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Derivation · the atom

Effective potential and the orbit equation for a central force

D-006 central-force-orbit-equation Home PU-201 Threads force · energy Depends on D-001, D-002 verified

Statement

Motion under any central force reduces to one-dimensional motion in an effective potential, and for an inverse-square force the resulting orbit is a conic section.

Why it matters

This is the single move that turns the two-body gravitational problem into something solvable by hand. It delivers all three of Kepler's laws as corollaries rather than separate discoveries, and it fixes the exact boundary — the inverse-square law — beyond which orbits stop closing. It is the classical baseline that relativity (PU-305) and the quantum atom (PU-101) are measured against.

Assumptions
The force is central: F = F(r).Depends only on separation and points along it. Drop this and angular momentum is no longer conserved and the motion is not planar. Two-body problem reduced to one body of reduced mass μ = m1m2/(m1+m2).Exact for two bodies; for three or more no such reduction exists and the problem is not integrable. Non-relativistic, and no radiation reaction.Drop the first and Mercury's perihelion precesses (PU-305); drop the second and a classical orbiting electron spirals into the nucleus in about 10⁻¹¹ s.
Derivation
1
L = ½μ(² + r²θ̇²) − V(r)
Plane polar coordinates. The motion is planar because L = r × p is conserved for a central force and r is always perpendicular to it. A
2
θ is cyclic ⟹ ≡ ∂L/∂θ̇ = μr²θ̇ = const
L contains θ̇ but not θ, so by D-001 its conjugate momentum is conserved. This is angular momentum, and it is also Kepler's second law: dA/dt = /2μ, equal areas in equal times. A
3
E = ½μṙ² + ²/2μr² + V(r) ≡ ½μṙ² + Veff(r)
Conserved by D-002, with θ̇ eliminated using step 2. The angular kinetic energy has become a term in a one-dimensional potential. This is the central trick: a 2-D problem is now a 1-D problem plus a quadrature for θ. B
4
u ≡ 1/r,   d/dt = (ℓu²/μ) d/dθ
Change variable from r(t) to u(θ). We want the shape of the orbit, not the timetable; eliminating t is what makes the equation solvable in closed form. B
5
u/dθ² + u = − (μ/²u²) F(1/u)
Substituting step 4 into the radial equation of motion. This is the Binet equation and it holds for any central force. Note its form: a harmonic oscillator in θ with a forcing term. C
6
F = −k/r² ⟹ d²u/dθ² + u = μk/²
For the inverse-square law the two factors of u² cancel exactly, leaving a constant on the right. This cancellation is special to the inverse square and is the reason that case alone gives closed orbits. C
Result
r(θ) = (²/μk) / (1 + e cos θ),    e = √( 1 + 2E²/μk² )

Reading. A driven harmonic equation with constant forcing, solved by a constant plus a cosine. The eccentricity is fixed by the energy alone: E < 0 gives e < 1, an ellipse; E = 0 gives a parabola; E > 0 gives a hyperbola. Kepler's first law is a corollary, not a separate discovery.

Units check. ²/μk has units [kg m² s⁻¹]²/([kg][N m²]) = m. ✓

Limiting cases
  • The ²/2μr² term is repulsive and dominates at small r — this is the centrifugal barrier, and it is why a body with any angular momentum at all cannot reach the origin.
  • The minimum of Veff is the circular orbit. Its curvature gives the frequency of small radial oscillations about it; when that frequency equals the orbital frequency, the orbit closes. Bertrand's theorem shows this happens only for the inverse-square and the linear force laws.
  • Kepler's third law follows immediately: T² = 4π²μa³/k.
Breaks when
  • A third body is present. No closed-form solution exists and the motion can be chaotic.
  • Speeds approach c, or the field is strong — the orbit precesses and D-006 must be replaced by the geodesic treatment in PU-305.
  • The bodies are extended and tidally deformed, or the force law departs from the inverse square by any amount — closure is immediately lost.
Failure modes
  • Calling the centrifugal term a force. It is a term in an effective potential that appeared from eliminating θ̇; there is no outward force in the inertial frame.
  • Using m instead of μ when the masses are comparable. Fine for Earth–Sun, badly wrong for a binary star.
  • Assuming a small change in the exponent of the force law produces a small change in the orbit. It produces precession, which accumulates without bound.
Worked number

Integrate a force law F ∝ 1/r2+ε and measure the precession rate as a function of ε: at ε = 0 the orbit closes exactly, and any nonzero ε drives a perihelion that advances without bound. The forward link PU-305 recovers Mercury's 43″/century from general relativity. Run the check →

Discussion

The engine of D-006 is not a clever integral but a bookkeeping of symmetry. A central force has no preferred direction in the plane and no explicit clock, so two quantities are handed to us for free: angular momentum (rotational symmetry, step 2) and energy E (time-translation symmetry, step 3). Each conserved quantity removes one degree of freedom. What began as two coupled second-order equations for r(t) and θ(t) collapses to a single first-order statement, E = ½μṛ² + Veff(r), that a first-year student could read off a graph. The angular motion has not vanished; it has been repackaged as the ²/2μr² centrifugal term, a wall that any body with ≠ 0 cannot climb through — which is why nothing carrying angular momentum ever reaches the force centre.

The reason the answer is a conic section and not some transcendental curve is visible in step 6. The Binet equation is a harmonic oscillator in the angle θ driven by −(μ/²u²)F(1/u). Only for the inverse-square law does the awkward 1/u² prefactor cancel the u² hidden in F = −ku², leaving a constant drive. A constant-forced oscillator has the solution "constant plus one cosine", u = (1 + e cos θk/², and that single cosine is the ellipse. The eccentricity rides entirely on the energy, e = √(1 + 2E²/μk²): bound orbits (E < 0) close into ellipses, E = 0 is the marginal parabola, and E > 0 opens into a hyperbola. Kepler's first law is therefore a corollary of the algebra, not an independent empirical law.

The deeper statement is that the inverse-square orbit closes on itself — the perihelion never drifts — and this is overdetermination. Bertrand's theorem singles out only two force laws (the inverse square and the linear Hooke spring) for which every bound orbit closes; for these the radial oscillation frequency and the orbital frequency are locked in a rational ratio. Behind the Kepler case sits an extra conserved vector, the Laplace–Runge–Lenz vector A = p × Lμk, which points along the major axis and pins the ellipse in place. Its conservation reflects a hidden SO(4) dynamical symmetry of the bound Kepler problem, larger than the obvious SO(3) of rotations; the same symmetry, promoted to quantum operators, is what makes the hydrogen energy levels depend only on the principal quantum number and not on . Break the inverse-square law by any amount and A is no longer conserved — the axis rotates and the orbit precesses.

The same six lines describe far more than planets. Flip the sign of k and demand E > 0 and the identical orbit equation gives the hyperbolic trajectory of Rutherford scattering; the impact-parameter–to–deflection relation and the famous dσ/dΩ ∝ sin⁻⁴(θ/2) cross-section fall straight out of it. The parabolic E = 0 case is the marginal-escape trajectory used for interplanetary transfers. And the forward link to PU-305 is exactly the failure mode named above: general relativity adds a small effective −1/r³ term to the potential, the axis-fixing vector A ceases to be conserved, and Mercury's perihelion advances the observed 43″ per century.

Common misconceptions.

  • The centrifugal term is not a real force. It is a piece of Veff that appeared purely from eliminating θ̇ using = const; in the inertial plane there is no outward push, only the inward F(r).
  • Eccentricity is fixed by the energy alone, not by the angular momentum. Two orbits of the same E but different have the same e and the same major axis; only their size across (the semi-latus rectum ²/μk) differs.
  • Using the full mass m instead of the reduced mass μ. Harmless for Earth–Sun where μm, but for a comparable-mass binary it corrupts both the period and the eccentricity.
  • Assuming a tiny change in the force exponent gives a tiny change in the orbit. It gives precession, an angular error that grows without bound orbit after orbit — a qualitative change, not a small one.
Worked examples

Example 1 — Reconstructing a comet's orbit from one perihelion measurement. A comet is seen at perihelion at distance rp = 8.0×10¹⁰ m from the Sun moving at vp = 5.0×10⁴ m s⁻¹. Take GM = 1.327×10²⁰ m³ s⁻². Because the comet mass is negligible, μm, so we work per unit mass: εE/μ, h/μ, and k/μ = GM. Find e, the semi-major axis, the aphelion distance and the period.

1
ε = ½vp² − GM/rp = ½(5.0×10⁴)² − (1.327×10²⁰)/(8.0×10¹⁰) = 1.25×10⁹ − 1.659×10⁹ = −4.09×10⁴ J kg⁻¹
Specific energy (step 3 divided by μ). It is negative, so E < 0 and the orbit is a bound ellipse.
2
a = −GM/(2ε) = −(1.327×10²⁰)/(2×(−4.09×10⁴)) = 1.62×10¹¹ m
From E = −k/2a (the ellipse energy), which per unit mass reads ε = −GM/2a. About 1.08 AU.
3
h = rpvp = (8.0×10¹⁰)(5.0×10⁴) = 4.0×10¹⁵ m² s⁻¹,   p = h²/GM = (4.0×10¹⁵)²/(1.327×10²⁰) = 1.21×10¹¹ m
At perihelion the velocity is purely tangential, so h = rpvp. The semi-latus rectum p = ²/μk = h²/GM is the numerator of the orbit equation.
4
e = √(1 + 2εh²/(GM)²) = √(1 + 2(−4.09×10⁴)(1.6×10³¹)/(1.761×10⁴⁰)) = √(1 − 0.743) = 0.507
The eccentricity formula with μ cancelled top and bottom. Cross-check: p = a(1 − e²) ⇒ 1−e² = 1.21/1.62 = 0.743 ✓.
5
ra = a(1 + e) = 1.62×10¹¹(1.507) = 2.45×10¹¹ m,   T = 2π√(a³/GM) = 2π√((1.62×10¹¹)³/1.327×10²⁰) = 3.57×10⁷ s
Aphelion from the far apse of the ellipse; period from Kepler's third law (result list item 3, with μa³/k = a³/GM).
e = 0.51,  a = 1.62×10¹¹ m,  ra = 2.45×10¹¹ m,  T = 3.57×10⁷ s

Answer. The comet is on a bound ellipse of eccentricity 0.51 and semi-major axis 1.08 AU, swinging out to 1.64 AU at aphelion, with an orbital period of 3.57×10⁷ s ≈ 1.13 yr. A single position-and-velocity pair at one instant fixes the entire orbit, because E and are all the constants the motion has.

Example 2 — The circular orbit at the bottom of Veff, and why it closes. A satellite in a circular orbit sits exactly at the minimum of the effective potential. For a low Earth orbit at rc = 7.00×10⁶ m (GM = 3.986×10¹⁴ m³ s⁻²), find the orbital speed and period, then show the frequency of small radial oscillations equals the orbital frequency — the statement that the inverse-square orbit closes.

1
Veff′(rc) = 0 ⇒ ²/μrc³ = k/rc² ⇒ vc = √(GM/rc) = √((3.986×10¹⁴)/(7.00×10⁶)) = 7.55×10³ m s⁻¹
The circular orbit is the potential minimum: the inward force supplies exactly the centripetal requirement, μvc²/rc = k/rc².
2
ωorb = vc/rc = √(GM/rc³) = 1.078×10⁻³ rad s⁻¹,   T = 2π/ωorb = 5.83×10³ s
Orbital angular frequency and period; 5.83×10³ s ≈ 97 min, the familiar LEO number.
3
ωr² = Veff″(rc)/μ = (1/μ)(−3F/rcF′) ⇒ ωr²/ωorb² = 3 + rcF′/F
Expand Veff to second order about rc; small radial displacements oscillate as a spring of stiffness Veff″. Using ωorb² = −F/μrc gives the clean ratio.
4
F = −k/r² ⇒ rcF′/F = −2 ⇒ ωr²/ωorb² = 3 − 2 = 1 ⇒ ωr = ωorb = 1.078×10⁻³ rad s⁻¹
For the inverse-square law the two frequencies are equal. The apsidal angle is Δθ = π/√(3−n) = π for n = 2: the radius returns to minimum after exactly half a revolution, so the orbit closes after one full turn.
vc = 7.55 km s⁻¹,  T = 97 min,  ωr = ωorb

Answer. The circular LEO orbit has speed 7.55 km s⁻¹ and period 97 min. Because the inverse-square law gives ωr/ωorb = 1, a slightly non-circular version of this orbit returns to perigee after exactly one revolution — a closed ellipse. Had the exponent been n = 2 + ε, the ratio would be √(1−ε) ≠ 1 and the perigee would creep round each orbit; this is precisely how the closure of Kepler orbits is a knife-edge property of the inverse square.

Problems
  1. (Classification.) A probe around the Sun has specific energy ε = −1.5×10⁸ J kg⁻¹ and specific angular momentum h = 6.0×10¹⁵ m² s⁻¹ (GM = 1.327×10²⁰). Find the eccentricity, classify the orbit, and give the semi-major axis.
    Solution

    Use e = √(1 + 2εh²/(GM)²), the per-mass form of the result box. Compute 2εh² = 2(−1.5×10⁸)(3.6×10³¹) = −1.08×10⁴⁰; (GM)² = (1.327×10²⁰)² = 1.761×10⁴⁰. Ratio = −0.613, so e = √(1−0.613) = √0.387 = 0.62. Since ε < 0 (equivalently e < 1) the orbit is a bound ellipse. Semi-major axis a = −GM/2ε = (1.327×10²⁰)/(3.0×10⁸) = 4.42×10¹¹ m (≈ 2.95 AU).

  2. (Apsides.) From the orbit equation r(θ) = (²/μk)/(1 + e cos θ), show that the perihelion and aphelion distances are r± = p/(1 ∓ e) with p = ²/μk, and hence that a = p/(1−e²) and a = −k/2E.
    Solution

    r is extremal where cos θ = ±1. At θ = 0, rmin = p/(1+e) (perihelion); at θ = π, rmax = p/(1−e) (aphelion). The major axis is 2a = rmin + rmax = p[1/(1+e) + 1/(1−e)] = p·2/(1−e²), so a = p/(1−e²). Now substitute e² = 1 + 2E²/μk² so that 1−e² = −2E²/μk². Then a = (²/μk)/(−2E²/μk²) = k/2E. The size of the ellipse depends only on the energy; the shape (through e) mixes energy and angular momentum.

  3. (Kepler III for a binary — use μ.) Two stars of masses M1 = 2M and M2 = 3M orbit their common centre of mass; the semi-major axis of the relative orbit is a = 3.0×10¹¹ m. Find the period. (M = 1.989×10³⁰ kg, G = 6.674×10⁻¹¹.)
    Solution

    The result gives T² = 4π²μa³/k. Here k = GM1M2 and μ = M1M2/(M1+M2), so μ/k = 1/[G(M1+M2)] and T² = 4π²a³/[G(M1+M2)]. The individual masses cancel into their sum — the correct handling of the reduced mass. With M1+M2 = 5M = 9.945×10³⁰ kg: G(M1+M2) = 6.637×10²⁰; a³ = 2.7×10³⁴. So T² = 39.48×2.7×10³⁴/6.637×10²⁰ = 1.606×10¹⁵, giving T = 4.0×10⁷ s ≈ 1.27 yr. (Had we mistakenly used m = M2 instead of μ, the period would be badly wrong.)

  4. (Inverse problem via Binet.) A particle is observed to move on a logarithmic spiral r(θ) = r0e. What central force law produces this orbit?
    Solution

    Let u = 1/r = (1/r0)e. Then du/dθ = −ku and d²u/dθ² = k²u. Insert into the Binet equation (step 5): d²u/dθ² + u = (k² + 1)u = −(μ/²u²)F(1/u). Solving, F = −(²/μ)(1+k²)u³ = −(²(1+k²)/μ)·1/r³. The spiral is produced by an attractive inverse-cube force. Note this orbit does not close — the inverse cube is not one of Bertrand's laws — consistent with the spiral falling in to (or out from) the centre.

  5. (Precession from a perturbed potential.) Add an inverse-cube perturbation, F(r) = −k/r² − λ/r³ with λ > 0 small. Solve the Binet equation, show the orbit is a precessing ellipse, and find the apsidal angle and the perihelion advance per revolution. Relate this to the forward link to PU-305.
    Solution

    With F(1/u) = −ku² − λu³, the Binet equation becomes d²u/dθ² + u = −(μ/²u²)(−ku²−λu³) = μk/² + (μλ/²)u. Collect the u terms: d²u/dθ² + Ω²u = μk/², with Ω² ≡ 1 − μλ/². This is still a constant-forced oscillator, but with shifted frequency Ω < 1. Its solution is u = μk/(²Ω²) + A cos(Ωθ) — an ellipse-like curve whose radius returns to perihelion each time Ωθ increases by 2π. The angle between successive perihelia is therefore Δθ = 2π/Ω, exceeding 2π because Ω < 1. The advance per orbit is Δφ = 2π(1/Ω − 1). For small λ, Ω ≈ 1 − μλ/2², so 1/Ω ≈ 1 + μλ/2² and Δφπμλ/² per revolution (prograde). This is the mechanism behind the forward link: general relativity contributes an effective −1/r³ term to the potential, which by exactly this calculation makes Mercury's perihelion advance — 43″ per century after Newtonian planetary perturbations are subtracted. A change in the force law that looks small produces an angular drift that accumulates without bound.