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Alkali (Rb/K) abundances in Allende barred‐olivine chondrules: Implications for the melting conditions of chondrules
Author(s) -
Matsuda Hitoshi,
Nakamura Noboru,
Noda Shinji
Publication year - 1990
Publication title -
meteoritics
Language(s) - English
Resource type - Journals
eISSN - 1945-5100
pISSN - 0026-1114
DOI - 10.1111/j.1945-5100.1990.tb00985.x
Subject(s) - chondrule , allende meteorite , chondrite , olivine , porphyritic , alkali metal , meteorite , geology , parent body , mineralogy , astrobiology , geochemistry , chemistry , physics , quartz , paleontology , organic chemistry
— In order to study abundances of alkali metals in chondrules, 25 petrographically characterized chondrules, including 18 barred olivine (BO) chondrules from the Allende (CV3) meteorite, were analyzed for alkalis (K and Rb) and alkaline earths (Sr, Ba, Ca and Mg) by mass spectrometric isotope dilution. Most BO chondrules with higher alkalis (>CI level) have nearly CI‐chondritic Rb/K ratios, while those with lower alkalis clearly show higher Rb/K ratios than the CI‐chondritic. In general, BO chondrules with higher Rb/K exhibit more depletion of alkalis relative to Ca. The mean olivine Fa for individual chondrules positively correlates with bulk alkali concentrations in BO type but not in porphyritic type chondrules. These observations suggest that some BO chondrules formed from more reducing assemblages of precursor minerals, which experienced more intensive vaporization losses of alkalis, accompanied by Rb/K fractionation, during the chondrule‐formation melting.