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NotesPhysics HLTopic 1.4
Unit 1 · Space, time and motion · Topic 1.4

IB Physics HL — Rigid body mechanics (HL)

Topic 1.4 of IB Physics covers Rigid body mechanics (HL), which is part of Unit 1: Space, time and motion. Students explore key concepts including Torque and rotational motion, Moment of inertia, Conservation of angular momentum. A strong understanding of rigid body mechanics (hl) is essential for IB Physics HL exams and builds the foundation for connected topics across the syllabus.

Higher Level students should use this topic hub as a map: start with the shared sub-topics, then follow the HL-only extensions and exam-skill links where this topic asks for deeper analysis.

Exam technique guidePractice questions

Key concepts in Rigid body mechanics (HL)

Key Idea: Watch an ice skater pull in their arms and whirl faster, or a spanner turn a stubborn bolt — that is rigid body mechanics, the rotational twin of straight-line motion. Every idea you know for motion in a line has a spinning version — swap distance for angle, mass for moment of inertia, force for torque, momentum for angular momentum. Learn the dictionary once and the whole topic falls into place. It is HL only and appears on Paper 1A (quick one-liners) and Paper 2 (a multi-step rotational problem).

🔄 The rotation–translation dictionary

Straight-line motionRotational motion
displacement sangle turned θ (rad)
velocity vangular velocity ω
acceleration aangular acceleration α
mass mmoment of inertia I = Σmr²
force Ftorque τ = Fr sinθ
F = maτ = Iα
momentum p = mvangular momentum L = Iω
kinetic energy ½mv²rotational KE ½Iω²

📐 The formulas you're given

τ=Frsin⁡θI=∑mr2τ=Iα\tau = F r \sin\theta \qquad I = \sum m r^{2} \qquad \tau = I\alphaτ=FrsinθI=∑mr2τ=Iα
τ\tauτ
torque (N m) — the turning effect of a force
III
moment of inertia (kg m²) — rotation's mass
α\alphaα
angular acceleration (rad s⁻²)
L=IωEk=12Iω2L = I\omega \qquad E_{k} = \tfrac{1}{2} I \omega^{2}L=IωEk​=21​Iω2
LLL
angular momentum (kg m² s⁻¹) — conserved if no external torque
EkE_{k}Ek​
rotational kinetic energy (J)
ω\omegaω
angular velocity (rad s⁻¹)
1. A body is balanced (rotational equilibrium) when the clockwise torques equal the anticlockwise torques about any point: Στ = 0. 2. Spin is conserved. With no external torque, I₁ω₁ = I₂ω₂ — pull mass inward (smaller I) and the spin speeds up (the ice-skater).

✏️ IB-style worked examples (one per micro)

IB-style questionDetermine[3 marks]

A uniform beam of length 3.0 m and weight 200 N is hinged to a wall and held horizontal by a vertical cable at its far end. Determine the tension in the cable.

🔒 Model answer plan

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IB-style questionDetermine[4 marks]

A solid disc (I = ½MR²) has mass 4.0 kg and radius 0.30 m. A net torque of 1.8 N m acts on it. Determine its angular acceleration.

🔒 Model answer plan

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IB-style questionDetermine[3 marks]

A turntable (I = 0.50 kg m²) spins freely at 12 rad s⁻¹. A lump of clay dropped on it adds 0.10 kg m² to the moment of inertia. Determine the new angular velocity.

🔒 Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

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Important: 1. Work in radians, not degrees — and convert revolutions with × 2π. 2. In I = Σmr² the distance is squared — never forget to square r. 3. When two objects stick (clay on a disc), angular momentum is conserved but kinetic energy is NOT — use I₁ω₁ = I₂ω₂, never energy conservation.

Tap each card to reveal the answer.

What is the rotational version of mass? Moment of inertia, I = Σmr² — it measures how hard a body is to spin up, and depends on how far the mass sits from the axis.

When is a rigid body balanced? In rotational equilibrium: the total torque about any point is zero (Στ = 0), clockwise = anticlockwise.

A skater pulls their arms in. What happens to their spin? It speeds up. I decreases, so ω increases to keep L = Iω constant (no external torque).

Torque of a 12 N force 0.40 m from the pivot, at 90°? 4.8 N m — τ = Fr sinθ = 12 × 0.40 × sin90°.

A hoop and a disc have the same M and R — which has more I? The hoop (I = MR²); the disc is ½MR², because its mass is spread inward.

Double a flywheel's angular velocity — what happens to its rotational KE? It quadruples — Eₖ = ½Iω², and ω is squared.

Exam tips

  • Build the rotation–translation dictionary in your head; then every rotational question is one you already know.
  • Take torques about an unknown force's line so it drops out of the equation.
  • Spot 'no external torque' → conserve angular momentum (I₁ω₁ = I₂ω₂), not energy.
  • The exam gives you the shape's moment-of-inertia formula — recognise it and substitute.
  • Carry units throughout: N m for torque, kg m² for I, kg m² s⁻¹ for L.

What you'll learn in Topic 1.4

  • 1.4.1 Torque and rotational motion
  • 1.4.2 Moment of inertia
  • 1.4.3 Conservation of angular momentum
Suggested study order: Read the notes for each sub-topic below → test yourself with flashcards → attempt practice questions → review exam technique.

Study resources — 1.4 Rigid body mechanics (HL)

1.4.1

Torque and rotational motion

Notes
1.4.2

Moment of inertia

Notes
1.4.3

Conservation of angular momentum

Notes

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Topic 1.4 Rigid body mechanics (HL) forms a core part of Unit 1: Space, time and motion in IB Physics HL. Mastering these concepts will strengthen your understanding of connected topics across the syllabus and prepare you for exam questions that require analysis, evaluation, and real-world application.

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