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Astrobiology – the final frontier in chemical reaction dynamics

Published online by Cambridge University Press:  08 May 2002

Ralf I. Kaiser
Affiliation:
Department of Chemistry, University of York, York YO10 5DD, UK. e-mail: rik1@york.ac.uk
Nadia Balucani
Affiliation:
Dipartimento di Chimica, Università di Perugia, 06123 Perugia, Italy. e-mail: deneb@impact.dyn.unipg.it

Abstract

Crossed-beam experiments on the reactions of cyano CN(X2Σ+) and ethinyl C2H(X2Σ+) radicals with the unsaturated hydrocarbons acetylene, ethylene, methylacetylene allene and benzene have been carried out under single-collision conditions to investigate synthetic routes to form nitriles, polyynes and substituted allenes in hydrocarbon-rich atmospheres of planets and their moons. All reactions were found to proceed without an entrance barrier, to have exit barriers well below the energy of the reactant molecules and to be strongly exothermic. The predominant identification of the radical versus atomic hydrogen exchange channel makes these reactions compelling candidates for the formation of complex organic chemicals – precursors to biologically important amino acids – in Solar system environments and in the interstellar medium.

Type
Research Article
Copyright
© 2002 Cambridge University Press

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