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HCN and chromophore formation on JupiterReaction paths for the formation of HCN and chromophores on Jupiter are suggested. The reactions involve photolysis of ammonia/acetylene mixtures. Experimental data supporting these pathways are reported.
Document ID
19870052392
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1038/326777a0
Authors
Ferris, James P. (Rensselaer Polytechnic Inst. Troy, NY, United States)
Ishikawa, Yoji (Rensselaer Polytechnic Institute, Troy, NY, United States)
Date Acquired
August 13, 2013
Publication Date
April 23, 1987
Publication Information
Publication: Nature
Volume: 326
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Accession Number
87A39666
Funding Number(s)
CONTRACT_GRANT: NAGW-476
Distribution Limits
Public
Copyright
Other

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