Anyway, that's why there's an equilibrium distance where the forces balance. But superconductors also exhibit a very strange phenomenon called flux pinning [1] where a levitating object is held in place by magnetic field lines and you can even turn the whole thing upside down and it still levitates even though the forces don't cancel each other out anymore!
[1] https://en.wikipedia.org/wiki/Flux_pinning
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¹ To be fair, "the entire planet" is also around 6000 km away, calculation-wise, but still!
> Magnetic force scales as 1/r^3, not 1/r^2 like gravity
The magnetic force and gravity are two of the four fundamental forces, no? The others being the strong and weak nuclear force? At what rate do those two scale at?I remember once hearing that the rate of those forces' decay indicates (but does not prove) that they decay in more than three dimensions. This was an accomplished chemist talking, so I'm sure that she was being concise but factual.
For a complicated shape, the formula is (something like[1]) F=A/r^2+B/r^3+C/r^4+... , where r is the distance to the "center" (and some parts are closer and some parts are more far away).
An important property of magnets is that A=0, so the r^2 term dissapears. And in many cases it can be simplified to F=B/r^3 [1, again].
[1] The complete formula considers also the directions, so it's longer https://en.wikipedia.org/wiki/Multipole_expansion
This one has a table that summarizes the answer to your question
Is that a mistake?
The claim here was that "magnetic force decayed by 1/r³" which is the result of seeing a dipole ("two sources") from far away. Each pole decays by 1/r² and the net result (the combined effect of both poles on a test particle) is proportional to 1/r³
I would look at these:
https://physics.stackexchange.com/questions/184211/why-does-...
https://physics.stackexchange.com/questions/293310/why-does-...
And understand both electrostatic and magnetic dipoles in analogous terms.
You can still get that effect if both forces are r^2. You can even get it with the same force—consider standing on the moon looking up at the earth. It will just be a more marked change with r^3.