Peptide Bonds in the Interstellar Medium: Facile Catalytic Formation from Nitriles on Water-Ice Grains.

Boutheïna Kerkeni, John M Simmie
Author Information
  1. Boutheïna Kerkeni: ISAMM, Université de la Manouba, Tunisia 2010; Faculté des Sciences de Tunis, Laboratoire de Physique de la Matière Condensée, Université Tunis el Manar, Tunis 2092, Tunisia. ORCID
  2. John M Simmie: School of Chemistry, University of Galway Galway H91 TK33, Ireland. ORCID

Abstract

A recent suggestion that acetamide, CHC(O)NH, could be readily formed on water-ice grains by the acid induced addition of water across the C≡N bond has now been shown to be credible. Computational modeling of the reaction between R-CN (R = H, CH) and a cluster of 32 molecules of water and one HO proceeds catalytically to form first a hydroxy imine R-C(OH)═NH and second an amide R-C(O)NH. Quantum mechanical tunneling, computed from small-curvature estimates, plays a key role in the rates of these reactions. This work represents the first reasonable effort to show, in general, how amides can be formed from nitriles and water, which are abundant substrates, reacting on a water-ice cluster containing catalytic amounts of hydrons in the interstellar medium with consequential implications toward the origins of life.

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