Learn / Lesson packs
Space in ten lessons
The shortest way round the whole subject. Ten first looks, from how big it all is to how it began, each needing nothing but curiosity.
10 lessons in 4 parts. Every one can be read again at a deeper level.

Part 1
Where we are
The size of things, and the two ideas that explain why anything moves the way it does.
- 1How big is space
The true spacing of the Solar System and the stars, on a scale you can walk.
With moving pictures and photographs
- 2What gravity is
Everything pulls on everything else. The pull grows with mass and fades with distance, and it never quite reaches zero.
With moving pictures and photographs
- 3What an orbit is
An orbit is a fall that never reaches the ground. Newton's cannonball shows how.
With moving pictures and photographs
Part 2
Our own corner
The Sun and what goes round it.
- 4What the Sun is
The Sun is a star seen close up: a ball of glowing gas, layered like an onion, with a furnace in the middle.
With moving pictures and photographs
- 5Rock, gas, ice: three kinds of planet
The eight planets come in three sorts, and where each one formed explains which sort it is.
- 6What a moon is
Anything that orbits a planet is a moon. There are more than 400, from worlds bigger than Mercury to rocks a kilometre across.
Part 3
The stars
What the points of light are, and what becomes of them.
- 7What a star is
A star is a ball of gas heavy enough to light its own fire. How heavy it is decides almost everything else about it.
With moving pictures and photographs
- 8How stars live and die
Stars form in clouds of gas, shine steadily for most of their lives, and end as white dwarfs or in explosions, depending on their mass.
With moving pictures and photographs
Part 4
Everything else
Our galaxy, and the universe it is one small part of.
- 9The Milky Way
Our galaxy is a flat, turning disc of a few hundred billion stars. We live inside it, about half way out, and have never seen it from outside.
- 10The expanding universe
Distant galaxies are all moving away from us, and from each other. Run the film backwards and you arrive at a hot, dense beginning 13.8 billion years ago.
Go and look
- Fly through it in 3D
From the Sun out to the oldest light, with everything where it is measured to be.
- Tonight’s sky
What is overhead where you are, right now.