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Radioactivity. Detection, shielding, dating and half-life

13/03/2026

The online radioactivity simulations on this page will help you understand the basic principles of radioactivity and enlighten you on some of its most important associated concepts such as radioactive detection, radioactive shielding, radioactive dating and radioactive half-life.

What is radioactivity

Radioactivity is the phenomenon by which some chemical elements, called radioisotopes, spontaneously emit radiation. This radiation can be in the form of alpha particles, beta particles, gamma rays or a combination of these types of radiation.

Radioactivity occurs due to the nuclear instability of certain atoms. The nuclei of these atoms are unstable and tend to decay, releasing energy in the form of radiation. This radiation can have ionizing effects, which means that it can release electrons from the atoms and molecules with which it interacts.

Applications of radioactivity

Radioisotopes are used in a variety of applications, such as in nuclear medicine for the diagnosis and treatment of disease, in industry for the inspection of materials, and in nuclear power generation.

Risks associated with radioactivity

Radioactivity can be dangerous to living beings if excessive exposure occurs or if radioactive materials are released into the environment in an uncontrolled manner. Prolonged exposure to ionizing radiation can have detrimental health effects, such as cell damage, genetic mutations and increased risk of developing cancer. Therefore, precautions must be taken and safety limits established to minimize exposure to radioactivity and protect people and the environment.

In the event of a nuclear or radiological incident, it is important to follow the directions of the authorities and evacuate or take protective measures as necessary. Regulatory agencies and nuclear safety programs are responsible for monitoring and regulating the use of radioactive materials to ensure the protection of public health and the environment.

Explore the exciting STEM world with our free, online, simulations and accompanying companion courses! With them you’ll be able to experience and learn hands-on. Take this opportunity to immerse yourself in virtual experiences while advancing your education – awaken your scientific curiosity and discover all that the STEM world has to offer!

Radioactivity simulations

Radioactivity detection


Radioactivity shielding


Half-Life I


In radioactivity, the half-life is the time interval required for half of the atomic nuclei in a radioactive sample to decay. If the half-life passes again, half of the remaining mass will remain (1/2, 1/4, 1/8, 1/16, 1/32, …) The mass gets smaller and smaller, but there is always a little bit left.






Half-Life II


Radioactivity dating


This simulation explains the concept of half-life, including the random nature of half-life, in terms of single particles and larger samples. It describes decay processes, including how elements change and emit energy and/or particles. Explains how radiometric dating works and why different elements are used for dating different objects. Also identifies that 1/2 life is the average time for a radioactive substance to decay.
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Radioactivity is a natural process in which unstable atomic nuclei spontaneously transform into more stable configurations by emitting energy in the form of particles or electromagnetic radiation. This phenomenon shows that nuclei are not rigid or static objects but dynamic systems whose stability depends on the balance between protons and neutrons. When this balance is not optimal, the nucleus undergoes transformations such as alpha, beta, or gamma decay to reach a more stable state. Radioactivity is essential for understanding the internal structure of matter, the formation and evolution of chemical elements, the origin of nuclear energy, and natural processes such as geological dating and the heat generated inside Earth.
The types of radiation differ in their physical nature, energy, and ability to penetrate materials. Alpha radiation consists of helium nuclei and has low penetration but high ionizing power. Beta radiation consists of electrons or positrons and has intermediate penetration. Gamma radiation is high‑energy electromagnetic radiation capable of passing through dense materials. These differences determine how each type interacts with matter, what shielding is required to stop it, and what biological or technological effects it may produce. Understanding these distinctions is crucial for safely handling radioactive materials and for applying them in medicine, industry, and scientific research.
An element becomes radioactive when the combination of protons and neutrons in its nucleus is not stable. If there are too many protons, the electric repulsion becomes excessive; if there are too many neutrons, the nuclear forces also fall out of balance. The nucleus does not consciously decide anything; it simply cannot maintain its structure indefinitely. When the internal forces no longer balance properly, the nucleus emits particles or energy to reorganize itself into a more stable configuration.
It depends entirely on the type of radiation, the intensity, and the duration of exposure. Alpha radiation cannot penetrate the skin but is dangerous if inhaled or ingested. Beta radiation can enter the body more easily, and gamma radiation can pass through it entirely. Radioactivity is not inherently harmful or beneficial; it is a physical phenomenon that becomes dangerous only when exposure exceeds safe limits. At the same time, it is extremely useful in medicine, industry, energy production, and scientific analysis. The key is understanding it and applying proper safety measures.
Radioactive materials do not disappear immediately because each nucleus has a fixed probability of decaying over time. This probability defines the half‑life, which can range from fractions of a second to millions of years. As long as there are unstable nuclei present, the material will continue to emit radiation. The process is gradual and statistical: each atom decays independently, so the overall activity decreases smoothly rather than abruptly. This is why some radioactive elements persist for geological timescales.

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