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 …

One key feature of our protoplanetary disk that shaped its transformation into a system of
planetary bodies was its vast magnetic field. Unique constraints on the properties of this field …

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 …

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 …

Remanent magnetization of carbonaceous chondrite meteorites apparently reflects the
presence of a strong magnetic field during the formation of the solar system. This remanence …

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 …

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 …

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

Astronomical observations and isotopic measurements of meteorites suggest that
substructures are common in protoplanetary disks and may even have existed in the solar …