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4.4 Atomic Structure
Fission and Fusion
Nuclear fusion: Atomic structure: Physics: GCSE (9:1)
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Nuclear fusion
The joining of two
light nuclei
to form a
heavier nucleus
Fusion products
A
heavier nucleus
and
energy
in the form of
gamma rays
Spontaneous fusion
Occurs in stars when two hydrogen nuclei fuse together to form a nucleus of helium
Conditions required for fusion
Very high
temperatures
and
pressure
Mass-energy conversion
When some of the mass of the fusing particles is converted into the energy of the emitted radiation
repulsion
it requires the
fusing
of
nuclei
, which are
positive particles
; two positive charges
repel
each other
What happens when two nuclei approach each other
They
repel
each other because they have the
same charge
How to overcome nuclei repulsion
Fusion has to happen under
intense pressure
and
very high temperatures
in order to
force
the
nuclei
together
Advantages of fusion over fission
There are
no radioactive waste products
from
fusion
Disadvantages of fusion over fission
The very
high temperatures
and
pressures
required for
fusion
makes it very
difficult
to build a viable
power station