Several chondritic meteorites contain magnetizations that have been attributed to either
solar nebula fields or to core dynamos that may have operated within partially differentiated …

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 solar nebula carried a strong magnetic field that had a stable intensity and direction for
periods of a thousand years or more1. The solar nebular field may have produced post …

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 …

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 …

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 …

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

The origin of magnetization in Allende may have significant implications for our
understanding of core formation/differentiation/dynamo processes in chondrite parent …

More Evidence for a Partially Differentiated CV Parent Body from the Meteorite Kaba - NASA/ADS
Now on home page ads icon ads Enable full ADS view NASA/ADS More Evidence for a …

Meteorites represent the earliest records of the evolution of the solar system, providing
information on the conditions, processes and chronology for formation of first solids …