Early and elongated epochs of planetesimal dynamo generation
Accreting in the first few million years (Ma) of the Solar System, planetesimals record conditions in the protoplanetary disc and are the remnants of planetary formation processes. The meteorite paleomagnetic record carries key insights into the thermal history of planetesimals and their extent of d...
Κύριοι συγγραφείς: | Sanderson, HR, Bryson, JFJ, Nichols, CIO |
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Μορφή: | Journal article |
Γλώσσα: | English |
Έκδοση: |
Elsevier
2024
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Παρόμοια τεκμήρια
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The thermal evolution of planetesimals during accretion and differentiation: consequences for dynamo generation by thermally-driven convection
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A Long‐Lived Planetesimal Dynamo Powered by Core Crystallization
ανά: Maurel, Clara, κ.ά.
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Pallasite paleomagnetism: quiescence of a core dynamo
ανά: Nichols, CIO, κ.ά.
Έκδοση: (2016)