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Isotopes of hafnium

From Wikipedia, the free encyclopedia

Isotopes ofhafnium (72Hf)
Main isotopes[1]Decay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
172Hfsynth1.87 yε172Lu
174Hf0.16%3.8×1016 y[2]α170Yb
175Hfsynth69.90 d[3]ε175Lu
176Hf5.26%stable
177Hf18.6%stable
178Hf27.3%stable
178m2Hfsynth31 yIT178Hf
179Hf13.6%stable
180Hf35.1%stable
181Hfsynth42.39 dβ181Ta
182Hfsynth8.90×106 yβ182Ta
Standard atomic weightAr°(Hf)

Naturalhafnium (72Hf) consists of five observationally stableisotopes (176Hf,177Hf,178Hf,179Hf, and180Hf) and one very long-livedradioisotope,174Hf, with ahalf-life of3.8×1016 years.[2] The next most stable radioisotope is182Hf with a half-life of 8.90 million years, anextinct radionuclide used inhafnium–tungsten dating to study the chronology ofplanetary differentiation.[6]

Other isotopes have been synthesized running from153Hf to192Hf, but none of the 33 others has a half-life over 1.87 years, and most have half-lives under five minutes. There are also at least 41nuclear isomers, the most stable of which is178m2Hf with a half-life of 31 years. All isotopes of hafnium are either radioactive orobservationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed.

List of isotopes

[edit]


Nuclide
[n 1]
ZNIsotopic mass(Da)[7]
[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 energy[n 5]Normal proportion[1]Range of variation
153Hf7281152.97069(32)#400# ms
[>200 ns]
1/2+#
154Hf7282153.96486(32)#2(1) sβ+154Lu0+
α (rare)150Yb
154mHf2721(50)# keV9(4) μsIT154Hf(10+)
155Hf7283154.96317(32)#843(30) msβ+155Lu7/2−#
156Hf7284155.95940(16)23(1) msα152Yb0+
156mHf1958.8(10) keV480(40) μsα152Yb(8+)
157Hf7285156.95829(22)#115(1) msα (94%)153Yb7/2−
β+ (6%)157Lu
158Hf7286157.954801(19)2.85(7) sβ+ (55.7%)158Lu0+
α (44.3%)154Yb
159Hf7287158.953996(18)5.20(10) sβ+ (65%)159Lu7/2−
α (35%)155Yb
160Hf7288159.950683(10)13.6(2) sβ+ (99.3%)160Lu0+
α (0.7%)156Yb
161Hf7289160.950278(25)18.4(4) sβ+ (99.71%)161Lu(7/2−)
α (0.29%)157Yb
161mHf329.0(5) keV4.8(2) μsIT161Hf(13/2+)
162Hf7290161.9472155(96)39.4(9) sβ+ (99.99%)162Lu0+
α (0.008%)158Yb
163Hf7291162.947107(28)40.0(6) sβ+163Lu(5/2−)
164Hf7292163.944371(17)111(8) sβ+164Lu0+
165Hf7293164.944567(30)76(4) sβ+165Lu(5/2−)
166Hf7294165.942180(30)6.77(30) minβ+166Lu0+
167Hf7295166.942600(30)2.05(5) minβ+167Lu(5/2)−
168Hf7296167.940568(30)25.95(20) minEC (98%)168Lu0+
β+ (2%)168Lu
169Hf7297168.941259(30)3.24(4) minβ+169Lu(5/2−)
170Hf7298169.939609(30)16.01(13) hEC170Lu0+
171Hf7299170.940492(31)12.1(4) hβ+171Lu7/2+
171mHf21.93(9) keV29.5(9) sIT171Hf1/2−
172Hf72100171.939450(26)1.87(3) yEC172Lu0+
172mHf2005.84(11) keV163(3) nsIT172Hf(8−)
173Hf72101172.940513(30)23.6(1) hβ+173Lu1/2−
173m1Hf107.16(5) keV180(8) nsIT173Hf5/2−
173m2Hf197.47(10) keV160(40) nsIT173Hf7/2+
174Hf[n 9]72102173.9400484(24)3.8+1.7
−0.9
×1016 y
[2]
α[n 10]170Yb0+0.0016(12)
174m1Hf1549.26(4) keV138(4) nsIT174Hf6+
174m2Hf1797.59(7) keV2.39(4) μsIT174Hf8−
174m3Hf3312.07(6) keV3.7(2) μsIT174Hf14+
175Hf72103174.9415114(25)69.90(7) d[3]EC175Lu5/2−
175m1Hf125.89(12) keV53.7(15) μsIT175Hf1/2−
175m2Hf1433.41(12) keV1.10(8) μsIT175Hf19/2+
175m3Hf3015.6(4) keV1.21(15) μsIT175Hf35/2−
175m4Hf4636.2(12) keV1.9(1) μsIT175Hf45/2+
176Hf[n 11]72104175.9414098(16)Observationally Stable[n 12]0+0.0526(70)
176m1Hf1333.07(7) keV9.6(3) μsIT176Hf6+
176m2Hf1559.31(9) keV9.9(2) μsIT176Hf8−
176m3Hf2865.8(7) keV401(6) μsIT176Hf14−
176m4Hf4863.6(9) keV43(4) μsIT176Hf22−
177Hf72105176.9432302(15)Observationally Stable[n 13]7/2−0.1860(16)
177m1Hf1315.4502(8) keV1.09(5) sIT177Hf23/2+
177m2Hf1342.4(10) keV55.9(12) μsIT177Hf(19/2−)
177m3Hf2740.02(15) keV51.4(5) minIT177Hf37/2−
178Hf72106177.9437083(15)Observationally Stable[n 14]0+0.2728(28)
178m1Hf1147.416(6) keV4.0(2) sIT178Hf8−
178m2Hf2446.09(8) keV31(1) yIT178Hf16+
178m3Hf2572.4(3) keV68(2) μsIT178Hf14−
179Hf72107178.9458257(15)Observationally Stable[n 15]9/2+0.1362(11)
179m1Hf375.0352(25) keV18.67(4) sIT179Hf1/2−
179m2Hf1106.412(33) keV25.00(17) dIT179Hf25/2−
179m3Hf3775.2(21) keV15(5) μsIT179Hf(43/2+)
180Hf72108179.9465595(15)Observationally Stable[n 16]0+0.3508(33)
180m1Hf1141.552(15) keV5.53(2) hIT (99.69%)180Hf8−
β (0.31%)180m1Ta[8]
180m2Hf1374.36(4) keV570(20) μsIT180Hf4−
180m3Hf2485.5(5) keV0.94(11) μsIT180Hf12+
180m4Hf3599.0(10) keV90(10) μsIT180Hf(18−)
181Hf72109180.9491108(15)42.39(6) dβ181Ta1/2−
181m1Hf595.27(4) keV80(5) μsIT181Hf(9/2+)
181m2Hf1043.5(8) keV~100 μsIT181Hf(17/2+)
181m3Hf1741.9(13) keV1.5(5) msIT181Hf(25/2−)
182Hf[n 17]72110181.9505637(66)8.90(9)×106 yβ182Ta0+
182m1Hf1172.87(18) keV61.5(15) minβ (54%)182Ta8−
IT (46%)182Hf
182m2Hf2571.3(12) keV40(10) μsIT182Hf(13+)
183Hf72111182.953533(32)1.018(2) hβ183Ta(3/2−)
183mHf1464(64) keV40(30) sIT183Hf27/2−#
184Hf72112183.955449(43)4.12(5) hβ184Ta0+
184m1Hf1272.2(4) keV48(10) sIT184Hf8−
184m2Hf2477(10) keV16(7) min15+#
185Hf72113184.958862(69)3.5(6) minβ185Ta(9/2−)
186Hf72114185.960897(55)2.6(12) minβ186Ta0+
186mHf2968(43) keV>20 s17+#
187Hf72115186.96457(22)#14# s
[>300 ns]
9/2−#
187mHf500(300)# keV270(80) nsIT187Hf3/2−#
188Hf72116187.96690(32)#7# s
[>300 ns]
0+
189Hf72117188.97085(32)#400# ms
[>300 ns]
3/2−#
190Hf72118189.97338(43)#600# ms
[>300 ns]
0+
191Hf[9]72119
192Hf[9]721200+
This table header & footer:
  1. ^mHf – 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. ^abc# – 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
  7. ^Bold symbol as daughter – Daughter product is stable.
  8. ^( ) spin value – Indicates spin with weak assignment arguments.
  9. ^primordialradionuclide
  10. ^Theorized to also undergo β+β+ decay to174Yb
  11. ^Used inlutetium-hafnium dating
  12. ^Believed to undergo α decay to172Yb
  13. ^Believed to undergo α decay to173Yb with a half-life over 1.3×1018 y.
  14. ^Believed to undergo α decay to174Yb
  15. ^Believed to undergo α decay to175Yb
  16. ^Believed to undergo α decay to176Yb
  17. ^Extinct radionuclide, used inhafnium–tungsten dating[6]

See also

[edit]

Daughter products other than hafnium

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. ^abcBelli, P.; Bernabei, R.; Cappella, F.; Caracciolo, V.; Cerulli, R.; Incicchitti, A.; Laubenstein, M.; Leoncini, A.; Merlo, V.; Nagorny, S.S.; Nahorna, V.V.; Nisi, S.; Wang, P. (January 2025). "A new measurement of 174Hf alpha decay".Nuclear Physics A.1053 122976.doi:10.1016/j.nuclphysa.2024.122976.
  3. ^abKmak, K. N.; Neupane, S.; Kolos, K.; et al. (2025)."Measurement of the175Hf half-life".Physical Review C.111 (024308).doi:10.1103/PhysRevC.111.024308.
  4. ^"Standard Atomic Weights: Hafnium".CIAAW. 2019.
  5. ^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.
  6. ^abKleine T, Walker RJ (August 2017)."Tungsten Isotopes in Planets".Annual Review of Earth and Planetary Sciences.45 (1):389–417.Bibcode:2017AREPS..45..389K.doi:10.1146/annurev-earth-063016-020037.PMC 6398955.PMID 30842690.
  7. ^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.
  8. ^McCutchan, E.A. (May 2015)."Nuclear Data Sheets for A = 180".Nuclear Data Sheets.126:151–372.doi:10.1016/j.nds.2015.05.002.
  9. ^abHaak, K.; Tarasov, O. B.; Chowdhury, P.; et al. (2023). "Production and discovery of neutron-rich isotopes by fragmentation of198Pt".Physical Review C.108 (34608) 034608.Bibcode:2023PhRvC.108c4608H.doi:10.1103/PhysRevC.108.034608.S2CID 261649436.
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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