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Space, Time, and Motion

Kinematics, momentum, rotation and relativity — the five subtopics examiners love to combine

Diagram linking linear and rotational mechanics with a spacecraft firing thrusters
Subject
Physics
Curriculum
IB Diploma Programme
Grade
DP
Topic
Space, Time, and Motion
Reading
8 min
Difficulty
Advanced

Quick facts

Difficulty
★★★★☆
Exam weight
Core Topic A — appears in every paper
Prerequisites
Vectors, basic algebra, SUVAT equations
You'll learn
Momentum, torque, angular momentum, relativistic momentum
HL extensions
Rigid body mechanics & special relativity
Revision time
2-3 hours

Space, Time and Motion is IB DP Physics' Topic A, and it rewards students who see the pattern underneath the equations rather than memorising formulas in isolation. At SL, you master kinematics, forces and momentum, and work-energy-power in their familiar linear form. At HL, the same physics gets rotated into rigid body mechanics — where torque, moment of inertia and angular momentum mirror force, mass and momentum exactly — and boosted to relativistic speeds in special relativity, where momentum stops being simply . Examiners routinely layer these ideas: a question might start as a straightforward collision and finish by asking for angular momentum or relativistic effects. This teaser walks through the five concepts that show up most often, the traps built into IB-style questions, and the sign conventions and symbolic-first habits that protect your marks. For the full worked examples, data-booklet formulas and standard shapes table, head to the complete revision notes.

What you’ll be able to do

Distinguish the five subtopics of Space, Time and Motion and how SL/HL differ
Apply the general form of Newton's second law, $F=\Delta p/\Delta t$
Use impulse as the area under a force-time graph, including non-constant force
Apply conservation of momentum correctly using signed velocities
Translate linear mechanics formulas into their rotational twins (HL)
Explain why moment of inertia depends on axis, not just mass
State when and why momentum becomes relativistic, $p=\gamma mv$ (HL)
Identify examiner traps involving unnecessary given quantities
1

The Big Picture: Five Subtopics, One Exam Strategy

SL students meet kinematics, forces/momentum, and work-energy-power in clean linear form. HL students get the exact same physics twice more: rotated into rigid body mechanics, and boosted to near-light speeds in special relativity. Examiners love layering subtopics — a question can begin as a basic SUVAT problem and end by asking for angular momentum, or start as a momentum collision and finish asking for energy released as rest mass.

Mind map of the five Space, Time and Motion subtopics

Exam tip

Read the whole question before choosing a formula — the final part often needs a completely different subtopic than the opening.

Mini summary

Five subtopics, same underlying physics — SL in linear form, HL adds rotation and relativity.

2

Forces and Momentum: Newton's Second Law Beyond F = ma

The deepest form of Newton's second law is , not — the mass-times-acceleration version only works when mass stays constant. Momentum is always conserved for an isolated system regardless of whether a collision is elastic, but momentum is a vector, so direction is where most marks disappear. Impulse equals the area under a force-time graph, which for a non-constant force means finding the actual area, not multiplying a single force value by time.

Two trolleys colliding with signed velocity vectors and a force-time graph

Exam tip

'Show that' momentum questions want the symbolic conservation equation written out first, values substituted second — jumping to a decimal loses the method mark.

Common mistake

Treating momentum as a scalar and adding magnitudes when objects move in opposite directions, instead of assigning signed velocities from the start.

Mini summary

F=Δp/Δt is the real Newton's second law; momentum conserves in every isolated collision, but always with signs.

3

Rigid Body Mechanics (HL): The Rotational Mirror World

Every linear quantity has a rotational twin: mass becomes moment of inertia, force becomes torque, momentum becomes angular momentum. The genuinely new idea is that moment of inertia depends on how mass is arranged relative to the rotation axis — doubling the radius at which mass sits quadruples its contribution to , since it scales as . Angular momentum is conserved whenever net external torque is zero, exactly like linear momentum, and rolling without slipping links the two worlds via .

Spinning flywheel with torque, radius and moment of inertia labelled
Linear quantityRotational twin
Force, Torque,
Mass, Moment of inertia,
Momentum, Angular momentum,
Velocity, Angular velocity,
Acceleration, Angular acceleration,

Exam tip

If a question gives three quantities but only two are needed, that's deliberate — check whether answers it directly without ever needing .

Common mistake

Writing or mixing linear and rotational formulas — always write the rotational equation in full symbolic form (, ) before substituting numbers.

Mini summary

F→τ, m→I, p→L, v→ω — same physics, rotated, with I depending on axis and mass distribution.

4

Special Relativity at HL: When Momentum Isn't p = mv

Once speed becomes a significant fraction of the speed of light , momentum is no longer simply — it becomes . This relativistic momentum only reduces back to the classical formula when , since in that limit. This extension is examined within the kinematics and energy strands rather than as a fully separate block, so expect it folded into questions that start with everyday mechanics.

Graph of relativistic momentum against velocity approaching the speed of light

Exam tip

Check the size of relative to before deciding which momentum formula applies — classical is only ever an approximation.

Mini summary

Relativistic momentum p=γmv replaces p=mv only when v is a significant fraction of c.

5

Work, Energy and Power: The Third Conserved Quantity

Work is the energy transferred by a force acting through a displacement, and the work-energy theorem links the net work done on an object directly to its change in kinetic energy. This subtopic sits alongside kinematics and momentum as the third pillar of SL mechanics, tracking how much 'oomph' is transferred between objects and systems. Together with momentum conservation, work-energy reasoning is the standard toolkit for combined mechanics problems.

Force applied through a displacement showing work done and resulting change in kinetic energy

Exam tip

When a problem mixes momentum and energy, check first whether the collision is elastic — only then does kinetic energy stay conserved alongside momentum.

Mini summary

Work transfers energy through a force acting over a displacement; net work equals the change in kinetic energy.

Quick formula sheet

Torque of a force F applied at radius r, angle theta between r and FTorque is force with leverage — bigger radius or angle, bigger turning effect
Rotational form of Newton's second lawSwap F→τ, m→I, a→α from the linear version
Angular momentum, the rotational analogue of linear momentum p=mv
Angular impulse-momentum theorem, the rotational twin of Δp = FΔtOften the fastest route — skips I entirely if it isn't needed
Rotational kinetic energy
Links translational speed to angular speed for rolling without slipping
General form of Newton's second law, valid even when mass changes
Impulse-momentum theorem; equals the area under a force-time graph
Conservation of momentum for an isolated system
Relativistic momentum (HL only); reduces to p=mv when v is much less than c

Practice questions

Easy
  1. Define torque and state its SI unit.
  2. Write the general (most fundamental) form of Newton's second law in terms of momentum.
  3. State the two quantities that are always conserved in an elastic collision.
Medium
  1. A wheel with moment of inertia 0.20 kg m² experiences a constant torque of 0.50 N m for 4.0 s, starting from rest. Find its angular momentum after this time.
  2. A ball of mass 0.50 kg moving at 4.0 m/s collides head-on with a stationary 0.50 kg ball and they stick together. Find their common velocity after the collision.
  3. Explain why relativistic momentum reduces to at everyday speeds.
Challenge
  1. A spacecraft applies a constant torque of 15 N m for 5.0 s to a rotor with moment of inertia 300 kg m². Explain why the moment of inertia value is irrelevant if the question only asks for the change in angular momentum.
  2. A cylinder rolls without slipping down a slope. Explain how connects its translational and rotational motion.
  3. Two objects collide and momentum is conserved but kinetic energy is not. Explain what this tells you about the type of collision and where the missing energy has gone.

Frequently asked questions

What's the difference between SL and HL Space, Time and Motion?+

SL covers kinematics, forces/momentum, and work-energy-power in linear form. HL adds two extra standalone blocks: rigid body mechanics and special relativity, examined alongside the SL content.

Is torque the rotational equivalent of force?+

Yes — torque, , plays exactly the role for rotation that force plays for linear motion, and it's torque, not force alone, that changes angular velocity.

Why does moment of inertia depend on the rotation axis?+

Moment of inertia depends on how mass is distributed relative to a specific axis, not just total mass, so the same object can have different I values for different axes.

When does momentum become relativistic in IB Physics?+

Once speed v becomes a significant fraction of the speed of light c, momentum is rather than ; the classical formula is only an approximation for v much less than c.

Do IB exam questions combine these subtopics?+

Yes — expect questions that begin as a SUVAT or momentum problem and finish by asking for angular momentum or a relativistic quantity, so read the full question before choosing a formula.

What's the fastest way to solve angular impulse problems?+

Use directly whenever torque and time are given — it often lets you skip finding moment of inertia or angular velocity entirely.

Master Space, Time and Motion with the full DP Physics revision notes

Complete data-booklet formulas plus the standard moment of inertia shapes table Fully worked examples showing the exact examiner traps in context Step-by-step guidance on combining momentum, rotation and relativity in one question Practice questions with clear method structure for full exam-style mock papers
Get the Space, Time, and Motion notes on RevisionPrep

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