Radioactive decay is the spontaneous transformation of an unstable atomic nucleus into a different nucleus, emitting radiation.Radioactive decay is the spontaneous process by which an unstable atomic nucleus loses energy by emitting radiation. This transformation changes the original element into a different element or a different isotope of the same element, often leaving the nucleus in a more stable configuration. It is a fundamental phenomenon in nuclear physics, underlying everything from the heat of Earth's interior to the dating of archaeological artifacts and the operation of nuclear reactors.
Discovered in 1896 by Henri Becquerel, who found that uranium salts fogged photographic plates. Marie and Pierre Curie subsequently isolated polonium and radium, and Ernest Rutherford identified alpha and beta particles and proposed the concept of half-life.
The nucleus of an atom is held together by the strong nuclear force, which competes with the electrostatic repulsion between protons. In unstable nuclei, this balance is off, and the nucleus can spontaneously emit particles or electromagnetic radiation to shed excess energy. Common modes include alpha decay (emitting a helium nucleus), beta decay (converting a neutron to a proton or vice versa, emitting an electron or positron), and gamma decay (emitting high-energy photons). The process is probabilistic: for a given nucleus, there is a constant probability per unit time of decay, characterized by the half-life.
Used in radiometric dating (e.g., carbon-14), medical imaging and cancer treatment (radiotherapy), nuclear power generation, and as a power source for spacecraft (radioisotope thermoelectric generators).
The decay of a single atom was first observed in 2019 using a technique that trapped a radioactive atom and detected the emitted particle, confirming a prediction made by Einstein in 1917.





