sophiecentaur said:
Why are you defending the article as a matter of principle?
I'm not "defending" the article "as a matter of principle". I'm saying the mechanism it describes looks valid to me.
sophiecentaur said:
It does not explain (doesn't even seem to consider) how the process of locking actually stops.
Sure it does:
"
Tidal locking (also called
gravitational locking or
captured rotation) occurs when the long-term interaction between a pair of co-orbiting
astronomical bodies drives the rotation rate of at least one of them into the state where there is no more net transfer of
angular momentum between this body (e.g. a planet) and its orbit around the second body (e.g. a star); this condition of "no net transfer" must be satisfied over the course of one orbit around the second body."
There's the stopping condition.
sophiecentaur said:
Why would the torques, once they have produced angular acceleration (which initially reduces the Moon's rotation), then produce a counter acceleration to stop it?
We've already discussed this. You said:
sophiecentaur said:
The Moon would go past its maximum orbit size and then return ad infinitum.
And I agreed:
PeterDonis said:
There will indeed be oscillations about an equilibrium
What I disagreed with was your claim that the equilibrium in question is an "energy minimum". It isn't: the torques acting to produce the oscillation about this equilibrium are conservative: total energy and angular momentum are conserved. That's why this equilibrium is not stable.
There have also been two additional factors discussed in this thread:
(1) The Moon's mass asymmetry, which produces an additional torque that acts to align the mass asymmetry radially. This torque is also conservative, so there will be oscillations about this equilibrium as well.
(2) Dissipation due to friction in both the Earth and the Moon. This acts to reduce the total energy of the system, which in turn means that the equilibrium point (the point where all torques are zero) shifts to a smaller average separation between the Earth and the Moon (i.e., the system becomes more tightly bound).
The only other point that hasn't yet been discussed is whether dissipation will also decrease the amplitude of oscillations about the equilibrium point. It seems to me that it would. So if that's the point you're trying to make, it's a valid point: but it certainly isn't the same as saying dissipation is what
causes tidal locking. If the torques on the tidal bulges of the Earth and Moon (and on the Moon's mass asymmetry) were not present, the Moon would not be facing the same side to the Earth at all, and dissipation wouldn't change that; it would just slowly decrease the Moon's average distance from Earth, without driving its period of rotation toward its period of revolution.