Chondrules are igneous spherical objects preserved in chondritic meteorites and believed
to have formed during transient heating events in the solar protoplanetary disk. Chondrules …

We report on the petrology, magnesium isotopes and mass-independent 54 Cr/52 Cr
compositions (μ 54 Cr) of 42 chondrules from CV (Vigarano and NWA 3118) and CR (NWA …

Chondrules are the major high-temperature components of chondritic meteorites, which are
conventionally viewed as the samples from the very first generation of undifferentiated …

The magnesium isotopic composition of Calcium-, Aluminium-rich Inclusions (CAIs) and
chondrules from the CBb chondrites HH237 and QUE94411 was measured using MC …

The CB chondrites are metal‐rich meteorites with characteristics that sharply distinguish
them from other chondrite groups. Their unusual chemical and petrologic features and a …

Planetary bodies a few hundred kilometers in radii are the precursors to larger planets but it
is unclear whether these bodies themselves formed very rapidly or accreted slowly over …

Understanding the genetic relationship between different chondritic components will help to
decipher their origin and dynamical evolution within the protoplanetary disk. Here, we obtain …

Chondrite meteorites are samples of primitive asteroidal bodies that have escaped melting
and differentiation. The only record of our Solar System's formative stages comes from the …

By investigating the petrology and chemical composition of type II (FeO-rich) chondrules in
the Mighei-like carbonaceous (CM) chondrites we constrain their thermal histories and …

Chondrites are undifferentiated meteorites that can provide information on the compositions
of materials in the early solar System, including the building blocks of the terrestrial planets …