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% 40Ar and mostly (85%) 36Ar.
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.[2] 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.[3]
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)[4][n 1] |
daughter isotope(s)[n 2] |
nuclear spin |
representative isotopic composition (mole fraction) |
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 | 0+ | 0.003336(4) | |||
37Ar | 18 | 19 | 36.96677632(22) | 35.04(4) d | EC | 37Cl | 3/2+ | ||
38Ar | 18 | 20 | 37.9627324(4) | Stable | 0+ | 6.29(1)×10−4 | |||
39Ar[n 3] | 18 | 21 | 38.964313(5) | 269(3) a | β− | 39K | 7/2- | Trace[n 4] | |
40Ar[n 5] | 18 | 22 | 39.9623831225(29) | Stable | 0+ | 0.996035(4)[n 6] | |||
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 |
- ^ Abbreviations:
EC: Electron capture - ^ Bold for stable isotopes
- ^ Used in argon-argon dating
- ^ Cosmogenic nuclide
- ^ Used in argon-argon dating and potassium-argon dating
- ^ Generated from 40K in rocks. Actually far less abundant than 36Ar.
Notes
- 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.
See also
References
- ^ a b "40Ar/39Ar dating and errors". Archived from the original on 2007-05-09. Retrieved 2007-03-07.
- ^
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.
{{cite journal}}
: Explicit use of et al. in:|author=
(help) - ^
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.
{{cite journal}}
: Explicit use of et al. in:|author=
(help) - ^ 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.
{{cite journal}}
: CS1 maint: multiple names: authors list (link)
- 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.
{{cite journal}}
: CS1 maint: multiple names: authors list (link) - 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.
{{cite journal}}
: Unknown parameter|laysummary=
ignored (help)
- 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.
- 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.
{{cite journal}}
: CS1 maint: multiple names: authors list (link) - National Nuclear Data Center. "NuDat 2.1 database". Brookhaven National Laboratory. Retrieved September 2005.
{{cite web}}
: Check date values in:|accessdate=
(help) - N. E. Holden (2004). "Table of the Isotopes". In D. R. Lide (ed.). CRC Handbook of Chemistry and Physics (85th ed.). CRC Press. Section 11. ISBN 978-0849304859.
{{cite book}}
: Unknown parameter|nopp=
ignored (|no-pp=
suggested) (help)
- 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.