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