Synthesis of organic compounds under conditions simulating the Jovian atmosphere

Details Synthesis of organic compounds under conditions simulating the Jovian atmosphere Synthesis of organic compounds under conditions simulating the Jovian atmosphere

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977dossr.236..245k&link_type=abstract

Akademiia Nauk SSSR, Doklady, vol. 236, Sept. 1, 1977, p. 245-248. In Russian.

Computer Science

Atmospheric Chemistry, Chemical Evolution, Electric Discharges, Jupiter Atmosphere, Organic Compounds, Ammonia, Atmospheric Electricity, Carbonyl Compounds, Clouds, Hydrogen, Methane

Scientific paper

Due to the presence of H2, CH4, and NH3, the Jovian atmosphere is of interest to the study of the evolution of carbon compounds on planets. The experiments described in the present paper were carried out to study the synthesis of organic compounds under the influence of electric discharges at the level of the Jovian water-ammonium clouds in the model proposed by Lewis (1969). Several classes of organic compounds are found to form under such conditions. Specifically, a substantial amount of carbon transforms to carbonyl compounds which, in a medium containing CN(-) and ammonium, yield amino acids and their derivatives.

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