The thermal evolution of planetesimals during accretion and differentiation: consequences for dynamo generation by thermally-driven convection
The meteorite paleomagnetic record indicates that differentiated (and potentially, partially differentiated) planetesimals generated dynamo fields in the first 5-40 Myr after the formation of calcium-aluminium-rich inclusions (CAIs). This early period of dynamo activity has been attributed to therma...
Autori principali: | Dodds, K, Bryson, J, Neufeld, J, Harrison, R |
---|---|
Natura: | Journal article |
Lingua: | English |
Pubblicazione: |
Wiley
2021
|
Documenti analoghi
-
Unlocking planetesimal magnetic field histories: a refined, versatile model for thermal evolution and dynamo generation
di: Sanderson, HR, et al.
Pubblicazione: (2024) -
Early and elongated epochs of planetesimal dynamo generation
di: Sanderson, HR, et al.
Pubblicazione: (2024) -
Meteorite evidence for partial differentiation and protracted accretion of planetesimals
di: Bryson, J, et al.
Pubblicazione: (2020) -
Meteorite evidence for partial differentiation and protracted accretion of planetesimals
di: Maurel, Clara, et al.
Pubblicazione: (2021) -
Meteorite evidence for partial differentiation and protracted accretion of planetesimals
di: Maurel, Clara, et al.
Pubblicazione: (2022)