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

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 …

We present evidence for both early-and late-stage magnetic activity on the CV and L/LL
parent bodies respectively from chondrules in Vigarano and Bjurböle. Using micro-CT scans …

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 …

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 …

Magnetic fields in the solar nebula may have played a central role in mass and angular
momentum transport in the protosolar disk and facilitated the accretion of the first …

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

Paleomagnetic studies of meteorites have shown that the solar nebula was likely
magnetized and that many early planetary bodies generated dynamo magnetic fields in their …