Synthesis of Cystine in Simulated Primitive Conditions

Details Synthesis of Cystine in Simulated Primitive Conditions Synthesis of Cystine in Simulated Primitive Conditions

Aug 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971natur.232..577k&link_type=abstract

Nature, Volume 232, Issue 5312, pp. 577-579 (1971).

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8

Scientific paper

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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