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c059741
NotesPhysicsTopic 1.3
Unit 1 · Space, time and motion · Topic 1.3

IB Physics — Work, energy and power

Topic 1.3 of IB Physics covers Work, energy and power, which is part of Unit 1: Space, time and motion. Students explore key concepts including Work done & force-distance graphs, Kinetic energy & the work-energy principle, Gravitational PE & conservation of energy, and more. A strong understanding of work, energy and power is essential for IB Physics exams and builds the foundation for connected topics across the syllabus.

Exam technique guidePractice questions

Key concepts in Work, energy and power

Key Idea: This topic is the energy toolkit: forces do work, which is stored as kinetic, gravitational or elastic energy, transferred at a rate set by power, and never destroyed — only shared out and partly wasted as heat. It is examined on both papers: quick definition and 'double the speed' MCQs on Paper 1A, and multi-step calculations (force–distance areas, slide-to-rest, falling-body speeds, spring collisions, power against drag, efficiency) on Paper 2.

📐 The six given equations

Every equation below is given in the data booklet (Theme A.3) — tap any one for the booklet entry. Knowing which to reach for is the skill, so the table after them sorts that out.

W=Fscos⁡θW = Fs\cos\thetaW=Fscosθ
Work done by a force. When the force is along the motion θ = 0 and cos 0 = 1, so W = Fs.
WWW
work done = energy transferred (J)
FFF
force applied (N)
sss
distance moved (m)
θ\thetaθ
angle between the force and the direction of motion (°)
Ek=12mv2=p22mE_k = \tfrac{1}{2}mv^{2} = \frac{p^{2}}{2m}Ek​=21​mv2=2mp2​
Kinetic energy — ½mv² when you know the speed, p²/2m when you know the momentum.
EkE_kEk​
kinetic energy — the energy of motion (J)
mmm
mass (kg)
vvv
speed (m s⁻¹)
ppp
momentum, p = mv (kg m s⁻¹)
ΔEp=mg Δh\Delta E_p = mg\,\Delta hΔEp​=mgΔh
Change in gravitational PE — equal to the kinetic energy gained in a free fall.
ΔEp\Delta E_pΔEp​
change in gravitational PE (J)
mmm
mass (kg)
ggg
gravitational field strength (≈ 9.8 N kg⁻¹ on Earth)
Δh\Delta hΔh
change in height (m)
EH=12k Δx2E_H = \tfrac{1}{2}k\,\Delta x^{2}EH​=21​kΔx2
Elastic potential energy stored in a stretched or squashed spring. Convert any cm to m before squaring Δx.
EHE_HEH​
elastic potential energy stored in the spring (J)
kkk
spring constant — the stiffness (N m⁻¹)
Δx\Delta xΔx
extension or compression from the natural length (m)
P=ΔWΔt=FvP = \frac{\Delta W}{\Delta t} = FvP=ΔtΔW​=Fv
Power. Use ΔW/Δt with energy and time; use Fv when a force moves at a steady speed (e.g. cruising against drag).
PPP
power — energy transferred per second (W = J s⁻¹)
ΔW\Delta WΔW
work done / energy transferred (J)
Δt\Delta tΔt
time taken (s)
FFF
force (N) — at constant speed, equal to the resistive force
vvv
speed in the direction of the force (m s⁻¹)
η=useful outtotal in\eta = \frac{\text{useful out}}{\text{total in}}η=total inuseful out​
Efficiency — the useful fraction of the energy (or power) supplied. Always between 0 and 1; × 100 for a %.
η\etaη
efficiency — the useful fraction (0 to 1; × 100 for a %), no unit
useful out\text{useful out}useful out
useful work or power that comes out (J or W)
total in\text{total in}total in
total work or power put in (J or W)

🧭 Which one when?

You're told…UseWatch out for
a force pushing through a distanceW = Fs cos θθ is between the force and the motion; force across the motion (90°) does no work
a force–distance grapharea under the line = workrectangle for a flat line, triangle for a sloping spring line — the area is energy (J), not a speed
mass and speed (or momentum)Eₖ = ½mv² (or p²/2m)square the speed; double v → four times the energy
a change of heightΔEₚ = mgΔhuse the vertical rise only; the mass cancels when you set mgΔh = ½mv²
a spring's stiffness and stretchEH = ½kΔx²square Δx and convert cm → m first
energy (or work) and timeP = ΔW/Δtanswer is in watts (J s⁻¹)
a steady speed against a resistive forceP = FvF here is the resistive (drag) force, since the speeds aren't changing
useful vs total energyη = useful ÷ totalalways ≤ 1; over 100% means you swapped 'useful' and 'total'

🔁 Conservation, transfers & waste

IdeaWhat it saysTypical use
Work–energy principlenet work done = change in kinetic energy (Wₙₑₜ = ΔEₖ)a push speeds an object up; friction does negative work that removes Eₖ → slide-to-rest distance
Conservation of energyfor a free fall (no air resistance) PE lost = KE gained → mgΔh = ½mv²landing speeds, pendulum swing speeds — the mass cancels
Energy transfer / degradationenergy is never lost, only moved — the wasted branch is almost always thermal energy (heat)Sankey accounting: useful + wasted branches add up to the input
When something slides to a stop, friction takes away all its kinetic energy: friction force × distance = Eₖ, so distance = Eₖ ÷ friction force.

✏️ IB-style worked examples

IB-style questionDetermine[4 marks]

A 3.0 kg trolley starts from rest on a smooth track. A constant net force of 12 N acts on it as it moves 5.0 m, shown on a force–distance graph. (a) State what the area under the graph represents. (b) Find the trolley's final speed.

🔒 Model answer plan

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

Unlock free for 7 days →
IB-style questionDetermine[3 marks]

A 0.60 kg ball falls from rest through a height of 2.0 m. Air resistance is negligible and g = 9.8 N kg⁻¹. Find its speed just before it lands.

🔒 Model answer plan

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

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IB-style questionDetermine[4 marks]

A van cruises at a steady 20 m s⁻¹ against a total resistive force of 600 N. (a) Find the useful power the van delivers to overcome drag. (b) The engine is supplied with 18 kW of power. Find its efficiency.

🔒 Model answer plan

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

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🧠 Quick self-check

Tap each card to reveal the answer.

A force acts at 90° to the motion — how much work does it do? Zero — cos 90° = 0, so W = Fs cos θ = 0 (e.g. the normal force on a sliding block).

You double an object's speed — what happens to its kinetic energy? It becomes four times as big, because the speed is squared (2² = 4).

Does a falling object's landing speed depend on its mass? No — in mgΔh = ½mv² the mass cancels, so heavy and light objects reach the same speed (no air resistance).

How does the energy stored in a spring change if you stretch it twice as far? It becomes four times as big — EH = ½kΔx² has the stretch squared.

What is the power of a vehicle cruising at constant speed? P = Fv, where F is the resistive (drag) force the engine has to balance.

Where does the 'wasted' energy in a machine usually go? Almost always to thermal energy (heat) — it isn't destroyed, just spread out and made useless.


🎯 Exam tips

Exam Tips

  • Pick the equation from what you're GIVEN: force × distance → W = Fs cos θ; mass & speed → Eₖ = ½mv²; height → ΔEₚ = mgΔh; spring stretch → EH = ½kΔx²; energy & time (or steady-speed force) → P; useful vs total → η.
  • Area under a force–distance graph = the work done — a rectangle for a flat line, a triangle for a sloping spring line. The area is energy in joules, not a speed.
  • Always square the variable that's squared: v in ½mv² and Δx in ½kΔx². Double it → four times the energy (the classic 'stopping distance' point).
  • Conservation of energy: set PE lost = KE gained → mgΔh = ½mv²; the mass cancels, so don't carry it through.
  • Slide-to-rest against friction: friction force × distance = Eₖ, so distance = Eₖ ÷ friction force.
  • At constant speed use P = Fv with F as the resistive force; convert kW ↔ W and cm ↔ m before substituting.
  • Efficiency is a fraction ≤ 1 — if you get more than 100%, you've divided total by useful instead of useful by total.

What you'll learn in Topic 1.3

  • 1.3.1 Work done & force-distance graphs
  • 1.3.2 Kinetic energy & the work-energy principle
  • 1.3.3 Gravitational PE & conservation of energy
  • 1.3.4 Elastic potential energy
  • 1.3.5 Power & efficiency
  • 1.3.6 Energy in collisions & systems (Sankey/energy transfers)
Suggested study order: Read the notes for each sub-topic below → test yourself with flashcards → attempt practice questions → review exam technique.

Study resources — 1.3 Work, energy and power

1.3.1

Work done & force-distance graphs

Notes
1.3.2

Kinetic energy & the work-energy principle

Notes
1.3.3

Gravitational PE & conservation of energy

Notes
1.3.4

Elastic potential energy

Notes
1.3.5

Power & efficiency

Notes
1.3.6

Energy in collisions & systems (Sankey/energy transfers)

Notes

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Topic 1.3 Work, energy and power forms a core part of Unit 1: Space, time and motion in IB Physics. 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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