Isotopes of neon
Neon (10Ne) possesses three stable isotopes, 20Ne, 21Ne, and 22Ne. In addition, 17 radioactive isotopes have been discovered ranging from 15Ne to 34Ne, all short-lived. The longest-lived is 24Ne with a half-life of 3.38 minutes. All others are under a minute, most under a second. The least stable is 15Ne with a half-life of 7.7×10−22 s. See isotopes of carbon for notes about the measurement.
| ||||||||||||||||||||||||||||||
Standard atomic weight Ar, standard(Ne) |
| |||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
List of isotopes
Nuclide[2] [n 1] |
Z | N | Isotopic mass (Da)[3] [n 2][n 3] |
Half-life [resonance width] |
Decay mode [n 4] |
Daughter isotope [n 5] |
Spin and parity [n 6] |
Natural abundance (mole fraction) | |
---|---|---|---|---|---|---|---|---|---|
Excitation energy | Normal proportion | Range of variation | |||||||
15Ne[4] | 10 | 5 | 15.04317(7) | 7.7(3)×10−22 s [0.59(23)− 2.522(60) MeV] |
2p | 13O | (3/2−) | ||
16Ne | 10 | 6 | 16.025751(22) | > 5.7×10−21 s [122(37) keV] |
2p | 14O | 0+ | ||
17Ne[n 7] | 10 | 7 | 17.0177140(4) | 109.2(6) ms | β+, p (96.0%) | 16O | 1/2− | ||
β+, α (2.7%) | 13N | ||||||||
β+ (1.3%) | 17F | ||||||||
18Ne | 10 | 8 | 18.0057087(4) | 1.66420(47) s | β+ | 18F | 0+ | ||
19Ne | 10 | 9 | 19.00188090(17) | 17.274(10) s | β+ | 19F | 1/2+ | ||
20Ne | 10 | 10 | 19.9924401762(17) | Stable | 0+ | 0.9048(3) | 0.8847–0.9051 | ||
21Ne | 10 | 11 | 20.99384669(4) | Stable | 3/2+ | 0.0027(1) | 0.0027–0.0171 | ||
22Ne | 10 | 12 | 21.991385110(19) | Stable | 0+ | 0.0925(3) | 0.0920–0.0996 | ||
23Ne | 10 | 13 | 22.99446690(11) | 37.140(28) s | β− | 23Na | 5/2+ | ||
24Ne | 10 | 14 | 23.9936106(6) | 3.38(2) min | β− | 24Na | 0+ | ||
25Ne | 10 | 15 | 24.997810(30) | 602(8) ms | β− | 25Na | 1/2+ | ||
26Ne | 10 | 16 | 26.000516(20) | 197(2) ms | β− (99.87%) | 26Na | 0+ | ||
β−, n (0.13%) | 25Na | ||||||||
27Ne | 10 | 17 | 27.00757(10) | 31.5(13) ms | β− (98.0%) | 27Na | (3/2+) | ||
β−, n (2.0%) | 26Na | ||||||||
28Ne | 10 | 18 | 28.01213(14) | 20(1) ms | β− (84.3%) | 28Na | 0+ | ||
β−, n (12.0%) | 27Na | ||||||||
β−, 2n (3.7%) | 26Na | ||||||||
29Ne | 10 | 19 | 29.01975(16) | 14.7(4) ms | β− (68%) | 29Na | (3/2−) | ||
β−, n (28%) | 28Na | ||||||||
β−, 2n (4%) | 27Na | ||||||||
30Ne | 10 | 20 | 30.02499(27) | 7.22(18) ms | β− | 30Na (78.1%) | 0+ | ||
β−, n (13.0%) | 29Na | ||||||||
β−, 2n (8.9%) | 28Na | ||||||||
31Ne | 10 | 21 | 31.03347(29) | 3.4(8) ms | β− | 31Na | (3/2−) | ||
β−, n | 30Na | ||||||||
32Ne | 10 | 22 | 32.03972(54)# | 3.5(9) ms | β− | 32Na | 0+ | ||
β−, n | 31Na | ||||||||
34Ne | 10 | 24 | 34.05673(55)# | 1# ms [>1.5 µs] | β− | 34Na | 0+ |
- mNe – 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:
n: Neutron emission p: Proton emission - Bold symbol as daughter – Daughter product is stable.
- ( ) spin value – Indicates spin with weak assignment arguments.
- Has 2 halo protons.
- The isotopic composition refers to that in air.
gollark: Also database normalization is confusing.
gollark: Oh dear. Initiate contingency Ctrl+W?
gollark: yeh
gollark: I mean, my phone is vaguely waterproofed and could be used probably okay as long as all the ports are closed.
gollark: Of course, osmarks interweb notes™ lack such problems, and do not need to use fixed-size ordered pages, which are a mere implementation detail of real-world systems.
References
- Meija, Juris; 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.
- Half-life, decay mode, nuclear spin, and isotopic composition is sourced in:
Audi, G.; Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S. (2017). "The NUBASE2016 evaluation of nuclear properties" (PDF). Chinese Physics C. 41 (3): 030001. Bibcode:2017ChPhC..41c0001A. doi:10.1088/1674-1137/41/3/030001. - Wang, M.; Audi, G.; Kondev, F. G.; Huang, W. J.; Naimi, S.; Xu, X. (2017). "The AME2016 atomic mass evaluation (II). Tables, graphs, and references" (PDF). Chinese Physics C. 41 (3): 030003-1–030003-442. doi:10.1088/1674-1137/41/3/030003.
- Wamers, F.; Marganiec, J.; Aksouh, F.; Aksyutina, Yu.; Álvarez-Pol, H.; Aumann, T.; Beceiro-Novo, S.; Boretzky, K.; Borge, M. J. G.; Chartier, M.; Chatillon, A.; Chulkov, L. V.; Cortina-Gil, D.; Emling, H.; Ershova, O.; Fraile, L. M.; Fynbo, H. O. U.; Galaviz, D.; Geissel, H.; Heil, M.; Hoffmann, D. H. H.; Johansson, H. T.; Jonson, B.; Karagiannis, C.; Kiselev, O. A.; Kratz, J. V.; Kulessa, R.; Kurz, N.; Langer, C.; Lantz, M.; Le Bleis, T.; Lemmon, R.; Litvinov, Yu. A.; Mahata, K.; Müntz, C.; Nilsson, T.; Nociforo, C.; Nyman, G.; Ott, W.; Panin, V.; Paschalis, S.; Perea, A.; Plag, R.; Reifarth, R.; Richter, A.; Rodriguez-Tajes, C.; Rossi, D.; Riisager, K.; Savran, D.; Schrieder, G.; Simon, H.; Stroth, J.; Sümmerer, K.; Tengblad, O.; Weick, H.; Wimmer, C.; Zhukov, M. V. (4 April 2014). "First Observation of the Unbound Nucleus 15Ne" (PDF). Physical Review Letters. 112 (13): 132502. doi:10.1103/PhysRevLett.112.132502 – via APS.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.