Issue 16, 2012

On the formation of polyacetylenes and cyanopolyacetylenes in Titan's atmosphere and their role in astrobiology

Abstract

This tutorial review compiles recent experimental and theoretical studies on the formation of polyacetylenes (H(C[triple bond, length as m-dash]C)nH) and cyanopolyacetylenes (H(C[triple bond, length as m-dash]C)nCN) together with their methyl-substituted counterparts (CH3(C[triple bond, length as m-dash]C)nH, CH3(C[triple bond, length as m-dash]C)nCN) as probed under single collision conditions in crossed beam studies via the elementary reactions of ethynyl (CCH) and cyano radicals (CN) with unsaturated hydrocarbons. The role of these key reaction classes in the chemical evolution of Titan's orange-brownish haze layers is also discussed. We further comment on astrobiological implications of our findings with respect to proto-Earth and present a brief outlook on future research directions.

Graphical abstract: On the formation of polyacetylenes and cyanopolyacetylenes in Titan's atmosphere and their role in astrobiology

Article information

Article type
Tutorial Review
Submitted
07 Mar 2012
First published
28 Jun 2012

Chem. Soc. Rev., 2012,41, 5490-5501

On the formation of polyacetylenes and cyanopolyacetylenes in Titan's atmosphere and their role in astrobiology

R. I. Kaiser and A. M. Mebel, Chem. Soc. Rev., 2012, 41, 5490 DOI: 10.1039/C2CS35068H

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