Introduction: Thermal and aqueous alteration are common occurrences in the lifetime of
carbonaceous chondrites. These alteration processes must be well understood in order to …

Carbonaceous chondrites experienced varying degrees of aqueous alteration on their
parent asteroids, which influenced their mineralogies, textures, and bulk chemical and …

Carbonaceous chondrites of the CM and CI families are among the most pristine samples
identified yet from the early Solar System. They contain up to~ 20 wt% water, in the form of …

Magnetic fields in the solar nebula may have played a key role in the radial transport of
angular momentum and mass during the early accretional phase of the solar system …

Constraints on the Ice Composition of Carbonaceous Chondrites - NASA/ADS Now on home
page ads icon ads Enable full ADS view NASA/ADS Constraints on the Ice Composition of …

Introduction: Magnetite is one of the first products formed in carbonaceous chondrites during
aqueous alteration, providing a valuable timeline for metamorphic changes on …

Bulk isotopic and elemental compositions of CV and CK chondrites have led to the
suggestion that both originate from the same asteroid. It has been argued that magnetite …

Thermomagnetic analysis was made on samples of all known C3 and C4 chondrites in a
controlled oxygen atmosphere. Considerable variation was noted in the occurrence of …

The study of the paleomagnetism of carbonaceous chondrites can lead to an estimate of the
magnetic fields present in the early solar system. CM chondrites contain abundant magnetite …

We present low temperature magnetic data (thermal demagnetization, hysteresis) obtained
on thirty three ordinary chondrite meteorites. A magnetic transition is observed in the 40–80 …