Racemic amino acids from the ultraviolet photolysis of interstellar ice analogues

Max P. Bernstein (), Jason P. Dworkin, Scott A. Sandford, George W. Cooper and Louis J. Allamandola
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Max P. Bernstein: The Center for the Study of Life in the Universe, SETI Institute
Jason P. Dworkin: The Center for the Study of Life in the Universe, SETI Institute
Scott A. Sandford: NASA-Ames Research Center
George W. Cooper: NASA-Ames Research Center
Louis J. Allamandola: NASA-Ames Research Center

Nature, 2002, vol. 416, issue 6879, 401-403

Abstract: Abstract The delivery of extraterrestrial organic molecules to Earth by meteorites may have been important for the origin and early evolution of life1. Indigenous amino acids have been found in meteorites2—over 70 in the Murchison meteorite alone3. Although it has been generally accepted that the meteoritic amino acids formed in liquid water4 on a parent body, the water in the Murchison meteorite is depleted in deuterium5 relative to the indigenous organic acids6,7. Moreover, the meteoritical evidence8 for an excess of laevo-rotatory amino acids is hard to understand in the context of liquid-water reactions on meteorite parent bodies. Here we report a laboratory demonstration that glycine, alanine and serine naturally form from ultraviolet photolysis of the analogues of icy interstellar grains. Such amino acids would naturally have a deuterium excess similar to that seen in interstellar molecular clouds, and the formation process could also result in enantiomeric excesses if the incident radiation is circularly polarized. These results suggest that at least some meteoritic amino acids are the result of interstellar photochemistry, rather than formation in liquid water on an early Solar System body.

Date: 2002
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DOI: 10.1038/416401a

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