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Although '''[[thorium]]''' ('''Th'''), with atomic number 90, has 6 naturally occurring '''[[isotope]]s''', none of these isotopes are stable; however, one isotope, <sup>232</sup>Th, is ''relatively'' stable, with a half-life of 14.05 billion years, considerably longer than the [[age of the earth]], and even slightly longer than the generally accepted [[age of the universe]]. This isotope makes up nearly all natural thorium. As such, thorium is considered to be [[mononuclidic elements|mononuclidic]]. It has a characteristic terrestrial isotopic composition and thus an atomic mass can be given.
Although '''[[thorium]]''' ('''Th'''), with atomic number 90, has 6 naturally occurring '''[[isotope]]s''', none of these isotopes are stable; however, one isotope, <sup>232</sup>Th, is ''relatively'' stable, with a half-life of 14.05 billion years, considerably longer than the [[age of the earth]], and even slightly longer than the generally accepted [[age of the universe]]. This isotope makes up nearly all natural thorium. As such, thorium is considered to be [[mononuclidic elements|mononuclidic]]. It has a characteristic terrestrial isotopic composition and thus an atomic mass can be given.
:Standard atomic mass: 232.03806(2) [[unified atomic mass unit|u]]
Standard atomic mass: 232.03806(2)&nbsp;[[atomic mass unit|u]].


Thirty [[radioisotope]]s have been characterized, with the most stable (after <sup>232</sup>Th) being <sup>230</sup>Th with a half-life of 75,380 years, <sup>229</sup>Th with a half-life of 7,340 years, and <sup>228</sup>Th with a half-life of 1.92 years. All of the remaining [[radioactive]] isotopes have half-lives that are less than thirty days and the majority of these have half-lives that are less than ten minutes. One isotope, <sup>229</sup>Th, has a [[nuclear isomer]] (or metastable state) with a remarkably low excitation energy,<ref name=Ruchowska>{{cite journal|author=E. Ruchowska|title=Nuclear structure of <sup>229</sup>Th |journal=Phys. Rev. C|volume= 73|pages=044326|year=2006 |doi=10.1103/PhysRevC.73.044326|issue=4 |bibcode = 2006PhRvC..73d4326R |display-authors=etal}}</ref> recently measured to be 7.6 ± 0.5 eV.<ref name=Beck>{{cite journal|author=B. R. Beck|title=Energy splitting in the ground state doublet in the nucleus <sup>229</sup>Th |journal=[[Physical Review Letters]]|volume= 98|pages=142501|date=2007-04-06 |doi=10.1103/PhysRevLett.98.142501 |pmid=17501268 |bibcode=2007PhRvL..98n2501B|issue=14|display-authors=etal}}</ref>
Thirty [[radioisotope]]s have been characterized, with the most stable (after <sup>232</sup>Th) being <sup>230</sup>Th with a half-life of 75,380 years, <sup>229</sup>Th with a half-life of 7,340 years, and <sup>228</sup>Th with a half-life of 1.92 years. All of the remaining [[radioactive]] isotopes have half-lives that are less than thirty days and the majority of these have half-lives that are less than ten minutes. One isotope, <sup>229</sup>Th, has a [[nuclear isomer]] (or metastable state) with a remarkably low excitation energy,<ref name=Ruchowska>{{cite journal|author=E. Ruchowska|title=Nuclear structure of <sup>229</sup>Th |journal=Phys. Rev. C|volume= 73|pages=044326|year=2006 |doi=10.1103/PhysRevC.73.044326|issue=4 |bibcode = 2006PhRvC..73d4326R}}</ref> recently measured to be 7.6 ± 0.5&nbsp;eV.<ref name=Beck>{{cite journal|author=B. R. Beck|title=Energy splitting in the ground state doublet in the nucleus <sup>229</sup>Th |journal=[[Physical Review Letters]]|volume= 98|pages=142501|date=2007-04-06 |doi=10.1103/PhysRevLett.98.142501 |pmid=17501268 |bibcode=2007PhRvL..98n2501B|issue=14|display-authors=etal}}</ref>


The known isotopes of thorium range in [[mass number]] from 209<ref name=Ikezoe>{{cite journal|author=H. Ikezoe|title=alpha decay of a new isotope of <sup>209</sup>Th |year=1996| journal=[[Physical Review C]]| volume=54| issue=4| page=2043|doi=10.1103/PhysRevC.54.2043 |bibcode = 1996PhRvC..54.2043I |display-authors=etal}}</ref> to 238.
The known isotopes of thorium range in [[mass number]] from 209<ref name=Ikezoe>{{cite journal|author=H. Ikezoe|title=alpha decay of a new isotope of <sup>209</sup>Th |year=1996| journal=[[Physical Review C]]| volume=54| issue=4| page=2043|doi=10.1103/PhysRevC.54.2043 |bibcode = 1996PhRvC..54.2043I |display-authors=etal}}</ref> to 238.
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=== Thorium-228 ===
=== Thorium-228 ===
'''<sup>228</sup>Th''' is an [[isotope]] of [[thorium]] which has 138 [[neutrons]]. It was once named Radiothorium, due to its occurrence in the [[disintegration chain]] of thorium-232. It has a [[half-life]] of 1.9116 years. It undergoes [[alpha decay]] to [[isotopes of radium|<sup>224</sup>Ra]]. Occasionally it decays by the unusual route of [[cluster decay]], emitting a nucleus of [[isotopes of oxygen|<sup>20</sup>O]] and producing stable [[isotopes of lead|<sup>208</sup>Pb]]. It is a daughter isotope of [[isotopes of uranium#Uranium-232|<sup>232</sup>U]].
'''<sup>228</sup>Th''' is an [[isotope]] of [[thorium]] with 138 [[neutrons]]. It was once named Radiothorium, due to its occurrence in the [[disintegration chain]] of thorium-232. It has a [[half-life]] of 1.9116 years. It undergoes [[alpha decay]] to [[isotopes of radium|<sup>224</sup>Ra]]. Occasionally it decays by the unusual route of [[cluster decay]], emitting a nucleus of [[isotopes of oxygen|<sup>20</sup>O]] and producing stable [[isotopes of lead|<sup>208</sup>Pb]]. It is a daughter isotope of [[isotopes of uranium#Uranium-232|<sup>232</sup>U]].


Th-228 has an atomic weight of 228.0287411&nbsp;grams/mole. [[Uranium-232]] decays to this nuclide by alpha emission.
Th-228 has an atomic weight of 228.0287411&nbsp;grams/mole. [[Uranium-232]] decays to this nuclide by alpha emission.
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===Thorium-229===
===Thorium-229===
'''<sup>229</sup>Th''' is a [[radioactive]] [[isotope]] of [[thorium]] that decays by [[alpha particle|alpha]] emission with a [[half-life]] of 7340 years.
'''<sup>229</sup>Th''' is a [[radioactive]] [[isotope]] of [[thorium]] that decays by [[alpha particle|alpha]] emission with a [[half-life]] of 7340 years.
<sup>229</sup>Th is produced by the decay of [[uranium-233]], and its principal use is for the production of the [[nuclear medicine|medical isotopes]] [[actinium-225]] and [[bismuth-213]].<ref>[http://www.ne.doe.gov/pdfFiles/U233RptConMarch2001.pdf Report to Congress on the extraction of medical isotopes from U-233]. U.S. Department of Energy. March 2001</ref>
<sup>229</sup>Th is produced by the decay of [[uranium-233]], and its principal use is for the production of the [[nuclear medicine|medical isotopes]] [[actinium-225]] and [[bismuth-213]].<ref>[http://www.ne.doe.gov/pdfFiles/U233RptConMarch2001.pdf Report to Congress on the extraction of medical isotopes from U-233]. U.S. Department of Energy. March 2001</ref>


====Thorium-229m====
====Thorium-229m====
[[Gamma ray spectroscopy]] has indicated that <sup>229</sup>Th has a [[nuclear isomer]] <sup>229''m''</sup>Th with a remarkably low excitation energy. This would make it the lowest-energy nuclear isomer known, and it might be possible to excite this nuclear state using [[laser]]s with wavelengths in the [[vacuum ultraviolet]]. The isomer might have application for high density energy storage,<ref>
[[Gamma ray spectroscopy]] has indicated that <sup>229</sup>Th has a [[nuclear isomer]] <sup>229''m''</sup>Th with a remarkably low excitation energy. This would make it the lowest-energy nuclear isomer known, and it might be possible to excite this nuclear state using [[laser]]s with wavelengths in the [[vacuum ultraviolet]]. The isomer might have application for high density energy storage,<ref>
{{cite conference
{{cite conference
| last1=Poppe |first1=C. H. |last2=Weiss |first2=M. S. |last3=Anderson |first3=J. D.
| last1=Poppe |first1=C. H. |last2=Weiss |first2=M. S. |last3=Anderson |first3=J. D.
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| first1=E. |last1=Peik
| first1=E. |last1=Peik
| first2=Chr. |last2=Tamm
| first2=Chr. |last2=Tamm
| title = Nuclear laser spectroscopy of the 3.5 eV transition in <sup>229</sup>Th
| title = Nuclear laser spectroscopy of the 3.5&nbsp;eV transition in <sup>229</sup>Th
| url = http://www.ptb.de/cms/fileadmin/internet/fachabteilungen/abteilung_4/4.4_zeit_und_frequenz/pdf/th001.pdf
| url = http://www.ptb.de/cms/fileadmin/internet/fachabteilungen/abteilung_4/4.4_zeit_und_frequenz/pdf/th001.pdf
| journal = Europhysics Letters
| journal = Europhysics Letters
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| bibcode = 2003EL.....61..181P
| bibcode = 2003EL.....61..181P
| accessdate = 2013-12-14
| accessdate = 2013-12-14
}}</ref> as a [[qubit]] for [[quantum computing]], or to test the effect of the chemical environment on nuclear decay rates.<ref name=Tkalya>{{cite journal
}}</ref> as a [[qubit]] for [[quantum computing]], or to test the effect of the chemical environment on nuclear decay rates.<ref name=Tkalya>{{cite journal
| last1=Tkalya |first1=Eugene V. |last2=Zherikhin |first2=Alexander N. |last3=Zhudov |first3=Valerii I.
| last1=Tkalya |first1=Eugene V. |last2=Zherikhin |first2=Alexander N. |last3=Zhudov |first3=Valerii I.
| title = Decay of the low-energy nuclear isomer <sup>229</sup>Th<sup>''m''</sup> (3/2<sup>+</sup>, 3.5±1.0 eV) in solids (dielectrics and metals): A new scheme of experimental research
| title = Decay of the low-energy nuclear isomer <sup>229</sup>Th<sup>''m''</sup> (3/2<sup>+</sup>, 3.5±1.0&nbsp;eV) in solids (dielectrics and metals): A new scheme of experimental research
| journal = [[Physical Review C]]
| journal = [[Physical Review C]]
| volume = 61
| volume = 61
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| year = 2000
| year = 2000
| pages = 064308
| pages = 064308
| doi = 10.1103/PhysRevC.61.064308
| doi = 10.1103/PhysRevC.61.064308
| bibcode = 2000PhRvC..61f4308T }}</ref>
| bibcode = 2000PhRvC..61f4308T }}</ref>


The lifetime of the isomer has been measured to be 6±1&nbsp;hours. The measurement was done by collecting recoiled <sup>229m</sup>Th atoms in a MgF<sub>s</sub> crystal and measuring the light emission variation over time.<ref name="Zhao2012">{{cite journal|last=Zhao|first=Xinxin|coauthors=Yenny Natali Martinez de Escobar, Robert Rundberg, Evelyn M. Bond, Allen Moody, David J. Vieira|year=2012|title=Observation of the Deexcitation of the ^{229m}Th Nuclear Isomer|journal=Physical Review Letters|volume=109|issue=16|issn=0031-9007|doi=10.1103/PhysRevLett.109.160801}}</ref> If this isomer were to decay it would produce a [[gamma ray]] (defined by its origin, not its wavelength) in the ultraviolet range.
The lifetime of the isomer has been measured to be 6±1&nbsp;hours. The measurement was done by collecting recoiled <sup>229m</sup>Th atoms in a MgF<sub>s</sub> crystal and measuring the light emission variation over time.<ref name="Zhao2012">{{cite journal|last=Zhao|first=Xinxin|coauthors=Yenny Natali Martinez de Escobar, Robert Rundberg, Evelyn M. Bond, Allen Moody, David J. Vieira|year=2012|title=Observation of the Deexcitation of the ^{229m}Th Nuclear Isomer|journal=Physical Review Letters|volume=109|issue=16|issn=0031-9007|doi=10.1103/PhysRevLett.109.160801}}</ref> If this isomer were to decay it would produce a [[gamma ray]] (defined by its origin, not its wavelength) in the ultraviolet range.


The isomer transition energy of <sup>229</sup>Th is currently derived from indirect measurements of the gamma-ray spectrum resulting from the decay of <sup>233</sup>U. In 1989–1993 first measurements were performed using high-quality germanium detectors, resulting in an estimate of E = 3.5±1.0 eV for the <sup>229</sup>Th isomer transition energy.<ref name=Helmer1990>
The isomer transition energy of <sup>229</sup>Th is currently derived from indirect measurements of the gamma-ray spectrum resulting from the decay of <sup>233</sup>U. In 1989–1993 first measurements were performed using high-quality germanium detectors, resulting in an estimate of E = 3.5±1.0&nbsp;eV for the <sup>229</sup>Th isomer transition energy.<ref name=Helmer1990>
{{cite journal
{{cite journal
| title = Energy separation of the doublet of intrinsic states at the ground state of <sup>229</sup>Th
| title = Energy separation of the doublet of intrinsic states at the ground state of <sup>229</sup>Th
| author = Reich, C. W. and Helmer, R. G.
| author = Reich, C. W. and Helmer, R. G.
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| year=1994
| year=1994
| author=Helmer, R. G.; Reich, C. W.
| author=Helmer, R. G.; Reich, C. W.
| title = An Excited State of Th-229 at 3.5 eV
| title = An Excited State of Th-229 at 3.5&nbsp;eV
| doi=10.1103/PhysRevC.49.1845
| doi=10.1103/PhysRevC.49.1845
| issue=4
| issue=4
|bibcode = 1994PhRvC..49.1845H }}
|bibcode = 1994PhRvC..49.1845H }}
</ref> This unnaturally low value triggered a multitude of investigations, both theoretical and experimental, trying to determine the transition energy precisely and to specify other properties of the isomer state of <sup>229</sup>Th (such as the lifetime and the magnetic moment). However, searches for direct photon emission from the low-lying excited state have failed to report an unambiguous signal. New indirect measurements with an advanced high-resolution x-ray microcalorimeter were carried out in 2007<ref name=Beck/> yielding a new value for the transition energy of E = 7.6±0.5 eV, corrected to E = 7.8±0.5 eV in 2009.<ref name=BeckReview>
</ref> This unnaturally low value triggered a multitude of investigations, both theoretical and experimental, trying to determine the transition energy precisely and to specify other properties of the isomer state of <sup>229</sup>Th (such as the lifetime and the magnetic moment). However, searches for direct photon emission from the low-lying excited state have failed to report an unambiguous signal. New indirect measurements with an advanced high-resolution x-ray microcalorimeter were carried out in 2007<ref name=Beck/> yielding a new value for the transition energy of E = 7.6±0.5&nbsp;eV, corrected to E = 7.8±0.5&nbsp;eV in 2009.<ref name=BeckReview>
{{cite conference
{{cite conference
| title = Improved value for the energy splitting of the ground-state doublet in the nucleus <sup>229</sup>Th
| title = Improved value for the energy splitting of the ground-state doublet in the nucleus <sup>229</sup>Th
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===Thorium-230===
===Thorium-230===
'''<sup>230</sup>Th''' is a [[radioactive]] [[isotope]] of [[thorium]] which can be used to date [[coral]]s and determine [[ocean current]] flux. '''Ionium''' was a name given early in the study of radioactive elements to the <sup>230</sup>Th [[isotope]] produced in the [[decay chain]] of [[Uranium-238|<sup>238</sup>U]] before it was realized that ionium and [[thorium]] are chemically identical. The symbol '''Io''' was used for this supposed element. (The name is still used in [[ionium-thorium dating]].)
'''<sup>230</sup>Th''' is a [[radioactive]] [[isotope]] of [[thorium]] that can be used to date [[coral]]s and determine [[ocean current]] flux. '''Ionium''' was a name given early in the study of radioactive elements to the <sup>230</sup>Th [[isotope]] produced in the [[decay chain]] of [[Uranium-238|<sup>238</sup>U]] before it was realized that ionium and [[thorium]] are chemically identical. The symbol '''Io''' was used for this supposed element. (The name is still used in [[ionium-thorium dating]].)


===Thorium-231===
===Thorium-231===
'''<sup>231</sup>Th''' has 141 [[neutrons]]. It is the decay product of [[uranium-235]]. It is found in very small amounts on the [[earth]] and has a [[half-life]] of 25.5 hours. When it decays it emits a [[beta ray]] and forms [[protactinium-231]]. It has a decay energy of 0.39 MeV. It has a mass of 231.0363043&nbsp;grams/mole.
'''<sup>231</sup>Th''' has 141 [[neutrons]]. It is the decay product of [[uranium-235]]. It is found in very small amounts on the [[earth]] and has a [[half-life]] of 25.5 hours. When it decays it emits a [[beta ray]] and forms [[protactinium-231]]. It has a decay energy of 0.39&nbsp;MeV. It has a mass of 231.0363043&nbsp;grams/mole.


===Thorium-232===
===Thorium-232===
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<sup>232</sup>Th is a [[fertile material]] able to [[neutron capture|absorb]] a [[neutron]] and undergo [[Nuclear transmutation|transmutation]] into the [[fissile]] [[nuclide]] [[uranium-233]], which is the basis of the [[thorium fuel cycle]].<ref>{{cite web |url=http://www.world-nuclear.org/info/inf62.html |title=Thorium |author=[[World Nuclear Association]] |accessdate=2010-01-25}}</ref>
<sup>232</sup>Th is a [[fertile material]] able to [[neutron capture|absorb]] a [[neutron]] and undergo [[Nuclear transmutation|transmutation]] into the [[fissile]] [[nuclide]] [[uranium-233]], which is the basis of the [[thorium fuel cycle]].<ref>{{cite web |url=http://www.world-nuclear.org/info/inf62.html |title=Thorium |author=[[World Nuclear Association]] |accessdate=2010-01-25}}</ref>


In the form of [[Thorotrast]], a [[thorium dioxide]] [[suspension (chemistry)|suspension]], it was used as [[contrast medium]] in early [[X-ray]] diagnostics. Thorium-232 is now classified as [[carcinogen]]ic.<ref>{{cite journal |last1= Krasinskas |first1= Alyssa M |authorlink= Alyssa M. Krasinskas et al. |last2= Minda |first2= Justina |last3= Saul |first3= Scott H |last4= Shaked |first4= Abraham |last5= Furth |first5= Emma E |title=Redistribution of thorotrast into a liver allograft several years following transplantation: a case report |journal= [[Nature (journal)|Nature]] |volume= 17 |pages= 117–120 |year= 2004 |doi= 10.1038/modpathol.3800008 |pmid=14631374 |issue=1}}</ref>
In the form of [[Thorotrast]], a [[thorium dioxide]] [[suspension (chemistry)|suspension]], it was used as [[contrast medium]] in early [[X-ray]] diagnostics. Thorium-232 is now classified as [[carcinogen]]ic.<ref>{{cite journal |last1= Krasinskas |first1= Alyssa M |display-authors=etal |last2= Minda |first2= Justina |last3= Saul |first3= Scott H |last4= Shaked |first4= Abraham |last5= Furth |first5= Emma E |title=Redistribution of thorotrast into a liver allograft several years following transplantation: a case report |journal= [[Nature (journal)|Nature]] |volume= 17 |pages= 117–120 |year= 2004 |doi= 10.1038/modpathol.3800008 |pmid=14631374 |issue=1}}</ref>


===Thorium-233===
===Thorium-233===
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===Thorium-234===
===Thorium-234===
'''<sup>234</sup>Th''' is an [[isotope]] of [[thorium]] whose [[Atomic nucleus|nuclei]] contain 144 [[neutron]]s. Th-234 has a [[half-life]] of 24.1 days, and when it decays, it emits a [[beta particle]], and in so doing, it [[Nuclear transmutation|transmutes]] into [[protactinium]]-234. Th-234 has a mass of 234.0436 [[atomic mass unit]]s (amu), and it has a decay energy of about 270 keV (kilo[[electron-volt]]s). [[Uranium]]-238 usually decays into this isotope of thorium. (It can undergo [[spontaneous fission]].)
'''<sup>234</sup>Th''' is an [[isotope]] of [[thorium]] whose [[Atomic nucleus|nuclei]] contain 144 [[neutron]]s. Th-234 has a [[half-life]] of 24.1 days, and when it decays, it emits a [[beta particle]], and in so doing, it [[Nuclear transmutation|transmutes]] into [[protactinium]]-234. Th-234 has a mass of 234.0436 [[atomic mass unit]]s (amu), and it has a decay energy of about 270&nbsp;keV (kilo[[electron-volt]]s). [[Uranium]]-238 usually decays into this isotope of thorium. (It can undergo [[spontaneous fission]].)


== Table ==
== Table ==
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! &nbsp;<br />isotopic mass (u)<br />&nbsp;
! &nbsp;<br />isotopic mass (u)<br />&nbsp;
! rowspan="2" | half-life<ref group="n">Bold for nuclides with half-lives longer than the age of the universe (nearly stable)</ref>
! rowspan="2" | half-life<ref group="n">Bold for nuclides with half-lives longer than the age of the universe (nearly stable)</ref>
! rowspan="2" | decay<br>mode(s)<ref>http://www.nucleonica.net/unc.aspx</ref><ref group="n">Abbreviations:<br>CD: [[Cluster decay]]<br>EC: [[Electron capture]]<br>IT: [[Isomeric transition]]<br>SF: [[Spontaneous fission]]</ref>
! rowspan="2" | decay<br>mode(s)<ref>{{cite web |url=http://www.nucleonica.net/unc.aspx |title=Universal Nuclide Chart |publisher=nucleonica |registration=yes}}</ref><ref group="n">Abbreviations:<br>CD: [[Cluster decay]]<br>EC: [[Electron capture]]<br>IT: [[Isomeric transition]]<br>SF: [[Spontaneous fission]]</ref>
! rowspan="2" | daughter<br>isotope(s)<ref group="n">Bold for stable isotopes</ref>
! rowspan="2" | daughter<br>isotope(s)<ref group="n">Bold for stable isotopes</ref>
! rowspan="2" | nuclear<br />spin
! rowspan="2" | nuclear<br />spin
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| style="text-align:right" | 119
| style="text-align:right" | 119
| 209.01772(11)
| 209.01772(11)
| 7(5) ms<br>[3.8(+69-15)]
| 7(5)&nbsp;ms<br>[3.8(+69−15)]
|
|
|
|
| 5/2-#
| 5/2−#
|
|
|
|
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| rowspan=2 style="text-align:right" | 120
| rowspan=2 style="text-align:right" | 120
| rowspan=2|210.015075(27)
| rowspan=2|210.015075(27)
| rowspan=2|17(11) ms<br>[9(+17-4) ms]
| rowspan=2|17(11)&nbsp;ms<br>[9(+17−4)&nbsp;ms]
| [[alpha decay|α]]
| [[alpha decay|α]]
| <sup>206</sup>Ra
| <sup>206</sup>Ra
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| rowspan=2 style="text-align:right" | 121
| rowspan=2 style="text-align:right" | 121
| rowspan=2|211.01493(8)
| rowspan=2|211.01493(8)
| rowspan=2|48(20) ms<br>[0.04(+3-1) s]
| rowspan=2|48(20)&nbsp;ms<br>[0.04(+3−1)&nbsp;s]
| α
| α
| <sup>207</sup>Ra
| <sup>207</sup>Ra
| rowspan=2|5/2-#
| rowspan=2|5/2−#
| rowspan=2|
| rowspan=2|
| rowspan=2|
| rowspan=2|
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| rowspan=2 style="text-align:right" | 122
| rowspan=2 style="text-align:right" | 122
| rowspan=2|212.01298(2)
| rowspan=2|212.01298(2)
| rowspan=2|36(15) ms<br>[30(+20-10) ms]
| rowspan=2|36(15)&nbsp;ms<br>[30(+20-10)&nbsp;ms]
| α (99.7%)
| α (99.7%)
| <sup>208</sup>Ra
| <sup>208</sup>Ra
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| rowspan=2 style="text-align:right" | 123
| rowspan=2 style="text-align:right" | 123
| rowspan=2|213.01301(8)
| rowspan=2|213.01301(8)
| rowspan=2|140(25) ms
| rowspan=2|140(25)&nbsp;ms
| α
| α
| <sup>209</sup>Ra
| <sup>209</sup>Ra
| rowspan=2|5/2-#
| rowspan=2|5/2−#
| rowspan=2|
| rowspan=2|
| rowspan=2|
| rowspan=2|
Line 203: Line 203:
| style="text-align:right" | 124
| style="text-align:right" | 124
| 214.011500(18)
| 214.011500(18)
| 100(25) ms
| 100(25)&nbsp;ms
| α
| α
| <sup>210</sup>Ra
| <sup>210</sup>Ra
Line 215: Line 215:
| style="text-align:right" | 125
| style="text-align:right" | 125
| 215.011730(29)
| 215.011730(29)
| 1.2(2) s
| 1.2(2)&nbsp;s
| α
| α
| <sup>211</sup>Ra
| <sup>211</sup>Ra
| (1/2-)
| (1/2−)
|
|
|
|
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| rowspan=2 style="text-align:right" | 126
| rowspan=2 style="text-align:right" | 126
| rowspan=2|216.011062(14)
| rowspan=2|216.011062(14)
| rowspan=2|26.8(3) ms
| rowspan=2|26.8(3)&nbsp;ms
| α (99.99%)
| α (99.99%)
| <sup>212</sup>Ra
| <sup>212</sup>Ra
Line 239: Line 239:
| style="text-indent:1em" | <sup>216m1</sup>Th
| style="text-indent:1em" | <sup>216m1</sup>Th
|
|
| colspan="3" style="text-indent:2em" | 2042(13) keV
| colspan="3" style="text-indent:2em" | 2042(13)&nbsp;keV
| 137(4) µs
| 137(4)&nbsp;µs
|
|
|
|
Line 249: Line 249:
| style="text-indent:1em" | <sup>216m2</sup>Th
| style="text-indent:1em" | <sup>216m2</sup>Th
|
|
| colspan="3" style="text-indent:2em" | 2637(20) keV
| colspan="3" style="text-indent:2em" | 2637(20)&nbsp;keV
| 615(55) ns
| 615(55)&nbsp;ns
|
|
|
|
| (11-)
| (11−)
|
|
|
|
Line 262: Line 262:
| style="text-align:right" | 127
| style="text-align:right" | 127
| 217.013114(22)
| 217.013114(22)
| 240(5) µs
| 240(5)&nbsp;µs
| α
| α
| <sup>213</sup>Ra
| <sup>213</sup>Ra
Line 274: Line 274:
| style="text-align:right" | 128
| style="text-align:right" | 128
| 218.013284(14)
| 218.013284(14)
| 109(13) ns
| 109(13)&nbsp;ns
| α
| α
| <sup>214</sup>Ra
| <sup>214</sup>Ra
Line 286: Line 286:
| rowspan=2 style="text-align:right" | 129
| rowspan=2 style="text-align:right" | 129
| rowspan=2|219.01554(5)
| rowspan=2|219.01554(5)
| rowspan=2|1.05(3) µs
| rowspan=2|1.05(3)&nbsp;µs
| α
| α
| <sup>215</sup>Ra
| <sup>215</sup>Ra
Line 301: Line 301:
| rowspan=2 style="text-align:right" | 130
| rowspan=2 style="text-align:right" | 130
| rowspan=2|220.015748(24)
| rowspan=2|220.015748(24)
| rowspan=2|9.7(6) µs
| rowspan=2|9.7(6)&nbsp;µs
| α
| α
| <sup>216</sup>Ra
| <sup>216</sup>Ra
Line 316: Line 316:
| style="text-align:right" | 131
| style="text-align:right" | 131
| 221.018184(10)
| 221.018184(10)
| 1.73(3) ms
| 1.73(3)&nbsp;ms
| α
| α
| <sup>217</sup>Ra
| <sup>217</sup>Ra
Line 328: Line 328:
| rowspan=2 style="text-align:right" | 132
| rowspan=2 style="text-align:right" | 132
| rowspan=2|222.018468(13)
| rowspan=2|222.018468(13)
| rowspan=2|2.237(13) ms
| rowspan=2|2.237(13)&nbsp;ms
| α
| α
| <sup>218</sup>Ra
| <sup>218</sup>Ra
Line 343: Line 343:
| style="text-align:right" | 133
| style="text-align:right" | 133
| 223.020811(10)
| 223.020811(10)
| 0.60(2) s
| 0.60(2)&nbsp;s
| α
| α
| <sup>219</sup>Ra
| <sup>219</sup>Ra
Line 355: Line 355:
| rowspan=2 style="text-align:right" | 134
| rowspan=2 style="text-align:right" | 134
| rowspan=2|224.021467(12)
| rowspan=2|224.021467(12)
| rowspan=2|1.05(2) s
| rowspan=2|1.05(2)&nbsp;s
| α
| α
| <sup>220</sup>Ra
| <sup>220</sup>Ra
Line 370: Line 370:
| rowspan=2 style="text-align:right" | 135
| rowspan=2 style="text-align:right" | 135
| rowspan=2|225.023951(5)
| rowspan=2|225.023951(5)
| rowspan=2|8.72(4) min
| rowspan=2|8.72(4)&nbsp;min
| α (90%)
| α (90%)
| <sup>221</sup>Ra
| <sup>221</sup>Ra
Line 385: Line 385:
| style="text-align:right" | 136
| style="text-align:right" | 136
| 226.024903(5)
| 226.024903(5)
| 30.57(10) min
| 30.57(10)&nbsp;min
| α
| α
| <sup>222</sup>Ra
| <sup>222</sup>Ra
Line 397: Line 397:
| style="text-align:right" | 137
| style="text-align:right" | 137
| 227.0277041(27)
| 227.0277041(27)
| 18.68(9) d
| 18.68(9)&nbsp;d
| α
| α
| <sup>223</sup>Ra
| <sup>223</sup>Ra
Line 409: Line 409:
| rowspan=2 style="text-align:right" | 138
| rowspan=2 style="text-align:right" | 138
| rowspan=2|228.0287411(24)
| rowspan=2|228.0287411(24)
| rowspan=2|1.9116(16) a
| rowspan=2|1.9116(16)&nbsp;y
| α
| α
| <sup>224</sup>Ra
| <sup>224</sup>Ra
Line 424: Line 424:
| style="text-align:right" | 139
| style="text-align:right" | 139
| 229.031762(3)
| 229.031762(3)
| 7.34(16)&times;10<sup>3</sup> a
| 7.34(16)&times;10<sup>3</sup>&nbsp;y
| α
| α
| <sup>225</sup>Ra
| <sup>225</sup>Ra
Line 433: Line 433:
| style="text-indent:1em" | <sup>229m</sup>Th
| style="text-indent:1em" | <sup>229m</sup>Th
|
|
| colspan="3" style="text-indent:2em" | 0.0076(5) keV
| colspan="3" style="text-indent:2em" | 0.0076(5)&nbsp;keV
| 70(50) h
| 70(50)&nbsp;h
| [[Isomeric transition|IT]]
| [[Isomeric transition|IT]]
| <sup>229</sup>Th
| <sup>229</sup>Th
Line 446: Line 446:
| rowspan=3 style="text-align:right" | 140
| rowspan=3 style="text-align:right" | 140
| rowspan=3|230.0331338(19)
| rowspan=3|230.0331338(19)
| rowspan=3|7.538(30)&times;10<sup>4</sup> a
| rowspan=3|7.538(30)&times;10<sup>4</sup>&nbsp;y
| α
| α
| <sup>226</sup>Ra
| <sup>226</sup>Ra
| rowspan=3|0+
| rowspan=3|0+
| rowspan=3|Trace<ref group="n" name="us">Intermediate decay product of [[Uranium-238|<sup>238</sup>U]]</ref>
| rowspan=3|Trace <ref group="n" name="us">Intermediate decay product of [[Uranium-238|<sup>238</sup>U]]</ref>
| rowspan=3|
| rowspan=3|
|-
|-
Line 464: Line 464:
| rowspan=2 style="text-align:right" | 141
| rowspan=2 style="text-align:right" | 141
| rowspan=2|231.0363043(19)
| rowspan=2|231.0363043(19)
| rowspan=2|25.52(1) h
| rowspan=2|25.52(1)&nbsp;h
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>231</sup>Pa
| <sup>231</sup>Pa
Line 479: Line 479:
| rowspan=4 style="text-align:right" | 142
| rowspan=4 style="text-align:right" | 142
| rowspan=4|232.0380553(21)
| rowspan=4|232.0380553(21)
| rowspan=4|'''1.405(6)&times;10<sup>10</sup> a'''
| rowspan=4|'''1.405(6)&times;10<sup>10</sup>&nbsp;y'''
| α
| α
| <sup>228</sup>Ra
| <sup>228</sup>Ra
Line 500: Line 500:
| style="text-align:right" | 143
| style="text-align:right" | 143
| 233.0415818(21)
| 233.0415818(21)
| 21.83(4) min
| 21.83(4)&nbsp;min
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>233</sup>Pa
| <sup>233</sup>Pa
Line 512: Line 512:
| style="text-align:right" | 144
| style="text-align:right" | 144
| 234.043601(4)
| 234.043601(4)
| 24.10(3) d
| 24.10(3)&nbsp;d
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>234m</sup>Pa
| <sup>234m</sup>Pa
Line 524: Line 524:
| style="text-align:right" | 145
| style="text-align:right" | 145
| 235.04751(5)
| 235.04751(5)
| 7.2(1) min
| 7.2(1)&nbsp;min
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>235</sup>Pa
| <sup>235</sup>Pa
Line 536: Line 536:
| style="text-align:right" | 146
| style="text-align:right" | 146
| 236.04987(21)#
| 236.04987(21)#
| 37.5(2) min
| 37.5(2)&nbsp;min
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>236</sup>Pa
| <sup>236</sup>Pa
Line 548: Line 548:
| style="text-align:right" | 147
| style="text-align:right" | 147
| 237.05389(39)#
| 237.05389(39)#
| 4.8(5) min
| 4.8(5)&nbsp;min
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>237</sup>Pa
| <sup>237</sup>Pa
Line 560: Line 560:
| style="text-align:right" | 148
| style="text-align:right" | 148
| 238.0565(3)#
| 238.0565(3)#
| 9.4(20) min
| 9.4(20)&nbsp;min
| β<sup>−</sup>
| β<sup>−</sup>
| <sup>238</sup>Pa
| <sup>238</sup>Pa
Line 572: Line 572:
* Geologically exceptional samples are known in which the isotopic composition lies outside the reported range. The uncertainty in the atomic mass may exceed the stated value for such specimens.
* Geologically exceptional samples are known in which the isotopic composition lies outside the reported range. The uncertainty in the atomic mass may exceed the stated value for such specimens.
* Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
* Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
* Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC which use expanded uncertainties.
* Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC, which use expanded uncertainties.


== Uses ==
== Uses ==
Thorium has been suggested for use as a source of nuclear energy. Presumably, it would need to be exposed to neutrons in a nuclear reactor, to convert the common isotope to some species that is fissionable.
Thorium has been suggested for use as a source of nuclear energy. Presumably, it would need to be exposed to neutrons in a nuclear reactor, to convert the common isotope to some species that is fissionable.


It is currently used in cathodes of vacuum tubes, for a combination of physical stability at high temperature and a low work energy required to remove an electron from its surface.
It is currently used in cathodes of vacuum tubes, for a combination of physical stability at high temperature and a low work energy required to remove an electron from its surface.
Line 583: Line 583:
Thorium was also used in certain glass elements of Aero-Ektar lenses made by Kodak during World War II. Thus they are mildly radioactive. Two of the glass elements in the f/2.5 Aero-Ektar lenses are 11 and 13% thorium by weight. The Thorium-containing glasses were used because they have a high refractive index with a low dispersion (variation of index with wavelength), a highly desirable property. Many surviving Aero-Ektar lenses have a tea colored tint, possibly due to radiation damage to the glass.
Thorium was also used in certain glass elements of Aero-Ektar lenses made by Kodak during World War II. Thus they are mildly radioactive. Two of the glass elements in the f/2.5 Aero-Ektar lenses are 11 and 13% thorium by weight. The Thorium-containing glasses were used because they have a high refractive index with a low dispersion (variation of index with wavelength), a highly desirable property. Many surviving Aero-Ektar lenses have a tea colored tint, possibly due to radiation damage to the glass.


As these lenses were used for aerial reconnaissance, the radiation level is not high enough to fog film over a short period. This would indicate the radiation level is reasonably safe. However. when not in use, it would be prudent to store these lenses as far as possible from normally inhabited areas; allowing the inverse square relationship to attenuate the radiation.<ref>{{Cite web|title = Aero-Ektar Lenses|url = http://home.earthlink.net/~michaelbriggs/aeroektar/aeroektar.html|website = home.earthlink.net|accessdate = 2015-08-28}}</ref>
As these lenses were used for aerial reconnaissance, the radiation level is not high enough to fog film over a short period. This would indicate the radiation level is reasonably safe. However. when not in use, it would be prudent to store these lenses as far as possible from normally inhabited areas; allowing the inverse square relationship to attenuate the radiation.<ref>{{Cite web|title = Aero-Ektar Lenses|url = http://home.earthlink.net/~michaelbriggs/aeroektar/aeroektar.html |author=Michael S. Briggs |date=January 16, 2002 |accessdate = 2015-08-28}}</ref>


==References==
==References==
{{Reflist}}
{{Reflist}}
* Isotope masses from:
* Isotope masses from:
**{{cite journal |author=G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon |year=2003 |title=The NUBASE evaluation of nuclear and decay properties |url=http://www.nndc.bnl.gov/amdc/nubase/Nubase2003.pdf |journal=[[Nuclear Physics A]] |volume=729 |issue= |pages=3–128 |doi=10.1016/j.nuclphysa.2003.11.001 |bibcode=2003NuPhA.729....3A}}
**{{cite journal |author=G. Audi |author2=A. H. Wapstra |author3=C. Thibault |author4=J. Blachot |author5=O. Bersillon |year=2003 |title=The NUBASE evaluation of nuclear and decay properties |url=http://www.nndc.bnl.gov/amdc/nubase/Nubase2003.pdf |journal=[[Nuclear Physics A]] |volume=729 |issue= |pages=3–128 |doi=10.1016/j.nuclphysa.2003.11.001 |bibcode=2003NuPhA.729....3A}}
* Isotopic compositions and standard atomic masses from:
* Isotopic compositions and standard atomic masses from:
**{{cite journal |author=J. R. de Laeter, J. K. Böhlke, P. De Bièvre, H. Hidaka, H. S. Peiser, K. J. R. Rosman and P. D. P. Taylor |year=2003 |title=Atomic weights of the elements. Review 2000 (IUPAC Technical Report) |url=http://www.iupac.org/publications/pac/75/6/0683/pdf/ |journal=[[Pure and Applied Chemistry]] |volume=75 |issue=6 |pages=683–800 |doi=10.1351/pac200375060683}}
**{{cite journal |author=J. R. de Laeter |author2=J. K. Böhlke |author3=P. De Bièvre |author4=H. Hidaka |author5=H. S. Peiser |author6=K. J. R. Rosman |author7=P. D. P. Taylor |year=2003 |title=Atomic weights of the elements. Review 2000 (IUPAC Technical Report) |url=http://www.iupac.org/publications/pac/75/6/0683/pdf/ |journal=[[Pure and Applied Chemistry]] |volume=75 |issue=6 |pages=683–800 |doi=10.1351/pac200375060683}}
**{{cite journal |author=M. E. Wieser |year=2006 |title=Atomic weights of the elements 2005 (IUPAC Technical Report) |url=http://iupac.org/publications/pac/78/11/2051/pdf/ |journal=[[Pure and Applied Chemistry]] |volume=78 |issue=11 |pages=2051–2066 |doi=10.1351/pac200678112051 |laysummary=http://old.iupac.org/news/archives/2005/atomic-weights_revised05.html}}
**{{cite journal |author=M. E. Wieser |year=2006 |title=Atomic weights of the elements 2005 (IUPAC Technical Report) |url=http://iupac.org/publications/pac/78/11/2051/pdf/ |journal=[[Pure and Applied Chemistry]] |volume=78 |issue=11 |pages=2051–2066 |doi=10.1351/pac200678112051 |laysummary=http://old.iupac.org/news/archives/2005/atomic-weights_revised05.html}}
* Half-life, spin, and isomer data selected from the following sources. See editing notes on [[Talk:Isotopes of thorium|this article's talk page]].
* Half-life, spin, and isomer data selected from the following sources. See editing notes on [[Talk:Isotopes of thorium|this article's talk page]].
**{{cite journal |author=G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon |year=2003 |title=The NUBASE evaluation of nuclear and decay properties |url=http://amdc.in2p3.fr/nubase/Nubase2003.pdf |journal=[[Nuclear Physics A]] |volume=729 |issue= |pages=3–128 |doi=10.1016/j.nuclphysa.2003.11.001 |bibcode=2003NuPhA.729....3A}}
**{{cite journal |author=G. Audi |author2=A. H. Wapstra |author3=C. Thibault |author4=J. Blachot |author5=O. Bersillon |year=2003 |title=The NUBASE evaluation of nuclear and decay properties |url=http://amdc.in2p3.fr/nubase/Nubase2003.pdf |journal=[[Nuclear Physics A]] |volume=729 |issue= |pages=3–128 |doi=10.1016/j.nuclphysa.2003.11.001 |bibcode=2003NuPhA.729....3A}}
**{{cite web |author=[[National Nuclear Data Center]] |title=NuDat 2.1 database |url=http://www.nndc.bnl.gov/nudat2/ |publisher=[[Brookhaven National Laboratory]] |accessdate=September 2005}}
**{{cite web |author=[[National Nuclear Data Center]] |title=NuDat 2.1 database |url=http://www.nndc.bnl.gov/nudat2/ |publisher=[[Brookhaven National Laboratory]] |accessdate=September 2005}}
**{{cite book |author=N. E. Holden |year=2004 |editor=D. R. Lide |chapter=Table of the Isotopes |title=[[CRC Handbook of Chemistry and Physics]] |page=Section 11 |nopp=yes |edition=85th |publisher=[[CRC Press]] |isbn=978-0-8493-0485-9}}
**{{cite book |author=N. E. Holden |year=2004 |editor=D. R. Lide |chapter=Table of the Isotopes |title=[[CRC Handbook of Chemistry and Physics]] |page=Section 11 |nopp=yes |edition=85th |publisher=[[CRC Press]] |isbn=978-0-8493-0485-9}}

Revision as of 07:31, 7 October 2015

Actinides[1] by decay chain Half-life
range (a)
Fission products of 235U by yield[2]
4n 4n + 1 4n + 2 4n + 3 4.5–7% 0.04–1.25% <0.001%
228Ra 4–6 a 155Euþ
244Cmƒ 241Puƒ 250Cf 227Ac 10–29 a 90Sr 85Kr 113mCdþ
232Uƒ 238Puƒ 243Cmƒ 29–97 a 137Cs 151Smþ 121mSn
248Bk[3] 249Cfƒ 242mAmƒ 141–351 a

No fission products have a half-life
in the range of 100 a–210 ka ...

241Amƒ 251Cfƒ[4] 430–900 a
226Ra 247Bk 1.3–1.6 ka
240Pu 229Th 246Cmƒ 243Amƒ 4.7–7.4 ka
245Cmƒ 250Cm 8.3–8.5 ka
239Puƒ 24.1 ka
230Th 231Pa 32–76 ka
236Npƒ 233Uƒ 234U 150–250 ka 99Tc 126Sn
248Cm 242Pu 327–375 ka 79Se
1.53 Ma 93Zr
237Npƒ 2.1–6.5 Ma 135Cs 107Pd
236U 247Cmƒ 15–24 Ma 129I
244Pu 80 Ma

... nor beyond 15.7 Ma[5]

232Th 238U 235Uƒ№ 0.7–14.1 Ga

Although thorium (Th), with atomic number 90, has 6 naturally occurring isotopes, none of these isotopes are stable; however, one isotope, 232Th, is relatively stable, with a half-life of 14.05 billion years, considerably longer than the age of the earth, and even slightly longer than the generally accepted age of the universe. This isotope makes up nearly all natural thorium. As such, thorium is considered to be mononuclidic. It has a characteristic terrestrial isotopic composition and thus an atomic mass can be given. Standard atomic mass: 232.03806(2) u.

Thirty radioisotopes have been characterized, with the most stable (after 232Th) being 230Th with a half-life of 75,380 years, 229Th with a half-life of 7,340 years, and 228Th with a half-life of 1.92 years. All of the remaining radioactive isotopes have half-lives that are less than thirty days and the majority of these have half-lives that are less than ten minutes. One isotope, 229Th, has a nuclear isomer (or metastable state) with a remarkably low excitation energy,[6] recently measured to be 7.6 ± 0.5 eV.[7]

The known isotopes of thorium range in mass number from 209[8] to 238.

Some notable isotopes

Thorium-228

228Th is an isotope of thorium with 138 neutrons. It was once named Radiothorium, due to its occurrence in the disintegration chain of thorium-232. It has a half-life of 1.9116 years. It undergoes alpha decay to 224Ra. Occasionally it decays by the unusual route of cluster decay, emitting a nucleus of 20O and producing stable 208Pb. It is a daughter isotope of 232U.

Th-228 has an atomic weight of 228.0287411 grams/mole. Uranium-232 decays to this nuclide by alpha emission.

Thorium-229

229Th is a radioactive isotope of thorium that decays by alpha emission with a half-life of 7340 years. 229Th is produced by the decay of uranium-233, and its principal use is for the production of the medical isotopes actinium-225 and bismuth-213.[9]

Thorium-229m

Gamma ray spectroscopy has indicated that 229Th has a nuclear isomer 229mTh with a remarkably low excitation energy. This would make it the lowest-energy nuclear isomer known, and it might be possible to excite this nuclear state using lasers with wavelengths in the vacuum ultraviolet. The isomer might have application for high density energy storage,[10] an accurate clock,[11] as a qubit for quantum computing, or to test the effect of the chemical environment on nuclear decay rates.[12]

The lifetime of the isomer has been measured to be 6±1 hours. The measurement was done by collecting recoiled 229mTh atoms in a MgFs crystal and measuring the light emission variation over time.[13] If this isomer were to decay it would produce a gamma ray (defined by its origin, not its wavelength) in the ultraviolet range.

The isomer transition energy of 229Th is currently derived from indirect measurements of the gamma-ray spectrum resulting from the decay of 233U. In 1989–1993 first measurements were performed using high-quality germanium detectors, resulting in an estimate of E = 3.5±1.0 eV for the 229Th isomer transition energy.[14][15] This unnaturally low value triggered a multitude of investigations, both theoretical and experimental, trying to determine the transition energy precisely and to specify other properties of the isomer state of 229Th (such as the lifetime and the magnetic moment). However, searches for direct photon emission from the low-lying excited state have failed to report an unambiguous signal. New indirect measurements with an advanced high-resolution x-ray microcalorimeter were carried out in 2007[7] yielding a new value for the transition energy of E = 7.6±0.5 eV, corrected to E = 7.8±0.5 eV in 2009.[16] This value is currently the most accepted one in the community but cannot be considered definite until a direct measurement is made successfully. The shift into the VUV domain probably explains why previous attempts to directly observe the transition were unsuccessful.

Thorium-230

230Th is a radioactive isotope of thorium that can be used to date corals and determine ocean current flux. Ionium was a name given early in the study of radioactive elements to the 230Th isotope produced in the decay chain of 238U before it was realized that ionium and thorium are chemically identical. The symbol Io was used for this supposed element. (The name is still used in ionium-thorium dating.)

Thorium-231

231Th has 141 neutrons. It is the decay product of uranium-235. It is found in very small amounts on the earth and has a half-life of 25.5 hours. When it decays it emits a beta ray and forms protactinium-231. It has a decay energy of 0.39 MeV. It has a mass of 231.0363043 grams/mole.

Thorium-232

As Thorium is mononuclidic, the main article on thorium effectively discusses this isotope.

232Th is the only primordial isotope of thorium and makes up effectively all of natural thorium, with other isotopes of thorium appearing only in trace amounts as relatively short-lived decay products of uranium and thorium.[17]

232Th decays by alpha decay with a half-life of 1.405×1010 years, over three times the age of the earth and more than the age of the universe. Its decay chain is the thorium series eventually ending in lead-208. The remainder of the chain is quick; the longest half-lives in it are 5.75 years for radium-228 and 1.91 years for thorium-228, with all other half-lives totaling less than 5 days.[18]

232Th is a fertile material able to absorb a neutron and undergo transmutation into the fissile nuclide uranium-233, which is the basis of the thorium fuel cycle.[19]

In the form of Thorotrast, a thorium dioxide suspension, it was used as contrast medium in early X-ray diagnostics. Thorium-232 is now classified as carcinogenic.[20]

Thorium-233

233Th is an isotope of thorium that decays into protactinium-233 through beta decay. It has a half-life of 21.83 minutes.[21]

Thorium-234

234Th is an isotope of thorium whose nuclei contain 144 neutrons. Th-234 has a half-life of 24.1 days, and when it decays, it emits a beta particle, and in so doing, it transmutes into protactinium-234. Th-234 has a mass of 234.0436 atomic mass units (amu), and it has a decay energy of about 270 keV (kiloelectron-volts). Uranium-238 usually decays into this isotope of thorium. (It can undergo spontaneous fission.)

Table

nuclide
symbol
historic
name
Z(p) N(n)  
isotopic mass (u)
 
half-life[n 1] decay
mode(s)[22][n 2]
daughter
isotope(s)[n 3]
nuclear
spin
representative
isotopic
composition
(mole fraction)
range of natural
variation
(mole fraction)
excitation energy
209Th 90 119 209.01772(11) 7(5) ms
[3.8(+69−15)]
5/2−#
210Th 90 120 210.015075(27) 17(11) ms
[9(+17−4) ms]
α 206Ra 0+
β+ (rare) 210Ac
211Th 90 121 211.01493(8) 48(20) ms
[0.04(+3−1) s]
α 207Ra 5/2−#
β+ (rare) 211Ac
212Th 90 122 212.01298(2) 36(15) ms
[30(+20-10) ms]
α (99.7%) 208Ra 0+
β+ (.3%) 212Ac
213Th 90 123 213.01301(8) 140(25) ms α 209Ra 5/2−#
β+ (rare) 213Ac
214Th 90 124 214.011500(18) 100(25) ms α 210Ra 0+
215Th 90 125 215.011730(29) 1.2(2) s α 211Ra (1/2−)
216Th 90 126 216.011062(14) 26.8(3) ms α (99.99%) 212Ra 0+
β+ (.006%) 216Ac
216m1Th 2042(13) keV 137(4) µs (8+)
216m2Th 2637(20) keV 615(55) ns (11−)
217Th 90 127 217.013114(22) 240(5) µs α 213Ra (9/2+)
218Th 90 128 218.013284(14) 109(13) ns α 214Ra 0+
219Th 90 129 219.01554(5) 1.05(3) µs α 215Ra 9/2+#
β+ (10−7%) 219Ac
220Th 90 130 220.015748(24) 9.7(6) µs α 216Ra 0+
EC (2×10−7%) 220Ac
221Th 90 131 221.018184(10) 1.73(3) ms α 217Ra (7/2+)
222Th 90 132 222.018468(13) 2.237(13) ms α 218Ra 0+
EC (1.3×10−8%) 222Ac
223Th 90 133 223.020811(10) 0.60(2) s α 219Ra (5/2)+
224Th 90 134 224.021467(12) 1.05(2) s α 220Ra 0+
β+β+ (rare) 224Ra
225Th 90 135 225.023951(5) 8.72(4) min α (90%) 221Ra (3/2)+
EC (10%) 225Ac
226Th 90 136 226.024903(5) 30.57(10) min α 222Ra 0+
227Th Radioactinium 90 137 227.0277041(27) 18.68(9) d α 223Ra 1/2+ Trace[n 4]
228Th Radiothorium 90 138 228.0287411(24) 1.9116(16) y α 224Ra 0+ Trace[n 5]
CD (1.3×10−11%) 208Pb
20O
229Th 90 139 229.031762(3) 7.34(16)×103 y α 225Ra 5/2+
229mTh 0.0076(5) keV 70(50) h IT 229Th 3/2+
230Th[n 6] Ionium 90 140 230.0331338(19) 7.538(30)×104 y α 226Ra 0+ Trace [n 7]
CD (5.6×10−11%) 206Hg
24Ne
SF (5×10−11%) (Various)
231Th Uranium Y 90 141 231.0363043(19) 25.52(1) h β 231Pa 5/2+ Trace[n 4]
α (10−8%) 227Ra
232Th[n 8] Thorium 90 142 232.0380553(21) 1.405(6)×1010 y α 228Ra 0+ 1.0000
ββ (rare) 232U
SF (1.1×10−9%) (various)
CD (2.78×10−10%) 182Yb
26Ne
24Ne
233Th 90 143 233.0415818(21) 21.83(4) min β 233Pa 1/2+
234Th Uranium X1 90 144 234.043601(4) 24.10(3) d β 234mPa 0+ Trace[n 7]
235Th 90 145 235.04751(5) 7.2(1) min β 235Pa (1/2+)#
236Th 90 146 236.04987(21)# 37.5(2) min β 236Pa 0+
237Th 90 147 237.05389(39)# 4.8(5) min β 237Pa 5/2+#
238Th 90 148 238.0565(3)# 9.4(20) min β 238Pa 0+
  1. ^ Bold for nuclides with half-lives longer than the age of the universe (nearly stable)
  2. ^ Abbreviations:
    CD: Cluster decay
    EC: Electron capture
    IT: Isomeric transition
    SF: Spontaneous fission
  3. ^ Bold for stable isotopes
  4. ^ a b Intermediate decay product of 235U
  5. ^ Intermediate decay product of 232Th
  6. ^ Used in Uranium-thorium dating
  7. ^ a b Intermediate decay product of 238U
  8. ^ Primordial radionuclide

Notes

  • Geologically exceptional samples are known in which the isotopic composition lies outside the reported range. The uncertainty in the atomic mass may exceed the stated value for such specimens.
  • Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
  • Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC, which use expanded uncertainties.

Uses

Thorium has been suggested for use as a source of nuclear energy. Presumably, it would need to be exposed to neutrons in a nuclear reactor, to convert the common isotope to some species that is fissionable.

It is currently used in cathodes of vacuum tubes, for a combination of physical stability at high temperature and a low work energy required to remove an electron from its surface. It has, for about a century, been used in mantles of gas and vapor lamps such as gas lights and camping lanterns. Its radioactivity is a consideration for its non-nuclear uses but is too small to rule it out.

Thorium was also used in certain glass elements of Aero-Ektar lenses made by Kodak during World War II. Thus they are mildly radioactive. Two of the glass elements in the f/2.5 Aero-Ektar lenses are 11 and 13% thorium by weight. The Thorium-containing glasses were used because they have a high refractive index with a low dispersion (variation of index with wavelength), a highly desirable property. Many surviving Aero-Ektar lenses have a tea colored tint, possibly due to radiation damage to the glass.

As these lenses were used for aerial reconnaissance, the radiation level is not high enough to fog film over a short period. This would indicate the radiation level is reasonably safe. However. when not in use, it would be prudent to store these lenses as far as possible from normally inhabited areas; allowing the inverse square relationship to attenuate the radiation.[23]

References

  1. ^ Plus radium (element 88). While actually a sub-actinide, it immediately precedes actinium (89) and follows a three-element gap of instability after polonium (84) where no nuclides have half-lives of at least four years (the longest-lived nuclide in the gap is radon-222 with a half life of less than four days). Radium's longest lived isotope, at 1,600 years, thus merits the element's inclusion here.
  2. ^ Specifically from thermal neutron fission of uranium-235, e.g. in a typical nuclear reactor.
  3. ^ Milsted, J.; Friedman, A. M.; Stevens, C. M. (1965). "The alpha half-life of berkelium-247; a new long-lived isomer of berkelium-248". Nuclear Physics. 71 (2): 299. Bibcode:1965NucPh..71..299M. doi:10.1016/0029-5582(65)90719-4.
    "The isotopic analyses disclosed a species of mass 248 in constant abundance in three samples analysed over a period of about 10 months. This was ascribed to an isomer of Bk248 with a half-life greater than 9 [years]. No growth of Cf248 was detected, and a lower limit for the β half-life can be set at about 104 [years]. No alpha activity attributable to the new isomer has been detected; the alpha half-life is probably greater than 300 [years]."
  4. ^ This is the heaviest nuclide with a half-life of at least four years before the "sea of instability".
  5. ^ Excluding those "classically stable" nuclides with half-lives significantly in excess of 232Th; e.g., while 113mCd has a half-life of only fourteen years, that of 113Cd is eight quadrillion years.
  6. ^ E. Ruchowska (2006). "Nuclear structure of 229Th". Phys. Rev. C. 73 (4): 044326. Bibcode:2006PhRvC..73d4326R. doi:10.1103/PhysRevC.73.044326.
  7. ^ a b B. R. Beck; et al. (2007-04-06). "Energy splitting in the ground state doublet in the nucleus 229Th". Physical Review Letters. 98 (14): 142501. Bibcode:2007PhRvL..98n2501B. doi:10.1103/PhysRevLett.98.142501. PMID 17501268.
  8. ^ H. Ikezoe; et al. (1996). "alpha decay of a new isotope of 209Th". Physical Review C. 54 (4): 2043. Bibcode:1996PhRvC..54.2043I. doi:10.1103/PhysRevC.54.2043.
  9. ^ Report to Congress on the extraction of medical isotopes from U-233. U.S. Department of Energy. March 2001
  10. ^ Poppe, C. H.; Weiss, M. S.; Anderson, J. D. (1992). "Nuclear isomers as ultra-high-energy-density materials". Air Force Meeting on High Energy Density Materials, Lancaster, CA. Bibcode:1992hedm.meet...23P. {{cite conference}}: Unknown parameter |booktitle= ignored (|book-title= suggested) (help)
  11. ^ Peik, E.; Tamm, Chr. (2003-01-15). "Nuclear laser spectroscopy of the 3.5 eV transition in 229Th" (PDF). Europhysics Letters. 61 (2): 181–186. Bibcode:2003EL.....61..181P. doi:10.1209/epl/i2003-00210-x. Retrieved 2013-12-14.
  12. ^ Tkalya, Eugene V.; Zherikhin, Alexander N.; Zhudov, Valerii I. (2000). "Decay of the low-energy nuclear isomer 229Thm (3/2+, 3.5±1.0 eV) in solids (dielectrics and metals): A new scheme of experimental research". Physical Review C. 61 (6): 064308. Bibcode:2000PhRvC..61f4308T. doi:10.1103/PhysRevC.61.064308.
  13. ^ Zhao, Xinxin (2012). "Observation of the Deexcitation of the ^{229m}Th Nuclear Isomer". Physical Review Letters. 109 (16). doi:10.1103/PhysRevLett.109.160801. ISSN 0031-9007. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  14. ^ Reich, C. W. and Helmer, R. G. (Jan 1990). "Energy separation of the doublet of intrinsic states at the ground state of 229Th". Phys. Rev. Lett. 64 (3). American Physical Society: 271–273. Bibcode:1990PhRvL..64..271R. doi:10.1103/PhysRevLett.64.271.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  15. ^ Helmer, R. G.; Reich, C. W. (1994). "An Excited State of Th-229 at 3.5 eV". Physical Review C. 49 (4): 1845–1858. Bibcode:1994PhRvC..49.1845H. doi:10.1103/PhysRevC.49.1845.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  16. ^ Beck B R, Wu C Y, Beiersdorfer P, Brown G V, Becker J A, Moody K J, Wilhelmy J B, Porter F S, Kilbourne C A and Kelley R L (2009-07-30). Improved value for the energy splitting of the ground-state doublet in the nucleus 229Th (PDF). 12th Int. Conf. on Nuclear Reaction Mechanisms (Varenna, Italy). LLNL-PROC-415170.{{cite conference}}: CS1 maint: multiple names: authors list (link)
  17. ^ Isotopes Project Home Page, Lawrence Berkeley National Laboratory. "Isotopes of Thorium (Z=90)". Retrieved 2010-01-18. {{cite web}}: |author= has generic name (help)
  18. ^ Rutherford Appleton Laboratory. "Th-232 Decay Chain". Retrieved 2010-01-25.
  19. ^ World Nuclear Association. "Thorium". Retrieved 2010-01-25.
  20. ^ Krasinskas, Alyssa M; Minda, Justina; Saul, Scott H; Shaked, Abraham; Furth, Emma E; et al. (2004). "Redistribution of thorotrast into a liver allograft several years following transplantation: a case report". Nature. 17 (1): 117–120. doi:10.1038/modpathol.3800008. PMID 14631374.
  21. ^ Georges, Audi (2003). "The NUBASE Evaluation of Nuclear and Decay Properties". Nuclear Physics A. 729. Atomic Mass Data Center: 3–128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.
  22. ^ "Universal Nuclide Chart". nucleonica. {{cite web}}: Unknown parameter |registration= ignored (|url-access= suggested) (help)
  23. ^ Michael S. Briggs (January 16, 2002). "Aero-Ektar Lenses". Retrieved 2015-08-28.