See also: list of Niobium isotopes.
Half-life T½ = 3.47(24) × 107 a respectively 1.0942992 × 1015 seconds s.
Decay mode | Daughter | Probability | Decay energy | γ energy (intensity) |
---|---|---|---|---|
β+ | 92Zr | > 99.95 % | 2.0057(18) MeV | |
β- | 92Mo | < 0.05 % | 0.3553(18) MeV |
Nuclear isomers or excited states with the activation energy in keV related to the ground state.
Nuclear Isomer | Excitation Energy | Half-life | Spin |
---|---|---|---|
92m1Nb | 135.5(4) keV | 10.15(2) d | (2)+ |
92m2Nb | 225.8(4) keV | 5.9(2) μs | (2)- |
92m3Nb | 2203.3(4) keV | 167(4) ns | (11-) |
Z | Isotone N = 51 | Isobar A = 92 |
---|---|---|
28 | 79Ni | |
29 | 80Cu | |
30 | 81Zn | |
31 | 82Ga | |
32 | 83Ge | |
33 | 84As | 92As |
34 | 85Se | 92Se |
35 | 86Br | 92Br |
36 | 87Kr | 92Kr |
37 | 88Rb | 92Rb |
38 | 89Sr | 92Sr |
39 | 90Y | 92Y |
40 | 91Zr | 92Zr |
41 | 92Nb | 92Nb |
42 | 93Mo | 92Mo |
43 | 94Tc | 92Tc |
44 | 95Ru | 92Ru |
45 | 96Rh | 92Rh |
46 | 97Pd | 92Pd |
47 | 98Ag | 92Ag |
48 | 99Cd | |
49 | 100In | |
50 | 101Sn |
[1] - Maria Schönbächler, Mark Rehkämper, Alex N. Halliday, Der-Chuen Lee, Michèle Bourot-Denise, Brigitte Zanda, Bodo Hattendorf, Detlef Günther:
Niobium-Zirconium Chronometry and Early Solar System Development.
In: Science, (2002), DOI 10.1126/science.1067400.
[2] - Makiko K. Haba, Yi-Jen Lai, Jörn-Frederik Wotzlaw, Akira Yamaguchi, Maria Lugaro, Maria Schönbächler:
Precise initial abundance of Niobium-92 in the Solar System and implications for p-process nucleosynthesis.
In: Proceedings of the National Academy of Sciences of the USA, PNAS, (2021), DOI 10.1073/pnas.2017750118.
Last update: 2021-03-01
Perma link: https://www.chemlin.org/isotope/niobium-92
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