No.
There are five Lagrangian points. All require that AA have a significantly greater mass than B, and that B have a significantly greater mass than c.
AA B c
Here, the extra gravity from B makes c orbit around AA faster than it would by itself, so that it keeps pace with B. This configuration is stable only as long as it is perfectly undisturbed.
AA c B
Here, the extra gravity from B makes c orbit around AA slower than it would by itself, so that it keeps pace with B. This configuration, too, will not repair itself.
c AA B
As long as c and B are in perfect opposition, this is stable.
These three positions are only hypothetical, in that they cannot be expected to occur naturally (though they can and do occur artificially). The following two positions, however, do occur in nature.
c
AA B
d
c (in B’s orbit around AA, 60 degrees ahead) and d (in B’s orbit around AA, 60 degrees behind) are stable. If disturbed, they will tend to fall back into place. There are a great many asteroids occupying these positions with respect to the Sun and Jupiter (the so-called “Trojan” asteroids), and there is some evidence that there are dust clouds occupying these positions with respect to the Earth and the Moon.
I should add that Zor’s remark:
should be emended slightly. They are not a “mystery to scientists”; the equations have been well known since Newton’s time. However, as equations, they have never been generally solved for systems of more than two bodies. That doesn’t mean that they can’t be solved by arithmetic and brute force. Furthermore, Lagrange did manage to work out five real, but partial, solutions, and that is why the Lagrangian points bear his name.
John W. Kennedy
“Compact is becoming contract; man only earns and pays.”
– Charles Williams