Isotopes of niobium
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Standard atomic weight Ar°(Nb) | ||||||||||||||||||||||||||||||||||||||||||||||||
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Naturally occurring niobium (41Nb) is composed of one stable isotope (93Nb). The most stable radioisotope is 92Nb with a half-life of 34.7 million years, followed by are 94Nb at a half-life of 20,400 years and 91Nb at 680 years. Other radioisotopes that have been synthesized range from 82Nb to 110Nb; these have half-lives that are less than two hours, except 95Nb (34.991 days), 96Nb (23.35 hours) and 90Nb (14.60 hours).
The most stable of the meta states is 93mNb with excitation energy 31 keV and a 16.1 year half-life; this is produced in the decay of 93Zr. The primary decay mode before stable 93Nb is electron capture to zirconium isotopes and the primary mode after is beta emission, with delayed neutron emission starting at 104Nb, leading to molybdenum isotopes.
Only 95Nb, along with 97Nb (72 minutes) and heavier isotopes (seconds) are fission products in significant quantity, as the other isotopes are shadowed by stable or very long-lived (93) isotopes of the preceding element zirconium from the usual mode of production through beta decay of neutron-rich fission fragments. 95Nb is the decay product of 95Zr (64 days), so disappearance of 95Nb in used nuclear fuel is slower than would be expected from its own 35-day half-life alone.
List of isotopes
Nuclide [n 1] |
Z | N | Isotopic mass (Da)[4] [n 2][n 3] |
Half-life[1] [n 4] |
Decay mode[1] [n 5] |
Daughter isotope [n 6][n 7] |
Spin and parity[1] [n 8][n 4] |
Isotopic abundance | |||||||||||
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Excitation energy[n 4] | |||||||||||||||||||
81Nb | 41 | 40 | |||||||||||||||||
82Nb | 41 | 41 | 81.94438(32) | 51(5) ms | β+ | 82Zr | (0+) | ||||||||||||
82mNb | 1180(1) keV | 93(20) ns | IT | 82Nb | (5+) | ||||||||||||||
83Nb | 41 | 42 | 82.93815(17) | 3.9(2) s | β+ | 83Zr | 9/2+# | ||||||||||||
84Nb | 41 | 43 | 83.93430571(43) | 9.8(9) s | β+ | 84Zr | (1+) | ||||||||||||
84m1Nb | 48(1) keV | 176(46) ns | IT | 84Nb | (3+) | ||||||||||||||
84m2Nb | 337.7(4) keV | 92(5) ns | IT | 84Nb | (5−) | ||||||||||||||
85Nb | 41 | 44 | 84.9288458(44) | 20.5(7) s | β+ | 85Zr | 9/2+# | ||||||||||||
85mNb | 150(80)# keV | 3.3(9) s | IT (?%) | 85Nb | (1/2−) | ||||||||||||||
β+ (?%) | 85Zr | ||||||||||||||||||
86Nb | 41 | 45 | 85.9257815(59) | 88(1) s | β+ | 86Zr | (6+) | ||||||||||||
86mNb[n 9] | 150(100)# keV | 20# s | β+ | 86Zr | (0−,1−,2−) | ||||||||||||||
87Nb | 41 | 46 | 86.9206925(73) | 3.7(1) min | β+ | 87Zr | (1/2)− | ||||||||||||
87mNb | 3.9(1) keV | 2.6(1) min | β+ | 87Zr | (9/2)+ | ||||||||||||||
88Nb | 41 | 47 | 87.918226(62) | 14.50(11) min | β+ | 88Zr | (8+) | ||||||||||||
88mNb[n 9] | 130(120) keV | 7.7(1) min | β+ | 88Zr | (4−) | ||||||||||||||
89Nb | 41 | 48 | 88.913445(25) | 2.03(7) h | β+ | 89Zr | (9/2+) | ||||||||||||
89mNb[n 9] | 0(30)# keV | 1.10(3) h | β+ | 89Zr | (1/2)− | ||||||||||||||
90Nb | 41 | 49 | 89.9112592(36) | 14.60(5) h | β+ | 90Zr | 8+ | ||||||||||||
90m1Nb | 122.370(22) keV | 63(2) μs | IT | 90Nb | 6+ | ||||||||||||||
90m2Nb | 124.67(25) keV | 18.81(6) s | IT | 90Nb | 4- | ||||||||||||||
90m3Nb | 171.10(10) keV | <1 μs | IT | 90Nb | 7+ | ||||||||||||||
90m4Nb | 382.01(25) keV | 6.19(8) ms | IT | 90m1Nb | 1+ | ||||||||||||||
90m5Nb | 1880.21(20) keV | 471(6) ns | IT | 90Nb | (11−) | ||||||||||||||
91Nb | 41 | 50 | 90.9069903(31) | 680(130) y | EC (99.99%) | 91Zr | 9/2+ | ||||||||||||
β+ (0.0138%) | |||||||||||||||||||
91m1Nb | 104.60(5) keV | 60.86(22) d | IT (96.6%) | 91Nb | 1/2− | ||||||||||||||
EC (3.4%) | 91Zr | ||||||||||||||||||
β+ (0.0028%) | |||||||||||||||||||
91m2Nb | 2034.42(20) keV | 3.76(12) μs | IT | 91Nb | (17/2−) | ||||||||||||||
92Nb | 41 | 51 | 91.9071886(19) | 3.47(24)×107 y | β+ | 92Zr | 7+ | Trace | |||||||||||
92m1Nb | 135.5(4) keV | 10.116(13) d | β+ | 92Zr | (2)+ | ||||||||||||||
92m2Nb | 225.8(4) keV | 5.9(2) μs | IT | 92Nb | (2)− | ||||||||||||||
92m3Nb | 2203.3(4) keV | 167(4) ns | IT | 92Nb | (11−) | ||||||||||||||
93Nb | 41 | 52 | 92.9063732(16) | Stable | 9/2+ | 1.0000 | |||||||||||||
93m1Nb | 30.760(5) keV | 16.12(12) y | IT | 93Nb | 1/2− | ||||||||||||||
93m2Nb | 7460(17) keV | 1.5(5) μs | IT | 93Nb | 33/2−# | ||||||||||||||
94Nb | 41 | 53 | 93.9072790(16) | 2.04(4)×104 y | β− | 94Mo | 6+ | Trace | |||||||||||
94mNb | 40.892(12) keV | 6.263(4) min | IT (99.50%) | 94Nb | 3+ | ||||||||||||||
β− (0.50%) | 94Mo | ||||||||||||||||||
95Nb[n 10] | 41 | 54 | 94.90683111(55) | 34.991(6) d | β− | 95Mo | 9/2+ | ||||||||||||
95mNb[n 10] | 235.69(2) keV | 3.61(3) d | IT (94.4%) | 95Nb | 1/2− | ||||||||||||||
β− (5.6%) | 95Mo | ||||||||||||||||||
96Nb | 41 | 55 | 95.90810159(16) | 23.35(5) h | β− | 96Mo | 6+ | ||||||||||||
97Nb | 41 | 56 | 96.9081016(46) | 72.1(7) min | β− | 97Mo | 9/2+ | ||||||||||||
97mNb | 743.35(3) keV | 58.7(18) s | IT | 97Nb | 1/2− | ||||||||||||||
98Nb | 41 | 57 | 97.9103326(54) | 2.86(6) s | β− | 98Mo | 1+ | ||||||||||||
98mNb | 84(4) keV | 51.1(4) min | β− | 98Mo | (5)+ | ||||||||||||||
99Nb | 41 | 58 | 98.911609(13) | 15.0(2) s | β− | 99Mo | 9/2+ | ||||||||||||
99mNb | 365.27(8) keV | 2.5(2) min | β− (?%) | 99Mo | 1/2− | ||||||||||||||
IT (?%) | 99Nb | ||||||||||||||||||
100Nb | 41 | 59 | 99.9143406(86) | 1.5(2) s | β− | 100Mo | 1+ | ||||||||||||
100m1Nb | 313(8) keV | 2.99(11) s | β− | 100Mo | (5+) | ||||||||||||||
100m2Nb | 347(8) keV | 460(60) ns | IT | 100Nb | (4−,5−) | ||||||||||||||
100m3Nb | 734(8) keV | 12.43(26) μs | IT | 100Nb | (8−) | ||||||||||||||
101Nb | 41 | 60 | 100.9153065(40) | 7.1(3) s | β− | 101Mo | 5/2+ | ||||||||||||
102Nb | 41 | 61 | 101.9180904(27) | 4.3(4) s | β− | 102Mo | (4+) | ||||||||||||
102mNb | 94(7) keV | 1.31(16) s | β− | 102Mo | (1+) | ||||||||||||||
103Nb | 41 | 62 | 102.9194534(42) | 1.34(7) s | β− | 103Mo | 5/2+ | ||||||||||||
104Nb | 41 | 63 | 103.9229077(19) | 0.98(5) s | β− (99.95%) | 104Mo | (1+) | ||||||||||||
β−, n (0.05%) | 103Mo | ||||||||||||||||||
104mNb[n 9] | 9.8(26) keV | 4.9(3) s | β− (99.94%) | 104Mo | (0−,1−) | ||||||||||||||
β−, n (0.06%) | 103Mo | ||||||||||||||||||
105Nb | 41 | 64 | 104.9249426(43) | 2.91(5) s | β− (98.3%) | 105Mo | (5/2+) | ||||||||||||
β−, n (1.7%) | 104Mo | ||||||||||||||||||
106Nb | 41 | 65 | 105.9289285(15) | 900(20) ms | β− (95.5%) | 106Mo | 1−# | ||||||||||||
β−, n (4.5%) | 105Mo | ||||||||||||||||||
106m1Nb | 100(50)# keV | 1.20(6) s | β− | 106Mo | (4−) | ||||||||||||||
106m2Nb | 204.8(5) keV | 820(38) ns | IT | 106Nb | (3+) | ||||||||||||||
107Nb | 41 | 66 | 106.9315897(86) | 286(8) ms | β− (92.6%) | 107Mo | (5/2+) | ||||||||||||
β−, n (7.4%) | 106Mo | ||||||||||||||||||
108Nb | 41 | 67 | 107.9360756(88) | 201(4) ms | β− (93.7%) | 108Mo | (2+) | ||||||||||||
β−, n (6.3%) | 107Mo | ||||||||||||||||||
108mNb | 166.6(5) keV | 109(2) ns | IT | 108Nb | 6−# | ||||||||||||||
109Nb | 41 | 68 | 108.93914(46) | 106.9(49) ms | β− (69%) | 109Mo | 3/2−# | ||||||||||||
β−, n (31%) | 108Mo | ||||||||||||||||||
109mNb | 312.5(4) keV | 115(8) ns | IT | 109Nb | 7/2+# | ||||||||||||||
110Nb | 41 | 69 | 109.94384(90) | 75(1) ms | β− (60%) | 110Mo | 5+# | ||||||||||||
β−, n (40%) | 109Mo | ||||||||||||||||||
110mNb[n 9] | 100(50)# keV | 94(9) ms | β− (60%) | 110Mo | 2+# | ||||||||||||||
β−, n (40%) | 109Mo | ||||||||||||||||||
111Nb | 41 | 70 | 110.94744(32)# | 54(2) ms | β− | 111Mo | 3/2−# | ||||||||||||
112Nb | 41 | 71 | 111.95269(32)# | 38(2) ms | β− | 112Mo | 1+# | ||||||||||||
113Nb | 41 | 72 | 112.95683(43)# | 32(4) ms | β− | 113Mo | 3/2−# | ||||||||||||
114Nb | 41 | 73 | 113.96247(54)# | 17(5) ms | β− | 114Mo | 2−# | ||||||||||||
115Nb | 41 | 74 | 114.96685(54)# | 23(8) ms | β− | 115Mo | 3/2−# | ||||||||||||
116Nb | 41 | 75 | 115.97291(32)# | 12# ms [>550 ns] |
1−# | ||||||||||||||
117Nb[5] | 41 | 76 | |||||||||||||||||
This table header & footer: |
- ^ mNb – Excited nuclear isomer.
- ^ ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
- ^ # – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
- ^ a b c # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
- ^
Modes of decay:
EC: Electron capture
IT: Isomeric transition n: Neutron emission p: Proton emission - ^ Bold italics symbol as daughter – Daughter product is nearly stable.
- ^ Bold symbol as daughter – Daughter product is stable.
- ^ ( ) spin value – Indicates spin with weak assignment arguments.
- ^ a b c d e Order of ground state and isomer is uncertain.
- ^ a b Fission product
Niobium-92
Niobium-92 is an extinct radionuclide[6] with a half-life of 34.7 million years, decaying predominantly via β+ decay. Its abundance relative to the stable 93Nb in the early Solar System, estimated at 1.7×10−5, has been measured to investigate the origin of p-nuclei.[6][7] A higher initial abundance of 92Nb has been estimated for material in the outer protosolar disk (sampled from the meteorite NWA 6704), suggesting that this nuclide was predominantly formed via the gamma process (photodisintegration) in a nearby core-collapse supernova.[8]
Niobium-92, along with niobium-94, has been detected in refined samples of terrestrial niobium and may originate from bombardment by cosmic ray muons in Earth's crust.[9]
See also
Daughter products other than niobium
References
- ^ a b c d Kondev, 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.
- ^ "Standard Atomic Weights: Niobium". CIAAW. 2017.
- ^ 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.
- ^ 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.
- ^ Sumikama, T.; et al. (2021). "Observation of new neutron-rich isotopes in the vicinity of Zr110". Physical Review C. 103 (1): 014614. Bibcode:2021PhRvC.103a4614S. doi:10.1103/PhysRevC.103.014614. hdl:10261/260248. S2CID 234019083.
{{cite journal}}
: CS1 maint: article number as page number (link) - ^ a b Iizuka, Tsuyoshi; Lai, Yi-Jen; Akram, Waheed; Amelin, Yuri; Schönbächler, Maria (2016). "The initial abundance and distribution of 92Nb in the Solar System". Earth and Planetary Science Letters. 439: 172–181. arXiv:1602.00966. Bibcode:2016E&PSL.439..172I. doi:10.1016/j.epsl.2016.02.005. S2CID 119299654.
- ^ Hibiya, Y; Iizuka, T; Enomoto, H (2019). THE INITIAL ABUNDANCE OF NIOBIUM-92 IN THE OUTER SOLAR SYSTEM (PDF). Lunar and Planetary Science Conference (50th ed.). Retrieved 7 September 2019.
- ^ Hibiya, Y.; Iizuka, T.; Enomoto, H.; Hayakawa, T. (2023). "Evidence for enrichment of niobium-92 in the outer protosolar disk". Astrophysical Journal Letters. 942 (L15): L15. Bibcode:2023ApJ...942L..15H. doi:10.3847/2041-8213/acab5d. S2CID 255414098.
- ^ Clayton, Donald D.; Morgan, John A. (1977). "Muon production of 92,94Nb in the Earth's crust". Nature. 266 (5604): 712–713. doi:10.1038/266712a0. S2CID 4292459.