Put and . The Euler-Lagrange equations are and , where . Adding shows that is conserved. Subtracting gives the equation of a simple pendulum
The relative equilibria are and modulo . The relative energy has a strict minimum at zero, proving stability there. Linearization gives near zero and near , so the latter is unstable. The small-oscillation period is . These are equilibria of the relative angle; a nonzero conserved total angular momentum permits common rotation of both particles.

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