¹Zachary A. Torrano,¹Conel M.O’D. Alexander,¹Richard W. Carlson,²Jan Render,²Gregory A. Brennecka,¹Emma S. Bullock
Earth and Planetary Science Letters 627, Link to Article [https://doi.org/10.1016/j.epsl.2023.118551]
¹Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, United States
²Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore, CA, United States
Copyright Elsevier

Amoeboid olivine aggregates (AOAs) are the most abundant type of refractory inclusions found in most carbonaceous chondrite groups. AOAs are thought to be genetically related to calcium-aluminum-rich inclusions (CAIs) and potential chondrule precursor components, although the precise physical and temporal details of AOA formation and their relationship to other chondritic components remain unclear. In this study, we measured the chromium and titanium isotopic compositions of eight AOAs from four different CV chondrites with the goal of evaluating potential genetic links between AOAs, CAIs, and chondrules. These are the first Cr and Ti isotopic data reported beyond a single AOA previously measured for Cr and a different single AOA previously measured for Ti. The results presented here show that the ε54Cr and ε50Ti isotopic compositions of AOAs are indistinguishable from those of CAIs, suggesting that AOAs and CAIs formed from a common region of the disk. We also demonstrate, based on the comparison of the Cr and Ti isotopic composition of AOAs to previously measured chondrules, that mixing between AOAs and an NC compositional endmember alone cannot fully explain the range of measured chondrule compositions. Although AOAs may have been important chondrule precursor components along with AOA olivine, CAIs, fragments of earlier generation chondrules, and fine-grained matrix material, this observation requires another currently unknown component to be involved in chondrule formation.