Destination Space
Earth’s Protective Systems
- Subject Area
- Space Science
- Estimated Classroom time
- 50 minutes
Why don't we get fried by the Sun?
Main Theme: Earth is protected by two invisible shields working together: the atmosphere, which blocks radiation and burns up debris, and the magnetosphere, which deflects the solar wind. Without either one, life on the surface would not be possible.
Grab your resources
Session Plan
The full session, stage by stage: what to say, what to do, and what to expect from the students.
Slide Deck
Everything you'll put on the board, in order. Speaker notes included.
ITZA Pathways
One link covers everything for this session: both pathways, the minigame for early finishers, and the extension activities.
Learner Journal
The five-part reflection learners complete in the plenary of every session.
Session objectives
Describe how Earth’s atmosphere formed from volcanic gases and what it protects us from.
Identify the five layers of the atmosphere and what each one does.
Explain what the ozone layer is, how it was damaged, and how the Montreal Protocol fixed it.
Explain what the magnetosphere is, how it is generated and what it protects Earth from, using Mars to show what happens when a planet loses its magnetic shield.
Describe the risks a major solar storm poses to modern technology.
Misconceptions to watch for
The ozone hole is fixed and we don’t need to think about it anymore.
The ozone layer is recovering but is not fully healed. Full recovery over most of the world is expected around 2040, more than 50 years after the Montreal Protocol was signed.
If the magnetosphere disappeared, everyone would die instantly.
The effects would build up gradually, over a very long time, as seen on Mars. The immediate effects would be technological: compasses failing, satellites at greater risk, more radiation reaching near-Earth space.
If a student asks…
- Where does the atmosphere end and space begin?
- The atmosphere has no sharp edge. It simply thins out gradually across the exosphere until it becomes indistinguishable from space.
- Isn’t the magnetosphere just part of the atmosphere?
- They are different systems. The atmosphere is a layer of gas held by gravity. The magnetosphere is a magnetic field generated deep inside Earth’s core. Mars lost its magnetosphere first, which is what allowed the solar wind to strip away its atmosphere afterwards.
Got longer?
Teacher Tips
Hook
- It helps to dim the lights before the torch demonstration. It makes the beam more dramatic and sets up the astronaut slide better.
- It helps not to let the class settle for “the atmosphere” when you ask what’s protecting us. You might push straight into the blanket question: a blanket stops a punch but not a bullet or an X-ray, so “How does a thin layer of gas stop a star attacking us?” It’s worth leaving that open rather than answering it.
- It’s worth giving the beach photo a moment before moving on. The contrast with the spacesuit slide is what makes the mystery work.
ITZA Pathways
- On the atmosphere pathway, you could ask which of the five layers learners think matters most. There’s no single right answer. The point is to get them seeing that the layers do different jobs, rather than treating “the atmosphere” as one thing.
- On the magnetosphere pathway, you might ask “What would happen today if Earth’s core suddenly stopped moving?” Most learners assume instant disaster. The real answer, that very little changes for a very long time, is worth having ready.
- “Which fact surprised you most?” works well here too if someone’s disengaged.
Classroom Activity
- It helps to start with the ozone layer as a worked example for the whole class. Talk through what’s lost and the immediate and long-term effects together before groups go off on their own. That gives them the template to apply themselves.
- Groups then work through the mesosphere and whole-atmosphere scenarios as a fixed pair, with 4 minutes before feedback. After that, they choose one of the final two, the magnetic field or a solar storm, also with 4 minutes.
- Watch for groups who assume losing the magnetic field means instant disaster. You could push back with Mars: the atmosphere doesn’t vanish immediately, it strips away over a very long time.
- The mesosphere scenario tends to surprise learners the most. Most don’t realise meteors usually burn up before reaching the ground.
Plenary
- The reflective question asks learners to finish “Earth is like a giant spacesuit”. It helps to push for the atmosphere, the ozone layer and the magnetosphere all getting a mention, not just whichever one they remember best.
- The lock-in is from Ulf Merbold, a German physicist and astronaut with the European Space Agency, speaking after his 1983 flight. He’d always been told the atmosphere was an “ocean of air”, and what he saw was a thin line, which scared him. You might read it slowly, then ask “What did he expect to see, and what did he see instead?”
Extensions
Explore(opens in a new tab)Extension 1
No Air to Spare
Up at 400 km above Earth, astronauts have to recreate our atmosphere artificially, and there’s no room for anything to go wrong.
Explore(opens in a new tab)Extension 2
The Day the Dinosaurs’ World Ended
66 million years ago, something far too big for the atmosphere to stop was heading straight for Earth. What happened next?
Curriculum links
- Physics
- The magnetosphere as a deflector of the solar wind. Electromagnetic radiation and energy transfer.
- Chemistry
- The composition and structure of Earth's atmosphere. The ozone layer (O3) and how it filters ultraviolet radiation.
- Geography
- Atmospheric change and its impact on living things. The Montreal Protocol as an international environmental agreement.
- History
- The 1985 discovery of the ozone hole by British scientists in Antarctica. The 1859 Carrington Event and its effect on global telegraph systems.
- English & Literacy
- Evaluating evidence and forming an argument about which protective system matters most. Explaining technical concepts in plain language.