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Grade C
Stars are formed from clouds of gas called
nebulae.
Particles of dust and
molecules of gas come slowly together under the force of gravity.
The process takes many millions of years to
happen, although the shock waves from the explosion of a
supernova may help the process.
In the case of the Solar System, it is thought
that the Sun and the planets formed from a slowly spinning disc of gas
and dust.
Smaller amounts of dust collect
together to form planet sized objects. If these are captured by the
gravity of a star, they will orbit as a planet. Smaller masses
of material may get captured by gravity to form satellites
(moons).
If sufficient gas and dust collects in one
place, it comes together under the force of gravity. The more mass
there is, the stronger the gravity, therefore more material comes
in. As it comes together, the whole thing starts to heat up. This is a
protostar. At this time the star is only giving off
radiation in the infra red and visible light regions. If
there is not sufficient material, then the whole mass will cool down
again.
If there is enough material, it will get hot
enough for fusion to occur. The temperatures involved have to be
around 15 million degrees Celsius. The star lights.
There are many solar systems in the Universe.
Our solar system is on the outer arm of a spiral galaxy called the Milky
Way. Like all galaxies, it is vast, consisting of hundred of
millions of stars. In the middle is thought to be a super-massive
black hole that gobbles up stars.
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