I bet the time scales for those phase transitions wouldn't be incalculable, even if gross estimates.
So, if the moon were a vapor bubble suspended in a vacuum, how long would that last? And how long for the heat to radiate out of it?
Sounds like that process would be pretty uniform, and dependent mostly on composition. But the uniformity of the temperature bleed would contribute to the maintenance of a stable orbit.
I'm imagining that, as the hot gases cool off, and condense onto floating debris, the molten/solid debris field will probably look pretty nebulous, and then settle into unstable bands. At that point, I figure the torus shape would be very apparent.
Once the hot gases were gone, I bet it probably took a while for the rest of the debris to get swept up into decaying orbits, and impact on either body (earth/moon).
If they could visualize it with a simulation, it'd probably be fun to watch, and tweak the parameters of the event.