- The origin of methane and biomolecules from a CO.sub.2./sub. cycle on…
Počet záznamů: 1  

The origin of methane and biomolecules from a CO.sub.2./sub. cycle on terrestrial planets

  1. 1.
    SYSNO ASEP0488421
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleThe origin of methane and biomolecules from a CO2 cycle on terrestrial planets
    Author(s) Civiš, S. (CZ)
    Knížek, A. (CZ)
    Ivanek, O. (CZ)
    Kubelík, Petr (FZU-D) RID, ORCID
    Zukalova, M. (CZ)
    Kavan, L. (CZ)
    Ferus, M. (CZ)
    Number of authors7
    Source TitleNature Astronomy. - : Nature Publishing Group - ISSN 2397-3366
    Roč. 1, č. 10 (2017), s. 721-726
    Number of pages6 s.
    Languageeng - English
    CountryUS - United States
    Keywordshigh-energy chemistry ; nucleobase formation ; martian atmosphere ; carbon-dioxide ; early earth ; Mars ; formamide ; surfaces ; exchange ; TiO2
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    R&D ProjectsLG15013 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Institutional supportFZU-D - RVO:68378271
    UT WOS000415270100010
    EID SCOPUS85037145417
    DOI https://doi.org/10.1038/s41550-017-0260-8
    AnnotationIn this study, an original scenario for the origin of methane on Mars and terrestrial planets is suggested. Carbon dioxide in Martian and other planetary atmospheres can be abiotically converted into a mixture of methane and carbon monoxide by ‘methanogenesis’ on porous mineral photoactive surfaces under soft ultraviolet irradiation. On young planets exposed to heavy bombardment by interplanetary matter, this process can be followed by biomolecule synthesis through the reprocessing of reactive reducing atmospheres by impact-induced shock waves. The proposed mechanism of methanogenesis may help to answer the question concerning the formation of methane and carbon monoxide by photochemical processes, the formation of biomolecules on early Earth and other terrestrial planets, and the source and seasonal variation of methane concentrations on Mars.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2018
Počet záznamů: 1  

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