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Solar wind nitrogen - Mechanisms for isotopic evolutionIsotope systematics of nitrogen implanted in the lunar regolith indicate that the N-15/N-14 ratio at the source of the nitrogen has increased substantially with time. This source is most plausibly identified as the solar wind reservoir. However, rigorous testing of possible mechanisms for isotopic evolution of the solar convective zone shows that they all fail, by large factors, to explain the observed effect. Evolutionary processes on the lunar surface may be similarly eliminated, leaving the lunar nitrogen isotope anomaly currently unexplained.
Document ID
19780057858
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Kerridge, J. F.
(California Univ. Los Angeles, CA, United States)
Kaplan, I. R.
(California Univ. Los Angeles, CA, United States)
Lingenfelter, R. E.
(California Univ. Los Angeles, CA, United States)
Boynton, W. V.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 14, 1977
End Date: March 18, 1977
Accession Number
78A41767
Funding Number(s)
CONTRACT_GRANT: NGR-05-007-289
CONTRACT_GRANT: NSF AST-76-08178
CONTRACT_GRANT: NSG-7335
Distribution Limits
Public
Copyright
Other

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