Physics:Isotopes of magnesium

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Short description: Nuclides with atomic number of 12 but with different mass numbers
Main isotopes of Chemistry:magnesium (12Mg)
Iso­tope Decay
abun­dance half-life (t1/2) mode pro­duct
24Mg 79.0% stable
25Mg 10.0% stable
26Mg 11.0% stable
Standard atomic weight Ar, standard(Mg)
  • [24.304, 24.307][1]
  • Conventional: 24.305
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Magnesium (12Mg) naturally occurs in three stable isotopes: 24Mg, 25Mg, and 26Mg. There are 19 radioisotopes that have been discovered, ranging from 18Mg to 40Mg (with the exception of 39Mg). The longest-lived radioisotope is 28Mg 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 18Mg 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.[2][3]

The abundances of the naturally occurring isotopes of magnesium.

List of isotopes

Nuclide
Z N Isotopic mass (u)
[n 1]
Half-life
[n 2]
Decay
mode

[n 3]
Daughter
isotope

[n 4]
Spin and
parity
[n 5][n 2]
Physics:Natural abundance (mole fraction)
Normal proportion Range of variation
18Mg[4] 12 6 4.0(3.4) zs 2p 16Ne 0+
19Mg 12 7 19.034180(60) 5(3) ps 2p 17Ne 1/2−#
20Mg 12 8 20.0187631(20) 90.4(5) ms β+ (69.7(1.2)%) 20Na 0+
β+p (30.3(1.2)%) 19Ne
21Mg 12 9 21.0117058(8) 120.0(4) ms β+ (79.8(2.1)%) 21Na 5/2+
β+p (20.1(2.1)%) 20Ne
β+α (0.116(18)%) 17F
β+pα (0.016(3)%) 16O
22Mg 12 10 21.99957060(17) 3.8745(7) s β+ 22Na 0+
23Mg 12 11 22.99412377(3) 11.3039(32) s β+ 23Na 3/2+
24Mg 12 12 23.985041689(14) Stable 0+ [0.78880.7905]
25Mg 12 13 24.98583697(5) Stable 5/2+ [0.099880.10034]
26Mg[n 6] 12 14 25.98259297(3) Stable 0+ [0.10960.1109]
27Mg 12 15 26.98434065(5) 9.435(27) min β 27Al 1/2+
28Mg 12 16 27.98387543(28) 20.915(9) h β 28Al 0+
29Mg 12 17 28.9886072(4) 1.30(12) s β 29Al 3/2+
30Mg 12 18 29.9904655(14) 317(4) ms β (> 99.94%) 30Al 0+
βn (< 0.06%) 29Al
31Mg 12 19 30.996648(3) 270(2) ms β (93.8(1.9)%) 31Al 1/2+
βn (6.2(1.9)%) 30Al
32Mg 12 20 31.999110(4) 80.4(4) ms β (94.5(5)%) 32Al 0+
βn (5.5(5)%) 31Al
33Mg 12 21 33.0053279(29) 92.0(1.2) ms β (86(2)%) 33Al 3/2−
βn (14(2)%) 32Al
β2n ?[n 7] 31Al ?
34Mg 12 22 34.008935(7) 44.9(4) ms β (> 78.9(7.0)%) 34Al 0+
βn (21(7)%) 33Al
β2n (< 0.1%) 32Al
35Mg 12 23 35.01679(29) 11.3(6) ms βn (52(46)%) 34Al (3/2−, 5/2−)
β (48(46)%) 35Al
β2n ?[n 7] 33Al ?
36Mg 12 24 36.02188(74) 3.9(1.3) ms β (52(12)%) 36Al 0+
βn (48(12)%) 35Al
β2n ?[n 7] 34Al ?
37Mg 12 25 37.03029(75) 8(4) ms β ?[n 7] 37Al ? (3/2−)
βn ?[n 7] 36Al ?
β2n ?[n 7] 35Al ?
38Mg 12 26 38.03658(54)# 3.1(4 (stat), 2 (sys)) ms[5] βn (81%) 37Al 0+
β (9%) 38Al
β2n (9%) 36Al
40Mg 12 28 40.05319(54)# 1# ms [> 170 ns] β ?[n 7] 40Al ? 0+
βn ?[n 7] 39Al ?
β2n ?[n 7] 38Al ?
  1. ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  2. 2.0 2.1 # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  3. Modes of decay:
    n: Neutron emission
    p: Proton emission
  4. Bold symbol as daughter – Daughter product is stable.
  5. ( ) spin value – Indicates spin with weak assignment arguments.
  6. Used in radiodating events early in the Solar System's history
  7. 7.0 7.1 7.2 7.3 7.4 7.5 7.6 7.7 7.8 Decay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide.

External links

References

  1. Meija, Juris; Coplen, Tyler B.; Berglund, Michael; Brand, Willi A.; De Bièvre, Paul; Gröning, Manfred; Holden, Norman E.; Irrgeher, Johanna et al. (2016). "Atomic weights of the elements 2013 (IUPAC Technical Report)". Pure and Applied Chemistry 88 (3): 265–91. doi:10.1515/pac-2015-0305. 
  2. glennroberts (2019-02-07). "New Measurements of Exotic Magnesium Suggest Surprising Shape-Shift" (in en-US). https://newscenter.lbl.gov/2019/02/07/new-measurements-exotic-magnesium-suggest-surprising-shape-shift/. 
  3. "NP A Change in Structure for a S... | U.S. DOE Office of Science(SC)" (in en-US). 2019-08-01. https://science.osti.gov/np/Highlights/2019/NP-2019-08-a. 
  4. Jin, Y. (2021). "First observation of the four-proton unbound nucleus 18Mg". Physical Review Letters 127 (262502): 262502. doi:10.1103/PhysRevLett.127.262502. PMID 35029460. 
  5. Crawford, H. L.Expression error: Unrecognized word "et". (2022). "Crossing N = 28 toward the neutron drip line: first measurement of half-lives at FRIB". Physical Review Letters 129 (212501): 212501. doi:10.1103/PhysRevLett.129.212501. PMID 36461950. Bibcode2022PhRvL.129u2501C.