This work extends our previous experimental studies of the chemistry of Titan's atmosphere by atmospheric glow discharge. The Titan's atmosphere seems to be similarly to early Earth atmospheric composition. The exploration of Titan atmosphere was initiated by the exciting results of the Cassini-Huygens mission and obtained results increased the interest about prebiotic atmospheres. Present work is devoted to the role of CO2 in the prebiotic atmosphere chemistry. Most of the laboratory studies of such atmosphere were focused on the chemistry of N2 + CH4 mixtures. The present work is devoted to the study of the oxygenated volatile species in prebiotic atmosphere, specifically CO2 reactivity. CO2 was introduced to the standard N2 + CH4 mixture at different mixing ratio up to 5 % CH4 and 3 % CO2. The reaction products were characterized by FTIR spectroscopy. This work shows that CO2 modifies the composition of the gas phase with the detection of oxygenated compounds: CO and others oxides. There is a strong influence of CO2 on increasing concentration other products as cyanide (HCN) and ammonia (NH3).

Department of Experimental Physics Comenius University Mlynska dolina F 2 842 48 Bratislava Slovakia

Department of Physics and Astronomy Open University Walton Hall Milton Keynes MK7 6AA UK

Faculty of Chemistry Brno University of Technology Purkynova 119 612 00 Brno Czech Republic

Faculty of Chemistry Brno University of Technology Purkynova 119 612 00 Brno Czech Republic Department of Physics and Astronomy Open University Walton Hall Milton Keynes MK7 6AA UK

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