Carbonaceous chondrites are considered to be the most primitive meteorites that contain
some of the earliest formed solar system phases, eg, Ca‐Al‐rich inclusions and chondrules …

The textures of chondritic meteorites demonstrate that they are not the products of planetary
melting processes. This has long been interpreted as evidence that chondrite parent bodies …

Chondritic meteorites are unmelted and variably metamorphosed aggregates of the earliest
solids of the solar system. The variety of metamorphic textures in chondrites motivated the …

The textures and accretion ages of chondrites have been used to argue that their parent
asteroids never differentiated. Without a core, undifferentiated planetesimals could not have …

Meteorite magnetizations can provide rare insight into early Solar System evolution. Such
data take on new importance with recognition of the isotopic dichotomy between non …

Recent paleomagnetic studies of Allende CV chondrite as well as thermal modeling suggest
the existence of partially differentiated asteroids with outer unmelted and variably …

We present a paleomagnetic study of seven CM carbonaceous chondrites. CM chondrites
are believed to be some of the most chemically primitive materials available in our solar …

Abstract Early Solar System planetesimal thermal models predict the heating of the
chondritic protolith and the preservation of a chondritic crust on differentiated parent bodies …

Meteorites are samples of dozens of small planetary bodies that formed in the early Solar
System. They exhibit great petrologic diversity, ranging from primordial accretional …

Chondritic meteorites have been traditionally thought to be samples of undifferentiated
bodies that never experienced large-scale melting. This view has been challenged by the …