Adeline Garcia, Yingfei Yan, Cornelia Meinert, Philippe Schmitt-Kopplin, Vassilissa Vinogradoff, Jean-Christophe Viennet, Laurent Remusat, Sylvain Bernard, Michel Righezza, Louis Le Sergeant d’Hendecourt and Grégoire Danger*,
{"title":"模拟碳质软玉母体中的分子多样性和氨基酸演化","authors":"Adeline Garcia, Yingfei Yan, Cornelia Meinert, Philippe Schmitt-Kopplin, Vassilissa Vinogradoff, Jean-Christophe Viennet, Laurent Remusat, Sylvain Bernard, Michel Righezza, Louis Le Sergeant d’Hendecourt and Grégoire Danger*, ","doi":"10.1021/acsearthspacechem.3c00366","DOIUrl":null,"url":null,"abstract":"<p >In interplanetary bodies, organics are found originating from various environments. We replicate the solid-phase conditions in a laboratory to elucidate the step-by-step evolution of organic matter, spanning from dense molecular cloud ices to processes occurring within meteorite parent bodies. The focus of our work is on amino acids, considered as potential chemical tracers of secondary alteration on asteroids. Using gas chromatography and high-resolution mass spectrometry, trace amounts of amino acids are identified in a preaccretional organic analogue formed from a dense molecular ice analogue. This analogue was subsequently exposed to aqueous alteration. This induced an increase in the formation of α- and β-amino acids over time. Supported by high-resolution mass spectrometry data, the reactions involved sugars and amine compounds, followed by amino acid destruction due to the Maillard reaction, which consumes both sugars and amino acids. Surprisingly, a second phase of amino acid formation, specifically α-amino acids, was observed, indicating the potential occurrence of the Strecker reaction. We demonstrate the intricate chemical network occurring within the presence of molecular diversity, similar to what might occur during parent body alteration. Therefore, investigations on reactivity within meteorite parent bodies have to take into account their molecular diversity, recognizing potential cross-reactions, as demonstrated in this work.</p>","PeriodicalId":15,"journal":{"name":"ACS Earth and Space Chemistry","volume":null,"pages":null},"PeriodicalIF":2.9000,"publicationDate":"2024-03-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Molecular Diversity and Amino Acid Evolution in Simulated Carbonaceous Chondrite Parent Bodies\",\"authors\":\"Adeline Garcia, Yingfei Yan, Cornelia Meinert, Philippe Schmitt-Kopplin, Vassilissa Vinogradoff, Jean-Christophe Viennet, Laurent Remusat, Sylvain Bernard, Michel Righezza, Louis Le Sergeant d’Hendecourt and Grégoire Danger*, \",\"doi\":\"10.1021/acsearthspacechem.3c00366\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p >In interplanetary bodies, organics are found originating from various environments. We replicate the solid-phase conditions in a laboratory to elucidate the step-by-step evolution of organic matter, spanning from dense molecular cloud ices to processes occurring within meteorite parent bodies. The focus of our work is on amino acids, considered as potential chemical tracers of secondary alteration on asteroids. Using gas chromatography and high-resolution mass spectrometry, trace amounts of amino acids are identified in a preaccretional organic analogue formed from a dense molecular ice analogue. This analogue was subsequently exposed to aqueous alteration. This induced an increase in the formation of α- and β-amino acids over time. Supported by high-resolution mass spectrometry data, the reactions involved sugars and amine compounds, followed by amino acid destruction due to the Maillard reaction, which consumes both sugars and amino acids. Surprisingly, a second phase of amino acid formation, specifically α-amino acids, was observed, indicating the potential occurrence of the Strecker reaction. We demonstrate the intricate chemical network occurring within the presence of molecular diversity, similar to what might occur during parent body alteration. Therefore, investigations on reactivity within meteorite parent bodies have to take into account their molecular diversity, recognizing potential cross-reactions, as demonstrated in this work.</p>\",\"PeriodicalId\":15,\"journal\":{\"name\":\"ACS Earth and Space Chemistry\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":2.9000,\"publicationDate\":\"2024-03-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"ACS Earth and Space Chemistry\",\"FirstCategoryId\":\"92\",\"ListUrlMain\":\"https://pubs.acs.org/doi/10.1021/acsearthspacechem.3c00366\",\"RegionNum\":3,\"RegionCategory\":\"化学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"CHEMISTRY, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"ACS Earth and Space Chemistry","FirstCategoryId":"92","ListUrlMain":"https://pubs.acs.org/doi/10.1021/acsearthspacechem.3c00366","RegionNum":3,"RegionCategory":"化学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"CHEMISTRY, MULTIDISCIPLINARY","Score":null,"Total":0}
Molecular Diversity and Amino Acid Evolution in Simulated Carbonaceous Chondrite Parent Bodies
In interplanetary bodies, organics are found originating from various environments. We replicate the solid-phase conditions in a laboratory to elucidate the step-by-step evolution of organic matter, spanning from dense molecular cloud ices to processes occurring within meteorite parent bodies. The focus of our work is on amino acids, considered as potential chemical tracers of secondary alteration on asteroids. Using gas chromatography and high-resolution mass spectrometry, trace amounts of amino acids are identified in a preaccretional organic analogue formed from a dense molecular ice analogue. This analogue was subsequently exposed to aqueous alteration. This induced an increase in the formation of α- and β-amino acids over time. Supported by high-resolution mass spectrometry data, the reactions involved sugars and amine compounds, followed by amino acid destruction due to the Maillard reaction, which consumes both sugars and amino acids. Surprisingly, a second phase of amino acid formation, specifically α-amino acids, was observed, indicating the potential occurrence of the Strecker reaction. We demonstrate the intricate chemical network occurring within the presence of molecular diversity, similar to what might occur during parent body alteration. Therefore, investigations on reactivity within meteorite parent bodies have to take into account their molecular diversity, recognizing potential cross-reactions, as demonstrated in this work.
期刊介绍:
The scope of ACS Earth and Space Chemistry includes the application of analytical, experimental and theoretical chemistry to investigate research questions relevant to the Earth and Space. The journal encompasses the highly interdisciplinary nature of research in this area, while emphasizing chemistry and chemical research tools as the unifying theme. The journal publishes broadly in the domains of high- and low-temperature geochemistry, atmospheric chemistry, marine chemistry, planetary chemistry, astrochemistry, and analytical geochemistry. ACS Earth and Space Chemistry publishes Articles, Letters, Reviews, and Features to provide flexible formats to readily communicate all aspects of research in these fields.