When the net external torque on a system is zero, the total angular momentum of the system is conserved: L_initial = L_final. Basis of figure-skater spin, planetary orbits, and rotating-bodies physics.
-- NCERT Class 11 Physics, Ch. 6, p. 6Conservation Angular Momentum
Lesson
Conservation of angular momentum is a direct consequence of Newton's second law for rotation: when the net external torque on a system is zero, the total angular momentum remains constant. Stated formally, if τ_ext = 0, then L = Iω = constant (NCERT Class 11 Physics Chapter 7, page 6).
The trap that costs marks: confusing conservation of angular momentum with conservation of rotational kinetic energy. These are different conservation laws with different conditions. When a body's moment of inertia changes through internal forces alone (no external torque), angular momentum L = Iω is conserved — but rotational kinetic energy KE = ½Iω² is NOT conserved. The internal forces do work, changing KE even as L stays fixed.
Why KE changes when L is conserved. Consider a spinning figure skater pulling her arms inward. No external torque acts, so L₁ = L₂, meaning I₁ω₁ = I₂ω₂. Since I₂ < I₁, the new angular velocity ω₂ > ω₁. Now check kinetic energy: KE₂ = L²/(2I₂) > L²/(2I₁) = KE₁. The kinetic energy increases — the skater's muscles did the work. The same logic applies to a collapsing star: as radius shrinks, I drops, ω rises, and rotational KE increases dramatically.
The deciding question for any problem: Is external torque zero? If yes → conserve L. Is there also no work done by any force? If yes → conserve KE too. In most NEET problems involving changing I, external torque is zero but internal work is done, so only L is conserved.
Watch out: if the problem gives a disc on a frictionless axle and a second disc is dropped onto it, this is an inelastic collision in rotation. L is conserved (no external torque from the axle along the rotation axis), but KE decreases — lost to friction between the surfaces during coupling.
Practice MCQs
Select an option to see the explanation. Wrong answers show why your choice was tempting — and name the exact trap it exploits.
Under what condition is the angular momentum of a system conserved?
The SI unit of angular momentum is:
A spinning figure skater pulls her arms inward. Which of the following quantities is conserved during this action?
A uniform disc of moment of inertia I is spinning at angular velocity ω about its central axis on a frictionless axle. An identical disc, initially at rest, is gently placed on top of it. After the discs reach a common angular velocity, what is the final angular velocity?
A star collapses under gravity and its radius becomes half the original value. Assuming no mass is lost and no external torque acts, the ratio of the new angular velocity to the original angular velocity is:
A particle of mass m moves with velocity v along a straight line. What is its angular momentum about a point at perpendicular distance d from the line of motion?
A disc of moment of inertia 4 kg·m² is spinning at 6 rad/s. A ring of moment of inertia 2 kg·m², initially at rest, is coaxially placed on the disc. After they reach a common angular velocity, the loss in rotational kinetic energy is:
A child of mass 30 kg stands at the edge of a merry-go-round of moment of inertia 600 kg·m² and radius 3.0 m, spinning at 2.0 rad/s. The child walks to the centre. What is the new angular velocity? (Treat the child as a point mass.)
Quick recall before you leave
Worked Example
Pattern: Body's angular speed changes when its moment of inertia changes (NEET 2025 pattern).
- 1
Given
A uniform solid sphere (a model star) has initial angular velocity ω₁ = 1.0 rad/s. Due to gravitational collapse, its radius shrinks to one-third of its original value. No mass is lost and no external torque acts during the collapse.
- 2
Required
(a) The final angular velocity ω₂. (b) The ratio of final to initial rotational kinetic energy, KE₂/KE₁.
- 3
Concept
When external torque is zero, angular momentum is conserved: I₁ω₁ = I₂ω₂. However, rotational KE is NOT conserved because internal gravitational forces do work during the collapse.
- 4
Formula
- Moment of inertia of a solid sphere: I = (2/5)MR² - Conservation of L: I₁ω₁ = I₂ω₂ - KE_rot = ½Iω² = L²/(2I)
- 5
Substitution
I₁ = (2/5)M R², I₂ = (2/5)M(R/3)² = (2/5)M(R²/9) = I₁/9. From L conservation: I₁ω₁ = (I₁/9)ω₂.
- 6
Calculation
ω₂ = 9ω₁ = 9 × 1.0 = 9.0 rad/s. KE₁ = ½I₁ω₁² = ½I₁(1.0)² = 0.5 I₁. KE₂ = ½I₂ω₂² = ½(I₁/9)(81) = ½ × 9 I₁ = 4.5 I₁. KE₂/KE₁ = 4.5 I₁ / 0.5 I₁ = 9. **Note on exact constants:** The fractions 2/5 and 1/9 are geometric constants of the sphere and the problem statement respectively. The angular velocity 1.0 rad/s is given as exact. These do not limit significant figures. The factor 9 in the final answer is exact.
- 7
Final answer
(a) ω₂ = 9.0 rad/s. (b) KE₂/KE₁ = 9. The rotational kinetic energy increases ninefold — the gravitational potential energy released during collapse does this work.
- 8
Common trap
A common confusion is to assume KE is also conserved when L is conserved. If you set ½I₁ω₁² = ½I₂ω₂², you would get ω₂ = 3ω₁ (from ω₂ = ω₁√(I₁/I₂) = ω₁ × 3), which contradicts L conservation. The correct approach is to apply L conservation first (ω₂ = 9ω₁), then compute KE separately.
- 9
Similar NEET-style question
A ballet dancer with arms extended has moment of inertia 4.0 kg·m² and spins at 3.0 rev/s. She pulls her arms in, reducing her moment of inertia to 1.0 kg·m². Find her new spin rate and the ratio of her final to initial rotational kinetic energy. (Answer: 12 rev/s; KE ratio = 4.) ---
Before solving, remember these
Formulas
8 formulas — click to collapse
Angular momentum
For a particle: L = r x p. For a rigid body about its rotation axis: L = I omega. Vector quantity.
| Symbol | Quantity | SI Unit |
|---|---|---|
| L | angular momentum | kg*m^2/s |
| I | moment of inertia | kg*m^2 |
| omega | angular velocity | rad/s |
Valid when
- Reference point/axis chosen
- I about same axis as omega
Centre of mass of n-particle system
The position of the centre of mass equals the mass-weighted average of particle positions. For continuous bodies use integral form.
| Symbol | Quantity | SI Unit |
|---|---|---|
| R_cm | CoM position | m |
| m_i | mass of i-th particle | kg |
| r_i | position of i-th particle | m |
Valid when
- System of point particles or rigid body
- Inertial reference frame
Moment of inertia for common rigid bodies
Standard moments of inertia about the symmetry axis. For other axes use parallel/perpendicular axes theorems.
| Symbol | Quantity | SI Unit |
|---|---|---|
| M | mass | kg |
| R | radius | m |
| L | length | m |
| I | moment of inertia | kg*m^2 |
Valid when
- Uniform mass distribution
- Rotation about symmetry axis (unless noted)
Parallel axes theorem
Moment of inertia about any axis = moment about parallel axis through CM + Md^2.
| Symbol | Quantity | SI Unit |
|---|---|---|
| I | MOI about given axis | kg*m^2 |
| I_cm | MOI about parallel CM axis | kg*m^2 |
| M | total mass | kg |
| d | perpendicular distance | m |
Valid when
- Both axes parallel
- I_cm known about CM axis
Perpendicular axes theorem (planar)
For planar lamina: MOI about axis perpendicular to plane = sum of MOI about two perpendicular in-plane axes through same point.
| Symbol | Quantity | SI Unit |
|---|---|---|
| I_z | MOI perp to plane | kg*m^2 |
| I_x, I_y | MOI in plane | kg*m^2 |
Valid when
- Body is planar (2D lamina)
- All three axes intersect at one point
Rotational kinematic equations (constant alpha)
Rotational analogues of linear kinematic equations under constant angular acceleration.
| Symbol | Quantity | SI Unit |
|---|---|---|
| omega | angular velocity | rad/s |
| alpha | angular acceleration | rad/s^2 |
| theta | angular displacement | rad |
| t | time | s |
Valid when
- Constant alpha
- Single rotation axis
Rotational kinetic energy
Energy of rotation about an axis. Adds to translational KE for rolling bodies.
| Symbol | Quantity | SI Unit |
|---|---|---|
| I | moment of inertia | kg*m^2 |
| omega | angular velocity | rad/s |
Valid when
- Rotation about fixed axis
- I and omega about same axis
Torque (moment of force)
Cross product of position vector and force vector. Magnitude r F sin(theta).
| Symbol | Quantity | SI Unit |
|---|---|---|
| tau | torque | N*m |
| r | position from pivot | m |
| F | force | N |
| theta | angle between r and F | rad |
Valid when
- Rigid body or extended object
- r measured from chosen pivot/axis
Exam Traps & Common Mistakes
These are the exact patterns that cause wrong answers in NEET. Each trap includes when it triggers and how to avoid it.
7 items — click to collapse
Category: Overthinking
Student answers L/2 for two-particle CoM regardless of mass ratio.
When it triggers
Question gives two masses on rigid rod and asks for CoM distance.
How to avoid
R_cm from m1 = m2*L/(m1+m2). Heavier mass pulls CoM closer to it.
Category: Similar Terms
Student conserves rotational KE when angular momentum is conserved (or vice versa). When I changes, L = Iω is conserved but KE = ½Iω² is NOT (it depends on I and ω together).
When it triggers
Question describes a body whose moment of inertia changes (skater pulling arms in, star collapsing).
How to avoid
L conservation requires zero external torque. KE conservation requires no work done — different criteria. When I changes via internal forces, L conserved, ω increases, KE increases.
Category: Similar Terms
Student confuses 2/5 (solid sphere) with 2/3 (hollow sphere) or 1/2 (disc) with 1 (ring).
When it triggers
Question gives a specific geometry and asks for I or radius of gyration.
How to avoid
Memorise: solid sphere 2/5, hollow sphere 2/3, disc/cylinder 1/2, ring/hoop 1, rod-centre 1/12, rod-end 1/3.
Category: Unit Conversion
Student plugs rpm directly into formulas requiring rad/s. 1 rpm = 2π/60 rad/s.
When it triggers
Question gives ω in rpm and asks for kinematic quantities in SI units.
How to avoid
Convert: ω(rad/s) = (2π/60) × rpm. Always check units before substituting.
Root cause: concept gap
Correction
L = Iω is conserved when external torque is zero. KE = ½Iω² is NOT conserved when I changes (since ω changes too). When skater pulls arms in, L conserved, ω increases, KE increases (work done by muscles).
Root cause: concept gap
Correction
Memorise standard moments of inertia. Solid sphere has more mass near axis (smaller MOI = 2MR²/5); hollow sphere has all mass at radius R (larger MOI = 2MR²/3).
Root cause: unit error
Correction
Convert: ω(rad/s) = (2π/60) × ω(rpm). For example, 1200 rpm = 1200 × 2π/60 = 125.66 rad/s.
Past Year Questions
10 questions from NEET 2021, 2022, 2023, 2024, 2025. Answers verified against NTA official keys. — click to collapse
The angular acceleration of a body, moving along the circumference of a circle, is
How NEET usually asks this
4 recurring patterns from past papers — click to collapse
Flywheel undergoing uniform angular acceleration; given initial/final omega and time, find alpha or theta.
Common distractors
forgets conversion rpm to rad s
Treats rpm as rad/s without 2*pi/60 conversion
Two-particle system on a rigid massless rod; find distance of CM from one of the masses. R_cm from m1 = m2*L/(m1+m2).
Common distractors
uses equal distribution
Default to L/2 regardless of mass ratio
Body's angular speed changes when its moment of inertia changes (e.g. star collapses, skater pulls in arms). Apply L = I*omega = constant when no external torque.
Common distractors
uses energy conservation instead
Confusing L conservation with KE conservation
Compare moments of inertia (or radii of gyration) of two standard rigid bodies (e.g. solid sphere vs hollow sphere; disc vs ring) about their natural axes. Apply tabulated I formulas; take ratio.
Common distractors
swap solid hollow coefficients
Confusing 2/5 (solid sphere) with 2/3 (hollow sphere)
Sources
Test yourself on this topic with real past-paper questions:
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