In 1804, John Dalton decided that all matter was made up of tiny particles called atoms.
J.J Thomson discovered the electron in 1897. This lead to the plum pudding model - a ball of positive charge with negative electrons embedded in it
Ernest Rutherford's gold foil experiment showed that most mass is concentrated at the centre of an atom (the nucleus)
Niels Bohr proposed that electrons orbit the nucleus in shells. Further evidence suggested that the nucleus contained positively charged particles called protons
In 1932, James Chadwick discovered the neutron, which was a particle that had a mass but no charge.
If an electron gains energy by absorbing EM radiation, they more to a higher energy level further from the nucleus.
If they lose energy and release EM radiation, the atom moves to a lower energy level closer to the nucleus
Isotopes are atoms of the same element with different numbers of neutrons.
Alpha Particles
Helium nuclei (Two neutrons and two protons)
Not very penetrating - stopped by paper
Strongly ionising
Beta particles
High speed electron
Moderately penetrating - stopped by aluminium
Moderately ionising
For every beta particle emitted, a neutron in the nucleus turns into a proton
Gamma rays
EM waves with a short wavelength
Very highly penetrating - stopped by concrete or lead
Very weakly ionising as they pass through rather than collide with atoms
During alpha decay, its atomic number reduces by 2 and its mass number reduces by 4
During beta decay, the atomic number increases by 1
The half-life is the time taken for one half of the radioactive material to decay
The count rate is the number of radiation counts per second
A Geiger counter measures the intensity of radiation using a scintillation detector which produces light when it detects radiation
Sources of background radiation
Naturally occurring unstable isotopes
Cosmic rays from the sun
Radiation due to human activity
Exposure to radiation is irradiation, this happens when an object is exposed to a source of radiation