Isotopes of magnesium
Appearance
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Standard atomic weight Ar°(Mg) | ||||||||||||||||||||||||||
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Magnesium (12Mg) naturally occurs in three stable isotopes: 24
Mg, 25
Mg, and 26
Mg. There are 19 radioisotopes that have been discovered, ranging from 18
Mg to 40
Mg (with the exception of 39
Mg). The longest-lived radioisotope is 28
Mg with a half-life of 20.915(9) h. The lighter isotopes mostly decay to isotopes of sodium while the heavier isotopes decay to isotopes of aluminium. The shortest-lived is proton-unbound 18
Mg with a half-life of 4.0(3.4) zeptoseconds.
A precise measurement of the neutron-rich 40Mg in 2019 showed the unexpected difference in its nuclear structure, compared to the lighter neighboring isotopes.[4][5]
List of isotopes
[edit]
Nuclide |
Z | N | Isotopic mass (Da)[6] [n 1] |
Half-life[1] [n 2] |
Decay mode[1] [n 3] |
Daughter isotope [n 4] |
Spin and parity[1] [n 5][n 2] |
Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Normal proportion[1] | Range of variation | ||||||||||||||||||
18 Mg[7] |
12 | 6 | 4.0(3.4) zs | 2p | 16 Ne |
0 | |||||||||||||
19 Mg |
12 | 7 | 19.034180(60) | 5(3) ps | 2p | 17 Ne |
1/2−# | ||||||||||||
20 Mg |
12 | 8 | 20.0187631(20) | 90.4(5) ms | β (69.7(1.2)%) | 20 Na |
0 | ||||||||||||
β p (30.3(1.2)%) | 19 Ne | ||||||||||||||||||
21 Mg |
12 | 9 | 21.0117058(8) | 120.0(4) ms | β (79.8(2.1)%) | 21 Na |
5/2 | ||||||||||||
β p (20.1(2.1)%) | 20 Ne | ||||||||||||||||||
β α (0.116(18)%) | 17 F | ||||||||||||||||||
β pα (0.016(3)%) | 16 O | ||||||||||||||||||
22 Mg |
12 | 10 | 21.99957060(17) | 3.8745(7) s | β | 22 Na |
0 | ||||||||||||
23 Mg |
12 | 11 | 22.99412377(3) | 11.3039(32) s | β | 23 Na |
3/2 | ||||||||||||
24 Mg |
12 | 12 | 23.985041689(14) | Stable | 0 | [0.7888, 0.7905] | |||||||||||||
25 Mg |
12 | 13 | 24.98583697(5) | Stable | 5/2 | [0.09988, 0.10034] | |||||||||||||
26 Mg[n 6] |
12 | 14 | 25.98259297(3) | Stable | 0 | [0.1096, 0.1109] | |||||||||||||
27 Mg |
12 | 15 | 26.98434065(5) | 9.435(27) min | β− | 27 Al |
1/2 | ||||||||||||
28 Mg |
12 | 16 | 27.98387543(28) | 20.915(9) h | β− | 28 Al |
0 | ||||||||||||
29 Mg |
12 | 17 | 28.9886072(4) | 1.30(12) s | β− | 29 Al |
3/2 | ||||||||||||
30 Mg |
12 | 18 | 29.9904655(14) | 317(4) ms | β− (> 99.94%) | 30 Al |
0 | ||||||||||||
β−n (< 0.06%) | 29 Al | ||||||||||||||||||
31 Mg |
12 | 19 | 30.996648(3) | 270(2) ms | β− (93.8(1.9)%) | 31 Al |
1/2 | ||||||||||||
β−n (6.2(1.9)%) | 30 Al | ||||||||||||||||||
32 Mg |
12 | 20 | 31.999110(4) | 80.4(4) ms | β− (94.5(5)%) | 32 Al |
0 | ||||||||||||
β−n (5.5(5)%) | 31 Al | ||||||||||||||||||
33 Mg |
12 | 21 | 33.0053279(29) | 92.0(1.2) ms | β− (86(2)%) | 33 Al |
3/2− | ||||||||||||
β−n (14(2)%) | 32 Al | ||||||||||||||||||
β−2n ?[n 7] | 31 Al ? | ||||||||||||||||||
34 Mg |
12 | 22 | 34.008935(7) | 44.9(4) ms | β− (> 78.9(7.0)%) | 34 Al |
0 | ||||||||||||
β−n (21(7)%) | 33 Al | ||||||||||||||||||
β−2n (< 0.1%) | 32 Al | ||||||||||||||||||
35 Mg |
12 | 23 | 35.01679(29) | 11.3(6) ms | β−n (52(46)%) | 34 Al |
(3/2−, 5/2−) | ||||||||||||
β− (48(46)%) | 35 Al | ||||||||||||||||||
β−2n ?[n 7] | 33 Al ? | ||||||||||||||||||
36 Mg |
12 | 24 | 36.02188(74) | 3.9(1.3) ms | β− (52(12)%) | 36 Al |
0 | ||||||||||||
β−n (48(12)%) | 35 Al | ||||||||||||||||||
β−2n ?[n 7] | 34 Al ? | ||||||||||||||||||
37 Mg |
12 | 25 | 37.03029(75) | 8(4) ms | β− ?[n 7] | 37 Al ? |
(3/2−) | ||||||||||||
β−n ?[n 7] | 36 Al ? | ||||||||||||||||||
β−2n ?[n 7] | 35 Al ? | ||||||||||||||||||
38 Mg |
12 | 26 | 38.03658(54)# | 3.1(4 (stat), 2 (sys)) ms[8] | β−n (81%) | 37 Al |
0 | ||||||||||||
β− (9%) | 38 Al | ||||||||||||||||||
β−2n (9%) | 36 Al | ||||||||||||||||||
40 Mg |
12 | 28 | 40.05319(54)# | 1# ms [> 170 ns] | β− ?[n 7] | 40 Al ? |
0 | ||||||||||||
β−n ?[n 7] | 39 Al ? | ||||||||||||||||||
β−2n ?[n 7] | 38 Al ? | ||||||||||||||||||
This table header & footer: |
- ^ ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
- ^ a b # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
- ^
Modes of decay:
n: Neutron emission p: Proton emission - ^ Bold symbol as daughter – Daughter product is stable.
- ^ ( ) spin value – Indicates spin with weak assignment arguments.
- ^ Used in radiodating events early in the Solar System's history
- ^ a b c d e f g h i Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide.
External links
[edit]References
[edit]- ^ a b c d e 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: Magnesium". CIAAW. 2011.
- ^ 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.
- ^ glennroberts (2019-02-07). "New Measurements of Exotic Magnesium Suggest Surprising Shape-Shift". Berkeley Lab News Center. Retrieved 2023-09-10.
- ^ "NP A Change in Structure for a S... | U.S. DOE Office of Science(SC)". science.osti.gov. 2019-08-01. Retrieved 2023-09-10.
- ^ 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.
- ^ Jin, Y.; et al. (2021). "First observation of the four-proton unbound nucleus 18Mg". Physical Review Letters. 127 (262502): 262502. doi:10.1103/PhysRevLett.127.262502. OSTI 1837749. PMID 35029460. S2CID 245434485.
- ^ Crawford, H. L.; Tripathi, V.; Allmond, J. M.; et al. (2022). "Crossing N = 28 toward the neutron drip line: first measurement of half-lives at FRIB". Physical Review Letters. 129 (212501): 212501. Bibcode:2022PhRvL.129u2501C. doi:10.1103/PhysRevLett.129.212501. PMID 36461950. S2CID 253600995.