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Standard atomic weight Ar°(Te) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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There are 39 known isotopes and 17 nuclear isomers of tellurium (52Te), with atomic masses that range from 104 to 142. These are listed in the table below.
Naturally-occurring tellurium on Earth consists of eight isotopes. Two of these have been found to be radioactive: 128Te and 130Te undergo double beta decay with half-lives of, respectively, 2.2×1024 (2.2 septillion) years (the longest half-life of all nuclides proven to be radioactive) [5] and 8.2×1020 (820 quintillion) years. The longest-lived artificial radioisotope of tellurium is 121Te with a half-life of about 19 days. Several nuclear isomers have longer half-lives, the longest being 121mTe with a half-life of 154 days.
The very-long-lived radioisotopes 128Te and 130Te are the two most common isotopes of tellurium. Of elements with at least one stable isotope, only indium and rhenium likewise have a radioisotope in greater abundance than a stable one.
It has been claimed that electron capture of 123Te was observed, but more recent measurements of the same team have disproved this. [6] The half-life of 123Te is longer than 9.2 × 1016 years, and probably much longer. [6]
124Te can be used as a starting material in the production of radionuclides by a cyclotron or other particle accelerators. Some common radionuclides that can be produced from tellurium-124 are iodine-123 and iodine-124.
The short-lived isotope 135Te (half-life 19 seconds) is produced as a fission product in nuclear reactors. It decays, via two beta decays, to 135Xe, the most powerful known neutron absorber, and the cause of the iodine pit phenomenon.
With the exception of beryllium, tellurium is the second lightest element observed to have isotopes capable of undergoing alpha decay, with isotopes 104Te to 109Te being seen to undergo this mode of decay. Some lighter elements, namely those in the vicinity of 8Be, have isotopes with delayed alpha emission (following proton or beta emission) as a rare branch.
Nuclide [n 1] | Z | N | Isotopic mass (Da) [7] [n 2] [n 3] | Half-life [1] [n 4] [n 5] | Decay mode [1] [n 6] | Daughter isotope [n 7] | Spin and parity [1] [n 8] [n 5] | Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy | Normal proportion [1] | Range of variation | |||||||||||||||||
104Te | 52 | 52 | 103.94672(34) | <4 ns | α | 100Sn | 0+ | ||||||||||||
105Te | 52 | 53 | 104.94330(32) | 633(66) ns | α | 101Sn | (7/2+) | ||||||||||||
106Te | 52 | 54 | 105.93750(11) | 78(11) μs | α | 102Sn | 0+ | ||||||||||||
107Te | 52 | 55 | 106.93488(11)# | 3.22(9) ms | α (70%) | 103Sn | 5/2+# | ||||||||||||
β+ (30%) | 107Sb | ||||||||||||||||||
108Te | 52 | 56 | 107.9293805(58) | 2.1(1) s | α (49%) | 104Sn | 0+ | ||||||||||||
β+ (48.6%) | 108Sb | ||||||||||||||||||
β+, p (2.4%) | 107Sn | ||||||||||||||||||
β+, α (<0.065%) | 104In | ||||||||||||||||||
109Te | 52 | 57 | 108.9273045(47) | 4.4(2) s | β+ (86.7%) | 109Sb | (5/2+) | ||||||||||||
β+, p (9.4%) | 108Sn | ||||||||||||||||||
α (3.9%) | 105Sn | ||||||||||||||||||
β+, α (<0.0049%) | 105In | ||||||||||||||||||
110Te | 52 | 58 | 109.9224581(71) | 18.6(8) s | β+ | 110Sb | 0+ | ||||||||||||
111Te | 52 | 59 | 110.9210006(69) | 26.2(6) s | β+ | 111Sb | (5/2)+ | ||||||||||||
β+, p (?%) | 110Sn | ||||||||||||||||||
112Te | 52 | 60 | 111.9167278(90) | 2.0(2) min | β+ | 112Sb | 0+ | ||||||||||||
113Te | 52 | 61 | 112.915891(30) | 1.7(2) min | β+ | 113Sb | (7/2+) | ||||||||||||
114Te | 52 | 62 | 113.912088(26) | 15.2(7) min | β+ | 114Sb | 0+ | ||||||||||||
115Te | 52 | 63 | 114.911902(30) | 5.8(2) min | β+ | 115Sb | 7/2+ | ||||||||||||
115m1Te [n 9] | 10(6) keV | 6.7(4) min | β+ | 115Sb | (1/2+) | ||||||||||||||
115m2Te | 280.05(20) keV | 7.5(2) μs | IT | 115Te | 11/2− | ||||||||||||||
116Te | 52 | 64 | 115.908466(26) | 2.49(4) h | β+ | 116Sb | 0+ | ||||||||||||
117Te | 52 | 65 | 116.908646(14) | 62(2) min | EC (75%) | 117Sb | 1/2+ | ||||||||||||
β+ | 117Sb | ||||||||||||||||||
117mTe | 296.1(5) keV | 103(3) ms | IT | 117Te | (11/2−) | ||||||||||||||
118Te | 52 | 66 | 117.905860(20) | 6.00(2) d | EC | 118Sb | 0+ | ||||||||||||
119Te | 52 | 67 | 118.9064057(78) | 16.05(5) h | EC (97.94%) | 119Sb | 1/2+ | ||||||||||||
β+ (2.06%) | 119Sb | ||||||||||||||||||
119mTe | 260.96(5) keV | 4.70(4) d | EC (99.59%) | 119Sb | 11/2− | ||||||||||||||
β+ (0.41%) | 119Sb | ||||||||||||||||||
120Te | 52 | 68 | 119.9040658(19) | Observationally Stable [n 10] | 0+ | 9(1)×10−4 | |||||||||||||
121Te | 52 | 69 | 120.904945(28) | 19.31(7) d | β+ | 121Sb | 1/2+ | ||||||||||||
121mTe | 293.974(22) keV | 164.7(5) d | IT (88.6%) | 121Te | 11/2− | ||||||||||||||
β+ (11.4%) | 121Sb | ||||||||||||||||||
122Te | 52 | 70 | 121.9030447(15) | Stable | 0+ | 0.0255(12) | |||||||||||||
123Te | 52 | 71 | 122,9042710(15) | Observationally Stable [n 11] | 1/2+ | 0.0089(3) | |||||||||||||
123mTe | 247.47(4) keV | 119.2(1) d | IT | 123Te | 11/2− | ||||||||||||||
124Te | 52 | 72 | 123.9028183(15) | Stable | 0+ | 0.0474(14) | |||||||||||||
125Te [n 12] | 52 | 73 | 124.9044312(15) | Stable | 1/2+ | 0.0707(15) | |||||||||||||
125mTe | 144.775(8) keV | 57.40(15) d | IT | 125Te | 11/2− | ||||||||||||||
126Te | 52 | 74 | 125.9033121(15) | Stable | 0+ | 0.1884(25) | |||||||||||||
127Te [n 12] | 52 | 75 | 126.9052270(15) | 9.35(7) h | β− | 127I | 3/2+ | ||||||||||||
127mTe | 88.23(7) keV | 106.1(7) d | IT (97.86%) | 127Te | 11/2− | ||||||||||||||
β− (2.14%) | 127I | ||||||||||||||||||
128Te [n 12] [n 13] | 52 | 76 | 127.90446124(76) | 2.25(9)×1024 y [n 14] | β−β− | 128Xe | 0+ | 0.3174(8) | |||||||||||
128mTe | 2790.8(3) keV | 363(27) ns | IT | 128Te | (10+) | ||||||||||||||
129Te [n 12] | 52 | 77 | 128.90659642(76) | 69.6(3) min | β− | 129I | 3/2+ | ||||||||||||
129mTe | 105.51(3) keV | 33.6(1) d | IT (64%) | 129Te | 11/2− | ||||||||||||||
β− (36%) | 129I | ||||||||||||||||||
130Te [n 12] [n 13] | 52 | 78 | 129.906222745(11) | 7.91(21)×1020 y | β−β− | 130Xe | 0+ | 0.3408(62) | |||||||||||
130m1Te | 2146.41(4) keV | 186(11) ns | IT | 130Te | 7− | ||||||||||||||
130m2Te | 2667.2(8) keV | 1.90(8) μs | IT | 130Te | (10+) | ||||||||||||||
130m3Te | 4373.9(9) keV | 53(8) ns | IT | 130Te | (15−) | ||||||||||||||
131Te [n 12] | 52 | 79 | 130.908522210(65) | 25.0(1) min | β− | 131I | 3/2+ | ||||||||||||
131m1Te | 182.258(18) keV | 32.48(11) h | β− (74.1%) | 131I | 11/2− | ||||||||||||||
IT (25.9%) | 131Te | ||||||||||||||||||
131m2Te | 1940.0(4) keV | 93(12) ms | IT | 131Te | (23/2+) | ||||||||||||||
132Te [n 12] | 52 | 80 | 131.9085467(37) | 3.204(13) d | β− | 132I | 0+ | ||||||||||||
132m1Te | 1774.80(9) keV | 145(8) ns | IT | 132Te | 6+ | ||||||||||||||
132m2Te | 1925.47(9) keV | 28.5(9) μs | IT | 132Te | 7− | ||||||||||||||
132m3Te | 2723.3(8) keV | 3.62(6) μs | IT | 132Te | (10+) | ||||||||||||||
133Te | 52 | 81 | 132.9109633(22) | 12.5(3) min | β− | 133I | 3/2+# | ||||||||||||
133m1Te | 334.26(4) keV | 55.4(4) min | β− (83.5%) | 133I | (11/2−) | ||||||||||||||
IT (16.5%) | 133Te | ||||||||||||||||||
133m2Te | 1610.4(5) keV | 100(5) ns | IT | 133Te | (19/2−) | ||||||||||||||
134Te | 52 | 82 | 133.9113964(29) | 41.8(8) min | β− | 134I | 0+ | ||||||||||||
134mTe | 1691.34(16) keV | 164.5(7) ns | IT | 134Te | 6+ | ||||||||||||||
135Te [n 15] | 52 | 83 | 134.9165547(18) | 19.0(2) s | β− | 135I | (7/2−) | ||||||||||||
135mTe | 1554.89(16) keV | 511(20) ns | IT | 135Te | (19/2−) | ||||||||||||||
136Te | 52 | 84 | 135.9201012(24) | 17.63(9) s | β− (98.63%) | 136I | 0+ | ||||||||||||
β−, n (1.37%) | 135I | ||||||||||||||||||
137Te | 52 | 85 | 136.9255994(23) | 2.49(5) s | β− (97.06%) | 137I | 3/2−# | ||||||||||||
β−, n (2.94%) | 136I | ||||||||||||||||||
138Te | 52 | 86 | 137.9294725(41) | 1.46(25) s | β− (95.20%) | 138I | 0+ | ||||||||||||
β−, n (4.80%) | 137I | ||||||||||||||||||
139Te | 52 | 87 | 138.9353672(38) | 724(81) ms | β− | 139I | 5/2−# | ||||||||||||
140Te | 52 | 88 | 139.939487(15) | 351(5) ms | β− (?%) | 140I | 0+ | ||||||||||||
β−, n (?%) | 139I | ||||||||||||||||||
141Te | 52 | 89 | 140.94560(43)# | 193(16) ms | β− | 141I | 5/2−# | ||||||||||||
142Te | 52 | 90 | 141.95003(54)# | 147(8) ms | β− | 142I | 0+ | ||||||||||||
143Te | 52 | 91 | 142.95649(54)# | 120(8) ms | β− | 143I | 7/2+# | ||||||||||||
144Te | 52 | 92 | 143.96112(32)# | 93(60) ms | β− | 144I | 0+ | ||||||||||||
145Te | 52 | 93 | 144.96778(32)# | 75# ms [>550 ns] | β− | 145I | |||||||||||||
This table header & footer: |
EC: | Electron capture |
IT: | Isomeric transition |
n: | Neutron emission |
p: | Proton emission |
There are seven stable isotopes of mercury (80Hg) with 202Hg being the most abundant (29.86%). The longest-lived radioisotopes are 194Hg with a half-life of 444 years, and 203Hg with a half-life of 46.612 days. Most of the remaining 40 radioisotopes have half-lives that are less than a day. 199Hg and 201Hg are the most often studied NMR-active nuclei, having spin quantum numbers of 1/2 and 3/2 respectively. All isotopes of mercury are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed. These isotopes are predicted to undergo either alpha decay or double beta decay.
There are two natural isotopes of iridium (77Ir), and 37 radioisotopes, the most stable radioisotope being 192Ir with a half-life of 73.83 days, and many nuclear isomers, the most stable of which is 192m2Ir with a half-life of 241 years. All other isomers have half-lives under a year, most under a day. All isotopes of iridium are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed.
Naturally occurring lutetium (71Lu) is composed of one stable isotope 175Lu and one long-lived radioisotope, 176Lu with a half-life of 37 billion years. Forty radioisotopes have been characterized, with the most stable, besides 176Lu, being 174Lu with a half-life of 3.31 years, and 173Lu with a half-life of 1.37 years. All of the remaining radioactive isotopes have half-lives that are less than 9 days, and the majority of these have half-lives that are less than half an hour. This element also has 18 meta states, with the most stable being 177mLu, 174mLu and 178mLu.
Naturally occurring gadolinium (64Gd) is composed of 6 stable isotopes, 154Gd, 155Gd, 156Gd, 157Gd, 158Gd and 160Gd, and 1 radioisotope, 152Gd, with 158Gd being the most abundant (24.84% natural abundance). The predicted double beta decay of 160Gd has never been observed; only a lower limit on its half-life of more than 1.3×1021 years has been set experimentally.
Naturally occurring samarium (62Sm) is composed of five stable isotopes, 144Sm, 149Sm, 150Sm, 152Sm and 154Sm, and two extremely long-lived radioisotopes, 147Sm and 148Sm, with 152Sm being the most abundant. 146Sm is also fairly long-lived, but is not long-lived enough to have survived in significant quantities from the formation of the Solar System on Earth, although it remains useful in radiometric dating in the Solar System as an extinct radionuclide. It is the longest-lived nuclide that has not yet been confirmed to be primordial.
Naturally occurring neodymium (60Nd) is composed of 5 stable isotopes, 142Nd, 143Nd, 145Nd, 146Nd and 148Nd, with 142Nd being the most abundant (27.2% natural abundance), and 2 long-lived radioisotopes, 144Nd and 150Nd. In all, 33 radioisotopes of neodymium have been characterized up to now, with the most stable being naturally occurring isotopes 144Nd (alpha decay, a half-life (t1/2) of 2.29×1015 years) and 150Nd (double beta decay, t1/2 of 7×1018 years), and for practical purposes they can be considered to be stable as well. All of the remaining radioactive isotopes have half-lives that are less than 12 days, and the majority of these have half-lives that are less than 70 seconds; the most stable artificial isotope is 147Nd with a half-life of 10.98 days. This element also has 13 known meta states with the most stable being 139mNd (t1/2 5.5 hours), 135mNd (t1/2 5.5 minutes) and 133m1Nd (t1/2 ~70 seconds).
Naturally occurring cerium (58Ce) is composed of 4 stable isotopes: 136Ce, 138Ce, 140Ce, and 142Ce, with 140Ce being the most abundant and the only one theoretically stable; 136Ce, 138Ce, and 142Ce are predicted to undergo double beta decay but this process has never been observed. There are 35 radioisotopes that have been characterized, with the most stable being 144Ce, with a half-life of 284.893 days; 139Ce, with a half-life of 137.640 days and 141Ce, with a half-life of 32.501 days. All of the remaining radioactive isotopes have half-lives that are less than 4 days and the majority of these have half-lives that are less than 10 minutes. This element also has 10 meta states.
Naturally occurring lanthanum (57La) is composed of one stable (139La) and one radioactive (138La) isotope, with the stable isotope, 139La, being the most abundant (99.91% natural abundance). There are 39 radioisotopes that have been characterized, with the most stable being 138La, with a half-life of 1.02×1011 years; 137La, with a half-life of 60,000 years and 140La, with a half-life of 1.6781 days. The remaining radioactive isotopes have half-lives that are less than a day and the majority of these have half-lives that are less than 1 minute. This element also has 12 nuclear isomers, the longest-lived of which is 132mLa, with a half-life of 24.3 minutes. Lighter isotopes mostly decay to isotopes of barium and heavy ones mostly decay to isotopes of cerium. 138La can decay to both.
Naturally occurring barium (56Ba) is a mix of six stable isotopes and one very long-lived radioactive primordial isotope, barium-130, identified as being unstable by geochemical means (from analysis of the presence of its daughter xenon-130 in rocks) in 2001. This nuclide decays by double electron capture (absorbing two electrons and emitting two neutrinos), with a half-life of (0.5–2.7)×1021 years (about 1011 times the age of the universe).
Naturally occurring xenon (54Xe) consists of seven stable isotopes and two very long-lived isotopes. Double electron capture has been observed in 124Xe and double beta decay in 136Xe, 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 this process has never been observed in these isotopes, so they are considered to be stable. Beyond these stable forms, 32 artificial unstable isotopes and various isomers have been studied, the longest-lived of which is 127Xe with a half-life of 36.345 days. All other isotopes have half-lives less than 12 days, most less than 20 hours. 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 11.934 days. 129Xe is produced by beta decay of 129I ; 131mXe, 133Xe, 133mXe, and 135Xe are some of the fission products of both 235U and 239Pu, so are used as indicators of nuclear explosions.
There are 40 known isotopes of iodine (53I) from 108I to 147I; all undergo radioactive decay except 127I, which is stable. Iodine is thus a monoisotopic element.
Tin (50Sn) is the element with the greatest number of stable isotopes. This is probably related to the fact that 50 is a "magic number" of protons. In addition, twenty-nine unstable tin isotopes are known, including tin-100 (100Sn) and tin-132 (132Sn), which are both "doubly magic". The longest-lived tin radioisotope is tin-126 (126Sn), with a half-life of 230,000 years. The other 28 radioisotopes have half-lives of less than a year.
Indium (49In) consists of two primordial nuclides, with the most common (~ 95.7%) nuclide (115In) being measurably though weakly radioactive. Its spin-forbidden decay has a half-life of 4.41×1014 years, much longer than the currently accepted age of the Universe.
Naturally occurring cadmium (48Cd) is composed of 8 isotopes. For two of them, natural radioactivity was observed, and three others are predicted to be radioactive but their decays have not been observed, due to extremely long half-lives. The two natural radioactive isotopes are 113Cd (beta decay, half-life is 8.04 × 1015 years) and 116Cd (two-neutrino double beta decay, half-life is 2.8 × 1019 years). The other three are 106Cd, 108Cd (double electron capture), and 114Cd (double beta decay); only lower limits on their half-life times have been set. Three isotopes—110Cd, 111Cd, and 112Cd—are theoretically stable. Among the isotopes absent in natural cadmium, the most long-lived are 109Cd with a half-life of 462.6 days, and 115Cd with a half-life of 53.46 hours. All of the remaining radioactive isotopes have half-lives that are less than 2.5 hours and the majority of these have half-lives that are less than 5 minutes. This element also has 12 known meta states, with the most stable being 113mCd (t1/2 14.1 years), 115mCd (t1/2 44.6 days) and 117mCd (t1/2 3.36 hours).
Naturally occurring rhodium (45Rh) is composed of only one stable isotope, 103Rh. The most stable radioisotopes are 101Rh with a half-life of 3.3 years, 102Rh with a half-life of 207 days, and 99Rh with a half-life of 16.1 days. Thirty other radioisotopes have been characterized with atomic weights ranging from 88.949 u (89Rh) to 121.943 u (122Rh). Most of these have half-lives that are less than an hour except 100Rh and 105Rh. There are also numerous meta states with the most stable being 102mRh (0.141 MeV) with a half-life of about 3.7 years and 101mRh (0.157 MeV) with a half-life of 4.34 days.
Naturally occurring ruthenium (44Ru) is composed of seven stable isotopes. Additionally, 27 radioactive isotopes have been discovered. Of these radioisotopes, the most stable are 106Ru, with a half-life of 373.59 days; 103Ru, with a half-life of 39.26 days and 97Ru, with a half-life of 2.9 days.
Naturally occurring niobium (41Nb) is composed of one stable isotope (93Nb). The most stable radioisotope is 92Nb with a half-life of 34.7 million years. The next longest-lived niobium isotopes are 94Nb and 91Nb with a half-life of 680 years. There is also a meta state of 93Nb at 31 keV whose half-life is 16.13 years. Twenty-seven other radioisotopes have been characterized. Most of these have half-lives that are less than two hours, except 95Nb, 96Nb and 90Nb. The primary decay mode before stable 93Nb is electron capture and the primary mode after is beta emission with some neutron emission occurring in 104–110Nb.
Rubidium (37Rb) has 36 isotopes, with naturally occurring rubidium being composed of just two isotopes; 85Rb (72.2%) and the radioactive 87Rb (27.8%).
Bromine (35Br) has two stable isotopes, 79Br and 81Br, and 35 known radioisotopes, the most stable of which is 77Br, with a half-life of 57.036 hours.
Naturally occurring vanadium (23V) is composed of one stable isotope 51V and one radioactive isotope 50V with a half-life of 2.71×1017 years. 24 artificial radioisotopes have been characterized (in the range of mass number between 40 and 65) with the most stable being 49V with a half-life of 330 days, and 48V with a half-life of 15.9735 days. All of the remaining radioactive isotopes have half-lives shorter than an hour, the majority of them below 10 seconds, the least stable being 42V with a half-life shorter than 55 nanoseconds, with all of the isotopes lighter than it, and none of the heavier, have unknown half-lives. In 4 isotopes, metastable excited states were found (including 2 metastable states for 60V), which adds up to 5 meta states.