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在泰坦大气中聚乙炔和氰基聚乙炔的形成及其在天体生物学中的作用。

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

机构信息

Department of Chemistry, University of Hawaii at Manoa, Honolulu, HI 96822, USA.

出版信息

Chem Soc Rev. 2012 Aug 21;41(16):5490-501. doi: 10.1039/c2cs35068h. Epub 2012 Jun 28.

Abstract

This tutorial review compiles recent experimental and theoretical studies on the formation of polyacetylenes (H(C≡C)(n)H) and cyanopolyacetylenes (H(C≡C)(n)CN) together with their methyl-substituted counterparts (CH(3)(C≡C)(n)H, CH(3)(C≡C)(n)CN) 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.

摘要

本教程综述汇集了最近关于聚乙炔(H(C≡C)(n)H)和氰基聚乙炔(H(C≡C)(n)CN)以及它们的甲基取代物(CH(3)(C≡C)(n)H、CH(3)(C≡C)(n)CN)在交叉束研究中单分子碰撞条件下通过乙炔基(CCH)和氰基自由基(CN)与不饱和烃的基本反应形成的实验和理论研究。还讨论了这些关键反应类在泰坦橙棕色霾层化学演化中的作用。我们进一步就我们的发现对原地球的天体生物学意义发表评论,并对未来的研究方向进行简要展望。

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