Radionuclide: Difference between revisions
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{{short description|Atom that has excess nuclear energy, making it unstable}} |
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{{refimprove|date=April 2010}} |
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{{distinguish|radionucleotide (disambiguation){{!}}radionucleotide}} |
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A '''radionuclide''' ('''radioactive nuclide''', '''radioisotope''' or '''radioactive isotope''') is a [[nuclide]] that has excess numbers of either [[neutron]]s or [[proton]]s, giving it excess nuclear energy, and making it unstable. This excess energy can be used in one of three ways: emitted from the nucleus as [[gamma radiation]]; transferred to one of its [[electron]]s to release it as a [[Internal conversion|conversion electron]]; or used to create and emit a new [[particle]] ([[alpha particle]] or [[beta particle]]) from the nucleus. During those processes, the radionuclide is said to undergo [[radioactive decay]].<ref>{{cite book |first=R. H. |last=Petrucci |first2=W. S. |last2=Harwood |first3=F. G. |last3=Herring |title=General Chemistry |edition=8th |publisher=Prentice-Hall |year=2002 |pages=1025–26 |isbn=0-13-014329-4 }}</ref> These emissions are considered [[ionizing radiation]] because they are energetic enough to liberate an electron from another atom. The radioactive decay can produce a stable nuclide or will sometimes produce a new unstable radionuclide which may undergo further decay. Radioactive decay is a random process at the level of single atoms: it is impossible to predict when one particular atom will decay.<ref name="not-predict">{{cite web|url=http://www.iem-inc.com/prhlfr.html|title=Decay and Half Life|access-date= 2009-12-14}}</ref><ref name="IntroductionToHealthPhysics">{{cite book |title=Radiation Protection and Dosimetry: An Introduction to Health Physics |last1=Stabin |first1=Michael G. |editor1-first=Michael G |editor1-last=Stabin |isbn=978-0387499826 |year=2007 |publisher=[[Springer Publishing|Springer]] |chapter=3 |doi=10.1007/978-0-387-49983-3|url=https://cds.cern.ch/record/1105894 <!--correct parameter-->|type=Submitted manuscript }}</ref><ref name="RadiationOncologyPrimer">{{cite book |title=Radiation Oncology Primer and Review |isbn=978-1620700044 |last1=Best |first1=Lara |last2=Rodrigues |first2=George |last3=Velker |first3=Vikram |publisher=[[Demos Medical Publishing]] |year=2013 |chapter=1.3}}</ref><ref>{{cite book |title=Modern Nuclear Chemistry |isbn=978-0-471-11532-8 |last1=Loveland |first1=W. |last2=Morrissey |first2=D. |author3-link=Glenn T. Seaborg |last3=Seaborg |first3=G.T. |publisher=Wiley-Interscience |year=2006 |page=57|bibcode=2005mnc..book.....L }}</ref> However, for a collection of atoms of a single nuclide the decay rate, and thus the [[half-life]] (''t''<sub>1/2</sub>) for that collection, can be calculated from their measured [[decay constant]]s. The range of the half-lives of radioactive atoms has no known limits and spans a time range of over 55 orders of magnitude. |
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A '''radionuclide''' or '''radioactive [[nuclide]]''', also referred to as a '''radioisotope''' or '''radioactive [[isotope]]''', is an [[atom]] with an unstable [[Atomic nucleus|nucleus]], characterized by excess energy available to be imparted either to a newly created radiation particle within the nucleus or via [[internal conversion]]. During this process, the radionuclide is said to undergo [[radioactive decay]], resulting in the emission of [[gamma ray]](s) and/or [[subatomic particle]]s such as [[alpha particle|alpha]] or [[beta particle]]s.<ref>R.H. Petrucci, W.S. Harwood and F.G. Herring, ''General Chemistry'' (8th ed., Prentice-Hall 2002), p.1025-26</ref> These emissions constitute [[ionizing radiation]]. Radionuclides occur naturally, or can be produced artificially. |
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There are about |
Radionuclides occur naturally or are artificially produced in [[nuclear reactor]]s, [[cyclotron]]s, [[particle accelerator]]s or [[radionuclide generator]]s. There are about 730 radionuclides with half-lives longer than 60 minutes (see [[list of nuclides]]). Thirty-two of those are [[primordial radionuclide]]s that were created before the Earth was formed. At least another 60 radionuclides 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 about 251 [[stable nuclide]]s. |
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All [[chemical element]]s |
All [[chemical element]]s can exist as radionuclides. Even the lightest element, [[hydrogen]], has a well-known radionuclide, [[tritium]]. Elements heavier than [[lead]], and the elements [[technetium]] and [[promethium]], exist only as radionuclides. |
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Unplanned exposure to radionuclides generally has a harmful effect on living organisms including humans, although low levels of exposure occur naturally without harm. 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 the most usual consequence. 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]]. |
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Radionuclides with suitable [[half-lives]] play an important part in a number of technologies, for example, [[nuclear medicine]] and ionization [[smoke detector]]s. Radionuclides can also present both real and perceived dangers to health. |
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==Origin== |
==Origin== |
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===Natural=== |
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Naturally occurring radionuclides fall into three categories: primordial radionuclides, secondary radionuclides, and [[cosmogenic]] radionuclides. Primordial radionuclides, such as [[uranium]] and [[thorium]], originate mainly from the interiors of [[star]]s and are still present as their [[half-life|half-lives]] are so long they have not yet completely decayed. Secondary radionuclides are radiogenic isotopes derived from the decay of primordial radionuclides. They have shorter half-lives than primordial radionuclides. Cosmogenic isotopes, such as [[carbon-14]], are present because they are continually being formed in the atmosphere due to [[cosmic ray]]s.<ref>{{cite book | chapter = | url = http://books.google.de/books?id=RqEhyic9VJMC&pg=PA134| pages = 134 | title = Environmental Radioactivity: From Natural, Industrial, and Military Sources | isbn = 9780122351549 | author1 = Eisenbud | first1 = Merril | last2 = Gesell | first2 = Thomas F | date = 1997-02-25}}</ref> |
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On Earth, naturally occurring radionuclides fall into three categories: primordial radionuclides, secondary radionuclides, and [[cosmogenic]] radionuclides. |
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* Radionuclides are produced in [[stellar nucleosynthesis]] and [[supernova explosions]] along with stable nuclides. Most decay quickly but can still be observed astronomically and can play a part in understanding astronomic processes. Primordial radionuclides, such as [[uranium]] and [[thorium]], exist in the present time because their [[half-life|half-lives]] are so long (>100 million years) that they have 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 decay may be observed in other nuclides, adding to this list of primordial radionuclides. |
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* 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]]. Examples include the natural isotopes of [[polonium]] and [[radium]]. |
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* [[Cosmogenic isotopes]], such as [[carbon-14]], are present because they are continually being formed in the atmosphere due to [[cosmic ray]]s.<ref>{{cite book |url = https://books.google.com/books?id=RqEhyic9VJMC&pg=PA134| pages = 134 |title = Environmental Radioactivity: From Natural, Industrial, and Military Sources |isbn = 9780122351549 |last1 = Eisenbud |first1 = Merril |last2 = Gesell |first2 = Thomas F |date = 1997-02-25| publisher = Elsevier }}</ref> |
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Many of these radionuclides exist only in trace amounts in nature, including all cosmogenic nuclides. Secondary radionuclides 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 about 0.1 mg per [[metric ton]] (1 part in 10<sup>10</sup>).<ref>Bagnall, K. W. (1962). "The Chemistry of Polonium". Advances in Inorganic Chemistry and Radiochemistry 4. New York: Academic Press. pp. 197–226. doi:10.1016/S0065-2792(08)60268-X. {{ISBN|0-12-023604-4}}. Retrieved June 14, 2012., p. 746</ref><ref>Bagnall, K. W. (1962). "The Chemistry of Polonium". Advances in Inorganic Chemistry and Radiochemistry 4. New York: Academic Press., p. 198</ref> Further radionuclides may occur in nature in virtually undetectable amounts as a result of rare events such as spontaneous fission or uncommon cosmic ray interactions. |
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Artificially produced radionuclides can be produced by [[nuclear reactor]]s, particle accelerators or by radionuclide generators: |
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*Radioisotopes produced with nuclear reactors exploit the high flux of [[neutron]]s present. These neutrons activate elements placed within the reactor. A typical product from a nuclear reactor is [[isotopes of thallium|thallium-201]] and [[iridium-192]]. The elements that have a large propensity to take up the neutrons in the reactor are said to have a high [[neutron cross-section]]. |
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*Particle accelerators such as [[cyclotron]]s accelerate particles to bombard a target to produce radionuclides. Cyclotrons accelerate protons at a target to produce positron-emitting radionuclides, e.g., [[fluorine-18]]. |
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*Radionuclide generators contain a parent radionuclide that decays to produce a radioactive daughter. The parent is usually produced in a nuclear reactor. A typical example is the [[technetium-99m generator]] used in [[nuclear medicine]]. The parent produced in the reactor is [[molybdenum-99]]. |
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*Radionuclides are produced as an unavoidable side-effect of nuclear and thermonuclear explosions. |
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===Nuclear fission=== |
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Trace radionuclides are those that occur in tiny amounts in nature either due to inherent rarity or due to [[half-life|half-lives]] that are significantly shorter than the age of the Earth. Synthetic isotopes are inherently not naturally occurring on Earth, but can be created by [[nuclear reaction]]s. |
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Radionuclides are produced as an unavoidable result of [[nuclear fission]] and [[thermonuclear device|thermonuclear explosions]]. The process of nuclear fission creates a wide range of [[fission products]], most of which are radionuclides. Further radionuclides can be 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.{{cn|date=November 2023}} |
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===Synthetic=== |
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[[File:Artificial nuclide americium-241 emitting alpha particles inserted into a cloud chamber for visualisation.jpg|thumb|[[Artificial]] [[nuclide]] [[americium-241]] emitting [[alpha particle]]s inserted into a [[cloud chamber]] for visualisation]] |
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[[Synthetic radionuclide]]s are deliberately synthesised using [[nuclear reactor]]s, particle accelerators or radionuclide generators:<ref>{{Cite web |date=2016-07-15 |title=Radioisotopes |url=https://www.iaea.org/topics/nuclear-science/isotopes/radioisotopes |access-date=2023-06-25 |website=www.iaea.org |language=en}}</ref> |
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* As well as being extracted from nuclear waste, radioisotopes can be produced deliberately with nuclear reactors, exploiting the high flux of [[neutron]]s present. These neutrons activate elements placed within the reactor. A typical product from a nuclear reactor is [[iridium-192]]. The elements that have a large propensity to take up the neutrons in the reactor are said to have a high [[neutron cross-section]]. |
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* Particle accelerators such as [[cyclotron]]s accelerate particles to bombard a target to produce radionuclides. Cyclotrons accelerate protons at a target to produce positron-emitting radionuclides, e.g. [[fluorine-18]]. |
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* Radionuclide generators contain a parent radionuclide that decays to produce a radioactive daughter. The parent is usually produced in a nuclear reactor. A typical example is the [[technetium-99m generator]] used in [[nuclear medicine]]. The parent produced in the reactor is [[molybdenum-99]]. |
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==Uses== |
==Uses== |
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Radionuclides are used in two major ways: either for their radiation alone ([[irradiation]], [[nuclear battery|nuclear batteries]]) or for the combination of chemical properties and their radiation (tracers, biopharmaceuticals). |
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* In [[biology]], radionuclides of [[carbon]] can serve as [[radioactive tracer]]s because they are chemically very similar to the nonradioactive nuclides, so most chemical, biological, and ecological processes treat them in a nearly identical way. One can then examine the result with a radiation detector, such as a [[Geiger counter]], to determine where the provided atoms were incorporated. For example, one might culture plants in an environment in which the [[carbon dioxide]] contained radioactive carbon; then the parts of the plant that incorporate atmospheric carbon would be radioactive. Radionuclides can be used to monitor processes such as [[DNA replication]] or [[amino acid]] transport. |
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* in [[physics]] and [[biology]] radionuclide X-ray fluorescence spectrometry is used to determine [[chemical composition]] of the [[Chemical compound|compound]]. [[X-ray|Radiation]] from a radionuclide source hits the sample and excites characteristic X-rays in the sample. This radiation is registered and the chemical composition of the sample can be determined from the analysis of the measured spectrum. By measuring the energy of the characteristic radiation lines, it is possible to determine the [[Atomic number|proton number]] of the [[chemical element]] that emits the radiation, and by measuring the number of emitted [[photon]]s, it is possible to determine the [[concentration]] of individual chemical elements. |
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* In [[nuclear medicine]], radioisotopes are used for diagnosis, treatment, and research. Radioactive chemical tracers emitting gamma rays or positrons can provide diagnostic information about internal anatomy and the functioning of specific organs, including the [[human brain]].<ref>{{cite journal|last1=Ingvar|first1=David H.|author-link1=:sv:David H. Ingvar|last2=Lassen|first2=Niels A.|author-link2=Niels A. Lassen|title=Quantitative determination of regional cerebral blood-flow in man|journal=[[The Lancet]]|year=1961|volume=278|issue=7206|pages=806–807|url=http://www.thelancet.com/journals/lancet/article/PIIS0140-6736%2861%2991092-3/fulltext|doi=10.1016/s0140-6736(61)91092-3}}</ref><ref>{{cite journal|last1=Ingvar|first1=David H.|author1-link=:sv:David H. Ingvar|last2=Franzén|first2=Göran|title=Distribution of cerebral activity in chronic schizophrenia|journal=[[The Lancet]]|year=1974|volume=304|issue=7895|pages=1484–1486|url=http://www.thelancet.com/journals/lancet/article/PIIS0140-6736%2874%2990221-9/abstract|doi=10.1016/s0140-6736(74)90221-9|pmid=4140398}}</ref><ref>{{cite journal|last1=Lassen|first1=Niels A.|author-link1=Niels A. Lassen|last2=Ingvar|first2=David H.|author-link2=:sv:David H. Ingvar|last3=Skinhøj|first3=Erik|author-link3=:da:Erik Skinhøj|title=Brain Function and Blood Flow| journal=[[Scientific American]]|volume=239|issue=4|pages=62–71|date=October 1978|doi=10.1038/scientificamerican1078-62|pmid=705327|bibcode=1978SciAm.239d..62L}}</ref> This is used in some forms of tomography: [[single-photon emission computed tomography]] and [[positron emission tomography]] (PET) scanning and [[Cherenkov luminescence imaging]]. Radioisotopes are also a method of treatment in [[hemopoietic]] forms of tumors; the success for treatment of solid tumors has been limited. More powerful gamma sources [[sterilization (microbiology)|sterilise]] syringes and other medical equipment. |
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* In [[food preservation]], radiation is used to stop the sprouting of root crops after harvesting, to kill parasites and pests, and to control the ripening of stored fruit and vegetables. [[Food irradiation]] usually uses beta-decaying nuclides with strong gamma emissions like [[cobalt-60]] or [[caesium-137]]. |
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* In [[Industrial sector|industry]], and in [[mining]], radionuclides are used to examine welds, to detect leaks, to study the rate of wear, erosion and corrosion of metals, and for on-stream analysis of a wide range of minerals and fuels. |
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* In [[spacecraft]], radionuclides are used to provide power and heat, notably through [[radioisotope thermoelectric generator]]s (RTGs) and [[radioisotope heater unit]]s (RHUs). |
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* In [[astronomy]] and [[physical cosmology|cosmology]], radionuclides play a role in understanding stellar and planetary process. |
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* In [[particle physics]], radionuclides help discover new physics ([[physics beyond the Standard Model]]) by measuring the energy and momentum of their beta decay products (for example, [[neutrinoless double beta decay]] and the search for [[weakly interacting massive particles]]).<ref>{{cite journal|doi=10.1103/RevModPhys.78.991|title=Tests of the standard electroweak model in nuclear beta decay|journal=Reviews of Modern Physics|volume=78|issue=3|pages=991–1040|year=2006|last1=Severijns|first1=Nathal|last2=Beck|first2=Marcus|last3=Naviliat-Cuncic|first3=Oscar|bibcode=2006RvMP...78..991S|arxiv = nucl-ex/0605029 |s2cid=18494258}}</ref> |
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* In [[ecology]], radionuclides are used to trace and analyze pollutants, to study the movement of surface water, and to measure water runoffs from rain and snow, as well as the flow rates of streams and rivers. |
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* In [[geology]], [[archaeology]], and [[paleontology]], natural radionuclides are used to measure ages of rocks, minerals, and fossil materials.<!-- When radioactive carbon, for example, is in the atmosphere, it rapidly becomes separated from its decay products. Once it is bound up in a solid, such as wood or paper, its decay products must remain in place. Therefore, by measuring how much of these decay products have accumulated, one can estimate the time when the carbon was captured into solid form. --> |
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==Examples== |
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Radionuclides are used in two major ways: for their chemical properties and as sources of [[radiation]]. |
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The following table lists properties of selected radionuclides illustrating the range of properties and uses. |
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Radionuclides of familiar elements such as [[carbon]] can serve as [[radioactive tracer]]s because they are chemically very similar to the nonradioactive nuclides, so most chemical, biological, and ecological processes treat them in a nearly identical way. One can then examine the result with a radiation detector, such as a [[Geiger counter]], to determine where the provided atoms ended up. For example, one might culture plants in an environment in which the [[carbon dioxide]] contained radioactive carbon; then the parts of the plant that had laid down atmospheric carbon would be radioactive. |
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{| class="wikitable sortable" |
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! Isotope !! ''Z'' !! ''N'' !! half-life !! DM !! DE<br /> [[keV]] !! Mode of formation !! Comments |
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In [[nuclear medicine]], radioisotopes are used for diagnosis, treatment, and research. Radioactive chemical tracers emitting gamma rays or positrons can provide diagnostic information about a person's internal anatomy and the functioning of specific organs. This is used in some forms of tomography: [[single-photon emission computed tomography]] and [[positron emission tomography]] scanning and [[Cerenkov luminescence imaging]]. |
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! [[Tritium]] (<sup>3</sup>H) |
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| 1 || 2 || 12.3 y || [[beta decay| |
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Radioisotopes are also a method of treatment in [[hemopoietic]] forms of tumors; the success for treatment of solid tumors has been limited. More powerful gamma sources [[Sterilisation (microbiology)|sterilise]] syringes and other medical equipment. |
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|- |
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! [[Beryllium-10]] |
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In [[biochemistry]] and [[genetics]], radionuclides label molecules and allow tracing chemical and physiological processes occurring in living organisms, such as [[DNA replication]] or [[amino acid]] transport. |
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| 4 || 6 || 1,387,000 y || |
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| Cosmogenic || used to examine soil erosion, soil formation from regolith, and the age of ice cores |
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In [[food preservation]], radiation [[food irradiation|is used]] to stop the sprouting of root crops after harvesting, to kill parasites and pests, and to control the ripening of stored fruit and vegetables. |
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|- |
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! [[Carbon-14]] |
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In [[industry]], and in [[mining]], radionuclides examine welds, to detect leaks, to study the rate of wear, erosion and corrosion of metals, and for on-stream analysis of a wide range of minerals and fuels. |
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| 6 || 8 || 5,700 y || |
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| Cosmogenic || used for [[radiocarbon dating]] |
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In [[particle physics]], radionuclides help discover new physics (beyond [[Standard Model]] [BSM] physics) by measuring the energy and momentum of their beta decay products.<ref>{{cite journal|doi=10.1103/RevModPhys.78.991|title=Tests of the standard electroweak model in nuclear beta decay|journal=Reviews of Modern Physics|volume=78|issue=3|pages=991|year=2006|last1=Severijns|first1=Nathal|last2=Beck|first2=Marcus|last3=Naviliat-Cuncic|first3=Oscar|bibcode=2006RvMP...78..991S|arxiv = nucl-ex/0605029 }}</ref> |
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|- |
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! [[Fluorine-18]] |
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Radionuclides are also used to trace and analyze pollutants, to study the movement of surface water, and to measure water runoffs from rain and snow, as well as the flow rates of streams and rivers. Natural radionuclides are used in [[geology]], [[archaeology]], and [[paleontology]] to measure ages of rocks, minerals, and fossil materials.<!-- When radioactive carbon, for example, is in the atmosphere, it rapidly becomes separated from its decay products. Once it is bound up in a solid, such as wood or paper, its decay products must remain in place. Therefore, by measuring how much of these decay products have accumulated, one can estimate the time when the carbon was captured into solid form. --> |
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| 9 || 9 || 110 min || |
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| Cosmogenic || positron source, synthesised for use as a medical [[radiotracer]] in [[positron emission tomography|PET scans]]. |
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dik with cheese |
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|- |
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! [[Aluminium-26]] |
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| 13 || 13|| 717,000 y || |
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===Americium-241=== |
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| Cosmogenic || exposure dating of rocks, sediment |
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! [[Chlorine-36]] |
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| 17 || 19 || 301,000 y || |
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| Cosmogenic || exposure dating of rocks, groundwater tracer |
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|- |
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! [[Potassium-40]] |
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| 19 || 21 || 1.24{{E|9}} y || |
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| Primordial || used for [[potassium-argon dating]], source of atmospheric [[argon]], source of [[radiogenic heat]], largest source of natural radioactivity |
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|- |
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! [[Isotopes of calcium|Calcium-41]] |
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| 20 || 21 || 99,400 y || EC || |
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| Cosmogenic || exposure dating of [[carbonate rocks]] |
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|- |
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! [[Cobalt-60]] |
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| 27 || 33 || 5.3 y || |
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| Synthetic || produces high energy gamma rays, used for radiotherapy, equipment sterilisation, food irradiation |
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|- |
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! [[Krypton-81]] |
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| 36 || 45 || 229,000 y || |
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|- |
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! [[Strontium-90]] |
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| 38 || 52 || 28.8 y || |
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| Fission product || [[medium-lived fission product]]; probably most dangerous component of nuclear fallout |
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|- |
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! [[Technetium-99]] |
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| 43 || 56 || 210,000 y || |
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| Fission product || most common isotope of the lightest unstable element, most significant of [[long-lived fission products]] |
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|- |
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! [[Technetium-99m]] |
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| 43 || 56 || 6 hr || [[gamma ray| |
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| Synthetic || most commonly used medical radioisotope, used as a radioactive tracer |
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|- |
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! [[Iodine-129]] |
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| 53 || 76 || 15,700,000 y || |
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| Cosmogenic || longest lived [[fission product]]; groundwater tracer |
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|- |
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! [[Iodine-131]] |
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| 53 || 78 || 8 d || |
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| Fission product || most significant short-term health hazard from nuclear fission, used in nuclear medicine, industrial tracer |
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|- |
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! [[Xenon-135]] |
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| 54 || 81 || 9.1 h || |
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| Fission product|| strongest known "nuclear poison" (neutron-absorber), with a major effect on nuclear reactor operation. |
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|- |
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! [[Caesium-137]] |
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| 55 || 82 || 30.2 y || |
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| Fission product || other major [[medium-lived fission product]] of concern |
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|- |
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! [[Gadolinium-153]] |
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| 64 || 89 || 240 d || EC || |
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| Synthetic || Calibrating nuclear equipment, bone density screening |
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|- |
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! [[Bismuth-209]] |
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| 83 || 126 || 2.01{{E|19}}y || [[alpha decay| |
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| Primordial || long considered stable, decay only detected in 2003 |
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|- |
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! [[Polonium-210]] |
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| 84 || 126 || 138 d || |
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| Decay product || Highly toxic, used in [[poisoning of Alexander Litvinenko]] |
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|- |
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! [[Radon-222]] |
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| 86 || 136 || 3.8 d || |
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| Decay product || gas, responsible for the majority of public exposure to ionizing radiation, second most frequent cause of lung cancer |
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|- |
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! [[Thorium-232]] |
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| 90 || 142 || 1.4{{E|10}} y || |
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| Primordial || basis of [[thorium fuel cycle]] |
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|- |
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! [[Uranium-235]] |
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| 92 || 143 || 7{{E|8}}y || |
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| Primordial || [[fissile]], main nuclear fuel |
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|- |
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! [[Uranium-238]] |
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| 92 || 146 || 4.5{{E|9}} y || |
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| Primordial || Main Uranium isotope |
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|- |
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! [[Plutonium-238]] |
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| 94 || 144 || 87.7 y || |
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| Synthetic || used in radioisotope thermoelectric generators (RTGs) and radioisotope heater units as an energy source for spacecraft |
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|- |
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! [[Plutonium-239]] |
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| 94 || 145 || 24,110 y || |
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| Synthetic || used for most modern nuclear weapons |
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|- |
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! [[Americium-241]] |
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| 95 || 146 || 432 y || |
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| Synthetic || used in household smoke detectors as an ionising agent |
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|- |
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! [[Californium-252]] |
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| 98 || 154 || 2.64 y || |
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| Synthetic || undergoes spontaneous fission (3% of decays), making it a powerful neutron source, used as a reactor initiator and for detection devices |
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|} |
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Key: ''Z'' = [[atomic number]]; ''N'' = [[neutron number]]; DM = decay mode; DE = decay energy; EC = [[electron capture]] |
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===Household smoke detectors=== |
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[[File:Americium-241.jpg|thumb|Americium-241 container in a smoke detector.]] |
[[File:Americium-241.jpg|thumb|Americium-241 container in a smoke detector.]] |
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[[File:Americium-241 Sample from Smoke Detector.JPG|thumb|Americium-241 capsule as found in smoke detector. The circle of darker metal in the center is americium-241; the surrounding casing is aluminium.]] |
[[File:Americium-241 Sample from Smoke Detector.JPG|thumb|Americium-241 capsule as found in smoke detector. The circle of darker metal in the center is americium-241; the surrounding casing is aluminium.]] |
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Radionuclides are present in many homes as they are used inside the most common household [[smoke detector]]s. The radionuclide used is [[americium-241]], which is created by bombarding plutonium with neutrons in a nuclear reactor. It decays by emitting [[alpha particle]]s and [[gamma radiation]] to become [[neptunium-237]]. Smoke detectors use a very small quantity of <sup>241</sup>Am (about 0.29 micrograms per smoke detector) in the form of [[americium dioxide]]. <sup>241</sup>Am 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.<ref>{{cite web|url=http://www.world-nuclear.org/info/inf57.html|title=Smoke Detectors and Americium|work=world-nuclear.org|url-status=dead|archive-url=https://web.archive.org/web/20101112082137/http://www.world-nuclear.org/info/inf57.html|archive-date=2010-11-12}}</ref><ref>[http://www.doh.wa.gov/ehp/rp/factsheets/factsheets-htm/fs23am241.htm Office of Radiation Protection – Am 241 Fact Sheet – Washington State Department of Health] {{webarchive|url=https://web.archive.org/web/20110318173013/http://www.doh.wa.gov/ehp/rp/factsheets/factsheets-htm/fs23am241.htm |date=2011-03-18 }}</ref> |
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Most household [[smoke detector]]s contain americium produced in [[nuclear reactor]]s. The radioisotope used is [[americium-241]]. |
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The element americium is created by bombarding plutonium with neutrons in a nuclear reactor. Its isotope, Am-241 decays by emitting [[alpha particle]]s and [[gamma radiation]] to become [[neptunium-237]]. |
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Most common household smoke detectors use a very small quantity of Am-241 (about 0.29 micrograms per smoke detector) in the form of [[americium dioxide]]. Smoke detectors use Am-241 since the alpha particles it emits collide with oxygen and nitrogen particles in the air. This occurs in the detector's [[ionization chamber]] where it produces charged particles or [[ion]]s. Then, these charged particles are collected by a small electric voltage that will create an electric current that will pass between two electrodes. Then, the ions that are flowing between the electrodes will be neutralized when coming in contact with smoke, thereby decreasing the electric current between the electrodes, which will activate the detector's alarm.<ref>[http://www.world-nuclear.org/info/inf57.html Smoke Detectors and Americium]</ref><ref>[http://www.doh.wa.gov/ehp/rp/factsheets/factsheets-htm/fs23am241.htm Office of Radiation Protection – Am 241 Fact Sheet – Washington State Department of Health]</ref> |
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====Steps for creating americium-241==== |
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The [[plutonium-241]] is formed in any nuclear reactor by neutron capture from [[uranium-238]]. |
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# {{SimpleNuclide2|link=yes|Uranium|238}} [[Neutron capture|+ {{SubatomicParticle|Neutron}}]] → {{SimpleNuclide2|link=yes|Uranium|239}} |
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# {{SimpleNuclide2|link=yes|Uranium|239}} → {{SimpleNuclide2|link=yes|Neptunium|239}} [[Beta decay#.CE.B2.E2.88.92 decay|+ {{SubatomicParticle|Electron}} + {{SubatomicParticle|Electron Antineutrino}}]] |
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# {{SimpleNuclide2|link=yes|Neptunium|239}} → {{SimpleNuclide2|link=yes|Plutonium|239}} [[Beta decay#.CE.B2.E2.88.92 decay|+ {{SubatomicParticle|Electron}} + {{SubatomicParticle|Electron Antineutrino}}]] |
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# {{SimpleNuclide2|link=yes|Plutonium|239}} [[Neutron capture|+ {{SubatomicParticle|Neutron}}]] → {{SimpleNuclide2|link=yes|Plutonium|240}} |
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# {{SimpleNuclide2|link=yes|Plutonium|240}} [[Neutron capture|+ {{SubatomicParticle|Neutron}}]] → {{SimpleNuclide2|link=yes|Plutonium|241}} |
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This will decay both in the reactor and subsequently to form Am-241, which has a half-life of 432.2 years.<ref>{{cite web|title=Smoke Detectors: Uses of Radioactive Isotopes|url=http://www.ausetute.com.au/smokedet.html|work=Chemistry Tutorial : Radioisotopes in Smoke Detectors|publisher=AUS-e-TUTE n.d.|accessdate=March 30, 2011}}</ref><ref>[http://www.youtube.com/v/9TEPjZpMzlA&hl=en_US&feature=player_embedded&version=3 Reaction in a Smoke Detector]</ref> |
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===Gadolinium-153=== |
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The [[Gadolinium-153|Gd-153]] isotope is used in X-ray fluorescence and [[osteoporosis]] screening. It is a gamma-emitter with an 8-month half-life, making it easier to use for medical purposes. In [[nuclear medicine]], it serves to calibrate the equipment needed like [[single-photon emission computed tomography]] systems (SPECT) to make [[x-ray]]s. It ensures that the machines work correctly to produce images of radioisotope distribution inside the patient. This isotope is produced in a nuclear reactor from [[europium]] or [[Isotope separation|enriched]] gadolinium.<ref>[http://radioisotopes.pnl.gov/gadolinium.stm PNNL: Isotope Sciences Program – Gadolinium-153]</ref> It can also detect the loss of [[calcium]] in the hip and back bones, allowing the ability to diagnose osteoporosis.<ref>{{cite web|title=Gadolinium|url=http://nobel.scas.bcit.ca/resource/ptable/gd.htm|work=BCIT Chemistry Resource Center|publisher=British Columbia Institute of Technology|accessdate=30 March 2011}}</ref> |
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<!-- [[File:gadolinium153.jpg|thumb|SPECT apparatus examination]] |
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This is an example of an image from a SPECT apparatus of the brain of an epileptic man. The middle and right columns show how the SPECT captures the functional aspects of the brain whereas the left column shows how an MRI test only captures the anatomical view of the brain. |
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--> |
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==Impacts on organisms== |
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==Dangers== |
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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 burn]]s 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."<ref name="Fact sheet N°371">{{cite web|url=https://www.who.int/mediacentre/factsheets/fs371/en/ |publisher=World Health Organization |title=Ionizing radiation, health effects and protective measures| date=November 2012 |access-date=January 27, 2014}}</ref> |
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==Summary table for classes of nuclides, stable and radioactive== |
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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 burn]]s 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."<ref name="Fact sheet N°371">{{cite web|url=http://www.who.int/mediacentre/factsheets/fs371/en/ |publisher=World Health Organization | title=Ionizing radiation, health effects and protective measures| date=November 2012 |accessdate=January 27, 2014}}</ref> |
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Following is a summary table for the [[list of nuclides|list of 989 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. |
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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 30 nuclides with measured half-lives longer than the estimated age of the universe (13.8 billion years<ref>{{cite web |title = Cosmic Detectives |url=http://www.esa.int/Our_Activities/Space_Science/Cosmic_detectives |
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==Summary table for classes of nuclides, "stable" and radioactive== |
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|publisher = The European Space Agency (ESA) |date = 2013-04-02 |access-date = 2013-04-15}}</ref>), and another four nuclides with half-lives long enough (> 100 million years) that they are radioactive [[primordial nuclide]]s, 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]]. |
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Following is a summary table for the total [[list of nuclides]] with half-lives greater than one hour. Ninety of these 905 nuclides are theoretically stable, except to proton-decay (which has never been observed). About 254 nuclides have never been observed to decay, and are classically considered stable. |
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The remaining 650 radionuclides have half-lives longer than 1 hour, and are well-characterized (see [[list of nuclides]] for a complete tabulation). They include 28 nuclides with measured half-lives longer than the estimated age of the universe (13.8 billion years<ref>{{cite web |title = Cosmic Detectives |url=http://www.esa.int/Our_Activities/Space_Science/Cosmic_detectives |
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|publisher = The European Space Agency (ESA) |date = 2013-04-02 |accessdate = 2013-04-15}}</ref>), and another 6 nuclides with half-lives long enough (> 80 million years) that they are radioactive [[primordial nuclide]]s, 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 ~51 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]]. |
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Numbers are not exact, and may change slightly in the future, as "stable nuclides" are observed to be radioactive with very long half-lives. |
Numbers are not exact, and may change slightly in the future, as "stable nuclides" are observed to be radioactive with very long half-lives. |
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This is a summary table |
This is a summary table<ref>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]]</ref> for the 989 nuclides with half-lives longer than one hour (including those that are stable), given in [[list of nuclides]]. |
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{| class="wikitable sortable" width="100%" |
{| class="wikitable sortable" width="100%" |
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! width="300" |Stability class |
! width="300" |Stability class |
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Line 95: | Line 191: | ||
| Includes first 40 elements. Proton decay yet to be observed. |
| Includes first 40 elements. Proton decay yet to be observed. |
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|- |
|- |
||
| |
| 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]] |
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| align="center"| |
| align="center"| 56 |
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| align="center"| |
| align="center"| 146 |
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| All nuclides that are ''possibly'' completely stable (spontaneous fission has never been observed for nuclides with mass number < 232). |
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|- |
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| Energetically unstable to one or more known decay modes, but no decay yet seen. All considered "stable" until decay detected. |
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| align="center"| 105 |
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| align="center"| 251 |
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| Total of classically [[stable nuclide]]s. |
| Total of classically [[stable nuclide]]s. |
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|- |
|- |
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| Radioactive [[primordial nuclide]]s. |
| Radioactive [[primordial nuclide]]s. |
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| align="center"| |
| align="center"| 35 |
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| align="center"| |
| align="center"| 286 |
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| Total primordial elements include [[uranium]], [[thorium]], [[bismuth]], [[rubidium-87]], [[potassium-40]] plus all stable nuclides. |
| Total primordial elements include [[uranium]], [[thorium]], [[bismuth]], [[rubidium-87]], [[potassium-40]], [[tellurium-128]] plus all stable nuclides. |
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|- |
|- |
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| Radioactive nonprimordial, but naturally occurring on Earth. |
| Radioactive nonprimordial, but naturally occurring on Earth. |
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| align="center"| |
| align="center"| 61 |
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| align="center"| |
| align="center"| 347 |
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| [[Carbon-14]] (and other isotopes generated by [[cosmic rays]]) and daughters of radioactive primordial elements, such as [[radium]], [[polonium]], etc. |
| [[Carbon-14]] (and other isotopes generated by [[cosmic rays]]) and daughters of radioactive primordial elements, such as [[radium]], [[polonium]], etc. 41 of these have a half life of greater than one hour. |
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|- |
|- |
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| Radioactive synthetic |
| Radioactive synthetic half-life ≥ 1.0 hour). Includes most useful [[radiotracer]]s. |
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| align="center"| |
| align="center"| 662 |
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| align="center"| |
| align="center"| 989 |
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| These |
| These 989 nuclides are listed in the article [[List of nuclides]]. |
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|- |
|- |
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| Radioactive synthetic (half-life < 1.0 hour). |
| Radioactive synthetic (half-life < 1.0 hour). |
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Line 123: | Line 224: | ||
==List of commercially available radionuclides== |
==List of commercially available radionuclides== |
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{{See also|List of nuclides|Table of nuclides}} |
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This list covers common isotopes, most of which are available in very small quantities to the general public in most countries. Others that are not publicly accessible are traded commercially in industrial, medical, and scientific fields and are subject to government regulation. For a complete list of all known isotopes for every element (minus activity data), see [[list of nuclides]], and [[Isotope lists|Isotope Lists]]. For a table see [[Table of nuclides (segmented, wide)|Table of Nuclides]]. |
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This list covers common isotopes, most of which are available in very small quantities to the general public in most countries. Others that are not publicly accessible are traded commercially in industrial, medical, and scientific fields and are subject to government regulation. |
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===Gamma emission only=== |
===Gamma emission only=== |
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{| class="wikitable" Border="1" |
{| class="wikitable" Border="1" |
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|- |
|- |
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Line 175: | Line 276: | ||
|- |
|- |
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| [[Technetium-99m]] |
| [[Technetium-99m]] |
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| {{val|1.95|e= |
| {{val|1.95|e=7}} TBq/kg (5.27 × 10<sup>5</sup> Ci/g) |
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| 6 hours |
| 6 hours |
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| 140 |
| 140 |
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Line 181: | Line 282: | ||
===Beta emission only=== |
===Beta emission only=== |
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{| class="wikitable" Border="1" |
{| class="wikitable" Border="1" |
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|- |
|- |
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Line 211: | Line 311: | ||
===Alpha emission only=== |
===Alpha emission only=== |
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{| class="wikitable" Border="1" |
{| class="wikitable" Border="1" |
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|- |
|- |
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Line 221: | Line 320: | ||
| [[Polonium-210]] |
| [[Polonium-210]] |
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| 166500 TBq/kg (4500 Ci/g) |
| 166500 TBq/kg (4500 Ci/g) |
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| 138 days |
| 138.376 days |
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| 5304.5 |
| 5304.5 |
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|- |
|- |
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| [[Uranium-238]] |
| [[Uranium-238]] |
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| 12580 |
| 12580 kBq/kg (0.00000034 Ci/g) |
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| 4.468 billion years |
| 4.468 billion years |
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| 4267 |
| 4267 |
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Line 231: | Line 330: | ||
===Multiple radiation emitters=== |
===Multiple radiation emitters=== |
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{| class="wikitable" Border="1" |
{| class="wikitable" Border="1" |
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|- |
|- |
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Line 254: | Line 352: | ||
==See also== |
==See also== |
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* [[List of nuclides]] shows all radionuclides with half-life > 1 hour |
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* [[Hyperaccumulators table – 3]] |
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*[[List of nuclides]] shows all radionuclides with half-life > 1 hour |
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* [[Radioactivity in biology]] |
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*[[Hyperaccumulators table – 3]] |
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* [[Radiometric dating]] |
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*[[Radioactivity in biology]] |
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* [[Radionuclide cisternogram]] |
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*[[Radiometric dating]] |
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* [[Uses of radioactivity in oil and gas wells]] |
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*[[Radionuclide cisternogram]] |
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*[[Radionuclides associated with hydraulic fracturing]] |
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==Notes== |
==Notes== |
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Line 266: | Line 363: | ||
==References== |
==References== |
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*{{cite journal | |
* {{cite journal |last1=Carlsson |first1=J. |title=Tumour therapy with radionuclides: assessment of progress and problems |journal=Radiotherapy and Oncology |volume=66 |issue=2 |year=2003 |pages=107–117 |pmid=12648782 |doi=10.1016/S0167-8140(02)00374-2 |first2=E | last2=Forssell Aronsson |last3=Hietala |first3=SO |last4=Stigbrand |first4=T |last5=Tennvall |first5=J |display-authors=etal}} |
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*{{cite web |url=http://world-nuclear.org/info/inf56.html |title=Radioisotopes in Industry |work=World Nuclear Association }} |
* {{cite web |url=http://world-nuclear.org/info/inf56.html |title=Radioisotopes in Industry |work=World Nuclear Association |access-date=2008-05-02 |archive-date=2013-02-27 |archive-url=https://web.archive.org/web/20130227084034/http://world-nuclear.org/info/inf56.html |url-status=dead }} |
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*{{cite book |last=Martin | |
* {{cite book |last=Martin |first=James |title=Physics for Radiation Protection: A Handbook |year=2006 |pages=130|publisher=John Wiley & Sons |isbn=978-3527406111 }} |
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==Further reading== |
==Further reading== |
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* {{Cite book | doi = 10.1002/14356007.a22_499.pub2| chapter = Radionuclides, 1. Introduction| title = Ullmann's Encyclopedia of Industrial Chemistry| year = 2011| last1 = Luig | first1 = H. | last2 = Kellerer | first2 = A. M. | last3 = Griebel | first3 = J. R. | isbn = 978-3527306732}} |
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*{{cite doi|10.1002/14356007.a22_499.pub2}} |
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==External links== |
==External links== |
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{{commons category|Radionuclides}} |
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* [http://www.epa.gov/rpdweb00/radionuclides/index.html EPA – Radionuclides] – EPA's Radiation Protection Program: Information. |
* [http://www.epa.gov/rpdweb00/radionuclides/index.html EPA – Radionuclides] – EPA's Radiation Protection Program: Information. |
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* [ |
* [https://www.fda.gov/Food/FoodSafety/FoodContaminantsAdulteration/ChemicalContaminants/Radionuclides/UCM078341#level98 FDA – Radionuclides] – FDA's Radiation Protection Program: Information. |
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* [http://www.nndc.bnl.gov/chart/ Interactive Chart of Nuclides] – A chart of all nuclides |
* [http://www.nndc.bnl.gov/chart/ Interactive Chart of Nuclides] – A chart of all nuclides |
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* [http://isotopes.gov/ National Isotope Development Center] – U.S. Government source of radionuclides – production, research, development, distribution, and information |
* [http://isotopes.gov/ National Isotope Development Center] – U.S. Government source of radionuclides – production, research, development, distribution, and information |
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* [http://www-nds.iaea.org/livechart The Live Chart of Nuclides – IAEA ] |
* [http://www-nds.iaea.org/livechart The Live Chart of Nuclides – IAEA ] |
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* [http://www-nds.iaea.org/mib Radionuclides production simulator – IAEA ] |
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{{Radiation}} |
{{Radiation}} |
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{{Radiopharmaceuticals}} |
{{Radiopharmaceuticals}} |
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{{Authority control}} |
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[[Category:Radioactivity]] |
[[Category:Radioactivity]] |
Latest revision as of 16:02, 17 September 2024
A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that has excess numbers of either neutrons or protons, giving it excess nuclear energy, and making it unstable. This excess energy can be used in one of three ways: emitted from the nucleus as gamma radiation; transferred to one of its electrons to release it as a conversion electron; or used to create and emit a new particle (alpha particle or beta particle) from the nucleus. During those processes, the radionuclide is said to undergo radioactive decay.[1] These emissions are considered ionizing radiation because they are energetic enough to liberate an electron from another atom. The radioactive decay can produce a stable nuclide or will sometimes produce a new unstable radionuclide which may undergo further decay. Radioactive decay is a random process at the level of single atoms: it is impossible to predict when one particular atom will decay.[2][3][4][5] However, for a collection of atoms of a single nuclide the decay rate, and thus the half-life (t1/2) for that collection, can be calculated from their measured decay constants. 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 or are artificially produced in nuclear reactors, cyclotrons, particle accelerators or radionuclide generators. There are about 730 radionuclides with half-lives longer than 60 minutes (see list of nuclides). Thirty-two of those are primordial radionuclides that were created before the Earth was formed. At least another 60 radionuclides 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 about 251 stable nuclides.
All chemical elements can exist as radionuclides. Even the lightest element, hydrogen, has a well-known radionuclide, tritium. Elements heavier than lead, and the elements technetium and promethium, exist only as radionuclides.
Unplanned exposure to radionuclides generally has a harmful effect on living organisms including humans, although low levels of exposure occur naturally without harm. 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 the most usual consequence. 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
[edit]Natural
[edit]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 can still be observed astronomically and can play a part in understanding astronomic processes. Primordial radionuclides, such as uranium and thorium, exist in the present time because their half-lives are so long (>100 million years) that they have 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 decay may be observed in other nuclides, adding to this list of primordial radionuclides.
- 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. Examples include the natural isotopes of polonium and radium.
- Cosmogenic isotopes, such as carbon-14, are present because they are continually being formed in the atmosphere due to cosmic rays.[6]
Many of these radionuclides exist only in trace amounts in nature, including all cosmogenic nuclides. Secondary radionuclides 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 about 0.1 mg per metric ton (1 part in 1010).[7][8] Further radionuclides may occur in nature in virtually undetectable amounts as a result of rare events such as spontaneous fission or uncommon cosmic ray interactions.
Nuclear fission
[edit]Radionuclides are produced as an unavoidable result of nuclear fission and thermonuclear explosions. The process of nuclear fission creates a wide range of fission products, most of which are radionuclides. Further radionuclides can be 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
[edit]Synthetic radionuclides are deliberately synthesised using nuclear reactors, particle accelerators or radionuclide generators:[9]
- 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. The elements that have a large propensity to take up the neutrons in the reactor are said to have a high neutron cross-section.
- Particle accelerators such as cyclotrons accelerate particles to bombard a target to produce radionuclides. Cyclotrons accelerate protons at a target to produce positron-emitting radionuclides, e.g. fluorine-18.
- Radionuclide generators contain a parent radionuclide that decays to produce a radioactive daughter. The parent is usually produced in a nuclear reactor. A typical example is the technetium-99m generator used in nuclear medicine. The parent produced in the reactor is molybdenum-99.
Uses
[edit]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).
- In biology, radionuclides of carbon can serve as radioactive tracers because they are chemically very similar to the nonradioactive nuclides, so most chemical, biological, and ecological processes treat them in a nearly identical way. One can then examine the result with a radiation detector, such as a Geiger counter, to determine where the provided atoms were incorporated. For example, one might culture plants in an environment in which the carbon dioxide contained radioactive carbon; then the parts of the plant that incorporate atmospheric carbon would be radioactive. Radionuclides can be used to monitor processes such as DNA replication or amino acid transport.
- in physics and biology radionuclide X-ray fluorescence spectrometry is used to determine chemical composition of the compound. Radiation from a radionuclide source hits the sample and excites characteristic X-rays in the sample. This radiation is registered and the chemical composition of the sample can be determined from the analysis of the measured spectrum. By measuring the energy of the characteristic radiation lines, it is possible to determine the proton number of the chemical element that emits the radiation, and by measuring the number of emitted photons, it is possible to determine the concentration of individual chemical elements.
- In nuclear medicine, radioisotopes are used for diagnosis, treatment, and research. Radioactive chemical tracers emitting gamma rays or positrons can provide diagnostic information about internal anatomy and the functioning of specific organs, including the human brain.[10][11][12] This is used in some forms of tomography: single-photon emission computed tomography and positron emission tomography (PET) scanning and Cherenkov luminescence imaging. Radioisotopes are also a method of treatment in hemopoietic forms of tumors; the success for treatment of solid tumors has been limited. More powerful gamma sources sterilise syringes and other medical equipment.
- In food preservation, radiation is used to stop the sprouting of root crops after harvesting, to kill parasites and pests, and to control the ripening of stored fruit and vegetables. Food irradiation usually uses beta-decaying nuclides with strong gamma emissions like cobalt-60 or caesium-137.
- In industry, and in mining, radionuclides are used to examine welds, to detect leaks, to study the rate of wear, erosion and corrosion of metals, and for on-stream analysis of a wide range of minerals and fuels.
- In spacecraft, radionuclides are used to provide power and heat, notably through radioisotope thermoelectric generators (RTGs) and radioisotope heater units (RHUs).
- In astronomy and cosmology, radionuclides play a role in understanding stellar and planetary process.
- In particle physics, radionuclides help discover new physics (physics beyond the Standard Model) by measuring the energy and momentum of their beta decay products (for example, neutrinoless double beta decay and the search for weakly interacting massive particles).[13]
- In ecology, radionuclides are used to trace and analyze pollutants, to study the movement of surface water, and to measure water runoffs from rain and snow, as well as the flow rates of streams and rivers.
- In geology, archaeology, and paleontology, natural radionuclides are used to measure ages of rocks, minerals, and fossil materials.
Examples
[edit]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 | 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 | 556 | Cosmogenic | used to examine soil erosion, soil formation from regolith, and the age of ice cores | |
Carbon-14 | 6 | 8 | 5,700 y | 156 | Cosmogenic | used for radiocarbon dating | |
Fluorine-18 | 9 | 9 | 110 min | 633/1655 | Cosmogenic | positron source, synthesised for use as a medical radiotracer in PET scans. | |
Aluminium-26 | 13 | 13 | 717,000 y | 4004 | Cosmogenic | exposure dating of rocks, sediment | |
Chlorine-36 | 17 | 19 | 301,000 y | 709 | Cosmogenic | exposure dating of rocks, groundwater tracer | |
Potassium-40 | 19 | 21 | 1.24×109 y | 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 | 2824 | Synthetic | produces high energy gamma rays, used for radiotherapy, equipment sterilisation, food irradiation | |
Krypton-81 | 36 | 45 | 229,000 y | Cosmogenic | groundwater dating | ||
Strontium-90 | 38 | 52 | 28.8 y | 546 | Fission product | medium-lived fission product; probably most dangerous component of nuclear fallout | |
Technetium-99 | 43 | 56 | 210,000 y | 294 | Fission product | most common isotope of the lightest unstable element, most significant of long-lived fission products | |
Technetium-99m | 43 | 56 | 6 hr | 141 | Synthetic | most commonly used medical radioisotope, used as a radioactive tracer | |
Iodine-129 | 53 | 76 | 15,700,000 y | 194 | Cosmogenic | longest lived fission product; groundwater tracer | |
Iodine-131 | 53 | 78 | 8 d | 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 | 1160 | Fission product | strongest known "nuclear poison" (neutron-absorber), with a major effect on nuclear reactor operation. | |
Caesium-137 | 55 | 82 | 30.2 y | 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 | 3137 | Primordial | long considered stable, decay only detected in 2003 | |
Polonium-210 | 84 | 126 | 138 d | 5307 | Decay product | Highly toxic, used in poisoning of Alexander Litvinenko | |
Radon-222 | 86 | 136 | 3.8 d | 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 | 4083 | Primordial | basis of thorium fuel cycle | |
Uranium-235 | 92 | 143 | 7×108y | 4679 | Primordial | fissile, main nuclear fuel | |
Uranium-238 | 92 | 146 | 4.5×109 y | 4267 | Primordial | Main Uranium isotope | |
Plutonium-238 | 94 | 144 | 87.7 y | 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 | 5245 | Synthetic | used for most modern nuclear weapons | |
Americium-241 | 95 | 146 | 432 y | 5486 | Synthetic | used in household smoke detectors as an ionising agent | |
Californium-252 | 98 | 154 | 2.64 y | 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
[edit]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.[14][15]
Impacts on organisms
[edit]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."[16]
Summary table for classes of nuclides, stable and radioactive
[edit]Following is a summary table for the list of 989 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.
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 30 nuclides with measured half-lives longer than the estimated age of the universe (13.8 billion years[17]), 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.
Numbers are not exact, and may change slightly in the future, as "stable nuclides" are observed to be radioactive with very long half-lives.
This is a summary table[18] for the 989 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. | 61 | 347 | Carbon-14 (and other isotopes generated by cosmic rays) and daughters of radioactive primordial elements, such as radium, polonium, etc. 41 of these have a half life of greater than one hour. |
Radioactive synthetic half-life ≥ 1.0 hour). Includes most useful radiotracers. | 662 | 989 | These 989 nuclides are listed in the article List of nuclides. |
Radioactive synthetic (half-life < 1.0 hour). | >2400 | >3300 | Includes all well-characterized synthetic nuclides. |
List of commercially available radionuclides
[edit]This list covers common isotopes, most of which are available in very small quantities to the general public in most countries. Others that are not publicly accessible are traded commercially in industrial, medical, and scientific fields and are subject to government regulation.
Gamma emission only
[edit]Isotope | Activity | Half-life | Energies (keV) |
---|---|---|---|
Barium-133 | 9694 TBq/kg (262 Ci/g) | 10.7 years | 81.0, 356.0 |
Cadmium-109 | 96200 TBq/kg (2600 Ci/g) | 453 days | 88.0 |
Cobalt-57 | 312280 TBq/kg (8440 Ci/g) | 270 days | 122.1 |
Cobalt-60 | 40700 TBq/kg (1100 Ci/g) | 5.27 years | 1173.2, 1332.5 |
Europium-152 | 6660 TBq/kg (180 Ci/g) | 13.5 years | 121.8, 344.3, 1408.0 |
Manganese-54 | 287120 TBq/kg (7760 Ci/g) | 312 days | 834.8 |
Sodium-22 | 237540 Tbq/kg (6240 Ci/g) | 2.6 years | 511.0, 1274.5 |
Zinc-65 | 304510 TBq/kg (8230 Ci/g) | 244 days | 511.0, 1115.5 |
Technetium-99m | 1.95×107 TBq/kg (5.27 × 105 Ci/g) | 6 hours | 140 |
Beta emission only
[edit]Isotope | Activity | Half-life | Energies (keV) |
---|---|---|---|
Strontium-90 | 5180 TBq/kg (140 Ci/g) | 28.5 years | 546.0 |
Thallium-204 | 17057 TBq/kg (461 Ci/g) | 3.78 years | 763.4 |
Carbon-14 | 166.5 TBq/kg (4.5 Ci/g) | 5730 years | 49.5 (average) |
Tritium (Hydrogen-3) | 357050 TBq/kg (9650 Ci/g) | 12.32 years | 5.7 (average) |
Alpha emission only
[edit]Isotope | Activity | Half-life | Energies (keV) |
---|---|---|---|
Polonium-210 | 166500 TBq/kg (4500 Ci/g) | 138.376 days | 5304.5 |
Uranium-238 | 12580 kBq/kg (0.00000034 Ci/g) | 4.468 billion years | 4267 |
Multiple radiation emitters
[edit]Isotope | Activity | Half-life | Radiation types | Energies (keV) |
---|---|---|---|---|
Caesium-137 | 3256 TBq/kg (88 Ci/g) | 30.1 years | Gamma & beta | G: 32, 661.6 B: 511.6, 1173.2 |
Americium-241 | 129.5 TBq/kg (3.5 Ci/g) | 432.2 years | Gamma & alpha | G: 59.5, 26.3, 13.9 A: 5485, 5443 |
See also
[edit]- List of nuclides shows all radionuclides with half-life > 1 hour
- Hyperaccumulators table – 3
- Radioactivity in biology
- Radiometric dating
- Radionuclide cisternogram
- Uses of radioactivity in oil and gas wells
Notes
[edit]- ^ Petrucci, R. H.; Harwood, W. S.; Herring, F. G. (2002). General Chemistry (8th ed.). Prentice-Hall. pp. 1025–26. ISBN 0-13-014329-4.
- ^ "Decay and Half Life". Retrieved 2009-12-14.
- ^ Stabin, Michael G. (2007). "3". In Stabin, Michael G (ed.). Radiation Protection and Dosimetry: An Introduction to Health Physics (Submitted manuscript). Springer. doi:10.1007/978-0-387-49983-3. ISBN 978-0387499826.
- ^ Best, Lara; Rodrigues, George; Velker, Vikram (2013). "1.3". Radiation Oncology Primer and Review. Demos Medical Publishing. ISBN 978-1620700044.
- ^ 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.
- ^ Eisenbud, Merril; Gesell, Thomas F (1997-02-25). Environmental Radioactivity: From Natural, Industrial, and Military Sources. Elsevier. p. 134. ISBN 9780122351549.
- ^ Bagnall, K. W. (1962). "The Chemistry of Polonium". Advances in Inorganic Chemistry and Radiochemistry 4. New York: Academic Press. pp. 197–226. doi:10.1016/S0065-2792(08)60268-X. ISBN 0-12-023604-4. Retrieved June 14, 2012., p. 746
- ^ Bagnall, K. W. (1962). "The Chemistry of Polonium". Advances in Inorganic Chemistry and Radiochemistry 4. New York: Academic Press., p. 198
- ^ "Radioisotopes". www.iaea.org. 2016-07-15. Retrieved 2023-06-25.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ "Smoke Detectors and Americium". world-nuclear.org. Archived from the original on 2010-11-12.
- ^ Office of Radiation Protection – Am 241 Fact Sheet – Washington State Department of Health Archived 2011-03-18 at the Wayback Machine
- ^ "Ionizing radiation, health effects and protective measures". World Health Organization. November 2012. Retrieved January 27, 2014.
- ^ "Cosmic Detectives". The European Space Agency (ESA). 2013-04-02. Retrieved 2013-04-15.
- ^ 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
[edit]- Carlsson, J.; Forssell Aronsson, E; Hietala, SO; Stigbrand, T; Tennvall, J; et al. (2003). "Tumour therapy with radionuclides: assessment of progress and problems". Radiotherapy and Oncology. 66 (2): 107–117. doi:10.1016/S0167-8140(02)00374-2. PMID 12648782.
- "Radioisotopes in Industry". World Nuclear Association. Archived from the original on 2013-02-27. Retrieved 2008-05-02.
- Martin, James (2006). Physics for Radiation Protection: A Handbook. John Wiley & Sons. p. 130. ISBN 978-3527406111.
Further reading
[edit]- Luig, H.; Kellerer, A. M.; Griebel, J. R. (2011). "Radionuclides, 1. Introduction". Ullmann's Encyclopedia of Industrial Chemistry. doi:10.1002/14356007.a22_499.pub2. ISBN 978-3527306732.
External links
[edit]- EPA – Radionuclides – EPA's Radiation Protection Program: Information.
- FDA – Radionuclides – FDA's Radiation Protection Program: Information.
- Interactive Chart of Nuclides – A chart of all nuclides
- National Isotope Development Center – U.S. Government source of radionuclides – production, research, development, distribution, and information
- The Live Chart of Nuclides – IAEA
- Radionuclides production simulator – IAEA