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Isotopes of selenium

From Wikipedia, the free encyclopedia

Isotopes ofselenium (34Se)
Main isotopes[1]Decay
abun­dancehalf-life(t1/2)modepro­duct
72Sesynth8.4 dε72As
74Se0.860%stable
75Sesynth119.8 dε75As
76Se9.23%stable
77Se7.60%stable
78Se23.7%stable
79Setrace3.27×105 yβ79Br
80Se49.8%stable
82Se8.82%8.76×1019 yββ82Kr
Standard atomic weightAr°(Se)

Selenium has six naturalisotopes that occur in significant quantities, along with the trace isotope79Se, which occurs in minute quantities inuranium ores. Five of these isotopes arestable:74Se,76Se,77Se,78Se, and80Se. The last three also occur asfission products, along with79Se, which has ahalf-life of 327,000 years,[4][5] and82Se, which has a very long half-life (~1020 years, decaying viadouble beta decay to82Kr) and for practical purposes can be considered to be stable. There are 23 other unstable isotopes that have been characterized, the longest-lived being79Se with a half-life 327,000 years,75Se with a half-life of 120 days, and72Se with a half-life of 8.40 days. Of the other isotopes,73Se has the longest half-life, 7.15 hours; most others have half-lives not exceeding 38 seconds.

List of isotopes

[edit]
Nuclide
[n 1]
ZNIsotopic mass(Da)[6]
[n 2][n 3]
Half-life[1]
[n 4][n 5]
Decay
mode
[1]
[n 6]
Daughter
isotope

[n 7]
Spin and
parity[1]
[n 8][n 5]
Natural abundance(mole fraction)
Excitation energyNormal proportion[1]Range of variation
63Se342962.98191(54)#13.2(39) msβ+,p (89%)62Ge3/2−#
β+ (11%)63As
2p? (<0.5%)61Ge
64Se343063.97117(54)#22.6(2) msβ+?64As0+
β+, p?63Ge
65Se343164.96455(32)#34.2(7) msβ+, p (87%)64Ge3/2−#
β+ (13%)65As
66Se343265.95528(22)#54(4) msβ+66As0+
β+, p?65Ge
67Se343366.949994(72)133(4) msβ+ (99.5%)67As5/2−#
β+, p (0.5%)66Ge
68Se343467.94182524(53)35.5(7) sβ+68As0+
69Se343568.9394148(16)27.4(2) sβ+ (99.95%)69As1/2−
β+, p (.052%)68Ge
69m1Se38.85(22) keV2.0(2) μsIT69Se5/2−
69m2Se574.0(4) keV955(16) nsIT69Se9/2+
70Se343669.9335155(17)41.1(3) minβ+70As0+
71Se343770.9322094(30)4.74(5) minβ+71As(5/2−)
71m1Se48.79(5) keV5.6(7) μsIT71Se(1/2−)
71m2Se260.48(10) keV19.0(5) μsIT71Se(9/2+)
72Se343871.9271405(21)8.40(8) dEC72As0+
73Se343972.9267549(80)7.15(9) hβ+73As9/2+
73mSe25.71(4) keV39.8(17) minIT (72.6%)73Se3/2−
β+ (27.4%)73As
74Se344073.922475933(15)Observationally Stable[n 9]0+0.0086(3)
75Se344174.922522870(78)119.78(3) dEC75As5/2+
76Se344275.919213702(17)Stable0+0.0923(7)
77Se[n 10]344376.919914150(67)Stable1/2−0.0760(7)
77mSe161.9223(10) keV17.36(5) sIT77Se7/2+
78Se[n 10]344477.91730924(19)Stable0+0.2369 (22)
79Se[n 11]344578.91849925(24)3.27(28)×105 yβ79Br7/2+
79mSe95.77(3) keV3.900(18) minIT (99.94%)79Se1/2−
β (0.056%)79Br
80Se[n 10]344679.9165218(10)Observationally Stable[n 12]0+0.4980(36)
81Se[n 10]344780.9179930(10)18.45(12) minβ81Br1/2−
81mSe[n 10]103.00(6) keV57.28(2) minIT (99.95%)81Se7/2+
β (0.051%)81Br
82Se[n 10][n 13]344881.91669953(50)8.76(15)×1019 yββ82Kr0+0.0882(15)
83Se344982.9191186(33)22.25(4) minβ83Br9/2+
83mSe228.92(7) keV70.1(4) sβ83Br1/2−
84Se345083.9184668(21)3.26(10) minβ84Br0+
85Se345184.9222608(28)32.9(3) sβ85Br(5/2)+
86Se345285.9243117(27)14.3(3) sβ86Br0+
β,n?85Br
87Se345386.9286886(24)5.50(6) sβ (99.50%)87Br(3/2+)
β, n (0.60%)86Br
88Se345487.9314175(36)1.53(6) sβ (99.01%)88Br0+
β, n (0.99%)87Br
89Se345588.9366691(40)430(50) msβ (92.2%)89Br5/2+#
β, n (7.8%)88Br
90Se345689.94010(35)210(80) msβ90Br0+
β, n?89Br
91Se345790.94570(47)270(50) msβ (79%)91Br1/2+#
β, n (21%)90Br
β, 2n?89Br
92Se345891.94984(43)#90# ms [>300 ns]β?92Br0+
β, n?91Br
β, 2n?90Br
92mSe3072(2) keV15.7(7) μsIT92Se(9−)
93Se345992.95614(43)#130# ms [>300 ns]β?93Br1/2+#
β, n?92Br
β, 2n?91Br
93mSe678.2(7) keV420(100) nsIT93Se
94Se346093.96049(54)#50# ms [>300 ns]β?94Br0+
β, n?93Br
β, 2n?92Br
94mSe2430.0(6) keV680(50) nsIT94Se(7−)
95Se346194.96730(54)#70# ms [>400 ns]β?95Br3/2+#
β, n?94Br
β, 2n?93Br
96Se[7]3462
97Se[7]3463
This table header & footer:
  1. ^mSe – Excitednuclear isomer.
  2. ^( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  3. ^# – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
  4. ^Bold half-life – nearly stable, half-life longer thanage of universe.
  5. ^ab# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  6. ^Modes of decay:
    EC:Electron capture


    IT:Isomeric transition
    n:Neutron emission
    p:Proton emission
  7. ^Bold symbol as daughter – Daughter product is stable.
  8. ^( ) spin value – Indicates spin with weak assignment arguments.
  9. ^Theoretically capable of β+β+ decay to74Ge; half-life is above2.3×1018 y.
  10. ^abcdefFission product
  11. ^Long-lived fission product
  12. ^Theoretically capable of ββ decay to80Kr
  13. ^Primordialradionuclide

Use of radioisotopes

[edit]

The isotope selenium-75 hasradiopharmaceutical uses. For example, it is used in high-dose-rate endorectalbrachytherapy, as an alternative toiridium-192.[8]

In paleobiogeochemistry, the ratio in amount of selenium-82 to selenium-76 (i.e, the value of δ82/76Se) can be used to track down theredox conditions on Earth during theNeoproterozoic era in order to gain a deeper understanding of therapid oxygenation that trigger the emergence of complex organisms.[9][10]

See also

[edit]

Daughter products other than selenium

References

[edit]
  1. ^abcdeKondev, 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.
  2. ^"Standard Atomic Weights: Selenium".CIAAW. 2013.
  3. ^Prohaska, Thomas; Irrgeher, Johanna; Benefield, Jacqueline; Böhlke, John K.; Chesson, Lesley A.; Coplen, Tyler B.; Ding, Tiping; Dunn, Philip J. H.; Gröning, Manfred; Holden, Norman E.; Meijer, Harro A. J. (2022-05-04)."Standard atomic weights of the elements 2021 (IUPAC Technical Report)".Pure and Applied Chemistry.doi:10.1515/pac-2019-0603.ISSN 1365-3075.
  4. ^The half-life of79SeArchived September 27, 2011, at theWayback Machine
  5. ^Jorg, Gerhard; Buhnemann, Rolf; Hollas, Simon; Kivel, Niko; Kossert, Karsten; Van Winckel, Stefaan; Gostomski, Christoph Lierse v. (2010). "Preparation of radiochemically pure79Se and highly precise determination of its half-life".Applied Radiation and Isotopes.68 (12):2339–51.doi:10.1016/j.apradiso.2010.05.006.PMID 20627600.
  6. ^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.
  7. ^abShimizu, Y.; Kubo, T.; Sumikama, T.; Fukuda, N.; Takeda, H.; Suzuki, H.; Ahn, D. S.; Inabe, N.; Kusaka, K.; Ohtake, M.; Yanagisawa, Y.; Yoshida, K.; Ichikawa, Y.; Isobe, T.; Otsu, H.; Sato, H.; Sonoda, T.; Murai, D.; Iwasa, N.; Imai, N.; Hirayama, Y.; Jeong, S. C.; Kimura, S.; Miyatake, H.; Mukai, M.; Kim, D. G.; Kim, E.; Yagi, A. (8 April 2024). "Production of new neutron-rich isotopes near the N = 60 isotones Ge 92 and As 93 by in-flight fission of a 345 MeV/nucleon U 238 beam".Physical Review C.109 (4).doi:10.1103/PhysRevC.109.044313.
  8. ^Shoemaker T; Vuong T; Glickman H; Kaifi S; Famulari G; Enger SA (2019). "Dosimetric Considerations for Ytterbium-169, Selenium-75, and Iridium-192 Radioisotopes in High-Dose-Rate Endorectal Brachytherapy".Int J Radiat Oncol Biol Phys.105 (4):875–883.doi:10.1016/j.ijrobp.2019.07.003.PMID 31330175.S2CID 198170324.
  9. ^Pogge von Strandmann, Philip A. E.; Stüeken, Eva E.; Elliott, Tim; Poulton, Simon W.; Dehler, Carol M.; Canfield, Don E.; Catling, David C. (2015-12-18)."Selenium isotope evidence for progressive oxidation of the Neoproterozoic biosphere".Nature Communications.6 (1): 10157.doi:10.1038/ncomms10157.ISSN 2041-1723.PMC 4703861.PMID 26679529.
  10. ^Stüeken, Eva E."Selenium isotopes as a biogeochemical proxy in deep time"(PDF).core.ac.uk.


Group12 3456789101112131415161718
PeriodHydrogen and
alkali metals
Alkaline
earth metals
Pnicto­gensChal­co­gensHalo­gensNoble gases
12
345678910
1112131415161718
192021222324252627282930313233343536
373839404142434445464748495051525354
55561 asterisk71727374757677787980818283848586
87881 asterisk103104105106107108109110111112113114115116117118
119120
1 asterisk5758596061626364656667686970 
1 asterisk8990919293949596979899100101102
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