Specifically, Earnshaw's Theorem states that in a static situation for pointlike particles, a 1/r potential does not have any maxima or minina (stable points) in an unoccupied region, since the sources themselves occupy space. When dynamics are added into the mix, there is an effective potential from the angular component which pushes away from the source and falls off as 1/r2. For example, with gravity, the potential is a combination of angular repulsion ([itex]\frac{1}{2}\frac{mh^2}{r^2}[/itex]) and gravitational attraction ([itex]\frac{GMm}{r}[/itex]), which gives a total potential of [itex]U=\frac{1}{2}\frac{mh^2}{r^2} - \frac{GMm}{r}[/itex], and a minimum at [itex]r=\frac{h^2}{GM}[/itex].
(h is angular momentum per mass)