Year 8 Physics

Energy, Space & Forces

Explore how energy moves through materials, discover our place in the Universe, and understand the forces that shape our world.

8 Topics 2 Simulations 8 Practice Questions
1

Energy Transfer

How thermal energy moves

Heat vs Temperature

These terms are often confused but mean different things:

Thermal Energy (Heat)

The total energy of all particles in an object. Measured in Joules (J). Depends on mass AND temperature.

A bath of warm water has MORE thermal energy than a cup of boiling water!

Temperature

How hot or cold something is. Measured in °C or K. Related to the average kinetic energy of particles.

A cup of boiling water is HOTTER than a bath of warm water!

Three Ways Energy Transfers

Conduction

Particles vibrate and pass energy to neighbours. Mainly in solids. Metals are best conductors.

Spoon in hot tea gets warm

Convection

Hot fluid rises, cold fluid sinks. Creates convection currents. Only in liquids and gases.

Radiator heating a room

Radiation

Infrared waves travel through space. No particles needed! All hot objects emit radiation.

Heat from the Sun reaching Earth

2

Conservation of Energy

Energy cannot be created or destroyed

The Law of Conservation of Energy

Energy cannot be created or destroyed. It can only be transferred from one store to another, or between objects.

Total energy input = Total energy output

This means the total amount of energy in the Universe is constant! When energy seems to "disappear", it has actually been transferred to another form, often as thermal energy (heat).

Sankey Diagrams

Sankey diagrams show energy transfers. The width of arrows represents the amount of energy:

100J Energy In Useful: 40J (Light) Wasted: 60J (Heat) Light Bulb

The thicker the arrow, the more energy. Wasted energy is usually shown going downward or to the right.

Efficiency

Efficiency tells us what fraction of energy is usefully transferred:

Efficiency = Useful Energy Output ÷ Total Energy Input

Efficiency = Useful Power Output ÷ Total Power Input

LED light bulb: ~80-90% efficient. Only 10-20% wasted as heat.

Incandescent bulb: ~5-10% efficient. 90-95% wasted as heat!

3

States of Matter

Expansion and density changes

Thermal Expansion

When materials are heated, particles vibrate more and take up more space. The material expands.

  • Solids: Expand slightly when heated
  • Liquids: Expand more than solids
  • Gases: Expand the most when heated

Application: Gaps in bridges allow for expansion in summer heat!

Density Changes

When materials expand, the same mass takes up more volume, so density decreases.

Density = Mass ÷ Volume

Hot water is less dense than cold water, so it rises - this causes convection currents!

The Anomalous Expansion of Water

Water behaves unusually near its freezing point. It's most dense at 4°C, not 0°C!

❄️

Ice (0°C)

Least dense - floats!

💧

Water (4°C)

Most dense - sinks

🌡️

Warm water

Less dense - rises

This is why ice forms on top of ponds, allowing fish to survive underneath!

4

The Solar System

Our cosmic neighbourhood

Historical Models

Geocentric Model (Ptolemy)

Earth at the centre, everything orbits around Earth.

Incorrect - but believed for 1400+ years

Heliocentric Model (Copernicus)

Sun at the centre, Earth and planets orbit the Sun.

Correct - our current understanding

The Eight Planets

Click on a planet to learn more about it:

Click a planet to see details

5

Beyond the Solar System

Stars, galaxies, and the Universe

Stars

A star is a massive ball of hot gas that produces its own light and heat through nuclear reactions.

  • • Our Sun is a medium-sized star
  • • Stars appear small because they are very far away
  • • Different colours indicate different temperatures
🌌

Galaxies

A galaxy is a huge collection of billions of stars, gas, and dust held together by gravity.

  • • Our galaxy is called the Milky Way
  • • Contains 100-400 billion stars
  • • Different shapes: spiral, elliptical, irregular

Scale of the Universe

🌍
Earth
☀️
Solar System
Milky Way
🌐
Universe

A light year is the distance light travels in one year (about 9.5 trillion km!)

6

Gravity & Orbits

The force that shapes the cosmos

Weight vs Mass

Mass

The amount of matter in an object. Never changes. Measured in kilograms (kg).

Weight

The force of gravity on an object. Changes with location. Measured in Newtons (N).

Weight (N) = Mass (kg) × Gravitational Field Strength (N/kg)

On Earth, g ≈ 10 N/kg

Orbits & Satellites

Gravity keeps objects in orbit. An orbit is a balance between forward motion and gravitational pull.

Moons: Natural satellites that orbit planets. Caused by gravity.

Artificial Satellites: Human-made objects orbiting Earth. Used for communication, GPS, weather monitoring.

7

Magnetism

Magnetic fields and forces

Magnetic Poles

All magnets have two poles - a north pole and a south pole. You cannot have a single pole on its own.

N

North pole points North when free to rotate

S

South pole is attracted to the North

Like poles repel (N-N or S-S) | Unlike poles attract (N-S)

Magnetic Fields

A magnetic field is the region around a magnet where magnetic forces can be detected.

  • • Field lines go from North to South outside the magnet
  • • The closer the lines, the stronger the field
  • • Compass needles point along field lines
  • • The Earth has a magnetic field - that's why compasses work!
8

Light & Reflection

How light travels and bounces

Properties of Light

  • 1
    Light travels in straight lines - this is why we get sharp shadows.
  • 2
    Light can travel through a vacuum (empty space) - it doesn't need a medium.
  • 3
    Light travels very fast - about 300,000 km/s (300 million m/s).
  • 4
    Light is a transverse wave - the vibrations are perpendicular to the direction of travel.

The Law of Reflection

Mirror Normal Incident ray Reflected ray i r

Key Points

  • Angle of incidence = Angle of reflection
  • The normal is an imaginary line perpendicular to the mirror surface
  • Angles are always measured from the normal, not from the mirror
  • Smooth surfaces give specular reflection (clear images)
  • Rough surfaces give diffuse reflection (scattered light)
Q

Practice Questions

Test your understanding

1

Energy Transfer [3 marks]

Explain how a metal spoon becomes hot when placed in a bowl of hot soup. Name the process involved.

Answer:

Process: Conduction [1 mark]

Explanation: The particles in the hot soup vibrate more and collide with particles in the metal spoon. Energy is transferred from particle to particle through the spoon. [2 marks]

Metals are good conductors because they have free electrons that can move through the metal and transfer energy quickly.

2

Efficiency Calculation [3 marks]

A motor takes in 500 J of electrical energy. It outputs 350 J of useful kinetic energy. The rest is wasted as heat.

a) Calculate the efficiency of the motor. [2 marks]

b) How much energy is wasted? [1 mark]

Mark Scheme:

a) Efficiency calculation:

Efficiency = Useful energy out ÷ Total energy in [1 mark for formula]

Efficiency = 350 ÷ 500 = 0.7 or 70% [1 mark for correct answer]

b) Wasted energy:

Wasted = 500 - 350 = 150 J [1 mark]

3

Solar System [3 marks]

a) Name the four planets closest to the Sun in order. [2 marks]

b) Why is Pluto no longer classified as a planet? [1 mark]

Answer:

a) Inner planets: Mercury, Venus, Earth, Mars [2 marks - 1 mark for correct order, 1 mark for correct planets]

b) Pluto is now classified as a dwarf planet because: It has not cleared its orbit of other objects (it shares its orbit with other bodies in the Kuiper Belt). [1 mark]

4

Reflection [3 marks]

A ray of light hits a mirror at an angle of 40° to the normal.

a) What is the angle of reflection? [1 mark]

b) What is the angle between the incident ray and the reflected ray? [2 marks]

Answer:

a) Angle of reflection = 40° [1 mark]

By the law of reflection: angle of incidence = angle of reflection

b) Angle between rays = 40° + 40° = 80° [2 marks]

The total angle is the sum of the incident and reflected angles.

Year 8 Science Complete!

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