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Synthesis of Cystine in Simulated Primitive Conditions

Abstract

IN an attempt to utilize the very abundant long wavelength ultraviolet solar radiation for prebiological organic chemistry, a series of experiments was performed in which H2S was introduced as the long wavelength photon acceptor. These experiments are described in detail elsewhere1, but in a typical experiment a spherical reaction vessel was filled with methane, ethane, ammonia, water vapour and H2S and the gases were irradiated in cylindrical geometry with the 2537 Å and/or 1849 Å resonance emission lines of mercury. The gases and their photolysis products were then circulated over a liquid water bath by a greaseless solenoid pump and returned to the reaction vessel (Fig. 1).

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KHARE, B., SAGAN, C. Synthesis of Cystine in Simulated Primitive Conditions. Nature 232, 577–579 (1971). https://doi.org/10.1038/232577a0

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