There are 20 isotopes of sodium (11Na), ranging from 17Na to 39Na (except for the still-unknown 36Na and 38Na), and five isomers (two for 22Na, and one each for 24Na, 26Na, and 32Na). 23Na is the only stable (and the only primordial) isotope. It is considered a monoisotopic element and it has a standard atomic weight of 22.98976928(2). Sodium has two radioactive cosmogenic isotopes (22Na, with a half-life of 2.6019(6) years; and 24Na, with a half-life of 14.9560(15) h). With the exception of those two isotopes, all other isotopes have half-lives under a minute, most under a second. The shortest-lived is the unbound 18Na, with a half-life of 1.3(4)×10−21 seconds (although the half-life of the similarly unbound 17Na is not measured).
Acute neutron radiation exposure (e.g., from a nuclear criticality accident) converts some of the stable 23Na (in the form of Na+ ion) in human blood plasma to 24Na. By measuring the concentration of this isotope, the neutron radiation dosage to the victim can be computed.
22Na is a positron-emitting isotope with a remarkably long half-life. It is used to create test-objects and point-sources for positron emission tomography.
List of isotopes
Nuclide3 | Z | N | Isotopic mass (Da)456 | Half-life78 | Decaymode910 | Daughterisotope11 | Spin andparity121314 | Isotopicabundance | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy | |||||||||||||||||||
17Na | 11 | 6 | 17.037270(60) | p | 16Ne | (1/2+) | |||||||||||||
18Na | 11 | 7 | 18.02688(10) | 1.3(4) zs | p ?15 | 17Ne | 1−# | ||||||||||||
19Na | 11 | 8 | 19.013880(11) | > 1 as | p | 18Ne | (5/2+) | ||||||||||||
20Na | 11 | 9 | 20.0073543(12) | 447.9(2.3) ms | β+ (75.0(4)%) | 20Ne | 2+ | ||||||||||||
β+α (25.0(4)%) | 16O | ||||||||||||||||||
21Na | 11 | 10 | 20.99765446(5) | 22.4550(54) s | β+ | 21Ne | 3/2+ | ||||||||||||
22Na | 11 | 11 | 21.99443742(18) | 2.6019(6) y16 | β+ (90.57(8)%) | 22Ne | 3+ | Trace17 | |||||||||||
ε (9.43(6)%) | 22Ne | ||||||||||||||||||
22m1Na | 583.05(10) keV | 243(2) ns | IT | 22Na | 1+ | ||||||||||||||
22m2Na | 657.00(14) keV | 19.6(7) ps | IT | 22Na | 0+ | ||||||||||||||
23Na | 11 | 12 | 22.9897692820(19) | Stable | 3/2+ | 1 | |||||||||||||
24Na | 11 | 13 | 23.990963012(18) | 14.9560(15) h | β− | 24Mg | 4+ | Trace18 | |||||||||||
24mNa | 472.2074(8) keV | 20.18(10) ms | IT (99.95%) | 24Na | 1+ | ||||||||||||||
β− (0.05%) | 24Mg | ||||||||||||||||||
25Na | 11 | 14 | 24.9899540(13) | 59.1(6) s | β− | 25Mg | 5/2+ | ||||||||||||
26Na | 11 | 15 | 25.992635(4) | 1.07128(25) s | β− | 26Mg | 3+ | ||||||||||||
26mNa | 82.4(4) keV | 4.35(16) μs | IT | 26Na | 1+ | ||||||||||||||
27Na | 11 | 16 | 26.994076(4) | 301(6) ms | β− (99.902(24)%) | 27Mg | 5/2+ | ||||||||||||
β−n (0.098(24)%) | 26Mg | ||||||||||||||||||
28Na | 11 | 17 | 27.998939(11) | 33.1(1.3) ms | β− (99.42(12)%) | 28Mg | 1+ | ||||||||||||
β−n (0.58(12)%) | 27Mg | ||||||||||||||||||
29Na | 11 | 18 | 29.002877(8) | 43.2(4) ms | β− (78%) | 29Mg | 3/2+ | ||||||||||||
β−n (22(3)%) | 28Mg | ||||||||||||||||||
β−2n ?19 | 27Mg ? | ||||||||||||||||||
30Na | 11 | 19 | 30.009098(5) | 45.9(7) ms | β− (70.2(2.2)%) | 30Mg | 2+ | ||||||||||||
β−n (28.6(2.2)%) | 29Mg | ||||||||||||||||||
β−2n (1.24(19)%) | 28Mg | ||||||||||||||||||
β−α (5.5(2)%×10−5) | 26Ne | ||||||||||||||||||
31Na | 11 | 20 | 31.013147(15) | 16.8(3) ms | β− (> 63.2(3.5)%) | 31Mg | 3/2+ | ||||||||||||
β−n (36.0(3.5)%) | 30Mg | ||||||||||||||||||
β−2n (0.73(9)%) | 29Mg | ||||||||||||||||||
β−3n (< 0.05%) | 28Mg | ||||||||||||||||||
32Na | 11 | 21 | 32.020010(40) | 12.9(3) ms | β− (66.4(6.2)%) | 32Mg | (3−) | ||||||||||||
β−n (26(6)%) | 31Mg | ||||||||||||||||||
β−2n (7.6(1.5)%) | 30Mg | ||||||||||||||||||
32mNa20 | 625 keV | 24(2) μs | IT | 32Na | (0+,6−) | ||||||||||||||
33Na | 11 | 22 | 33.02553(48) | 8.2(4) ms | β−n (47(6)%) | 32Mg | (3/2+) | ||||||||||||
β− (40.0(6.7)%) | 33Mg | ||||||||||||||||||
β−2n (13(3)%) | 31Mg | ||||||||||||||||||
34Na | 11 | 23 | 34.03401(64) | 5.5(1.0) ms | β−2n (~50%) | 32Mg | 1+ | ||||||||||||
β− (~35%) | 34Mg | ||||||||||||||||||
β−n (~15%) | 33Mg | ||||||||||||||||||
35Na | 11 | 24 | 35.04061(72)# | 1.5(5) ms | β− | 35Mg | 3/2+# | ||||||||||||
β−n ?21 | 34Mg ? | ||||||||||||||||||
β−2n ?22 | 33Mg ? | ||||||||||||||||||
37Na | 11 | 26 | 37.05704(74)# | 1# ms [> 1.5 μs] | β− ?23 | 37Mg ? | 3/2+# | ||||||||||||
β−n ?24 | 36Mg ? | ||||||||||||||||||
β−2n ?25 | 35Mg ? | ||||||||||||||||||
39Na26 | 11 | 28 | 39.07512(80)# | 1# ms [> 400 ns] | β− ?27 | 39Mg ? | 3/2+# | ||||||||||||
β−n ?28 | 38Mg ? | ||||||||||||||||||
β−2n ?29 | 37Mg ? | ||||||||||||||||||
This table header & footer:
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Sodium-22
Sodium-22 is a radioactive isotope of sodium, undergoing positron emission to 22Ne with a half-life of 2.6019(6) years. 22Na is being investigated as an efficient generator of "cold positrons" (antimatter) to produce muons for catalyzing fusion of deuterium. It is also commonly used as a positron source in positron annihilation spectroscopy.30
Sodium-23
Sodium-23 is an isotope of sodium with an atomic mass of 22.98976928. It is the only stable isotope of sodium and also the only primordial isotope. Because of its abundance, sodium-23 is used in nuclear magnetic resonance in various research fields, including materials science and battery research.31 Sodium-23 relaxation has applications in studying cation-biomolecule interactions, intracellular and extracellular sodium, ion transport in batteries, and quantum information processing.32
Sodium-24
Sodium-24 is radioactive and can be created from common sodium-23 by neutron activation. With a half-life of 14.9560(15) h, 24Na decays to 24Mg by emission of an electron and two gamma rays.3334
Exposure of the human body to intense neutron radiation creates 24Na in the blood plasma. Measurements of its quantity can be done to determine the absorbed radiation dose of a patient.35 This can be used to determine the type of medical treatment required.
When sodium is used as coolant in fast breeder reactors, 24Na is created, which makes the coolant radioactive. When the 24Na decays, it causes a buildup of magnesium in the coolant. Since the half-life is short, the 24Na portion of the coolant ceases to be radioactive within a few days after removal from the reactor. Leakage of the hot sodium from the primary loop may cause radioactive fires,36 as it can ignite in contact with air (and explodes in contact with water). For this reason the primary cooling loop is within a containment vessel.
Sodium has been proposed as a casing for a salted bomb, as it would convert to 24Na and produce intense gamma-ray emissions for a few days.3738
Notes
External links
References
Ahn, D.S.; et al. (2022-11-14). "Discovery of 39Na". Physical Review Letters. 129 (21) 212502: 212502. Bibcode:2022PhRvL.129u2502A. doi:10.1103/PhysRevLett.129.212502. PMID 36461972. S2CID 253591660. https://doi.org/10.1103%2FPhysRevLett.129.212502 ↩
Note that NUBASE2020 uses the tropical year to convert between years and other units of time, not the Gregorian year. The relationship between years and other time units in NUBASE2020 is as follows: 1 y = 365.2422 d = 31 556 926 s /wiki/Tropical_year ↩
mNa – Excited nuclear isomer. /wiki/Nuclear_isomer ↩
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. /wiki/Doi_(identifier) ↩
( ) – 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). ↩
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. https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf ↩
# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN). ↩
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. https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf ↩
Modes of decay: IT:Isomeric transitionn:Neutron emissionp:Proton emission /wiki/Isomeric_transition ↩
Bold symbol as daughter – Daughter product is stable. ↩
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. https://www-nds.iaea.org/amdc/ame2020/NUBASE2020.pdf ↩
( ) spin value – Indicates spin with weak assignment arguments. ↩
# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN). ↩
Decay mode shown has been observed, but its intensity is not known experimentally. ↩
Note that NUBASE2020 uses the tropical year to convert between years and other units of time, not the Gregorian year. The relationship between years and other time units in NUBASE2020 is as follows: 1 y = 365.2422 d = 31 556 926 s /wiki/Tropical_year ↩
Cosmogenic nuclide /wiki/Cosmogenic_nuclide ↩
Cosmogenic nuclide /wiki/Cosmogenic_nuclide ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Gray, T. J.; Allmond, J. M.; Xu, Z.; King, T. T.; Lubna, R. S.; Crawford, H. L.; Tripathi, V.; Crider, B. P.; Grzywacz, R.; Liddick, S. N.; Macchiavelli, A. O.; Miyagi, T.; Poves, A.; Andalib, A.; Argo, E.; Benetti, C.; Bhattacharya, S.; Campbell, C. M.; Carpenter, M. P.; Chan, J.; Chester, A.; Christie, J.; Clark, B. R.; Cox, I.; Doetsch, A. A.; Dopfer, J.; Duarte, J. G.; Fallon, P.; Frotscher, A.; Gaballah, T.; Harke, J. T.; Heideman, J.; Huegen, H.; Holt, J. D.; Jain, R.; Kitamura, N.; Kolos, K.; Kondev, F. G.; Laminack, A.; Longfellow, B.; Luitel, S.; Madurga, M.; Mahajan, R.; Mogannam, M. J.; Morse, C.; Neupane, S.; Nowicki, A.; Ogunbeku, T. H.; Ong, W.-J.; Porzio, C.; Prokop, C. J.; Rasco, B. C.; Ronning, E. K.; Rubino, E.; Ruland, T. J.; Rykaczewski, K. P.; Schaedig, L.; Seweryniak, D.; Siegl, K.; Singh, M.; Stuchbery, A. E.; Tabor, S. L.; Tang, T. L.; Wheeler, T.; Winger, J. A.; Wood, J. L. (13 June 2023). "Microsecond Isomer at the N = 20 Island of Shape Inversion Observed at FRIB". Physical Review Letters. 130 (24). arXiv:2302.11607. doi:10.1103/PhysRevLett.130.242501. /wiki/ArXiv_(identifier) ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Ahn, D.S.; et al. (2022-11-14). "Discovery of 39Na". Physical Review Letters. 129 (21) 212502: 212502. Bibcode:2022PhRvL.129u2502A. doi:10.1103/PhysRevLett.129.212502. PMID 36461972. S2CID 253591660. https://doi.org/10.1103%2FPhysRevLett.129.212502 ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide. ↩
Saro, Matúš; Kršjak, Vladimír; Petriska, Martin; Slugeň, Vladimír (2019-07-29). "Sodium-22 source contribution determination in positron annihilation measurements using GEANT4". AIP Conference Proceedings. 2131 (1): 020039. Bibcode:2019AIPC.2131b0039S. doi:10.1063/1.5119492. ISSN 0094-243X. S2CID 201349680. https://aip.scitation.org/doi/abs/10.1063/1.5119492 ↩
Gotoh, Kazuma (8 February 2021). "23Na Solid-State NMR Analyses for Na-Ion Batteries and Materials". Batteries & Supercaps. 4 (8): 1267–127. doi:10.1002/batt.202000295. S2CID 233827472. https://chemistry-europe.onlinelibrary.wiley.com/doi/10.1002/batt.202000295 ↩
Song, Yifan; Yin, Yu; Chen, Qinlong; Marchetti, Alessandro; Kong, Xueqian (2023). "23Na relaxometry: An overview of theory and applications". Magnetic Resonance Letters. 3 (2): 150–174. doi:10.1016/j.mrl.2023.04.001. https://doi.org/10.1016%2Fj.mrl.2023.04.001 ↩
"sodium-24". Encyclopædia Britannica. https://www.britannica.com/science/sodium-24 ↩
Ekendahl, Daniela; Rubovič, Peter; Žlebčík, Pavel; Hupka, Ivan; Huml, Ondřej; Bečková, Věra; Malá, Helena (7 November 2019). "Neutron dose assessment using samples of human blood and hair". Radiation Protection Dosimetry. 186 (2–3): 202–205. doi:10.1093/rpd/ncz202. PMID 31702764. /wiki/Doi_(identifier) ↩
Ekendahl, Daniela; Rubovič, Peter; Žlebčík, Pavel; Hupka, Ivan; Huml, Ondřej; Bečková, Věra; Malá, Helena (7 November 2019). "Neutron dose assessment using samples of human blood and hair". Radiation Protection Dosimetry. 186 (2–3): 202–205. doi:10.1093/rpd/ncz202. PMID 31702764. /wiki/Doi_(identifier) ↩
Unusual occurrences during LMFR operation, Proceedings of a Technical Committee meeting held in Vienna, 9–13 November 1998, IAEA. Pages 84, 122. https://www-pub.iaea.org/MTCD/Publications/PDF/te_1180_prn.pdf ↩
"Science: fy for Doomsday". Time. November 24, 1961. Archived from the original on March 14, 2016. http://content.time.com/time/magazine/article/0,9171,828877,00.html ↩
Clark, W. H. (1961). "Chemical and Thermonuclear Explosives". Bulletin of the Atomic Scientists. 17 (9): 356–360. Bibcode:1961BuAtS..17i.356C. doi:10.1080/00963402.1961.11454268. /wiki/Bulletin_of_the_Atomic_Scientists ↩