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Modeling of lunar basalt petrogenesis - Sr isotope evidence from Apollo 14 high-alumina basaltsThis paper reexamines the Sr isotope data available for the Apollo 14 high-alumina basalts in light of the assimilation and fractional crystallization (AFC) process model proposed by Neal et al. (1987, 1988, 1989). Positive linear correlations of Sr-87/Sr-86 with Rb-87/Rb-86 and the Sr abundance (both leading to KREEP) are used as evidence of such an AFC process in the petrogenesis of Apollo 14 high-alumina basalts. The existing Sr isotope data for Apollo 14 high-alumina basalts suggest that there were three AFC cycles.
Document ID
19900046409
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Neal, C. R.
(Tennessee Univ. Knoxville, TN, United States)
Taylor, L. A.
(Tennessee, University Knoxville, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Country: United States
Start Date: March 13, 1989
End Date: March 17, 1989
Accession Number
90A33464
Funding Number(s)
CONTRACT_GRANT: NAG9-62
Distribution Limits
Public
Copyright
Other

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