identifier.pmidPubMed: 34079034en_US


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