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

Protein and non-protein amino acids were synthesized following hydrolysis of products obtained by high frequency discharge techniques applied to model atmospheres consisting of N₂ as a nitrogen source together with CH₄ and/or CO₂ as a carbon source. Highest yields were obtained in the absence of CO₂ and from mixtures rich in CH₄. Amino acids would indeed be expected on the frozen surface of Titan with its CH₄–N₂ atmosphere.Paper presented at the 6th College Park Colloquium, October 1981.