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Rare gas studies in Luna 16-G-7 fines by stepwise heating technique - A low fission solar wind Xe.Examination of He, Ne, Kr, and Xe in a dust sample (equal to or less than 125 micrometer) of Luna 16 in 12 temperature steps with especially small intervals in the low temperature range (80 C steps). The gas concentrations, as well as their relative abundances, are in general agreement with values reported by Vinogradov (1971) for Luna 16 and values found in Apollo 11 fines except for Ne. Comparison is made with various other experimental results. The solar wind Xe was lower in the fission-affected isotopes than was found in Apollo 11 fines and in the 1000 C fraction of the Pesyanoe meteorite as measured by Marti (1969). Air-Xe is interpreted as a fractional solar wind Xe with the composition found in this study.
Document ID
19720038600
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kaiser, W. A.
(California, University Berkeley, Calif., United States)
Date Acquired
August 6, 2013
Publication Date
January 1, 1972
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 13
Subject Category
Space Sciences
Accession Number
72A22266
Funding Number(s)
CONTRACT_GRANT: NGL-05-003-409
Distribution Limits
Public
Copyright
Other

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