Is central motion stable with criteria for force function f(r)?

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Central motion stability is determined by the criteria f'(r) + 3/r > 0 for the force function f(r). This stability implies that if a satellite is slightly perturbed, it will not escape its orbit but will instead oscillate radially while continuing to orbit. The discussion raises questions about the nature of this stability, particularly regarding periodic orbits and its relation to the Lyapunov exponent. The concept of stability here suggests a sinusoidal oscillation superimposed on circular motion. Understanding these dynamics is crucial for analyzing orbital mechanics.
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In central motion we have criteria for stability. For function of force f(r)
we have stability if
f'(r)+\frac{3}{r}>0

This is stability in what sence? Do I have then periodic orbits or what? Is it in some connection with calculations of Lyapunov exponent? Thanks for the answer.
 
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Stability in the sense that if you give the satellite a little push, it doesn't escape the orbit, rather it oscillates in the radial direction, while orbiting!(Just imagine a sinusoid with a circle as the x axis!)
 
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