Neon-29 is a radioisotope of the chemical element neon, which has 19 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 29. The very short-lived, only artificially produced, unstable and thus radioactive nuclide has no practical significance; the study of 29Ne is exclusively for academic purposes and experimental research.
According to a report from 1985, the first observation of the neutron-rich isotope was made by irradiating a tantalum target with argon-40 ions accelerated to 44 MeV/u [1].
See also: List of individual Neon isotopes (and general data sources).
Half-life T½ = 14.7(4) ms respectively 1.47 × 10-2 seconds s.
| Decay mode | Daughter | Probability | Decay energy | γ energy (intensity) |
|---|---|---|---|---|
| β- | 29Na | 68.0(51) % | 15.720(150) MeV | |
| β-, n | 28Na | 28(5) % | 11.317(150) MeV | |
| β-, 2n | 27Na | 4(1) % |
| Z | Isotone N = 19 | Isobar A = 29 |
|---|---|---|
| 8 | 27O | |
| 9 | 28F | 29F |
| 10 | 29Ne | 29Ne |
| 11 | 30Na | 29Na |
| 12 | 31Mg | 29Mg |
| 13 | 32Al | 29Al |
| 14 | 33Si | 29Si |
| 15 | 34P | 29P |
| 16 | 35S | 29S |
| 17 | 36Cl | 29Cl |
| 18 | 37Ar | 29Ar |
| 19 | 38K | |
| 20 | 39Ca | |
| 21 | 40Sc | |
| 22 | 41Ti | |
| 23 | 42V | |
| 24 | 43Cr | |
| 25 | 44Mn | |
| 26 | 45Fe | |
| 27 | 46Co |
[1] - M. Langevin, E. Quiniou, M. Bernas, J. Galin et al.:
Production of neutron-rich nuclei at the limits of particles stability by fragmentation of 44 MeVu 40Ar projectiles.
In: Physics Letters B, 150(1-3), (1985), DOI 10.1016/0370-2693(85)90140-6.
Last update: 2024-10-23
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