Abstract Protein and non-protein amino acids were synthesized following hydrolysis of products obtained by high frequency discharge techniques applied to model atmospheres consisting of $ N_{2} $ as a nitrogen source together with $ CH_{4} $ and/or $ CO_{2} $ as a carbon source. Highest yields were obtained in the absence of $ CO_{2} $ and from mixtures rich in $ CH_{4} $. Amino acids would indeed be expected on the frozen surface of Titan with its $ CH_{4} $−$ N_{2} $ atmosphere.


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    Titel :

    Formation of amino acids from models of Titan and more oxidized atmospheres


    Beteiligte:
    Ishigami, Masahiro (Autor:in) / Kinjo, Masataka (Autor:in) / Nagano, Kei (Autor:in) / Hattori, Yuko (Autor:in)

    Erschienen in:

    Origins of life ; 12 , 3 ; 307-310


    Erscheinungsdatum :

    1982




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Print


    Sprache :

    Englisch



    Klassifikation :

    BKL:    44.71 Verkehrsmedizin
    Lokalklassifikation TIB:    535/3908/4290



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