Literature DB >> 28791552

Mechanism for the Coupled Photochemistry of Ammonia and Acetylene: Implications for Giant Planets, Comets and Interstellar Organic Synthesis.

Thomas C Keane1.   

Abstract

Laboratory studies provide a fundamental understanding of photochemical processes in planetary atmospheres. Photochemical reactions taking place on giant planets like Jupiter and possibly comets and the interstellar medium are the subject of this research. Reaction pathways are proposed for the coupled photochemistry of NH3 (ammonia) and C2H2 (acetylene) within the context Jupiter's atmosphere. We then extend the discussion to the Great Red Spot, Extra-Solar Giant Planets, Comets and Interstellar Organic Synthesis. Reaction rates in the form of quantum yields were measured for the decomposition of reactants and the formation of products and stable intermediates: HCN (hydrogen cyanide), CH3CN (acetonitrile), CH3CH = N-N = CHCH3 (acetaldazine), CH3CH = N-NH2 (acetaldehyde hydrazone), C2H5NH2 (ethylamine), CH3NH2 (methylamine) and C2H4 (ethene) in the photolysis of NH3/C2H2 mixtures. Some of these compounds, formed in our investigation of pathways for HCN synthesis, were not encountered previously in observational, theoretical or laboratory photochemical studies. The quantum yields obtained allowed for the formulation of a reaction mechanism that attempts to explain the observed results under varying experimental conditions. In general, the results of this work are consistent with the initial observations of Ferris and Ishikawa (1988). However, their proposed reaction pathway which centers on the photolysis of CH3CH = N-N = CHCH3 does not explain all of the results obtained in this study. The formation of CH3CH = N-N = CHCH3 by a radical combination reaction of CH3CH = N• was shown in this work to be inconsistent with other experiments where the CH3CH = N• radical is thought to form but where no CH3CH = N-N = CHCH3 was detected. The importance of the role of H atom abstraction reactions was demonstrated and an alternative pathway for CH3CH = N-N = CHCH3 formation involving nucleophilic reaction between N2H4 and CH3CH = NH is advanced.

Entities:  

Keywords:  Acetylene; Ammonia; Atmosphere; Comets; ExtraSolar Giant planets; Great red spot (organic chromophores); HCN; Interstellar medium; Jupiter; Photochemistry

Mesh:

Substances:

Year:  2017        PMID: 28791552     DOI: 10.1007/s11084-017-9545-2

Source DB:  PubMed          Journal:  Orig Life Evol Biosph        ISSN: 0169-6149            Impact factor:   1.950


  21 in total

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Authors:  Julianne I Moses; Channon Visscher; Thomas C Keane; Aubrey Sperier
Journal:  Faraday Discuss       Date:  2010       Impact factor: 4.008

6.  The chemistry in circumstellar envelopes of evolved stars: following the origin of the elements to the origin of life.

Authors:  Lucy M Ziurys
Journal:  Proc Natl Acad Sci U S A       Date:  2006-08-07       Impact factor: 11.205

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Journal:  Adv Space Res       Date:  1995       Impact factor: 2.152

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Journal:  Planet Space Sci       Date:  1995 Jan-Feb       Impact factor: 2.030

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Journal:  Science       Date:  1990-07-27       Impact factor: 47.728

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