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

TL;DR

This study combines oxygen, titanium, and chromium isotope data from individual chondrules to reveal fundamental isotopic differences between non-carbonaceous and carbonaceous chondrites, challenging the idea of disk-wide chondrule transport.

Contribution

First combined multi-isotope analysis of individual chondrules, demonstrating local heterogeneities and challenging previous transport models in the solar accretion disk.

Findings

NC chondrules are isotopically homogeneous and similar to their host chondrites.

CC chondrules show greater isotopic variability and do not overlap with NC chondrules in multi-isotope space.

Isotopic differences suggest local heterogeneities rather than disk-wide transport.

Abstract

Isotopic anomalies in chondrules hold important clues about the dynamics of mixing and transport processes in the solar accretion disk. These anomalies have been interpreted to indicate either disk-wide transport of chondrules or local heterogeneities of chondrule precursors. However, all previous studies relied on isotopic data for a single element (either Cr, Ti, or O), which does not allow distinguishing between source and precursor signatures as the cause of the chondrules isotope anomalies. Here we obtained the first combined O, Ti, and Cr isotope data for individual chondrules from enstatite, ordinary, and carbonaceous chondrites. We find that chondrules from non-carbonaceous (NC) chondrites have relatively homogeneous {\Delta}17O, {\epsilon}50Ti, and {\epsilon}54Cr, which are similar to the compositions of their host chondrites. By contrast, chondrules from carbonaceous chondrites (CC) have more variable compositions. Although the compositions of the analyzed CC and NC chondrules may overlap for either {\epsilon}50Ti, {\epsilon}54Cr, or {\Delta}17O, in multi-isotope space none of the CC chondrules plot in the compositional field of NC chondrites, and no NC chondrule plots within the field of CC chondrites. As such, our data reveal a fundamental isotopic difference between NC and CC chondrules, which is inconsistent with a disk-wide transport of chondrules across and between the NC and CC reservoirs. Instead, the isotopic variations among CC chondrules reflect local precursor heterogeneities, which most likely result from mixing between NC-like dust and a chemically diverse dust component that was isotopically similar to CAIs and AOAs.The same mixing processes, but on a larger, disk-wide scale, were likely responsible for establishing the distinct isotopic compositions of the NC and CC reservoirs, which represent in inner and outer disk, respectively.