Meet Our Neighbours: Sun

Explore the tactile version of our star, the Sun, made with household materials.

Breve descrição

Converting a visual experience to a tactile one, this activity lets visually impaired students learn about and explore our star, the Sun, and its main characteristics.


To explore our star, the Sun, through a tactile hands-on experience for visually impaired students and their non-visually impaired peers.

Objetivos de aprendizagem

  • Students will create a tactile version of the Sun using low cost household materials.
  • Students will explore characteristics of the Sun using the tactile model.
  • Students will be able to list the different features present on the Sun.


Call out a feature on the Sun (sunspot, solar surface, solar prominence) and ask the students to point it out on their model. For each feature give a brief description.e.g.:

  • These are small, dark, cool areas on the Sun surface (Answer: sunspot).
  • These are long loops of solar material held above the sun’s surface by a magnetic field (Answer: prominence).
  • We see light coming from this part of the Sun. It has a temperature of over 5000˚C! (Answer: solar surface)

Ask the class to suggest how the Sun affects us and helps life on Earth. (Ideas to include: the Sun provides us with a) heat which keeps us warm b) heat which keeps the oceans warm enough to be water rather than ice and c) light to see and give plants energy to grow. The Sun also produces solar flares- very large outbursts of energy which leave the Sun. When these flares reach the Earth, they can disrupt Earth satellites, interrupting GPS and mobile signals.)


  • Flat black sequins (for sunspots)
  • Yellow thread or wool (for solar prominence and outline)
  • Fabric of granular texture (bubble wrap or netting) (for surface of the Sun)
  • Print out 'Sun Features 1 PDF'
  • Print out 'Sun Features 2 PDF'

Informações de referência

The Sun is a "yellow dwarf" star of average dimension and mass. Its diameter is about 1,400,000 km, which means that more than 100 Earth could be lined up along the Sun's equator, and its mass is more than 300,000 times that of Earth. But compared to other types of stars, the Sun is quite average: the radius (mass) of the smallest type of stars, called "brown dwarfs", can be as low as 0.05 solar radius (0.01 solar mass) whereas that of the largest type of stars, called "supergiants" or "hypergiants", can reach 1000 solar radii (200 solar masses). The Sun produces its energy from thermonuclear reactions taking place at its very centre, where the temperature reaches 15 million degrees. This process, which involves "burning" hydrogen and transforming it into helium, has been going on for the last 4.5 billion years and is expected to last about the same amount of time.

The surface of the Sun, called "photosphere", is much cooler than its core, with a temperature of 5500°C. At certain locations on the photosphere, called "sunspots" the temperature is lowered by about 1000°C due to the action of the magnetic field which "punctures" the photosphere at these locations. This makes them appear darker than the surroundings. The spots always appear in pairs with opposite magnetic polarities (the four irregular shaped areas on the tactile model). The activity of the Sun can be measured by the number of spots appearing on the photosphere during a particular year. This activity varies periodically along a cycle of about 11 years. The last minimum occurred in 2014 and the next maximum is expected in 2019-2020. However, between two consecutive cycles, the magnetic field reverses itself; so a complete cycle is actually 22 years long.

Other remarkable features of the sun are the "solar prominences" (represented by loops of thin thread at the edge of the tactile model). They are actual bridges of matter between solar spots, shaped by the powerful magnetic field of the sun. Some of them can be lifted above the photosphere by as much as 350,000 km, which is almost the distance between the Earth and the Moon. They can also be completely disrupted by violent explosions before all the matter has time to fall back onto the surface, in which case some of the matter is sent flowing throughout the solar system.

The sun has an atmosphere, called the "chromosphere" because of its dark orange colour. It can only be seen during natural or artificial eclipses as a thin orange layer around the much brighter photosphere. Finally, above the chromosphere, lies the "corona", a region containing very rarefied gas heated up to one million degrees by a process which is still poorly understood. Like the chromosphere, it can only be seen during an eclipse as a shiny halo with bright streaks of hot plasma.

Descrição da atividade completa

Prior to the activity:

  • Print both Sun mold and Sun features PDFs for each group, and prepare the materials listed above.
  • Ask students what they know about the Sun, introducing it as the star closest to Earth and a hot ball of "burning" gas. Tell students they will be making models of the Sun to investigate its different features.

During the activity:

  • Put the students in groups of 5 (ideally 3 non-visually impaired to 2 visually impaired).
  • Distribute materials accordingly.
  • Close supervision is important. Follow each group and explain each of the tactile elements and their correspondence to each object feature.
  • Understand the different needs of each group of students to promote interaction between the students during the building of the tactile image – visually impaired students need to be familiarized with the different materials involved.
  • Give enough time to follow instructions and build the tactile image.

Step 1

Place the fabric on top of Sun mold sheet and draw the outline.

Step 2

Cut the fabric along the drawn outline.

Step 3

Apply glue on the surface of Sun on the Sun features sheet.

Step 4

Place the fabric on top of the glued area and wait for the model to dry.

Step 5

Glue the different sequins on top of the glued fabric.

Step 6

Glue the thin thread to the outer shape of the sun.

Step 7

Glue the thin thread to the prominence features.

Step 8

Wait for the model to dry (it might take a while before you can explore the model).

Exploring the tactile model:

There are several ways in which you can explore the scientific content of the tactile model. If you’re presenting the final tactile model to the students, first let them explore and feel the different textures. Questions will arise as students explore and it is important to guide them. Read “Background Information” section to understand the different features present in the Sun’s schematic tactile model.

The star’s outer shape is outlined by a thin thread (2). Follow the thread until you find (3) the solar prominence.The interior of the thin thread (2) is the fabric showing the sun’s surface (4). There are several sunspots (5) present.


Space Awareness curricula topics (EU and South Africa)

Our wonderful Universe, Sun-Earth-Moon

National UK

KS3 - Physics, Space Physics: Our Sun as a Star KS2: Year 5 - Science, Earth and Space KS2, Art and Design

Informações adicionais

Explore the solar system planets through "Meet Our Neighbours" in tactile form at Follow up discussion: How long does it take Sun light to travel to Earth? (take students outside during the day time to feel the sunshine). Answer: approximately 8 minutes (can be calculated from time= distance /speed = 150 million km / 300,000,000 metres per second = 150,000,000 m/300,000,000 m/s).


The activity concludes when the students have explored and experienced the tactile Sun and are able to identify the characteristics of the Sun.

This resource was developed by Nuclio and peer-reviewed by astroEDU.

Tópico curricular
Grande ideia científica
Sun, Solar System
Faixa etária
6 - 12
Nível de ensino
Primary, Middle School, Informal
Dimensão do grupo
Controlo de segurança
Low Cost
Small Indoor Setting (e.g. classroom)
Competências básicas
Developing and using models, Communicating information
Tipo de atividade de aprendizagem
Autor da atividade
Lina Canas, Núcleo Interativo de Astronomia
Ligação à atividade de origem
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