The identification of group II inclusions in carbonaceous chondrites by electron probe microanalysis of perovskite

Details The identification of group II inclusions in carbonaceous chondrites by electron probe microanalysis of perovskite The identification of group II inclusions in carbonaceous chondrites by electron probe microanalysis of perovskite

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985e%26psl..72...74k&link_type=abstract

Earth and Planetary Science Letters (ISSN 0012-821X), vol. 72, no. 1, Jan. 1985, p. 74-86.

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Carbonaceous Chondrites, Inclusions, Meteoritic Microstructures, Microanalysis, Perovskites, Abundance, Allende Meteorite, Aluminum, Calcium, Electron Probes, Meteorites, Carbonaceous Chondrites, Inclusions, Electron Microprobe, Analysis, Perovskite, Cais, Calcium, Aluminum, Refractory Elements, Lithophiles, Trace Elements, Depletion, Chemistry, Fractionation, Element Ratios, Anomalies, Epma, Titanium, Samples, Meteorite, Allende, Yttrium, Zirconium, Enrichment, Composition, Techniques, Patterns, Abundance,

Scientific paper

The technique developed by Kornacki (1984) for identifying group II Ca/Al-rich inclusions in carbonaceous chondrites by electron-microprobe analysis of the ZrO2 or Y2O3 content of their perovskite component is demonstrated using material from 20 Allende inclusions. The results are presented in tables and graphs and compared with findings obtained by other procedures. Group II inclusions are found to have perovskites generally containing less than 0.10 wt pct ZrO2 and/or Y2O3 (average of several grains), while those of groups I, III, V, and VI have more than 0.25 wt pct ZrO2. Analysis of data on eight Allende Ca/Al-rich inclusions shows that 75 percent of the fine-grained inclusions belong to group II. The implications of these findings for fractionation processes in the primitive solar nebula are indicated.

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