Isotopic anomalies in chondrules hold important clues about the dynamics of mixing and
transport processes in the solar accretion disk. The meaning of these anomalies is debated …

Understanding the relationships between and among chondritic components of various
chondrite groups is of prime importance for deciphering the dynamics of material transport …

Among primitive meteorites, CR chondrites have peculiar isotopic compositions, the origin of
which is uncertain and may have involved contributions from primordial molecular cloud …

Chondrules are the main components of primitive meteorites and possibly the building
blocks of planetary embryos and terrestrial planets. However, their ages and modes of …

Determining the origins of chondrule precursors is key to constraining how material migrated
in the early Solar System. Chondrules that were only partially melted during their formation …

Chondrules are major components of chondrites and are believed to drive the accretion of
planetary embryos. As such, constraining the timing and origin of chondrules is central for …

The systematic isotopic difference between refractory inclusions and chondrules, particularly
for oxygen, has long indicated an isotopic evolution of the solar protoplanetary disk …

Chondrules from different chondrite groups show characteristic properties, including
abundances of different chondrule textural types, chondrule sizes, oxygen isotope …

Deciphering the spatial and temporal evolution of chondrules allows for a better
understanding of how asteroidal seeds formed, migrated, and eventually accreted into …

We review the 26Al ages of chondrules in various type 3.0 chondrites. The 26Al ages of
chondrules are 1–3 Myr after calcium‐aluminum‐rich inclusion (CAI) for LL3. 0, CO3. 0, and …