← Teacher guide

How do we know the universe is expanding?

Students explain redshift as evidence that galaxies are moving away, describe Hubble's distance–speed pattern, and connect an expanding universe to the big bang model (AC9S10U03, node 3).

Year 10 Earth and space · The big bang · about 23 minutes · Open the student lesson

Classroom resources

Load these into Waypoints Prepare: choose Load URL and paste the copied address, or download the file and import it. In Prepare, the worksheet's Teacher edition shows the answers; the student copy hides them.

Students will be able to

Timing

Engage and Explore 9 min · Explain 8 min · Evaluate 3 min · Typical adds 2 min, Wider about 1 min

Before class

A concept tutorial for introducing or revising the idea. Set the width with ?width=minimum, typical (default) or wider.

Assumed: light as a wave with a wavelength, and a spectrum as light spread out by wavelength (Year 9 waves). No tutorial teaches these, so Explore opens with a short "Reading a spectrum" recap; if the class has not met spectra, show one through a diffraction grating or a prism first.

The misconception to watch is galaxies flying away from a centre (and us being at it). Changing the home galaxy shows the same pattern from everywhere.

Board notes: a 2D field of galaxies; "Let space expand" stretches every distance by 1.6. Distances are in millions of light-years (one grid square is 100 million) and speeds use a Hubble constant of about 70 km/s per megaparsec (21.5 km/s for every million light-years). Spectra show four hydrogen lines, with the shift drawn 5 times bigger. Strictly, cosmological redshift is space stretching the light, not a Doppler effect from motion through space; the Doppler explanation is the curriculum's model.

Running the lesson

  1. Engage: count how many chose 'we are at the centre'.
  2. Explore: collect a few class points on one graph.
  3. Explain: the big bang link is the checkpoint.

The hard part (on purpose)

Seeing that every galaxy sees the others moving away, so there is no centre. When a student says we are at the centre, ask what happened when they lived in another galaxy.

When students get stuck

What you will seeA question to askThe fix
A student says galaxies are moving away from us because we're special.What happened when you lived in another galaxy?The same pattern: every galaxy sees the others moving away.

Answers to the checks

  1. Engage: the centre?: Almost every galaxy is moving away from the Milky Way. What do you predict that means?
    Space is expanding, so from any galaxy, the others move away. There is no centre: the same pattern appears wherever you live.
  2. Reading a spectrum: First, reading light. A galaxy's spectrum runs from violet (short wavelengths) to red (long wavelengths). Its dark hydrogen lines sit further towards the red end than the same lines measured in a lab. What has happened to its light?
    It has been stretched to longer wavelengths
    Hydrogen always leaves its dark lines at the same wavelengths. Lines moved towards the red mean longer wavelengths: the light has been stretched. That is a redshift.
  3. Stretch space: Let space expand, then measure at least three galaxies at different distances.
  4. Redshift: What does a redshift in a galaxy's light tell us?
    The galaxy is moving away from us: its light is stretched to longer, redder wavelengths
  5. The pattern: On your graph, how does speed depend on distance?
    Farther galaxies move away faster, in proportion: double the distance, double the speed
  6. Back in time: How does an expanding universe support the big bang theory?
    Run the expansion backwards and all galaxies were once together, in a hot, dense state
  7. Two homes: Live in two different galaxies and let space expand from each.
  8. Same pattern: From the second home galaxy, what did the other galaxies do?
    They all moved away, farther ones faster: the same pattern as before
  9. Elaborate: a blueshift: The Andromeda galaxy, our nearest big neighbour, is blueshifted. Does this disprove the expanding universe?
    No: nearby galaxies' own motions under gravity can beat the expansion; over large distances, the redshift pattern is clear

Solutions

One possible solution for each task. Other correct programs are fine.

Elaborate: no centre › Two homes

Open task: any program that does what the step asks.

Elaborate: no centre › Same pattern

Open task: any program that does what the step asks.

Stretch and support

Stretch: Use the graph's slope to estimate how long ago the galaxies were together (distance ÷ speed).

Support: Give a two-column table (distance, speed) to fill from the board.

Coach prompt (optional)

For a student who has done the lesson and is still stuck. They paste it into an AI tool your school allows; it asks questions about this lesson's one idea and doesn't give answers. Students see it on the course recap page only through a link ending in ?coach=1: recap with coach prompts.

You are a patient science coach for a Year 10 student in Australia. Help me understand ONE idea only, from the lesson "How do we know the universe is expanding?".

The idea: Redshift and the expanding universe: I can explain how the redshift of light from distant galaxies provides evidence that the universe is expanding, and connect this to the big bang model.

What understanding looks like:
- Explains that redshift of light from distant galaxies indicates they are moving away from us
- Connects the expanding universe (evidenced by redshift) to the big bang model
- Describes Hubble's observations as a key evidential basis for the expanding universe

Mistakes students often make here:
- A student says galaxies are moving away from us because we're special.

How to coach me (rules from the Waypoints Kit coach):
- Ask me one short question at a time (2 to 4 sentences) and wait for my answer. Never give me the answer before you have heard my thinking, and don't hide the answer inside your question.
- Start in Discover: ask me to explain the idea in my own words, or to predict what happens in a simple example. I can switch any time: "teach it back" (you play a beginner and I explain), "spot the flaw" (you show me an answer with one common mistake and I find it), or "check" (I explain, and you tell me what is solid and what to revisit).
- If I am stuck or say "just tell me", ask what I think first, then give a small hint or a simpler example. Explain only after I have had a real go.
- If I seem to be missing the idea that comes before this one (The big bang model — origin and timeline of the universe), check it quickly, then come back.
- Stay in this idea: don't teach later ideas or add extra content. If I ask about something else, say it is for another lesson and bring me back.
- After you help, ask me one reflective question, such as how I know my answer is right or what I would check.
- Praise my effort and method, not my ability.
- You can be wrong: if I rely on something you said, remind me to check it against my notes or the lesson. If you don't know, say so.
- Use simple words.
- Stop when I can explain the idea in my own words and get one new example right. Then tell me to go back to the lesson "How do we know the universe is expanding?".

Exit ticket

What does redshift show, and how does it support the big bang?

Galaxies are moving away, farther ones faster: the universe is expanding. Run backwards, everything was once together in a hot, dense state.

What each step is for

Where it leads

Next: the cosmic microwave background and matter proportions (nodes 4 and 5), then Earth's energy balance (AC9S10U04).