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Low-temperature formation of pyridine and (iso)quinoline via neutral-neutral reactions
Yang, Zhenghai1; He, Chao1; Goettl, Shane J.1; Mebel, Alexander M.2; Velloso, Paulo F. G.3; Alves, Marcio O.3; Galvao, Breno R. L.3; Loison, Jean-Christophe4; Hickson, Kevin M.4; Dobrijevic, Michel5; Li, Xiaohu6,7; Kaiser, Ralf I.1
2024-05-13
Source PublicationNATURE ASTRONOMY
ISSN2397-3366
Pages13
Contribution Rank6
AbstractAromatic molecules represent fundamental building blocks in prebiotic chemistry and are contemplated as vital precursors to DNA and RNA nitrogen bases. However, despite the identification of some 300 molecules in extraterrestrial environments, the pathways to pyridine (C5H5N), pyridinyl (C5H4N) and (iso)quinoline (C9H7N)-the simplest representative mono- and bicyclic aromatic molecules carrying nitrogen-are elusive. Here we afford compelling evidence on the gas-phase formation of methylene amidogen (H2CN) and cyanomethyl (H2CCN) radicals via molecular beam studies and electronic structure calculations. The modelling of the chemistries of the Taurus molecular cloud (TMC-1) and Titan's atmosphere contemplates a complex chain of reactions synthesizing pyridine, pyridinyl and (iso)quinoline from H2CN and H2CCN at levels of up to 75%. This study affords unique entry points to precursors of DNA and RNA nitrogen bases in hydrocarbon-rich extraterrestrial environments thus changing the way we think about the origin of prebiotic molecules in our Galaxy. A pathway towards the formation of pyridine and (iso)quinoline, precursors to DNA and RNA, is revealed for conditions appropriate to Saturn's moon Titan and the Taurus molecular cloud, providing insight into the synthesis of prebiotic molecules in space.
DOI10.1038/s41550-024-02267-y
Indexed BySCI
Language英语
WOS KeywordPOLYCYCLIC AROMATIC-HYDROCARBONS ; ATMOSPHERE ; CHEMISTRY ; BENZENE ; TITAN ; IDENTIFICATION ; NUCLEOBASES ; MOLECULES ; DENSITY ; ATOMS
Funding ProjectUS Department of Energy, Basic Energy Sciences[DE-FG02-03ER15411] ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)[311508/2021-9] ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)[405524/2021-8]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001220931600001
PublisherNATURE PORTFOLIO
Funding OrganizationUS Department of Energy, Basic Energy Sciences ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6715
Collection射电天文研究室_天体化学研究团组
Corresponding AuthorMebel, Alexander M.; Galvao, Breno R. L.; Loison, Jean-Christophe; Li, Xiaohu; Kaiser, Ralf I.
Affiliation1.Univ Hawaii Manoa, Dept Chem, Honolulu, HI 96822 USA
2.Florida Int Univ, Dept Chem & Biochem, Miami, FL 33199 USA
3.Ctr Fed Educ Tecnol Minas Gerais, CEFET MG, Belo Horizonte, Brazil
4.Univ Bordeaux, Inst Sci Mol, CNRS, Talence, France
5.Univ Bordeaux, Lab Astrophys Bordeaux, CNRS, Pessac, France
6.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
7.Chinese Acad Sci, Key Lab Radio Astron, Urumqi, Peoples R China
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Yang, Zhenghai,He, Chao,Goettl, Shane J.,et al. Low-temperature formation of pyridine and (iso)quinoline via neutral-neutral reactions[J]. NATURE ASTRONOMY,2024:13.
APA Yang, Zhenghai.,He, Chao.,Goettl, Shane J..,Mebel, Alexander M..,Velloso, Paulo F. G..,...&Kaiser, Ralf I..(2024).Low-temperature formation of pyridine and (iso)quinoline via neutral-neutral reactions.NATURE ASTRONOMY,13.
MLA Yang, Zhenghai,et al."Low-temperature formation of pyridine and (iso)quinoline via neutral-neutral reactions".NATURE ASTRONOMY (2024):13.
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