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Radionuclide

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A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that is unstable and known to undergo radioactive decay into a different nuclide, which may be another radionuclide (see decay chain) or be stable. Radiation emitted by radionuclides is almost always ionizing radiation because it is energetic enough to liberate an electron from another atom.

Radioactive decay is a random process at the level of single atoms: it is impossible to predict when one particular atom will decay.[1][2] However, for a collection of atoms of a single nuclide, the decay rate (considered as a statistical average), and thus the half-life (t1/2) for that nuclide, can be calculated from the measurement of the decay. The range of the half-lives of radioactive atoms has no known limits and spans a time range of over 55 orders of magnitude.

Radionuclides occur naturally and are artificially produced in nuclear reactors, cyclotrons, particle accelerators or radionuclide generators. There are 735 known radionuclides with half-lives longer than an hour (see list of nuclides); 35 of those are primordial radionuclides whose presence on Earth has persisted from its formation, and another 62 are detectable in nature, either as daughters of primordial radionuclides or as radionuclides produced through natural production on Earth by cosmic radiation. More than 2400 radionuclides have half-lives less than 60 minutes. Most of those are only produced artificially, and have very short half-lives. For comparison, there are 251 stable nuclides.

All the chemical elements have radionuclides - even the lightest element, hydrogen, has one well-known radionuclide, tritium (though helium, lithium, and boron have none with half-life over a second). Elements heavier than lead, and the elements technetium and promethium, have only radionuclides and do not exist in stable forms, though bismuth can generally be treated as stable with the half-life of its natural isotope being extremely long and its decay normally undetectable.

Exposure to radionuclides generally has, due to their radiation, a harmful effect on living organisms including humans, although low levels of exposure occur naturally. The degree of harm will depend on the nature and extent of the radiation produced, the amount and nature of exposure (close contact, inhalation or ingestion), and the biochemical properties of the element; with increased risk of cancer considered unavoidable. However, radionuclides with suitable properties are used in nuclear medicine for both diagnosis and treatment. An imaging tracer made with radionuclides is called a radioactive tracer. A pharmaceutical drug made with radionuclides is called a radiopharmaceutical.

Origin

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Natural

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On Earth, naturally occurring radionuclides fall into three categories: primordial radionuclides, secondary radionuclides, and cosmogenic radionuclides.

  • Radionuclides are produced in stellar nucleosynthesis and supernova explosions along with stable nuclides. Most decay quickly, but some can be observed astronomically and can play a part in understanding astrophysical processes. Primordial radionuclides, such as uranium and thorium, still exist because their half-lives are so long (>100 million years) that the Earth's initial content has not yet completely decayed. Some radionuclides have half-lives so long (many times the age of the universe) that decay has only recently been detected, and for most practical purposes they can be considered stable, most notably bismuth-209: detection of this decay meant that bismuth was no longer considered stable. It is possible that decay may be observed in other nuclides now considered stable, adding to the list of primordial radionuclides.[citation needed]
  • Secondary radionuclides are radiogenic isotopes derived from the decay of primordial radionuclides. They have shorter half-lives than primordial radionuclides. They arise in the decay chain of the primordial isotopes thorium-232, uranium-238, and uranium-235 - such as the natural isotopes of polonium and radium - some are also produced by natural fission and other nucleogenic processes.[citation needed]
  • Cosmogenic isotopes, such as carbon-14, are present because they are continually being formed on Earth, typically in the atmosphere, due to the action of cosmic rays.[citation needed]

Many of these radionuclides exist only in trace amounts in nature, including all cosmogenic nuclides. Secondary radionuclides in a decay chain will occur in proportion to their half-lives, so short-lived ones will be very rare. For example, polonium can be found in uranium ores at a concentration about 1 part 1010 of uranium (0.1 mg per metric ton) by calculating the ratio of half-lives of polonium-210 to uranium-238, its ultimate parent.[citation needed]

Nuclear fission

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Radionuclides are produced as an unavoidable result of nuclear fission and nuclear explosions. The process of nuclear fission creates a wide range of fission products, most of which are radionuclides. Further radionuclides are created from irradiation of the nuclear fuel (creating a range of actinides) and of the surrounding structures, yielding activation products. This complex mixture of radionuclides with different chemistries and radioactivity makes handling nuclear waste and dealing with nuclear fallout particularly problematic.[citation needed]

Synthetic

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Americium-241 emitting alpha particles inserted into a cloud chamber

Synthetic radionuclides are created in nuclear reactors or by particle accelerators (not necesssarily on purpose) or as decay products of such:[3]

  • As well as being extracted from nuclear waste, radioisotopes can be produced deliberately with nuclear reactors, exploiting the high flux of neutrons present. These neutrons activate elements placed within the reactor. A typical product from a nuclear reactor is iridium-192, from activation of iridium targets. The elements that have a large propensity to take up neutrons in the reactor are said to have a high neutron cross-section, but even at low cross-sections this process is generally economical.
  • Particle accelerators such as cyclotrons accelerate particles to bombard a target to produce radionuclides. Cyclotrons accelerate (most often) protons at a target to produce positron-emitting radionuclides, e.g. fluorine-18.
  • Radionuclide generators, standard for many medical isotopes, contain a parent radionuclide that decays to produce a shorter-lived radioactive daughter. A typical example is the technetium-99m generator, which employs molybdenum-99 produced in a reactor.

Uses

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Radionuclides are used in two major ways: either for their radiation alone (irradiation, nuclear batteries) or for the combination of chemical properties and their radiation (tracers, biopharmaceuticals). For scientific study they may be used for their chemical properties alone when there is no stable form of that element.

Examples

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The following table lists properties of selected radionuclides illustrating the range of properties and uses.

Isotope Z N half-life DM DE
keV
Mode of formation Comments
Tritium (3H) 1 2 12.3 y β 19 Cosmogenic lightest radionuclide, used in artificial nuclear fusion, also used for radioluminescence and as oceanic transient tracer. Synthesized from neutron bombardment of lithium-6 or deuterium
Beryllium-10 4 6 1,387,000 y β 556 Cosmogenic used to examine soil erosion, soil formation from regolith, and the age of ice cores
Carbon-14 6 8 5,700 y β 156 Cosmogenic used for radiocarbon dating
Fluorine-18 9 9 110 min β+, EC 633/1655 Cosmogenic positron source, synthesised for use as a medical radiotracer in PET scans.
Aluminium-26 13 13 717,000 y β+, EC 4004 Cosmogenic exposure dating of rocks, sediment
Chlorine-36 17 19 301,000 y β, EC 709 Cosmogenic exposure dating of rocks, groundwater tracer
Potassium-40 19 21 1.24×109 y β, EC 1330 /1505 Primordial used for potassium-argon dating, source of atmospheric argon, source of radiogenic heat, largest source of natural radioactivity
Calcium-41 20 21 99,400 y EC Cosmogenic exposure dating of carbonate rocks
Cobalt-60 27 33 5.3 y β 2824 Synthetic produces high energy gamma rays, used for radiotherapy, equipment sterilisation, food irradiation
Krypton-81 36 45 229,000 y β+ Cosmogenic groundwater dating
Strontium-90 38 52 28.8 y β 546 Fission product medium-lived fission product; probably most dangerous component of nuclear fallout
Technetium-99 43 56 210,000 y β 294 Fission product most common isotope of the lightest unstable element, most significant of long-lived fission products
Technetium-99m 43 56 6 hr γ,IC 141 Synthetic most commonly used medical radioisotope, used as a radioactive tracer
Iodine-129 53 76 15,700,000 y β 194 Cosmogenic longest lived fission product; groundwater tracer
Iodine-131 53 78 8 d β 971 Fission product most significant short-term health hazard from nuclear fission, used in nuclear medicine, industrial tracer
Xenon-135 54 81 9.1 h β 1160 Fission product strongest known "nuclear poison" (neutron-absorber), with a major effect on nuclear reactor operation.
Caesium-137 55 82 30.2 y β 1176 Fission product other major medium-lived fission product of concern
Gadolinium-153 64 89 240 d EC Synthetic Calibrating nuclear equipment, bone density screening
Bismuth-209 83 126 2.01×1019y α 3137 Primordial long considered stable, decay only detected in 2003
Polonium-210 84 126 138 d α 5307 Decay product Highly toxic, used in poisoning of Alexander Litvinenko
Radon-222 86 136 3.8 d α 5590 Decay product gas, responsible for the majority of public exposure to ionizing radiation, second most frequent cause of lung cancer
Thorium-232 90 142 1.4×1010 y α 4083 Primordial basis of thorium fuel cycle
Uranium-235 92 143 7×108y α 4679 Primordial fissile, main nuclear fuel
Uranium-238 92 146 4.5×109 y α 4267 Primordial Main Uranium isotope
Plutonium-238 94 144 87.7 y α 5593 Synthetic used in radioisotope thermoelectric generators (RTGs) and radioisotope heater units as an energy source for spacecraft
Plutonium-239 94 145 24,110 y α 5245 Synthetic used for most modern nuclear weapons
Americium-241 95 146 432 y α 5486 Synthetic used in household smoke detectors as an ionising agent
Californium-252 98 154 2.64 y α/SF 6217 Synthetic undergoes spontaneous fission (3% of decays), making it a powerful neutron source, used as a reactor initiator and for detection devices

Key: Z = atomic number; N = neutron number; DM = decay mode; DE = decay energy; EC = electron capture

Household smoke detectors

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Americium-241 container in a smoke detector.
Americium-241 capsule as found in smoke detector. The circle of darker metal in the center is americium-241; the surrounding casing is aluminium.

Radionuclides are present in many homes as they are used inside the most common household smoke detectors. The radionuclide used is americium-241, which is created by bombarding plutonium with neutrons in a nuclear reactor. It decays by emitting alpha particles and gamma radiation to become neptunium-237. Smoke detectors use a very small quantity of 241Am (about 0.29 micrograms per smoke detector) in the form of americium dioxide. 241Am is used as it emits alpha particles which ionize the air in the detector's ionization chamber. A small electric voltage is applied to the ionized air which gives rise to a small electric current. In the presence of smoke, some of the ions are neutralized, thereby decreasing the current, which activates the detector's alarm.[8][9]

Impacts on organisms

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Radionuclides that find their way into the environment may cause harmful effects as radioactive contamination. They can also cause damage if they are excessively used during treatment or in other ways exposed to living beings, by radiation poisoning. Potential health damage from exposure to radionuclides depends on a number of factors, and "can damage the functions of healthy tissue/organs. Radiation exposure can produce effects ranging from skin redness and hair loss, to radiation burns and acute radiation syndrome. Prolonged exposure can lead to cells being damaged and in turn lead to cancer. Signs of cancerous cells might not show up until years, or even decades, after exposure."[10]

Summary table for classes of nuclides, stable and radioactive

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Following is a summary table for the list of 986 nuclides with half-lives greater than one hour. A total of 251 nuclides have never been observed to decay, and are classically considered stable. Of these, 90 are believed to be absolutely stable except to proton decay (which has never been observed), while the rest are "observationally stable" and theoretically can undergo radioactive decay with extremely long half-lives.[citation needed]

The remaining tabulated radionuclides have half-lives longer than 1 hour, and are well-characterized (see list of nuclides for a complete tabulation). They include 31 nuclides with measured half-lives longer than the estimated age of the universe (13.8 billion years[11]), and another four nuclides with half-lives long enough (> 100 million years) that they are radioactive primordial nuclides, and may be detected on Earth, having survived from their presence in interstellar dust since before the formation of the Solar System, about 4.6 billion years ago. Another 60+ short-lived nuclides can be detected naturally as daughters of longer-lived nuclides or cosmic-ray products. The remaining known nuclides are known solely from artificial nuclear transmutation.[citation needed]

Numbers may change slightly in the future as some nuclides now classified as stable are observed to be radioactive with very long half-lives.[citation needed]

This is a summary table[12] for the 986 nuclides with half-lives longer than one hour (including those that are stable), given in list of nuclides.

Stability class Number of nuclides Running total Notes on running total
Theoretically stable to all but proton decay 90 90 Includes first 40 elements. Proton decay yet to be observed.
Theoretically stable to alpha decay, beta decay, isomeric transition, and double beta decay but not spontaneous fission, which is possible for "stable" nuclides ≥ niobium-93 56 146 All nuclides that are possibly completely stable (spontaneous fission has never been observed for nuclides with mass number < 232).
Energetically unstable to one or more known decay modes, but no decay yet seen. All considered "stable" until decay detected. 105 251 Total of classically stable nuclides.
Radioactive primordial nuclides 35 286 Total primordial elements include uranium, thorium, bismuth, rubidium-87, potassium-40, tellurium-128 plus all stable nuclides.
Radioactive nonprimordial, but naturally occurring on Earth 62 348 Carbon-14 (and other isotopes generated by cosmic rays) and daughters of radioactive primordial elements, such as radium and polonium, of which 32 have a half-life of greater than one hour, also long-lived fission products.
Radioactive synthetic half-life ≥ 1.0 hour). Includes most useful radiotracers. 638 986 These comprise the remainder of the list of nuclides.
Radioactive synthetic (half-life < 1.0 hour). >2400 >3300 Includes all well-characterized synthetic nuclides.

See also

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Notes

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  1. ^ "Decay and Half Life". Retrieved 2009-12-14.
  2. ^ Loveland, W.; Morrissey, D.; Seaborg, G.T. (2006). Modern Nuclear Chemistry. Wiley-Interscience. p. 57. Bibcode:2005mnc..book.....L. ISBN 978-0-471-11532-8.
  3. ^ "Radioisotopes". www.iaea.org. 2016-07-15. Retrieved 2023-06-25.
  4. ^ Ingvar, David H. [in Swedish]; Lassen, Niels A. (1961). "Quantitative determination of regional cerebral blood-flow in man". The Lancet. 278 (7206): 806–807. doi:10.1016/s0140-6736(61)91092-3.
  5. ^ Ingvar, David H. [in Swedish]; Franzén, Göran (1974). "Distribution of cerebral activity in chronic schizophrenia". The Lancet. 304 (7895): 1484–1486. doi:10.1016/s0140-6736(74)90221-9. PMID 4140398.
  6. ^ Lassen, Niels A.; Ingvar, David H. [in Swedish]; Skinhøj, Erik [in Danish] (October 1978). "Brain Function and Blood Flow". Scientific American. 239 (4): 62–71. Bibcode:1978SciAm.239d..62L. doi:10.1038/scientificamerican1078-62. PMID 705327.
  7. ^ Severijns, Nathal; Beck, Marcus; Naviliat-Cuncic, Oscar (2006). "Tests of the standard electroweak model in nuclear beta decay". Reviews of Modern Physics. 78 (3): 991–1040. arXiv:nucl-ex/0605029. Bibcode:2006RvMP...78..991S. doi:10.1103/RevModPhys.78.991. S2CID 18494258.
  8. ^ "Smoke Detectors and Americium". world-nuclear.org. Archived from the original on 2010-11-12.
  9. ^ Office of Radiation Protection – Am 241 Fact Sheet – Washington State Department of Health Archived 2011-03-18 at the Wayback Machine
  10. ^ "Ionizing radiation, health effects and protective measures". World Health Organization. November 2012. Retrieved January 27, 2014.
  11. ^ "Cosmic Detectives". The European Space Agency (ESA). 2013-04-02. Retrieved 2013-04-15.
  12. ^ Table data is derived by counting members of the list; see WP:CALC. References for the list data itself are given below in the reference section in list of nuclides

References

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Further reading

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