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Conservation of energyAQA A-Level Physics: Revision notes

Section 1

The principle of conservation of energy

The principle of conservation of energy: energy cannot be created or destroyed; it can only be transferred from one form to another, or from one object to another. The total energy of an isolated system is constant.

In mechanics the key transfers are between gravitational potential energy, kinetic energy and thermal energy (also called internal energy) dissipated by work done against resistive forces. Comparing the energy at the start and at the end is the safest route to every question.

Key termsconservation of energythermal energydissipated
Common mistake

Energy is never 'lost'. Say it is dissipated or transferred to the surroundings as thermal energy.

Section 2

Gravitational potential and kinetic energy

Near the Earth's surface, where gg is constant, the change in gravitational potential energy when an object of mass mm changes height by Δh\Delta h is

ΔEp=mgΔh\Delta E_p=mg\Delta h

The kinetic energy of an object of mass mm moving at speed vv is

Ek=12mv2E_k=\tfrac12mv^2

Both are measured in joules. Kinetic energy depends on the speed squared, so doubling the speed quadruples the kinetic energy. For a 0.15 kg ball falling 3.2 m: ΔEp=0.15×9.81×3.2=4.7\Delta E_p=0.15\times9.81\times3.2=4.7 J.

Key termsgravitational potential energykinetic energy
Common mistake

Do not forget to square the speed in ½mv². Using ½mv instead is a very common slip.

Section 3

Applying conservation of energy with no resistive forces

If resistive forces are negligible, potential energy lost = kinetic energy gained:

mgΔh=12mv2  ⇒  v=2gΔhmg\Delta h=\tfrac12mv^2\;\Rightarrow\;v=\sqrt{2g\Delta h}

The mass cancels, so the speed after falling a height depends only on the height. A ball dropped from 3.2 m reaches v=2×9.81×3.2=7.9v=\sqrt{2\times9.81\times3.2}=7.9 m s⁻¹. A pendulum bob released from 0.20 m above its lowest point has speed 2×9.81×0.20=2.0\sqrt{2\times9.81\times0.20}=2.0 m s⁻¹ at the bottom, whatever its mass.

The same method works up as well as down: an object thrown upwards at speed vv rises until its kinetic energy is zero, a height v2/2gv^2/2g.

Key termsenergy transfer
Exam tip

Use energy rather than F = ma for problems where the path is curved or the acceleration changes; only the heights and speeds at the start and end matter.

Section 4

Work done against resistive forces

When resistive forces such as friction and air resistance act, some of the gravitational potential energy is dissipated as thermal energy:

energy dissipated=ΔEp−ΔEk=Fresistive×s\text{energy dissipated}=\Delta E_p-\Delta E_k=F_{resistive}\times s

where ss is the distance moved along the path, not the vertical height.

Example: a 70 kg skier descends 150 m vertically along a 600 m slope and reaches 20 m s⁻¹. ΔEp=1.03×105\Delta E_p=1.03\times10^5 J, ΔEk=1.4×104\Delta E_k=1.4\times10^4 J, so 8.9×1048.9\times10^4 J is dissipated and the mean resistive force is 8.9×104÷600≈1508.9\times10^4\div600\approx150 N.

Key termsresistive forcework done against
Common mistake

Use the distance along the slope, not the vertical height, when you work out the resistive force from F = W/s.

Section 5

Qualitative applications and bouncing

Bouncing ball. Kinetic energy at the floor is transferred to elastic energy then back to kinetic energy; some is dissipated as thermal energy and sound, so the rebound height is less. A ball dropped from 3.2 m that rebounds to 2.4 m dissipates 0.15×9.81×0.8=1.20.15\times9.81\times0.8=1.2 J.

Roller coaster. The carriage cannot rise higher than the release height if resistive forces act; with a resistive force the maximum height reached is less than the starting height, and extra energy is needed to climb a hill higher than the first.

Always describe the sequence: stored potential energy, kinetic energy, then thermal energy in the surroundings, with the total conserved.

Key termsreboundelastic energy
Exam tip

For 'explain' questions use the chain: energy store at the start, energy transferred, energy dissipated, total conserved.

Must know

  • Energy is conserved: it is transferred, never created or destroyed
  • ΔEp=mgΔh\Delta E_p=mg\Delta h and Ek=12mv2E_k=\tfrac12mv^2
  • With no resistive forces, v=2gΔhv=\sqrt{2g\Delta h} regardless of mass
  • With resistive forces, energy dissipated = ΔEp−ΔEk=F×s\Delta E_p-\Delta E_k=F\times s

That's the notes covered.

Carry on to the next subtopic.

Exam questions on Conservation of energy

  1. A ball of mass 0.15 kg is released from rest at a height of 3.2 m above a hard floor. Ignore air resistance until the ball hits the floor. Take g = 9.81 N kg⁻¹.
    The ball rebounds from the floor to a height of 2.4 m. Calculate the energy dissipated in the impact with the floor.2 marks
  2. A pendulum bob of mass 0.50 kg is held at rest with the bob 0.20 m above the lowest point of its swing, then released. Assume that air resistance and friction at the pivot are negligible. Take g = 9.81 N kg⁻¹.
    A second bob of mass 1.0 kg is released from the same height. Explain, using energy, why its speed at the lowest point is the same as that of the first bob.2 marks
  3. A skier of mass 70 kg starts from rest at the top of a straight ski slope that is 600 m long and has a vertical drop of 150 m. At the bottom of the slope the skier is moving at 20 m s⁻¹. Take g = 9.81 N kg⁻¹.
    Explain what happens to the gravitational potential energy lost by the skier.3 marks
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Written by the Exaim team, led by Shaun Daswani (Head of Upper Secondary, Improve ME Institute; MSc Financial Mathematics, Imperial College London; BSc, UCL) and Jason Daswani (operational lead, Improve ME Institute; LSE).