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Class 9–10 · Physics

Work, power and energy

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Work, power and energy

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.
Lessons in this chapter
  1. Work and direction
  2. Kinetic energy
  3. Potential energy
  4. Conservation of energy
  5. Power
  6. Efficiency
  7. Energy resources
  8. Levers and pulleys

Lessons

1

Work and direction

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Work uses the component of displacement parallel to force. It is positive along force, negative against it and zero perpendicular to it. Holding an object still does no mechanical work on it despite biological energy use.

Key relationship

W = Fs cosθ; 1 J = 1 N m

Worked example

10 N over 4 m ⇒ 40 J; friction 3 N opposite ⇒ −12 J; net 28 J

2

Kinetic energy

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Motion gives an object kinetic energy. Doubling speed quadruples it. Net work equals the change in kinetic energy, obtained by combining F = ma with the constant-acceleration relation v²−u² = 2as.

Key relationship

Ek = ½mv²; Wnet = ΔEk

Worked example

m = 2 kg: at 3 m/s ⇒ 9 J; at 6 m/s ⇒ 36 J; required net work 27 J

3

Potential energy

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Potential energy belongs to a configuration. Near Earth's surface its gravitational change is mgΔh relative to a chosen level. A stretched spring also stores energy. Only energy differences matter in these comparisons.

Key relationship

Ep = mgh; spring energy = ½kx²

Worked example

2 kg lifted 1.5 m ⇒ ΔEp = 2 × 9.8 × 1.5 = 29.4 J

4

Conservation of energy

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Energy transfers and changes form. During an ideal fall, potential energy becomes kinetic energy. Friction transfers mechanical energy into thermal energy and sound; total energy remains conserved.

Key relationship

no resistance: mgh = ½mv² ⇒ v = √(2gh)

Worked example

h = 5 m ⇒ v = √98 ≈ 9.9 m/s

5

Power

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Power is the rate of doing work or transferring energy. The same task completed faster requires more average power. For aligned force and velocity, instantaneous mechanical power is Fv. Total energy also depends on operating time.

Key relationship

P = W/t; 1 W = 1 J/s

Worked example

600 J in 3 s ⇒ 200 W; in 6 s ⇒ 100 W

6

Efficiency

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Efficiency is useful output divided by total input. Practical devices transfer some energy into unwanted forms. Compare energy totals or powers over a consistent interval.

Key relationship

η = useful output/input × 100%

Worked example

Input 500 J, useful 350 J ⇒ η = 70%; other transfers = 150 J

7

Energy resources

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

Sunlight, wind and flowing water are renewable resources; fossil fuel reserves are finite. Solar cells convert light directly, while hydropower drives a turbine. Evaluate environmental effects, reliability and storage rather than only the energy label.

Key relationship

E = Pt; 1 kWh = 3.6 × 10⁶ J

Worked example

100 W × 5 h = 0.1 kW × 5 h = 0.5 kWh

8

Levers and pulleys

mgh½mv²
In an ideal descent, gravitational potential energy becomes kinetic energy.

A lever balances moments about its pivot. A fixed pulley changes force direction; moving pulleys can distribute the load across supporting rope sections. A force advantage is exchanged for a greater effort distance, not free energy.

Key relationship

MA = load/effort; VR = effort distance/load distance; η = MA/VR × 100%

Worked example

Ideal moving pulley: 200 N load on 2 strands ⇒ effort 100 N; 1 m lift requires 2 m rope travel

Check your understanding

Try answering first, then open the question to compare your reasoning.

1. Triple speed: kinetic-energy factor?

Ek ∝ v² ⇒ 9

2. 20 N perpendicular to 5 m displacement: work?

W = 20 × 5 × cos90° = 0 J

3. 800 J in 4 s: power?

P = 800/4 = 200 W

4. 500 J input, 400 J useful: efficiency?

400/500 × 100 = 80%

5. Does mass affect ideal fall speed from a fixed height?

mgh = ½mv² ⇒ v = √(2gh), independent of m

Sources and scope

Original GetReady teaching notes. The 13 core chapters follow the existing site sequence. Physics to save life is an explicitly labelled older-edition supplement. Check your current book and board instructions for examination scope. Illustrations are schematic. Unless stated otherwise, use g = 9.8 m/s². A physics teacher should review content and edition coverage before it is relied on.