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ABSTRACT Many amino acids contain an asymmetric centre, occurring as laevorotatory, L, or dextrorotatory, D, compounds. It is generally assumed that abiotic synthesis of amino acids on the
early Earth resulted in racemic mixtures (L- and D-enantiomers in equal abundance). But the origin of life required, owing to conformational constraints, the almost exclusive selection of
either L- or D-enantiomers1,2, and the question of why living systems on the Earth consist of L-enantiomers rather than D-enantiomers is unresolved3. A substantial fraction of the organic
compounds on the early Earth may have been derived from comet and meteorite impacts4,5,6. It has been reported previously that amino acids in the Murchison meteorite exhibit an excess of
L-enantiomers7, raising the possibility that a similar excess was present in the initial inventory of organic compounds on the Earth. The stable carbon isotope compositions of individual
amino acids in Murchison support an extraterrestrial origin8—rather than a terrestrial overprint of biological amino acids—although reservations have persisted (see, for example, ref. 9).
Here we show that individual amino-acid enantiomers from Murchison are enriched in 15N relative to their terrestrial counterparts, so confirming an extraterrestrial source for an
L-enantiomer excess in the Solar System that may predate the origin of life on the Earth. Access through your institution Buy or subscribe This is a preview of subscription content, access
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Log in * Learn about institutional subscriptions * Read our FAQs * Contact customer support SIMILAR CONTENT BEING VIEWED BY OTHERS ABUNDANT AMMONIA AND NITROGEN-RICH SOLUBLE ORGANIC MATTER
IN SAMPLES FROM ASTEROID (101955) BENNU Article Open access 29 January 2025 INSIGHTS INTO THE FORMATION AND EVOLUTION OF EXTRATERRESTRIAL AMINO ACIDS FROM THE ASTEROID RYUGU Article Open
access 17 March 2023 PRIMORDIAL AQUEOUS ALTERATION RECORDED IN WATER-SOLUBLE ORGANIC MOLECULES FROM THE CARBONACEOUS ASTEROID (162173) RYUGU Article Open access 10 July 2024 REFERENCES *
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Press, Tucson, (1992). Download references ACKNOWLEDGEMENTS We thank S. Fulkerson for his support of this work, and V. Andrusevich and T.Brockwell for their assistance with the analyses.
This work was supported by the US NSF. Instrument time and travel funds were provided by Micromass Inc. AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * School of Geology and Geophysics, The
University of Oklahoma, Norman, 73019, Oklahoma, USA M. H. Engel * Department of Environmental Sciences, University of Virginia, Charlottesville, 22903, Virginia, USA S. A. Macko Authors *
M. H. Engel View author publications You can also search for this author inPubMed Google Scholar * S. A. Macko View author publications You can also search for this author inPubMed Google
Scholar CORRESPONDING AUTHOR Correspondence to M. H. Engel. RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Engel, M., Macko, S. Isotopic evidence for
extraterrestrial non- racemic amino acids in the Murchison meteorite. _Nature_ 389, 265–268 (1997). https://doi.org/10.1038/38460 Download citation * Received: 17 September 1996 * Accepted:
14 July 1997 * Issue Date: 18 September 1997 * DOI: https://doi.org/10.1038/38460 SHARE THIS ARTICLE Anyone you share the following link with will be able to read this content: Get shareable
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