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Cosmic ray synthesis of organic molecules in Titan's atmosphereThe possible synthesis of organic molecules by the absorption of galactic cosmic rays in an N2-CH4-H2 Titan model atmosphere has been studied. The cosmic-ray-induced ionization results in peak electron densities of 2000/cu cm, with NH(+), C3H9(+), and C4H9(+) being among the important positive ions. Details of the ion and neutral chemistry relevant to the production of organic molecules are discussed. The potential importance of N(2D) reactions with CH4 and H2 is also demonstrated. Although the integrated production rate of organic matter due to the absorption of the cosmic ray cascade is much less than that by solar ultraviolet radiation, the production of nitrogen-bearing organic molecules by cosmic rays may be greater.
Document ID
19810041857
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Capone, L. A.
(San Jose State University San Jose, Calif., United States)
Dubach, J.
(California, University Los Alamos Scientific Laboratory, Los Alamos, N. Mex., United States)
Whitten, R. C.
(NASA Ames Research Center Space Sciences Div., Moffett Field, Calif., United States)
Prasad, S. S.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Santhanam, K.
(Informatics, Inc. Palo Alto, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
October 1, 1980
Publication Information
Publication: Icarus
Volume: 44
Subject Category
Lunar And Planetary Exploration
Accession Number
81A26261
Funding Number(s)
CONTRACT_GRANT: NSG-2130
Distribution Limits
Public
Copyright
Other

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