The collinear Lagrange point beyond the smaller primary, away from the larger one, is . For a small mass ratio it lies approximately one Hill radius from the secondary and has a growing linear mode.
In unit binary separation and mean motion, displacements obey and , where at . The characteristic polynomial is . The small-secondary limit has .
For a small secondary-to-primary mass ratio, the unstable exponent at the outer collinear equilibrium is . Its inverse is approximately binary periods. Reaching a finite target distance takes this time multiplied by the logarithm of the ratio of final to initial unstable amplitudes.

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