Isotope effects at the origin of life: Fingerprints of the Strecker synthesis

Geochimica et Cosmochimica Acta (in Press) Link to Article []
1Department of Geological Sciences, University of Colorado—Boulder, Boulder, CO, 80309 USA
2Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, 91125, USA
3Dantari, Inc, Westlake Villiage, CA, 91361, USA
4Dottikon Exlusive Synthesis AG, Dottikon, 5605, CH
5Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, 91125, USA
Copyright Elsevier

Strecker synthesis creates α–amino acids from prebiotically plausible substrates (cyanide, ammonia, and aldehydes) and is widely hypothesized to be a key mechanism in the chemistry that led to life on Earth and on other planets. To better constrain the synthetic environments and precursors of abiotic α–amino acids, and to determine unique signatures of abiogenic amino acids, we measured the molecular-averaged and site-specific carbon and nitrogen isotope effects for the Strecker synthesis of alanine. The reaction steps of the Strecker synthesis can be divided into two groups: an initial series of reversible amination and nitrile-addition reactions (‘equilibration’) and a second series of irreversible hydrolysis reactions (‘hydrolysis’). The equilibration of cyanide, acetaldehyde, and ammonia with the intermediate, α–aminopropionitrile (α-APN), has a measured 55.1 ‰ equilibrium nitrogen isotope effect between the 15N–rich amine nitrogen in α-aminopropionitrile and the 15N–poor ammonia and a 20.0 ‰ equilibrium carbon isotope effect between the 13C-poor C–2 site in α–aminopropionitrile and the 13C–rich carbonyl carbon in acetaldehyde. The first irreversible hydrolysis step is inferred to have an up to 10 ‰ normal carbon fractionation (i.e., faster for 12C, slower for 13C) for the whole molecule, but it also has one or more side reactions that deplete the reactive α-APN reservoir by up to 15 ‰. The second hydrolysis step has a 15.4 ‰ normal kinetic isotope effect on the amide (C–1) site of alaninamide, which becomes the carboxyl site of alanine. Other α–amino acids will likely experience similar nitrogen isotope fractionations between ammonia and their amine sites, and similar carbon isotope fractionations between the carbonyl carbon in reactant aldehydes or ketones and the intermediate α–aminonitrile, and between cyanide and the carboxyl site. Therefore, these isotope effects allow us to predict the carbon and nitrogen isotopic contents and intramolecular structures of α-amino acids formed by Strecker synthesis based on their substrates’ isotopic compositions, or to infer the isotopic compositions of substrates from which amino acids formed, for example in the case of the amino-acid-rich carbonaceous chondrites. The site-specific C and N isotopic compositions of amino acids formed by Strecker chemistry contrast with those typical of terrestrial biosynthetic amino acids, so these data also provide a means of discriminating between biogenic and abiogenic α–amino acids.


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