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Isotopes of plutonium
open-in-new
<h2 id="list-of-isotopes">List of isotopes</h2> <table><tbody><tr><th rowspan="2">Nuclide<a class="footnote-ref" id="fnref:2" href="#fn:2"><sup>2</sup></a></th><th rowspan="1"><a href="/facts/Atomic_number/bgAr581S"><i>Z</i></a></th><th rowspan="1"><a href="/facts/Neutron_number/eNtwGnVL"><i>N</i></a></th><th rowspan="1"><a href="/facts/Atomic_mass/J1FJY9MV">Isotopic mass</a> (<a href="/facts/Dalton_(unit)/IMATU3vf">Da</a>)<a class="footnote-ref" id="fnref:3" href="#fn:3"><sup>3</sup></a><a class="footnote-ref" id="fnref:4" href="#fn:4"><sup>4</sup></a><a class="footnote-ref" id="fnref:5" href="#fn:5"><sup>5</sup></a></th><th rowspan="2"><a href="/facts/Half-life/kGVH8BAB">Half-life</a><a class="footnote-ref" id="fnref:6" href="#fn:6"><sup>6</sup></a></th><th rowspan="2"><a href="/facts/Decay_mode/Ya6FVjt4">Decaymode</a><a class="footnote-ref" id="fnref:7" href="#fn:7"><sup>7</sup></a><a class="footnote-ref" id="fnref:8" href="#fn:8"><sup>8</sup></a></th><th rowspan="2"><a href="/facts/Decay_product/hT0obfLv">Daughterisotope</a><a class="footnote-ref" id="fnref:9" href="#fn:9"><sup>9</sup></a><a class="footnote-ref" id="fnref:10" href="#fn:10"><sup>10</sup></a></th><th rowspan="2"><a href="/facts/Spin_(particle_physics)/4Jvp7e8P">Spin</a> and<a href="/facts/Parity_(physics)/emSbJ4hD">parity</a><a class="footnote-ref" id="fnref:11" href="#fn:11"><sup>11</sup></a><a class="footnote-ref" id="fnref:12" href="#fn:12"><sup>12</sup></a><a class="footnote-ref" id="fnref:13" href="#fn:13"><sup>13</sup></a></th><th rowspan="2"><a href="/facts/Natural_abundance/dGjaAwc9">Isotopicabundance</a></th></tr><tr><th colspan="3">Excitation energy</th></tr><tr><td>226Pu<a class="footnote-ref" id="fnref:14" href="#fn:14"><sup>14</sup></a></td><td>94</td><td>132</td><td>226.03825(22)#</td><td>≥1 ms</td><td>α</td><td>222U</td><td>0+</td><td></td></tr><tr><td>227Pu<a class="footnote-ref" id="fnref:15" href="#fn:15"><sup>15</sup></a></td><td>94</td><td>133</td><td>227.03947(11)#</td><td>0.78+0.39−0.19 s</td><td>α</td><td>223U</td><td>5/2+#</td><td></td></tr><tr><td>228Pu</td><td>94</td><td>134</td><td>228.038763(25)</td><td>2.1(13) s</td><td>α</td><td>224U</td><td>0+</td><td></td></tr><tr><td rowspan="3">229Pu</td><td rowspan="3">94</td><td rowspan="3">135</td><td rowspan="3">229.040145(65)</td><td rowspan="3">91(26) s</td><td>α (~50%)</td><td>225U</td><td rowspan="3">3/2+#</td><td rowspan="3"></td></tr><tr><td>β+ (~50%)</td><td>229Np</td></tr><tr><td><a href="/facts/Spontaneous_fission/0QuJoVKI">SF</a> (<7%)</td><td>(various)</td></tr><tr><td rowspan="2">230Pu</td><td rowspan="2">94</td><td rowspan="2">136</td><td rowspan="2">230.039648(16)</td><td rowspan="2">105(10) s</td><td>α (>73%)<a class="footnote-ref" id="fnref:16" href="#fn:16"><sup>16</sup></a></td><td>226U</td><td rowspan="2">0+</td><td rowspan="2"></td></tr><tr><td>β+ (<27%)</td><td>230Np</td></tr><tr><td rowspan="2">231Pu</td><td rowspan="2">94</td><td rowspan="2">137</td><td rowspan="2">231.041126(24)</td><td rowspan="2">8.6(5) min</td><td>β+ (87%)</td><td>231Np</td><td rowspan="2">(3/2+)</td><td rowspan="2"></td></tr><tr><td>α (13%)</td><td>227U</td></tr><tr><td rowspan="2">232Pu</td><td rowspan="2">94</td><td rowspan="2">138</td><td rowspan="2">232.041182(18)</td><td rowspan="2">33.7(5) min</td><td><a href="/facts/Electron_capture/EIccoV1u">EC</a> (77%)</td><td>232Np</td><td rowspan="2">0+</td><td rowspan="2"></td></tr><tr><td>α (23%)</td><td>228U</td></tr><tr><td rowspan="2">233Pu</td><td rowspan="2">94</td><td rowspan="2">139</td><td rowspan="2">233.042997(58)</td><td rowspan="2">20.9(4) min</td><td>β+ (99.88%)</td><td>233Np</td><td rowspan="2">5/2+#</td><td rowspan="2"></td></tr><tr><td>α (0.12%)</td><td>229U</td></tr><tr><td rowspan="2">234Pu</td><td rowspan="2">94</td><td rowspan="2">140</td><td rowspan="2">234.0433175(73)</td><td rowspan="2">8.8(1) h</td><td>EC (94%)</td><td>234Np</td><td rowspan="2">0+</td><td rowspan="2"></td></tr><tr><td>α (6%)</td><td>230U</td></tr><tr><td rowspan="2">235Pu</td><td rowspan="2">94</td><td rowspan="2">141</td><td rowspan="2">235.045285(22)</td><td rowspan="2">25.3(5) min</td><td>β+</td><td>235Np</td><td rowspan="2">(5/2+)</td><td rowspan="2"></td></tr><tr><td>α (0.0028%)</td><td>231U</td></tr><tr><td rowspan="3">236Pu</td><td rowspan="3">94</td><td rowspan="3">142</td><td rowspan="3">236.0460567(19)</td><td rowspan="3">2.858(8) y</td><td>α<a class="footnote-ref" id="fnref:17" href="#fn:17"><sup>17</sup></a></td><td>232U</td><td rowspan="3">0+</td><td rowspan="3"></td></tr><tr><td>SF (1.9×10−7%)</td><td>(various)</td></tr><tr><td><a href="/facts/Cluster_decay/sIelGo3t">CD</a> (2×10−12%)</td><td>208Pb28Mg</td></tr><tr><td>236mPu</td><td colspan="3">1185.45(15) keV</td><td>1.2(3) μs</td><td><a href="/facts/Isomeric_transition/L8DHcqnk">IT</a></td><td>236Pu</td><td>5−</td><td></td></tr><tr><td rowspan="2">237Pu</td><td rowspan="2">94</td><td rowspan="2">143</td><td rowspan="2">237.0484079(18)</td><td rowspan="2">45.64(4) d</td><td>EC</td><td>237Np</td><td rowspan="2">7/2−</td><td rowspan="2"></td></tr><tr><td>α (0.0042%)</td><td>233U</td></tr><tr><td>237m1Pu</td><td colspan="3">145.543(8) keV</td><td>180(20) ms</td><td>IT</td><td>237Pu</td><td>1/2+</td><td></td></tr><tr><td>237m2Pu</td><td colspan="3">2900(250) keV</td><td>1.1(1) μs</td><td>SF</td><td>(various)</td><td></td><td></td></tr><tr><td rowspan="5"><a href="/facts/Plutonium-238/JzY7TPFE">238Pu</a></td><td rowspan="5">94</td><td rowspan="5">144</td><td rowspan="5">238.0495582(12)</td><td rowspan="5">87.7(1) y</td><td>α</td><td>234U</td><td rowspan="5">0+</td><td rowspan="5">Trace<a class="footnote-ref" id="fnref:18" href="#fn:18"><sup>18</sup></a></td></tr><tr><td>SF (1.9×10−7%)</td><td>(various)</td></tr><tr><td>CD (1.4×10−14%)</td><td>206Hg32Si</td></tr><tr><td>CD (<6×10−15%)</td><td>210Pb28Mg</td></tr><tr><td>CD (<6×10−15%)</td><td>208Pb30Mg</td></tr><tr><td rowspan="2"><a href="/facts/Plutonium-239/eRobTXos">239Pu</a><a class="footnote-ref" id="fnref:19" href="#fn:19"><sup>19</sup></a><a class="footnote-ref" id="fnref:20" href="#fn:20"><sup>20</sup></a></td><td rowspan="2">94</td><td rowspan="2">145</td><td rowspan="2">239.0521616(12)</td><td rowspan="2">2.411(3)×104 y</td><td>α</td><td><i>235U</i></td><td rowspan="2">1/2+</td><td rowspan="2">Trace<a class="footnote-ref" id="fnref:21" href="#fn:21"><sup>21</sup></a></td></tr><tr><td>SF (3.1×10−10%)</td><td>(various)</td></tr><tr><td>239m1Pu</td><td colspan="3">391.584(3) keV</td><td>193(4) ns</td><td>IT</td><td>239Pu</td><td>7/2−</td><td></td></tr><tr><td>239m2Pu</td><td colspan="3">3100(200) keV</td><td>7.5(10) μs</td><td>SF</td><td>(various)</td><td>(5/2+)</td><td></td></tr><tr><td rowspan="3"><a href="/facts/Plutonium-240/kIWwdLkI">240Pu</a></td><td rowspan="3">94</td><td rowspan="3">146</td><td rowspan="3">240.0538117(12)</td><td rowspan="3">6.561(7)×103 y</td><td>α</td><td>236U</td><td rowspan="3">0+</td><td rowspan="3">Trace<a class="footnote-ref" id="fnref:22" href="#fn:22"><sup>22</sup></a></td></tr><tr><td>SF (5.796×10−6%)</td><td>(various)</td></tr><tr><td>CD (<1.3×10−11%)</td><td>206Hg34Si</td></tr><tr><td>240mPu</td><td colspan="3">1308.74(5) keV</td><td>165(10) ns</td><td>IT</td><td>240Pu</td><td>5−</td><td></td></tr><tr><td rowspan="3"><a href="/facts/Plutonium-241/vUyJGFrs">241Pu</a><a class="footnote-ref" id="fnref:23" href="#fn:23"><sup>23</sup></a></td><td rowspan="3">94</td><td rowspan="3">147</td><td rowspan="3">241.0568497(12)</td><td rowspan="3">14.329(29) y<a class="footnote-ref" id="fnref:24" href="#fn:24"><sup>24</sup></a></td><td>β−</td><td>241Am</td><td rowspan="3">5/2+</td><td rowspan="3"></td></tr><tr><td>α (0.00245%)</td><td>237U</td></tr><tr><td>SF (<2.4×10−14%)</td><td>(various)</td></tr><tr><td>241m1Pu</td><td colspan="3">161.6853(9) keV</td><td>0.88(5) μs</td><td>IT</td><td>241Pu</td><td>1/2+</td><td></td></tr><tr><td>241m2Pu</td><td colspan="3">2200(200) keV</td><td>20.5(22) μs</td><td>SF</td><td>(various)</td><td></td><td></td></tr><tr><td rowspan="2"><a href="/facts/Plutonium-242/o1fg0sBh">242Pu</a></td><td rowspan="2">94</td><td rowspan="2">148</td><td rowspan="2">242.0587410(13)</td><td rowspan="2">3.75(2)×105 y</td><td>α</td><td><i>238U</i></td><td rowspan="2">0+</td><td rowspan="2"></td></tr><tr><td>SF (5.510×10−4%)</td><td>(various)</td></tr><tr><td>243Pu<a class="footnote-ref" id="fnref:25" href="#fn:25"><sup>25</sup></a></td><td>94</td><td>149</td><td>243.0620021(27)</td><td>4.9553(25) h</td><td>β−</td><td>243Am</td><td>7/2+</td><td></td></tr><tr><td>243mPu</td><td colspan="3">383.64(25) keV</td><td>330(30) ns</td><td>IT</td><td>243Pu</td><td>(1/2+)</td><td></td></tr><tr><td rowspan="3"><a href="/facts/Plutonium-244/XGtUVghF">244Pu</a></td><td rowspan="3">94</td><td rowspan="3">150</td><td rowspan="3">244.0642044(25)</td><td rowspan="3">8.13(3)×107 y</td><td>α (99.88%)</td><td>240U</td><td rowspan="3">0+</td><td rowspan="3">Trace<a class="footnote-ref" id="fnref:26" href="#fn:26"><sup>26</sup></a></td></tr><tr><td>SF (0.123%)</td><td>(various)</td></tr><tr><td><a href="/facts/Double_beta_decay/ILmpbfqS">β−β−</a> (<7.3×10−9%)</td><td>244Cm</td></tr><tr><td>244mPu</td><td colspan="3">1216.0(5) keV</td><td>1.75(12) s</td><td>IT</td><td>244Pu</td><td>8−</td><td></td></tr><tr><td>245Pu</td><td>94</td><td>151</td><td>245.067825(15)</td><td>10.5(1) h</td><td>β−</td><td>245Am</td><td>(9/2−)</td><td></td></tr><tr><td>245m1Pu</td><td colspan="3">264.5(3) keV</td><td>330(20) ns</td><td>IT</td><td>245Pu</td><td>(5/2+)</td><td></td></tr><tr><td>245m2Pu</td><td colspan="3">2000(400) keV</td><td>90(30) ns</td><td>SF</td><td>(various)</td><td></td><td></td></tr><tr><td>246Pu</td><td>94</td><td>152</td><td>246.070204(16)</td><td>10.84(2) d</td><td>β−</td><td>246Am</td><td>0+</td><td></td></tr><tr><td>247Pu</td><td>94</td><td>153</td><td>247.07430(22)#</td><td>2.27(23) d</td><td>β−</td><td>247Am</td><td>1/2+#</td><td></td></tr><tr><th colspan="20"><i>This table header & footer:</i> <ul><li>view</li></ul></th></tr></tbody></table> <h2 id="actinides-vs-fission-products">Actinides vs fission products</h2> <table><tbody><tr><th colspan="9">Actinides and fission products by half-life <ul><li>v</li><li>t</li><li>e</li></ul></th></tr><tr><th colspan="4"><a href="/facts/Actinide/kHC4lxJV">Actinides</a><a class="footnote-ref" id="fnref:27" href="#fn:27"><sup>27</sup></a> by <a href="/facts/Decay_chain/JvTwPNBn">decay chain</a></th><th rowspan="2"><a href="/facts/Half-life/kGVH8BAB">Half-life</a> range (<a href="/facts/Year/51V242hh">a</a>)</th><th colspan="4"><a href="/facts/Fission_product/xJd9MXXH">Fission products</a> of <a href="/facts/Uranium-235/pe0RznDM">235U</a> by <a href="/facts/Fission_product_yield/5t9htHpQ">yield</a><a class="footnote-ref" id="fnref:28" href="#fn:28"><sup>28</sup></a></th></tr><tr><th><a href="/facts/Thorium_series/JvTwPNBn">4<i>n</i></a></th><th><a href="/facts/Neptunium_series/JvTwPNBn">4<i>n</i> + 1</a></th><th><a href="/facts/Uranium_series/JvTwPNBn">4<i>n</i> + 2</a></th><th><a href="/facts/Actinium_series/JvTwPNBn">4<i>n</i> + 3</a></th><th>4.5–7%</th><th>0.04–1.25%</th><th><0.001%</th></tr><tr><td><a href="/facts/Radium-228/T0SlGtRH">228</a>Ra№</td><td></td><td></td><td></td><th><a href="/facts/Medium-lived_fission_product/wxe6qNIp">4–6 a</a></th><td></td><td><a href="/facts/Europium-155/IUWzfhMI">155</a>Euþ</td><td></td></tr><tr><td><a href="/facts/Berkelium-248/RnvnlKK4">248</a>Bk<a class="footnote-ref" id="fnref:29" href="#fn:29"><sup>29</sup></a></td><td></td><td></td><td></td><th><a href="/facts/Medium-lived_fission_product/wxe6qNIp">> 9 a</a></th><td></td><td></td><td></td></tr><tr><td><a href="/facts/Curium-244/WnMh6VLE">244</a>Cmƒ</td><td><a href="/facts/Plutonium-241/vUyJGFrs">241</a>Puƒ</td><td><a href="/facts/Californium-250/tX06MlFX">250</a>Cf</td><td><a href="/facts/Actinium-227/vnv59EsB">227</a>Ac№</td><th><a href="/facts/Medium-lived_fission_product/wxe6qNIp">10–29 a</a></th><td><a href="/facts/Strontium-90/VJNoC5eR">90</a>Sr</td><td><a href="/facts/Krypton-85/c32MkhnV">85</a>Kr</td><td><a href="/facts/Cadmium-113m/2F42oNDz">113m</a>Cdþ</td></tr><tr><td><a href="/facts/Uranium-232/9sPn8oCm">232</a>Uƒ</td><td></td><td><a href="/facts/Plutonium-238/JzY7TPFE">238</a>Puƒ</td><td><a href="/facts/Curium-243/WnMh6VLE">243</a>Cmƒ</td><th><a href="/facts/Medium-lived_fission_product/wxe6qNIp">29–97 a</a></th><td><a href="/facts/Cs-137/NrY5Tb6j">137</a>Cs</td><td><a href="/facts/Samarium-151/e5wQw5B0">151</a>Smþ</td><td><a href="/facts/Tin-121m/C3yupbqu">121m</a>Sn</td></tr><tr><td></td><td><a href="/facts/Californium-249/tX06MlFX">249</a>Cfƒ</td><td><a href="/facts/Americium-242m/aqoWt39B">242m</a>Amƒ</td><td></td><th>141–351 a</th><td rowspan="7" colspan="3"><p>No fission products have a half-lifein the range of 100 a–210 ka ...</p></td></tr><tr><td></td><td><a href="/facts/Americium-241/HnXXm1nx">241</a>Amƒ</td><td></td><td><a href="/facts/Californium-251/tX06MlFX">251</a>Cfƒ<a class="footnote-ref" id="fnref:30" href="#fn:30"><sup>30</sup></a></td><th>430–900 a</th></tr><tr><td></td><td></td><td><a href="/facts/Radium-226/T0SlGtRH">226</a>Ra№</td><td><a href="/facts/Berkelium-247/RnvnlKK4">247</a>Bk</td><th>1.3–1.6 ka</th></tr><tr><td><a href="/facts/Plutonium-240/kIWwdLkI">240</a>Pu</td><td><a href="/facts/Thorium-229/lRb3opzg">229</a>Th</td><td><a href="/facts/Curium-246/WnMh6VLE">246</a>Cmƒ</td><td><a href="/facts/Americium-243/aqoWt39B">243</a>Amƒ</td><th>4.7–7.4 ka</th></tr><tr><td></td><td><a href="/facts/Curium-245/WnMh6VLE">245</a>Cmƒ</td><td><a href="/facts/Curium-250/WnMh6VLE">250</a>Cm</td><td></td><th>8.3–8.5 ka</th></tr><tr><td></td><td></td><td></td><td><a href="/facts/Plutonium-239/eRobTXos">239</a>Puƒ</td><th>24.1 ka</th></tr><tr><td></td><td></td><td><a href="/facts/Thorium-230/lRb3opzg">230</a>Th№</td><td><a href="/facts/Protactinium-231/AVGw4A8U">231</a>Pa№</td><th>32–76 ka</th></tr><tr><td><a href="/facts/Neptunium-236/X3bPWwX1">236</a>Npƒ</td><td><a href="/facts/Uranium-233/a6sMrk07">233</a>Uƒ</td><td><a href="/facts/Uranium-234/nKrs059u">234</a>U№</td><td></td><th><a href="/facts/Long-lived_fission_product/wxe6qNIp">150–250 ka</a></th><td><a href="/facts/Technetium-99/0w2EE0G2">99</a>Tc₡</td><td><a href="/facts/Tin-126/C3yupbqu">126</a>Sn</td></tr><tr><td><a href="/facts/Curium-248/WnMh6VLE">248</a>Cm</td><td></td><td><a href="/facts/Plutonium-242/o1fg0sBh">242</a>Pu</td><td></td><th><a href="/facts/Long-lived_fission_product/wxe6qNIp">327–375 ka</a></th><td></td><td><a href="/facts/Selenium-79/3TDcPNTR">79</a>Se₡</td></tr><tr><td></td><td></td><td></td><td></td><th><a href="/facts/Long-lived_fission_product/wxe6qNIp">1.33 Ma</a></th><td><a href="/facts/Caesium-135/m5AYV9tp">135</a>Cs₡</td></tr><tr><td></td><td><a href="/facts/Neptunium-237/X3bPWwX1">237</a>Npƒ</td><td></td><td></td><th><a href="/facts/Long-lived_fission_product/wxe6qNIp">1.61–6.5 Ma</a></th><td><a href="/facts/Zirconium-93/NzDqkTRf">93</a>Zr</td><td><a href="/facts/Palladium-107/deN3NNeY">107</a>Pd</td></tr><tr><td><a href="/facts/Uranium-236/1JepNWSb">236</a>U</td><td></td><td></td><td><a href="/facts/Curium-247/WnMh6VLE">247</a>Cmƒ</td><th><a href="/facts/Long-lived_fission_product/wxe6qNIp">15–24 Ma</a></th><td></td><td><a href="/facts/Iodine-129/oJDlGf5H">129</a>I₡</td></tr><tr><td><a href="/facts/Plutonium-244/XGtUVghF">244</a>Pu</td><td></td><td></td><td></td><th>80 Ma</th><td colspan="3" rowspan="2"><p>... nor beyond 15.7 Ma<a class="footnote-ref" id="fnref:31" href="#fn:31"><sup>31</sup></a></p></td></tr><tr><td><a href="/facts/Thorium-232/lRb3opzg">232</a>Th№</td><td></td><td><a href="/facts/Uranium-238/QhcHm6q8">238</a>U№</td><td><a href="/facts/Uranium-235/pe0RznDM">235</a>Uƒ№</td><th>0.7–14.1 Ga</th></tr><tr><td colspan="9"><ul><li>₡, has thermal <a href="/facts/Neutron_capture/elsFpM12">neutron capture</a> cross section in the range of 8–50 barns</li><li>ƒ, <a href="/facts/Fissile/XJR9qoxW">fissile</a></li><li>№, primarily a <a href="/facts/Naturally_occurring_radioactive_material/oUbIxWlg">naturally occurring radioactive material</a> (NORM)</li><li>þ, <a href="/facts/Neutron_poison/bkruR3yz">neutron poison</a> (thermal neutron capture cross section greater than 3k barns)</li></ul></td></tr></tbody></table> <h2 id="notable-isotopes">Notable isotopes</h2> <ul><li><a href="/facts/Plutonium-238/JzY7TPFE">Plutonium-238</a> has a half-life of 87.74 years<a class="footnote-ref" id="fnref:32" href="#fn:32"><sup>32</sup></a> and emits <a href="/facts/Alpha_particle/dzNMs9WP">alpha particles</a>. Pure 238Pu for <a href="/facts/Radioisotope_thermoelectric_generator/Tsjjvp5h">radioisotope thermoelectric generators</a> that power some <a href="/facts/Spacecraft/YQqQaUw0">spacecraft</a> is produced by neutron capture on <a href="/facts/Neptunium-237/X3bPWwX1">neptunium-237</a> but plutonium from <a href="/facts/Spent_nuclear_fuel/jWDWvJ6d">spent nuclear fuel</a> can contain as much as a few percent 238Pu, originating from 237Np, <a href="/facts/Alpha_decay/rCsHNIUE">alpha decay</a> of 242Cm, or (n,2n) reactions.</li> <li><a href="/facts/Plutonium-239/eRobTXos">Plutonium-239</a> has half-life 24,100 years. 239Pu and 241Pu are <a href="/facts/Fissile/XJR9qoxW">fissile</a>; meaning their nuclei can <a href="/facts/Nuclear_fission/LfkIylvm">split</a> by being bombarded by <a href="/facts/Neutron_temperature/UMKR4XgJ">slow</a> thermal neutrons, releasing energy, <a href="/facts/Gamma_radiation/5Drf913J">gamma radiation</a> and <a href="/facts/Neutron_radiation/LVJhCcwL">more neutrons</a>. It can therefore sustain a <a href="/facts/Nuclear_chain_reaction/3l0lHBM4">nuclear chain reaction</a>, leading to applications in <a href="/facts/Nuclear_weapon/QVdBcMdm">nuclear weapons</a> and <a href="/facts/Nuclear_reactor/8xqjIbge">nuclear reactors</a>. 239Pu is synthesized by irradiating <a href="/facts/Uranium-238/QhcHm6q8">uranium-238</a> with neutrons in a nuclear reactor, then recovered via <a href="/facts/Nuclear_reprocessing/aTMUoYaW">nuclear reprocessing</a> of the fuel. Further <a href="/facts/Neutron_capture/elsFpM12">neutron capture</a> produces successively heavier isotopes.</li> <li><a href="/facts/Plutonium-240/kIWwdLkI">Plutonium-240</a> has a high rate of spontaneous fission, raising the background <a href="/facts/Neutron_radiation/LVJhCcwL">neutron radiation</a> of plutonium. Plutonium is graded by proportion of 240Pu: <a href="/facts/Weapons_grade/o2S0c30F">weapons grade</a> (<7%), fuel grade (7–19%) and <a href="/facts/Reactor_grade/9S0PJquG">reactor grade</a> (>19%). Lower grades are less suited for bombs and <a href="/facts/Thermal_reactor/tQQ71GtJ">thermal reactors</a> but can fuel <a href="/facts/Fast_reactor/g5kt2e6R">fast reactors</a>.</li> <li><a href="/facts/Plutonium-241/vUyJGFrs">Plutonium-241</a> is fissile, but <a href="/facts/Beta_decay/vxTBlckp">beta decays</a> with a half-life of 14 years to <a href="/facts/Americium-241/HnXXm1nx">americium-241</a>.</li> <li><a href="/facts/Plutonium-242/o1fg0sBh">Plutonium-242</a> is not fissile, nor very fertile (requiring 3 more neutron captures to become fissile); and has a low neutron capture <a href="/facts/Neutron_cross-section/gAkJmXXA">cross section</a>, and a longer half-life than any of the lighter isotopes.</li> <li><a href="/facts/Plutonium-244/XGtUVghF">Plutonium-244</a> 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 243Pu has a short half-life, but some is produced in nuclear explosions. 244Pu has been found in interstellar space<a class="footnote-ref" id="fnref:33" href="#fn:33"><sup>33</sup></a> and has the second longest half-life of any non-primordial radioisotope.</li></ul> <h2 id="production-and-uses">Production and uses</h2> <p>239Pu, a fissile isotope that is the second most used <a href="/facts/Nuclear_fuel/8RhAomlJ">nuclear fuel</a> in nuclear reactors after <a href="/facts/Uranium-235/pe0RznDM">uranium-235</a>, and the most used fuel in the <a href="/facts/Nuclear_fission/LfkIylvm">fission</a> portion of <a href="/facts/Nuclear_weapon/QVdBcMdm">nuclear weapons</a>, is produced from <a href="/facts/Uranium-238/QhcHm6q8">uranium-238</a> by neutron capture followed by two beta decays. </p><p>240Pu, 241Pu, and 242Pu are produced by further neutron capture. The odd-mass isotopes 239Pu and 241Pu have about a 3/4 chance of undergoing fission on capture of a <a href="/facts/Thermal_neutron/UMKR4XgJ">thermal neutron</a> and about a 1/4 chance of retaining the <a href="/facts/Neutron/oRCM1geb">neutron</a> and becoming the next heavier isotope. The even-mass isotopes are <a href="/facts/Fertile_material/Gt9u52G8">fertile</a> but not fissile and also have a lower probability (<a href="/facts/Neutron_cross-section/gAkJmXXA">cross section</a>) of neutron capture; therefore, they tend to accumulate in nuclear fuel used in a thermal reactor, the design of nearly all <a href="/facts/Nuclear_power_plant/IJj5pJUn">nuclear power plants</a> today. In plutonium that has been used a second time in thermal reactors in <a href="/facts/MOX_fuel/3tKw5I8q">MOX fuel</a>, 240Pu may even be the most common isotope. All plutonium isotopes and other <a href="/facts/Actinide/kHC4lxJV">actinides</a>, however, are <a href="/facts/Fissionable/XJR9qoxW">fissionable</a> with <a href="/facts/Fast_neutron/UMKR4XgJ">fast neutrons</a>. 240Pu does have a moderate thermal neutron absorption cross section, so that 241Pu production in a thermal reactor becomes a significant fraction as large as 239Pu production. </p><p>241Pu has a half-life of 14 years, and has slightly higher thermal neutron cross sections than 239Pu for both fission and absorption. While nuclear fuel is being used in a reactor, a 241Pu nucleus is much more likely to fission or to capture a neutron than to decay. 241Pu accounts for a significant portion of fissions in thermal reactor fuel that has been used for some time. However, in <a href="/facts/Spent_nuclear_fuel/jWDWvJ6d">spent nuclear fuel</a> that does not quickly undergo nuclear reprocessing but instead is cooled for years after use, much or most of the 241Pu will beta decay to <a href="/facts/Americium-241/HnXXm1nx">americium-241</a>, one of the <a href="/facts/Minor_actinide/oaonA636">minor actinides</a>, a strong alpha emitter, and difficult to use in thermal reactors. </p><p>242Pu has a particularly low cross section for thermal neutron capture; and it takes three neutron absorptions to become another fissile isotope (either <a href="/facts/Curium/LMyWXg8l">curium</a>-245 or 241Pu) 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 <a href="/facts/Californium/AJVjoVut">californium</a>, which is a neutron emitter by spontaneous fission and difficult to handle) or becoming 242Pu again; so the mean number of neutrons absorbed before fission is even higher than 3. Therefore, 242Pu is particularly unsuited to recycling in a thermal reactor and would be better used in a <a href="/facts/Fast_reactor/g5kt2e6R">fast reactor</a> where it can be fissioned directly. However, 242Pu's low cross section means that relatively little of it will be transmuted during one cycle in a thermal reactor. 242Pu's half-life is about 15 times as long as 239Pu's half-life; therefore, it is 1/15 as radioactive and not one of the larger contributors to <a href="/facts/Nuclear_waste/MjYh5tlu">nuclear waste</a> radioactivity. 242Pu's <a href="/facts/Gamma_ray/5Drf913J">gamma ray</a> emissions are also weaker than those of the other isotopes.<a class="footnote-ref" id="fnref:34" href="#fn:34"><sup>34</sup></a> </p><p>243Pu has a half-life of only 5 hours, beta decaying to <a href="/facts/Americium-243/aqoWt39B">americium-243</a>. Because 243Pu has little opportunity to capture an additional neutron before decay, the <a href="/facts/Nuclear_fuel_cycle/flBannfd">nuclear fuel cycle</a> does not produce the long-lived 244Pu in significant quantity. </p><p>238Pu is not normally produced in as large quantity by the nuclear fuel cycle, but some is produced from <a href="/facts/Neptunium-237/X3bPWwX1">neptunium-237</a> by neutron capture (this reaction can also be used with purified neptunium to produce 238Pu relatively free of other plutonium isotopes for use in <a href="/facts/Radioisotope_thermoelectric_generator/Tsjjvp5h">radioisotope thermoelectric generators</a>), by the (n,2n) reaction of fast neutrons on 239Pu, or by alpha decay of <a href="/facts/Curium/LMyWXg8l">curium</a>-242, which is produced by neutron capture of 241Am. It has significant thermal neutron cross section for fission, but is more likely to capture a neutron and become 239Pu. </p> <h2 id="manufacture">Manufacture</h2> <h3>Plutonium-240, -241 and -242</h3> <p>The fission <a href="/facts/Cross_section_(physics)/lo014h2D">cross section</a> for 239Pu is 747.9 <a href="/facts/Barn_(unit)/0yCEtKJ9">barns</a> 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 <a href="/facts/Weapons_grade/o2S0c30F">weapons grade</a> plutonium. </p> The formation of 240Pu, 241Pu, and 242Pu from 238U<table><tbody><tr><th rowspan="2">Isotope</th><th colspan="2">Thermal neutroncross section<a class="footnote-ref" id="fnref:35" href="#fn:35"><sup>35</sup></a>(barns)</th><th rowspan="2">DecayMode</th><th rowspan="2">Half-life</th></tr><tr><th>Capture</th><th>Fission</th></tr><tr><td><a href="/facts/Uranium-238/QhcHm6q8">238U</a></td><td>2.683</td><td>0.000</td><td>α</td><td>4.468 x 109 years</td></tr><tr><td><a href="/facts/Uranium-239/zWIQ6MVL">239U</a></td><td>20.57</td><td>14.11</td><td>β−</td><td>23.45 minutes</td></tr><tr><td><a href="/facts/Neptunium-239/X3bPWwX1">239Np</a></td><td>77.03</td><td>–</td><td>β−</td><td>2.356 days</td></tr><tr><td><a href="/facts/Plutonium-239/eRobTXos">239Pu</a></td><td>270.7</td><td>747.9</td><td>α</td><td>24,110 years</td></tr><tr><td><a href="/facts/Plutonium-240/kIWwdLkI">240Pu</a></td><td>287.5</td><td>0.064</td><td>α</td><td>6,561 years</td></tr><tr><td><a href="/facts/Plutonium-241/vUyJGFrs">241Pu</a></td><td>363.0</td><td>1012</td><td>β−</td><td>14.325 years</td></tr><tr><td><a href="/facts/Plutonium-242/o1fg0sBh">242Pu</a></td><td>19.16</td><td>0.001</td><td>α</td><td>373,300 years</td></tr></tbody></table> <h3>Plutonium-239</h3> <p class="note">Main article: <a href="/facts/Plutonium-239/eRobTXos">Plutonium-239</a></p> <p>239Pu 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 <a href="/facts/Uranium-235/pe0RznDM">uranium-235</a> and <a href="/facts/Uranium-233/a6sMrk07">uranium-233</a>. 239Pu is virtually nonexistent in nature. It is made by bombarding <a href="/facts/Uranium-238/QhcHm6q8">uranium-238</a> with neutrons. Uranium-238 is present in quantity in most reactor fuel; hence 239Pu is continuously made in these reactors. Since 239Pu can itself be split by neutrons to release energy, 239Pu provides a portion of the energy generation in a nuclear reactor. </p> The formation of 239Pu from 238U<a class="footnote-ref" id="fnref:36" href="#fn:36"><sup>36</sup></a><table><tbody><tr><th>Element</th><th>Isotope</th><th>Thermal neutron capturecross section (barn)</th><th>Thermal neutron fission Cross section (barn)</th><th>decay mode</th><th>Half-life</th></tr><tr><th><a href="/facts/Uranium/n2sGWBzU">U</a></th><td>238</td><td>2.68</td><td>5·10−6</td><td>α</td><td>4.47 x 109 years</td></tr><tr><th><a href="/facts/Uranium/n2sGWBzU">U</a></th><td>239</td><td>22</td><td>15</td><td>β−</td><td>23 minutes</td></tr><tr><th><a href="/facts/Neptunium/pwp7Yvds">Np</a></th><td>239</td><td>30</td><td>1</td><td>β−</td><td>2.36 days</td></tr><tr><th><a href="/facts/Plutonium/4bUw9zH3">Pu</a></th><td>239</td><td>271</td><td>750</td><td>α</td><td>24,110 years</td></tr></tbody></table> <h3>Plutonium-238</h3> <p class="note">Main article: <a href="/facts/Plutonium-238/JzY7TPFE">Plutonium-238</a></p> <p>There are small amounts of 238Pu in the plutonium from usual reactors. However, isotopic separation would be quite expensive compared to another method: when 235U captures a neutron, it is converted to an excited state of 236U. Some of the excited 236U nuclei undergo fission, but some decay to the ground state of 236U by emitting gamma radiation. Further neutron capture creates 237U; which, with a half-life of 7 days, decays to 237Np. Since nearly all neptunium is produced in this way or consists of isotopes that decay quickly, one gets nearly pure 237Np. After chemical separation of neptunium, 237Np is again irradiated by reactor neutrons to be converted to 238Np, which decays to 238Pu with a half-life of 2 days. </p> The formation of 238Pu from 235U<table><tbody><tr><th>Element</th><th>Isotope</th><th>Thermal neutroncross section</th><th>decay mode</th><th>Half-life</th></tr><tr><th><a href="/facts/Uranium/n2sGWBzU">U</a></th><td>235</td><td>99</td><td>α</td><td>703,800,000 years</td></tr><tr><th><a href="/facts/Uranium/n2sGWBzU">U</a></th><td>236</td><td>5.3</td><td>α</td><td>23,420,000 years</td></tr><tr><th><a href="/facts/Uranium/n2sGWBzU">U</a></th><td>237</td><td>—</td><td>β−</td><td>6.75 days</td></tr><tr><th><a href="/facts/Neptunium/pwp7Yvds">Np</a></th><td>237</td><td>165 (capture)</td><td>α</td><td>2,144,000 years</td></tr><tr><th><a href="/facts/Neptunium/pwp7Yvds">Np</a></th><td>238</td><td>—</td><td>β−</td><td>2.11 days</td></tr><tr><th><a href="/facts/Plutonium/4bUw9zH3">Pu</a></th><td>238</td><td>—</td><td>α</td><td>87.7 years</td></tr></tbody></table> <h2 id="plutonium-240-as-an-obstacle-to-nuclear-weapons">Plutonium-240 as an obstacle to nuclear weapons</h2> <p>240Pu undergoes <a href="/facts/Spontaneous_fission/0QuJoVKI">spontaneous fission</a> at a small but significant rate (5.8×10−6%).<a class="footnote-ref" id="fnref:37" href="#fn:37"><sup>37</sup></a> The presence of 240Pu limits the plutonium's use in a <a href="/facts/Nuclear_bomb/QVdBcMdm">nuclear bomb</a>, because a neutron from spontaneous fission starts the <a href="/facts/Chain_reaction/5UwHTKXS">chain reaction</a> prematurely, causing an early release of energy that disperses the core before full <a href="/facts/Implosion_(mechanical_process)/sQ2J2wQk">implosion</a> is reached. This prevents most of the core from participation in the chain reaction and reduces the bomb's yield. </p><p>Plutonium consisting of more than about 90% 239Pu is called <a href="/facts/Weapons-grade_plutonium/o2S0c30F">weapons-grade plutonium</a>; plutonium from <a href="/facts/Spent_nuclear_fuel/jWDWvJ6d">spent nuclear fuel</a> from commercial power reactors generally contains at least 20% 240Pu and is called <a href="/facts/Reactor-grade_plutonium/9S0PJquG">reactor-grade plutonium</a>. However, modern nuclear weapons use <a href="/facts/Fusion_boosting/U11GQ2mf">fusion boosting</a>, which mitigates the predetonation problem; if the <a href="/facts/Pit_(nuclear_weapon)/8HGl80tM">pit</a> can generate a <a href="/facts/Nuclear_weapon_yield/53of1vqQ">nuclear weapon yield</a> of even a fraction of a <a href="/facts/Kiloton/nEQ5z8mp">kiloton</a>, which is enough to start <a href="/facts/Nuclear_fusion/hP0gLDqj">deuterium–tritium fusion</a>, the resulting burst of neutrons will fission enough plutonium to ensure a yield of tens of kilotons. </p><p>Contamination due to 240Pu is the reason plutonium weapons must use the <a href="/facts/Nuclear_weapon_design/gw0LEc74">implosion method</a>. Theoretically, pure 239Pu could be used in a <a href="/facts/Gun-type_bomb/e5g6L4gL">gun-type bomb</a>, but achieving this level of purity is prohibitively difficult. 240Pu contamination has proven a mixed blessing. While it created delays and headaches during the <a href="/facts/Manhattan_Project/gtg8yRK2">Manhattan Project</a> because of the need to develop implosion technology, those same difficulties are a barrier to <a href="/facts/Nuclear_proliferation/f8dSJyAR">nuclear proliferation</a>. Implosion bombs are also inherently more efficient and less prone to accidental detonation than are gun-type bombs. </p> <h2 id="notes">Notes</h2> <ul><li>Isotope masses from: <ul><li>Audi, Georges; Bersillon, Olivier; Blachot, Jean; <a href="/facts/Aaldert_Wapstra/9Ylvt18s">Wapstra, Aaldert Hendrik</a> (2003), <a href="https://hal.archives-ouvertes.fr/in2p3-00020241/document">"The NUBASE evaluation of nuclear and decay properties"</a>, <i>Nuclear Physics A</i>, 729: 3–128, <a href="/facts/Bibcode_(identifier)/9HtdQSGB">Bibcode</a>:<a href="https://ui.adsabs.harvard.edu/abs/2003NuPhA.729....3A">2003NuPhA.729....3A</a>, <a href="/facts/Doi_(identifier)/muM9Etpq">doi</a>:<a href="https://doi.org/10.1016%2Fj.nuclphysa.2003.11.001">10.1016/j.nuclphysa.2003.11.001</a></li></ul></li> <li>Half-life, spin, and isomer data selected from the following sources. <ul><li>Audi, Georges; Bersillon, Olivier; Blachot, Jean; <a href="/facts/Aaldert_Wapstra/9Ylvt18s">Wapstra, Aaldert Hendrik</a> (2003), <a href="https://hal.archives-ouvertes.fr/in2p3-00020241/document">"The NUBASE evaluation of nuclear and decay properties"</a>, <i>Nuclear Physics A</i>, 729: 3–128, <a href="/facts/Bibcode_(identifier)/9HtdQSGB">Bibcode</a>:<a href="https://ui.adsabs.harvard.edu/abs/2003NuPhA.729....3A">2003NuPhA.729....3A</a>, <a href="/facts/Doi_(identifier)/muM9Etpq">doi</a>:<a href="https://doi.org/10.1016%2Fj.nuclphysa.2003.11.001">10.1016/j.nuclphysa.2003.11.001</a></li> <li><a href="/facts/National_Nuclear_Data_Center/SgVzvxLk">National Nuclear Data Center</a>. <a href="http://www.nndc.bnl.gov/nudat2/">"NuDat 2.x database"</a>. <a href="/facts/Brookhaven_National_Laboratory/L2JrG0K1">Brookhaven National Laboratory</a>.</li> <li>Holden, Norman E. (2004). "11. Table of the Isotopes". In Lide, David R. (ed.). <i><a href="/facts/CRC_Handbook_of_Chemistry_and_Physics/qjxzC2Cu">CRC Handbook of Chemistry and Physics</a></i> (85th ed.). <a href="/facts/Boca_Raton%2c_Florida/9gcNen3S">Boca Raton, Florida</a>: <a href="/facts/CRC_Press/duTuH4hz">CRC Press</a>. <a href="/facts/ISBN_(identifier)/15AdSPa9">ISBN</a> 978-0-8493-0485-9.</li></ul></li></ul> <h2 id="sources">Sources</h2> <ul><li>Magurno, B. A.; Pearlstein, S., eds. (1981). <a href="https://www-nds.iaea.org/publications/indc/indc_usa_0085_II.pdf"><i>Proceedings of the conference on nuclear data evaluation methods and procedures. BNL-NCS 51363</i></a> (PDF). Vol. II. Upton: <a href="/facts/Brookhaven_National_Laboratory/L2JrG0K1">Brookhaven National Laboratory</a>. <a href="https://web.archive.org/web/20210308125416/https://www-nds.iaea.org/publications/indc/indc_usa_0085_II.pdf">Archived</a> (PDF) from the original on March 8, 2021. Retrieved August 6, 2014.</li> <li>Miner, William N.; Schonfeld, Fred W. (1968). <a href="https://archive.org/details/encyclopediaofch00hamp">"Plutonium"</a>. In Clifford A. Hampel (ed.). <i>The Encyclopedia of the Chemical Elements</i>. New York (NY): Reinhold Book Corporation. pp. <a href="https://archive.org/details/encyclopediaofch00hamp/page/540">540–546</a>. <a href="/facts/LCCN_(identifier)/5hb5Cw2V">LCCN</a> <a href="https://lccn.loc.gov/68029938">68029938</a>.</li></ul> <h2 id="references">References</h2> <ol> <li id="fn:1"><p>Primordial plutonium-244 is predicted to occur in trace quantities in rare-earth minerals. However, as of 2021, measurements of various bastnäsite samples have placed an upper limit of its concentration on the order of 10-19 by mass. [3] <a href="/wiki/Primordial_nuclide" target="_blank">/wiki/Primordial_nuclide</a> <a href="#fnref:1" class="footnote-back-ref">↩</a></p></li> <li id="fn:2"><p>mPu – Excited nuclear isomer. <a href="/wiki/Nuclear_isomer" target="_blank">/wiki/Nuclear_isomer</a> <a href="#fnref:2" class="footnote-back-ref">↩</a></p></li> <li id="fn:3"><p>Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*". Chinese Physics C. 45 (3): 030003. doi:10.1088/1674-1137/abddaf. <a href="/wiki/Doi_(identifier)" target="_blank">/wiki/Doi_(identifier)</a> <a href="#fnref:3" class="footnote-back-ref">↩</a></p></li> <li id="fn:4"><p>( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits. <a href="#fnref:4" class="footnote-back-ref">↩</a></p></li> <li id="fn:5"><p># – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS). <a href="#fnref:5" class="footnote-back-ref">↩</a></p></li> <li id="fn:6"><p>Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3): 030001. doi:10.1088/1674-1137/abddae. <a href="https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf" target="_blank">https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf</a> <a href="#fnref:6" class="footnote-back-ref">↩</a></p></li> <li id="fn:7"><p>Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3): 030001. doi:10.1088/1674-1137/abddae. <a href="https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf" target="_blank">https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf</a> <a href="#fnref:7" class="footnote-back-ref">↩</a></p></li> <li id="fn:8"><p>Modes of decay: EC:Electron captureCD:Cluster decayIT:Isomeric transitionSF:Spontaneous fission <a href="/wiki/Electron_capture" target="_blank">/wiki/Electron_capture</a> <a href="#fnref:8" class="footnote-back-ref">↩</a></p></li> <li id="fn:9"><p>Bold italics symbol as daughter – Daughter product is nearly stable. <a href="#fnref:9" class="footnote-back-ref">↩</a></p></li> <li id="fn:10"><p>Bold symbol as daughter – Daughter product is stable. <a href="#fnref:10" class="footnote-back-ref">↩</a></p></li> <li id="fn:11"><p>Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3): 030001. doi:10.1088/1674-1137/abddae. <a href="https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf" target="_blank">https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf</a> <a href="#fnref:11" class="footnote-back-ref">↩</a></p></li> <li id="fn:12"><p>( ) spin value – Indicates spin with weak assignment arguments. <a href="#fnref:12" class="footnote-back-ref">↩</a></p></li> <li id="fn:13"><p># – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN). <a href="#fnref:13" class="footnote-back-ref">↩</a></p></li> <li id="fn:14"><p>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 (2024). "Свойства радиоактивного распада нового ядра 227Pu" [Properties of Radioactive Decay of the New Nucleus 227Pu] (PDF). jinr.ru (in Russian). Joint Institute for Nuclear Research. Retrieved 9 November 2024. <a href="http://www1.jinr.ru/Preprints/2024/50(P7-2024-50).pdf" target="_blank">http://www1.jinr.ru/Preprints/2024/50(P7-2024-50).pdf</a> <a href="#fnref:14" class="footnote-back-ref">↩</a></p></li> <li id="fn:15"><p>Yang, H. B.; Gan, Z. G.; Zhang, Z. Y.; Huang, M. H.; Ma, L.; Yang, C. L.; Zhang, M. M.; Tian, Y. L.; Wang, Y. S.; Wang, J. G.; Zhou, H. B.; Hua, W.; Wang, J. Y.; Qiang, Y. H.; Zhao, Z.; Huang, X. Y.; Wen, X. J.; Li, Z. Y.; Zhang, H. T.; Xu, S. Y.; Li, Z. C.; Zhou, H.; Zhang, X.; Zhu, L.; Wang, Z.; Guan, F.; Yang, H. R.; Huang, W. X.; Ren, Z. Z.; Zhou, S. G.; Xu, H. S. (3 October 2024). "α decay of the new isotope Pu 227". Physical Review C. 110 (4). doi:10.1103/PhysRevC.110.044302. <a href="/wiki/Doi_(identifier)" target="_blank">/wiki/Doi_(identifier)</a> <a href="#fnref:15" class="footnote-back-ref">↩</a></p></li> <li id="fn:16"><p>Wilson, G. L.; Takeyama, M.; Andreyev, A. N.; Andel, B.; Antalic, S.; Catford, W. N.; Ghys, L.; Haba, H.; Heßberger, F. P.; Huang, M.; Kaji, D.; Kalaninova, Z.; Morimoto, K.; Morita, K.; Murakami, M.; Nishio, K.; Orlandi, R.; Smith, A. G.; Tanaka, K.; Wakabayashi, Y.; Yamaki, S. (13 October 2017). "β -delayed fission of Am 230". Physical Review C. 96 (4): 044315. doi:10.1103/PhysRevC.96.044315. ISSN 2469-9985. <a href="https://doi.org/10.1103%2FPhysRevC.96.044315" target="_blank">https://doi.org/10.1103%2FPhysRevC.96.044315</a> <a href="#fnref:16" class="footnote-back-ref">↩</a></p></li> <li id="fn:17"><p>Theorized to also undergo β+β+ decay to 236U <a href="#fnref:17" class="footnote-back-ref">↩</a></p></li> <li id="fn:18"><p>Double beta decay product of 238U <a href="/wiki/Double_beta_decay" target="_blank">/wiki/Double_beta_decay</a> <a href="#fnref:18" class="footnote-back-ref">↩</a></p></li> <li id="fn:19"><p>fissile nuclide <a href="#fnref:19" class="footnote-back-ref">↩</a></p></li> <li id="fn:20"><p>Most useful isotope for nuclear weapons <a href="#fnref:20" class="footnote-back-ref">↩</a></p></li> <li id="fn:21"><p>Neutron capture product of 238U <a href="/wiki/Neutron_capture" target="_blank">/wiki/Neutron_capture</a> <a href="#fnref:21" class="footnote-back-ref">↩</a></p></li> <li id="fn:22"><p>Intermediate decay product of 244Pu <a href="/wiki/Plutonium-244" target="_blank">/wiki/Plutonium-244</a> <a href="#fnref:22" class="footnote-back-ref">↩</a></p></li> <li id="fn:23"><p>fissile nuclide <a href="#fnref:23" class="footnote-back-ref">↩</a></p></li> <li id="fn:24"><p>Can undergo Bound-state β− decay with a half-life of 4.2 days when fully ionized[8] <a href="/wiki/Beta_decay#Bound-state_β−_decay" target="_blank">/wiki/Beta_decay#Bound-state_β−_decay</a> <a href="#fnref:24" class="footnote-back-ref">↩</a></p></li> <li id="fn:25"><p>fissile nuclide <a href="#fnref:25" class="footnote-back-ref">↩</a></p></li> <li id="fn:26"><p>Interstellar, some may also be primordial but such claims are disputed <a href="/wiki/Primordial_nuclide" target="_blank">/wiki/Primordial_nuclide</a> <a href="#fnref:26" class="footnote-back-ref">↩</a></p></li> <li id="fn:27"><p>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. <a href="/wiki/Polonium" target="_blank">/wiki/Polonium</a> <a href="#fnref:27" class="footnote-back-ref">↩</a></p></li> <li id="fn:28"><p>Specifically from thermal neutron fission of uranium-235, e.g. in a typical nuclear reactor. <a href="/wiki/Thermal_neutron" target="_blank">/wiki/Thermal_neutron</a> <a href="#fnref:28" class="footnote-back-ref">↩</a></p></li> <li id="fn:29"><p>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]." <a href="/wiki/Bibcode_(identifier)" target="_blank">/wiki/Bibcode_(identifier)</a> <a href="#fnref:29" class="footnote-back-ref">↩</a></p></li> <li id="fn:30"><p>This is the heaviest nuclide with a half-life of at least four years before the "sea of instability". <a href="/wiki/Sea_of_instability" target="_blank">/wiki/Sea_of_instability</a> <a href="#fnref:30" class="footnote-back-ref">↩</a></p></li> <li id="fn:31"><p>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. <a href="/wiki/Primordial_nuclide" target="_blank">/wiki/Primordial_nuclide</a> <a href="#fnref:31" class="footnote-back-ref">↩</a></p></li> <li id="fn:32"><p>Makhijani, Arjun; Seth, Anita (July 1997). "The Use of Weapons Plutonium as Reactor Fuel" (PDF). Energy and Security. Takoma Park, MD: Institute for Energy and Environmental Research. Retrieved 4 July 2016. <a href="http://ieer.org/wp/wp-content/uploads/1997/07/no-3.pdf" target="_blank">http://ieer.org/wp/wp-content/uploads/1997/07/no-3.pdf</a> <a href="#fnref:32" class="footnote-back-ref">↩</a></p></li> <li id="fn:33"><p>Wallner, A.; Faestermann, T.; Feige, J.; Feldstein, C.; Knie, K.; Korschinek, G.; Kutschera, W.; Ofan, A.; Paul, M.; Quinto, F.; Rugel, G.; Steier, P. (2015). "Abundance of live 244Pu in deep-sea reservoirs on Earth points to rarity of actinide nucleosynthesis". Nature Communications. 6: 5956. arXiv:1509.08054. Bibcode:2015NatCo...6.5956W. doi:10.1038/ncomms6956. ISSN 2041-1723. PMC 4309418. PMID 25601158. <a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4309418" target="_blank">https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4309418</a> <a href="#fnref:33" class="footnote-back-ref">↩</a></p></li> <li id="fn:34"><p>"Plutonium Isotopic Results of Known Samples Using the Snap Gamma Spectroscopy Analysis Code and the Robwin Spectrum Fitting Routine" (PDF). Archived from the original (PDF) on 2017-08-13. Retrieved 2013-03-15. <a href="https://web.archive.org/web/20170813191754/http://www.wmsym.org/archives/2001/21B/21B-18.pdf" target="_blank">https://web.archive.org/web/20170813191754/http://www.wmsym.org/archives/2001/21B/21B-18.pdf</a> <a href="#fnref:34" class="footnote-back-ref">↩</a></p></li> <li id="fn:35"><p>National Nuclear Data Center Interactive Chart of Nuclides Archived 2011-07-21 at the Wayback Machine <a href="/wiki/National_Nuclear_Data_Center" target="_blank">/wiki/National_Nuclear_Data_Center</a> <a href="#fnref:35" class="footnote-back-ref">↩</a></p></li> <li id="fn:36"><p>Miner 1968, p. 541 - Miner, William N.; Schonfeld, Fred W. (1968). "Plutonium". In Clifford A. Hampel (ed.). The Encyclopedia of the Chemical Elements. New York (NY): Reinhold Book Corporation. pp. 540–546. LCCN 68029938. <a href="https://archive.org/details/encyclopediaofch00hamp" target="_blank">https://archive.org/details/encyclopediaofch00hamp</a> <a href="#fnref:36" class="footnote-back-ref">↩</a></p></li> <li id="fn:37"><p>Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3): 030001. doi:10.1088/1674-1137/abddae. <a href="https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf" target="_blank">https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf</a> <a href="#fnref:37" class="footnote-back-ref">↩</a></p></li> </ol>