Isotopes of plutonium#Plutonium-237

{{Anchor|Plutonium-221|Plutonium-222|Plutonium-223|Plutonium-224|Plutonium-225|Plutonium-226}}

{{Isotopes table

|symbol=Pu

|refs=NUBASE2020, AME2020 II

|notes=m, unc(), mass#, spin(), spin#, daughter-st, daughter-nst, EC, SF, CD, IT

}}

|-id=Plutonium-226

| {{sup|226}}Pu{{Cite web |url=http://www1.jinr.ru/Preprints/2024/50(P7-2024-50).pdf |title=Свойства радиоактивного распада нового ядра ²²⁷Pu |trans-title=Properties of Radioactive Decay of the New Nucleus ²²⁷Pu |vauthors=Kuznetsova AA, Svirikhin AI, Isaev AV, Bychkov MA, Danilkin VD, Devarazha KM, Zamyatin NI, Izosimov IN, Liu Z, Malyshev ON, Mukhin RS, Popeko AG, Popov YA, Rachkov VA, Saylaubekov B, Sokol EA, Tezekbaeva MS, Ulanova II, Zhang FS, Chepigin VI, Chelnokov ML, Eremin AV |date=2024 |website=jinr.ru |publisher=Joint Institute for Nuclear Research |access-date=9 November 2024 |lang=ru}}

| style="text-align:right" | 94

| style="text-align:right" | 132

| 226.03825(22)#

| ≥1 ms

| α

| {{sup|222}}U

| 0+

|

|-id=Plutonium-227

| {{sup|227}}Pu{{cite journal |last1=Yang |first1=H. B. |last2=Gan |first2=Z. G. |last3=Zhang |first3=Z. Y. |last4=Huang |first4=M. H. |last5=Ma |first5=L. |last6=Yang |first6=C. L. |last7=Zhang |first7=M. M. |last8=Tian |first8=Y. L. |last9=Wang |first9=Y. S. |last10=Wang |first10=J. G. |last11=Zhou |first11=H. B. |last12=Hua |first12=W. |last13=Wang |first13=J. Y. |last14=Qiang |first14=Y. H. |last15=Zhao |first15=Z. |last16=Huang |first16=X. Y. |last17=Wen |first17=X. J. |last18=Li |first18=Z. Y. |last19=Zhang |first19=H. T. |last20=Xu |first20=S. Y. |last21=Li |first21=Z. C. |last22=Zhou |first22=H. |last23=Zhang |first23=X. |last24=Zhu |first24=L. |last25=Wang |first25=Z. |last26=Guan |first26=F. |last27=Yang |first27=H. R. |last28=Huang |first28=W. X. |last29=Ren |first29=Z. Z. |last30=Zhou |first30=S. G. |last31=Xu |first31=H. S. |title=α decay of the new isotope Pu 227 |journal=Physical Review C |date=3 October 2024 |volume=110 |issue=4 |doi=10.1103/PhysRevC.110.044302}}

| style="text-align:right" | 94

| style="text-align:right" | 133

| 227.03947(11)#

| {{val|0.78|0.39|0.19|u=s}}

| α

| {{sup|223}}U

| 5/2+#

|

|-id=Plutonium-228

| {{sup|228}}Pu

| style="text-align:right" | 94

| style="text-align:right" | 134

| 228.038763(25)

| 2.1(13) s

| α

| {{sup|224}}U

| 0+

|

|-id=Plutonium-229

| rowspan=3|{{sup|229}}Pu

| rowspan=3 style="text-align:right" | 94

| rowspan=3 style="text-align:right" | 135

| rowspan=3|229.040145(65)

| rowspan=3|91(26) s

| α (~50%)

| {{sup|225}}U

| rowspan=3|3/2+#

| rowspan=3|

|-

| β{{sup|+}} (~50%)

| {{sup|229}}Np

|-

| SF (<7%)

| (various)

|-id=Plutonium-230

| rowspan=2|{{sup|230}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 136

| rowspan=2|230.039648(16)

| rowspan=2|105(10) s

| α (>73%){{cite journal |last1=Wilson |first1=G. L. |last2=Takeyama |first2=M. |last3=Andreyev |first3=A. N. |last4=Andel |first4=B. |last5=Antalic |first5=S. |last6=Catford |first6=W. N. |last7=Ghys |first7=L. |last8=Haba |first8=H. |last9=Heßberger |first9=F. P. |last10=Huang |first10=M. |last11=Kaji |first11=D. |last12=Kalaninova |first12=Z. |last13=Morimoto |first13=K. |last14=Morita |first14=K. |last15=Murakami |first15=M. |last16=Nishio |first16=K. |last17=Orlandi |first17=R. |last18=Smith |first18=A. G. |last19=Tanaka |first19=K. |last20=Wakabayashi |first20=Y. |last21=Yamaki |first21=S. |title=β -delayed fission of Am 230 |journal=Physical Review C |date=13 October 2017 |volume=96 |issue=4 |page=044315 |doi=10.1103/PhysRevC.96.044315 |language=en |issn=2469-9985|doi-access=free }}

| {{sup|226}}U

| rowspan=2|0+

| rowspan=2|

|-

| β{{sup|+}} (<27%)

| {{sup|230}}Np

|-id=Plutonium-231

| rowspan=2|{{sup|231}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 137

| rowspan=2|231.041126(24)

| rowspan=2|8.6(5) min

| β{{sup|+}} (87%)

| {{sup|231}}Np

| rowspan=2|(3/2+)

| rowspan=2|

|-

| α (13%)

| {{sup|227}}U

|-id=Plutonium-232

| rowspan=2|{{sup|232}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 138

| rowspan=2|232.041182(18)

| rowspan=2|33.7(5) min

| EC (77%)

| {{sup|232}}Np

| rowspan=2|0+

| rowspan=2|

|-

| α (23%)

| {{sup|228}}U

|-id=Plutonium-233

| rowspan=2|{{sup|233}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 139

| rowspan=2|233.042997(58)

| rowspan=2|20.9(4) min

| β{{sup|+}} (99.88%)

| {{sup|233}}Np

| rowspan=2|5/2+#

| rowspan=2|

|-

| α (0.12%)

| {{sup|229}}U

|-id=Plutonium-234

| rowspan=2|{{sup|234}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 140

| rowspan=2|234.0433175(73)

| rowspan=2|8.8(1) h

| EC (94%)

| {{sup|234}}Np

| rowspan=2|0+

| rowspan=2|

|-

| α (6%)

| {{sup|230}}U

|-id=Plutonium-235

| rowspan=2|{{sup|235}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 141

| rowspan=2|235.045285(22)

| rowspan=2|25.3(5) min

| β{{sup|+}}

| {{sup|235}}Np

| rowspan=2|(5/2+)

| rowspan=2|

|-

| α (0.0028%)

| {{sup|231}}U

|-id=Plutonium-236

| rowspan=3|{{sup|236}}Pu

| rowspan=3 style="text-align:right" | 94

| rowspan=3 style="text-align:right" | 142

| rowspan=3|236.0460567(19)

| rowspan=3|2.858(8) y

| αTheorized to also undergo β⁺β⁺ decay to ²³⁶U

| {{sup|232}}U

| rowspan=3|0+

| rowspan=3|

|-

| SF (1.9×10{{sup|−7}}%)

| (various)

|-

| CD (2×10{{sup|−12}}%)

| {{sup|208}}Pb
{{sup|28}}Mg

|-id=Plutonium-236m

| style="text-indent:1em" | {{sup|236m}}Pu

| colspan="3" style="text-indent:2em" | 1185.45(15) keV

| 1.2(3) μs

| IT

| {{sup|236}}Pu

| 5−

|

|-id=Plutonium-237

| rowspan=2|{{sup|237}}Pu

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 143

| rowspan=2|237.0484079(18)

| rowspan=2|45.64(4) d

| EC

| {{sup|237}}Np

| rowspan=2|7/2−

| rowspan=2|

|-

| α (0.0042%)

| {{sup|233}}U

|-id=Plutonium-237m1

| style="text-indent:1em" | {{sup|237m1}}Pu

| colspan="3" style="text-indent:2em" | 145.543(8) keV

| 180(20) ms

| IT

| {{sup|237}}Pu

| 1/2+

|

|-id=Plutonium-237m2

| style="text-indent:1em" | {{sup|237m2}}Pu

| colspan="3" style="text-indent:2em" | 2900(250) keV

| 1.1(1) μs

| SF

| (various)

|

|

|-

| rowspan=5|Plutonium-238

| rowspan=5 style="text-align:right" | 94

| rowspan=5 style="text-align:right" | 144

| rowspan=5|238.0495582(12)

| rowspan=5|87.7(1) y

| α

| {{sup|234}}U

| rowspan=5|0+

| rowspan=5|TraceDouble beta decay product of uranium-238

|-

| SF (1.9×10{{sup|−7}}%)

| (various)

|-

| CD (1.4×10{{sup|−14}}%)

| {{sup|206}}Hg
{{sup|32}}Si

|-

| CD (<6×10{{sup|−15}}%)

| {{sup|210}}Pb
{{sup|28}}Mg

|-

| CD (<6×10{{sup|−15}}%)

| {{sup|208}}Pb
{{sup|30}}Mg

|-

| rowspan=2|Plutonium-239fissile nuclideMost useful isotope for nuclear weapons

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 145

| rowspan=2|239.0521616(12)

| rowspan=2|2.411(3)×10⁴ y

| α

| {{sup|235}}U

| rowspan=2|1/2+

| rowspan=2|TraceNeutron capture product of uranium-238

|-

| SF (3.1×10{{sup|−10}}%)

| (various)

|-id=Plutonium-239m1

| style="text-indent:1em" | {{sup|239m1}}Pu

| colspan="3" style="text-indent:2em" | 391.584(3) keV

| 193(4) ns

| IT

| ²³⁹Pu

| 7/2−

|

|-id=Plutonium-239m2

| style="text-indent:1em" | {{sup|239m2}}Pu

| colspan="3" style="text-indent:2em" | 3100(200) keV

| 7.5(10) μs

| SF

| (various)

| (5/2+)

|

|-

| rowspan=3|plutonium-240

| rowspan=3 style="text-align:right" | 94

| rowspan=3 style="text-align:right" | 146

| rowspan=3|240.0538117(12)

| rowspan=3|6.561(7)×10{{sup|3}} y

| α

| {{sup|236}}U

| rowspan=3|0+

| rowspan=3|TraceIntermediate decay product of plutonium-244

|-

| SF (5.796×10{{sup|−6}}%)

| (various)

|-

| CD (<1.3×10{{sup|−11}}%)

| {{sup|206}}Hg
{{sup|34}}Si

|-id=Plutonium-240m

| style="text-indent:1em" | {{sup|240m}}Pu

| colspan="3" style="text-indent:2em" | 1308.74(5) keV

| 165(10) ns

| IT

| ²⁴⁰Pu

| 5−

|

|-

| rowspan=3|plutonium-241

| rowspan=3 style="text-align:right" | 94

| rowspan=3 style="text-align:right" | 147

| rowspan=3|241.0568497(12)

| rowspan=3|14.329(29) y{{refn|group=n|Can undergo Bound-state β⁻ decay with a half-life of 4.2 days when fully ionized{{cite journal |last1=Takahashi |first1=K. |last2=Boyd |first2=R. N. |last3=Mathews |first3=G. J. |last4=Yokoi |first4=K. |title=Bound-state beta decay of highly ionized atoms |journal=Physical Review C |date=1 October 1987 |volume=36 |issue=4 |pages=1522–1528 |doi=10.1103/PhysRevC.36.1522 |url=https://www.researchgate.net/publication/13335547_Bound-state_beta_decay_of_highly_ionized_atoms}}}}

| β{{sup|−}}

| {{sup|241}}Am

| rowspan=3|5/2+

| rowspan=3|

|-

| α (0.00245%)

| {{sup|237}}U

|-

| SF (<2.4×10{{sup|−14}}%)

| (various)

|-id=Plutonium-241m1

| style="text-indent:1em" | {{sup|241m1}}Pu

| colspan="3" style="text-indent:2em" | 161.6853(9) keV

| 0.88(5) μs

| IT

| ²⁴¹Pu

| 1/2+

|

|-id=Plutonium-241m2

| style="text-indent:1em" | {{sup|241m2}}Pu

| colspan="3" style="text-indent:2em" | 2200(200) keV

| 20.5(22) μs

| SF

| (various)

|

|

|-

| rowspan=2|plutonium-242

| rowspan=2 style="text-align:right" | 94

| rowspan=2 style="text-align:right" | 148

| rowspan=2|242.0587410(13)

| rowspan=2|3.75(2)×10{{sup|5}} y

| α

| {{sup|238}}U

| rowspan=2|0+

| rowspan=2|

|-

| SF (5.510×10{{sup|−4}}%)

| (various)

|-id=Plutonium-243

| {{sup|243}}Pu

| style="text-align:right" | 94

| style="text-align:right" | 149

| 243.0620021(27)

| 4.9553(25) h

| β{{sup|−}}

| {{sup|243}}Am

| 7/2+

|

|-id=Plutonium-243m

| style="text-indent:1em" | {{sup|243m}}Pu

| colspan="3" style="text-indent:2em" | 383.64(25) keV

| 330(30) ns

| IT

| ²⁴³Pu

| (1/2+)

|

|-

| rowspan=3|plutonium-244

| rowspan=3 style="text-align:right" | 94

| rowspan=3 style="text-align:right" | 150

| rowspan=3|244.0642044(25)

| rowspan=3|8.13(3)×10{{sup|7}} y

| α (99.88%)

| {{sup|240}}U

| rowspan=3|0+

| rowspan=3|TraceInterstellar, some may also be primordial but such claims are disputed

|-

| SF (0.123%)

| (various)

|-

| Double beta decay (<7.3×10{{sup|−9}}%)

| {{sup|244}}Cm

|-id=Plutonium-244m

| style="text-indent:1em" | {{sup|244m}}Pu

| colspan="3" style="text-indent:2em" | 1216.0(5) keV

| 1.75(12) s

| IT

| ²⁴⁴Pu

| 8−

|

|-id=Plutonium-245

| {{sup|245}}Pu

| style="text-align:right" | 94

| style="text-align:right" | 151

| 245.067825(15)

| 10.5(1) h

| β{{sup|−}}

| {{sup|245}}Am

| (9/2−)

|

|-id=Plutonium-245m1

| style="text-indent:1em" | {{sup|245m1}}Pu

| colspan="3" style="text-indent:2em" | 264.5(3) keV

| 330(20) ns

| IT

| ²⁴⁵Pu

| (5/2+)

|

|-id=Plutonium-245m2

| style="text-indent:1em" | {{sup|245m2}}Pu

| colspan="3" style="text-indent:2em" | 2000(400) keV

| 90(30) ns

| SF

| (various)

|

|

|-id=Plutonium-246

| {{sup|246}}Pu

| style="text-align:right" | 94

| style="text-align:right" | 152

| 246.070204(16)

| 10.84(2) d

| β{{sup|−}}

| {{sup|246}}Am

| 0+

|

|-id=Plutonium-247

| {{sup|247}}Pu

| style="text-align:right" | 94

| style="text-align:right" | 153

| 247.07430(22)#

| 2.27(23) d

| β{{sup|−}}

| {{sup|247}}Am

| 1/2+#

|

{{Isotopes table/footer}}

{{Actinidesvsfissionproducts}}

{{Clear}}

• Plutonium-238 has a half-life of 87.74 years{{cite magazine|last1=Makhijani|first1=Arjun|last2=Seth|first2=Anita|date=July 1997|title=The Use of Weapons Plutonium as Reactor Fuel|url=http://ieer.org/wp/wp-content/uploads/1997/07/no-3.pdf|magazine=Energy and Security|location=Takoma Park, MD|publisher=Institute for Energy and Environmental Research|access-date=4 July 2016}} and emits alpha particles. Pure {{sup|238}}Pu for radioisotope thermoelectric generators that power some spacecraft is produced by neutron capture on neptunium-237 but plutonium from spent nuclear fuel can contain as much as a few percent {{sup|238}}Pu, originating from {{sup|237}}Np, alpha decay of {{sup|242}}Cm, or (n,2n) reactions.
• Plutonium-239 has half-life 24,100 years. {{sup|239}}Pu and {{sup|241}}Pu are fissile; meaning their nuclei can split by being bombarded by slow thermal neutrons, releasing energy, gamma radiation and more neutrons. It can therefore sustain a nuclear chain reaction, leading to applications in nuclear weapons and nuclear reactors. {{sup|239}}Pu is synthesized by irradiating uranium-238 with neutrons in a nuclear reactor, then recovered via nuclear reprocessing of the fuel. Further neutron capture produces successively heavier isotopes.
• Plutonium-240 has a high rate of spontaneous fission, raising the background neutron radiation of plutonium. Plutonium is graded by proportion of {{sup|240}}Pu: weapons grade (<7%), fuel grade (7–19%) and reactor grade (>19%). Lower grades are less suited for bombs and thermal reactors but can fuel fast reactors.
• Plutonium-241 is fissile, but beta decays with a half-life of 14 years to americium-241.
• Plutonium-242 is not fissile, nor very fertile (requiring 3 more neutron captures to become fissile); and has a low neutron capture cross section, and a longer half-life than any of the lighter isotopes.
• Plutonium-244 is the most stable isotope of plutonium, with a half-life of about 80 million years. It is not significantly produced in nuclear reactors because {{sup|243}}Pu has a short half-life, but some is produced in nuclear explosions. {{sup|244}}Pu has been found in interstellar space{{cite journal |last1=Wallner |first1=A. |last2=Faestermann |first2=T. |last3=Feige |first3=J. |last4=Feldstein |first4=C. |last5=Knie |first5=K. |last6=Korschinek |first6=G. |last7=Kutschera |first7=W. |last8=Ofan |first8=A. |last9=Paul |first9=M. |last10=Quinto |first10=F. |last11=Rugel |first11=G. |last12=Steier |first12=P. |title=Abundance of live 244Pu in deep-sea reservoirs on Earth points to rarity of actinide nucleosynthesis|journal=Nature Communications |volume=6 |year=2015 |pages=5956 |issn=2041-1723 |doi=10.1038/ncomms6956 |pmid=25601158 |pmc=4309418 |arxiv=1509.08054 |bibcode=2015NatCo...6.5956W}} and has the second longest half-life of any non-primordial radioisotope.

File:Plutonium pellet.jpgs.]]

File:Sasahara.svg flow between {{sup|238}}Pu and {{sup|244}}Cm in LWR.{{cite journal|title=Neutron and Gamma Ray Source Evaluation of LWR High Burn-up UO2 and MOX Spent Fuels |journal=Journal of Nuclear Science and Technology |volume=41 |issue=4 |pages=448–456 |date=April 2004 |doi=10.3327/jnst.41.448 |last1=Sasahara |first1=Akihiro |last2=Matsumura |first2=Tetsuo |last3=Nicolaou |first3=Giorgos |last4=Papaioannou |first4=Dimitri |doi-access=free }}
Transmutation speed not shown and varies greatly by nuclide. {{sup|245}}Cm–{{sup|248}}Cm are long-lived with negligible decay.]]

{{sup|239}}Pu, a fissile isotope that is the second most used nuclear fuel in nuclear reactors after uranium-235, and the most used fuel in the fission portion of nuclear weapons, is produced from uranium-238 by neutron capture followed by two beta decays.

{{sup|240}}Pu, {{sup|241}}Pu, and {{sup|242}}Pu are produced by further neutron capture. The odd-mass isotopes {{sup|239}}Pu and {{sup|241}}Pu have about a 3/4 chance of undergoing fission on capture of a thermal neutron and about a 1/4 chance of retaining the neutron and becoming the next heavier isotope. The even-mass isotopes are fertile but not fissile and also have a lower probability (cross section) of neutron capture; therefore, they tend to accumulate in nuclear fuel used in a thermal reactor, the design of nearly all nuclear power plants today. In plutonium that has been used a second time in thermal reactors in MOX fuel, {{sup|240}}Pu may even be the most common isotope. All plutonium isotopes and other actinides, however, are fissionable with fast neutrons. {{sup|240}}Pu does have a moderate thermal neutron absorption cross section, so that {{sup|241}}Pu production in a thermal reactor becomes a significant fraction as large as {{sup|239}}Pu production.

{{sup|241}}Pu has a half-life of 14 years, and has slightly higher thermal neutron cross sections than {{sup|239}}Pu for both fission and absorption. While nuclear fuel is being used in a reactor, a {{sup|241}}Pu nucleus is much more likely to fission or to capture a neutron than to decay. {{sup|241}}Pu accounts for a significant portion of fissions in thermal reactor fuel that has been used for some time. However, in spent nuclear fuel that does not quickly undergo nuclear reprocessing but instead is cooled for years after use, much or most of the {{sup|241}}Pu will beta decay to americium-241, one of the minor actinides, a strong alpha emitter, and difficult to use in thermal reactors.

{{sup|242}}Pu has a particularly low cross section for thermal neutron capture; and it takes three neutron absorptions to become another fissile isotope (either curium-245 or {{sup|241}}Pu) and fission. Even then, there is a chance either of those two fissile isotopes will fail to fission but instead absorb a fourth neutron, becoming curium-246 (on the way to even heavier actinides like californium, which is a neutron emitter by spontaneous fission and difficult to handle) or becoming {{sup|242}}Pu again; so the mean number of neutrons absorbed before fission is even higher than 3. Therefore, {{sup|242}}Pu is particularly unsuited to recycling in a thermal reactor and would be better used in a fast reactor where it can be fissioned directly. However, {{sup|242}}Pu's low cross section means that relatively little of it will be transmuted during one cycle in a thermal reactor. {{sup|242}}Pu's half-life is about 15 times as long as {{sup|239}}Pu's half-life; therefore, it is 1/15 as radioactive and not one of the larger contributors to nuclear waste radioactivity.

{{sup|242}}Pu's gamma ray emissions are also weaker than those of the other isotopes.{{cite web|url=http://www.wmsym.org/archives/2001/21B/21B-18.pdf|title=Plutonium Isotopic Results of Known Samples Using the Snap Gamma Spectroscopy Analysis Code and the Robwin Spectrum Fitting Routine|access-date=2013-03-15|archive-date=2017-08-13|archive-url=https://web.archive.org/web/20170813191754/http://www.wmsym.org/archives/2001/21B/21B-18.pdf|url-status=dead}}

{{sup|243}}Pu has a half-life of only 5 hours, beta decaying to americium-243. Because {{sup|243}}Pu has little opportunity to capture an additional neutron before decay, the nuclear fuel cycle does not produce the long-lived {{sup|244}}Pu in significant quantity.

{{sup|238}}Pu is not normally produced in as large quantity by the nuclear fuel cycle, but some is produced from neptunium-237 by neutron capture (this reaction can also be used with purified neptunium to produce {{sup|238}}Pu relatively free of other plutonium isotopes for use in radioisotope thermoelectric generators), by the (n,2n) reaction of fast neutrons on {{sup|239}}Pu, or by alpha decay of curium-242, which is produced by neutron capture of {{sup|241}}Am. It has significant thermal neutron cross section for fission, but is more likely to capture a neutron and become {{sup|239}}Pu.

==Manufacture==

The fission cross section for {{sup|239}}Pu is 747.9 barns for thermal neutrons, while the activation cross section is 270.7 barns (the ratio approximates to 11 fissions for every 4 neutron captures). The higher plutonium isotopes are created when the uranium fuel is used for a long time. For high burnup used fuel, the concentrations of the higher plutonium isotopes will be higher than the low burnup fuel that is reprocessed to obtain weapons grade plutonium.

{{Main|Plutonium-239}}

File:Plutonium ring.jpg.]]

{{sup|239}}Pu is one of the three fissile materials used for the production of nuclear weapons and in some nuclear reactors as a source of energy. The other fissile materials are uranium-235 and uranium-233. {{sup|239}}Pu is virtually nonexistent in nature. It is made by bombarding uranium-238 with neutrons. Uranium-238 is present in quantity in most reactor fuel; hence {{sup|239}}Pu is continuously made in these reactors. Since {{sup|239}}Pu can itself be split by neutrons to release energy, {{sup|239}}Pu provides a portion of the energy generation in a nuclear reactor.

{{Main|Plutonium-238}}

There are small amounts of {{sup|238}}Pu in the plutonium from usual reactors. However, isotopic separation would be quite expensive compared to another method: when {{sup|235}}U captures a neutron, it is converted to an excited state of {{sup|236}}U. Some of the excited {{sup|236}}U nuclei undergo fission, but some decay to the ground state of {{sup|236}}U by emitting gamma radiation. Further neutron capture creates {{sup|237}}U; which, with a half-life of 7 days, decays to {{sup|237}}Np. Since nearly all neptunium is produced in this way or consists of isotopes that decay quickly, one gets nearly pure {{sup|237}}Np. After chemical separation of neptunium, {{sup|237}}Np is again irradiated by reactor neutrons to be converted to {{sup|238}}Np, which decays to {{sup|238}}Pu with a half-life of 2 days.

{{sup|240}}Pu undergoes spontaneous fission at a small but significant rate ({{val|5.8|e=-6}}%).{{NUBASE2020|ref}} The presence of {{sup|240}}Pu limits the plutonium's use in a nuclear bomb, because a neutron from spontaneous fission starts the chain reaction prematurely, causing an early release of energy that disperses the core before full implosion is reached. This prevents most of the core from participation in the chain reaction and reduces the bomb's yield.

Plutonium consisting of more than about 90% {{sup|239}}Pu is called weapons-grade plutonium; plutonium from spent nuclear fuel from commercial power reactors generally contains at least 20% {{sup|240}}Pu and is called reactor-grade plutonium. However, modern nuclear weapons use fusion boosting, which mitigates the predetonation problem; if the pit can generate a nuclear weapon yield of even a fraction of a kiloton, which is enough to start deuterium–tritium fusion, the resulting burst of neutrons will fission enough plutonium to ensure a yield of tens of kilotons.

Contamination due to {{sup|240}}Pu is the reason plutonium weapons must use the implosion method. Theoretically, pure {{sup|239}}Pu could be used in a gun-type bomb, but achieving this level of purity is prohibitively difficult. {{sup|240}}Pu contamination has proven a mixed blessing. While it created delays and headaches during the Manhattan Project because of the need to develop implosion technology, those same difficulties are a barrier to nuclear proliferation. Implosion bombs are also inherently more efficient and less prone to accidental detonation than are gun-type bombs.

{{reflist|group=note}}

• Isotope masses from:
• {{NUBASE 2003 |ref=none}}
• Half-life, spin, and isomer data selected from the following sources.
• {{NUBASE 2003 |ref=none}}
• {{NNDC |ref=none}}
• {{CRC85|chapter=11 |ref=none}}

{{Reflist}}

• {{Cite book |url=https://www-nds.iaea.org/publications/indc/indc_usa_0085_II.pdf |title=Proceedings of the conference on nuclear data evaluation methods and procedures. BNL-NCS 51363. |date=1981 |publisher=Brookhaven National Laboratory |editor-last=Magurno |editor-first=B. A. |volume=II |location=Upton |access-date=August 6, 2014 |editor-last2=Pearlstein |editor-first2=S. |archive-url=https://web.archive.org/web/20210308125416/https://www-nds.iaea.org/publications/indc/indc_usa_0085_II.pdf |archive-date=March 8, 2021 |url-status=live}}
• {{Cite book |last1=Miner |first1=William N. |title=The Encyclopedia of the Chemical Elements |last2=Schonfeld, Fred W. |publisher=Reinhold Book Corporation |year=1968 |editor-last=Clifford A. Hampel |location=New York (NY) |pages=[https://archive.org/details/encyclopediaofch00hamp/page/540 540–546] |chapter=Plutonium |lccn=68029938 |ref=CITEREFMiner1968 |chapter-url=https://archive.org/details/encyclopediaofch00hamp |chapter-url-access=registration}}

{{Navbox element isotopes}}

{{Isotopes of plutonium}}

{{Authority control}}

Category:Plutonium

Plutonium