Isotopes of neon
Encyclopedia
Neon
(Ne) possesses three stable isotopes, 20Ne, 21Ne, and 22Ne. In addition, 16 radioactive isotopes have been discovered ranging from 16Ne 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 16Ne with a half-life of 122 (37) keV. See isotopes of carbon for notes about the measurement.
Standard atomic mass: 20.1797(6) u
Neon
Neon is the chemical element that has the symbol Ne and an atomic number of 10. Although a very common element in the universe, it is rare on Earth. A colorless, inert noble gas under standard conditions, neon gives a distinct reddish-orange glow when used in either low-voltage neon glow lamps or...
(Ne) possesses three stable isotopes, 20Ne, 21Ne, and 22Ne. In addition, 16 radioactive isotopes have been discovered ranging from 16Ne 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 16Ne with a half-life of 122 (37) keV. See isotopes of carbon for notes about the measurement.
Standard atomic mass: 20.1797(6) u
Table
nuclide symbol |
Z(p Proton The proton is a subatomic particle with the symbol or and a positive electric charge of 1 elementary charge. One or more protons are present in the nucleus of each atom, along with neutrons. The number of protons in each atom is its atomic number.... ) |
N(n Neutron The neutron is a subatomic hadron particle which has the symbol or , no net electric charge and a mass slightly larger than that of a proton. With the exception of hydrogen, nuclei of atoms consist of protons and neutrons, which are therefore collectively referred to as nucleons. The number of... ) |
isotopic mass (u) |
half-life | decay mode(s) | daughter isotope(s)Bold for stable isotopes |
nuclear spin |
representative isotopic composition (mole fraction) |
range of natural variation (mole fraction) |
---|---|---|---|---|---|---|---|---|---|
16Ne | 10 | 6 | 16.025761(22) | 9×10−21 s [122(37) keV] |
2p Proton emission Proton emission is a type of radioactive decay in which a proton is ejected from a nucleus. Proton emission can occur from high-lying excited states in a nucleus following a beta decay, in which case the process is known as beta-delayed proton emission, or can occur from the ground state of very... |
14O | 0+ | ||
17NeHas 2 halo protons | 10 | 7 | 17.017672(29) | 109.2(6) ms | β+ Beta decay In nuclear physics, beta decay is a type of radioactive decay in which a beta particle is emitted from an atom. There are two types of beta decay: beta minus and beta plus. In the case of beta decay that produces an electron emission, it is referred to as beta minus , while in the case of a... , p (96.0%) |
16O | 1/2- | ||
β+, α Alpha decay Alpha decay is a type of radioactive decay in which an atomic nucleus emits an alpha particle and thereby transforms into an atom with a mass number 4 less and atomic number 2 less... (2.7%) |
13C | ||||||||
β+ (1.3%) | 17F | ||||||||
18Ne | 10 | 8 | 18.0057082(3) | 1.672(8) s | β+ | 18F | 0+ | ||
2p (possibly 2He Diproton A diproton is a hypothetical isotope of helium nucleus consisting of two protons and no neutrons, and is predicted to be less stable than 5He... ) |
16O | ||||||||
19Ne | 10 | 9 | 19.0018802(3) | 17.296(5) s+ | β+ | 19F | 1/2+ | ||
20Ne | 10 | 10 | 19.9924401754(19) | Stable | 0+ | 0.9048(3) | 0.8847-0.9051 | ||
21Ne | 10 | 11 | 20.99384668(4) | Stable | 3/2+ | 0.0027(1) | 0.0027-0.0171 | ||
22Ne | 10 | 12 | 21.991385114(19) | Stable | 0+ | 0.0925(3) | 0.0920-0.0996 | ||
23Ne | 10 | 13 | 22.99446690(11) | 37.24(12) s | β- | 23Na | 5/2+ | ||
24Ne | 10 | 14 | 23.9936108(4) | 3.38(2) min | β- | 24Na | 0+ | ||
25Ne | 10 | 15 | 24.997737(28) | 602(8) ms | β- | 25Na | (3/2)+ | ||
26Ne | 10 | 16 | 26.000461(29) | 197(1) ms | β- (99.87%) | 26Na | 0+ | ||
β-, n Neutron emission Neutron emission is a type of radioactive decay of atoms containing excess neutrons, in which a neutron is simply ejected from the nucleus. Two examples of isotopes which emit neutrons are helium-5 and beryllium-13... (.13%) |
25Na | ||||||||
27Ne | 10 | 17 | 27.00759(12) | 32(2) ms | β- (98.0%) | 27Na | (3/2+)# | ||
β-, n (2.0%) | 26Na | ||||||||
28Ne | 10 | 18 | 28.01207(16) | 18.3(22) ms | β- (78.0%) | 28Na | 0+ | ||
β-, n (22.0%) | 27Na | ||||||||
29Ne | 10 | 19 | 29.01939(29) | 15.6(5) ms | β- | 29Na | (3/2+)# | ||
30Ne | 10 | 20 | 30.02480(61) | 5.8(2) ms | β- | 30Na | 0+ | ||
31Ne | 10 | 21 | 31.03311(97)# | 3.4(8) ms | β- | 31Na | 7/2-# | ||
β-, n | 30Na | ||||||||
32Ne | 10 | 22 | 32.04002(86)# | 3.5(9) ms | β-, n | 31Na | 0+ | ||
β- | 32Na | ||||||||
33Ne | 10 | 23 | 33.04938(86)# | <260 ns | 7/2-# | ||||
34Ne | 10 | 24 | 34.05703(87)# | 1# ms [>1.5 µs] | 0+ |