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Rebuilding the Universe: Discovering Matter, Space, and Radiation

How do we rebuild the universe from nothing? In this hands-on activity, students explore the fundamental building blocks of reality โ€” matter, space and radiation โ€” and how they interact to form everything we observe in the cosmos. Through guided exploration and discussion, learners develop a deeper understanding of how the universe is structured, from the smallest particles to the vastness of space itself.

This activity is part of our live SpacewardBound sessions delivered in schools across New Zealand.

Physical World, Nature of Science
Astrophysics
Phase 1: 10โ€“15 min, Phase 2: 10 min, Phase 3: 10 min, Extension: optional
Activity

Why is this good to know

Learning outcomes

Describe the difference between matter, space and radiation
__________
Explain how these components interact to form the observable universe
__________
Identify examples of matter and energy in real-world and cosmic contexts
__________
Develop models to represent how the universe is structured
__________
Communicate scientific ideas using appropriate terminology

Prior knowledge

none

What’s the first thing you remember about the night sky? Maybe it was the brightness of the full Moon. Maybe it was the miriads of stars in the Milky Way on a moonless night. The way we perceive our surroundings, along with the questions we received from our school visits, inspired us to create this resource.

The Universe does not arrive at us as facts. It arrives as light in our eyes, pressure on our skin, and motion through space. From these experiences, we begin to build understanding. In this activity, students retrace that journey. We are switching definitions with perception, to uncover a simple way to organise the cosmos: matter, space, and radiation, the three baskets that make the observable Universe.

Big idea

We can understand the Universe by organising it into:

  • Radiationย (what travels and allows us to see)
  • Matterย (what things are)
  • Spaceย (where things are)

Students begin with their own experiences and build toward a scientific model of the Universe.

This activity builds a conceptual model rather than a complete physical description.

Teacher Notes

Students (and most people) may initially think we โ€œsee objects directly.โ€

Guide them toward the idea that we seeย light interacting with objects. At nighttime, for example, as the light gets dimmer, we can see less than we do in daytime. Turn the light off, and it would be very hard to see anything.


NASA astronaut Christina Koch is illuminated by a screen inside the darkened Orion spacecraft on the third day of the agency’s Artemis II mission. To the right of the image’s center, CSA (Canadian Space Agency) astronaut Jeremy Hansen is seen in profile peering out of one of Orion’s windows. Lights are turned off to avoid glare on the windows. Credit: NASA

The core idea
Instead of starting with physics, we can start with โ€œHow do we know anything about the world?โ€ And let the studentsย reverse-engineer reality.

Activity Structure (3 Phases)


Phase 1: โ€œWhat can we detect?โ€

โ€œImagine you are on an alien world. What are all the different ways you can detect or experience things?โ€

Students brainstorm:

Youโ€™ll get things like:

  • touch
  • seeing
  • hearing
  • movement
  • temperature

Write everything up.

Group their answers into 3 clusters:

1. Things we canย touch2. Things aboutย where things are3. Things weย detect without touching
solid objects
surfaces
resistance
distance
direction
movement
light
heat
signals

Do NOT name the baskets yet.

Phase 2: โ€œWhat must exist for these to happen?โ€

So the question is…

โ€œIf these are the ways we experience the worldโ€ฆ what must existย out thereย for this to be possible?โ€

This is how physics begun too

Guide them toward:

For touch โ†’ something must exist

โ€œstuffโ€

For distance/movement โ†’ there must be separation

โ€œspaceโ€

For seeing/heat/signals โ†’ something must travel

โ€œsomething moving through spaceโ€

Drumroll …

Phase 3: Naming the Universe

The great reveal:

โ€œPhysicists organise the Universe in a very similar way.โ€

Introducing:

MatterSpaceRadiation (Light)
โ†’ the โ€œstuffโ€ we can touchโ†’ the โ€œbetweenโ€โ†’ what travels and lets us see

Cool fact

Radiation (light) is one of the main ways we detect the Universe โ€” it travels through space and allows us to see. We donโ€™t actually see objects. We see light coming from them or bouncing off them. We perceive heat coming from a certain source.

Ask the students:

โ€œSo what are we really seeing /feeling?โ€

Answer:

radiation

How can you tell? If you turn the lights off or at night, it is very hard to distinguish – see, objects.


Next level additions

  • add aย misconception trapย (โ€œDo we see objects directly?โ€)
  • use aย dark room + torch demo
  • integrate aย brain/perception discussion

For older students

Sometimes light can turn into matter – this is where the good old T-shirt with E=mc^2 makes sense.

Briefly describe:

  • gamma ray โ†’ electron + positron

No equations needed โ€” just the idea.


Variant: Physical role-play

Assign roles:

  • some students =ย matterย (stand still, form objects)
  • some =ย radiationย (move across the room carrying โ€œinformationโ€)
  • the room itself =ย space

Then:

  • radiation โ€œbouncesโ€ off matter
  • โ€œobserverโ€ students only see via radiation

This isnโ€™t the only way to describe the Universe but itโ€™s a powerful way to begin understanding it.

We take concepts like this and turn them into interactive, hands-on learning experiences students actually understand.

Weโ€™ve worked with 200+ schools and 40,000+ students,
helping make complex space science understandable and engaging.

Want to bring this experience into your classroom?

This activity is part of our live SpacewardBound sessions delivered directly in schools. We run it as a full interactive experience using our mobile planetarium and hands-on activities.

Used by schools across New Zealand

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