The Solar System (Cambridge O Level Physics)

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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

Examiner Tip

You need to know the order of the 8 planets in the solar system. The following mnemonic gives the first letter of each of the planets to help you recall them:

My Very Excellent Mother Just Served UNoodles

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune

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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:

s p e e d italic space equals italic space fraction numerator d i s t a n c e over denominator t i m e end fraction

  • And rearranging it for time:

t i m e italic space equals italic space fraction numerator d i s t a n c e over denominator s p e e d end fraction

Worked example

The radius of Mercury's orbit around the Sun is 5.8 × 109 m.

Calculate the time taken for light from the Sun to reach Mercury.

Answer:

Step 1: State the equation for the time taken for light to travel a certain distance

t i m e italic space equals italic space fraction numerator d i s t a n c e over denominator s p e e d end fraction

Step 2: Substitute the values into the equation

  • The distance travelled is the radius of the orbit = 5.8 × 109 m
  • Speed = the speed of light = 3.0 × 108 m/s

t i m e space equals space fraction numerator 5.8 space cross times space 10 to the power of 9 over denominator 3.0 space cross times space 10 to the power of 8 end fraction space equals space 19.33333

Step 3: Round up the answer and include units

time space equals space 19.3 space straight s space

Examiner Tip

The speed of light is very fast. This is why in our everyday life things like switching on a light seem to be instant. However, this is only because the light travels very fast and the distances are very small. In large, astronomical distances which can be millions or even billions of kilometres, the limit of the speed of light starts to have an effect.

For example, it takes light 8 minutes to travel from the Sun to the Earth. This means we are seeing the Sun as it was eight minutes ago. If the Sun was to disappear, we would not notice till eight minutes later. Although, by that time, time delay would be the least of our worries...

p.s.: The Sun is not going to vanish!

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Katie M

Author: Katie M

Expertise: Physics

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.