Living in the Milky Way

Build a model of the Milky Way to discover the size of our galaxy and what it contains.

Σύντομη Περιγραφή

During the activity, students build a model of the Milky Way and develop an understanding of the objects contained in the Milky Way and of the distances between these objects.


The activity introduces our galaxy, the Milky Way, to students. They learn what the Milky Way looks like and what objects it contains through building a model of the Milky Way. Students watch a video to gain an idea of the distances in the Milky Way and answer questions on the worksheet.

It is important for students to know about the Milky Way because our Solar System is located in this galaxy. Moreover, galaxies as a whole are very important in the study of how the Universe formed and how it evolves.

Μαθησιακοί Στόχοι

After implementing the activity, students will be able to:

  • describe what the Milky Way looks like,
  • identify the position of our Solar System in the Milky Way,
  • explain that the Milky Way contains dust, gas, and lots of stars,
  • explain that the Earth and the Milky Way are very tiny compared to the universe,
  • describe where the name Milky Way comes from.


After students have made their models, offer descriptions of different objects in the Milky Way and ask students to point them out on their models. Can they locate where the Solar System is? Ask students how big the Milky Way is and how this compares to the size of the Solar System. Ask students to explain where the name Milky Way came from.

Another way to evaluate students’ knowledge is to ask them to compare the Milky Way with images of other galaxies (classification).

Students can also be invited to think how the Milky Way moves and to imagine how we know its size. Some methods used to infer the size of the Milky Way are included on this website:

More traditional methods, i.e. matching terms with their explanation or filling in the blanks of a text with the appropriate words can also be useful.


Per student or model:

  • worksheet in PDF
  • 1 sheet black A4 card
  • drawing compass
  • scissors
  • white paint
  • red paint
  • paintbrush
  • cotton wool
  • glue
  • red clay
  • 5 cocktail sticks
  • fishing line

As a class:

Θεωρητικές πληροφορίες

The Milky Way:

Our home Galaxy consists of about 200 billion stars, with the Sun being a fairly typical specimen. The Milky Way is a fairly large spiral galaxy and it has three main components: a disk, in which the Solar System resides, a central bulge at the core, and an all-encompassing halo.

The disk of the Milky Way has four spiral arms and it is approximately 300 parsecs thick (1 parsec is approximately 3.26 light-years) and 30,000 parsecs in diameter. Compare this to the four hours it takes light to travel from the Sun to Neptune! Our Galaxy is made up predominantly of Population I stars, which tend to be blue and are reasonably young, spanning a million and ten billion years in age.

The bulge at the centre of the Galaxy is a flattened ellipse of 1000 parsecs by 6000 parsecs. This is a high-density region where Population II stars predominate- stars that tend toward red and are very old: about 10 billion years. There is growing evidence for a very massive black hole at its centre.

The halo, a diffused spherical region, surrounds the disk. It has a low density of old stars mainly in globular clusters (consisting of between 10,000 and 1,000,000 stars). The halo is believed to be composed mostly of dark matter, which may extend well beyond the edge of the disk.


A light-year is how astronomers measure astronomical distances and it is equivalent to the distance that light travels in one year, nearly 9.46 trillion kilometres.

Black holes

Black holes are the monsters of space! Anything that gets too close to a Black Hole is pulled to it with such a strong force that it has no chance of escape. The monster will gobble it up! Even light – the fastest thing in the Universe – is doomed if it goes near one of these monsters. This is why black holes are black. However, they are not really holes and they are not empty. Black Holes are actually filled with a lot of material that is crammed into an extremely small region.

Dark Matter

According to scientists roughly 80 per cent of the mass of the universe is made up of material that they cannot observe directly. This material, known as dark matter, does not emit light or energy.

Classification of Galaxies:

There are two main categories of galaxies, the spiral and elliptical, and two others lenticular and irregular.

Our Galaxy belongs to the spiral category. Spiral galaxies fall into several classes depending on their shape and the relative size of the bulge: ordinary spirals are labelled either Sa, b, c, d, or m while those that have developed a bar in the interior region of the spiral arms are labelled SBa, b, c, d, or m. Spiral galaxies are characterised by the presence of gas in the disk, which implies that star formation is active at the present time, hence the younger population of stars. Spirals are usually found in a low-density galactic field where their delicate shape can avoid disruption by tidal forces from neighbouring galaxies.

Elliptical galaxies are placed in categories E0-7 depending on their degree of ellipticity, with E0 being least elliptical. They have a uniform luminosity and are similar to the bulge in a spiral galaxy, but with no disk. The stars are old and there is no gas present. Ellipticals are usually found in a high-density field, at the centre of clusters.

Lenticulars are labelled S0 and, although they possess both a bulge and a disk, they have no spiral arms. There is little or no gas and so all the stars are old. They appear to be an intermediate.

Irregulars are small galaxies, labelled Irr, with no bulge and an ill-defined shape.

Tidal forces

These forces are a secondary effect of the gravitational forces between two objects orbiting each other, such as the Earth and the Moon. Tidal forces are responsible for the fluctuation of the tides as well as for the synchronous rotation of certain moons as they orbit their planets.

Πλήρης Περιγραφή της Δραστηριότητας

Tip: You can see the Milky Way with the naked eye. You can see it best in January when the Moon is new. Encourage the students to look for this if possible.


For the activity Further and further away use the link provided in the materials to access Powers of Ten on youtube. Watch this video and pay attention so that you know precisely when each question is discussed. Prepare to show the film to the class. During the first six minutes, scales from 1m to beyond the scale of clusters of galaxies are shown.

Activity 1: Further and further away

Step 1:

Read the e-mail in Task 1 of the worksheet with the students. The students need to find answers to the following questions from the researchers:

  • What does the Milky Way look like?
  • Whereabouts in the Milky Way is our Solar System?
  • Why can't we see the whole Milky Way from Earth?
  • Is Earth large or small compared with the universe?
  • Is the Milky Way large or small compared with the universe?
  • What is the Milky Way made of?

Step 2:

Watch the film Powers of Ten with the students in order to find the answers to the researchers' questions. This film shows a journey from a picnic in a grassy meadow in America to a location far beyond the Milky Way. Halfway through the film the journey returns to the grassy meadow and into the hand of one of the picnickers. You are recommended to play the film until the journey returns to the picnic field so that the students get a good impression of the immense size of the universe, and just how tiny the Earth is in comparison.

Step 3:

Start by watching the whole film with the students. Explain what they are seeing. Then watch the film again, but this time pause it where relevant to give the students the opportunity to answer the research questions. After they have seen the film, the students will be able to answer questions a to e. Once they have completed the "Make a Milky Way" craft project, the students can answer the final question.

Step 4:

The students investigate what the Milky Way looks like and the position of the Solar System within it.

Activity 2: Make a Milky Way

Now the students have some idea of what the Milky Way looks like, they are going to make a model of it. The students complete Task 2 on the worksheet.

Activity 3: What do you know about the Milky Way?

The students read the instructions in Task 3 and write all the answers to the research questions in the e-mail in Task 1. If necessary, watch the film Powers of Ten one more time. Discuss the answers in the e-mail.

  • If we could view the Milky Way from the side, it would look like a saucer with a bulge in the middle.
  • The Earth's solar system is situated on a spiral arm about two-thirds of the way from the centre of the Milky Way.
  • We don't have any telescopes that can reach far enough out from the Milky Way to take a good photograph of it as a whole. The existing pictures of the Milky Way look like real photographs, but are in fact an artist's impression of what we think it looks like. Explain that it is possible to see part of the Milky Way disc at night when the sky is dark. It is easy to photograph the Milky Way disc from Earth, because this is the part we can see.
  • The most important aspect of this question is that the students see that our Solar System is only a tiny part of the Milky Way.
  • Here again, the Milky Way is only a tiny part of a much larger universe.
  • The Milky Way is a galaxy made up of dust, gas, and at least 200 billion stars, most of which can be found in the disc. The system contains old stars, younger stars, dust, and gas clouds. It is composed of a central bulge and a disc with four large and several smaller spiral arms.

Good to know:

It takes 8 minutes for light from the Sun to reach Earth. It takes much longer for light from the other stars to reach Earth. So when we look at the universe we are really looking into the past. The mass of the universe is estimated to be 100 billion times greater than the mass of the Sun.

Activity 4: The name Milky Way

Ask the students if they know where the name Milky Way comes from.

Egyptian mythology describes the Milky Way as being formed by the milk from a celestial cow. The four feet of the cow were supported by the four corners of the Earth. Greek mythology tells the story that Hera, the wife of Zeus had been given the baby Heracles to breastfeed. When she realised he was not her own child, she pushed him away. The milk that was spilled became the Milky Way.

It is important that the students realise that long ago people had no idea what the Milky Way really was.

Πρόγραμμα σπουδών

Space Awareness curricula topics (EU and South Africa)

Our wonderful Universe, Galaxies

National Curricula UK

KS2: Year 5, Maths: Number – number and place value: count forwards or backwards in steps of powers of 10 for any given number up to 1 000 000.

KS1, Art and Design: To use drawing, painting and sculpture to develop and share their ideas, experiences and imagination.

KS1: Year 1, English: Reading- comprehension: develop pleasure in reading, motivation to read, vocabulary and understanding by: listening to and discussing a wide range of poems, stories and non-fiction at a level beyond that at which they can read independently.

Περισσότερες πληροφορίες

What Part Of The Milky Way Can We See?

Explore the different shapes of galaxies by contributing to the citizen science project "Galaxy Zoo":


This activity helps students to learn what the Milky Way looks like and the objects it contain. They also gain an idea about the distances involved, and the place of the Solar System in our Galaxy. During the activity, students build a model of the Milky Way.

This resource was developed by ESERO NL/ESA, peer-reviewed by astroEDU, and revised by Space Awareness.

Θέμα αναλυτικού προγράμματος
Μεγάλη Επιστημονική Ιδέα
Galaxy, Milky Way, Solar system, stars
6 - 10
Εκπαιδευτική βαθμίδα
Primary, Informal
Μέγεθος ομάδας
Επιβλεπόμενο για λόγους ασφάλειας
High Cost
Small Indoor Setting (e.g. classroom)
Βασικές Δεξιότητες
Asking questions, Developing and using models, Communicating information
Τύπος μαθησιακής δραστηριότητας
Συγγραφέας της δραστηριότητας
NEMO Science Museum, ESERO NL / ESA
Σύνδεσμος για την πηγή της δραστηριότητας
Συναφείς πόροι