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Rolling Delays the Ball's Departure

Irodov 1.263DifficultyDifficulty 3 of 5UniquenessUniqueness 3 of 5

Problem Irodov 1.263

A uniform solid ball of radius rr starts, with negligible speed, from the highest point of a fixed sphere of radius RR and rolls down the sphere’s outer surface without slipping. At some point of the descent the ball leaves the surface. Find the ball’s angular velocity at that instant.

The ball of radius r on the outside of the fixed sphere of radius R. Its center stays a distance R+r from the sphere's center O, and θ is the angle from the upward vertical (dashed) to the radius through the contact.

The ball of radius rr on the outside of the fixed sphere of radius RR. Its center stays a distance R+rR+r from the sphere’s center OO, and θ\theta is the angle from the upward vertical (dashed) to the radius through the contact.

The ball alone on the sphere's local tangent plane at the same instant, showing the center's velocity v, the spin ω, the marked contact point, and the radius line of length r from the center to the rim.

The ball alone on the sphere’s local tangent plane at the same instant, showing the center’s velocity v\vect v, the spin ω\omega, the marked contact point, and the radius line of length rr from the center to the rim.

Given
  • RR
  • rr
  • rolls without slipping
  • negligible initial speed
Find
the angular velocity ω\omega at the moment the ball breaks off

Solution

Step 1The kinetic energy of a ball that rolls

Let mm be the ball’s mass, vv the speed of its center and ω\omega its angular velocity. Rolling without slipping means the contact point is momentarily at rest, so the center’s speed and the spin are locked together, and the moment of inertia is that of a uniform solid ball about a central axis.

v=ωr,I=25mr2(1) v = \omega r, \qquad I = \frac{2}{5}mr^2 \tag{1}

Adding the translational and rotational parts and eliminating ω\omega,

K=12mv2+12Iω2=12mv2+12⋅25mr2⋅v2r2=12mv2+15mv2\begin{align*}K &= \frac{1}{2}mv^2 + \frac{1}{2}I\omega^2 \\ &= \frac{1}{2}mv^2 + \frac{1}{2}\cdot\frac{2}{5}mr^2\cdot\frac{v^2}{r^2} \\ &= \frac{1}{2}mv^2 + \frac{1}{5}mv^2\end{align*}
K=710mv2K = \dfrac{7}{10}mv^2
(2)
Step 2Energy conservation fixes the speed at every angle

Both surface forces, the normal force and the static friction, are applied at the contact point, which rolling without slipping holds instantaneously at rest, so neither of them does any work and all the potential energy released goes into the kinetic energy (2). The center starts at height R+rR+r above OO and at angle θ\theta it stands at height (R+r)cos⁡θ(R+r)\cos\theta, so the drop is

h=(R+r)(1−cos⁡θ)h = (R+r)(1 - \cos\theta)

and equating the energy released to the kinetic energy gained,

710mv2=mgh=mg(R+r)(1−cos⁡θ)\begin{align*}\frac{7}{10}mv^2 &= mgh \\ &= mg(R+r)(1-\cos\theta)\end{align*}
v2=107g(R+r)(1−cos⁡θ)v^2 = \dfrac{10}{7}g(R+r)(1-\cos\theta)
(3)
Step 3The break-off condition

While the ball stays on the sphere its center travels on a circle of radius R+rR+r about OO, so the resultant force along that radius must supply the centripetal acceleration. The two forces are the sphere’s push, which can only be outward along the radius, and the weight, which makes the angle θ\theta with that radius.

The two forces on the ball at the angle θ: the normal force N outward along the radius through the contact, away from O, and the weight m g vertical at the ball's center.

The two forces on the ball at the angle θ\theta: the normal force N\vect N outward along the radius through the contact, away from OO, and the weight mgm\vect g vertical at the ball’s center.

Resolving the weight along the inward radius and subtracting the outward normal force,

mv2R+r=mgcos⁡θ−N\frac{mv^2}{R+r} = mg\cos\theta - N

The ball breaks off at the instant the surface stops pushing, that is when NN falls to zero, and putting N=0N=0 into the line above leaves

v2=g(R+r)cos⁡θv^2 = g(R+r)\cos\theta
(4)
Step 4The angle at which the ball leaves

Both (3) and (4) give the same v2v^2, and they can only agree at one angle. Setting them equal and canceling the common factor g(R+r)g(R+r),

107g(R+r)(1−cos⁡θ)=g(R+r)cos⁡θ10(1−cos⁡θ)=7cos⁡θ10=17cos⁡θ\begin{align*}\frac{10}{7}g(R+r)(1-\cos\theta) &= g(R+r)\cos\theta \\ 10(1-\cos\theta) &= 7\cos\theta \\ 10 &= 17\cos\theta\end{align*}
cos⁡θ=1017\cos\theta = \dfrac{10}{17}
(5)

Neither RR nor rr survives, so a rolling ball always leaves at this same angle.

Step 5The angular velocity at that instant

Substituting the break-off angle (5) into (4) gives the speed of the center there, and the rolling condition (1) converts it into the spin.

v2=g(R+r)⋅1017ω2=v2r2=10g(R+r)17r2\begin{align*}v^2 &= g(R+r)\cdot\frac{10}{17} \\ \omega^2 &= \frac{v^2}{r^2} = \frac{10g(R+r)}{17r^2}\end{align*}
ω=10g(R+r)17r2\omega = \sqrt{\dfrac{10g(R+r)}{17r^2}}
(6)
Check

Rebuild the speed (3) without invoking energy at all. Along the surface Newton’s second law for the center reads m dv/dt=mgsin⁡θ−fm\,dv/dt = mg\sin\theta - f, while friction is the only force with a moment about the ball’s own center, fr=25mr2 dω/dtfr = \frac{2}{5}mr^{2}\,d\omega/dt; rolling keeps v=ωrv = \omega r at every instant, so f=25m dv/dtf = \frac{2}{5}m\,dv/dt and the two equations together leave dv/dt=57gsin⁡θdv/dt = \frac{5}{7}g\sin\theta. Writing dv/dt=v dv/dsdv/dt = v\,dv/ds with ds=(R+r) dθds = (R+r)\,d\theta and integrating from rest at θ=0\theta = 0 returns v2=107g(R+r)(1−cos⁡θ)v^{2} = \frac{10}{7}g(R+r)(1-\cos\theta), which is (3) term for term, reached by forces rather than by energy. For a fixed path radius R+rR+r the boxed answer scales as 1/r1/r, as it must, since a smaller ball has to spin faster to roll at the same speed. Dimensionally g(R+r)/r2g(R+r)/r^2 carries units of s−2\mathrm{s}^{-2}, whose square root is indeed an angular velocity. The ball’s mass canceled from every equation, as it must when gravity is the only force doing work.

Remark

Compare the same descent with the friction switched off, so the ball slides instead of rolling. Then all the released energy goes into the center’s motion, the energy balance reads v2=2g(R+r)(1−cos⁡θ)v^2 = 2g(R+r)(1-\cos\theta), and the same break-off condition gives cos⁡θ=2/3\cos\theta = 2/3. Rolling therefore delays the departure, because a rolling ball has to spend part of the released energy on spin and so arrives at any given angle moving more slowly, which lets the surface keep curving away underneath it for longer. Both cases are one formula: writing the moment of inertia as I=kmr2I = kmr^2, the ball leaves at cos⁡θ=2/(3+k)\cos\theta = 2/(3+k), which is 2/32/3 for the sliding particle, 10/1710/17 for the uniform ball, and 1/21/2 for a thin hoop rolling on its rim.