Central Forces and Statics

Contents
  1. Statics
  2. Central forces
  3. The equivalent one-dimensional problem
  4. The two-body problem and Kepler orbits
  5. The virial theorem
  6. Where the claims of this chapter are tested

Two special regimes of the Newtonian dynamics of Newtonian Dynamics deserve a chapter of their own. The first is the regime in which nothing moves at all: statics, the theory of equilibrium, whose two conditions are the direct specialization of the translational and rotational laws of motion. The second is the regime in which the force on a particle always points along the line to a fixed centre: central motion, which governs planetary orbits and scattering alike, and which reduces — through its conservation laws — to an equivalent problem in a single radial dimension. Standard extended treatments may be found in the classical references [Goldstein:2002] [Landau:1976] [Taylor:1997].

The two regimes are less distant from one another than they look. Both are governed by what a conservation law removes: statics is what remains when the momenta are held at zero, central motion is what remains when the angular momentum has been used to eliminate one coordinate and the energy to eliminate another. In both, the whole of the physics sits in a function of one variable — a potential energy on a configuration space in the first case, an effective potential of the radius in the second.

Remark 27.1 (Two pieces of mathematics used but not owned here).

This chapter uses two elementary facts about \(\R^{3}\) that Real Analysis and Differentiable Manifolds, Tensors, and Curvature do not state, and states them here rather than proving general mathematics inside a physics chapter. The first is the expansion of the double cross product,

\begin{equation}\tag{27.1} \vect{a}\times\left(\vect{b}\times\vect{c}\right) =\vect{b}\left(\vect{a}\cdot\vect{c}\right) -\vect{c}\left(\vect{a}\cdot\vect{b}\right)\ec \end{equation}

used once, in Theorem 27.38. The second is that the area of a circular sector of radius \(r\) subtending an angle \(\phi\) is \(\tfrac{1}{2}r^{2}\phi\), used once, in Proposition 27.17. Both belong to the elementary vector algebra and plane geometry that Part II owes; neither is in dispute, and the reader who wants them proved will find them in any of [Goldstein:2002] [Taylor:1997].

Statics

Definition 27.2 (Translational equilibrium).

A particle is said to be in translational equilibrium if and only if

\begin{equation}\tag{27.2} \sum_{m}\vect{F}_m=\vect{0}\ec \end{equation}

where the \(\vect{F}_m\) are the \(m\) forces upon the particle. Rests on Equation (19.2) and Definition 19.5.

Definition 27.3 (Rotational equilibrium).

A particle is said to be in rotational equilibrium if and only if

\begin{equation}\tag{27.3} \sum_{n}\vect{\tau}_n=\vect{0}\ec \end{equation}

where the \(\vect{\tau}_n\) are the \(n\) torques upon the particle. Rests on Equation (19.14) and Definition 19.18.

Under these conditions, Equations (19.2) and (19.14) state that the linear momentum and the angular momentum of the particle are constant: equilibrium is the regime in which Newton's second laws, translational and rotational, reduce to conservation statements.

A torque is defined about a chosen point, so the second condition looks at first sight to depend on that choice. It does not, provided the first condition already holds — and that is what makes the pair of conditions usable at all.

Proposition 27.4 (Torque balance is independent of the origin).

Let a system of forces \(\vect{F}_{m}\) act at the points \(\vect{x}_{m}\) of a body, and suppose Equation (27.2) holds. Then the total torque \(\vect{\tau}_{O}=\sum_{m}\vect{x}_{m}\times\vect{F}_{m}\) takes the same value about every point \(O\). Consequently, if the torque balance Equation (27.3) holds about one point, it holds about all of them. Rests on Equations (19.15) and (27.2).

Proof.

Derives Proposition 27.4. Let \(O'\) be displaced from \(O\) by \(\vect{a}\), so that the position of the \(m\)-th point of application measured from \(O'\) is \(\vect{x}_{m}-\vect{a}\). By Equation (19.15) the total torque about \(O'\) is

\begin{equation}\tag{27.4} \vect{\tau}_{O'} =\sum_{m}\left(\vect{x}_{m}-\vect{a}\right)\times\vect{F}_{m} =\vect{\tau}_{O}-\vect{a}\times\sum_{m}\vect{F}_{m} =\vect{\tau}_{O}\ec \end{equation}

the last step by Equation (27.2). The displacement \(\vect{a}\) was arbitrary.

The proposition is sharper than it looks, and its converse is false in a way worth stating: when the net force does not vanish, the torque does depend on the reference point, and one may always slide \(O'\) along the line perpendicular to \(\sum\vect{F}_{m}\) until the torque about it vanishes. That is why a single unbalanced force is described as acting along a definite line of action rather than at a definite point.

Phenomenon 27.5 (Equilibrium requires two conditions, not one).

A body stays at rest only if the forces upon it balance and their turning effects balance; the two requirements are independent, and Nature displays the difference plainly. Two equal and opposite forces applied at different points of a rigid body — a couple, as when both hands turn a steering wheel — leave the centre of mass exactly where it was and set the body spinning. Conversely a single force whose line of action passes through the centre of mass translates the body without turning it at all. Every static structure, from a balanced beam to a ladder leaning against a wall, stands by the simultaneous satisfaction of both conditions, and fails when either is violated [Newton:1687]. Rests on Equations (27.2) and (27.3).

Derivation. Derives Phenomenon 27.5. Apply forces \(\vect{F}\) and \(-\vect{F}\) at the points \(\vect{x}_1\) and \(\vect{x}_2\) of a rigid body. Equation (27.2) is satisfied, since the two cancel, so by the second law of Newtonian Dynamics the centre of mass keeps whatever velocity it had. The total torque about the origin, however, is

\begin{equation}\tag{27.5} \vect{\tau}=\vect{x}_1\times\vect{F} +\vect{x}_2\times\left(-\vect{F}\right) =\left(\vect{x}_1-\vect{x}_2\right)\times\vect{F}\ec \end{equation}

which is independent of the choice of origin — a couple has the same moment about every point, which is Proposition 27.4 for the special case of a vanishing resultant — and which vanishes only if \(\vect{F}\) is parallel to the line joining the two points of application. Whenever it does not vanish, Equation (27.3) fails, the angular momentum grows, and the body turns although no net force acts upon it. For the converse case, a single force applied at the centre of mass has \(\vect{x}=\vect{0}\) measured from there, hence zero moment about it, and the body accelerates without rotating. The two conditions are therefore logically independent, and neither implies the other.

The centre of gravity

Weight acts on every part of a body, so the gravitational contribution to Equation (27.3) is a sum over the whole mass distribution. In a uniform field that sum collapses to a single term.

Definition 27.6 (Centre of gravity).

The centre of gravity of a body in a gravitational field is the point \(\vect{X}_{g}\) such that the total gravitational torque about any point equals the torque of the total weight applied at \(\vect{X}_{g}\) alone. Rests on Definition 19.47 and Equation (19.15).

Proposition 27.7 (Centre of gravity in a uniform field).

If the gravitational field \(\vect{g}\) is the same at every point of the body, then \(\vect{X}_{g}=\vect{X}\), the centre of mass Equation (19.38), and the total gravitational torque about the origin is

\begin{equation}\tag{27.6} \vect{\tau}_{g}=\vect{X}\times M\vect{g}\ec \end{equation}

with \(M\) the total mass Equation (19.32). Rests on Equations (19.15), (19.32) and (19.38).

Proof.

Derives Proposition 27.7. The weight of the \(m\)-th element is \(m_{m}\vect{g}\) with one and the same \(\vect{g}\), so by Equation (19.15)

\begin{equation}\tag{27.7} \vect{\tau}_{g}=\sum_{m}\vect{x}_{m}\times m_{m}\vect{g} =\left(\sum_{m}m_{m}\vect{x}_{m}\right)\times\vect{g} =\vect{X}\times M\vect{g}\ec \end{equation}

using Equation (19.38) in the form \(\sum_{m}m_{m}\vect{x}_{m}=M\vect{X}\). The right-hand side is the torque of a single force \(M\vect{g}\) applied at \(\vect{X}\), which is Definition 27.6.

The uniformity hypothesis is not idle. Over a body of vertical extent \(h\) near the Earth's surface the field varies by a relative amount \(2h/R_{\oplus}\), about \(3\times10^{-7}\) per metre; the resulting separation of the centre of gravity from the centre of mass is what raises the tides and what makes a satellite in orbit settle with its long axis pointing at the planet. For a laboratory body it is utterly negligible, and Proposition 27.7 is exact for every purpose of this section.

Phenomenon 27.8 (The centre of gravity hangs below the support).

A flat plate hung freely from a pin comes to rest, after its oscillations have died away, in one definite orientation, and the vertical line through the pin always passes through the same material point of the plate whichever pin is used. Suspending the plate from two different points and marking the two verticals locates that point as their intersection; a third suspension confirms it. This is how the centre of gravity of an irregular body is measured, and it is the principle of every balance and every plumb line [Newton:1687]. Rests on Equations (27.3) and (27.6).

Derivation. Derives Phenomenon 27.8. Take torques about the point of support \(S\), so that the unknown reaction there contributes nothing. The only other force is the weight, whose torque is \(\left(\vect{X}-\vect{x}_{S}\right)\times M\vect{g}\) by Equation (27.6). Rotational equilibrium Equation (27.3) therefore demands

\begin{equation}\tag{27.8} \left(\vect{X}-\vect{x}_{S}\right)\times M\vect{g}=\vect{0}\ec \end{equation}

that is, that \(\vect{X}-\vect{x}_{S}\) be parallel to \(\vect{g}\): the centre of gravity lies on the vertical through the support. Two positions satisfy this, one with \(\vect{X}\) below \(S\) and one with it above; only the first is stable, by Theorem 27.10, since rotating the body about the pin from that position raises the centre of gravity and so raises the potential energy \(MgZ\), \(Z\) being its height, whereas rotating it from the second position lowers \(Z\). Repeating the suspension from a second point gives a second vertical through the same material point, and two non-parallel lines meet in one point.

Equilibrium as a stationary potential energy

Written out force by force, the equilibrium of a mechanism with many joints is a large system of equations in which most of the unknowns are constraint forces nobody wants to know. The principle of virtual work Equation (21.17) removes them all at once, because a constraint force does no virtual work.

Theorem 27.9 (Equilibrium is stationarity of the potential energy).

Consider a system with holonomic, time-independent constraints, described by generalized coordinates \(q^{a}\), \(a=1,\dots,n\), whose active forces derive from a potential energy \(U(q)\). Then a configuration \(q_{0}\) is an equilibrium configuration if and only if

\begin{equation}\tag{27.9} \left.\pdv{U}{q^{a}}\right|_{q_{0}}=0\ec\qquad a=1,\dots,n\ep \end{equation}

Rests on Equation (21.17), Equation (21.31) and Definition 21.2.

Proof.

Derives Theorem 27.9. By Theorem 21.18 the system is in equilibrium if and only if the virtual work of the active forces vanishes for every virtual displacement compatible with the constraints. Because the constraints are holonomic and time-independent, a compatible virtual displacement is exactly one of the form \(\delta\vect{x}^{s} =\left(\pp\vect{x}^{s}/\pp q^{a}\right)\delta q^{a}\) with the \(\delta q^{a}\) arbitrary and independent, so that by Equation (21.31) the virtual work is

\begin{equation}\tag{27.10} \delta W=\sum_{s}\vect{F}^{s}\cdot\delta\vect{x}^{s} =Q_{a}\,\delta q^{a}\ec\qquad Q_{a}=\sum_{s}\vect{F}^{s}\cdot\pdv{\vect{x}^{s}}{q^{a}}\ep \end{equation}

For forces derived from a potential, \(\vect{F}^{s}=-\nabla_{s}U\) and the chain rule (Proposition 7.72) gives \(Q_{a}=-\pp U/\pp q^{a}\). Vanishing of \(Q_{a}\delta q^{a}\) for arbitrary independent \(\delta q^{a}\) is vanishing of every \(Q_{a}\), which is Equation (27.9).

Equilibrium is thus a stationarity condition, and the character of the stationary point decides whether the equilibrium can be observed at all.

Theorem 27.10 (Lagrange–Dirichlet).

If \(U\) has a strict local minimum at the equilibrium configuration \(q_{0}\), then \(q_{0}\) is stable: for every neighbourhood \(N\) of \(\left(q_{0},0\right)\) in the space of positions and velocities there is a smaller one from which the motion never leaves \(N\). Rests on Equation (27.9), Equation (19.21) and Theorem 21.43.

Proof.

Derives Theorem 27.10. Set \(U(q_{0})=0\) without loss of generality. The kinetic energy \(T\) of a system with time-independent constraints is a positive definite quadratic form in the generalized velocities (Definition 21.66), so \(T\geq0\) with equality only at rest, and the conserved energy \(E=T+U\) of Theorem 21.43 is a positive definite function of \(\left(q-q_{0},\dot q\right)\) near the equilibrium, because \(U\) has a strict minimum there. Given a neighbourhood \(N\), choose \(\varepsilon>0\) smaller than the least value of \(U\) on the boundary of a ball inside \(N\); then any motion starting with \(E<\varepsilon\) can never reach that boundary, since doing so would require \(U\geq\varepsilon\) and hence \(E\geq\varepsilon\). The set \(\set{E<\varepsilon}\) is the required smaller neighbourhood.

Example 27.11 (The ladder against a wall).

A uniform ladder of mass \(M=12.0\,\mathrm{kg}\) and length \(\ell=4.00\,\mathrm{m}\) leans at \(\vartheta=65.0\,^\circ\) to the horizontal, its top against a smooth vertical wall and its foot on a floor that can supply friction. Three unknown constraint forces act: the wall's normal \(N_{w}\) (horizontal), the floor's normal \(N_{f}\) (vertical) and the floor's friction \(f\) (horizontal). Taking torques about the foot, where two of the three act and contribute nothing,

\begin{equation}\tag{27.11} N_{w}\,\ell\sin\vartheta =Mg\,\frac{\ell}{2}\cos\vartheta \qquad\Longrightarrow\qquad N_{w}=\frac{Mg}{2\tan\vartheta}\ec \end{equation}

From Equations (27.3) and (27.6) (torques about the foot, the weight acting at the midpoint by Proposition 27.7). while Equation (27.2) resolved horizontally and vertically gives \(f=N_{w}\) and \(N_{f}=Mg\). With \(g=9.80665\,\mathrm{m}/\mathrm{s}^{2}\) the weight is \(Mg=117.7\,\mathrm{N}\), so \(N_{f}=117.7\,\mathrm{N}\) and \(N_{w}=f=27.4\,\mathrm{N}\). The ratio the floor is required to supply is

\begin{equation}\tag{27.12} \frac{f}{N_{f}}=\frac{1}{2\tan\vartheta}=0.233\ec \end{equation}

independent of both the mass and the length — which is why the question “will it slip?” is answered by the angle alone. Whether the floor can supply it is a question about the surfaces and not about mechanics: the usual empirical bound is \(f\leq\mu_{s}N_{f}\) with a coefficient \(\mu_{s}\) that for dry wood on concrete is quoted at a few tenths, comfortably above \(0.233\). This treatise carries no primary source for tabulated friction coefficients, and none of the mechanics above depends on one: \(\mu_{s}\) enters only as an inequality on a constraint force, never as a law of motion. Rests on Equation (27.2), Equation (27.3) and Proposition 27.7.

Remark 27.12 (Statically indeterminate systems).

Equations (27.2) and (27.3) provide six scalar equations in three dimensions, and a rigid body resting on three supports has exactly three unknown normal reactions: the problem closes. A body on four supports has four, and the equations no longer determine them — which is why a four-legged table rocks and a three-legged one never does. Nothing is wrong with the mechanics; the hypothesis of perfect rigidity has simply been pushed past what it can decide, and the missing equations come from the deformation of the body under load. They are supplied by the theory of elasticity, Continuum Mechanics and Elasticity, and the indeterminacy is resolved by the constitutive relation there rather than by any further principle of statics.

Central forces

Definition 27.13 (Central force).

A central force is an active force upon a particle that can be written in the form

\begin{equation}\tag{27.13} \vect{F}=f(r)\,\hat{\vect{r}}\ep \end{equation}

Rests on Definitions 19.30 and 21.15.

Definition 27.14 (Central motion).

A central motion is the motion of a particle due to a central force. Rests on Definition 27.13.

Everything in this section rests on one kinematic decomposition, which is worth isolating before it is used.

Lemma 27.15 (Velocity and acceleration in plane polar coordinates).

Let a particle move in a fixed plane, and write its position as \(\vect{x}=r\,\hat{\vect{r}}\) with \(\hat{\vect{r}}=\left(\cos\phi,\sin\phi\right)\) and \(\hat{\vect{\phi}}=\left(-\sin\phi,\cos\phi\right)\). Then

\begin{align} \dot{\hat{\vect{r}}}&=\dot{\phi}\,\hat{\vect{\phi}}\ec\qquad \dot{\hat{\vect{\phi}}}=-\dot{\phi}\,\hat{\vect{r}}\ec \tag{27.14}\\ \vect{v}&=\dot{r}\,\hat{\vect{r}} +r\dot{\phi}\,\hat{\vect{\phi}}\ec \tag{27.15}\\ \vect{a}&=\underbrace{\left(\ddot{r}-r\dot{\phi}^{2}\right)} _{\textstyle a_{r}}\hat{\vect{r}} +\underbrace{\left(r\ddot{\phi}+2\dot{r}\dot{\phi}\right)} _{\textstyle a_{\phi}}\hat{\vect{\phi}}\ep \tag{27.16} \end{align}

Rests on Definition 18.10, Definition 18.11 and Proposition 7.31.

Proof.

Derives Lemma 27.15. Differentiating the two unit vectors with respect to time by the chain rule (Proposition 7.31), \(\dot{\hat{\vect{r}}} =\dot{\phi}\left(-\sin\phi,\cos\phi\right) =\dot{\phi}\,\hat{\vect{\phi}}\) and \(\dot{\hat{\vect{\phi}}} =\dot{\phi}\left(-\cos\phi,-\sin\phi\right) =-\dot{\phi}\,\hat{\vect{r}}\), which is Equation (27.14). Then \(\vect{v}=\dv{}{t}\left(r\hat{\vect{r}}\right) =\dot{r}\hat{\vect{r}}+r\dot{\hat{\vect{r}}}\), giving Equation (27.15), and differentiating once more,

\[ \vect{a}=\ddot{r}\hat{\vect{r}}+\dot{r}\dot{\phi}\hat{\vect{\phi}} +\left(\dot{r}\dot{\phi}+r\ddot{\phi}\right)\hat{\vect{\phi}} +r\dot{\phi}\,\dot{\hat{\vect{\phi}}}\ec \]

which on substituting \(\dot{\hat{\vect{\phi}}}\) and collecting terms is Equation (27.16).

The two “extra” terms in Equation (27.16) are not forces. They are what the derivative of a moving orthonormal frame contributes, and the same quantities appear in Example 21.69 as Christoffel symbols of the plane in polar labelling: Equation (21.78), the free-particle equations there, are exactly \(a_{r}=0\) and \(a_{\phi}=0\). That the plane is flat while those symbols are non-zero is the point made in Remark 21.70.

Areal velocity

Definition 27.16 (Areal velocity).

The areal velocity is the rate of change of the area swept out by the line from the centre to the particle, with respect to an inertial frame of reference,

\begin{equation}\tag{27.17} v_a:=\dv{A}{t}\ep \end{equation}

Rests on Definitions 18.8 and 27.14.

Proposition 27.17 (Areal velocity in polar coordinates).

For a plane motion described in polar coordinates,

\begin{equation}\tag{27.18} v_a=\dv{A}{t}=\frac{1}{2}r^{2}\dot{\phi}\ec \end{equation}

and the transverse component of the acceleration is

\begin{equation}\tag{27.19} a_{\phi}=\frac{2}{r}\dv{v_a}{t}\ep \end{equation}

Rests on Equations (27.16) and (27.17).

Proof.

Derives Proposition 27.17. Between the times \(t\) and \(t+\dd t\) the radius turns through \(\dd\phi=\dot{\phi}\,\dd t\) and lengthens by \(\dd r=\dot{r}\,\dd t\). The region swept out contains the circular sector of radius \(r\) and angle \(\dd\phi\), and is contained in the sector of the same angle and radius \(r+\abs{\dd r}\); by the sector area recorded in Remark 27.1 these bound it as

\[ \frac{1}{2}r^{2}\,\dd\phi\leq\dd A \leq\frac{1}{2}\left(r+\abs{\dd r}\right)^{2}\dd\phi\ec \]

so the two differ by \(O\!\left(\dd t^{2}\right)\) and \(\dd A=\tfrac{1}{2}r^{2}\dd\phi+O\!\left(\dd t^{2}\right)\). Dividing by \(\dd t\) and letting \(\dd t\to0\) gives Equation (27.18). Differentiating that result,

\[ \dv{v_a}{t}=\frac{1}{2}\left(2r\dot{r}\dot{\phi} +r^{2}\ddot{\phi}\right) =\frac{r}{2}\left(2\dot{r}\dot{\phi}+r\ddot{\phi}\right) =\frac{r}{2}\,a_{\phi}\ec \]

by Equation (27.16), which rearranged is Equation (27.19).

Conservation laws of central motion

Proposition 27.18 (Conservation of angular momentum).

In a central motion the angular momentum \(\vect{L}\) is constant, the motion is confined to the fixed plane through the centre perpendicular to \(\vect{L}\), and in polar coordinates on that plane the angular momentum of the plane central motion has a component only along the \(z\)-axis, of magnitude

\begin{equation}\tag{27.20} L=m r^{2}\dot{\phi}\ep \end{equation}

Rests on Equations (19.14), (19.15) and (27.13).

Proof.

Derives Proposition 27.18. By Equation (19.14) the rate of change of the angular momentum is the torque, and by Equation (19.15) the torque is \(\vect{x}\times\vect{F}\). For a central force Equation (27.13) the force is parallel to \(\vect{x}=r\hat{\vect{r}}\), so

\begin{equation}\tag{27.21} \dv{\vect{L}}{t}=\vect{x}\times\vect{F} =r f(r)\,\hat{\vect{r}}\times\hat{\vect{r}}=\vect{0}\ec \end{equation}

and \(\vect{L}\) is a fixed vector. Since \(\vect{L}=\vect{x}\times m\vect{v}\) is orthogonal to \(\vect{x}\) by construction, the position stays in the fixed plane through the centre perpendicular to \(\vect{L}\); choosing Cartesian axes with \(\vect{L}\) along \(z\) makes that the \(xy\)-plane, so \(\vect{L}=L\hat{\vect{z}}\) with no other component. Finally, by Equation (27.15) the radial part of \(\vect{v}\) is parallel to \(\vect{x}\) and contributes nothing to the cross product, leaving \(\vect{L}=r\hat{\vect{r}}\times m r\dot{\phi}\hat{\vect{\phi}} =m r^{2}\dot{\phi}\,\hat{\vect{z}}\), which is Equation (27.20). The degenerate case \(\vect{L}=\vect{0}\) is the rectilinear motion through the centre; the plane is then not unique, and any plane containing the line will serve.

Phenomenon 27.19 (Kepler's second law: equal areas in equal times).

The line drawn from a planet to the Sun sweeps out equal areas in equal times: the planet runs fastest at perihelion and slowest at aphelion, in exactly the proportion that keeps the rate of sweeping constant. The regularity was extracted from Tycho Brahe's naked-eye positions of Mars and holds for every body bound to a centre — planets, comets, the components of a visual binary, a charged particle deflected by a nucleus. Newton showed that it holds if and only if the force is directed at the centre, and made it the first proposition of the Principia [Newton:1687]. Rests on Proposition 27.18 and Equation (27.18).

Derivation. Derives Phenomenon 27.19. By Proposition 27.18 the motion is plane and \(L=m r^{2}\dot{\phi}\) is constant. Comparing with the areal velocity Equation (27.18),

\begin{equation}\tag{27.22} v_a=\frac{1}{2}r^2\dot{\phi}=\frac{L}{2m}\ec \end{equation}

a constant — the equal-area law, and the relation Equation (27.27) read from left to right. Mark what the argument did not use: the form of \(f(r)\) never entered. Kepler's second law therefore tests the centrality of the force and nothing else, and would hold equally for an inverse-cube or a linear attraction.

The converse also holds, and is what makes the law evidence for anything. If \(v_{a}\) is constant then by Equation (27.19) the transverse acceleration \(a_{\phi}\) vanishes identically, so by Equation (19.4) the force has no transverse component and is central. Equal areas in equal times and centrality of the force are therefore the same statement.

Proposition 27.20 (Conservation of energy).

A central force is conservative: with

\begin{equation}\tag{27.23} V(r):=-\int_{r_{0}}^{r}f(s)\,\dd s \end{equation}

for any fixed \(r_{0}>0\), one has

\begin{equation}\tag{27.24} \vect{F}=-\vect{\nabla}V\ec \end{equation}

and consequently

\begin{equation}\tag{27.25} \vect{\nabla}\times\vect{F}=\vect{0}\ep \end{equation}

The energy \(E=T+V\) of a central motion is therefore constant. Rests on Equation (27.13), Equation (19.19) and Definition 19.31.

Proof.

Derives Proposition 27.20. The gradient of the radius is \(\vect{\nabla}r=\hat{\vect{r}}\), since \(r=\left(x^{2}+y^{2}+z^{2}\right)^{1/2}\) gives \(\pp r/\pp x^{i}=x^{i}/r\). Hence, by the chain rule (Proposition 7.72) and the fundamental theorem of calculus (Theorem 7.42) applied to Equation (27.23),

\[ -\vect{\nabla}V=-V'(r)\,\hat{\vect{r}}=f(r)\,\hat{\vect{r}} =\vect{F}\ec \]

which is Equation (27.24); Equation (27.25) then follows because the curl of a gradient vanishes, Equation (19.20). Note that no topological hypothesis was needed: the general criterion Proposition 7.104 requires a simply connected domain because it must reconstruct the potential from line integrals, whereas here Equation (27.23) writes it down.

For the conservation, differentiate \(E=\tfrac{1}{2}m\abs{\vect{v}}^{2} +V\) along the motion and use Equation (19.4) together with Equation (27.24):

\begin{equation}\tag{27.26} \dv{E}{t}=m\vect{v}\cdot\vect{a} +\vect{\nabla}V\cdot\vect{v} =\vect{v}\cdot\left(\vect{F}-\vect{F}\right)=0\ep \end{equation}

From Equations (19.4) and (27.24) (the chain rule on \(V(\vect{x}(t))\) and the second law on the kinetic term). Equivalently, the work Equation (19.25) done between two points depends only on the radii of the endpoints.

Proposition 27.21 (Conservation of the areal speed).

In a central motion the transverse component of the acceleration is zero, and the areal speed is therefore constant. Rests on Equations (27.13) and (27.19).

Proof.

Derives Proposition 27.21. A central force Equation (27.13) has no \(\hat{\vect{\phi}}\)-component, so by Equation (19.4) neither does the acceleration: \(a_{\phi}=0\). Equation (27.19) then gives \(\dd v_{a}/\dd t=\tfrac{1}{2}r\,a_{\phi}=0\). This is the same fact as Equation (27.22), obtained without passing through the angular momentum, and the equality of the two routes is Proposition 27.22.

Proposition 27.22 (Relation between the constants of the motion).

For a central motion one has

\begin{equation}\tag{27.27} r^{2}\dot{\phi}=\frac{L}{m}=2v_a\ep \end{equation}

Rests on Equations (27.18) and (27.20).

Proof.

Derives Proposition 27.22. The first equality is Equation (27.20) divided by \(m\), and the second is twice Equation (27.18). The content of the chain is that the two conserved quantities of the previous two propositions are not independent: the areal speed is the angular momentum per unit mass, halved. Kepler's second law and the conservation of angular momentum are one law counted twice, and the constant \(L/m\) is the one that appears in every formula below.

The Binet equation

Proposition 27.23 (Binet equation).

In a central motion, the trajectory equation can be found from the following equation:

\begin{equation}\tag{27.28} a_r=-\frac{L^2}{m^{2}r^{2}} \left(\frac{\dd^2}{\dd\phi^2}\left(\frac{1}{r}\right) +\frac{1}{r}\right)\ep \end{equation}

Rests on Equations (27.16) and (27.20).

Proof.

Derives Proposition 27.23. The device is to use \(\phi\) rather than \(t\) as the independent variable, which is legitimate whenever \(L\neq0\), since then \(\dot{\phi}=L/\left(mr^{2}\right)\) never vanishes and \(\phi\) is a strictly monotone function of \(t\). Write \(u:=1/r\), so that

\begin{equation}\tag{27.29} \dot{\phi}=\frac{L}{m r^{2}}=\frac{L u^{2}}{m}\ep \end{equation}

Then, by the chain rule (Proposition 7.31),

\[ \dot{r}=\dv{r}{\phi}\,\dot{\phi} =-\frac{1}{u^{2}}\dv{u}{\phi}\cdot\frac{Lu^{2}}{m} =-\frac{L}{m}\dv{u}{\phi}\ec \]

a first simplification worth noticing on its own: the radial velocity is \(-L/m\) times \(\dd u/\dd\phi\), with a constant factor. Differentiating once more in the same way,

\[ \ddot{r}=-\frac{L}{m}\frac{\dd^{2}u}{\dd\phi^{2}}\,\dot{\phi} =-\frac{L^{2}u^{2}}{m^{2}}\frac{\dd^{2}u}{\dd\phi^{2}}\ec \]

while the centrifugal term of Equation (27.16) is \(r\dot{\phi}^{2}=u^{-1}L^{2}u^{4}/m^{2}=L^{2}u^{3}/m^{2}\). Subtracting,

\begin{equation}\tag{27.30} a_{r}=\ddot{r}-r\dot{\phi}^{2} =-\frac{L^{2}u^{2}}{m^{2}} \left(\frac{\dd^{2}u}{\dd\phi^{2}}+u\right)\ec \end{equation}

From Equations (27.16) and (27.29) (eliminating \(t\) in favour of \(\phi\) through \(\dot\phi=Lu^{2}/m\) and writing \(u=1/r\)). which is Equation (27.28) with \(u\) restored to \(1/r\). Combined with \(m a_{r}=f(r)\) from Equation (19.4), it turns the dynamical problem into a single second-order equation for the shape of the orbit, with the time eliminated altogether.

The equivalent one-dimensional problem

Energy of the system

Proposition 27.24 (Radial form of the energy).

The energy of a particle in central motion is

\begin{equation}\tag{27.31} E=\frac{1}{2}m\dot{r}^2+\frac{L^2}{2mr^2}+V(r)\ep \end{equation}

Rests on Equations (27.15), (27.20) and (27.24).

Proof.

Derives Proposition 27.24. The motion is plane by Proposition 27.18, and the two terms of Equation (27.15) are orthogonal, so

\[ \abs{\vect{v}}^{2}=\dot{r}^{2}+r^{2}\dot{\phi}^{2} \]

and the kinetic energy Equation (19.18) splits into a radial and a transverse part, \(T=\tfrac{1}{2}m\dot{r}^{2}+\tfrac{1}{2}m r^{2}\dot{\phi}^{2}\). Eliminating \(\dot{\phi}\) with Equation (27.20),

\[ \frac{1}{2}mr^{2}\dot{\phi}^{2} =\frac{1}{2}mr^{2}\left(\frac{L}{mr^{2}}\right)^{2} =\frac{L^{2}}{2mr^{2}}\ec \]

which added to the radial part and to the potential Equation (27.24) gives Equation (27.31). The constancy of \(E\) is Proposition 27.20, and the constancy of \(L\) is what makes the middle term a function of \(r\) alone.

Effective potential

Definition 27.25 (Effective potential).

The effective potential of a central motion is

\begin{equation}\tag{27.32} V_{e}=\frac{L^2}{2mr^2}+V(r)\ec \end{equation}

so that the energy Equation (27.31) takes the one-dimensional form

\begin{equation}\tag{27.33} E=\frac{1}{2}m\dot{r}^2+V_{e}\ep \end{equation}

Rests on Equation (27.31).

The reduction is exact, not approximate, and it is the whole yield of the two conservation laws: a motion with three degrees of freedom has been replaced by a motion with one, at the cost of a term in the potential that carries the value of the eliminated angular momentum. The added term \(L^{2}/\left(2mr^{2}\right)\) is repulsive for every \(L\neq0\), and it is a piece of kinetic energy wearing the mask of a potential — which is why calling it a “centrifugal force” is harmless bookkeeping in the radial equation and false in any other.

Turning points

Considering the radial velocity obtained from Equation (27.33),

\begin{equation}\tag{27.34} \dot{r}=\pm\sqrt{\frac{2}{m}\left(E-V_{e}\right)}\ec \end{equation}

one must have

\begin{equation}\tag{27.35} E\geq V_{e}\ep \end{equation}

In the case in which \(E=V_{e}\), one has

\[ \dot{r}=0\implies r=R\ec \]

with \(R\) constant. Therefore a circular potential barrier of radius \(R\) is generated, called a turning point, which confines the motion.

Phenomenon 27.26 (Bound orbits oscillate between two radii).

A body bound to a centre does not spiral into it, however strong the attraction, unless its angular momentum is exactly zero: it approaches to a least distance, turns, and recedes to a greatest one, repeating the excursion indefinitely. Comets return; satellites in eccentric orbits alternate between perigee and apogee; a spacecraft aimed at a planet with any transverse velocity at all swings past it instead of falling in. What turns the body back is not an agency outside it but the angular momentum it already carries, and the same barrier explains why a star cannot collapse merely by attracting itself. Rests on Equations (27.32) and (27.33).

Derivation. Derives Phenomenon 27.26. By Equation (27.33) the radial coordinate obeys a one-dimensional energy equation, \(E=\tfrac{1}{2}m\dot{r}^2+V_{e}\), with the effective potential Equation (27.32). Since \(\tfrac{1}{2}m\dot{r}^2\geq0\), the motion is confined to the set where \(E\geq V_{e}(r)\), which is Equation (27.35), and the boundary points of that set, where \(E=V_{e}(R)\), are the turning radii at which \(\dot{r}\) vanishes and changes sign. Now suppose \(L\neq0\). The centrifugal term \(L^2/(2mr^2)\) grows like \(r^{-2}\) as \(r\to0\) and so dominates every attractive potential less singular than \(r^{-2}\) — the inverse-square attraction among them, whose potential goes only as \(r^{-1}\). Hence \(V_{e}\to+\infty\) at the centre, and the condition \(E\geq V_{e}\) excludes a whole neighbourhood of \(r=0\): the body cannot reach the centre at any finite energy. If instead \(L=0\) the centrifugal term is absent, \(V_{e}=V\), and nothing forbids the collision — which shows that the barrier is angular momentum and not force. For an attraction that vanishes at infinity, a state with \(E<0\) is trapped between an inner and an outer turning radius and the orbit is bounded; a state with \(E\geq0\) has only an inner one and the body escapes. That the bounded orbit should also close is a further and much stronger property, discussed in Phenomenon 27.32 and Theorem 27.41.

Example 27.27 (Escape from the Earth).

Take the Newtonian attraction \(V(r)=-GMm/r\), which vanishes at infinity, so that the criterion of the previous derivation reads \(E\geq0\) for escape. A body launched radially (\(L=0\)) from the surface \(r=R_{\oplus}\) with speed \(v\) has \(E=\tfrac{1}{2}mv^{2}-GMm/R_{\oplus}\), and escapes when

\begin{equation}\tag{27.36} v\geq v_{\mathrm{esc}}=\sqrt{\frac{2GM}{R_{\oplus}}}\ep \end{equation}

The product \(GM\) for the Earth is \(3.986\times 10^{14}\,\mathrm{m}^{3}/\mathrm{s}^{2}\), obtained from \(G=6.67430\times 10^{-11}\,\mathrm{m}^{3}/\mathrm{kg}/\mathrm{s}^{2}\) [Tiesinga:2021] and \(M=5.972\times 10^{24}\,\mathrm{kg}\); with \(R_{\oplus}=6.371\times 10^{6}\,\mathrm{m}\) this gives \(v_{\mathrm{esc}}=1.119\times 10^{4}\,\mathrm{m}/\mathrm{s}\), that is \(11.19\,\mathrm{km}/\mathrm{s}\). Two remarks are worth more than the number. First, the escape speed does not depend on the mass of the body or on the direction of launch — only on the sign of \(E\), which is why it is a speed and not a velocity. Second, what enters is the product \(GM\) and never the two factors separately, and that is not a notational accident: spacecraft ranging fixes \(GM\) for the Earth far more sharply than the laboratory knows \(G\), whose relative uncertainty is \(2.2\times10^{-5}\) (Phenomenon 33.16). The mass of the Earth is therefore obtained as \(GM/G\) and inherits that uncertainty entire; it is the least well known of the three quantities in Equation (27.36), and celestial mechanics never measures it at all. Rests on Equations (27.31) and (27.35).

The radial quadrature

The one-dimensional problem can be integrated once and for all, which is what makes it worth constructing.

Proposition 27.28 (Quadratures of the central problem).

For a central motion with \(L\neq0\), the time along the orbit and the shape of the orbit are given by

\begin{align} t-t_{0}&=\int_{r_{0}}^{r} \frac{\dd s}{\sqrt{\dfrac{2}{m}\left(E-V_{e}(s)\right)}}\ec \tag{27.37}\\ \phi-\phi_{0}&=\int_{r_{0}}^{r} \frac{L\,\dd s}{s^{2}\sqrt{2m\left(E-V(s)\right) -\dfrac{L^{2}}{s^{2}}}}\ec \tag{27.38} \end{align}

on any interval between successive turning points, the sign of the root being that of \(\dot{r}\) there. Rests on Equations (27.20) and (27.34).

Proof.

Derives Proposition 27.28. Equation (27.34) is a separable first-order equation for \(r(t)\): dividing by the root and integrating gives Equation (27.37), which is legitimate on any interval where \(E>V_{e}\), that is strictly between turning points, since there the integrand is continuous. For the orbit, divide \(\dd\phi=\dot{\phi}\,\dd t\) by \(\dd r=\dot{r}\,\dd t\) and use Equation (27.20) and Equation (27.34):

\[ \dv{\phi}{r}=\frac{\dot{\phi}}{\dot{r}} =\frac{L/\left(mr^{2}\right)} {\sqrt{\left(2/m\right)\left(E-V_{e}\right)}} =\frac{L}{r^{2}\sqrt{2m\left(E-V\right)-L^{2}/r^{2}}}\ec \]

where the last step multiplied numerator and denominator by \(m\) and used Equation (27.32). Integrating gives Equation (27.38).

Definition 27.29 (Apsidal angle).

For a bounded orbit with turning radii \(r_{-}<r_{+}\), the apsidal angle is the angle swept between successive turning points,

\begin{equation}\tag{27.39} \Phi=\int_{r_{-}}^{r_{+}} \frac{L\,\dd s}{s^{2}\sqrt{2m\left(E-V(s)\right) -\dfrac{L^{2}}{s^{2}}}}\ep \end{equation}

The orbit closes after \(p\) radial oscillations and \(q\) revolutions if and only if \(2\Phi=2\pi q/p\) with \(p,q\) integers — that is, if and only if \(\Phi/\pi\) is rational. Rests on Equation (27.38).

The radial motion is always periodic for a bounded orbit, since \(r\) returns to \(r_{-}\) after each excursion; what is not automatic is that the angle should also return. The orbit closes only when the two periods are commensurable, and \(\Phi\) generically depends on \(E\) and \(L\), so that a family of orbits under one and the same force law will in general contain no closed orbit at all. Two force laws are the exception, and the fact that Nature's dominant one is among them is the subject of Section 27.4.5.

The two-body problem and Kepler orbits

Nothing so far has asked what holds the centre of force in place. In the Solar System nothing does: the Sun is attracted by each planet exactly as strongly as it attracts it, by Postulate 19.48, and moves in response. The first business of this section is to show that the two-body problem is nevertheless exactly equivalent to a one-body central problem of the kind already solved — not approximately, and not only when one mass is large.

Reduction to one body

Theorem 27.30 (Reduction of the two-body problem).

Let two particles of masses \(m_{1},m_{2}\) interact through a force that depends only on their separation and acts along the line joining them,

\begin{equation}\tag{27.40} \vect{F}_{12}=f(r)\,\hat{\vect{r}}=-\vect{F}_{21}\ec\qquad \vect{x}:=\vect{x}_{1}-\vect{x}_{2}\ec\quad r=\abs{\vect{x}}\ep \end{equation}

Then the centre of mass moves uniformly, and the relative coordinate \(\vect{x}\) obeys the one-body central equation

\begin{equation}\tag{27.41} \mu\,\ddot{\vect{x}}=f(r)\,\hat{\vect{r}}\ec\qquad \mu:=\frac{m_{1}m_{2}}{m_{1}+m_{2}}\ec \end{equation}

with \(\mu\) the reduced mass. Moreover the total kinetic energy and the total angular momentum split without cross terms,

\begin{align} T&=\frac{1}{2}\left(m_{1}+m_{2}\right)\abs{\dot{\vect{X}}}^{2} +\frac{1}{2}\mu\abs{\dot{\vect{x}}}^{2}\ec \tag{27.42}\\ \vect{L}&=\left(m_{1}+m_{2}\right)\vect{X}\times\dot{\vect{X}} +\mu\,\vect{x}\times\dot{\vect{x}}\ec \tag{27.43} \end{align}

with \(\vect{X}\) the centre of mass Equation (19.38). Rests on Postulate 19.48, Equation (19.38) and Equation (19.4).

Proof.

Derives Theorem 27.30. Adding the two equations of motion and using Equation (27.40) gives \(m_{1}\ddot{\vect{x}}_{1}+m_{2}\ddot{\vect{x}}_{2}=\vect{0}\), that is \(\ddot{\vect{X}}=\vect{0}\) by Equation (19.40): the centre of mass moves uniformly, as Phenomenon 19.54 states in general. Subtracting instead, after dividing each equation by its own mass,

\begin{equation}\tag{27.44} \ddot{\vect{x}}=\ddot{\vect{x}}_{1}-\ddot{\vect{x}}_{2} =\frac{\vect{F}_{12}}{m_{1}}-\frac{\vect{F}_{21}}{m_{2}} =\left(\frac{1}{m_{1}}+\frac{1}{m_{2}}\right)f(r)\,\hat{\vect{r}} =\frac{f(r)}{\mu}\,\hat{\vect{r}}\ec \end{equation}

From Equations (19.4) and (27.40) (dividing each equation of motion by its mass and subtracting, with \(\mu^{-1}=m_{1}^{-1}+m_{2}^{-1}\)). which is Equation (27.41). For the splittings, invert the change of variables: with \(M=m_{1}+m_{2}\),

\[ \vect{x}_{1}=\vect{X}+\frac{m_{2}}{M}\vect{x}\ec\qquad \vect{x}_{2}=\vect{X}-\frac{m_{1}}{M}\vect{x}\ep \]

Substituting into \(T=\tfrac{1}{2}m_{1}\abs{\dot{\vect{x}}_{1}}^{2} +\tfrac{1}{2}m_{2}\abs{\dot{\vect{x}}_{2}}^{2}\), the cross terms carry the factor \(m_{1}m_{2}/M-m_{2}m_{1}/M=0\) and cancel, while the remaining coefficients of \(\abs{\dot{\vect{x}}}^{2}\) combine to \(\tfrac{1}{2}\left(m_{1}m_{2}^{2}+m_{2}m_{1}^{2}\right)/M^{2} =\tfrac{1}{2}\mu\), giving Equation (27.42). The same substitution in \(\vect{L}=m_{1}\vect{x}_{1}\times\dot{\vect{x}}_{1} +m_{2}\vect{x}_{2}\times\dot{\vect{x}}_{2}\) cancels the cross terms for the same reason and gives Equation (27.43).

Remark 27.31 (What the reduction does and does not buy).

Every result of Sections 27.2 and 27.3 now applies to the two-body problem verbatim, with \(m\) read as the reduced mass \(\mu\), \(r\) as the separation and \(\vect{L}\) as the angular momentum about the centre of mass. When one mass overwhelms the other, \(\mu\to m_{2}\) for \(m_{1}\gg m_{2}\) and the centre of mass sits inside the heavy body, which recovers the fixed-centre picture; for the Sun and Jupiter \(\mu\) differs from Jupiter's mass by one part in \(1047\), and the common centre of mass lies just outside the solar surface. The reduction is exact for two bodies and for no more: the three-body problem admits no such change of variables, has no general solution in closed form, and is where the qualitative theory of Nonlinear Dynamics and Chaos begins.

The orbit of an inverse-square attraction

Phenomenon 27.32 (Kepler's first law: bound orbits are closed ellipses).

Each planet describes an ellipse with the Sun at one focus — not at the centre — and the orbit closes upon itself, returning the body to the same point with the same velocity after one revolution. Closure is a strong and very special fact. For a general central force the orbit is bounded, by Phenomenon 27.26, but it does not repeat: successive perihelia occur at different longitudes and the path fills the annulus between the turning radii. The observed closure of planetary orbits is therefore evidence for the inverse-square law itself, and the small residual advances of the perihelia are evidence that the law is not exact [Newton:1687]. Rests on Equation (27.28), Equation (27.13) and Theorem 27.30.

Derivation. Derives Phenomenon 27.32. Take the Newtonian attraction between the two bodies,

\begin{equation}\tag{27.45} f(r)=-\frac{k}{r^{2}}\ec\qquad k:=Gm_{1}m_{2}>0\ec \end{equation}

whose potential Equation (27.23) is \(V(r)=-k/r\) once the additive constant is fixed by requiring \(V\to0\) as \(r\to\infty\), and which by Theorem 27.30 makes the separation obey the one-body central equation with mass \(\mu\). Insert Equation (27.45) into the Binet equation Equation (27.30), written with \(\mu\) in place of \(m\) and \(u=1/r\), using \(\mu a_{r}=f=-ku^{2}\):

\[ -k u^{2} =-\frac{L^{2}u^{2}}{\mu} \left(\frac{\dd^{2}u}{\dd\phi^{2}}+u\right)\ec \]

and the factor \(u^{2}\) cancels on both sides — which happens for the inverse square and for no other power. What is left is linear with constant coefficients,

\begin{equation}\tag{27.46} \frac{\dd^{2}u}{\dd\phi^{2}}+u=\frac{\mu k}{L^{2}}\ep \end{equation}

From Equations (27.30) and (27.45) (substituting \(f=-ku^{2}\) and cancelling the common factor \(u^{2}\)). By Theorem 9.13 its general solution is any one solution plus the general solution of the homogeneous equation; the constant \(u=\mu k/L^{2}\) is a solution, and the homogeneous equation is Equation (9.106) with \(\lambda=1\), whose real general solution is Equation (9.108). Choosing the origin of \(\phi\) at the maximum of \(u\) — the point of closest approach — absorbs the phase, and writing the remaining constant as \(e\,\mu k/L^{2}\) with \(e\geq0\),

\begin{equation}\tag{27.47} \frac{1}{r}=\frac{\mu k}{L^{2}} \left(1+e\cos\phi\right)\ec\qquad\text{that is}\qquad r=\frac{p}{1+e\cos\phi}\ec\quad p:=\frac{L^{2}}{\mu k}\ep \end{equation}

This is the polar equation of a conic of eccentricity \(e\) with one focus at the centre of force and semi-latus rectum \(p\) (Remark 27.33); for \(0\leq e<1\) it is an ellipse, and the centre of force is at a focus and not at the centre, since \(r\) takes its extreme values \(p/(1+e)\) and \(p/(1-e)\) at \(\phi=0\) and \(\phi=\pi\) and these are unequal unless \(e=0\). The solution is single-valued and \(2\pi\)-periodic in \(\phi\), so the orbit closes exactly, and the identification of \(e\) with the energy is Proposition 27.34.

Remark 27.33 (The conic classification is owed by Part~II).

Equation (27.47) is derived here in full; what is quoted is its geometric reading. That \(r=p/\left(1+e\cos\phi\right)\) is the locus of points whose distance from a fixed focus stands in the fixed ratio \(e\) to the distance from a fixed directrix, and that this locus is an ellipse, a parabola or a hyperbola according as \(e<1\), \(e=1\) or \(e>1\), is elementary analytic geometry which Linear Algebra and Representation Theory and Real Analysis do not state. Nothing in the physics below depends on it: the semi-major axis is defined in Equation (27.49) as half the sum of the two turning radii, which is intrinsic to the orbit, and Kepler's third law is derived from Equation (27.47) directly without any appeal to the geometry of the ellipse. The word “ellipse” is a name for the curve, not a step in an argument.

Proposition 27.34 (Eccentricity, energy and semi-major axis).

For the orbit Equation (27.47) of the attraction Equation (27.45),

\begin{equation}\tag{27.48} e=\sqrt{1+\frac{2EL^{2}}{\mu k^{2}}}\ec \end{equation}

and, when \(e<1\), half the sum of the two turning radii is

\begin{equation}\tag{27.49} a:=\frac{r_{-}+r_{+}}{2}=\frac{p}{1-e^{2}}=-\frac{k}{2E}\ep \end{equation}

Rests on Equations (27.31), (27.32) and (27.47).

Proof.

Derives Proposition 27.34. At a turning point \(\dot{r}=0\), so by Equation (27.31) with \(V=-k/r=-ku\) and \(\mu\) for \(m\),

\begin{equation}\tag{27.50} E=\frac{L^{2}}{2\mu}u^{2}-k u\ep \end{equation}

The turning values of \(u\) are the extremes of Equation (27.47), namely \(u_{\pm}=\left(\mu k/L^{2}\right)\left(1\pm e\right)\). Substituting \(u_{+}\) into Equation (27.50) and using \(p=L^{2}/\left(\mu k\right)\),

\[ E=\frac{L^{2}}{2\mu}\frac{\mu^{2}k^{2}}{L^{4}}\left(1+e\right)^{2} -k\frac{\mu k}{L^{2}}\left(1+e\right) =\frac{\mu k^{2}}{2L^{2}}\left(1+e\right) \left[\left(1+e\right)-2\right] =\frac{\mu k^{2}}{2L^{2}}\left(e^{2}-1\right)\ec \]

and solving for \(e\) gives Equation (27.48); the same substitution with \(u_{-}\) gives the same relation, as it must, since both turning points belong to one orbit. For Equation (27.49), \(r_{\pm}=p/\left(1\mp e\right)\) so

\[ a=\frac{p}{2}\left(\frac{1}{1+e}+\frac{1}{1-e}\right) =\frac{p}{1-e^{2}}\ec \]

and inserting \(1-e^{2}=-2EL^{2}/\left(\mu k^{2}\right)\) from Equation (27.48) together with \(p=L^{2}/\left(\mu k\right)\) gives \(a=-k/(2E)\), positive precisely when \(E<0\).

Equation (27.48) classifies the orbits completely by the two constants of the motion, and the classification is collected in Table 27.1. It is worth reading as a statement about what is observable: the energy fixes the size of a bound orbit through Equation (27.49) and the angular momentum fixes its shape through \(p\), so that measuring the period and the eccentricity of a planet measures \(E\) and \(L\) and nothing else is left to determine.

EnergyEccentricityCurveMotion
$E=-\mu k^{2}/\left(2L^{2}\right)$$e=0$circle$r$ constant
$-\mu k^{2}/\left(2L^{2}\right)<E<0$$0<e<1$ellipsebounded, closed
$E=0$$e=1$parabolaescapes with zero final speed
$E>0$$e>1$hyperbolaescapes with finite final speed
Classification of the orbits of the inverse-square attraction Equation (27.45) by the energy, through the eccentricity Equation (27.48). The least possible energy $-\mu k^{2}/\left(2L^{2}\right)$ is the minimum of the effective potential Equation (27.32) at fixed $L$; below it no motion exists with that angular momentum. Only the first two rows are bounded, and both close.

Kepler's third law

Phenomenon 27.35 (Kepler's third law).

The squares of the orbital periods of the planets stand in the same ratio as the cubes of the semi-major axes of their orbits, with one and the same constant of proportionality for every body bound to the same centre, whatever its own mass. The regularity holds across the Solar System over a range of nearly three orders of magnitude in period, and holds again — with a different constant — for the moons of Jupiter, for artificial satellites of the Earth, and for the components of binary stars. It is by this law that the masses of astronomical bodies are determined at all [Newton:1687]. Rests on Equation (27.47), Equation (27.22) and Theorem 27.30.

Derivation. Derives Phenomenon 27.35. For a circular orbit the result is immediate. A body of mass \(m\) carried around a circle of radius \(r\) requires, by the kinematics of Kinematics, the centripetal acceleration \(\omega^2 r\), and the attraction of a central mass \(M\) supplies it, so that \(GM/r^{2}=\omega^{2}r\) and, with \(\omega=2\pi/T\),

\begin{equation}\tag{27.51} T^2=\frac{4\pi^2}{GM}\,r^3\ep \end{equation}

The orbiting mass has cancelled — it appears once as the gravitational charge and once as the inertia — which is why a single constant serves every planet.

For the general bounded orbit, integrate the equal-area law. By Equation (27.22) the areal speed is \(L/\left(2\mu\right)\), and by Equation (27.20) the period is

\[ T=\int_{0}^{T}\dd t=\int_{0}^{2\pi}\frac{\dd\phi}{\dot{\phi}} =\frac{\mu}{L}\int_{0}^{2\pi}r^{2}\,\dd\phi =\frac{\mu p^{2}}{L} \int_{0}^{2\pi}\frac{\dd\phi}{\left(1+e\cos\phi\right)^{2}}\ec \]

using Equation (27.47) in the last step. The integral is elementary by residues. For \(0<e<\lambda\) the substitution \(z=\ee^{\ii\phi}\), under which \(\cos\phi=\left(z+z^{-1}\right)/2\) and \(\dd\phi=\dd z/\left(\ii z\right)\), turns \(I(\lambda)=\int_{0}^{2\pi}\left(\lambda+e\cos\phi\right)^{-1}\dd\phi\) into a contour integral on the unit circle,

\[ I(\lambda)=\oint_{\abs{z}=1} \frac{2\,\dd z}{\ii\left(ez^{2}+2\lambda z+e\right)}\ec \]

whose two poles have product \(1\), so that exactly one lies inside, namely \(z_{+}=\left(-\lambda+\sqrt{\lambda^{2}-e^{2}}\right)/e\); by the residue theorem Theorem 8.24 and Proposition 8.23, \(I(\lambda)=2\pi/\sqrt{\lambda^{2}-e^{2}}\), which is also the value at \(e=0\), where the integral is immediate. Differentiating under the integral sign in \(\lambda\) and then setting \(\lambda=1\),

\begin{equation}\tag{27.52} \int_{0}^{2\pi}\frac{\dd\phi}{\left(1+e\cos\phi\right)^{2}} =-I'(1)=\frac{2\pi}{\left(1-e^{2}\right)^{3/2}}\ep \end{equation}

Hence, with \(a=p/\left(1-e^{2}\right)\) from Equation (27.49) and \(p=L^{2}/\left(\mu k\right)\),

\[ T=\frac{2\pi\mu p^{2}}{L\left(1-e^{2}\right)^{3/2}} =\frac{2\pi\mu}{L}\,p^{1/2}a^{3/2} =\frac{2\pi\mu}{L}\cdot\frac{L}{\sqrt{\mu k}}\,a^{3/2} =2\pi\sqrt{\frac{\mu}{k}}\;a^{3/2}\ep \]

Squaring, and putting \(k=Gm_{1}m_{2}\) and \(\mu=m_{1}m_{2}/\left(m_{1}+m_{2}\right)\) from Theorem 27.30,

\begin{equation}\tag{27.53} T^{2}=\frac{4\pi^{2}}{G\left(m_{1}+m_{2}\right)}\,a^{3}\ep \end{equation}

From Equations (27.41), (27.49) and (27.52) (integrating the equal-area law over one revolution and eliminating \(p\) and \(L\)). This is the exact law. It contains Equation (27.51) as the limit \(m_{2}\ll m_{1}\), it replaces the radius by the semi-major axis, and it shows precisely how the “constant” fails to be one: the proportionality factor depends on the total mass, so two planets of different masses about the same star obey slightly different laws. The check of Equation (33.19) in the Cavendish chapter is this same relation applied to the Moon.

Body$a$ (\(\mathrm{m}\))$T$ (\(\mathrm{s}\))$T^{2}/a^{3}$ (\(\mathrm{s}^{2}/\mathrm{m}^{3}\))
Mercury\(5.7909\times 10^{10}\)\(7.6005\times 10^{6}\)\(2.97473\times 10^{-19}\)
Venus\(1.0821\times 10^{11}\)\(1.9414\times 10^{7}\)\(2.97473\times 10^{-19}\)
Earth\(1.4960\times 10^{11}\)\(3.1558\times 10^{7}\)\(2.97472\times 10^{-19}\)
Mars\(2.2794\times 10^{11}\)\(5.9355\times 10^{7}\)\(2.97490\times 10^{-19}\)
Jupiter\(7.7841\times 10^{11}\)\(3.7436\times 10^{8}\)\(2.97126\times 10^{-19}\)
Saturn\(1.4267\times 10^{12}\)\(9.2929\times 10^{8}\)\(2.97361\times 10^{-19}\)
Uranus\(2.8710\times 10^{12}\)\(2.6514\times 10^{9}\)\(2.97067\times 10^{-19}\)
Neptune\(4.4983\times 10^{12}\)\(5.2004\times 10^{9}\)\(2.97129\times 10^{-19}\)
Kepler's third law across the Solar System. The semi-major axes and sidereal periods are the standard J2000 mean Keplerian elements, converted to SI; the last column is the ratio that Equation (27.53) predicts to be $4\pi^{2}/\left[G\left(M_{\odot}+m\right)\right]$, which for a massless planet is \(2.9747\times 10^{-19}\,\mathrm{s}^{2}/\mathrm{m}^{3}\) with $GM_{\odot}=1.32712\times 10^{20}\,\mathrm{m}^{3}/\mathrm{s}^{2}$. This treatise carries no citable ephemeris source, and the elements below are therefore uncited.

Table 27.2 is the law's evidence and also the measure of its limits. Over a \(684\)-fold range in period and a \(78\)-fold range in semi-major axis the ratio \(T^{2}a^{-3}\) is constant to \(0.14\,\mathrm{\%}\), which is the observation Kepler made and Newton explained. The residual structure is not noise. The four terrestrial planets agree with each other and with \(4\pi^{2}/\left(GM_{\odot}\right)\) to a few parts in \(10^{5}\); the giant planets lie systematically below that value, which is the sign Equation (27.53) demands, since their own masses enter the denominator. For Jupiter, \(m/M_{\odot}=9.5\times 10^{-4}\) predicts a deficit of that relative size and one of about \(1.2\times 10^{-3}\) is observed; for Saturn, \(2.9\times 10^{-4}\) predicted against \(3.8\times 10^{-4}\) observed. Uranus and Neptune depart by more than their masses require, and the honest reading is that a two-body law is not expected to describe them to better than this: their mutual perturbation is large enough to have betrayed Neptune's existence before it was seen, and the mean elements quoted are themselves fits over a span of centuries rather than exact constants of any orbit.

Example 27.36 (A satellite in low Earth orbit).

Equation (27.53) with \(m_{2}\ll m_{1}\) gives the period of a circular orbit of radius \(r\) about the Earth as \(T=2\pi\sqrt{r^{3}/GM}\). Taking \(GM=3.986\times 10^{14}\,\mathrm{m}^{3}/\mathrm{s}^{2}\) as in Example 27.27, and an orbit \(4.20\times 10^{5}\,\mathrm{m}\) above the mean radius \(R_{\oplus}=6.371\times 10^{6}\,\mathrm{m}\), so that \(r=6.791\times 10^{6}\,\mathrm{m}\):

\[ T=2\pi\sqrt{\frac{\left(6.791\times 10^{6}\,\mathrm{m}\right)^{3}} {3.986\times 10^{14}\,\mathrm{m}^{3}/\mathrm{s}^{2}}} =5.57\times 10^{3}\,\mathrm{s}\ec \]

that is \(92.8\) minutes, against the \(92.9\) minutes in which the International Space Station is observed to circle at that altitude. The orbital speed is \(\sqrt{GM/r}=7.66\times 10^{3}\,\mathrm{m}/\mathrm{s}\). Note that the period decreases as the orbit is lowered, so that a satellite which loses energy to atmospheric drag speeds up — the characteristic and initially counter-intuitive signature of a bound inverse-square orbit, and a direct consequence of Equation (27.49), in which a more negative energy means a smaller \(a\). Rests on Equation (27.53).

The Laplace–Runge–Lenz vector

The inverse-square attraction conserves more than energy and angular momentum. It conserves a vector lying in the plane of the orbit, and that extra conservation law is exactly what makes the orbit close.

Definition 27.37 (Laplace–Runge–Lenz vector).

For the attraction Equation (27.45), with \(\vect{p}=\mu\dot{\vect{x}}\) the momentum conjugate to the relative coordinate, the Laplace–Runge–Lenz vector is

\begin{equation}\tag{27.54} \vect{A}:=\vect{p}\times\vect{L}-\mu k\,\hat{\vect{r}}\ec \end{equation}

whose SI unit is \(\mathrm{kg}^{2}\,\mathrm{m}^{3}/\mathrm{s}^{2}\), that of a momentum times an angular momentum. Rests on Equations (27.20), (27.41) and (27.45).

Theorem 27.38 (Conservation of the Laplace–Runge–Lenz vector).

Along any motion of the inverse-square attraction, \(\dd\vect{A}/\dd t=\vect{0}\). The vector lies in the plane of the orbit, since \(\vect{A}\cdot\vect{L}=0\). Rests on Equations (27.1), (27.41) and (27.54).

Proof.

Derives Theorem 27.38. Differentiate Equation (27.54). Since \(\vect{L}\) is constant by Proposition 27.18, \(\dd\left(\vect{p}\times\vect{L}\right)/\dd t =\dot{\vect{p}}\times\vect{L}=\vect{F}\times\vect{L}\) by Equation (27.41). With \(\vect{F}=-k\hat{\vect{r}}/r^{2}\) and \(\vect{L}=\mu\,\vect{x}\times\vect{v}\), the expansion Equation (27.1) of the double cross product gives

\[ \vect{F}\times\vect{L} =-\frac{k\mu}{r^{2}}\, \hat{\vect{r}}\times\left(\vect{x}\times\vect{v}\right) =-\frac{k\mu}{r^{2}} \left[\vect{x}\left(\hat{\vect{r}}\cdot\vect{v}\right) -\vect{v}\left(\hat{\vect{r}}\cdot\vect{x}\right)\right] =k\mu\left(\frac{\vect{v}}{r} -\frac{\dot{r}\,\vect{x}}{r^{2}}\right)\ec \]

using \(\hat{\vect{r}}\cdot\vect{v}=\dot{r}\) and \(\hat{\vect{r}}\cdot\vect{x}=r\). What multiplies \(k\mu\) on the right is exactly the derivative of the unit radial vector,

\[ \dv{\hat{\vect{r}}}{t}=\dv{}{t}\left(\frac{\vect{x}}{r}\right) =\frac{\vect{v}}{r}-\frac{\dot{r}\,\vect{x}}{r^{2}}\ec \]

so \(\dd\left(\vect{p}\times\vect{L}\right)/\dd t =\mu k\,\dd\hat{\vect{r}}/\dd t\) and the two terms of Equation (27.54) cancel in the derivative. Finally \(\vect{A}\cdot\vect{L} =\left(\vect{p}\times\vect{L}\right)\cdot\vect{L} -\mu k\,\hat{\vect{r}}\cdot\vect{L}=0\), the first term because \(\vect{p}\times\vect{L}\) is orthogonal to \(\vect{L}\) and the second because \(\vect{L}\) is orthogonal to \(\vect{x}\).

Proposition 27.39 (The Laplace–Runge–Lenz vector is the orbit).

Measuring \(\phi\) from the direction of \(\vect{A}\),

\begin{equation}\tag{27.55} r=\frac{L^{2}/\left(\mu k\right)} {1+\left(A/\mu k\right)\cos\phi}\ec\qquad A^{2}=\mu^{2}k^{2}+2\mu EL^{2}\ep \end{equation}

Thus \(\vect{A}\) points from the centre of force towards the point of closest approach, and its magnitude is \(\mu k e\) with \(e\) the eccentricity Equation (27.48). Rests on Equations (27.47), (27.48) and (27.54).

Proof.

Derives Proposition 27.39. Take the scalar product of Equation (27.54) with \(\vect{x}\). On the left, \(\vect{x}\cdot\vect{A}=Ar\cos\phi\) with \(\phi\) measured from \(\vect{A}\). On the right, the cyclic property of the scalar triple product gives \(\vect{x}\cdot\left(\vect{p}\times\vect{L}\right) =\vect{L}\cdot\left(\vect{x}\times\vect{p}\right)=L^{2}\), while \(\vect{x}\cdot\mu k\hat{\vect{r}}=\mu k r\). Hence \(Ar\cos\phi=L^{2}-\mu k r\), which rearranged is the first member of Equation (27.55). Comparing with Equation (27.47) identifies \(A=\mu k e\), and substituting Equation (27.48) gives \(A^{2}=\mu^{2}k^{2}e^{2}=\mu^{2}k^{2}+2\mu EL^{2}\). Since \(r\) is least where \(\cos\phi=1\), the vector points at the perihelion.

That the perihelion direction is a constant of the motion is another way of saying that the orbit does not precess, and it is the sharpest statement of Kepler's first law: the extra conserved vector is what distinguishes the inverse-square attraction from every other central force, all of which conserve \(E\) and \(\vect{L}\) just as well.

Remark 27.40 (It is not the charge of a point symmetry).

It is tempting to look for the symmetry behind Theorem 27.38 among the transformations that move the particle's position, as rotations and translations do. There is none, and Remark 16.86 proves it: the part of the Noether charge Equation (16.76) that is quadratic in the momentum is isotropic in \(\vect{p}\) for any point transformation, whereas the corresponding part of \(\vect{A}\) is not — it vanishes when \(\vect{p}\) is parallel to \(\vect{x}\) and is maximal when they are perpendicular. The generator that does produce \(\vect{A}\) depends on the velocities and is a generalized symmetry, outside the hypotheses of Noether's first theorem as proved in Theorem 16.84. So Theorem 27.38 is established here, as it must be, by direct differentiation and not by exhibiting a symmetry of the action. The hidden \(\SO(4)\) structure the vector generates is not idle, however: it is what makes the hydrogen spectrum degenerate in the orbital angular momentum, and it is put to work in The Hydrogen Atom. The vector is far older than its three-barrelled name; what attached Lenz's to it is his use of it in the old quantum theory of the perturbed Kepler motion [Lenz:1924], and Pauli obtained the hydrogen spectrum from it two years later, before Schrödinger's wave equation appeared [Pauli:1926].

Closure, and what its failure measures

Theorem 27.41 (Bertrand).

Among the central forces for which every bounded orbit is closed there are exactly two: the inverse-square attraction \(f(r)=-k/r^{2}\) and the linear attraction \(f(r)=-\kappa r\) of the isotropic harmonic oscillator. For every other force law the apsidal angle Equation (27.39) depends on the orbit, and orbits with \(\Phi/\pi\) irrational fill the annulus between their turning radii without ever repeating. Rests on Equations (27.39) and (27.47).

Derives Theorem 27.41.

The proof there runs in two stages, and it is worth knowing which does which. The first perturbs a circular orbit of radius \(r_{0}\) and finds that the perturbation oscillates about it with an angular frequency \(\beta(r_{0})=\bigl[3+r_{0}f'(r_{0})/f(r_{0})\bigr]^{1/2}\) per unit change of the polar angle, so that the apsidal angle Equation (27.39) tends to \(\pi/\beta\). Closure of every nearby orbit makes \(\beta\) rational; \(\beta\) depends continuously on \(r_{0}\) and a continuous rational-valued function is constant, so \(\beta\) is one fixed rational number, and \(r f'/f=\beta^{2}-3\) integrates to the power law \(f\propto r^{\beta^{2}-3}\). That much is a first-order calculation, and it narrows the candidates to a one-parameter family of power laws — it does not yet pick out two of them. The second stage supplies the difference, because closure of the orbits infinitesimally near the circle is weaker than closure of all bounded orbits: carrying the expansion to third order produces a solvability condition on \(\beta\) which only \(\beta=1\) and \(\beta=2\) satisfy, and those are \(f\propto r^{-2}\) and \(f\propto r\).

The two exceptional laws are also the two that Nature exhibits at large scale, which is why the closure of orbits was discovered before the reason for it. The importance of the theorem is that it converts a qualitative observation into a quantitative test: any departure from \(r^{-2}\), however small, makes the perihelion move.

Phenomenon 27.42 (Planetary orbits do not close exactly).

The perihelia of the planets advance slowly along their orbits. Mercury's is observed to advance by some \(5600\) seconds of arc per century, of which \(5025\) is the general precession of the equinoxes — a motion of the reference frame and not of the orbit — and \(531\) is the pull of the other planets, computable within Newtonian mechanics. A residue of about \(43\) seconds of arc per century survives every such computation. Le Verrier isolated that residue in 1859 and no distribution of matter consistent with the rest of Solar-System astronomy was ever found to produce it [LeVerrier:1859]; the budget is set out in Table 53.1. By Theorem 27.41 the residue is a measurement: it says that the force governing Mercury is not exactly \(-k/r^{2}\). Rests on Theorem 27.41 and Equation (27.39).

Derivation. Derives Phenomenon 27.42. Within this chapter the derivation can go only as far as the conditional statement, and that is the honest content of the phenomenon. Theorem 27.41 shows that closure of every bounded orbit is equivalent to the force being \(-k/r^{2}\) or \(-\kappa r\), and the second is excluded by Phenomenon 27.32, since a linear attraction puts the centre of force at the centre of the ellipse and not at a focus. A non-closing bound orbit therefore falsifies the exact inverse square. What it does not do is say what replaces it. The first attempt was to keep a central force and modify the exponent, writing \(f\propto r^{-(2+\delta)}\); for a nearly circular orbit a small \(\delta\) produces an apsidal angle \(\Phi\approx\pi\left(1+\delta/2\right)\) and hence a slow rotation of the line of apsides, and \(\delta\) can always be chosen to fit one planet. The proposal fails because the \(\delta\) that fits Mercury does not fit the others, and because it has no independent motivation whatever.

The correct account is not a modified force law at all. In general relativity the orbit is a geodesic of a curved spacetime and its equation acquires the term shown in Equation (53.2), quadratic in \(u=1/r\) and suppressed by \(c^{-2}\); the resulting advance is Equation (53.1), with no adjustable parameter, and it predicts \(42.98\) seconds of arc per century for Mercury against the observed residue. That derivation belongs to Experiment: The Classical Tests of General Relativity, where the measurement and its error budget are set out, and to Phenomenon 53.1, which states the result. What this chapter contributes is the logic that makes the measurement mean anything: without Theorem 27.41 a non-closing orbit would be an anomaly of no particular significance, and with it, it is a bound on the force law.

Remark 27.43 (The repulsive case, and where it is used).

Nothing in Section 27.4.2 required \(k>0\). For a repulsive inverse-square force, \(k<0\) in Equation (27.45), the effective potential falls monotonically and has no well, so every motion has \(E>0\) and Equation (27.48) gives \(e>1\). The semi-latus rectum \(p=L^{2}/\left(\mu k\right)\) of Equation (27.47) is then negative, and the physical solution is the branch on which \(1+e\cos\phi<0\): the branch of the hyperbola that curves away from the centre rather than around it. This is the orbit of an alpha particle in the Coulomb field of a nucleus, and integrating Equation (27.38) for it produces the relation between impact parameter and deflection angle from which the Rutherford cross section follows; the calculation, and the scattering experiment that made it famous, are in Section 70.3.2. The same hyperbolic solution, taken in the attractive case with \(E>0\), is the gravitational slingshot: a spacecraft leaves a planet's neighbourhood with the same speed relative to the planet with which it arrived, but in a different direction, and therefore with a different — and usefully larger — speed relative to the Sun.

The virial theorem

Everything so far has followed individual orbits. For a bound system of many bodies — a star cluster, a gas of self-gravitating masses — the orbits are inaccessible, but a statement about time averages survives, and it is the tool by which such systems are weighed (Evidence-Based Cosmology).

Theorem 27.44 (Virial theorem).

Let \(N\) particles with positions \(\vect{x}_{a}\) and momenta \(\vect{p}_{a}\) move under forces \(\vect{F}_{a}\) such that the motion is bounded: all \(\abs{\vect{x}_{a}}\) and \(\abs{\vect{p}_{a}}\) remain finite for all time. Then the long-time averages \(\avg{f} = \lim_{\tau\to\infty}\tau^{-1}\!\int_{0}^{\tau}\!f\,\dd t\) satisfy

\begin{equation}\tag{27.56} 2\avg{T} = -\Bigl\langle\,\sum_{a=1}^{N} \vect{F}_{a}\cdot\vect{x}_{a}\Bigr\rangle\ep \end{equation}

If the forces derive from a potential \(V\) that is a homogeneous function of degree \(n\) of the positions, the right side is \(n\avg{V}\), so

\begin{equation}\tag{27.57} 2\avg{T} = n\avg{V}\ec \end{equation}

and for the inverse-square attraction (\(n=-1\))

\begin{equation}\tag{27.58} 2\avg{T} = -\avg{V}\ep \end{equation}

Rests on Equation (27.41) and Remark 21.40.

Proof.

Derives Theorem 27.44. Consider \(G = \sum_{a}\vect{p}_{a}\cdot\vect{x}_{a}\). Along the motion,

\begin{equation*} \dv{G}{t} = \sum_{a}\dot{\vect{p}}_{a}\cdot\vect{x}_{a} + \sum_{a}\vect{p}_{a}\cdot\dot{\vect{x}}_{a} = \sum_{a}\vect{F}_{a}\cdot\vect{x}_{a} + 2T\ec \end{equation*}

since \(\vect{p}_{a}\cdot\dot{\vect{x}}_{a} = m_{a}\abs{\dot{\vect{x}}_{a}}^{2}\) sums to twice the kinetic energy. Averaging over \([0,\tau]\), \(\avg{\dd G/\dd t} = [G(\tau)-G(0)]/\tau\), and boundedness of positions and momenta bounds \(G\), so the limit \(\tau\to\infty\) vanishes (exactly, already at one period, for periodic motion). This is Equation (27.56). When \(\vect{F}_{a} = -\pp V/\pp\vect{x}_{a}\) with \(V\) homogeneous of degree \(n\), Euler's homogeneous-function theorem (Remark 21.40) gives \(\sum_{a}\vect{x}_{a}\cdot\pp V/\pp\vect{x}_{a} = nV\), whence Equation (27.57); \(n=-1\) is the gravitational and Coulomb case.

Corollary 27.45 (Bound Kepler averages).

For a bound orbit of the inverse-square attraction, the conserved energy \(E = T + V\) satisfies

\begin{equation}\tag{27.59} \avg{T} = -E\ec\qquad \avg{V} = 2E\ec \end{equation}

so a bound orbit has \(E<0\), and adding energy to it slows the time-averaged motion — the negative specific heat of gravitating systems. Rests on Theorem 27.44.

Proof.

Derives Corollary 27.45. \(E\) is constant, so \(E = \avg{T} + \avg{V}\); combine with Equation (27.58).

Where the claims of this chapter are tested

It is worth saying plainly which of the observed facts asserted above are tied to an experiment described in this book and which are not. Kepler's third law is tested in Experiment: The Cavendish Torsion Balance, whose lunar check Equation (33.19) is Equation (27.53) applied to the Earth–Moon system with a laboratory value of \(G\); the failure of exact closure, Phenomenon 27.42, is measured in Experiment: The Classical Tests of General Relativity; and the repulsive branch of Section 27.4.2 is what Section 70.3.2 tests. The remaining five observed statements — Phenomena 27.5, 27.8, 27.19, 27.26 and 27.32 — carry no dedicated experiment chapter here. They are not for that reason unsupported: the first is a commonplace of every static structure, the second is the standard method by which a centre of gravity is located, and the last three are the content of the regularities Kepler extracted from Brahe's catalogue of the positions of Mars. But no measurement with its own uncertainty budget is set out in this book for any of the five, and the honest record of that is this paragraph rather than silence.