An attractive inverse-square force together with radial drag preserves angular momentum but modifies the Binet equation for by a first derivative. For and , the reciprocal radius is a decaying oscillation about . Forward angular distance makes its damping sign explicit for either orbital orientation.
A bounded trajectory in the damped Binet equation with nonzero angular momentum asymptotically becomes circular. Energy loss is nonnegative in magnitude and vanishes only for zero radial velocity. The centrifugal effective potential energy excludes collision; bounded radius forces indefinitely increasing forward angular distance, so the reciprocal-radius oscillation decays. Escaping trajectories are excluded by the boundedness hypothesis.
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