Difference between revisions of "Isotopes of fermium"

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| 69 260(220)#
 
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| 69 010(280)
 
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| 145
 
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| 70220(280)#
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| 70 220(280)#
 
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| align=center | +½#
+
| align=center | +{{frac|2}}#
 
| 4.2(13) s
 
| 4.2(13) s
 
| α (? %); β<sup>+</sup> (4.2%#); SF (0.13%#)
 
| α (? %); β<sup>+</sup> (4.2%#); SF (0.13%#)
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|-
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| <sup>246</sup>Fm
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| 100
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| 146
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|
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| 70 140(40)
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|
 +
|
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| align=center | 0
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| 1.1(2) s
 +
| α (? %); β<sup>+</sup> (> 10%); SF (4.5–13%); β<sup>+</sup>SF (10–5%)
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|-
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| <sup>247</sup>Fm
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| 100
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| 147
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| 71 580(140)#
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| align=center | +{{frac|5|2}}#
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| 35(4) s
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| α (≥ 50%); β<sup>+</sup> (≤ 50%)
 
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| colspan=10 | Values marked # are estimated from systematic trends rather than experimentally measured.<br/>Spins quoted in parentheses are uncertain in value and/or parity.<br/>''Sources'': Except as otherwise noted,  
 
| colspan=10 | Values marked # are estimated from systematic trends rather than experimentally measured.<br/>Spins quoted in parentheses are uncertain in value and/or parity.<br/>''Sources'': Except as otherwise noted,  

Revision as of 16:28, 24 September 2010

Fermium is an artificial element, and has no stable or naturally occuring isotopes. The first isotope to be discovered was 255100Fm, in fallout from the first test of a hydrogen bomb, codenamed 'Ivy Mike', in 1952. 250100Fm was discovered independently in 1954.

Symbol Z(p) N(n) Mass/u Excess energy
MeV
Binding energy/A
MeV
β-decay energy
MeV
Spin Half life Decay mode,
proportion
Excitation energy/MeV
242Fm 100 142 242.073 43(43)# 68 400(401)# 7465(2)# 0 0.8(2) ms SF (? %); α (? %)
243Fm 100 143 69 260(220)# 72# 210(60) ms α;[Note 1] β+ (? %); SF (59%#)
244Fm 100 144 69 010(280) 0 3.3(0.5) ms SF (≈100%); α (0.4%#)
245Fm 100 145 70 220(280)# +12# 4.2(13) s α (? %); β+ (4.2%#); SF (0.13%#)
246Fm 100 146 70 140(40) 0 1.1(2) s α (? %); β+ (> 10%); SF (4.5–13%); β+SF (10–5%)
247Fm 100 147 71 580(140)# +52# 35(4) s α (≥ 50%); β+ (≤ 50%)
Values marked # are estimated from systematic trends rather than experimentally measured.
Spins quoted in parentheses are uncertain in value and/or parity.
Sources: Except as otherwise noted,
isotopic masses and associated energies are taken from the AME 2003 dataset;[1]
nuclear spins and decay properties are taken from NUBASE 2003.[2]

Notes and references

Notes

  1. The α ranching ratio depends on the uncertain branching ratio of the daughter 239Cf.

References

  1. Wapstra, A. H.; Audi, G.; Thibault, C. The AME2003 atomic mass evaluation (I). Evaluation of input data, adjustment procedures. Nucl. Phys. A 2003, 729, 129–336. DOI: 10.1016/j.nuclphysa.2003.11.002. Wapstra, A. H.; Audi, G.; Thibault, C. The AME2003 atomic mass evaluation (II). Tables, graphs, and references. Nucl. Phys. A 2003, 729, 337–676. DOI: 10.1016/j.nuclphysa.2003.11.003. Data tables.
  2. Audi, G.; Bersillon, O.; Blachot, J.; Wapstra, A. H. The NUBASE evaluation of nuclear and decay properties. Nucl. Phys. A 2003, 729, 3–128. doi:10.1016/j.nuclphysa.2003.11.001, <http://amdc.in2p3.fr/nubase/Nubase2003.pdf>.
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