Initial Cr-Isotopic and Iridium Measurements of Concentrates from Late Eocene Cpx-Spherule Deposits

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Scientific paper

Cr-isotopic compositions of separates from Late Eocene cpx-spherule
deposits show that most of the Cr is meteoritic. C- and E- chondrites
are ruled out as a source and ordinary chondrites are favored.
Implications for solar system history follow.

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