NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Lunar meteorites - Siderophile element contents, and implications for the composition and origin of the moonData for 10 siderophile elements in all of the known lunar meteorites except for Y793274 are reported. Bulk compositional data for Ni, Ge, Cd, Re, Os, Ir, and Au were obtained from radiochemical neutron activation analysis (Warren et al., 1986). Data for Fe, Co, and Zn, and additional data for Ni, Ir, and Au were obtained by instrumental neutron activation analysis (Kallemeyn et al., 1988). Except for the case of Au in Y791197, there was good agreement between the results obtained by the two methods. The differences observed between the lunar-meteoritic regolith samples and central nearside highlands regolith samples are discussed.
Document ID
19890042931
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Warren, Paul H.
(California Univ. Los Angeles, CA, United States)
Jerde, Eric A.
(California Univ. Los Angeles, CA, United States)
Kallemeyn, Gregory W.
(California, University Los Angeles, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 91
Issue: 3-4
ISSN: 0012-821X
Subject Category
Lunar And Planetary Exploration
Accession Number
89A30302
Funding Number(s)
CONTRACT_GRANT: NAG9-87
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available