Topic Overview

What students will cover

This topic brings the mechanics ideas together through energy transfer and rate of working. You should be able to move between force, displacement, kinetic energy, gravitational potential energy, power, and efficiency without treating each equation as a separate trick.

This is a shorter Side A topic, so keep the progression clear as you revise. Start with work and energy, then practise conservation and energy-change calculations before using power and efficiency to judge how quickly and how usefully energy is transferred.

Revision

Topic revision route

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Recall vocabulary

  • work done

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • energy transfer

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  • conservation of energy

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • gravitational potential energy

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • kinetic energy

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • Power

    work done per unit time.

  • efficiency

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • P = W/t

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • P = Fv

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

Resource bank

Lesson resources
9
Topic resources
1

Open the relevant lesson first, then use its linked slides, worksheets, simulations, or practice tasks.

Syllabus

CIE 9702 coverage in this topic

11 points across 3 lessons

Show details
5.1.1

understand the concept of work, and recall and use work done = force × displacement in the direction of the force

5.1.2

recall and apply the principle of conservation of energy

5.1.3

recall and understand that the efficiency of a system is the ratio of useful energy output from the system to the total energy input

5.1.4

use the concept of efficiency to solve problems

5.1.5

define power as work done per unit time

5.1.6

solve problems using P = W / t

5.1.7

derive P = Fv and use it to solve problems

5.2.1

derive, using W = Fs, the formula ∆EP = mg∆ h for gravitational potential energy changes in a uniform gravitational field

5.2.2

recall and use the formula ∆EP = mg∆ h for gravitational potential energy changes in a uniform gravitational field 1

5.2.3

derive, using the equations of motion, the formula for kinetic energy EK = 2 mv2 1

5.2.4

recall and use EK = 2 mv2

Lessons

Lesson sequence

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Shared Materials

Optional topic materials

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