Stars - CCEA

Part ofPhysics (Single Science)Unit 2: Space physics

What are the key learning points about stars?

  • Formation of a .

  • Lifecycles of stars.

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How was the Sun formed?

The Solar System was formed around 4.6 billion years ago from a giant cloud called a , mainly made up of hydrogen gas and dust.

The nebula collapsed under its own gravity and, as it did, temperature and pressure increased.

It became denser and rotated more rapidly, spiralling inwards.

The hot core in the centre is called a .

The collapsing and joining together of gas and dust under gravity is called accretion.

Eventually gravity compressed the hydrogen so much that the temperature reached about 15 million °C.

At this temperature and pressure began and our Sun was born.

It is therefore called a star.

WATCH: How the Earth was formed

Brian Cox explains how the Earth was formed

In fusion reactions:

  • Hydrogen fuse together to form helium nuclei.

  • Energy is released and radiates outwards.

A star, like the Sun, in its period, is stable.

There are two equal and opposite forces acting on the star:

  • The inward force of gravity.

  • The outward force due to the thermal expansion from the nuclear reactions.

These forces are balanced, therefore the star remains the same size for most of its life.

The Sun is expected to be a main sequence star for billions of years.

The Sun in equilibrium with the force of gravity inwards balanced by an outward thermal expansion.
Figure caption,
The Sun in equilibrium - the force of gravity inwards is balanced by the outward thermal expansion.
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What is the life cycle of stars? (Higher tier only)

The life cycle for a particular star depends on its size.

The diagram shows the life cycles of stars that are:

  • About the same size as the Sun.

  • Much greater than the Sun in size.

The different stages in the life cycle of a star.

All stars begin life in the same way.

A cloud of dust and gas, also known as a nebula, becomes a , which goes on to become a star.

Following this, stars develop in different ways depending on their size.

Stars that are a similar size to the Sun follow the left hand path shown in the diagram above:

\({protostar}\rightarrow{main~sequence~star}\rightarrow{red~giant}\rightarrow{white~dwarf}\rightarrow{black~dwarf}\)

Image gallerySkip image gallerySlide1 of 6, A star is formed from massive clouds of dust and gas in space, known as a nebula. These are mostly composed of hydrogen., A nebula A star forms from massive clouds of dust and gas in space, also known as a nebula. Nebulae are mostly composed of hydrogen.
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What is a supernova? (Higher tier only)

The different stages in the formation of a star and its life cycle.

More massive stars than the Sun have a very different life cycle and follow the right hand path in the diagram above:

\({Nebula}\rightarrow{protostar}\rightarrow{main~sequence~star}\rightarrow{red~super~giant}\rightarrow\)\({supernova}\rightarrow{neutron~star,~or~a~black~hole~(depending~on~size)}\)

After the period, they expand and become red super giants.

This is followed by an explosion in which the outer layers of the star are ejected.

This is called a supernova.

The star will shine as supernova for a relatively short period of time with the brightness of 10 billion suns.

After the supernova the remaining core of the star may collapse further.

Some become while very massive ones become .

A star expands following the main sequence period to become a red super giant
Figure caption,
Red super giant

An exploding supernova throws hot gas into space.

An exploding supernova ejecting hot gas into space.

What are neutron stars and black holes?

Depending on the mass at the start of its life, a supernova will leave behind either a neutron star or a black hole.

A black hole is made when the centre of a very big star falls in upon itself, or collapses.

All the of the star becomes squeezed into a tiny volume of space and the force of gravity increases greatly.

There is such a strong in a black hole that nothing can escape from it, including electromagnetic radiation such as light.

Since no light can escape, it appears black, and hence the name black hole.

A black hole

Key fact

There is such a strong gravitational field in a black hole that nothing can escape from it, including electromagnetic radiation such as light.

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What is a fusion reaction? (Higher tier only)

In a star, hydrogen fuse together to form helium nuclei.

This happens in several steps, but one way to simplify the overall change is:

\(_{1}^{2}\textrm{H} +~ _{1}^{3}\textrm{H} \rightarrow _{2}^{4}\textrm{He} +~ _{0}^{1}\textrm{n}\)

Two hydrogen nuclei fuse to produce a helium nucleus and a .

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What role did a supernova play in the formation of the Solar System?

Scientists believe that at the start of the Universe, 13.8 billion years ago, only hydrogen gas was present.

All the naturally occurring elements apart from hydrogen have been formed by in stars.

For example, beryllium and carbon nuclei can be produced from helium nuclei:

During the majority of the lifetime of a star, hydrogen nuclei fuse together to form helium

As the star runs out of hydrogen, other fusion reactions take place forming the nuclei of other elements.

Elements heavier than iron are formed in the explosions of high mass stars.

When the supernova explodes, all the elements produced are thrown out into the Universe.

The heavy elements found on Earth, such as gold, came from material thrown out in previous supernova explosions.

The presence of gold and other heavier elements such as uranium in the Earth is evidence that the Solar System was formed from the remains of a supernova.

WATCH: Brian Cox on the death of stars

Professor Brian Cox demonstrates how the chemical elements are made in the death throes of a dying star

Key fact

All the naturally occurring elements apart from hydrogen are formed by nuclear fusion in stars.

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How much do you know about stars?

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