How It Works

PICTURING THE PLANETS

Over 3,000 years ago, Babylonian astronomers discovered that five bright points of light moved across the night sky in a different way from all the other stars. These were the planets we now call Mercury, Venus, Mars, Jupiter and Saturn. In those early days, the only way to observe astronomical objects was with the unaided eye, making it impossible to discern any detail. A planet looked virtually identical to any other star, the only difference being its distinctive wandering motion. The very word planet comes from the Greek planētēs, meaning ‘wanderer’.

The next major step forward came in 1609, when Galileo first observed the night sky with an early telescope. This showed the planets to be extended discs rather than star-like points of light, and it was only with this discovery that people came to realise that the planets might be other worlds like Earth. As telescopes improved over time, two further such worlds were discovered that had previously been too faint to see: Uranus in 1781, followed by Neptune in

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