Replication Data for: Early evolution of the solar accretion disk inferred from Cr-Ti-O isotopes in individual chondrules

Highlights • First combined Cr, Ti, O isotope data for individual chondrules. • Isotopic compositions of NC chondrules distinct from CC chondrules. • Isotopic variability not due to chondrule transport, but precursor heterogeneity. • Incomplete mixing of NC-like and CAI-like nebular components in the disk at all scales.