Isotopes of aluminium
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cosmic-ray protons. Aluminium isotopes have found practical application in dating marine sediments, manganese nodules, glacial ice, quartz in rock exposures, and meteorites. The ratio of 26Al to 10Be has been used to study the role of sediment transport, deposition, and storage, as well as burial times, and erosion, on 105 to 106 year time scales.[citation needed
] 26Al has also played a significant role in the study of meteorites.
List of isotopes
Nuclide[5] [n 1] |
Z | N | Isotopic mass (Da)[6] [n 2][n 3] |
Half-life |
Daughter isotope [n 5] |
Isotopic abundance | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy[n 7] | |||||||||||||||||||
22Al | 13 | 9 | 22.01954(43)# | 91.1(5) ms | β+, p (55%) | 21Na | (4)+ | ||||||||||||
β+ (43.862%) | 22Mg | ||||||||||||||||||
β+, 2p (1.1%) | 20Ne | ||||||||||||||||||
β+, α (0.038%) | 18Ne | ||||||||||||||||||
23Al | 13 | 10 | 23.0072444(4) | 470(30) ms | β+ (99.54%) | 23Mg | 5/2+ | ||||||||||||
β+, p (0.46%) | 22Na | ||||||||||||||||||
24Al | 13 | 11 | 23.99994754(25) | 2.053(4) s | β+ (99.9634%) | 24Mg | 4+ | ||||||||||||
β+, α (.035%) | 20Ne | ||||||||||||||||||
β+, p (.0016%) | 23Na | ||||||||||||||||||
24mAl | 425.8(1) keV | 130(3) ms | IT (82.5%)
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24Al | 1+ | ||||||||||||||
β+ (17.5%) | 24Mg | ||||||||||||||||||
β+, α (.028%) | 20Ne | ||||||||||||||||||
25Al | 13 | 12 | 24.99042831(7) | 7.183(12) s | β+ | 25Mg | 5/2+ | ||||||||||||
26Al[n 8] | 13 | 13 | 25.98689186(7) | 7.17(24)×105 y | β+ (85%) | 26Mg | 5+ | Trace[n 9] | |||||||||||
ε (15%)[7] | |||||||||||||||||||
26mAl | 228.306(13) keV | 6.3460(8) s | β+ | 26Mg | 0+ | ||||||||||||||
27Al | 13 | 14 | 26.98153841(5) | Stable | 5/2+ | 1.0000 | |||||||||||||
28Al | 13 | 15 | 27.98191009(8) | 2.245(5) min | β− | 28Si | 3+ | ||||||||||||
29Al | 13 | 16 | 28.9804532(4) | 6.56(6) min | β− | 29Si | 5/2+ | ||||||||||||
30Al | 13 | 17 | 29.982968(3) | 3.62(6) s | β− | 30Si | 3+ | ||||||||||||
31Al | 13 | 18 | 30.9839498(24) | 644(25) ms | β− (98.4%) | 31Si | 5/2(+) | ||||||||||||
β−, n (1.6%) | 30Si | ||||||||||||||||||
32Al | 13 | 19 | 31.988084(8) | 33.0(2) ms | β− (99.3%) | 32Si | 1+ | ||||||||||||
β−, n (.7%) | 31Si | ||||||||||||||||||
32mAl | 955.7(4) keV | 200(20) ns | IT | 32Al | (4+) | ||||||||||||||
33Al | 13 | 20 | 32.990878(8) | 41.7(2) ms | β− (91.5%) | 33Si | 5/2+ | ||||||||||||
β−, n (8.5%) | 32Si | ||||||||||||||||||
34Al | 13 | 21 | 33.996779(3) | 56.3(5) ms | β− (74%) | 34Si | (4−) | ||||||||||||
β−, n (26%) | 33Si | ||||||||||||||||||
34mAl | 550(100)# keV | 26(1) ms | β− (70%) | 34Si | (1+) | ||||||||||||||
β−, n (30%) | 33Si | ||||||||||||||||||
35Al | 13 | 22 | 34.999760(8) | 37.2(8) ms | β− (62%) | 35Si | 5/2+# | ||||||||||||
β−, n (38%) | 34Si | ||||||||||||||||||
36Al | 13 | 23 | 36.00639(16) | 90(40) ms | β− (70%) | 36Si | |||||||||||||
β−, n (30%) | 35Si | ||||||||||||||||||
37Al | 13 | 24 | 37.01053(19) | 11.5(4) ms | β− (71%) | 37Si | 5/2+# | ||||||||||||
β−, n (29%) | 36Si | ||||||||||||||||||
38Al | 13 | 25 | 38.0174(4) | 9.0(7) ms | β− | 38Si | |||||||||||||
39Al | 13 | 26 | 39.02217(43)# | 7.6(16) ms | β−, n (90%) | 38Si | 5/2+# | ||||||||||||
β− (10%) | 39Si | ||||||||||||||||||
40Al | 13 | 27 | 40.02962(43)# | 5.7(3 ( sys)) ms[8]
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β−, n (64%) | 39Si | |||||||||||||
β−, 2n (20%) | 38Si | ||||||||||||||||||
β− (16%) | 40Si | ||||||||||||||||||
41Al | 13 | 28 | 41.03588(54)# | 3.5(8 (stat), 4 (sys)) ms[8] | β−, n (86%) | 40Si | 5/2+# | ||||||||||||
β−, 2n (11%) | 39Si | ||||||||||||||||||
β− (3%) | 41Si | ||||||||||||||||||
42Al | 13 | 29 | 42.04305(64)# | 1# ms [>170 ns] | β− | 42Si | |||||||||||||
43Al | 13 | 30 | 43.05048(86)# | 1# ms [>170 ns] | β− | 43Si | |||||||||||||
This table header & footer: |
- ^ mAl – 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).
- ^
Modes of decay:
IT: Isomeric transition - ^ Bold symbol as daughter – Daughter product is stable.
- ^ ( ) spin value – Indicates spin with weak assignment arguments.
- ^ a b # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
- radiodating events early in the Solar System's history and meteorites
- ^ cosmogenic
Aluminium-26
asteroids after their formation 4.55 billion years ago.[10]
References
- .
- .
- ^ "Standard Atomic Weights: Aluminium". CIAAW. 2017.
- ISSN 1365-3075.
- .
- .
- ^ a b "Physics 6805 Topics in Nuclear Physics". Ohio State University. Retrieved 12 June 2019.
- ^ S2CID 253600995.
- . Retrieved 12 June 2019.
- ^
R. T. Dodd (1986). Thunderstones and Shooting Stars. Harvard University Press. pp. 89–90. ISBN 978-0-674-89137-1.