How does Ganymede sustain a core dynamo today? · revision history
Revision 2
Accepted · core change · record
Changes against revision 1:
- Title
- How does Ganymede sustain a core dynamo today?
- Plain
- Jupiter's moon Ganymede is the only moon known to make its own magnetic field. Models of how such a small body cools suggest its core should have stopped stirring long ago.
- Precise · changed · core
- Revision 1: Galileo detected an intrinsic dipole with surface equatorial strength near 7e-3 G. Identify the power source that keeps Ganymede's Fe-FeS core convecting after 4.5 Gyr: iron snow, FeS crystallization, compositional convection, or heat from past tidal heating during resonance passage. An answer is a thermal-chemical evolution model producing a present dynamo of the observed strength.
- Revision 2: Galileo detected an intrinsic dipole with surface equatorial strength near $7 \times 10^{-3}$ G. Identify the power source that keeps Ganymede's Fe-FeS core convecting after 4.5 Gyr: iron snow, FeS crystallization, compositional convection, or heat from past tidal heating during resonance passage. An answer is a thermal-chemical evolution model producing a present dynamo of the observed strength.
- Settled by
- JUICE orbital measurements of field harmonics, induction response and gravity (Love numbers) constraining core size and state.
- Kind
- phenomenon
- Answer type
- mechanism
- References
- (empty)
- Literature status
- open
- Status note
- JUICE is planned to arrive at Jupiter in 2031 and orbit Ganymede from 2034.
- Posed since
- 1996
Decisions
- Accept · 2026-10-15 · record