Thanks MKreur,MKruer wrote:Whoops missed that one. As to your questions,
The L4 and L5 points are home to stable orbits so long as the mass ratio between the two large masses exceeds 24.96
http://www.physics.montana.edu/faculty/ ... range.html
L1-L3 will continue to exist regardless.
My model already includes the 24.96 threshold in it's calculations (you'll notice it doesn't include Charon-L4 and Charon-L5 for the Pluto-Charon system).
What I was actually questioning is whether the existence of the 4th body (Charon) breaks the model altogether for Nix and Hydra. (Remember that the formulae are based on a 3-body approximation)
Charon's orbit lies about 1/2 way between Pluto and Nix/Hydra) and given it's significant mass,...intuitively I suspect that the perturbative effects of Charon on the orbits of Nix and Hydra (and by implication their theoretical lagrange locations), would be so significant that to model them with this 3-body approximation would be unrealistic. (Including the L1,L2,L3 points)
What I suspect is that if they exist at all, stable or semi-stable Lissajous Orbits in the Nix and Hydra systems would be somewhat more complex than in the Earth-Moon system.