Classical-Mechanics · Unit 11 · Video 5 · Interactive Practice

The Two-Direction Rule: Circular Motion on a Cone and a Turntable

IKey Formulas

FormulaNameWhat you need
Ncosθ=mv02r,Nsinθ=mgN\cos\theta = \dfrac{m v_0^2}{r}, \qquad N\sin\theta = mgNewton's law in two directions (cone)Half-angle θ\theta, speed v0v_0
r=v02gtanθr = \dfrac{v_0^2}{g}\tan\thetaOrbit radius inside the conev0v_0, θ\theta
T=2πrv0=2πv0tanθgT = \dfrac{2\pi r}{v_0} = \dfrac{2\pi v_0 \tan\theta}{g}Period of one orbitv0v_0, θ\theta
ωmax=μgR\omega_{\max} = \sqrt{\dfrac{\mu g}{R}}Turntable slipping limitμ\mu, RR

Key Insight: The contact force always splits into two jobs — one component cancels mgmg, the other supplies mv2/rmv^2/r. Dividing the vertical equation by the radial one kills both NN and mm, which is why neither the radius nor the slipping speed depends on how heavy the object is.

IIInside the Cone: One Push, Two Jobs

A single wall push must cancel gravity and bend the path — what speed does a given radius demand?

As θ90°\theta \to 90\degree the wall flattens out and Ncosθ0N\cos\theta \to 0: a horizontal frictionless surface has no inward push left to give, so no radius can hold a moving object at all.

IIIThe Turntable: Friction Has a Ceiling

Static friction alone bends the coin's path, and it cannot grow past μN\mu N — how fast is too fast?

Nothing caps the cone's normal force — it simply tilts and grows to match any speed — but friction is capped at μN\mu N, and that ceiling is what fails first on the turntable.

IVTwo Equations, Every Time

One direction balances gravity, the other supplies mv2/rmv^2/r — and dividing them cancels NN and mm.

1 — Radial, inward negative

Ncosθ=mv02r    Ncosθ=mv02r-N\cos\theta = -\frac{m v_0^2}{r} \;\Longrightarrow\; N\cos\theta = \frac{m v_0^2}{r}

2 — Vertical, no acceleration

Nsinθmg=0    Nsinθ=mgN\sin\theta - mg = 0 \;\Longrightarrow\; N\sin\theta = mg

3 — Divide vertical by radial

NsinθNcosθ=mgmv02/r    tanθ=rgv02\frac{N\sin\theta}{N\cos\theta} = \frac{mg}{m v_0^2 / r} \;\Longrightarrow\; \tan\theta = \frac{rg}{v_0^2}

4 — Solve for the radius

r=v02gtanθr = \frac{v_0^2}{g}\tan\theta

5 — One circumference at constant speed

T=2πrv0=2πv0tanθgT = \frac{2\pi r}{v_0} = \frac{2\pi v_0 \tan\theta}{g}

1 — Radial, inward negative

fs=mRω2    fs=mRω2-f_s = -m R \omega^2 \;\Longrightarrow\; f_s = m R \omega^2

2 — Vertical, no acceleration

Nmg=0    N=mgN - mg = 0 \;\Longrightarrow\; N = mg

3 — Friction has a ceiling

(fs)max=μN=μmg(f_s)_{\max} = \mu N = \mu m g

4 — On the verge of slipping

μmg=mRωmax2\mu m g = m R \omega_{\max}^2

5 — The mass cancels

ωmax=μgR\omega_{\max} = \sqrt{\frac{\mu g}{R}}

VQuiz Questions

Problem 1 · Radius Inside the Cone

Given: an object slides without friction inside a cone of apex half-angle θ=60°\theta = 60\degree at constant speed v0=3.0v_0 = 3.0 m/s, with g=9.8g = 9.8 m/s² — find the orbit radius rr.

✅ Correct! r=v02gtanθ=9.09.8(1.732)=1.59r = \dfrac{v_0^2}{g}\tan\theta = \dfrac{9.0}{9.8}(1.732) = 1.59 m — a wide, shallow cone (θ\theta near 90°90\degree) pushes the orbit far from the axis.
❌ The ratio is upside down. Dividing the vertical equation by the radial one gives tanθ=rg/v02\tan\theta = rg/v_0^2, so rr carries a factor of tanθ\tan\theta, not cotθ\cot\theta. You computed v02gcot60°=0.53\dfrac{v_0^2}{g}\cot 60\degree = 0.53 m.
❌ The geometry is missing. 0.920.92 m is just v02/gv_0^2/g — that would be the answer only for θ=45°\theta = 45\degree, where tanθ=1\tan\theta = 1. The wall's tilt must enter through tanθ\tan\theta.
❌ Not quite. Check the units: v02tanθv_0^2\tan\theta has units of m²/s², so it must be divided by gg to leave a length.
Show solution

Radial direction (inward negative), where the inward part of the normal force is NcosθN\cos\theta:

Ncosθ=mv02r    Ncosθ=mv02r-N\cos\theta = -\frac{m v_0^2}{r} \;\Longrightarrow\; N\cos\theta = \frac{m v_0^2}{r}

Vertical direction (the object neither rises nor falls):

Nsinθ=mgN\sin\theta = mg

Divide the vertical equation by the radial one — both NN and mm cancel:

tanθ=rgv02    r=v02gtanθ\tan\theta = \frac{rg}{v_0^2} \;\Longrightarrow\; r = \frac{v_0^2}{g}\tan\theta

Substituting v0=3.0v_0 = 3.0 m/s, θ=60°\theta = 60\degree, g=9.8g = 9.8 m/s²:

r=(3.0)29.8tan60°=(0.918)(1.732)=1.59 mr = \frac{(3.0)^2}{9.8}\tan 60\degree = (0.918)(1.732) = 1.59\ \text{m}

Problem 2 · Does the Mass Matter?

Given: two pucks circle inside the same frictionless cone at the same speed v0v_0. Puck A has twice the mass of puck B — compare their orbit radii and the normal forces they feel.

✅ Correct! r=v02gtanθr = \dfrac{v_0^2}{g}\tan\theta contains no mm, while N=mgsinθN = \dfrac{mg}{\sin\theta} is proportional to mm — the wall pushes a heavier puck harder in exactly the right proportion.
❌ Mass does not set the radius. mm appears on both sides of Ncosθ=mv02/rN\cos\theta = mv_0^2/r and Nsinθ=mgN\sin\theta = mg, so it cancels when you divide. Heavier means a bigger NN, not a bigger circle.
❌ Half right. The radius really is mass-independent, but NN is not: the vertical balance Nsinθ=mgN\sin\theta = mg forces N=mg/sinθN = mg/\sin\theta, which doubles when the mass doubles.
❌ Not quite. Solve each equation separately: rr comes from the ratio (mass cancels), but NN comes from the vertical balance alone (mass survives).
Show solution

The two equations of motion are

Ncosθ=mv02r,Nsinθ=mgN\cos\theta = \frac{m v_0^2}{r}, \qquad N\sin\theta = mg

Radius: dividing removes NN and mm:

tanθ=rgv02    r=v02gtanθ\tan\theta = \frac{rg}{v_0^2} \;\Longrightarrow\; r = \frac{v_0^2}{g}\tan\theta

Same v0v_0 and same θ\theta means the same radius, whatever the mass.

Normal force: from the vertical equation alone,

N=mgsinθ    NANB=mAmB=2N = \frac{mg}{\sin\theta} \;\Longrightarrow\; \frac{N_A}{N_B} = \frac{m_A}{m_B} = 2

Puck A feels twice the normal force. This is exactly why the mass drops out: doubling mm doubles both the required centripetal force and the wall's push, leaving the geometry untouched.

Problem 3 · When Does the Coin Fly Off?

Given: a coin rests at the rim of a turntable, R=0.15R = 0.15 m from the axis, with coefficient of static friction μ=0.30\mu = 0.30 and g=9.8g = 9.8 m/s² — find ωmax\omega_{\max}, then the turntable's rotation period TT at that instant.

What is the maximum angular speed?

What is the rotation period at that speed?

✅ Correct! ωmax=μg/R=19.6=4.43\omega_{\max} = \sqrt{\mu g/R} = \sqrt{19.6} = 4.43 rad/s, and T=2π/ωmax=1.42T = 2\pi/\omega_{\max} = 1.42 s — about 42 revolutions per minute.
❌ You stopped one step early. μg/R=19.6\mu g/R = 19.6 is ωmax2\omega_{\max}^2 (units s2^{-2}), not ωmax\omega_{\max}. Take the square root: 19.6=4.43\sqrt{19.6} = 4.43 rad/s.
❌ Check which symbols belong inside the root. Setting μmg=mRωmax2\mu m g = m R\omega_{\max}^2 and cancelling mm leaves ωmax=μg/R\omega_{\max} = \sqrt{\mu g/R} — dropping μ\mu gives 8.088.08 rad/s, dropping RR gives 1.711.71 rad/s.
❌ Check the period relation. T=2π/ωT = 2\pi/\omega: dividing by 2π2\pi instead gives the frequency 0.700.70 rev/s, forgetting 2π2\pi altogether gives 0.230.23 s, and multiplying by 2π2\pi gives 27.827.8 s.
Show solution

Step 1 — radial: static friction is the only inward force, so it supplies the centripetal force:

fs=mRω2f_s = m R \omega^2

Step 2 — vertical: the coin stays flat on the table, so N=mgN = mg, and friction's ceiling is

(fs)max=μN=μmg(f_s)_{\max} = \mu N = \mu m g

Step 3 — on the verge of slipping, required equals maximum; the mass cancels:

μmg=mRωmax2    ωmax=μgR=(0.30)(9.8)0.15=19.6=4.43 rad/s\mu m g = m R \omega_{\max}^2 \;\Longrightarrow\; \omega_{\max} = \sqrt{\frac{\mu g}{R}} = \sqrt{\frac{(0.30)(9.8)}{0.15}} = \sqrt{19.6} = 4.43\ \text{rad/s}

Step 4 — period:

T=2πωmax=6.2834.43=1.42 sT = \frac{2\pi}{\omega_{\max}} = \frac{6.283}{4.43} = 1.42\ \text{s}

Problem 4 · Two Coins, One Table

Given: two identical coins sit on the same turntable — one at the rim (radius RR), one at radius R/4R/4. The table is slowly spun faster and faster — which slips first, and at what angular speed does the other one go?

✅ Correct! ωmax(r)=μg/r\omega_{\max}(r) = \sqrt{\mu g/r}, so quartering the radius multiplies the limit by 4=2\sqrt{4} = 2 — the outermost coin always goes first.
μ\mu sets the ceiling, not the demand. Both coins share the same ceiling μg\mu g, but the required centripetal acceleration rω2r\omega^2 grows with rr — so the rim coin reaches its ceiling at a lower ω\omega.
❌ The demand shrinks with radius. The required inward acceleration is rω2r\omega^2, which is smaller at smaller rr for the same ω\omega. A tighter circle at a fixed angular speed means a slower linear speed, hence less friction needed.
❌ Watch the square root. ωmax1/r\omega_{\max}\propto 1/\sqrt{r}, not 1/r1/r — quartering the radius doubles the limit, it does not quadruple it.
Show solution

For a coin at radius rr the two-direction rule gives fs=mrω2f_s = m r\omega^2 and N=mgN = mg, so slipping begins when

μmg=mrω2    ωmax(r)=μgr\mu m g = m r \omega^2 \;\Longrightarrow\; \omega_{\max}(r) = \sqrt{\frac{\mu g}{r}}

The limit falls off as 1/r1/\sqrt{r}, so the rim coin slips first. For the inner coin at r=R/4r = R/4:

ωmax(R/4)=μgR/4=4μgR=2μgR=2ωmax(R)\omega_{\max}(R/4) = \sqrt{\frac{\mu g}{R/4}} = \sqrt{\frac{4\mu g}{R}} = 2\sqrt{\frac{\mu g}{R}} = 2\,\omega_{\max}(R)

Equivalently, at a common ω\omega the required inward acceleration is rω2r\omega^2: the rim coin demands four times as much friction as the coin at R/4R/4, while both are held by the same ceiling μg\mu g.

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