1. UV Image of the Hubble Deep Field
What can you see in the image?

2. Complete the page entitled Supernova

3. LO’s
- To be able to explain the stages in a star’s life cycle and how these stages are dependent upon the stars mass.
Understand the processes that keep a star stable during its main phase and why this processes cannot continue indefinitely.

4. The Story of a Star
The Story of a Star

5. Made of Star Dust....
The universe has had 4 generations of stars, When the largest of these past generations reach the end of their ‘life’ they explode in a supernova! The remnants, are mostly gases and small particles of dust. These are attracted towards each other by gravity and create nebulae. All solar systems start off as nebulae.

6. Nebulae come in different shapes and sizes and are mostly hydrogen and dust.

7. The nebula begins to collapse (why
The nebula begins to collapse (why?) and material is pulled towards the centre. The dust and gas and starts to spin, creating huge amounts of heat energy . Eventually enough to allow fusion to take place in the core.
Most of the dust forms a star and some that is left outside forms the planets.

8. Twinkle, Twinkle, Little Star ...
Hubble Heritage image of Sagittarius Star field. Note that along the horizontal axis, the image is 13.3 light-years across.
Ask audience what they notice by looking at this image. Hopefully they will notice the different colors. You can then ask them what the different colors mean [different temperatures]
Image from
The sun is one of many billions of stars in space!
What do you notice about these stars?

9. Twinkle, Twinkle, Little Star ...
Hubble Heritage image of Sagittarius Star field. Note that along the horizontal axis, the image is 13.3 light-years across.
Ask audience what they notice by looking at this image. Hopefully they will notice the different colors. You can then ask them what the different colors mean [different temperatures]
Image from
Stars are different! Most obviously they have different colours which indicate different temperatures

10. is the Sun? Are all stars the same?
Our Sun is quite average, it’s about in the middle in terms of size and temperature of the stars we have seen.
All stars are different and we classify them using different names. Our sun is a Main Sequence Star.
Stars go through phases in their life just like we go through; baby, child, teenager etc.
Remember star evolution is SLOW! Millions/billions of years it is only by studying distant stars we can see how they form from a nebula to a main sequence and beyond...

11. Main Sequence Star

12. Matter is pulled towards the centre of the star due to its weight.
Compacted particles in the centre get very hot, about 15 million degrees in the centre. Once a star is hot and small enough it will ‘ignite’.
All Main Sequence Stars are undergoing a process called fusion.
When the Sun was young, like all stars, it was nearly 100% hydrogen. As fusion takes place hydrogen atoms fuse together and release energy. The hydrogen then changes into helium and is used up.
Energy released from fusion opposes the inward force of gravity so the star does not expand or contract!

14. Stars burn a succession of elements towards the end of their life.
Iron is the most stable element and cannot be fused further.
Instead of releasing energy when fusing, it uses energy when split.

15. This means that all elements up to iron in the periodic table are formed through fusion.

16. The Death of a Star
Once a star has exhausted its supply of hydrogen it will leave the main sequence.
Its fate is now dependant on the mass of the star (and the will of the emperor)

17. Red Giant

19. The fate of small stars…
White Dwarf
Black Dwarf

20. The fate of large stars…
Supernova
Movie clip; red
giant goes supernova

22. Neutron Star

23. Black Hole

24. Teacher notes
This three-stage animation explains how we know black holes exist, and where, even though they cannot be seen.

25. Supernova Remnants: Cas A
Optical
X-ray
Cas A is 300 years old. The remnant is about 10 light-years in diameter, and 10,000 light-years away.
X-ray: outer shock wave is from the initial supernova explosion ripping through the interstellar medium at 10 million miles per hour. Temperatures may reach 50 million degrees. The inner shock is the ejecta from the SN heating up the circumstellar shell, heating it to 10 million degrees
The optical image of Cas A shows matter with a temperature of about ten thousand degrees. Some of these wisps contain high concentrations of heavy elements and are thought to be dense clumps of ejected stellar material.
Cas A x-ray and optical images from

26. Your Task Read through the text ‘The Story of a Star’
Learning Objectives
By the end of this lesson you should…
Be able to explain the stages in a star’s life cycle
Understand the processes that keep the star stable throughout its stable phases
Know what causes a star to leave a stable phase
Know how the fate of a large star differs from the fate of a small star
Your Task
Read through the text ‘The Story of a Star’
Highlight any important terms and facts
Use the information to fill in the ‘Stellar Evolution’ flow chart
In the boxes write down the stage of the star and a brief description of it
In the clouds write down the process that causes the change in the star.
Finished that?
Colour in the arrows blue that show the star contracting
Colour in the arrows red that show the star expanding
Highlight on your flow chart the route our Sun will take as it evolves

27. Learning Objectives
By the end of this lesson you should…
Be able to explain the stages in a star’s life cycle
Understand the processes that keep the star stable throughout its stable phases
Know what causes a star to leave a stable phase
Know how the fate of a large star differs from the fate of a small star
Small Stars
Hydrogen runs out, star swells and begins to fuse helium. Star is cooler and red.
Fusion of hydrogen nuclei produces heat and light. Outward forces balanced by inward gravitational pull.
To help students complete stages – could be printed off and offered as a hint sheet
Helium runs out causing the star to cool and contract.
Gravity causes gases to spiral together.

28. Large Stars Gravity causes gases to spiral together.
Learning Objectives
By the end of this lesson you should…
Be able to explain the stages in a star’s life cycle
Understand the processes that keep the star stable throughout its stable phases
Know what causes a star to leave a stable phase
Know how the fate of a large star differs from the fate of a small star
Large Stars
Gravity causes gases to spiral together.
A very small, dense core is left.
Hydrogen runs out, star swells and begins to fuse helium. Star is cooler and red.
Fusion of hydrogen nuclei produces heat and light. Outward forces balanced by inward gravitational pull.
Helium runs out causing the star to contract, this collapse causes a supernova explosion.