The life of a Star

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The life of a Star

           

Overview of the life of a star
By observing stars of different ages, scientists have plotted the life of a star, from it’s birth to it’s death.
Stars are huge spinning balls of glowing hydrogen and helium gas. What happens to a star during it’s life depends on how much of these gases it contains. Stars with a lot of material have shorter life spans.

All stars start their lives in a spinning, dense cloud of gas and dust, a
nebula. the cloud spins, small pockets of material form inside it and begin to shrink to form spinning balls, through Gravitational attraction between the atoms of gas gradually drawing them together. Each ball is a protostar.
The balls of material continue to shrink due to gravity acting on it, becoming denser and it’s temperature rises. When the temperature in the centre of the core reaches around 10million degrees. This causes a new, young star to shine.  

Nuclear fusion in the core of the ball starts to turn hydrogen atoms into atoms of a heavier gas-helium. Each time an atom of helium is formed into hydrogen, a little energy is released in the form of light and heat. Most of the stars’ energy is given off into space, but a little is retained, causing the star to grow hotter.
The stars’ core may get denser and hotter as it uses up its hydrogen, and when all the hydrogen is spent, the star expands. It’s surface cools and its colour changes to red. The star is now a
red giant.

Eventually the star burns it’s helium to make carbon, which makes it very unstable. It contracts and expands alternately, ejecting its exterior layers into space as it does so, creating a
planetary nebula.

Nebula are the remnants of a Red Giant which has completely imploded, before proceeding to explode releasing most of their energy. It expels large amounts of dust and gas in the process.

Eventually the star collapses, forming a small dense, hot star called a
white dwarf (a star about the size of Earth). Over millions of years the white dwarf cools down, eventually becoming a black dwarf; too cold to shine. By this time it is very near the end of it’s life.
If the red giant is a massive star, it generates heavy elements, like iron, and grows to form a
supergiant. If the entire supergiant explodes, it evolves into a supernova, shooting matter out into space.

Depending on its mass, the supernova gives birth either to a
neutron star or, when the exploded supergiant is of sufficiently high mass, a black hole.

As the star collapses, its material is increasingly compressed together until it is joint a point in space. It is so dense that its gravity pulls everything towards it, allowing nothing to escape, not even light.

If only the outer part of the supergiant explodes, a
nova forms.

                                                 


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Red Giants & Red Super Giants

Red Giants, and Red Super Giants are the two possible forms of a star after is has been deprived of hydrogen. They are large (red super giants being massive!), highly luminous and have a relatively cool surface, though have a large core temperature. They are of similar mass to our Sun, or slightly greater, and are swelling up towards the end of their lives. Our own Sun will eventually evolve into a red giant, billions ...

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