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Isotopes of neptunium: Difference between revisions

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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
|-
|-
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| 225.03391(8)
| 225.03391(8)
| 3# ms [>2 µs]
| 3# ms [>2 µs]
| [[alpha decay|α]]
| <sup>221</sup>Pa
| 9/2-#
| 9/2-#
|-
|-
Line 63: Line 67:
| 226.03515(10)#
| 226.03515(10)#
| 35(10) ms
| 35(10) ms
| α
| <sup>222</sup>Pa
|
|
|-
|-
| {{SimpleNuclide2|Neptunium|227}}
| rowspan=2|{{SimpleNuclide2|Neptunium|227}}
| style="text-align:right" | 93
| rowspan=2 style="text-align:right" | 93
| style="text-align:right" | 134
| rowspan=2 style="text-align:right" | 134
| 227.03496(8)
| rowspan=2|227.03496(8)
| 510(60) ms
| rowspan=2|510(60) ms
| α (99.95%)
| 5/2-#
| <sup>223</sup>Pa
| rowspan=2|5/2-#
|-
|-
| β<sup>+</sup> (.05%)
| {{SimpleNuclide2|Neptunium|228}}
| <sup>227</sup>U
| style="text-align:right" | 93
| style="text-align:right" | 135
| 228.03618(21)#
| 61.4(14) s
|
|-
|-
| {{SimpleNuclide2|Neptunium|229}}
| rowspan=3|{{SimpleNuclide2|Neptunium|228}}
| style="text-align:right" | 93
| rowspan=3 style="text-align:right" | 93
| style="text-align:right" | 136
| rowspan=3 style="text-align:right" | 135
| rowspan=3|228.03618(21)#
| 229.03626(9)
| 4.0(2) min
| rowspan=3|61.4(14) s
| β<sup>+</sup> (59%)
| 5/2+#
| <sup>228</sup>U
| rowspan=3|
|-
|-
| α (41%)
| {{SimpleNuclide2|Neptunium|230}}
| <sup>224</sup>Pa
| style="text-align:right" | 93
| style="text-align:right" | 137
| 230.03783(6)
| 4.6(3) min
|
|-
|-
| β<sup>+</sup>, [[Spontaneous fission|SF]] (.012%)
| {{SimpleNuclide2|Neptunium|231}}
| (various)
| style="text-align:right" | 93
| style="text-align:right" | 138
| 231.03825(5)
| 48.8(2) min
| (5/2)(+#)
|-
|-
| {{SimpleNuclide2|Neptunium|232}}
| rowspan=2|{{SimpleNuclide2|Neptunium|229}}
| style="text-align:right" | 93
| rowspan=2 style="text-align:right" | 93
| style="text-align:right" | 139
| rowspan=2 style="text-align:right" | 136
| rowspan=2|229.03626(9)
| 232.04011(11)#
| 14.7(3) min
| rowspan=2|4.0(2) min
| (4+)
| α (51%)
| <sup>225</sup>Pa
| rowspan=2|5/2+#
|-
|-
| β<sup>+</sup> (49%)
| {{SimpleNuclide2|Neptunium|233}}
| <sup>229</sup>U
| style="text-align:right" | 93
|-
| style="text-align:right" | 140
| rowspan=2|{{SimpleNuclide2|Neptunium|230}}
| 233.04074(5)
| rowspan=2 style="text-align:right" | 93
| 36.2(1) min
| rowspan=2 style="text-align:right" | 137
| (5/2+)
| rowspan=2|230.03783(6)
| rowspan=2|4.6(3) min
| β<sup>+</sup> (97%)
| <sup>230</sup>U
| rowspan=2|
|-
| α (3%)
| <sup>226</sup>Pa
|-
| rowspan=2|{{SimpleNuclide2|Neptunium|231}}
| rowspan=2 style="text-align:right" | 93
| rowspan=2 style="text-align:right" | 138
| rowspan=2|231.03825(5)
| rowspan=2|48.8(2) min
| β<sup>+</sup> (98%)
| <sup>231</sup>U
| rowspan=2|(5/2)(+#)
|-
| α (2%)
| <sup>227</sup>Pa
|-
| rowspan=2|{{SimpleNuclide2|Neptunium|232}}
| rowspan=2 style="text-align:right" | 93
| rowspan=2 style="text-align:right" | 139
| rowspan=2|232.04011(11)#
| rowspan=2|14.7(3) min
| β<sup>+</sup> (99.99%)
| <sup>232</sup>U
| rowspan=2|(4+)
|-
| α (.003%)
| <sup>228</sup>Pa
|-
| rowspan=2|{{SimpleNuclide2|Neptunium|233}}
| rowspan=2 style="text-align:right" | 93
| rowspan=2 style="text-align:right" | 140
| rowspan=2|233.04074(5)
| rowspan=2|36.2(1) min
| β<sup>+</sup> (99.99%)
| <sup>233</sup>U
| rowspan=2|(5/2+)
|-
| α (.001%)
| <sup>229</sup>Pa
|-
|-
| {{SimpleNuclide2|Neptunium|234}}
| {{SimpleNuclide2|Neptunium|234}}
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| 234.042895(9)
| 234.042895(9)
| 4.4(1) d
| 4.4(1) d
| β<sup>+</sup>
| <sup>234</sup>U
| (0+)
| (0+)
|-
|-
| {{SimpleNuclide2|Neptunium|235}}
| rowspan=2|{{SimpleNuclide2|Neptunium|235}}
| style="text-align:right" | 93
| rowspan=2 style="text-align:right" | 93
| style="text-align:right" | 142
| rowspan=2 style="text-align:right" | 142
| 235.0440633(21)
| rowspan=2|235.0440633(21)
| 396.1(12) d
| rowspan=2|396.1(12) d
| [[Electron capture|EC]]
| 5/2+
| <sup>235</sup>U
| rowspan=2|5/2+
|-
|-
| α (.0026%)
| {{SimpleNuclide2|Neptunium|236}}
| <sup>231</sup>Pa
| style="text-align:right" | 93
| style="text-align:right" | 143
| 236.04657(5)
| 1.54(6)E+5 a
| (6-)
|-
|-
| style="text-indent:1em" | {{SimpleNuclide2|Neptunium|236m}}
| rowspan=3|{{SimpleNuclide2|Neptunium|236}}
| colspan="3" style="text-indent:2em" | 60(50) keV
| rowspan=3 style="text-align:right" | 93
| rowspan=3 style="text-align:right" | 143
| 22.5(4) h
| rowspan=3|236.04657(5)
| 1
| rowspan=3|1.54(6)E+5 a
| EC (87.3%)
| <sup>236</sup>U
| rowspan=3|(6-)
|-
|-
| β<sup>-</sup> (12.5%)
| {{SimpleNuclide2|Neptunium|237}}
| <sup>236</sup>Pu
| style="text-align:right" | 93
|-
| style="text-align:right" | 144
| 237.0481734(20)
| α (.16%)
| <sup>232</sup>Pa
| 2.144(7)E+6 a
|-
| 5/2+
| rowspan=2 style="text-indent:1em" | {{SimpleNuclide2|Neptunium|236m}}
| rowspan=2 colspan="3" style="text-indent:2em" | 60(50) keV
| rowspan=2|22.5(4) h
| EC (52%)
| <sup>236</sup>U
| rowspan=2|1
|-
| β<sup>-</sup> (48%)
| <sup>236</sup>Pu
|-
| rowspan=3|{{SimpleNuclide2|Neptunium|237}}
| rowspan=3 style="text-align:right" | 93
| rowspan=3 style="text-align:right" | 144
| rowspan=3|237.0481734(20)
| rowspan=3|2.144(7)E+6 a
| α
| <sup>233</sup>Pa
| rowspan=3|5/2+
|-
| [[Spontaneous fission|SF]] (2E-10%)
| (various)
|-
| [[Cluster decay|CD]] (4E-12%)
| <sup>207</sup>Tl, <sup>30</sup>Mg
|-
|-
| {{SimpleNuclide2|Neptunium|238}}
| {{SimpleNuclide2|Neptunium|238}}
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| 238.0509464(20)
| 238.0509464(20)
| 2.117(2) d
| 2.117(2) d
| β<sup>-</sup>
| <sup>238</sup>Pu
| 2+
| 2+
|-
|-
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| colspan="3" style="text-indent:2em" | 2300(200)# keV
| colspan="3" style="text-indent:2em" | 2300(200)# keV
| 112(39) ns
| 112(39) ns
|
|
|
|
|-
|-
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| 239.0529390(22)
| 239.0529390(22)
| 2.356(3) d
| 2.356(3) d
| β<sup>-</sup>
| <sup>239</sup>Pu
| 5/2+
| 5/2+
|-
|-
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| 240.056162(16)
| 240.056162(16)
| 61.9(2) min
| 61.9(2) min
| β<sup>-</sup>
| <sup>240</sup>Pu
| (5+)
| (5+)
|-
|-
| style="text-indent:1em" | {{SimpleNuclide2|Neptunium|240m}}
| rowspan=2 style="text-indent:1em" | {{SimpleNuclide2|Neptunium|240m}}
| colspan="3" style="text-indent:2em" | 20(15) keV
| rowspan=2 colspan="3" style="text-indent:2em" | 20(15) keV
| 7.22(2) min
| rowspan=2|7.22(2) min
| 1(+)
| rowspan=2|1(+)
| β<sup>-</sup> (99.89%)
| <sup>240</sup>Pu
|-
| [[Isomeric transition|IT]] (.11%)
| <sup>240</sup>Np
|-
|-
| {{SimpleNuclide2|Neptunium|241}}
| {{SimpleNuclide2|Neptunium|241}}
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| 241.05825(8)
| 241.05825(8)
| 13.9(2) min
| 13.9(2) min
| β<sup>-</sup>
| <sup>241</sup>Pu
| (5/2+)
| (5/2+)
|-
|-
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| 242.06164(21)
| 242.06164(21)
| 2.2(2) min
| 2.2(2) min
| β<sup>-</sup>
| <sup>242</sup>Pu
| (1+)
| (1+)
|-
|-
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| colspan="3" style="text-indent:2em" | 0(50)# keV
| colspan="3" style="text-indent:2em" | 0(50)# keV
| 5.5(1) min
| 5.5(1) min
|
|
| 6+#
| 6+#
|-
|-
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| 243.06428(3)#
| 243.06428(3)#
| 1.85(15) min
| 1.85(15) min
| β<sup>-</sup>
| <sup>243</sup>Pu
| (5/2-)
| (5/2-)
|-
|-
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| 244.06785(32)#
| 244.06785(32)#
| 2.29(16) min
| 2.29(16) min
| β<sup>-</sup>
| <sup>244</sup>Pu
| (7-)
| (7-)
|}
|}

Revision as of 12:24, 18 May 2011

Neptunium (Np) has no stable isotopes. A standard atomic mass cannot be given.

19 neptunium radioisotopes have been characterized, with the most stable being 237
Np
with a half-life of 2.14 million years, 236
Np
with a half-life of 154,000 years, and 235
Np
with a half-life of 396.1 days. All of the remaining radioactive isotopes have half-lives that are less than 4.5 days, and the majority of these have half lifes that are less than 50 minutes. This element also has 4 meta states, with the most stable being 236m
Np
(t½ 22.5 hours).

The isotopes of neptunium range in atomic weight from 225.0339 u (225
Np
) to 244.068 u (244
Np
). The primary decay mode before the most stable isotope, 237
Np
, is electron capture (with a good deal of alpha emission), and the primary mode after is beta emission. The primary decay products before 237
Np
are element 92 (uranium) isotopes (alpha emission produces element 91, protactinium, however) and the primary products after are element 94 (plutonium) isotopes.

Some notable isotopes

Neptunium-235

Neptunium-235 is a radioactive isotope of neptunium with 93 electrons and protons and 142 neutrons. It has a half-life of 400 days. This isotope of Neptunium either decays by:

This particular isotope of neptunium has a weight of 235.0440633 grams/mole. It is not abundant in nature because it is unstable.

Neptunium-236

Neptunium-236 is a radioactive isotope of neptunium with 93 electrons and protons and 143 neutrons. It has a half-life of 154,000 years. It can decay by the following methods -

This particular isotope of neptunium has a mass of 236.04657 grams/mole. It is a fissile material with a critical mass of 7 kg. It is not found on earth because it is unstable.

possible parent nuclides: alpha from Am-240

Neptunium-237

Neptunium-237 decay scheme (simplified)
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

237
Np
decays via the neptunium series to thallium, unlike most other actinides which decay to isotopes of lead.

237
Np
was recently shown to be capable of sustaining a chain reaction with fast neutrons, as in a nuclear weapon.[6] However, it has a low probability of fission on bombardment with thermal neutrons, which makes it unsuitable as a fuel for nuclear power plants.

237
Np
is the only neptunium isotope produced in significant quantity in the nuclear fuel cycle, both by successive neutron capture on uranium-235 (which fissions most but not all of the time) and uranium-236, or (n,2n) reactions where a fast neutron occasionally knocks a neutron loose from uranium-238 or isotopes of plutonium. Over the long term, 237
Np
also forms in spent nuclear fuel as the decay product of americium-241.

237
Np
is projected to be one of the most mobile nuclides at the Yucca Mountain nuclear waste repository.

Table

nuclide
symbol
Z(p) N(n)  
isotopic mass (u)
 
half-life decay
mode(s)[7][n 1]
daughter
isotope(s)
nuclear
spin
excitation energy
225
Np
93 132 225.03391(8) 3# ms [>2 µs] α 221Pa 9/2-#
226
Np
93 133 226.03515(10)# 35(10) ms α 222Pa
227
Np
93 134 227.03496(8) 510(60) ms α (99.95%) 223Pa 5/2-#
β+ (.05%) 227U
228
Np
93 135 228.03618(21)# 61.4(14) s β+ (59%) 228U
α (41%) 224Pa
β+, SF (.012%) (various)
229
Np
93 136 229.03626(9) 4.0(2) min α (51%) 225Pa 5/2+#
β+ (49%) 229U
230
Np
93 137 230.03783(6) 4.6(3) min β+ (97%) 230U
α (3%) 226Pa
231
Np
93 138 231.03825(5) 48.8(2) min β+ (98%) 231U (5/2)(+#)
α (2%) 227Pa
232
Np
93 139 232.04011(11)# 14.7(3) min β+ (99.99%) 232U (4+)
α (.003%) 228Pa
233
Np
93 140 233.04074(5) 36.2(1) min β+ (99.99%) 233U (5/2+)
α (.001%) 229Pa
234
Np
93 141 234.042895(9) 4.4(1) d β+ 234U (0+)
235
Np
93 142 235.0440633(21) 396.1(12) d EC 235U 5/2+
α (.0026%) 231Pa
236
Np
93 143 236.04657(5) 1.54(6)E+5 a EC (87.3%) 236U (6-)
β- (12.5%) 236Pu
α (.16%) 232Pa
236m
Np
60(50) keV 22.5(4) h EC (52%) 236U 1
β- (48%) 236Pu
237
Np
93 144 237.0481734(20) 2.144(7)E+6 a α 233Pa 5/2+
SF (2E-10%) (various)
CD (4E-12%) 207Tl, 30Mg
238
Np
93 145 238.0509464(20) 2.117(2) d β- 238Pu 2+
238m
Np
2300(200)# keV 112(39) ns
239
Np
93 146 239.0529390(22) 2.356(3) d β- 239Pu 5/2+
240
Np
93 147 240.056162(16) 61.9(2) min β- 240Pu (5+)
240m
Np
20(15) keV 7.22(2) min 1(+) β- (99.89%) 240Pu
IT (.11%) 240Np
241
Np
93 148 241.05825(8) 13.9(2) min β- 241Pu (5/2+)
242
Np
93 149 242.06164(21) 2.2(2) min β- 242Pu (1+)
242m
Np
0(50)# keV 5.5(1) min 6+#
243
Np
93 150 243.06428(3)# 1.85(15) min β- 243Pu (5/2-)
244
Np
93 151 244.06785(32)# 2.29(16) min β- 244Pu (7-)

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.

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. ^ P. Weiss (26 October 2002). "Little-studied metal goes critical - Neptunium Nukes?". Science News. Retrieved 2006-09-29.
  7. ^ http://www.nucleonica.net/unc.aspx