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range, an atomic nucleus loses energy by emitting a gamma ray. Gamma
radiation is the most penetrating of the three and will travel through several
centimetres of lead. Beta particles will be absorbed by a few millimetres of
aluminium, while alpha particles will be stopped in their tracks by a few
centimetres of air, or a sheet of paper.
Half-lives and probability
Radioactive decay is determined by quantum mechanics – which is
inherently probabilistic. So, it’s impossible to work out when any particular
atom will decay, but we can make predictions
based on the statistical
behavior of large numbers of atoms. The half-life of a radioactive isotope is
the time after which, on average, half of the
original material will have
decayed. After two half-lives, half of that will have decayed again and a
quarter of the original material will remain, and so on.
Uranium and plutonium are only weakly radioactive but have very long
half-lives – in the case of uranium-238, around four billion years, roughly
the same as the current age of the Earth, or the estimated remaining lifetime
of the Sun. The half of the uranium-238 around now will still be here when
the Sun dies. Iodine-131
has a half-life of eight days, so, once fission has
stopped, less than 1% of iodine-131 produced in a nuclear reactor will
remain after about eight weeks. Other radioisotopes of iodine are even
shorter-lived. Caesium-137, however, sticks around for longer. It has a half-
life of around 30 years, and, because of this and because it decays via the
more
hazardous beta process, is thought to be the greatest health risk if
leaked into the environment.
Although some radioactive materials are produced artificially, many
occur naturally and result in there being a certain amount of radiation in our
environment all the time – the «background radiation».
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