Radioactivity

Overview

Radioactivity refers to the sudden ejection of particles from an unstable atomic nucleus. This instability arises from an imbalance in the forces holding protons and neutrons together at the center of an atom, leading to excess energy. By ejecting particles with this energy—a process called radioactive decay—the atomic nucleus becomes stabilized. These energetic particles comprise ionizing radiation, which, like gamma rays, X-rays, and high-energy UV light, can break chemical bonds and damage DNA.

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Hours of research by our editors, distilled into minutes of clarity.

  • An overview of radioactivity, which can spontaneously change one element into another

    Unstable atomic nuclei can transmute into a new element—an atom with a different number of protons—by emitting an alpha particle (two protons and two neutrons) or a beta particle (an electron). The electron can emerge from the nucleus when a neutron, which has no charge, suddenly transforms into a proton and an electron, thereby maintaining zero charge before and after the transformation, but altering the original element.

  • View summaries of the most common types of radioactive decay and their associated particles

    The alpha particle has the strongest ability to ionize other atoms it strikes, but it also does not travel very far before colliding with something and being absorbed. Gamma particles—high-energy photons—do not interact with matter as easily and therefore possess the greatest penetrating power, though this also makes their ionizing potential the smallest.

  • Less common types of radioactive decay include emitting neutrons and antimatter

    Through neutron emission, one or more neutrons are ejected from atoms that have far fewer protons. Neutrons can also be released by artificially inducing the fission, or separation, of a large atomic nucleus into smaller ones. During beta-plus decay, a positron—the antimatter version of an electron—is produced when a proton turns into a neutron.

  • The nuclear shell model explains why certain isotopes undergo radioactive decay

    When the number of protons and neutrons completely fills shells within the nucleus, the binding energy that prevents these particles from being pulled apart increases. These are called "magic numbers," and they produce atoms with exceptionally stable nuclear configurations.

  • Learn about ionizing radiation and see the most radioactive places on Earth

    The average person is exposed to radiation every day, though most of it is either harmless non-ionizing radiation or ionizing radiation at doses too small to significantly affect an individual. The highest doses of ionizing radiation are received by smokers due to the radioactive polonium and radioactive lead in tobacco products.

  • Where radon comes from and why it may be the most dangerous source of radioactivity

    Released from underground bedrock before passing through soil, this radioactive gas is produced from the decay of uranium, thorium, and radium and accounts for about half of all human exposure to radiation. It is the leading cause of lung cancer among non-smokers and can build up in enclosed spaces such as buildings without proper ventilation to dilute the gas.

  • Why taking potassium iodide to protect against radioactivity is unlikely to be effective

    Since the thyroid gland cannot distinguish between radioactive and non-radioactive iodine, taking potassium iodide pills causes the thyroid to absorb the medication, leaving it unable to take up radioactive iodine from the environment. However, while this protects the sensitive gland against the most prominent radioisotope produced in nuclear accidents, it does not protect other body parts or shield against other radioactive substances.

  • Simulate the decay of a radioactive substance to visualize its half-life

    By definition, the half-life is the amount of time it takes for half of a radioactive sample to decay. With each half-life that has elapsed, half of the starting sample is left, leaving less to decay each time. This results in the number of undecayed atoms decreasing exponentially, with less stable substances having shorter half-lives and decreasing exponentially more rapidly.

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