aimnova.
DashboardMy LearningPaper MasteryStudy Plan

Stay in the loop

Study tips, product updates, and early access to new features.

aimnova.

AI-powered IB study platform with personalised plans, instant feedback, and examiner-style marking.

IB Subjects
  • All IB Subjects
  • IB Diploma
  • IB ESS
  • IB Economics
  • IB Business Management
  • IB Math AI
  • IB Math AA
Question Banks
  • ESS Question Bank
  • Economics Question Bank
  • Business Management Question Bank
  • Math AI Question Bank
  • Math AA Question Bank
Predicted Topics 2026
  • ESS Predictions 2026
  • Economics Predictions 2026
  • Business Management Predictions 2026
  • Math AI Predictions 2026
  • Math AA Predictions 2026

Study Resources

  • Free Study Notes
  • Mock Exams
  • Revision Guide
  • Flashcards
  • Exam Skills
  • Command Terms
  • Past Paper Feedback
  • Grade Calculator
  • Exam Timetable 2026

Company

  • Features
  • Pricing
  • About Us
  • Blog
  • Contact
  • Terms
  • Privacy
  • Cookies

© 2026 Aimnova. All rights reserved.

Made with 💜 for IB students worldwide

v0.1.1039
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?


🔁 Conservation, transfers & waste

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 question — work from a graph, then a speed

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.

Solution:

  1. (a) The area under a force–distance graph is the work done by the force:

    area=W=Fs=12×5.0=60 J\text{area} = W = Fs = 12 \times 5.0 = 60\ \text{J}area=W=Fs=12×5.0=60 J
  2. (b) From rest, all this work becomes kinetic energy — use the given formula:

    Ek=12mv2E_k = \tfrac{1}{2}mv^{2}Ek​=21​mv2
  3. Set Eₖ = 60 J, put in m = 3.0 and solve for v:

    60=12×3.0×v2  ⇒  v2=4060 = \tfrac{1}{2}\times 3.0 \times v^{2} \;\Rightarrow\; v^{2} = 4060=21​×3.0×v2⇒v2=40
  4. Take the square root — keep the unit:

    v=40=6.3 m s−1v = \sqrt{40} = 6.3\ \text{m s}^{-1}v=40​=6.3 m s−1
Final answer:

(a) the work done on the trolley (= 60 J); (b) v = 6.3 m s⁻¹. The area gives energy in joules — you still need ½mv² to get the speed.

IB-style question — falling-body speed (mass cancels)

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.

Solution:

  1. Energy is conserved, so set the PE lost equal to the KE gained:

    mg Δh=12mv2mg\,\Delta h = \tfrac{1}{2}mv^{2}mgΔh=21​mv2
  2. The mass cancels — put in g = 9.8 and Δh = 2.0:

    9.8×2.0=12v2  ⇒  v2=39.29.8 \times 2.0 = \tfrac{1}{2}v^{2} \;\Rightarrow\; v^{2} = 39.29.8×2.0=21​v2⇒v2=39.2
  3. Take the square root — keep the unit:

    v=39.2=6.3 m s−1v = \sqrt{39.2} = 6.3\ \text{m s}^{-1}v=39.2​=6.3 m s−1
Final answer:

v = 6.3 m s⁻¹ — and it would be the same for any mass, because m cancels out.

IB-style question — power against drag, then efficiency

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.

Solution:

  1. (a) At constant speed the driving force equals the resistive force, so use the given P = Fv:

    P=Fv=600×20=12 000 W=12 kWP = Fv = 600 \times 20 = 12\,000\ \text{W} = 12\ \text{kW}P=Fv=600×20=12000 W=12 kW
  2. (b) Efficiency is the useful power out over the total power in — use the given formula:

    η=useful outtotal in=1218\eta = \frac{\text{useful out}}{\text{total in}} = \frac{12}{18}η=total inuseful out​=1812​
  3. Work it out, then × 100 for a percentage:

    η=0.67=67%\eta = 0.67 = 67\%η=0.67=67%
Final answer:

(a) 12 kW; (b) η ≈ 0.67 (67%). The other ~6 kW is wasted, mostly as thermal energy (heat).


🧠 Quick self-check

Tap each card to reveal the answer.


🎯 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

Ready to study Work, energy and power?

Get AI-powered practice questions, personalised feedback, and a study planner tailored to your IB Physics exam date.

Start studying free

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.

Previous topic
1.2 Forces and momentum
Next topic
2.1 Thermal energy transfers
All Physics topics
Exam technique

Ready to practice?

Get AI-graded practice questions, mock exams, flashcards, and a personalised study plan — all aligned to your IB syllabus.

Start Studying Free

No credit card required · Cancel anytime