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Radioactivity. Detection, shielding, dating and half-life

08/06/2026

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.

This Thematic Unit is part of our Chemistry collection

STEM OnLine mini dictionary

Alpha Emission (α)

Type of decay where the nucleus emits a heavy particle composed of two protons and two neutrons (Helium-4 nucleus).

Beta Emission (β)

Nuclear process where a neutron transforms into a proton by emitting a high-energy electron or positron.

Gamma Radiation (γ)

Emission of high-frequency electromagnetic waves with high penetrating power that often accompanies alpha and beta processes.

Half-life

Time required for half of the nuclei in a radioactive sample to decay into a different element.

Natural Radioactivity

Phenomenon present in nature due to unstable isotopes existing in the Earth’s crust or produced by cosmic rays.

Nuclear Stability

Balance of forces within the nucleus that determines whether an atom will remain intact or undergo spontaneous decay.

Nuclide

Atomic species characterized by its number of protons and neutrons, and its nuclear energy state.

Radioactivity

Spontaneous process of decay of unstable atomic nuclei through the emission of particles and electromagnetic energy.

What Is radioactivity

Radioactivity is a physical and chemical phenomenon in which the nuclei of certain unstable atoms lose energy by spontaneously emitting radiation. These atoms are known as radioisotopes.

To understand why this happens, we must look inside the atom’s nucleus, where protons and neutrons coexist. In nature, most of the atoms around us are stable; their nuclei have a perfect balance of forces and remain unchanged over time. However, when a nucleus is too large or has a clear excess of protons or neutrons, it becomes unstable.

To release that internal tension and seek stability, the nucleus decays naturally. During this decay process, the atom “spits out” particles or bursts of pure energy. We refer to this entire set of emissions as radiation. This process continues spontaneously until the unstable atom transforms into a completely different and chemically stable element, such as uranium, which, after many decays, eventually becomes lead.

Types of ionizing radiation

Radiation emitted by unstable nuclei has ionizing effects. This means it has enough energy to knock electrons out of the atoms it collides with, altering the structure of matter. Depending on the nature of the emission, physicists classify this radiation into three broad categories.

Alpha (α) radiation: heavy particles

Alpha radiation occurs when an atom’s nucleus is too large and needs to lose mass quickly. The nucleus emits an alpha particle, which consists of two protons and two neutrons (equivalent to a helium nucleus). Because these particles are so large and heavy, they have a high positive electric charge and move at relatively slow speeds. Due to their large size, they have very little penetrating power: a single sheet of paper or the outer layer of our skin is enough to stop them completely.

Beta radiation (β): escaping electrons

Beta radiation occurs when the nucleus has an imbalance between its protons and neutrons. To correct this, a neutron transforms into a proton, and in the process, the nucleus ejects an electron at extremely high speed, known as a beta particle. Since they are thousands of times smaller than alpha particles, they have moderate penetrating power. They can pass through paper and travel a few meters through the air, but they can be easily stopped by a thin sheet of aluminum or a piece of wood.

Gamma rays (γ): pure energy

Unlike the previous types, gamma radiation does not involve the emission of material particles, but rather the emission of high-energy electromagnetic waves (photons). It occurs when the nucleus, following an alpha or beta decay, still has excess accumulated energy and needs to fully stabilize. Since they have no mass or electric charge, gamma rays travel at the speed of light and have extremely high penetrating power. They can pass through the human body and require very dense materials, such as thick concrete walls or lead plates, to be stopped.

Half-life. How long does radioactivity last?

The decay of an atom is a purely random event; it is impossible to predict exactly which millisecond a specific nucleus will decay. However, when we analyze a sample containing millions of unstable atoms, the behavior becomes predictable and follows a strict mathematical law.

To measure the rate at which an element’s radioactivity decays, we use the concept of half-life, a term you’ll also find in physics and chemistry textbooks referred to as the half-life period. Both concepts mean exactly the same thing: it is the time required for half of the radioactive nuclei in an initial sample to decay and transform into stable elements.

For example, if you have a sample of 100 grams of a radioisotope with a half-life of one year, after twelve months you will have 50 grams of radioactive material left. After another year, the amount will be reduced to half of what remained, that is, 25 grams, and so on.

This rate of decay varies drastically depending on the chemical element being measured:

–    Uranium-238 has a half-life of about 4.5 billion years, nearly the age of the Earth.

–    Carbon-14 has a half-life of 5,730 years, which allows archaeologists to date ancient organic remains.

–    Iodine-131, used in medical treatments, has a half-life of just 8 days, ensuring that it does not remain in the body for very long.

Practical applications of radioisotopes

Despite the negative reputation that often surrounds nuclear energy, controlled radiation is an indispensable tool in modern society. By knowing the exact half-life of each radioisotope and the type of particle it emits, science has learned to use them for the benefit of health and technical progress.

Nuclear medicine and diagnostics

In hospitals, very short-lived radioisotopes are used for two main purposes: diagnosis and treatment. For diagnosis, small doses of radioactive substances are introduced into the patient’s body to act as tracers, allowing advanced scanners such as PET to obtain detailed images of the interior of organs. In the field of treatment, techniques such as radiation therapy use intense sources of gamma radiation directed with pinpoint accuracy to destroy cancer cells and slow tumor growth.

Nuclear energy and industry

In the industrial sector, radioisotopes are used as high-precision inspection tools. Gamma emissions enable industrial radiography to check the quality of welds in pipes or detect invisible cracks in aircraft structures without having to disassemble them. On the other hand, the best-known application is electricity generation in nuclear power plants, where the immense amount of thermal energy released during the fission of heavy nuclei such as uranium is harnessed.

Risks Associated with Radioactivity

Radioactivity can be dangerous to living organisms if there is excessive exposure or if radioactive materials are released into the environment in an uncontrolled manner. Prolonged exposure to ionizing radiation can have harmful health effects, such as cellular damage, genetic mutations, and an 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.

To work safely with radioactive materials, medical physics and engineering rely on three fundamental pillars of radiation protection:

Time

The accumulated radiation dose is directly proportional to the time spent near the source. Reducing handling time to the absolute minimum is the first line of defense.

Distance

The intensity of radiation decreases dramatically as we move away from the source. Doubling the distance reduces exposure to one-fourth.

Shielding

Placing adequate physical barriers between the source and people blocks the particles. As we saw when analyzing the types of radiation, aluminum sheets are used for beta particles, and thick walls of lead or concrete are used to contain gamma rays.

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

STEM OnLine mini dictionary

Alpha Emission (α)

Type of decay where the nucleus emits a heavy particle composed of two protons and two neutrons (Helium-4 nucleus).

Beta Emission (β)

Nuclear process where a neutron transforms into a proton by emitting a high-energy electron or positron.

Gamma Radiation (γ)

Emission of high-frequency electromagnetic waves with high penetrating power that often accompanies alpha and beta processes.

Half-life

Time required for half of the nuclei in a radioactive sample to decay into a different element.

Natural Radioactivity

Phenomenon present in nature due to unstable isotopes existing in the Earth’s crust or produced by cosmic rays.

Nuclear Stability

Balance of forces within the nucleus that determines whether an atom will remain intact or undergo spontaneous decay.

Nuclide

Atomic species characterized by its number of protons and neutrons, and its nuclear energy state.

Radioactivity

Spontaneous process of decay of unstable atomic nuclei through the emission of particles and electromagnetic energy.

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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