Destination Space
The Sun
- Subject Area
- Space Science
- Estimated Classroom time
- 50 minutes
- Difficulty
- 2 of 3 — Moderate
How do stars work, and how can we read what they are made of from nothing but their light?
Main Theme: The Sun is a nuclear engine powered by gravity and fusion. Like all stars, its chemical composition can be read from its light, revealing both its ingredients and its place in the story of the universe.
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
State that the Sun is a third-generation star made mostly of hydrogen and helium.
Explain nuclear fusion: how gravity squeezes hydrogen together to release energy.
Identify the main layers of a star, from core to corona.
Describe how spectroscopy uses light to identify the elements inside a star.
Explain how the amount of heavy elements in a star reveals its generation and approximate age.
Misconceptions to watch for
The Sun is burning like a fire.
Burning needs oxygen, and there is no oxygen in the Sun’s core and no chemical burning at all. Fusion converts mass directly into energy, which is a completely different process.
The Sun is the biggest, most powerful thing in the universe.
The Sun is an average, middle-of-the-road star. The Milky Way alone holds between 100 and 400 billion stars and many are far larger. The Sun matters to us because it is close, not because it is big.
If a student asks…
- How can we know what stars are made of if nobody has been there?
- Spectroscopy reads the composition of any star whose light reaches us, however far away. The same elements found on Earth turn up in every mature star we have studied.
- Does a star with lots of heavy elements have to be older?
- It is the other way round. Heavy elements are inherited from earlier stars that had already died, so a metal-rich star formed later in cosmic history. First-generation stars have almost no heavy elements at all.
Got longer?
Teacher Tips
Hook
- It helps to reveal the answer to the hook (spectroscopy) only after learners have had a chance to discuss, debate and disagree.
- “Send a probe” is a response worth staying with rather than moving past. You might ask “How close could a probe actually get?” Someone may know about the Parker Solar Probe, which flew through the Sun’s outer atmosphere, and they’d be right. It still can’t reach the core, though, and it tells us nothing at all about a star in another galaxy. That is the gap spectroscopy fills.
- If someone says “guess from the colour”, it’s worth saying out loud that they’re the closest. Colour is a crude version of the real method, and a learner who hears their answer was nearly right tends to stay with you for the next twenty minutes.
ITZA Pathways
- It helps to listen for the word “burning”. Learners use it casually about the Sun, and it carries a whole wrong model with it: fire, oxygen, fuel being consumed. You might ask “What does fire need that the Sun hasn’t got?” No oxygen, no burning.
- Pathway 1’s layers hotspot is the card that gets clicked through fastest, and the fusion slider is the one worth stopping at. “What is actually lost when hydrogen becomes helium?” works well here. The answer is a small amount of mass, and it leaves as light.
- Pathway 2 has a true or false on whether heavier elements mean an older star. Nearly everyone answers wrong first time, and it’s the one idea in this session that is exactly backwards rather than merely fuzzy. It’s worth catching it here, because it tends to reappear in every answer during the activity.
Classroom Activity
- It helps to do the practice star with the whole class before letting pairs loose. It looks like a slide you could skip when time is tight, but learners who haven’t watched you match a pattern once tend to declare an element present on a single coincidental line.
- You might find it works to ask for two or more matching lines before anyone claims an element, and to ask “What’s missing as well as what’s there?” Star B is identified by the absence of heavy lines, not the presence of anything, and that’s a harder move than spotting a match.
- The mystery element slide is the best challenge in the session, so it’s worth not rushing to the reveal. You could ask “What should a scientist do when the pattern matches nothing in the library?” The honest answer, that the library is smaller than the universe and you go and find a bigger one, is a better lesson about science than any of the correct identifications.
Plenary
- The lock-in quote is from Carl Sagan, the astronomer and science communicator. It says that the nitrogen, calcium, iron and carbon in our bodies were made inside stars. That’s the “inherited” idea from Pathway 2 in a single line, so if there’s time you could ask two or three learners “Where did the iron in your blood come from?”
- Part 2 will fill with facts unless you say otherwise. It’s worth stating plainly that you’re asking what they think, not what they remember, and that “it doesn’t change anything” is a perfectly acceptable answer if they can say why.
Learner journal tip
If using the editable journal, it helps to have each learner make their own copy at the start of the course and save it somewhere easy to find again. Perhaps in a folder on their laptop or in their school drive. It carries across every session, so if the plenary runs short, they can finish Part 2 or the later sections at home without losing earlier reflections.
Extensions
Explore(opens in a new tab)Extension 1
Chase the Sun
Animals across the planet run their lives by the Sun. Take that signal away, or muddle it, and what happens to them?
Explore(opens in a new tab)Extension 2
Hiding the Sun
For most of history, the Sun going dark in the middle of the day was terrifying. Then people worked out why it happened. Why did understanding the cause change everything?
Curriculum links
- Science & Physics
- Nuclear fusion, energy transfer and the electromagnetic spectrum. How light carries information about a star's composition.
- Chemistry
- Properties of hydrogen, helium, sodium, calcium and iron. How elements absorb and emit light at specific wavelengths.
- Maths
- Astronomical scale and percentages: 99.86% of the solar system's mass, 70% hydrogen, trace metals across stellar generations.
- History
- The timeline from the Big Bang to the present, and how heavier elements were built by successive generations of stars.
- English & Literacy
- Decoding scientific riddles, explaining the barcode analogy to peers, and building an evidence-based answer.