Size‐frequency distributions of chondrules in CO3 chondrites
- 1 September 1989
- journal article
- Published by Wiley in Meteoritics
- Vol. 24 (3) , 179-189
- https://doi.org/10.1111/j.1945-5100.1989.tb00960.x
Abstract
Abstract— The size‐frequency distributions of chondrules in 11 CO3 chondrites were determined by petrographic analysis of thin sections. CO chondrites have the smallest chondrules of any major chondrite group. In order of decreasing chondrule size, chondrite groups can be arranged as CV ≥ LL > L > H ≥ CM ≥ EH > CO. Chondrule size varies significantly among different CO chondrites; there is a tendency for chondrules to increase in average size with increasing metamorphic grade of the whole‐rock. Different chondrule types in CO chondrites have distinct size‐frequency distributions: in order of decreasing chondrule size, BO > PO > PP > POP > RP = C. The large size of BO chondrules is problematic; however, PO chondrules are among the largest because ∼20% of them contain very coarse relict olivine grains that constitute 40–90 vol.% of the individual chondrules. PP chondrules may be larger than POP chondrules because some of them contain coarse relict pyroxene grains; a compound object consisting of a POP chondrule attached to a large relict pyroxene grain occurs in Lancé.The mean proportions of chondrule types in CO chondrites are estimated to be 69% POP, 18% PP, 8% PO, 2% BO, 2% RP, 1% C and <0.1% GOP. CO chondrites thus contain a smaller proportion of nonporphyritic chondrules than ordinary or EH chondrites, but a larger proportion than CV chondrites. Relative proportions of chondrule types vary with size interval: PO chondrules decrease fairly regularly in abundance with decreasing chondrule size, and RP chondrules appear to be most abundant in the smallest size intervals.Keywords
This publication has 40 references indexed in Scilit:
- ALH85085: a unique volatile-poor carbonaceous chondrite with possible implications for nebular fractionation processesEarth and Planetary Science Letters, 1988
- A New Component of the Mezö‐Madaras Breccia: A Microchondrule‐ and Carbon‐Bearing L‐Related ChondriteMeteoritics, 1988
- Chondrules in the Qingzhen type-3 enstatite chondrite: Possible precursor components and comparison to ordinary chondrite chondrulesGeochimica et Cosmochimica Acta, 1985
- Refractory precursor components of Semarkona chondrules and the fractionation of refractory elements among chondritesGeochimica et Cosmochimica Acta, 1983
- Evidence for primitive nebular components in chondrules from the Chainpur chondriteGeochimica et Cosmochimica Acta, 1982
- RELATIVE ABUNDANCES OF CHONDRULE PRIMARY TEXTURAL TYPES IN ORDINARY CHONDRITES AND THEIR BEARING ON CONDITIONS OF CHONDRULE FORMATIONMeteoritics, 1981
- Elemental abundances in chondrules from unequilibrated chondrites: Evidence for chondrule origin by melting of pre-existing materialsEarth and Planetary Science Letters, 1980
- Volatiles in chainpur chondrulesGeophysical Research Letters, 1979
- Accretion of the ordinary chondritesEarth and Planetary Science Letters, 1976
- Brazos River bar [Texas]; a study in the significance of grain size parametersJournal of Sedimentary Research, 1957