The Life Cycle of a Star - Star Death

The Death of Small and Medium-sized Stars

In about 4 to 5 billion years from now the Sun will will begin to exhaust its supply of hydrogen fuel.

The Sun's core will then collapse under its own gravity as the outward pressure of the core decreases (because fusion reactions deep within the core are less prevelant).

This will make the core hotter.

Its atmosphere (the outer atom nuclei) will become unstable because of the increased pressure from the hotter core and start to expand.

This will transform the Sun into a huge red giant star.

At the bloated surface, the increased amount of energy will be spread out over a larger area so each square metre will be cooler.

The surface will have a red colour because it is so much cooler than it was at the yellow stable stage and will be much further from the center than during the main sequence.

Our Sun will swell in size to encompass the inner planets (perhaps Earth too) when this happens!

Despite its cooler surface temperature, a red giant is very luminous because of its enormous surface area; so even if the Earth is not swallowed up when our Sun becomes a red giant, conditions on the planet will become impossible for life to exist. The surface temperature would be so high that the oceans and atmosphere would have evaporated away. 

Finally, when the fuel runs out completely the crushing force of gravity makes the star collapse under the force of its own weight; as it is a relatively small star, it will collapse gently and remains collapsed. Such a collapsed star, at its life's end, is called a white dwarf.  Our Sun will probably end its life in this way. 

It will continue to shine as radiation will still given out from electron promotion/demotion transitions until the kinetic energy of the atoms diminishes enough to stop radiation emission - it will then be a black dwarf - a cold mass moving through space.

 

 

The Death of Large Stars

A different fate awaits a large star. Its final collapse generates a violent explosion, blowing the innards of the star out into space - this is called a supernova.

This is a really violent explosion and is seen as a star increasing in brightness to very bright star. During this supernova event fusion of nuclei cause large nuclei to form - larger ones than would form in a small star.

The materials of the exploded star are flung out into space and mix with the primeval hydrogen of the universe as dust. Later in the history of the galaxy, other stars are formed out of such clouds of dust and gas - nebulae (see above) and the whole cycle begins again.

After the supernovas has blown all of the atoms from the outer star into space the dense core becomes a neutron star or even a black hole.

Our Sun and solar system contains the debris of countless other stars that exploded before the Sun was born.

The heavier elements that are in our solar system - and you! - are star dust. As the 60s hit says - 'We are stardust!'

 

to find out about Star Birth

to find out about the Main Sequence

to for the summary diagram of the life cycle of a star.