Isotopes of argon
Argon (Ar) has 24 known isotopes, from 30Ar to 53Ar and 1 isomer (32mAr), three of which are stable, 36Ar, 38Ar, and 40Ar. On Earth, 40Ar makes up 99.6% of natural argon. The longest-lived radioactive isotopes are 39Ar with a half-life of 269 years, 42Ar with a half-life of 32.9 years, and 37Ar with a half-life of 35.04 days. All other isotopes have half-lives less than 2 hours, and most less than a minute. The least stable is 30Ar with a half-life shorter than 20 nanoseconds.
Naturally occurring 40K with a half-life of 1.248×109 (3) years, decays to stable 40Ar (10.72%) by electron capture and by positron emission, and also transforms to stable 40Ca (89.28%) via beta decay. These properties and ratios are used to determine the age of rocks through potassium-argon dating.[1]
Despite trapping of 40Ar in many rocks, it can be released by melting, grinding, and diffusion. Almost all of the argon in the Earth's atmosphere is the product of potassium-40 decay, since 99.6% of Earth atmospheric argon is 40Ar, whereas in the Sun and presumably in primordial star-forming clouds, argon consists of < 15% 38Ar and mostly (85%) 36Ar. Similarly, the ratio of the three isotopes 36Ar: 38Ar: 40Ar in the atmospheres of the outer planets is measured to be 8400: 1600: 1[2]
In the Earth's atmosphere, radioactive 39Ar (half-life 269 years) is made by cosmic ray activity, primarily from 40Ar. In the subsurface environment, it is also produced through neutron capture by 39K or alpha emission by calcium. The content of 39Ar in natural argon is measured to be of (8.0±0.6)×10−16 g/g, or (1.01±0.08) Bq/kg of 36, 38, 40Ar.[3] The content of 42Ar (half-life 33 years) in the Earth's atmosphere is lower than 6×10−21 parts per part of 36, 38, 40Ar.[4] In December 2013, 36Argon, in the form of argon hydride, was found in cosmic dust associated with the Crab nebula supernova.[5][6] This was the first time a noble molecule was detected in outer space.[5][6]
Radioactive 37Ar is a synthetic radionuclide that is created from the neutron spallation of 40Ca as a result of subsurface nuclear explosions. It has a half-life of 35 days.[1]
Standard argon atomic mass: 39.948(1) u.
Table
nuclide symbol |
Z(p) | N(n) | isotopic mass (u) |
half-life | decay mode(s)[7] |
daughter isotope(s)[n 1] |
nuclear spin |
representative isotopic composition (mole fraction)[n 2] |
range of natural variation (mole fraction) |
---|---|---|---|---|---|---|---|---|---|
excitation energy | |||||||||
30Ar | 18 | 12 | 30.02156(32)# | <20 ns | p | 29Cl | 0+ | ||
31Ar | 18 | 13 | 31.01212(22)# | 14.4(6) ms | β+, p (55.0%) | 30S | 5/2(+#) | ||
β+ (40.4%) | 31Cl | ||||||||
β+, 2p (2.48%) | 29P | ||||||||
β+, 3p (2.1%) | 28Si | ||||||||
32Ar | 18 | 14 | 31.9976380(19) | 98(2) ms | β+ (56.99%) | 32Cl | 0+ | ||
β+, p (43.01%) | 31S | ||||||||
32mAr | 5600(100)# keV | unknown | 5-# | ||||||
33Ar | 18 | 15 | 32.9899257(5) | 173.0(20) ms | β+ (61.35%) | 33Cl | 1/2+ | ||
β+, p (38.65%) | 32S | ||||||||
34Ar | 18 | 16 | 33.9802712(4) | 844.5(34) ms | β+ | 34Cl | 0+ | ||
35Ar | 18 | 17 | 34.9752576(8) | 1.775(4) s | β+ | 35Cl | 3/2+ | ||
36Ar | 18 | 18 | 35.967545106(29) | Observationally Stable[n 3] | 0+ | 0.003336(4) | |||
37Ar | 18 | 19 | 36.96677632(22) | 35.04(4) d | ε | 37Cl | 3/2+ | ||
38Ar | 18 | 20 | 37.9627324(4) | Stable | 0+ | 6.29(1)×10−4 | |||
39Ar[n 4] | 18 | 21 | 38.964313(5) | 269(3) a | β− | 39K | 7/2- | Trace[n 5] | |
40Ar[n 6] | 18 | 22 | 39.9623831225(29) | Stable | 0+ | 0.996035(4)[n 7] | |||
41Ar | 18 | 23 | 40.9645006(4) | 109.61(4) min | β− | 41K | 7/2- | ||
42Ar | 18 | 24 | 41.963046(6) | 32.9(11) a | β− | 42K | 0+ | Trace | |
43Ar | 18 | 25 | 42.965636(6) | 5.37(6) min | β− | 43K | (5/2-) | ||
44Ar | 18 | 26 | 43.9649240(17) | 11.87(5) min | β− | 44K | 0+ | ||
45Ar | 18 | 27 | 44.9680400(6) | 21.48(15) s | β− | 45K | (1/2,3/2,5/2)- | ||
46Ar | 18 | 28 | 45.96809(4) | 8.4(6) s | β− | 46K | 0+ | ||
47Ar | 18 | 29 | 46.97219(11) | 1.23(3) s | β− (99%) | 47K | 3/2-# | ||
β−, n (1%) | 46K | ||||||||
48Ar | 18 | 30 | 47.97454(32)# | 0.48(40) s | β− | 48K | 0+ | ||
49Ar | 18 | 31 | 48.98052(54)# | 170(50) ms | β− | 49K | 3/2-# | ||
50Ar | 18 | 32 | 49.98443(75)# | 85(30) ms | β− | 50K | 0+ | ||
51Ar | 18 | 33 | 50.99163(75)# | 60# ms [>200 ns] | β− | 51K | 3/2-# | ||
52Ar | 18 | 34 | 51.99678(97)# | 10# ms | β− | 52K | 0+ | ||
53Ar | 18 | 35 | 53.00494(107)# | 3# ms | β− | 53K | (5/2-)# | ||
β−, n | 52K |
- ↑ Bold for stable isotopes
- ↑ Isotopic composition refers to that in air. 36Ar is actually far more abundant than 40Ar, universally. 40Ar is most abundant in air because most of it is radiogenic. Such 40Ar atoms are a decay product from 40K via electron capture, whereas 40K goes under mostly β− decay to 40Ca. 40Ar escapes the 40K-containing rocks into the atmosphere, thus making the argon in the air mostly 40Ar, not 36Ar.
- ↑ Believed to undergo double electron capture to 36S (lightest theoretically unstable nuclide for which no evidence of radioactivity has been observed)
- ↑ Used in argon-argon dating
- ↑ Cosmogenic nuclide
- ↑ Used in argon-argon dating and potassium-argon dating
- ↑ Generated from 40K in rocks. These ratios are terrestrial. Cosmic abundance is far less than 36Ar.
Notes
- Nuclide masses are given by IUPAP Commission on Symbols, Units, Nomenclature, Atomic Masses and Fundamental Constants (SUNAMCO).
- Isotope abundances are given by IUPAC Commission on Isotopic Abundances and Atomic Weights.
See also
References
- ↑ 1.0 1.1 "40Ar/39Ar dating and errors". Archived from the original on 2007-05-09. Retrieved 2007-03-07.
- ↑ Cameron, A. G. W., "Elemental and Isotopic Abundances of the Volatile Elements in the Outer Planets" (Article published in the Space Science Reviews special issue on 'Outer Solar System Exploration - An Overview', ed. by J. E. Long and D. G. Rea.) Journal: Space Science Reviews, Volume 14, Issue 3-4, pp. 392-400 (1973).
- ↑ P. Benetti et al. (2007). "Measurement of the specific activity of 39Ar in natural argon". Nuclear Instruments and Methods A 574: 83. arXiv:astro-ph/0603131. Bibcode:2007NIMPA.574...83B. doi:10.1016/j.nima.2007.01.106.
- ↑ V. D. Ashitkov et al. (1998). "New experimental limit on the 42Ar content in the Earth's atmosphere". Nuclear Instruments and Methods A 416: 179. doi:10.1016/S0168-9002(98)00740-2.
- ↑ 5.0 5.1 Quenqua, Douglas (13 December 2013). "Noble Molecules Found in Space". New York Times. Retrieved 13 December 2013.
- ↑ 6.0 6.1 Barlow, M. J. et al. (2013). "Detection of a Noble Gas Molecular Ion, 36ArH+, in the Crab Nebula". Science 342 (6164): 1343–1345. doi:10.1126/science.124358213.
- ↑ http://www.nucleonica.net/unc.aspx
- Isotope masses from:
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A 729: 3–128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.
- Isotopic compositions and standard atomic masses from:
- J. R. de Laeter, J. K. Böhlke, P. De Bièvre, H. Hidaka, H. S. Peiser, K. J. R. Rosman and P. D. P. Taylor (2003). "Atomic weights of the elements. Review 2000 (IUPAC Technical Report)". Pure and Applied Chemistry 75 (6): 683–800. doi:10.1351/pac200375060683.
- M. E. Wieser (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". Pure and Applied Chemistry 78 (11): 2051–2066. doi:10.1351/pac200678112051. Lay summary.
- Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A 729: 3–128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.
- National Nuclear Data Center. "NuDat 2.1 database". Brookhaven National Laboratory. Retrieved September 2005.
- N. E. Holden (2004). "Table of the Isotopes". In D. R. Lide. CRC Handbook of Chemistry and Physics (85th ed.). CRC Press. Section 11. ISBN 978-0-8493-0485-9.
External links
Isotopes of chlorine | Isotopes of argon | Isotopes of potassium |
Table of nuclides |
Isotopes of the chemical elements | |||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1 H |
2 He | ||||||||||||||||
3 Li |
4 Be |
5 B |
6 C |
7 N |
8 O |
9 F |
10 Ne | ||||||||||
11 Na |
12 Mg |
13 Al |
14 Si |
15 P |
16 S |
17 Cl |
18 Ar | ||||||||||
19 K |
20 Ca |
21 Sc |
22 Ti |
23 V |
24 Cr |
25 Mn |
26 Fe |
27 Co |
28 Ni |
29 Cu |
30 Zn |
31 Ga |
32 Ge |
33 As |
34 Se |
35 Br |
36 Kr |
37 Rb |
38 Sr |
39 Y |
40 Zr |
41 Nb |
42 Mo |
43 Tc |
44 Ru |
45 Rh |
46 Pd |
47 Ag |
48 Cd |
49 In |
50 Sn |
51 Sb |
52 Te |
53 I |
54 Xe |
55 Cs |
56 Ba |
72 Hf |
73 Ta |
74 W |
75 Re |
76 Os |
77 Ir |
78 Pt |
79 Au |
80 Hg |
81 Tl |
82 Pb |
83 Bi |
84 Po |
85 At |
86 Rn | |
87 Fr |
88 Ra |
104 Rf |
105 Db |
106 Sg |
107 Bh |
108 Hs |
109 Mt |
110 Ds |
111 Rg |
112 Cn |
113 Uut |
114 Fl |
115 Uup |
116 Lv |
117 Uus |
118 Uuo | |
57 La |
58 Ce |
59 Pr |
60 Nd |
61 Pm |
62 Sm |
63 Eu |
64 Gd |
65 Tb |
66 Dy |
67 Ho |
68 Er |
69 Tm |
70 Yb |
71 Lu | |||
89 Ac |
90 Th |
91 Pa |
92 U |
93 Np |
94 Pu |
95 Am |
96 Cm |
97 Bk |
98 Cf |
99 Es |
100 Fm |
101 Md |
102 No |
103 Lr | |||
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