Evidence for Non-steady Accretion in the Solar Nebula Inferred from Paleomagnetism of CO Chondrules
Abstract
Our paleomagnetic study with chondrules from carbonaceous chondrites supports the presence in the early solar system of magnetic inhomogeneities, associated with the formation of a disk substructure, or variations in the accretion rate over time.
- Publication:
-
52nd Lunar and Planetary Science Conference
- Pub Date:
- March 2021
- Bibcode:
- 2021LPI....52.2546B