Abstract
We report trace element concentrations of silicate phases in chondrules from LL3 ordinary chondrites Bishunpur and Semarkona. Results are similar to previously reported data for carbonaceous chondrites, with rare earth element (REE) concentrations increasing in the sequence olivine. ~10. K/h) than type I chondrules. Appreciable Na concentrations (3-221. ppm) are measured in olivine from both chondrule types; type II chondrules seem to have behaved as closed systems, which may require chondrule formation in the vicinity of protoplanets or planetesimals. At any rate, higher solid concentrations in type II chondrule forming regions may explain the higher oxygen fugacities they record compared to type I chondrules. Type I and type II chondrules formed in different environments and the correlation between high solid concentrations and/or oxygen fugacities with rapid cooling rates is a key constraint that chondrule formation models must account for.
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CITATION STYLE
Jacquet, E., Alard, O., & Gounelle, M. (2015). Trace element geochemistry of ordinary chondrite chondrules: The type I/type II chondrule dichotomy. Geochimica et Cosmochimica Acta, 155, 47–67. https://doi.org/10.1016/j.gca.2015.02.005
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