Isotopic homogeneity of iron in the early solar nebula

Abstract

The chemical and isotopic homogeneity of the early solar nebula, and the processes producing fractionation during its evolution, are central issues of cosmochemistry. Studies of the relative abundance variations of three or more isotopes of an element can in principle determine if the initial reservoir of material was a homogeneous mixture or if it… (More)
DOI: 10.1038/35085525

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