A spinning body is most stable with its mass farthest from its spin axis ... On Europa, variations in the thickness of its outer shell caused a mass imbalance, so the rotation axis reoriented to a new stable state.
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A spinning body is most stable with its mass farthest from its spin axis ... On Europa, variations in the thickness of its outer shell caused a mass imbalance, so the rotation axis reoriented to a new stable state.
It suggests that planetary bodies might be more prone to reorientation than we thought.
The large reorientation on Europa required to explain the circular depressions implies that its outer ice shell is decoupled from the core by a liquid layer ... Therefore, our study provides an independent test for the presence of an interior liquid layer.
There could still be some reorientation, and we should still look out for fractures, but this rim effect would be very important