Neon-22 is a radioisotope of the chemical element neon, which has 12 neutrons in its atomic nucleus in addition to the element-specific 10 protons; the sum of the number of these atomic nucleus building blocks results in a mass number of 22.
22Ne is one of the three stable isotopes that make up the natural Ne gas on earth, accounting for 9.25 %.
The discovery of neon-22 is attributed to the British Joseph John Thomson, who was the first to describe the observation of an isotope of a stable element (1913) and recognized that neon is composed of different isotopes [1].
See also: list of Neon isotopes.
Direct parent isotopes are: 23F, 22Na.
Atomic Mass ma | Quantity | Half-life | Spin | |
---|---|---|---|---|
Neon Isotopic mixture | 20.1797 u | 100 % | ||
Isotope 20Ne | 19.99244018(2) u | 90.48(3) % [88.47 - 90.51 %] | stable | 0+ |
Isotope 21Ne | 20.9938467(3) u | 0.27(1) % | stable | 3/2+ |
Isotope 22Ne | 21.9913851(2) u | 9.25(3) % | stable | 0+ |
Z | Isotone N = 12 | Isobar A = 22 |
---|---|---|
4 | 16Be | |
5 | 17B | |
6 | 18C | 22C |
7 | 19N | 22N |
8 | 20O | 22O |
9 | 21F | 22F |
10 | 22Ne | 22Ne |
11 | 23Na | 22Na |
12 | 24Mg | 22Mg |
13 | 25Al | 22Al |
14 | 26Si | 22Si |
15 | 27P | |
16 | 28S | |
17 | 29Cl | |
18 | 30Ar |
[1] - Joseph John Thomson:
Bakerian Lecture: Rays of positive electricity.
In: Proceedings of the Royal Society A, 89, 607, (1913), DOI 10.1098/rspa.1913.0057.
Last update: 2024-10-23
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