Number of the records: 1  

HNCO-based synthesis of formamide in planetary atmospheres

  1. 1.
    SYSNO ASEP0495088
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleHNCO-based synthesis of formamide in planetary atmospheres
    Author(s) Ferus, Martin (UFCH-W) ORCID, RID
    Laitl, Vojtěch (UFCH-W) ORCID
    Knížek, Antonín (UFCH-W) ORCID, RID, SAI
    Kubelík, Petr (UFCH-W) RID, ORCID
    Šponer, Jiří (BFU-R) RID, ORCID
    Kára, J. (CZ)
    Šponer, Judit E. (BFU-R) RID, ORCID
    Lefloch, B. (FR)
    Cassone, Giuseppe (BFU-R) ORCID
    Civiš, Svatopluk (UFCH-W) RID, ORCID, SAI
    Number of authors10
    Article numberA150
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 616, SEP 5 2018 (2018)
    Number of pages11 s.
    Publication formOnline - E
    Languageeng - English
    CountryFR - France
    Keywordsnucleic-acid components ; ab-initio calculations ; high-energy chemistry ; prebiotic synthesis ; gas-phase ; interstellar formamide ; emission-spectroscopy ; nucleobase formation ; molecular-dynamics ; unified mechanism
    Subject RIVCF - Physical ; Theoretical Chemistry
    OECD categoryPhysical chemistry
    Subject RIV - cooperationJ. Heyrovsky Institute of Physical Chemistry - Physical ; Theoretical Chemistry
    R&D ProjectsGA17-05076S GA ČR - Czech Science Foundation (CSF)
    GA17-04844S GA ČR - Czech Science Foundation (CSF)
    Institutional supportBFU-R - RVO:68081707 ; UFCH-W - RVO:61388955
    UT WOS000444015000001
    DOI10.1051/0004-6361/201833003
    AnnotationTime-resolved Fourier transform infrared emission spectroscopy, Fourier transform absorption infrared spectroscopy, and high-resolution UV-ViS emission spectroscopy have been used to characterize the chemistry of isocyanic acid (HNCO) under glow discharge conditions in planetary atmospheres. HNCO mixtures (i.e., composed of di-hydrogen or ammonia) have been investigated in order to unveil the possible reaction pathways leading to the synthesis of the key prebiotic molecule formamide (HCONH2), upon planetary atmospheres containing isocyanic acid in presence of di-hydrogen and, separately, of ammonia. In addition, ab initio molecular dynamics simulations coupled with a modern metadynamics technique have been performed in order to identify the most likely chemical pathways connecting HNCO to formamide. It turned out that the direct hydrogenation of HNCO is thermodynamically favored. Incidentally, the experimental results supplied by a simplified kinetic model also proved the favorability of the reaction HNCO + H-2> HCONH2 which, moreover, spontaneously takes place in unbiased ab initio molecular dynamics simulations carried out under the effect of intense electric fields.
    WorkplaceInstitute of Biophysics
    ContactJana Poláková, polakova@ibp.cz, Tel.: 541 517 244
    Year of Publishing2019
Number of the records: 1  

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