| ||||||||||||||||||||||||||||||||||||||
Standard atomic weight Ar°(Bi) | ||||||||||||||||||||||||||||||||||||||
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Bismuth (83Bi) has 41 known isotopes, ranging from 184Bi to 224Bi. Bismuth has no stable isotopes, but does have one very long-lived isotope; thus, the standard atomic weight can be given as 208.98040(1). Although bismuth-209 is now known to be radioactive, it has classically been considered to be a stable isotope because it has a half-life of approximately 2.01×1019 years, which is more than a billion times the age of the universe. Besides 209Bi, the most stable bismuth radioisotopes are 210mBi with a half-life of 3.04 million years, 208Bi with a half-life of 368,000 years and 207Bi, with a half-life of 32.9 years, none of which occurs in nature. All other isotopes have half-lives under 1 year, most under a day. Of naturally occurring radioisotopes, the most stable is radiogenic 210Bi with a half-life of 5.012 days. 210mBi is unusual for being a nuclear isomer with a half-life multiple orders of magnitude longer than that of the ground state.
Nuclide [n 1] | Historic name | Z | N | Isotopic mass (Da) [4] [n 2] [n 3] | Half-life [1] [n 4] | Decay mode [1] [n 5] | Daughter isotope [n 6] | Spin and parity [1] [n 7] [n 8] | Isotopic abundance | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy [n 8] | |||||||||||||||||||
184Bi [5] | 83 | 101 | 184.00135(13)# | 6.6(15) ms | α | 180Tl | 3+# | ||||||||||||
184mBi [n 9] | 150(100)# keV | 13(2) ms | α | 180Tl | 10−# | ||||||||||||||
185Bi [6] | 83 | 102 | 184.99760(9)# | 2.8+2.3 −1.0 μs | p (92%) | 184Pb | (1/2+) | ||||||||||||
α (8%) | 181Tl | ||||||||||||||||||
185mBi | 70(50)# keV | 58(2) μs | IT | 185Bi | (7/2−, 9/2−) | ||||||||||||||
186Bi | 83 | 103 | 185.996623(18) | 14.8(7) ms | α (99.99%) | 182Tl | (3+) | ||||||||||||
β+ (?%) | 186Pb | ||||||||||||||||||
β+, SF (0.011%) | (various) | ||||||||||||||||||
186mBi [n 9] | 170(100)# keV | 9.8(4) ms | α (99.99%) | 182Tl | (10−) | ||||||||||||||
β+ (?%) | 186Pb | ||||||||||||||||||
β+, SF (0.011%) | (various) | ||||||||||||||||||
187Bi | 83 | 104 | 186.993147(11) | 37(2) ms | α | 183Tl | (9/2−) | ||||||||||||
187m1Bi | 108(8) keV | 370(20) μs | α | 183Tl | 1/2+ | ||||||||||||||
187m2Bi | 252(3) keV | 7(5) μs | IT | 187Bi | (13/2+) | ||||||||||||||
188Bi | 83 | 105 | 187.992276(12) | 60(3) ms | α | 184Tl | (3+) | ||||||||||||
β+, SF (0.0014%) | (various) | ||||||||||||||||||
188m1Bi | 66(30) keV | >5 μs | 7+# | ||||||||||||||||
188m2Bi | 153(30) keV | 265(15) ms | α | 184Tl | (10−) | ||||||||||||||
β+, SF (0.0046%) | (various) | ||||||||||||||||||
189Bi | 83 | 106 | 188.989195(22) | 688(5) ms | α | 185Tl | 9/2− | ||||||||||||
189m1Bi | 184(5) keV | 5.0(1) ms | α (83%) | 185Tl | 1/2+ | ||||||||||||||
IT (17%) | 189Bi | ||||||||||||||||||
189m2Bi | 357.6(5) keV | 880(50) ns | IT | 189Bi | 13/2+ | ||||||||||||||
190Bi | 83 | 107 | 189.988625(23) | 6.3(1) s | α (77%) | 186Tl | (3+) | ||||||||||||
β+ (23%) | 190Pb | ||||||||||||||||||
β+, SF (6×10-6%) | (various) | ||||||||||||||||||
190m1Bi | 120(40) keV | 6.2(1) s | α (70%) | 186Tl | 10− | ||||||||||||||
β+ (30%) | 190Pb | ||||||||||||||||||
β+, SF (4×10-6%) | (various) | ||||||||||||||||||
190m2Bi | 121(15) keV | 175(8) ns | IT | 190Bi | (5−) | ||||||||||||||
190m3Bi | 394(40) keV | 1.3(8) μs | IT | 190Bi | (8−) | ||||||||||||||
191Bi | 83 | 108 | 190.985787(8) | 12.4(3) s | α (51%) | 187Tl | 9/2− | ||||||||||||
β+ (49%) | 191Pb | ||||||||||||||||||
191m1Bi | 242(4) keV | 125(8) ms | α (68%) | 187Tl | 1/2+ | ||||||||||||||
IT (?%) | 191Bi | ||||||||||||||||||
β+ (?%) | 191Pb | ||||||||||||||||||
191m2Bi | 429.7(5) keV | 562(10) ns | IT | 191Bi | 13/2+ | ||||||||||||||
191m3Bi | 1875(25)# keV | 400(40) ns | IT | 191Bi | 25/2-# | ||||||||||||||
192Bi | 83 | 109 | 191.98547(3) | 34.6(9) s | β+ (88%) | 192Pb | (3+) | ||||||||||||
α (12%) | 188Tl | ||||||||||||||||||
192mBi | 140(30) keV | 39.6(4) s | β+ (90%) | 192Pb | 10− | ||||||||||||||
α (10%) | 188Tl | ||||||||||||||||||
193Bi | 83 | 110 | 192.982947(8) | 63.6(30) s | β+ (96.5%) | 193Pb | 9/2− | ||||||||||||
α (3.5%) | 189Tl | ||||||||||||||||||
193m1Bi | 305(6) keV | 3.20(14) s | α (84%) | 189Tl | 1/2+ | ||||||||||||||
β+ (16%) | 193Pb | ||||||||||||||||||
193m2Bi | 605.53(18) keV | 153(10) ns | IT | 193Bi | 13/2+ | ||||||||||||||
193m3Bi | 2349.6(6) keV | 85(3) μs | IT | 193Bi | 29/2+ | ||||||||||||||
193m4Bi | 2405.1(7) keV | 3.02(8) μs | IT | 193Bi | (29/2−) | ||||||||||||||
194Bi | 83 | 111 | 193.982799(6) | 95(3) s | β+ (99.54%) | 194Pb | 3+ | ||||||||||||
α (0.46%) | 190Tl | ||||||||||||||||||
194m1Bi | 150(50) keV | 125(2) s | β+ | 194Pb | (6+, 7+) | ||||||||||||||
194m2Bi | 163(4) keV | 115(4) s | β+ (99.80%) | 194Pb | (10−) | ||||||||||||||
α (0.20%) | 190Tl | ||||||||||||||||||
195Bi | 83 | 112 | 194.980649(6) | 183(4) s | β+ (99.97%) | 195Pb | 9/2− | ||||||||||||
α (0.030%) | 191Tl | ||||||||||||||||||
195m1Bi | 399(6) keV | 87(1) s | β+ (67%) | 195Pb | 1/2+ | ||||||||||||||
α (33%) | 191Tl | ||||||||||||||||||
195m2Bi | 2381.0(5) keV | 614(5) ns | IT | 195Bi | (29/2−) | ||||||||||||||
195m3Bi | 2615.9(5) keV | 1.49(1) μs | IT | 195Bi | 29/2+ | ||||||||||||||
196Bi | 83 | 113 | 195.980667(26) | 5.13(20) min | β+ | 196Pb | (3+) | ||||||||||||
α (0.00115%) | 192Tl | ||||||||||||||||||
196m1Bi | 166.4(29) keV | 0.6(5) s | IT | 196Bi | (7+) | ||||||||||||||
196m2Bi | 272(3) keV | 4.00(5) min | β+ (74.2%) | 196Pb | (10−) | ||||||||||||||
IT (25.8%) | 196Bi | ||||||||||||||||||
α (3.8×10−4%) | 196Bi | ||||||||||||||||||
197Bi | 83 | 114 | 196.978865(9) | 9.33(50) min | β+ | 197Pb | 9/2− | ||||||||||||
197m1Bi | 533(12) keV | 5.04(16) min | α (55%) | 193Tl | 1/2+ | ||||||||||||||
β+ (45%) | 197Pb | ||||||||||||||||||
197m2Bi | 2403(12) keV | 263(13) ns | IT | 197Bi | (29/2−) | ||||||||||||||
197m3Bi | 2929.5(5) keV | 209(30) ns | IT | 197Bi | (31/2−) | ||||||||||||||
198Bi | 83 | 115 | 197.979201(30) | 10.3(3) min | β+ | 198Pb | 3+ | ||||||||||||
198m1Bi | 290(40) keV | 11.6(3) min | β+ | 198Pb | 7+ | ||||||||||||||
198m2Bi | 540(40) keV | 7.7(5) s | IT | 198Bi | 10− | ||||||||||||||
199Bi | 83 | 116 | 198.977673(11) | 27(1) min | β+ | 199Pb | 9/2− | ||||||||||||
199m1Bi | 667(3) keV | 24.70(15) min | β+ (>98%) | 199Pb | (1/2+) | ||||||||||||||
IT (<2%) | 199Bi | ||||||||||||||||||
α (0.01%) | 195Tl | ||||||||||||||||||
199m2Bi | 1962(23) keV | 0.10(3) μs | IT | 199Bi | 25/2+# | ||||||||||||||
199m3Bi | 2548(23) keV | 168(13) ns | IT | 199Bi | 29/2−# | ||||||||||||||
200Bi | 83 | 117 | 199.978131(24) | 36.4(5) min | β+ | 200Pb | 7+ | ||||||||||||
200m1Bi [n 9] | 100(70)# keV | 31(2) min | β+ (?%) | 200Pb | (2+) | ||||||||||||||
IT (?%) | 200Bi | ||||||||||||||||||
200m2Bi | 428.20(10) keV | 400(50) ms | IT | 200Bi | (10−) | ||||||||||||||
201Bi | 83 | 118 | 200.976995(13) | 103(3) min | β+ | 201Pb | 9/2− | ||||||||||||
201m1Bi | 846.35(18) keV | 57.5(21) min | β+ | 201Pb | 1/2+ | ||||||||||||||
α (?%) | 197Tl | ||||||||||||||||||
201m2Bi | 1973(23) keV | 118(28) ns | IT | 201Bi | 25/2+# | ||||||||||||||
201m3Bi | 2012(23) keV | 105(75) ns | IT | 201Bi | 27/2+# | ||||||||||||||
201m4Bi | 2781(23) keV | 124(4) ns | IT | 201Bi | 29/2−# | ||||||||||||||
202Bi | 83 | 119 | 201.977723(15) | 1.72(5) h | β+ | 202Pb | 5+ | ||||||||||||
α (<10−5%) | 198Tl | ||||||||||||||||||
202m1Bi | 625(12) keV | 3.04(6) μs | IT | 202Bi | 10−# | ||||||||||||||
202m2Bi | 2617(12) keV | 310(50) ns | IT | 202Bi | (17+) | ||||||||||||||
203Bi | 83 | 120 | 202.976892(14) | 11.76(5) h | β+ | 203Pb | 9/2− | ||||||||||||
203m1Bi | 1098.21(9) keV | 305(5) ms | IT | 203Bi | 1/2+ | ||||||||||||||
203m2Bi | 2041.5(6) keV | 194(30) ns | IT | 203Bi | 25/2+ | ||||||||||||||
204Bi | 83 | 121 | 203.977836(10) | 11.22(10) h | β+ | 204Pb | 6+ | ||||||||||||
204m1Bi | 805.5(3) keV | 13.0(1) ms | IT | 204Bi | 10− | ||||||||||||||
204m2Bi | 2833.4(11) keV | 1.07(3) ms | IT | 204Bi | 17+ | ||||||||||||||
205Bi | 83 | 122 | 204.977385(5) | 14.91(7) d | β+ | 205Pb | 9/2− | ||||||||||||
205m1Bi | 1497.17(9) keV | 7.9(7) μs | IT | 205Bi | 1/2+ | ||||||||||||||
205m2Bi | 2064.7(4) keV | 100(6) ns | IT | 205Bi | 21/2+ | ||||||||||||||
205m3Bi | 2139.0(7) keV | 220(25) ns | IT | 205Bi | 25/2+ | ||||||||||||||
206Bi | 83 | 123 | 205.978499(8) | 6.243(3) d | β+ | 206Pb | 6+ | ||||||||||||
206m1Bi | 59.897(17) keV | 7.7(2) μs | IT | 206Bi | 4+ | ||||||||||||||
206m2Bi | 1044.8(7) keV | 890(10) μs | IT | 206Bi | 10− | ||||||||||||||
206m3Bi | 9233.3(8) keV | 155(15) ns | IT | 206Bi | (28−) | ||||||||||||||
206m4Bi | 10170.5(8) keV | >2 μs | IT | 206Bi | (31+) | ||||||||||||||
207Bi | 83 | 124 | 206.9784706(26) | 31.22(17) y | β+ | 207Pb | 9/2− | ||||||||||||
207mBi | 2101.61(16) keV | 182(6) μs | IT | 207Bi | 21/2+ | ||||||||||||||
208Bi | 83 | 125 | 207.9797421(25) | 3.68(4)×105 y | β+ | 208Pb | 5+ | ||||||||||||
208mBi | 1571.1(4) keV | 2.58(4) ms | IT | 208Bi | 10− | ||||||||||||||
209Bi [n 10] [n 11] | 83 | 126 | 208.9803986(15) | 2.01(8)×1019 y [n 12] | α | 205Tl | 9/2− | 1.0000 | |||||||||||
210Bi | Radium E | 83 | 127 | 209.9841202(15) | 5.012(5) d | β− | 210Po | 1− | Trace [n 13] | ||||||||||
α (1.32×10−4%) | 206Tl | ||||||||||||||||||
210mBi | 271.31(11) keV | 3.04(6)×106 y | α | 206Tl | 9− | ||||||||||||||
211Bi | Actinium C | 83 | 128 | 210.987269(6) | 2.14(2) min | α (99.72%) | 207Tl | 9/2− | Trace [n 14] | ||||||||||
β− (0.276%) | 211Po | ||||||||||||||||||
211mBi | 1257(10) keV | 1.4(3) μs | IT | 211Bi | (25/2−) | ||||||||||||||
212Bi | Thorium C | 83 | 129 | 211.991285(2) | 60.55(6) min | β− (64.05%) | 212Po | 1− | Trace [n 15] | ||||||||||
α (35.94%) | 208Tl | ||||||||||||||||||
β−, α (0.014%) | 208Pb | ||||||||||||||||||
212m1Bi | 250(30) keV | 25.0(2) min | α (67%) | 208Tl | (8−, 9−) | ||||||||||||||
β−, α (30%) | 208Pb | ||||||||||||||||||
β− (3%) | 212Po | ||||||||||||||||||
212m2Bi | 1479(30) keV | 7.0(3) min | β− | 212Po | (18−) | ||||||||||||||
213Bi [n 16] [n 17] | 83 | 130 | 212.994384(5) | 45.60(4) min | β− (97.91%) | 213Po | 9/2− | Trace [n 18] | |||||||||||
α (2.09%) | 209Tl | ||||||||||||||||||
213mBi | 1353(21) keV | >168 s | 25/2−# | ||||||||||||||||
214Bi | Radium C | 83 | 131 | 213.998711(12) | 19.9(4) min | β− (99.98%) | 214Po | 1− | Trace [n 13] | ||||||||||
α (0.021%) | 210Tl | ||||||||||||||||||
β−, α (0.003%) | 210Pb | ||||||||||||||||||
214mBi | 539(30) keV | >93 s | 8−# | ||||||||||||||||
215Bi | 83 | 132 | 215.001749(6) | 7.62(13) min | β− | 215Po | (9/2−) | Trace [n 14] | |||||||||||
215mBi | 1367(20)# keV | 36.9(6) s | IT (76.9%) | 215Bi | (25/2−) | ||||||||||||||
β− (23.1%) | 215Po | ||||||||||||||||||
216Bi | 83 | 133 | 216.006306(12) | 2.21(4) min | β− | 216Po | (6−, 7−) | ||||||||||||
216mBi [n 9] | 24(19) keV | 6.6(21) min | β− | 216Po | 3−# | ||||||||||||||
217Bi | 83 | 134 | 217.009372(19) | 98.5(13) s | β− | 217Po | 9/2−# | ||||||||||||
217mBi | 1491(20) keV | 3.0(2) μs | IT | 217Bi | 25/2−# | ||||||||||||||
218Bi | 83 | 135 | 218.014188(29) | 33(1) s | β− | 218Po | 8−# | ||||||||||||
219Bi | 83 | 136 | 219.01752(22)# | 8.7(29) s | β− | 219Po | 9/2−# | ||||||||||||
220Bi | 83 | 137 | 220.02250(32)# | 9.5(57) s | β− | 220Po | 1−# | ||||||||||||
221Bi | 83 | 138 | 221.02598(32)# | 2# s [>300 ns] | 9/2−# | ||||||||||||||
222Bi | 83 | 139 | 222.03108(32)# | 3# s [>300 ns] | 1−# | ||||||||||||||
223Bi | 83 | 140 | 223.03461(43)# | 1# s [>300 ns] | 9/2−# | ||||||||||||||
224Bi | 83 | 141 | 224.03980(43)# | 1# s [>300 ns] | 1−# | ||||||||||||||
This table header & footer: |
EC: | Electron capture |
IT: | Isomeric transition |
p: | Proton emission |
Bismuth-213 (213Bi) has a half-life of 45 minutes and decays via alpha emission. Commercially, bismuth-213 can be produced by bombarding radium with bremsstrahlung photons from a linear particle accelerator, which populates its progenitor actinium-225. In 1997, an antibody conjugate with 213Bi was used to treat patients with leukemia. This isotope has also been tried in targeted alpha therapy (TAT) program to treat a variety of cancers. [7] Bismuth-213 is also found in the decay chain of uranium-233, which is the fuel bred by thorium reactors.
Protactinium (91Pa) has no stable isotopes. The four naturally occurring isotopes allow a standard atomic weight to be given.
Lead (82Pb) has four observationally stable isotopes: 204Pb, 206Pb, 207Pb, 208Pb. Lead-204 is entirely a primordial nuclide and is not a radiogenic nuclide. The three isotopes lead-206, lead-207, and lead-208 represent the ends of three decay chains: the uranium series, the actinium series, and the thorium series, respectively; a fourth decay chain, the neptunium series, terminates with the thallium isotope 205Tl. The three series terminating in lead represent the decay chain products of long-lived primordial 238U, 235U, and 232Th. Each isotope also occurs, to some extent, as primordial isotopes that were made in supernovae, rather than radiogenically as daughter products. The fixed ratio of lead-204 to the primordial amounts of the other lead isotopes may be used as the baseline to estimate the extra amounts of radiogenic lead present in rocks as a result of decay from uranium and thorium.
Thallium (81Tl) has 41 isotopes with atomic masses that range from 176 to 216. 203Tl and 205Tl are the only stable isotopes and 204Tl is the most stable radioisotope with a half-life of 3.78 years. 207Tl, with a half-life of 4.77 minutes, has the longest half-life of naturally occurring Tl radioisotopes. All isotopes of thallium are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed.
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.
Gold (79Au) has one stable isotope, 197Au, and 40 radioisotopes, with 195Au being the most stable with a half-life of 186 days. Gold is currently considered the heaviest monoisotopic element. Bismuth formerly held that distinction until alpha-decay of the 209Bi isotope was observed. All isotopes of gold are either radioactive or, in the case of 197Au, observationally stable, meaning that 197Au is predicted to be radioactive but no actual decay has been observed.
Naturally occurring platinum (78Pt) consists of five stable isotopes (192Pt, 194Pt, 195Pt, 196Pt, 198Pt) and one very long-lived (half-life 4.83×1011 years) radioisotope (190Pt). There are also 34 known synthetic radioisotopes, the longest-lived of which is 193Pt with a half-life of 50 years. All other isotopes have half-lives under a year, most under a day. All isotopes of platinum are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed. Platinum-195 is the most abundant isotope.
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.
Natural tantalum (73Ta) consists of two stable isotopes: 181Ta (99.988%) and 180m
Ta
(0.012%).
Natural hafnium (72Hf) consists of five observationally stable isotopes (176Hf, 177Hf, 178Hf, 179Hf, and 180Hf) and one very long-lived radioisotope, 174Hf, with a half-life of 7.0×1016 years. In addition, there are 34 known synthetic radioisotopes, the most stable of which is 182Hf with a half-life of 8.9×106 years. This extinct radionuclide is used in hafnium–tungsten dating to study the chronology of planetary differentiation.
Naturally occurring erbium (68Er) is composed of six stable isotopes, with 166Er being the most abundant. Thirty-nine radioisotopes have been characterized with between 74 and 112 neutrons, or 142 to 180 nucleons, with the most stable being 169Er with a half-life of 9.4 days, 172Er with a half-life of 49.3 hours, 160Er with a half-life of 28.58 hours, 165Er with a half-life of 10.36 hours, and 171Er with a half-life of 7.516 hours. All of the remaining radioactive isotopes have half-lives that are less than 3.5 hours, and the majority of these have half-lives that are less than 4 minutes. This element also has numerous meta states, with the most stable being 167mEr.
Natural holmium (67Ho) contains one observationally stable isotope, 165Ho. The below table lists 36 isotopes spanning 140Ho through 175Ho as well as 33 nuclear isomers. Among the known synthetic radioactive isotopes; the most stable one is 163Ho, with a half-life of 4,570 years. All other radioisotopes have half-lives not greater than 1.117 days in their ground states, and most have half-lives under 3 hours.
Naturally occurring terbium (65Tb) is composed of one stable isotope, 159Tb. Thirty-seven radioisotopes have been characterized, with the most stable being 158Tb with a half-life of 180 years, 157Tb with a half-life of 71 years, and 160Tb with a half-life of 72.3 days. All of the remaining radioactive isotopes have half-lives that are less than 6.907 days, and the majority of these have half-lives that are less than 24 seconds. This element also has 27 meta states, with the most stable being 156m1Tb, 154m2Tb and 154m1Tb.
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 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 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).
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.
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 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 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.