Racemization Mechanisms and Chemistry of D-Amino Acids
Photolysis of rac-Leucine with Circularly Polarized Synchrotron Radiation
Article first published online: 16 JUN 2010
DOI: 10.1002/cbdv.200900311
Copyright © 2010 Verlag Helvetica Chimica Acta AG, Zürich
Issue
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Chemistry & Biodiversity
Special Issue: D-Amino Acid Research in Chemistry, Life Sciences, and Biotechnology
Volume 7, Issue 6, pages 1651–1659, June 2010
Additional Information
How to Cite
Meierhenrich, U., Filippi, J.-J., Meinert, C., Hoffmann, S., Bredehöft, J. and Nahon, L. (2010), Photolysis of rac-Leucine with Circularly Polarized Synchrotron Radiation. Chemistry & Biodiversity, 7: 1651–1659. doi: 10.1002/cbdv.200900311
Publication History
- Issue published online: 16 JUN 2010
- Article first published online: 16 JUN 2010
- Abstract
- References
- Cited By
Keywords:
- D-Amino acids;
- Photolysis;
- Circularly polarized synchrotron radiation;
- Synchrotron radiation;
- Origin of life;
- Origin of biomolecular homochirality
Abstract
Amino acids that pass the RNA machinery in living organisms occur in L-configuration. The question on the evolutionary origin of this biomolecular asymmetry remains unanswered to this day. Amino acids were detected in artificially produced interstellar ices, and L-enantiomer-enriched amino acids were identified in CM-type meteorites. This hints at a possible interstellar/circumstellar origin of the amino acids themselves as well as their stereochemical asymmetry. Based upon the current knowledge about the occurrence of circularly-polarized electromagnetic radiation in interstellar environments, we subjected rac-leucine to far-UV circularly-polarized synchrotron radiation. Asymmetric photolysis was followed by an analysis in an enantioselective GC/MS system. Here, we report on an advanced photolysis rate of more than 99% for leucine. The results indicate that high photolysis rates can occur under the chosen conditions, favoring enantioselective photolysis. In 2014, the obtained results will be reexamined by cometary mission Rosetta.

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