By shooting a neutron at the
nucleus of Uranium-235 creates
Uranium-236 which is unstable
To create daughter atoms with spare neutron
Nuclear Fusion
Is the process of forcing two
nucli together so they form
one larger nucleus.
You use the 2 isotopes of
hydrogen to make a helium atom
with spare neutrons
Nuclear Issues
The major source of
background radiation is
radon gas, which seepes
through the ground.
This admits alpha particals
Other sorces are
X-rays
Nuclear wepon testing
Uranium and plutonium
are chemicly removed
from used fuel rods from
nuclear reacton as they
can be used again
Workers
should... To
reduce nuclear
radiation
Keep as far
away as posible
from the sourse
Shield themself with lead or concreate
Spend as
little time as
posible
asposed to
the sorce
The Early universe
Big Bang 13 billion years ago
At first the univers was a hot glowing ball of radiation
As the univers expands, over millions of years, it's tempricher fell
Uncharged atoms were formed
Before Galaxies
and Stars formed,
the universe was
a dark cloud of
Hydrogen and
Helium
Dust and Gas
were pulled
together by
gravitational
atraction to
form start
The resulting
intensiy heat
started off nuclear
fusion reactions in
the stars so they
omited light
A galexy is a colection of billion stars held together by there own gravity
How the
chemical
elements
formed
Chemical elements
are formed by fusion
processes in stars
The process
releases large
amounts of
energy
Elements hevier than Iorn are only formed in
the final staged of the life of a big star. This
is because the process requires the input of
energy
All the elements get distabuted
through space by the supernova
explosion
The presence of
the hevier
elements in the
sun and inner
planets is
evidence that
they were formes
from debris
scattered by a
supernova.
The life History of a Star
Gravitational forces pull clouds of dust
and gas together to form a protostar
The core gets brighter and hotter because other elements start to fuse together
Eventually a star runs out of hydrogen nuclei, swells, cools down and turn red
Stars radiate energy because of hydrogen fusion in the
core. This stage can continue for billions of years untill
the star runs out of hydrogen nuclei.
The star is stable because the inwards
force of gravity is balanced by the outer
force of radiation from the core this is
called a main sequence star
What happens next depends on the size
A star Similar size to our sun is a red giant
Helium and other light elements fuse to form heavier elements
Fusion stops and the star will contract to form a white dwarf
Eventually no more light is emmited nad it becomes a
black dwarf
star bigger than the Sun will swell to become a supergiant
Eventually the star explodes in a supernova. the outher layers
are thrown into space and the core is left as a nutron star
If this is strong enough it will form a black hole