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The Solar System

Exam code: 5054
Written by: Ashika|Reviewed by: Caroline Carroll|Updated 2 July 2026

The Solar Systemvideo

The Solar System

The Solar System

  • The Solar System consists of:

    1. The Sun

    2. Eight planets

    3. Natural and artificial satellites

    4. Dwarf planets

    5. Asteroids and comets

Objects in the Solar System

The Solar System, downloadable IGCSE & GCSE Physics revision notes

The Solar System contains a star (the Sun), 8 planets, minor planets, moons and other smaller bodies

The Sun & the Planets

  • The Sun lies at the centre of the Solar System

    • The Sun is a star that makes up over 99% of the mass of the solar system

  • There are eight planets and an unknown number of dwarf planets which orbit the Sun

    • The gravitational field around planets is strong enough to have pulled in all nearby objects with the exception of natural satellites

    • The gravitational field around a dwarf planet is not strong enough to have pulled in nearby objects

  • The 8 planets in our Solar System in ascending order of the distance from the Sun are:

    • Mercury

    • Venus

    • Earth

    • Mars

    • Jupiter

    • Saturn

    • Uranus

    • Neptune

Satellites

  • There are two types of satellite:

    • Natural

    • Artificial

  • Some planets have moons which orbit them

    • Moons are an example of natural satellites

  • Artificial satellites are man-made and can orbit any object in space

    • The International Space Station (ISS) orbits the Earth and is an example of an artificial satellite

Asteroids & Comets

  • Asteroids and comets also orbit the sun

  • An asteroid is a small rocky object which orbits the Sun

    • The asteroid belt lies between Mars and Jupiter

  • Comets are made of dust and ice and orbit the Sun in a different orbit to those of planets

    • The ice melts when the comet approaches the Sun and forms the comet’s tail

Light Speedvideo

Light Speed

Light Speed

  • The planets and moons of the Solar System are visible from Earth when they reflect light from the Sun

    • The outer regions of the Solar System are around 5 × 1012 m from the Sun, which means even light takes some time to travel these distances

  • The light we receive on Earth from the Sun takes 8 minutes to reach us

    • The nearest star to us after the Sun is so far away that light from it takes 4 years to reach us

    • The Milky Way galaxy contains billions of stars, huge distances away, with the light taking even longer to be seen from Earth

  • The speed of light, equal to 3 × 108 m/s, is constant everywhere in the Universe

  • The time taken to travel a certain distance in the Solar System can be calculated by using the equation:

speed = distancetime{"language":"en","fontFamily":"Times New Roman","fontSize":"18","autoformat":true}

  • And rearranging it for time:

time = distancespeed{"language":"en","fontFamily":"Times New Roman","fontSize":"18","autoformat":true}