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! &nbsp;<br />isotopic mass (u)<br />&nbsp;
! &nbsp;<br />isotopic mass (u)<br />&nbsp;
! rowspan="2" | half-life
! rowspan="2" | half-life
! 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" | daughter<br>isotope(s)
! rowspan="2" | nuclear<br />spin
! rowspan="2" | nuclear<br />spin
|-
|-
! colspan="3" | excitation energy
! colspan="3" | excitation energy
|-
|-
| <sup>231</sup>Am
| rowspan=2|<sup>231</sup>Am
| style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 95
| style="text-align:right" | 136
| rowspan=2 style="text-align:right" | 136
| 231.04556(32)#
| rowspan=2|231.04556(32)#
| 30# s
| rowspan=2|30# s
| [[beta decay|β<sup>+</sup>]]
|
| <sup>231</sup>Pu
| rowspan=2|
|-
|-
| [[alpha decay|α]] (rare)
| <sup>232</sup>Am
| <sup>227</sup>Np
| style="text-align:right" | 95
| style="text-align:right" | 137
| 232.04659(32)#
| 79(2) s
|
|-
|-
| <sup>233</sup>Am
| rowspan=3|<sup>232</sup>Am
| style="text-align:right" | 95
| rowspan=3 style="text-align:right" | 95
| style="text-align:right" | 138
| rowspan=3 style="text-align:right" | 137
| 233.04635(11)#
| rowspan=3|232.04659(32)#
| 3.2(8) min
| rowspan=3|79(2) s
| β<sup>+</sup> (98%)
|
| <sup>233</sup>Pu
| rowspan=3|
|-
|-
| α (2%)
| <sup>234</sup>Am
| <sup>228</sup>Np
| style="text-align:right" | 95
| style="text-align:right" | 139
| 234.04781(22)#
| 2.32(8) min
|
|-
|-
| <sup>235</sup>Am
| β<sup>+</sup>, [[Spontaneous fission|SF]] (.069%)
| (various)
| style="text-align:right" | 95
| style="text-align:right" | 140
| 235.04795(13)#
| 9.9(5) min
| 5/2-#
|-
|-
| <sup>236</sup>Am
| rowspan=2|<sup>233</sup>Am
| style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 95
| style="text-align:right" | 141
| rowspan=2 style="text-align:right" | 138
| 236.04958(11)#
| rowspan=2|233.04635(11)#
| 3.6(1) min
| rowspan=2|3.2(8) min
| β<sup>+</sup>
|
| <sup>233</sup>Pu
| rowspan=2|
|-
|-
| α
| <sup>237</sup>Am
| <sup>229</sup>Np
| style="text-align:right" | 95
| style="text-align:right" | 142
| 237.05000(6)#
| 73.0(10) min
| 5/2(-)
|-
|-
| <sup>238</sup>Am
| rowspan=3|<sup>234</sup>Am
| style="text-align:right" | 95
| rowspan=3 style="text-align:right" | 95
| style="text-align:right" | 143
| rowspan=3 style="text-align:right" | 139
| rowspan=3|234.04781(22)#
| 238.05198(5)
| 98(2) min
| rowspan=3|2.32(8) min
| β<sup>+</sup> (99.95%)
| 1+
| <sup>234</sup>Pu
| rowspan=3|
|-
| α (.04%)
| <sup>230</sup>Np
|-
| β<sup>+</sup>, SF (.0066%)
| (various)
|-
| rowspan=2|<sup>235</sup>Am
| rowspan=2 style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 140
| rowspan=2|235.04795(13)#
| rowspan=2|9.9(5) min
| β<sup>+</sup>
| <sup>235</sup>Pu
| rowspan=2|5/2-#
|-
| α (rare)
| <sup>231</sup>Np
|-
| rowspan=2|<sup>236</sup>Am
| rowspan=2 style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 141
| rowspan=2|236.04958(11)#
| rowspan=2|3.6(1) min
| β<sup>+</sup>
| <sup>236</sup>Pu
| rowspan=2|
|-
| α
| <sup>232</sup>Np
|-
| rowspan=2|<sup>237</sup>Am
| rowspan=2 style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 142
| rowspan=2|237.05000(6)#
| rowspan=2|73.0(10) min
| β<sup>+</sup> (99.97%)
| <sup>237</sup>Pu
| rowspan=2|5/2(-)
|-
| α (.025%)
| <sup>233</sup>Np
|-
| rowspan=2|<sup>238</sup>Am
| rowspan=2 style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 143
| rowspan=2|238.05198(5)
| rowspan=2|98(2) min
| β<sup>+</sup>
| <sup>238</sup>Pu
| rowspan=2|1+
|-
| α (1E-4%)
| <sup>234</sup>Np
|-
|-
| style="text-indent:1em" | <sup>238m</sup>Am
| style="text-indent:1em" | <sup>238m</sup>Am
| colspan="3" style="text-indent:2em" | 2500(200)# keV
| colspan="3" style="text-indent:2em" | 2500(200)# keV
| 35(10) µs
| 35(10) µs
|
|
|
|
|-
|-
| <sup>239</sup>Am
| rowspan=2|<sup>239</sup>Am
| style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 95
| style="text-align:right" | 144
| rowspan=2 style="text-align:right" | 144
| 239.0530245(26)
| rowspan=2|239.0530245(26)
| 11.9(1) h
| rowspan=2|11.9(1) h
| [[Electron capture|EC]] (99.99%)
| (5/2)-
| rowspan=2|(5/2)-
|-
| α (.01%)
| <sup>235</sup>Np
|-
|-
| style="text-indent:1em" | <sup>239m</sup>Am
| style="text-indent:1em" | <sup>239m</sup>Am
| colspan="3" style="text-indent:2em" | 2500(200) keV
| colspan="3" style="text-indent:2em" | 2500(200) keV
| 163(12) ns
| 163(12) ns
|
|
| (7/2+)
| (7/2+)
|-
|-
| <sup>240</sup>Am
| rowspan=2|<sup>240</sup>Am
| style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 95
| style="text-align:right" | 145
| rowspan=2 style="text-align:right" | 145
| 240.055300(15)
| rowspan=2|240.055300(15)
| 50.8(3) h
| rowspan=2|50.8(3) h
| β<sup>+</sup>
| (3-)
| <sup>240</sup>Pu
| rowspan=2|(3-)
|-
|-
| α (1.9E-4%)
| [[Americium-241|<sup>241</sup>Am]]
| <sup>236</sup>Np
| style="text-align:right" | 95
|-
| style="text-align:right" | 146
| rowspan=3|<sup>241</sup>Am
| 241.0568291(20)
| rowspan=3| style="text-align:right" | 95
| 432.2(7) a
| rowspan=3 style="text-align:right" | 146
| 5/2-
| rowspan=3|241.0568291(20)
| rowspan=3|432.2(7) a
| α
| <sup>237</sup>Np
| rowspan=3|5/2-
|-
| SF (4.3E-10%)
| (various)
|-
| [[Cluster decay|CD]] (7.4E-10%)
| <sup>207</sup>Tl, <sup>34</sup>Si
|-
|-
| style="text-indent:1em" | <sup>241m</sup>Am
| style="text-indent:1em" | <sup>241m</sup>Am
| colspan="3" style="text-indent:2em" | 2200(100) keV
| colspan="3" style="text-indent:2em" | 2200(100) keV
| 1.2(3) µs
| 1.2(3) µs
|
|
|
|
|-
|-
| [[Americium-242|<sup>242</sup>Am]]
| rowspan=2|<sup>242</sup>Am
| style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 95
| style="text-align:right" | 147
| rowspan=2 style="text-align:right" | 147
| 242.0595492(20)
| rowspan=2|242.0595492(20)
| 16.02(2) h
| rowspan=2|16.02(2) h
| β<sup>-</sup> (82.7%)
| 1-
| <sup>242</sup>Cm
| rowspan=2|1-
|-
|-
| EC (17.3%)
| style="text-indent:1em" | <sup>242m1</sup>Am
| <sup>242</sup>Pu
| colspan="3" style="text-indent:2em" | 48.60(5) keV
|-
| 141(2) a
| rowspan=3 style="text-indent:1em" | <sup>242m1</sup>Am
| 5-
| rowspan=3 colspan="3" style="text-indent:2em" | 48.60(5) keV
| rowspan=3|141(2) a
| [[Isomeric transition|IT]] (99.54%)
| <sup>242</sup>Am
| rowspan=3|5-
|-
| α (.46%)
| <sup>238</sup>Np
|-
| SF (1.5E-8%)
| (various)
|-
|-
| style="text-indent:1em" | <sup>242m2</sup>Am
| style="text-indent:1em" | <sup>242m2</sup>Am
| colspan="3" style="text-indent:2em" | 2200(80) keV
| colspan="3" style="text-indent:2em" | 2200(80) keV
| 14.0(10) ms
| 14.0(10) ms
|
|
| (2+,3-)
| (2+,3-)
|-
|-
| [[Americium-243|<sup>243</sup>Am]]
| rowspan=2|<sup>243</sup>Am
| style="text-align:right" | 95
| rowspan=2 style="text-align:right" | 95
| style="text-align:right" | 148
| rowspan=2 style="text-align:right" | 148
| 243.0613811(25)
| rowspan=2|243.0613811(25)
| 7.37(4)E+3 a
| rowspan=2|7.37(4)E+3 a
| 5/2-
| α
| <sup>239</sup>Np
| rowspan=2|5/2-
|-
| SF (3.7E-9%)
| (various)
|-
|-
| <sup>244</sup>Am
| <sup>244</sup>Am
Line 208: Line 299:
| 244.0642848(22)
| 244.0642848(22)
| 10.1(1) h
| 10.1(1) h
| β<sup>-</sup>
| <sup>244</sup>Cm
| (6-)#
| (6-)#
|-
|-
| style="text-indent:1em" | <sup>244m</sup>Am
| rowspan=2 style="text-indent:1em" | <sup>244m</sup>Am
| colspan="3" style="text-indent:2em" | 86.1(10) keV
| rowspan=2 colspan="3" style="text-indent:2em" | 86.1(10) keV
| 26(1) min
| rowspan=2|26(1) min
| β<sup>-</sup> (99.96%)
| 1+
| <sup>244</sup>Cm
| rowspan=2|1+
|-
| EC (.0361%)
| <sup>244</sup>Pl
|-
|-
| <sup>245</sup>Am
| <sup>245</sup>Am
Line 220: Line 318:
| 245.066452(4)
| 245.066452(4)
| 2.05(1) h
| 2.05(1) h
| β<sup>-</sup>
| <sup>245</sup>Cm
| (5/2)+
| (5/2)+
|-
|-
Line 227: Line 327:
| 246.069775(20)
| 246.069775(20)
| 39(3) min
| 39(3) min
| β<sup>-</sup>
| <sup>246</sup>Cm
| (7-)
| (7-)
|-
|-
| style="text-indent:1em" | <sup>246m1</sup>Am
| rowspan=2 style="text-indent:1em" | <sup>246m1</sup>Am
| colspan="3" style="text-indent:2em" | 30(10) keV
| rowspan=2 colspan="3" style="text-indent:2em" | 30(10) keV
| 25.0(2) min
| rowspan=2|25.0(2) min
| β<sup>-</sup> (99.99%)
| 2(-)
| <sup>246</sup>Cm
| rowspan=2|2(-)
|-
| IT (.01%)
| <sup>246</sup>Am
|-
|-
| style="text-indent:1em" | <sup>246m2</sup>Am
| style="text-indent:1em" | <sup>246m2</sup>Am
| colspan="3" style="text-indent:2em" | ~2000 keV
| colspan="3" style="text-indent:2em" | ~2000 keV
| 73(10) µs
| 73(10) µs
|
|
|
|
|-
|-
Line 244: Line 353:
| 247.07209(11)#
| 247.07209(11)#
| 23.0(13) min
| 23.0(13) min
| β<sup>-</sup>
| <sup>247</sup>Cm
| (5/2)#
| (5/2)#
|-
|-
Line 251: Line 362:
| 248.07575(22)#
| 248.07575(22)#
| 3# min
| 3# min
| β<sup>-</sup>
| <sup>248</sup>Cm
|
|
|-
|-
Line 258: Line 371:
| 249.07848(32)#
| 249.07848(32)#
| 1# min
| 1# min
| β<sup>-</sup>
| <sup>249</sup>Cm
|
|
|}
|}
<references group="n" />


=== Notes ===
=== Notes ===

Revision as of 08:38, 20 May 2011

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

Americium (Am) has no stable isotopes. A standard atomic mass cannot be given.

19 radioisotopes of americium have been characterized, with the most stable being 243Am with a half-life of 7370 years, and 241Am with a half-life of 432.7 years. All of the remaining radioactive isotopes have half-lives that are less than 51 hours, and the majority of these have half-lives that are less than 100 minutes. This element also has 8 meta states, with the most stable being 242mAm (t½ 141 years). The isotopes of americium range in atomic weight from 231.046 u (231Am) to 249.078 u (249Am).

Some notable isotopes

Americium-241

Americium-241 used in a smoke detector.

Americium-241 is the most prevalent isotope of americium in nuclear waste.[6] It is the americium isotope used in smoke detectors based on ionization chambers. It is a potential fuel for long-lifetime radioisotope thermoelectric generators.

Parameter Value
Atomic mass 241.056823 u
Mass excess 52930 keV
Beta decay energy -767 keV
Spin 5/2-
Half life 432.2 years
Spontaneous fissions 1200 per kg/s
Decay heat 114 watts/kg

Possible parent nuclides: beta from Pu-241, electron capture from Cm-241, alpha from Bk-245

Americium-241 decays by alpha emission, with a by-product of gamma rays. Its presence in plutonium is determined by the original concentration of plutonium-241 and the sample age. Because of the low penetration of alpha radiation, Americium-241 only poses a health risk when ingested or inhaled. Older samples of plutonium containing plutonium-241 contain a buildup of Am-241. A chemical removal of americium from reworked plutonium, e.g. during reworking of plutonium pits, may be required.

Americium-242m

Transmutation flow between 238Pu and 244Cm in LWR.[7]
Fission percentage is 100 minus shown percentages.
Total rate of transmutation varies greatly by nuclide.
245Cm–248Cm are long-lived with negligible decay.
242mAm decay modes (halflife: 141 years)
Probability Decay mode Decay energy Decay product
99.54% isomeric transition 0.05 MeV 242Am
0.46% alpha decay 5.64 MeV 238Np
(1.5±0.6)×10−10[8] spontaneous fission ~200 MeV fission products

Americium-242m is one of the isotopes of americium, with 95 protons and electrons and 147 neutrons and a mass of 242.0595492 g/mol. It is one of the rare cases, like tantalum-180m, where a higher-energy nuclear isomer is more stable than the lower-energy one, Americium-242.[9]

242mAm is fissile (because it has an odd number of neutrons) and has a low critical mass, comparable to that of plutonium-239.[10] It has a very high cross section for fission, and if in a nuclear reactor is destroyed relatively quickly. Another report claims that 242mAm has a much lower critical mass, can sustain a chain reaction even as a thin film, and could be used for a novel type of nuclear rocket.[11]

242Am decay modes (halflife: 16 hours)
Probability Decay mode Decay energy Decay product
82.70% beta decay 0.665 MeV 242Cm
17.30% electron capture 0.751 MeV 242Pu

Americium-243

Americium-243 is a radioactive isotope of americium having 95 electrons and protons and 148 neutrons and has a mass of 243.06138 g/mol.

It has a half-life of 7370 years, the longest lasting of all americium isotopes, however, it is still not found in nature. It is formed in the nuclear fuel cycle by neutron capture on plutonium-242 followed by beta decay. [12] Production increases exponentially with increasing burnup as a total of 5 neutron captures on uranium-238 are required.

It either decays by emitting an alpha particle (the decay energy is 5.27MeV)[13] to turn into neptunium-239, which then quickly decays to plutonium-239, or infrequently, by spontaneous fission. [14]

Americium-243 is a hazardous substance, because it can cause cancer. Neptunium-239, which is formed from Americium-243, emits dangerous gamma rays, making Americium-243 the most dangerous isotope of Americium. [15]

Table

nuclide
symbol
Z(p) N(n)  
isotopic mass (u)
 
half-life decay
mode(s)[16][n 1]
daughter
isotope(s)
nuclear
spin
excitation energy
231Am 95 136 231.04556(32)# 30# s β+ 231Pu
α (rare) 227Np
232Am 95 137 232.04659(32)# 79(2) s β+ (98%) 233Pu
α (2%) 228Np
β+, SF (.069%) (various)
233Am 95 138 233.04635(11)# 3.2(8) min β+ 233Pu
α 229Np
234Am 95 139 234.04781(22)# 2.32(8) min β+ (99.95%) 234Pu
α (.04%) 230Np
β+, SF (.0066%) (various)
235Am 95 140 235.04795(13)# 9.9(5) min β+ 235Pu 5/2-#
α (rare) 231Np
236Am 95 141 236.04958(11)# 3.6(1) min β+ 236Pu
α 232Np
237Am 95 142 237.05000(6)# 73.0(10) min β+ (99.97%) 237Pu 5/2(-)
α (.025%) 233Np
238Am 95 143 238.05198(5) 98(2) min β+ 238Pu 1+
α (1E-4%) 234Np
238mAm 2500(200)# keV 35(10) µs
239Am 95 144 239.0530245(26) 11.9(1) h EC (99.99%) (5/2)-
α (.01%) 235Np
239mAm 2500(200) keV 163(12) ns (7/2+)
240Am 95 145 240.055300(15) 50.8(3) h β+ 240Pu (3-)
α (1.9E-4%) 236Np
241Am style="text-align:right" | 95 146 241.0568291(20) 432.2(7) a α 237Np 5/2-
SF (4.3E-10%) (various)
CD (7.4E-10%) 207Tl, 34Si
241mAm 2200(100) keV 1.2(3) µs
242Am 95 147 242.0595492(20) 16.02(2) h β- (82.7%) 242Cm 1-
EC (17.3%) 242Pu
242m1Am 48.60(5) keV 141(2) a IT (99.54%) 242Am 5-
α (.46%) 238Np
SF (1.5E-8%) (various)
242m2Am 2200(80) keV 14.0(10) ms (2+,3-)
243Am 95 148 243.0613811(25) 7.37(4)E+3 a α 239Np 5/2-
SF (3.7E-9%) (various)
244Am 95 149 244.0642848(22) 10.1(1) h β- 244Cm (6-)#
244mAm 86.1(10) keV 26(1) min β- (99.96%) 244Cm 1+
EC (.0361%) 244Pl
245Am 95 150 245.066452(4) 2.05(1) h β- 245Cm (5/2)+
246Am 95 151 246.069775(20) 39(3) min β- 246Cm (7-)
246m1Am 30(10) keV 25.0(2) min β- (99.99%) 246Cm 2(-)
IT (.01%) 246Am
246m2Am ~2000 keV 73(10) µs
247Am 95 152 247.07209(11)# 23.0(13) min β- 247Cm (5/2)#
248Am 95 153 248.07575(22)# 3# min β- 248Cm
249Am 95 154 249.07848(32)# 1# min β- 249Cm

Notes

  • 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.

See also

Template:Wikipedia-Books

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. ^ "Americium". Argonne National Laboratory, EVS. Retrieved 25 December 2009.
  7. ^ Sasahara, Akihiro; Matsumura, Tetsuo; Nicolaou, Giorgos; Papaioannou, Dimitri (April 2004). "Neutron and Gamma Ray Source Evaluation of LWR High Burn-up UO2 and MOX Spent Fuels". Journal of NUCLEAR SCIENCE and TECHNOLOGY. 41 (4): 448–456. doi:10.3327/jnst.41.448.
  8. ^ Phys. Rev. 155 (1967): J. T. Caldwell, S. C. Fultz, C. D. Bowman, and R. W. Hoff - Spontaneous Fission Half-Life of 242mAm (halflife (9.5±3.5)×1011
  9. ^ 95-Am-242
  10. ^ http://typhoon.jaea.go.jp/icnc2003/Proceeding/paper/6.5_022.pdf
  11. ^ Extremely Efficient Nuclear Fuel Could Take Man To Mars In Just Two Weeks
  12. ^ "Americium-243". Oak Ridge National Laboratory. Retrieved 25 December 2009.
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