Naturally occurring xenon (54Xe) consists of nine isotopes: seven stable isotopes and two very long-lived radioactive isotopes: double electron capture has been observed in 124Xe (half-life 1.1 ± 0.2stat ± 0.1sys×1022 years), and double beta decay in 136Xe (half-life 2.18 ×1021 years), which are among the longest measured half-lives of all nuclides. The isotopes 126Xe and 134Xe are also predicted to undergo double beta decay, but such decay processes have not been observed. Artificial unstable isotopes have been prepared from 108Xe to 150Xe, the longest-lived of which is 127Xe with a half-life of 36.342 days. All other nuclides have half-lives less than 12 days, most less than one hour. The shortest-lived isotope, 108Xe, has a half-life of 58 μs, and is the heaviest known nuclide with equal numbers of protons and neutrons. Of known isomers, the longest-lived is 131mXe with a half-life of 11.95 days, the second longest of all xenon's nuclides.

129Xe is produced by beta decay of natural or artificial 129I (half-life 16.1 million years); 131mXe, 133Xe, 133mXe, and 135Xe are some of the fission products of both 235U and 239Pu, so are used as indicators of nuclear explosions.

The artificial isotope 135Xe is of considerable significance in the operation of nuclear fission reactors. 135Xe has a huge cross section for thermal neutrons, 2.65 million barns, so it acts as a neutron absorber or "poison" that can slow or stop the chain reaction after a period of operation. This was discovered in the earliest nuclear reactors built by the American Manhattan Project for plutonium production. Because of this effect, designers must make provisions to increase the reactor's reactivity (the number of neutrons per fission that go on to fission other atoms of nuclear fuel) over the initial value needed to start the chain reaction. For the same reason, the xenon fission products produced in a nuclear explosion and a power plant differ significantly as a large share of 135Xe will absorb neutrons in a steady state reactor, while in a bomb it can be assumed that none of the 135I will have had time to decay to xenon before the explosion disperses it, removing it from the neutron radiation.

Relatively high concentrations of radioactive xenon isotopes are also found emanating from nuclear reactors due to the release of this fission gas from cracked fuel rods or fissioning of uranium in cooling water.[citation needed] The concentrations of these isotopes are still usually low compared to the naturally occurring radioactive noble gas 222Rn.

Because xenon is a tracer for two parent isotopes, Xe isotope ratios in meteorites are a powerful tool for studying the formation of the Solar System. The I-Xe method of dating gives the time elapsed between nucleosynthesis and the condensation of a solid object from the solar nebula (xenon being a gas, only that part of it that formed after condensation will be present inside the object). Xenon isotopes are also a powerful tool for understanding terrestrial differentiation. Excess 129Xe found in carbon dioxide well gases from New Mexico was believed to be from the decay of mantle-derived gases soon after Earth's formation. It has been suggested[clarification needed] that the isotopic composition of atmospheric xenon fluctuated prior to the GOE before stabilizing, perhaps as a result of the rise in atmospheric O2.

List of isotopes

NuclideZNIsotopic mass (Da)Discovery yearHalf-lifeDecay modeDaughter isotopeSpin and parityNatural abundance (mole fraction)
Excitation energyNormal proportionRange of variation
108Xe5454107.95423(41)72(35) μsα104Te0+
109Xe5455108.95076(32)#13(2) msα105Te(7/2+)
110Xe5456109.94426(11)93(3) msα (64%)106Te0+
β+ (36%)110I
111Xe5457110.941460(64)740(200) msβ+ (89.6%)111I5/2+#
α (10.4%)107Te
112Xe5458111.9355591(89)2.7(8) sβ+ (98.8%)112I0+
α (1.2%)108Te
113Xe5459112.9332217(73)2.74(8) sβ+ (92.98%)113I5/2+#
β+, p (7%)112Te
α (?%)109Te
β+, α (~0.007%)109Sb
113mXe403.6(14) keV6.9(3) μsIT113Xe(11/2−)
114Xe5460113.927980(12)10.0(4) sβ+114I0+
115Xe5461114.926294(13)18(3) sβ+ (99.66%)115I(5/2+)
β+, p (0.34%)114Te
116Xe5462115.921581(14)59(2) sβ+116I0+
117Xe5463116.920359(11)61(2) sβ+117I5/2+
β+, p (0.0029%)116Te
118Xe5464117.916179(11)3.8(9) minβ+118I0+
119Xe5465118.915411(11)5.8(3) minβ+ (79%)119I5/2+
EC (21%)119I
120Xe5466119.911784(13)46.0(6) minβ+120I0+
121Xe5467120.911453(11)40.1(20) minβ+121I5/2+
122Xe5468121.908368(12)20.1(1) hEC122I0+
123Xe5469122.908482(10)2.08(2) hβ+123I1/2+
123mXe185.18(11) keV5.49(26) μsIT123Xe7/2−
124Xe5470123.9058852(15)1.1(2)×1022 yDouble EC124Te0+9.5(5)×10−4
125Xe5471124.9063876(15)16.87(8) hEC / β+125I1/2+
125m1Xe252.61(14) keV56.9(9) sIT125Xe9/2−
125m2Xe295.89(15) keV0.14(3) μsIT125Xe7/2+
126Xe5472125.904297422(6)Observationally Stable0+8.9(3)×10−4
127Xe5473126.9051836(44)36.342(3) dEC127I1/2+
127mXe297.10(8) keV69.2(9) sIT127Xe9/2−
128Xe5474127.9035307534(56)Stable0+0.01910(13)
128mXe2787.2(3) keV(1984)83(2) nsIT128Xe8−
129Xe5475128.9047808574(54)Stable1/2+0.26401(138)
129mXe236.14(3) keV8.88(2) dIT129Xe11/2−
130Xe5476129.903509346(10)Stable0+0.04071(22)
131Xe5477130.9050841281(55)Stable3/2+0.21232(51)
131mXe163.930(8) keV11.948(12) dIT131Xe11/2−
132Xe5478131.9041550835(54)Stable0+0.26909(55)
132mXe2752.21(17) keV8.39(11) msIT132Xe(10+)
133Xe5479132.9059107(26)5.2474(5) dβ−133Cs3/2+
133m1Xe233.221(15) keV2.198(13) dIT133Xe11/2−
133m2Xe2147(20)# keV8.64(13) msIT133Xe(23/2+)
134Xe5480133.905393030(6)Observationally Stable0+0.10436(35)
134m1Xe1965.5(5) keV(1968)290(17) msIT134Xe7−
134m2Xe3025.2(15) keV5(1) μsIT134Xe(10+)
135Xe5481134.9072314(39)9.14(2) hβ−135Cs3/2+
135mXe526.551(13) keV15.29(5) minIT (99.70%)135Xe11/2−
β− (0.30%)135Cs
136Xe5482135.907214474(7)2.18(5)×1021 yβ−β−136Ba0+0.08857(72)
136mXe1891.74(7) keV2.92(3) μsIT136Xe6+
137Xe5483136.91155777(11)3.818(13) minβ−137Cs7/2−
138Xe5484137.9141463(30)14.14(7) minβ−138Cs0+
139Xe5485138.9187922(23)39.68(14) sβ−139Cs3/2−
140Xe5486139.9216458(25)13.60(10) sβ−140Cs0+
141Xe5487140.9267872(31)1.73(1) sβ− (99.96%)141Cs5/2−
β−, n (0.044%)140Cs
142Xe5488141.9299731(29)1.23(2) sβ− (99.63%)142Cs0+
β−, n (0.37%)141Cs
143Xe5489142.9353696(50)511(6) msβ− (99.00%)143Cs5/2−
β−, n (1.00%)142Cs
144Xe5490143.9389451(57)0.388(7) sβ− (97.0%)144Cs0+
β−, n (3.0%)143Cs
145Xe5491144.944720(12)188(4) msβ− (95.0%)145Cs3/2−#
β−, n (5.0%)144Cs
146Xe5492145.948518(26)146(6) msβ−146Cs0+
β−, n (6.9%)145Cs
147Xe5493146.95448(22)#88(14) msβ− (>92%)147Cs3/2−#
β−, n (<8%)146Cs
148Xe5494147.95851(32)#85(15) msβ−148Cs0+
149Xe5495148.96457(32)#50# ms [>550 ms]3/2−#
150Xe5496149.96888(32)#40# ms [>550 ns]0+
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Xenon-124

Xenon-124 is an isotope of xenon that undergoes double electron capture to tellurium-124 with a very long half-life of 1.1×1022 years, approximately 12 orders of magnitude longer than the age of the universe. This decay was observed in the XENON1T detector in 2019, and is the slowest one ever directly observed. (Even slower decays of other nuclei have been measured, but by detecting decay products that have accumulated over billions of years rather than observing them directly.)

Xenon-129

MRI with inhaled 129Xe shows improved ventilation over time. H (grayscale) + 129Xe MRI (cyan) slices at day 0, day 28, 1-y and 2.5-y follow-up, Anti-IL-5Rα (benralizumab)-treated Eosinophilic Asthma

Xenon-129 is a stable nuclide that is inhaled to assess pulmonary function, and to image the lungs by xenon NMR (see image).

Xenon-133

Xenon-133 is a radioisotope of xenon, beta decaying to stable caesium-133 with half-life 5.2474 days. Sold as a drug under the brand name Xeneisol, (ATC code V09EX03 ()) it is inhaled to assess pulmonary function, and to image the lungs. It is also used to image blood flow, particularly in the brain. 133Xe is a fission product produced by fission of uranium-235. It is discharged to the atmosphere in small quantities by some nuclear power plants.

Xenon-135

Xenon-135 is a radioactive isotope of xenon, produced as a fission product of uranium. It has a half-life of 9.14 hours and is the most powerful known neutron-absorbing nuclear poison (having a neutron absorption cross-section of about 2 million barns). The overall yield of xenon-135 from fission is 6.3%, without considering any loss by neutron capture. 135Xe exerts a significant effect on nuclear reactor operation (xenon pit). It is discharged to the atmosphere in small quantities by some nuclear power plants.

Xenon-136

Xenon-136 is an isotope of xenon that undergoes double beta decay to barium-136 with a very long half-life of 2.18×1021 years, approximately 11 orders of magnitude longer than the age of the universe. It is being used in the Enriched Xenon Observatory experiment to search for neutrinoless double beta decay.

See also

Daughter products other than xenon