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Atoms – Nuclides, isotopes and radioactivity

Everything around us is made up of atoms. A nuclide is a type of atom, and nuclides that are radioactive are called radionuclides. Radionuclides of the same element are called radioisotopes.

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Atoms

An atom has protons and neutrons that make up the nucleus. Electrons orbit the nucleus in clouds (or shells) and carry a negative charge. The negative electrons are attracted to the positive nucleus by an electrical force. This attraction is what keeps the electrons orbiting the nucleus.

Protons are positively charged but neutrons don’t carry a charge. The nucleus therefore carries a positive charge.

The strong nuclear force binds the protons and neutrons to hold the nucleus together, despite protons repelling each other.

This image shows the structure of an atom made up of a nucleus that consists of protons (positive) and neutrons (neutral) in the center with orbiting electrons (negative).

Each element is identified using a unique atomic number, which is also the number of protons in the nucleus of each atom forming that element. For example, carbon has the atomic number 6 on the periodic table because there are 6 protons in the nucleus of a carbon atom.

Periodic table of elements

Periodic Table

An atom is stable when the number of neutrons and protons in the nucleus is balanced (although balance does not always mean an equal number of neutrons and protons). When there is a major imbalance between the number of neutrons and protons in the nucleus, an atom becomes unstable.

The atom may then transform by releasing energy to become stable. This process emits energy in the form of ionizing radiation, and is called radioactive decay.

Atoms from 1 or more elements can combine to form a larger compound called a molecule. For example, a molecule of water (H2O), is made up of 2 atoms of hydrogen (H) combined with 1 atom of oxygen (O).

This image shows a water molecule, made up of one oxygen atom and two hydrogen atoms.

Nuclides

nuclide is a specific type of atom defined by the total number of protons and neutrons in its nucleus. This number represents the nuclide’s approximate mass and is called the mass number.

A nuclide’s mass number is measured in atomic mass units (amu). For example, Carbon-12 has 6 protons and 6 neutrons, and a mass of 12 amu.

This image shows how an atom is characterized in the periodic table. The example used is Carbon with an atomic number of 6 in the upper left hand corner, the chemical symbol of “C” in the center, with the chemical name “Carbon” below and the atomic mass of 12.011 g / mol.

Isotopes

Nuclides of an element that have the same number of protons but a different number of neutrons are called isotopes of that element. They are a variant of a basic element. For example, there are 3 isotopes (or versions) of hydrogen:

  • Hydrogen-1 or protium has 1 proton and no neutrons.
  • Hydrogen-2 or deuterium has 1 proton and 1 neutron.
  • Hydrogen-3 or tritium has 1 proton and 2 neutrons.

Isotopes of hydrogen

This image shows the atomic structure of hydrogen and two hydrogen isotopes, Hydrogen-2 (Deuterium) which has an additional neutron, and Hydrogen-3 (Tritium) which has two extra neutrons.

Isotopes of uranium include:

  • uranium-235, with 92 protons and 143 neutrons
  • uranium-238, with 92 protons and 146 neutrons

Stable isotopes

Many isotopes are stable. They do not undergo radioactive decay and do not give off radiation. An isotope is stable when there is a balance between the number of neutrons and protons. This balance does not always mean the 2 are present in equal numbers however.

When an isotope is small and stable, it contains close to an equal number of protons and neutrons. Isotopes that are larger and stable have increasingly more neutrons than protons. This balances repulsion from the positively charged protons near each other.

An example of a stable isotope is carbon-12, which has 6 protons and 6 neutrons, for a total mass of 12 amu.

This image shows the atomic structure of Hydrogen-1 and Carbon-12.
This image shows the atomic structure of two isotopes of carbon, carbon-12 and carbon-14. The number after the atom name indicates the number of protons and neutrons. Both of the carbon isotopes contain 6 protons; carbon-12 has 6 neutrons, whereas carbon-14 has 8 neutrons.

Unstable isotopes

An unstable isotope is an atom with an unstable nucleus due to an imbalance between protons and neutrons. Unstable isotopes are radioactive, so they are called radioisotopes.

The imbalance often happens when the ratio of neutrons to protons is too low. When this happens, the atom loses energy by giving off ionizing radiation in order to obtain a stable state. This causes the atom to decrease its mass and become a different element. Some atoms may also gain stability through other means, such as spontaneous nuclear fission.

These spontaneous processes that emit energy are known as radioactive decay. Energy can be emitted in the form of alpha particles, beta particles (electrons and positrons) and/or gamma rays. There are 3 main types of radioactive decay:

  • alpha decay
  • beta decay
  • gamma decay

Alpha decay

Alpha decay happens when a particle consisting of 2 neutrons and 2 protons is ejected from an atom’s nucleus.

This causes the atomic number to decrease by 2 and the mass to decrease by 4.

Beta decay

In the most common type of beta decay, a neutron turns into a proton by emitting an electron from the atom’s nucleus.

The atomic number (number of protons) increases by 1. The mass decreases only slightly – because electrons contribute a very small amount to an atom’s mass.

Gamma decay

Gamma decay takes place when there is residual energy in the nucleus following either alpha or beta decay. The residual energy is released as a photon of gamma radiation. Gamma decay generally does not affect the mass or atomic number of the nuclide.

It can also take place after neutron capture in a nuclear reactor.

This image shows three types of radioactive decay, alpha decay, beta decay, and gamma decay. In Alpha decay two neutrons and two protons are ejected, in beta decay a neutron is turned into a proton and an electron is ejected, in gamma decay a photon of gamma radiation is emitted.

Radionuclides

When a nuclide disintegrates spontaneously, it emits excess energy that is a form of ionizing radiation called T, in other words, activity. The nuclide that changes and emits radiation is called a radionuclide.

These disintegrations are expressed or measured in a unit called a becquerel (Bq). 1 Bq = 1 disintegration per second.

Half-life

Half-life is the time it takes for a radionuclide to decay to half of its starting activity. The decay is exponential.

Each radionuclide has a unique half-life that can range from a fraction of a second to billions of years. For example, iodine-131 takes 8 days to reach half of its original activity, while plutonium-239 takes 24,000 years.

The symbol for half-life is t½. You can predict how long a radionuclide will take to decay if the original source of the radioactivity is known. The reverse is also true: if you know a radionuclide’s half-life, you can identify the radionuclide.

This image shows a graph demonstrating the decay of Iodine-131. The graph shows the percent of Iodine-131 decreasing with each half-life (8 days each).

Specific activity

Specific activity is the activity (the disintegration rate of a nuclide that gives off radiation, or the number of decays per second) per unit of mass of a radionuclide.

Half-life and specific activity have an inversely proportional relationship. The shorter a radionuclide’s half-life is, the more activity the radionuclide gives off.

Cobalt-60, for example, has a shorter half-life than uranium-238 and gives off more radiation per second by gram. It decays more quickly than uranium-238, which gives off less radiation per second by gram and decays more slowly.

Three circular diagrams titled Polonium-210, Technetium-99, and Uranium-235, each showing a stylized decay radiation pattern radiating outward from a small central icon of a weight. Below each diagram are three lines of text showing the activity, weight, and half-life: Polonium-210 has 1 gigabecquerel, 0.006 mg, and a half-life of 138.4 days; Technetium-99 has 1 gigabecquerel, 1.6 g, and a half-life of 214,000 years; Uranium-235 has 1 gigabecquerel, 12 kg, and a half-life of 703,800,000 years.

The following table compares different radionuclides with different half-lives and shows the inverse relationship between half-life and specific activity. The last column shows how many milligrams of the isotope are required to yield 1 MBq of activity. Specific activity is expressed in units of becquerels per gram, and depends on each radionuclide’s half-life and atomic mass.

Comparison of radionuclide half-lives and specific activity

 Radionuclide Half-life Specific activity* Milligrams (mg) per megabecquerel (MBq)
Polonium-210 138.4 days 166.3E12
(166.3 TBq/gr)
0.000006
Cobalt-60 5.3 years 41.9E12
(41.9 TBq/gr)
0.0000239
Cesium-137 30.04 years 3.2E12
(3.2 TBq/gr)
0.0003109
Carbon-14 5,700 years 165.7E9
(165.7 GBq/gr)
0.006
Technetium-99 214,000 years 624.9E6
(624.9 MBq/gr)
1.6
Uranium-235 703.8 million years 80.0E3
(80.0 kBq/gr)
12,000.5
Uranium-238 4.468 billion years 12.4E3
(12.4 kBq/gr)
80,000.4

*TBq: terabecquerel (1 trillion Bq)
GBq: gigabecquerel (1 billion Bq)
MBq: megabecquerel (1 million Bq)
kBq: kilobecquerel (1,000 Bq)

Natural versus artificial sources of radionuclides

Many radionuclides occur naturally and originate from the formation of the solar system. Some radionuclides, such as tritium, come from the interaction of cosmic rays with molecules in the atmosphere.

Some radionuclides – like uranium and thorium – that were formed at the time of the solar system’s origin have half-lives of billions of years. They are still in our environment.

Radionuclides are also created as a by-product of the operation of nuclear reactors and by radionuclide generators, such as cyclotrons. Many artificial radionuclides are used in:

  1. nuclear medicine and biochemistry
  2. the manufacturing industry
  3. agriculture

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