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Circular relative orbits of the central model: the critical-point criterion , uniform rotation of both labels about the centre of mass, and the linearised radial frequency
Circular relative motion in the adopted central model: the critical-point condition of the effective potential, stated equivalently as the balance between the central force and the circular motion; the explicit uniform rotation of the relative coordinate and of both labels about the centre of mass; the necessity of the condition for a constant separation; and the frequency of the linearised radial equation at a critical point satisfying the nondegeneracy condition . The linearised clause is a statement about the quadratic approximation only; no nonlinear stability, no existence of circular orbits at arbitrary radii and no empirical claim is made.
Statement
Adopt the central-force model of Adopted central-force model class: static central pair potentials, the reduced one-label problem, the fixed-centre idealization, reading conventions and exclusions clause (i) with masses , , reduced mass , and static central pair potential , and time window . Fix , an oriented orthonormal triad , and a radius , and put Then:
- (Criterion.) The following are equivalent:
- (Existence and the two labels.) If the condition of clause 1 holds, then for every the curve is a central-force trajectory for defined on all of , with , angular momentum and constant energy ; and for every interval with nonempty interior and affine centre-of-mass curve with , the restrictions to reconstruct a motion of the two-label model (Two-body reduction of a static central pair-potential model: the relative coordinate is a central-force trajectory for the reduced mass, the centre of mass moves uniformly, and the reconstruction is a bijection clause 4) has both labels moving uniformly on circles about the centre of mass: with angular velocity about .
- (Necessity.) Conversely, if a motion of the model has constant separation on a time interval with nonempty interior and nonzero constant angular momentum , then and its polar angular coordinate satisfies ; the relative motion is the uniform rotation of clause 2 up to the initial value of , and both labels move uniformly on the circles of clause 2 about the affine centre of mass.
- (Linearised radial frequency.) If and , then , and a twice differentiable on an interval with at least two points solves the linearised radial equation if and only if for some and . This is a statement about the quadratic radial approximation at ; it does not assert nonlinear stability of the circular orbit.
Facts & Assumptions
Given: The central-force model of class (i) with the potential on the open interval , the data , the oriented orthonormal triad , the radius , and the functions and constant of the statement.
Reduction and attached objects (Two-body reduction of a static central pair-potential model: the relative coordinate is a central-force trajectory for the reduced mass, the centre of mass moves uniformly, and the reconstruction is a bijection clauses 3-4, Central-force trajectories: the central-force equation, angular momentum, energy and the effective potential, Adopted central-force model class: static central pair potentials, the reduced one-label problem, the fixed-centre idealization, reading conventions and exclusions clause (ii)): the relative coordinate of every motion is a central-force trajectory for ; conversely every central-force trajectory for together with an affine centre-of-mass curve reconstructs a motion of the model, with and .
Mathematical supplier (Circular orbits of a non-radial central-force trajectory: the critical-point condition and the squared frequency of the linearised radial equation clauses 1-3, Oriented orthonormal triads in : existence over any unit vector, and the orthonormal expansion with no fourth orthogonal direction, Solutions of are exactly the functions , Central-force trajectories: the central-force equation, angular momentum, energy and the effective potential): for a central-force trajectory for with constant , , and , (i) if then and , the trajectory being with ; (ii) if then for every the displayed is a central-force trajectory on with and ; (iii) if and , the solutions of the linearised equation on an interval with at least two points are exactly with .
Differentiation and trigonometry (The chain rule, in one line from Carathéodory: if is differentiable at and is differentiable at , then is differentiable at with , Sums, scalar multiples, products and quotients: , , , and when , Euclidean maps and diffeomorphisms): derivatives of the displayed trigonometric curves and of the potential expressions are computed by the chain rule and the algebra of derivatives; the barrier term has derivative on .
Intervals and dimensions: is open, , and (Intervals of : the nine order-convex forms, nondegeneracy, and length).
Proof
Clause 1: differentiating the definition of with [L3] gives , so the first two conditions are equivalent; and by the definition of , so is equivalent to .
Clause 2: assume . By [L2] clause (ii) the displayed curve is a central-force trajectory for on with , and ; restricted to any interval with nonempty interior and combined with an affine , [L1] clause 4 reconstructs a motion on of the two-label model with and . Taking norms gives the displayed constant radii; and since is tangent to the circle and , each label traverses its circle with angular velocity .
Clause 3: assume on with , . By [L1] and [L2] clause (i), , the polar angular coordinate satisfies , so on up to the additive constant, and is the uniform rotation of clause 2; the reconstruction of [L1] clause 4 gives the two labels on the circles of clause 2 about the affine centre of mass.
Clause 4: under the two derivatives hypotheses, [L2] clause (iii) gives exactly the stated solutions of the linearised equation with the stated positive frequency , as an identity on any interval with at least two points containing .
Remarks
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The criterion is a force balance. The condition says that the effective central force at provides exactly the centripetal acceleration of uniform circular motion with angular velocity ; no circular orbit exists at a radius where the effective potential has no critical point.
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Linearisation only. Clause 4 is a statement about the quadratic approximation of the radial equation. Nothing here proves that small radial perturbations of the circular orbit stay small for all future times; only a nonlinear argument could, and none is made on this page.
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Model status. , , and the masses are model data. The statement is conditional on the adopted central model and reports no observation.
Depends on
Adopted central-force model class: static central pair potentials, the reduced one-label problem, the fixed-centre idealization, reading conventions and exclusions
Two-body reduction of a static central pair-potential model: the relative coordinate is a central-force trajectory for the reduced mass, the centre of mass moves uniformly, and the reconstruction is a bijection
Circular orbits of a non-radial central-force trajectory: the critical-point condition and the squared frequency of the linearised radial equation
Central-force trajectories: the central-force equation, angular momentum, energy and the effective potential
Oriented orthonormal triads in : existence over any unit vector, and the orthonormal expansion with no fourth orthogonal direction
Solutions of are exactly the functions
Euclidean maps and diffeomorphisms
Intervals of : the nine order-convex forms, nondegeneracy, and length
The chain rule, in one line from Carathéodory: if is differentiable at and is differentiable at , then is differentiable at with
Sums, scalar multiples, products and quotients: , , , and when
Dependency tree · 2 levels
Sources
- Konstantin Likharev, Essential Graduate Physics: Classical Mechanics (title page last edited September 1, 2026), Section 3.4, Eqs. (3.51)-(3.54), chapter page 12 (PDF page 45): the circular orbit at the minimum of the effective potential with $\mathrm dU_{\rm ef}/\mathrm dr=0$, the identification with the radial force balance, and the angular velocity $\omega=v/r_0$
- David Tong, Classical Dynamics (University of Cambridge), Section 2.5.4, printed pp. 31-33 (PDF pp. 37-39) and Figure 15: circular orbits as the minimum of the effective potential $V_{\rm eff}(r)=V(r)+J^2/(2\mu r^2)$
- Iain Stewart, Advanced Classical Mechanics (MIT 8.09/8.309 Fall 2014 course text), Section 4.5, printed pp. 79-81 (PDF pp. 82-84), Eqs. (4.151)-(4.156): the effective potential and the circular orbit $\varepsilon=0$ of the gravity-like potential with the minimum of $V_{\rm eff}$