Mechanisms of Prebiotic Adenine Synthesis from HCN by Oligomerization in the Gas Phase

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초록

We explored the potential energy surfaces for adenine synthesis by oligomerizations of HCN or HNC from CBS-QB3 calculations. The pathways have been obtained for the formation of the covalently bound HCN dimer, trimer, tetramer, and pentamer (adenine) by sequential additions of HCN or HNC. The activation energies of the individual oligomerization stages are a few hundred kilojoules per mole, which prevent efficient adenine synthesis in interstellar space or in the atmosphere of Titan. On the other hand, when the oligomerizations start from HCNH+, the activation energies of sequential HCN or HNC additions are significantly reduced. Kinetic analyses results suggest that adenine synthesis by proton-catalyzed oligomerizations cannot occur efficiently in interstellar space or in the atmosphere of Titan, even though some oligomerization stages can occur under the latter condition.

키워드

Prebiotic chemistryAstrobiologyChemical evolutionTitanISM chemistryPOTENTIAL-ENERGY SURFACESDISSOCIATIVE RECOMBINATIONAMINO-ACIDSCHEMICAL EVOLUTIONAB-INITIOPURINE PRECURSORSHYDROGEN-CYANIDEATMOSPHERECHEMISTRYTHERMOSPHERE
제목
Mechanisms of Prebiotic Adenine Synthesis from HCN by Oligomerization in the Gas Phase
저자
Jung, Sun HwaChoe, Joong Chul
DOI
10.1089/ast.2013.0973
발행일
2013-05
유형
Article
저널명
Astrobiology
13
5
페이지
465 ~ 475