Oxygen isotopes of chondritic components

Hisayoshi Yurimoto, Alexander N. Krot, Byeon Gak Choi, Jerome Aléon, Takuya Kunihiro, Adrian J. Brearley

Research output: Contribution to journalArticle

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Abstract

We review the oxygen isotopic compositions of chondrite components (refractory inclusions, chondrules, and matrix) and their inter- and intra- crystalline oxygen isotopic distributions. Primary oxygen isotopic compositions, acquired before planetesimal accretion, are easily disturbed by parent-body processes such as aqueous alternation and thermal metamorphism. Primary or original oxygen isotopic compositions of refractory inclusions (Ca-, Al-rich inclusions and amoeboid olivine aggregates) distribute along a slope-1 line on the three-oxygen isotope diagram over the range of -60‰ <δ 17O ≈ δ18O <+10‰. The variations suggest that oxygen isotopic compositions of the solar nebular gas temporally and spatially varied between 16O-rich and 17O-, 18O-rich during refractory inclusion formation. On the other hand, primary minerals of most chondrules have small isotopic variations and are enriched in 17O and 18O relative to refractory inclusions, suggesting that chondrule formation occurred in 17O-, 18O-rich nebular gas. However, rare 16O-rich chondrules have been found, suggesting some overlap in the timing of formation of chondrules and refractory inclusions in the solar nebula. Oxygen isotopic compositions of matrix grains distribute along the slope-1 line over the same range as refractory inclusions and chondrules. The similarity in oxygen isotopic distributions suggests that matrix was originally a mechanical mixture of nebular dusts co-generated with chondrules and refractory inclusions. Presolar grains with oxygen isotopic compositions that are clearly distinct from those of solar nebular materials are a trace component of chondrite matrices. Based on these oxygen isotopic characteristics, more than 99.5% of the solid materials in the nebula formed locally in the solar nebula, and the remainder formed in interstellar space. The astrophysical setting of chondrite component formation in the early Solar System is also discussed. Refractory inclusions and 16O-rich matrix dusts formed around the inner edge of the solar nebula. On the other hand, most chondrules and 17O-, 18O-rich matrix dusts seem to have formed elsewhere in the solar nebula. Efficient, large-scale radial mixing of the solar nebular materials may have been an essential process in the formation of chondritic planetesimals.

Original languageEnglish
Pages (from-to)141-186
Number of pages46
JournalReviews in Mineralogy and Geochemistry
Volume68
DOIs
Publication statusPublished - 2008

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Oxygen Isotopes
chondrule
oxygen isotope
Refractory materials
Oxygen
oxygen
isotopic composition
matrix
Chemical analysis
chondrite
Dust
planetesimal
dust
Gases
Solar system
parent body
gas
solar system
Minerals
olivine

ASJC Scopus subject areas

  • Geochemistry and Petrology

Cite this

Yurimoto, H., Krot, A. N., Choi, B. G., Aléon, J., Kunihiro, T., & Brearley, A. J. (2008). Oxygen isotopes of chondritic components. Reviews in Mineralogy and Geochemistry, 68, 141-186. https://doi.org/10.2138/rmg.2008.68.8

Oxygen isotopes of chondritic components. / Yurimoto, Hisayoshi; Krot, Alexander N.; Choi, Byeon Gak; Aléon, Jerome; Kunihiro, Takuya; Brearley, Adrian J.

In: Reviews in Mineralogy and Geochemistry, Vol. 68, 2008, p. 141-186.

Research output: Contribution to journalArticle

Yurimoto, H, Krot, AN, Choi, BG, Aléon, J, Kunihiro, T & Brearley, AJ 2008, 'Oxygen isotopes of chondritic components', Reviews in Mineralogy and Geochemistry, vol. 68, pp. 141-186. https://doi.org/10.2138/rmg.2008.68.8
Yurimoto, Hisayoshi ; Krot, Alexander N. ; Choi, Byeon Gak ; Aléon, Jerome ; Kunihiro, Takuya ; Brearley, Adrian J. / Oxygen isotopes of chondritic components. In: Reviews in Mineralogy and Geochemistry. 2008 ; Vol. 68. pp. 141-186.
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