1. Physics
  2. Rotational Motion
  3. Angular Momentum

Rotational Motion · JEE & NEET Physics

Angular Momentum: notes and previous year questions

The momentum of turning: L = r × p and L = Iω, τ = dL/dt, conservation when no outside torque acts, energy, joining up, and orbits.

Angular Momentum in short

  • Angular momentum is the momentum of turning: L = r × p, size mvr⊥.
  • A particle moving in a straight line has constant L about any point.
  • For a spinning body L = Iω, the twin of p = mv.
  • Torque is the rate of change of angular momentum; a steady torque gives ΔL = τΔt.

1Angular momentum of a particle

Angular momentum L⃗\vec L is the momentum of turning, measured about a point (or an axis).

L⃗=r⃗×p⃗=r⃗×mv⃗\vec L = \vec r \times \vec p = \vec r \times m\vec v
L=mvrsin⁡θ=mv r⊥L = mvr\sin\theta = mv\,r_\perpr⊥: the shortest distance from the point to the line of motion. Unit: kg m²/s (= J s).

Even a body moving in a straight line has angular momentum about a point off its path. A 2 kg ball at 5 m/s passing 3 m from O: as it moves, rr and θ\theta change, but rsin⁡θr\sin\theta stays 3 m, so L=2×5×3=30L = 2 \times 5 \times 3 = 30 kg m²/s stays constant.

Example: 0.5 kg at 8 m/s, 2 m from an axis: L=8L = 8 kg m²/s.

2L = Iω for a spinning body

Each bit of a spinning body moves at v=ωrv = \omega r, so its angular momentum is m(ωr)r=mωr2m(\omega r)r = m\omega r^2. Adding all the bits:

L=(∑mr2)ω=IωL = \Big(\sum mr^2\Big)\omega = I\omegaThe twin of p = mv. L points along the axis, by the right-hand rule.
Moving in a lineTurning
p=mvp = mvL=IωL = I\omega
F=dp/dtF = dp/dtτ=dL/dt\tau = dL/dt
no outside force: pp keptno outside torque: LL kept
kg m/skg m²/s

3Torque changes angular momentum

τ⃗=dL⃗dt\vec\tau = \frac{d\vec L}{dt}The twin of F = dp/dt. For a rigid body, d(Iω)/dt = Iα.
ΔL=τ Δt\Delta L = \tau\,\Delta tAngular impulse of a steady torque. The slope of an L–t graph is the torque.

4Conservation of angular momentum

If the net outside torque is zero, dL/dt=0dL/dt = 0 and the angular momentum stays constant:

I1ω1=I2ω2I_1\omega_1 = I_2\omega_2Smaller I, faster spin.

Forces inside the system (muscles, friction between parts) can change II, but they come in pairs whose torques cancel, so they cannot change LL.

5Energy is not conserved

KE=12Iω2=L22IKE = \tfrac12 I\omega^2 = \frac{L^2}{2I}

With LL fixed, a smaller II means more kinetic energy: KE2=I1I2KE1KE_2 = \frac{I_1}{I_2}KE_1. Pulling the weights from 1 m to 0.5 m (I 8 → 5, ω 0.5 → 0.8 rad/s) raises the kinetic energy from 1 J to 1.6 J. The extra energy is the work the muscles do pulling the weights inward.

6Joining up

I1ω1+I2ω2=(I1+I2) ωI_1\omega_1 + I_2\omega_2 = (I_1 + I_2)\,\omegaTake one sense of turning as positive: an opposite spin counts as negative.

7Orbits and real life

The Sun's pull on a planet points straight at the Sun, so it has no torque about the Sun: the planet's angular momentum is kept. Near the Sun it moves fast, far away slowly, and it sweeps out equal areas in equal times (Kepler's second law).

v1r1=v2r2v_1r_1 = v_2r_2At the nearest and farthest points, where v is square to r.

A comet at 50 km/s, 1 unit from the Sun, moves at 10 km/s at 5 units. A spacecraft that fires its engine along its path does feel a torque about the Earth or Sun, so its LL changes during the burn; afterwards, on its new orbit, v1r1=v2r2v_1r_1 = v_2r_2 again. For example, 8.2 km/s at perigee 7000 km gives about 5.7 km/s at apogee 10 000 km.

Summary

Key ideas

  • Angular momentum is the momentum of turning: L = r × p, size mvr⊥.
  • A particle moving in a straight line has constant L about any point.
  • For a spinning body L = Iω, the twin of p = mv.
  • Torque is the rate of change of angular momentum; a steady torque gives ΔL = τΔt.
  • With no outside torque, L is conserved: I₁ω₁ = I₂ω₂.
  • Internal forces can change I but not L.
  • KE = L²/2I: pulling in raises the kinetic energy; joining up loses some.
  • Opposite spins have opposite signs.
  • About a pivot, L is kept in a collision even though momentum is not.
  • Planets keep L: v₁r₁ = v₂r₂, equal areas in equal times.

Every equation

Particle
L⃗=r⃗×p⃗\vec L = \vec r \times \vec p
Size
L=mvrsin⁡θ=mvr⊥L = mvr\sin\theta = mvr_\perp
Spinning body
L=IωL = I\omega
Torque
τ=dL/dt\tau = dL/dt
Angular impulse
ΔL=τΔt\Delta L = \tau\Delta t
Conservation
I1ω1=I2ω2I_1\omega_1 = I_2\omega_2
Kinetic energy
KE=L2/2IKE = L^2/2I
KE when I changes
KE2=(I1/I2)KE1KE_2 = (I_1/I_2)KE_1
Joining up
I1ω1+I2ω2=(I1+I2)ωI_1\omega_1 + I_2\omega_2 = (I_1 + I_2)\omega
Ball sticking to a pivoted rod
mvd=(Irod+md2)ωmvd = (I_{rod} + md^2)\omega
Orbit ends
v1r1=v2r2v_1r_1 = v_2r_2

Previous year questions with solutions

Real JEE and NEET questions on angular momentum. Try each one before you open the solution.

Q1NEET 2025One correct option

The Sun rotates around its centre once in 27 days. What will be the period of revolution if the Sun were to expand to twice its present radius without any external influence? Assume the Sun to be a sphere of uniform density.

  1. A115 days
  2. B108 days
  3. C100 days
  4. D105 days
Show answer and solution

Answer: Option B

Nothing outside acts, so IωI\omega is kept. Twice the radius with the same mass makes I=25MR2I = \tfrac{2}{5}MR^{2} four times as large, so ω\omega becomes a quarter as large and the period four times as long: 4×27=1084 \times 27 = 108 days.

The trap is to double the period along with the radius, 5454 days, which is not even offered; the radius enters II squared. The mass has not changed, only how far out it sits.

Q2JEE Main 2024Numerical answer

A body of mass 5kg5 \mathrm{kg} moving with a uniform speed 32ms−13\sqrt{2}{\mathrm{ms}}^{-1} in X−YX-Y plane along the line y=x+4y=x+4. The angular momentum of the particle about the origin will be _________ kgm2s−1\mathrm{kg}m^{2}s^{-1}.

Show answer and solution

Answer: 60 kg m²/s

Two ways. Components: (0, 4)(0,\ 4) is a point on the line, and a line of slope 11 has a direction with equal xx and yy parts, so a speed of 323\sqrt{2} along it is the velocity (3, 3)(3,\ 3), taking the body to be moving towards +x+x. Then Lz=m(xvy−yvx)=5(0×3−4×3)=−60L_{z} = m(xv_{y} - yv_{x}) = 5(0 \times 3 - 4 \times 3) = -60: a size of 60 kg m2/s60\ \mathrm{kg\,m^{2}/s}, clockwise.

Perpendicular distance: the line cuts the axes at (0, 4)(0,\ 4) and (−4, 0)(-4,\ 0), and the perpendicular from O meets it halfway between them, at (−2, 2)(-2,\ 2), which is 22 m2\sqrt{2}\ \mathrm{m} from O. So L=mv r⊥=5×32×22=60L = mv\,r_{\perp} = 5 \times 3\sqrt{2} \times 2\sqrt{2} = 60.

The trap is taking the intercept, 4 m4\ \mathrm{m}, as r⊥r_{\perp}, which gives 602≈8560\sqrt{2} \approx 85: the 4 m4\ \mathrm{m} is measured along the yy-axis, not at right angles to the line. The body is moving at a steady speed along a straight line, so 6060 holds at every point of its path.

Q3JEE Main 2024One correct option

A particle of mass mm is projected with a velocity 'uu' making an angle of 30∘{30}^{\circ } with the horizontal. The magnitude of angular momentum of the projectile about the point of projection when the particle is at its maximum height hh is :

  1. Amu32g\frac{{\mathrm{mu}}^{3}}{\sqrt{2} g}
  2. Bzero
  3. C32mu2g\frac{\sqrt{3}}{2}\frac{{\mathrm{mu}}^{2}}{ g}
  4. D316mu3g\frac{\sqrt{3}}{16}\frac{{\mathrm{mu}}^{3}}{ g}
Show answer and solution

Answer: Option D

At the top the velocity is horizontal, ucos⁡30∘=32uu\cos 30^{\circ} = \dfrac{\sqrt{3}}{2}u, and its line is the height hh above the point of projection: h=u2sin⁡230∘2g=u28gh = \dfrac{u^{2}\sin^{2}30^{\circ}}{2g} = \dfrac{u^{2}}{8g}. So L=m×32u×u28g=316mu3gL = m \times \dfrac{\sqrt{3}}{2}u \times \dfrac{u^{2}}{8g} = \dfrac{\sqrt{3}}{16}\dfrac{mu^{3}}{g}.

B is the trap of the last question: at the top the vertical velocity is zero, not the angular momentum. C cannot be right, since mu2g\dfrac{mu^{2}}{g} is a mass times a length, not a unit of angular momentum. A is far too big: it would need the height to be 2u23g\dfrac{\sqrt{2}u^{2}}{\sqrt{3}g}, more than the u22g\dfrac{u^{2}}{2g} that even a straight-up throw reaches.

Practice questions, easy to hard

Three questions from the angular momentum practice ladder: one easy, one medium, one hard.

Q4One correct option

τ⃗=dL⃗dt\vec{\tau} = \dfrac{d\vec{L}}{dt} is a vector equation: in a short time dtdt, L⃗\vec{L} changes by τ⃗ dt\vec{\tau}\,dt, in the direction of the torque. A torque along L⃗\vec{L} makes it longer or shorter. A torque at right angles to L⃗\vec{L} turns L⃗\vec{L} without changing its size — just as a force at right angles to a velocity, a centripetal force, turns the velocity without changing the speed.

A wheel spins with L⃗=2i^ kg m2/s\vec{L} = 2\hat{i}\ \mathrm{kg\,m^{2}/s}. A torque of 0.1j^ N m0.1\hat{j}\ \mathrm{N\,m} acts on it for 0.2 s0.2\ \mathrm{s}. Afterwards, its angular momentum is

  1. A2.02i^ kg m2/s2.02\hat{i}\ \mathrm{kg\,m^{2}/s}
  2. B1.98i^ kg m2/s1.98\hat{i}\ \mathrm{kg\,m^{2}/s}
  3. C0.02j^ kg m2/s0.02\hat{j}\ \mathrm{kg\,m^{2}/s}
  4. D(2i^+0.02j^) kg m2/s(2\hat{i} + 0.02\hat{j})\ \mathrm{kg\,m^{2}/s}: practically the same size, turned slightly towards j^\hat{j}
Show answer and solution

Answer: Option D

ΔL⃗=τ⃗ Δt=0.02j^\Delta\vec{L} = \vec{\tau}\,\Delta t = 0.02\hat{j}, so L⃗=2i^+0.02j^\vec{L} = 2\hat{i} + 0.02\hat{j}. Its size is 4+0.0004≈2.0001\sqrt{4 + 0.0004} \approx 2.0001: practically unchanged, while its direction has swung through about 0.022=0.01 rad\dfrac{0.02}{2} = 0.01\ \mathrm{rad} towards j^\hat{j}.

A and B add or subtract the sizes as if the torque lay along L⃗\vec{L}. C forgets that the torque adds to the angular momentum already there instead of replacing it.

Q5One correct option

When a particle hits a free rod, the blow between them is internal to the pair, so the pair keeps both its total linear momentum and its total angular momentum about any fixed point. For a body that moves and spins at once, its angular momentum about a fixed point is the sum of two parts: Mvcmr⊥Mv_{\mathrm{cm}}r_{\perp}, from its centre of mass moving as one particle (as in the bump questions), plus IcmωI_{\mathrm{cm}}\omega, from its spin about its own centre of mass, each with its direction by the right-hand rule. Take the fixed point where the rod's centre is at the instant of the hit: the rod's centre moves straight through it, so the first part is zero and the rod has just IcmωI_{\mathrm{cm}}\omega.

A small ball of mass mm slides at vv on a smooth table, at right angles to a uniform rod of mass 4m4m and length LL lying at rest, and hits the rod at one end. The ball stops dead. What is the rod's angular speed just after?

  1. A3v4L\dfrac{3v}{4L}
  2. Bv2L\dfrac{v}{2L}
  3. C3v2L\dfrac{3v}{2L}
  4. D6vL\dfrac{6v}{L}
Show answer and solution

Answer: Option C

Linear momentum: mv=4m vcmmv = 4m\,v_{\mathrm{cm}}, so vcm=v4v_{\mathrm{cm}} = \dfrac{v}{4}. Angular momentum about the rod's centre: the ball's line is L2\dfrac{L}{2} from it, so mvL2=4mL212ωmv\dfrac{L}{2} = \dfrac{4mL^{2}}{12}\omega, and ω=3v2L\omega = \dfrac{3v}{2L}.

A takes the rod as turning about its far end, with 4mL23\dfrac{4mL^{2}}{3} and an arm of LL. B assumes the far end stays still, ω=vcmL/2\omega = \dfrac{v_{\mathrm{cm}}}{L/2}. D forgets the rod's mass is 4m4m.

Check the energy: after, 12(4m)(v4)2+12mL23(3v2L)2=mv28+3mv28=12mv2\tfrac{1}{2}(4m)\left(\dfrac{v}{4}\right)^{2} + \tfrac{1}{2}\dfrac{mL^{2}}{3}\left(\dfrac{3v}{2L}\right)^{2} = \dfrac{mv^{2}}{8} + \dfrac{3mv^{2}}{8} = \tfrac{1}{2}mv^{2}, all the ball had. So this is an elastic collision; with a lighter rod the ball could not stop dead.