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Standard atomic weight Ar°(Dy) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Naturally occurring dysprosium (66Dy) is composed of 7 stable isotopes, 156Dy, 158Dy, 160Dy, 161Dy, 162Dy, 163Dy and 164Dy, with 164Dy being the most abundant (28.18% natural abundance). Twenty-nine radioisotopes have been characterized, with the most stable being 154Dy with a half-life of 1.4 million years, 159Dy with a half-life of 144.4 days, and 166Dy with a half-life of 81.6 hours. All of the remaining radioactive isotopes have half-lives that are less than 10 hours, and the majority of these have half-lives that are less than 30 seconds. This element also has 12 meta states, with the most stable being 165mDy (half-life 1.257 minutes), 147mDy (half-life 55.7 seconds) and 145mDy (half-life 13.6 seconds).
The primary decay mode before the most abundant stable isotope, 164Dy, is electron capture, and the primary mode after is beta decay. The primary decay products before 164Dy are terbium isotopes, and the primary products after are holmium isotopes. Dysprosium is the heaviest element to have isotopes that are predicted to be stable rather than observationally stable isotopes that are predicted to be radioactive.
Nuclide [n 1] | Z | N | Isotopic mass (Da) [5] [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 4] | Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy | Normal proportion [1] | Range of variation | |||||||||||||||||
139Dy | 66 | 73 | 138.95953(54)# | 600(200) ms | β+ (~89%) | 139Tb | (7/2+) | ||||||||||||
β+, p (~11%) | 138Gd | ||||||||||||||||||
140Dy | 66 | 74 | 139.95402(43)# | 700# ms | β+? | 140Tb | 0+ | ||||||||||||
β+, p? | 139Gd | ||||||||||||||||||
140mDy | 2166.1(5) keV | 7.0(5) μs | IT | 140Dy | 8− | ||||||||||||||
141Dy | 66 | 75 | 140.95128(32)# | 0.90(14) s | β+ | 141Tb | (9/2−) | ||||||||||||
β+, p? | 140Gd | ||||||||||||||||||
142Dy | 66 | 76 | 141.94619(78)# | 2.3(3) s | β+ (90%) | 142Tb | 0+ | ||||||||||||
EC (10%) | |||||||||||||||||||
β+, p (0.06%) | 141Gd | ||||||||||||||||||
143Dy | 66 | 77 | 142.943994(14) | 5.6(10) s | β+ | 143Tb | (1/2+) | ||||||||||||
β+, p? | 142Gd | ||||||||||||||||||
143m1Dy | 310.7(6) keV | 3.0(3) s | β+ | 143Tb | (11/2−) | ||||||||||||||
β+, p? | 142Gd | ||||||||||||||||||
143m2Dy | 406.3(8) keV | 1.2(3) μs | IT | 143Dy | (7/2−) | ||||||||||||||
144Dy | 66 | 78 | 143.9392695(77) | 9.1(4) s | β+ | 144Tb | 0+ | ||||||||||||
β+, p? | 143Gd | ||||||||||||||||||
145Dy | 66 | 79 | 144.9374740(70) | 9.5(10) s | β+ | 145Tb | (1/2+) | ||||||||||||
β+, p? | 144Gd | ||||||||||||||||||
145mDy | 118.2(2) keV | 14.1(7) s | β+ | 145Tb | (11/2−) | ||||||||||||||
β+, p (~50%) | 144Gd | ||||||||||||||||||
146Dy | 66 | 80 | 145.9328445(72) | 33.2(7) s | β+ | 146Tb | 0+ | ||||||||||||
146mDy | 2934.5(4) keV | 150(20) ms | IT | 146Dy | 10+ | ||||||||||||||
147Dy | 66 | 81 | 146.9310827(95) | 67(7) s | β+ (99.95%) | 147Tb | (1/2+) | ||||||||||||
β+, p (0.05%) | 146Tb | ||||||||||||||||||
147m1Dy | 750.5(4) keV | 55.2(5) s | β+ (68.9%) | 147Tb | (11/2−) | ||||||||||||||
IT (31.1%) | 147Dy | ||||||||||||||||||
147m2Dy | 3407.2(8) keV | 0.40(1) μs | IT | 147Dy | (27/2−) | ||||||||||||||
148Dy | 66 | 82 | 147.9271499(94) | 3.3(2) min | β+ | 148Tb | 0+ | ||||||||||||
148mDy | 2919.1(10) keV | 471(20) ns | IT | 148Dy | 10+ | ||||||||||||||
149Dy | 66 | 83 | 148.9273275(99) | 4.20(14) min | β+ | 149Tb | 7/2− | ||||||||||||
149mDy | 2661.1(4) keV | 490(15) ms | IT (99.3%) | 149Dy | 27/2− | ||||||||||||||
β+ (0.7%) | 149Tb | ||||||||||||||||||
150Dy | 66 | 84 | 149.9255931(46) | 7.17(5) min | β+ (66.4%) | 150Tb | 0+ | ||||||||||||
α (33.6%) | 146Gd | ||||||||||||||||||
151Dy | 66 | 85 | 150.9261913(35) | 17.9(3) min | β+ (94.4%) | 151Tb | 7/2− | ||||||||||||
α (5.6%) | 147Gd | ||||||||||||||||||
152Dy | 66 | 86 | 151.9247253(49) | 2.38(2) h | EC (99.90%) | 152Tb | 0+ | ||||||||||||
α (0.100%) | 148Gd | ||||||||||||||||||
153Dy | 66 | 87 | 152.9257717(43) | 6.4(1) h | β+ (99.99%) | 153Tb | 7/2− | ||||||||||||
α (0.0094%) | 149Gd | ||||||||||||||||||
154Dy | 66 | 88 | 153.9244289(80) | 1.40(8)×106 y [6] | α [n 8] | 150Gd | 0+ | ||||||||||||
155Dy | 66 | 89 | 154.925758(10) | 9.9(2) h | β+ | 155Tb | 3/2− | ||||||||||||
155mDy | 234.33(3) keV | 6(1) μs | IT | 155Dy | 11/2− | ||||||||||||||
156Dy | 66 | 90 | 155.9242836(11) | Observationally Stable [n 9] | 0+ | 5.6(3)×10−4 | |||||||||||||
157Dy | 66 | 91 | 156.9254696(55) | 8.14(4) h | β+ | 157Tb | 3/2− | ||||||||||||
157m1Dy | 161.99(3) keV | 1.3(2) μs | IT | 157Dy | 9/2+ | ||||||||||||||
157m2Dy | 199.38(7) keV | 21.6(16) ms | IT | 157Dy | 11/2− | ||||||||||||||
158Dy | 66 | 92 | 157.9244148(25) | Observationally Stable [n 10] | 0+ | 9.5(3)×10−4 | |||||||||||||
159Dy | 66 | 93 | 158.9257459(15) | 144.4(2) d | EC | 159Tb | 3/2− | ||||||||||||
159mDy | 352.77(14) keV | 122(3) μs | IT | 159Dy | 11/2− | ||||||||||||||
160Dy | 66 | 94 | 159.92520358(75) | Observationally Stable [n 11] | 0+ | 0.02329(18) | |||||||||||||
161Dy | 66 | 95 | 160.92693943(75) | Observationally Stable [n 12] | 5/2+ | 0.18889(42) | |||||||||||||
161mDy | 485.56(16) keV | 0.76(17) μs | IT | 161Dy | 11/2− | ||||||||||||||
162Dy | 66 | 96 | 161.92680451(75) | Observationally Stable [n 13] | 0+ | 0.25475(36) | |||||||||||||
162mDy | 2188.1(3) keV | 8.3(3) μs | IT | 162Dy | 8+ | ||||||||||||||
163Dy | 66 | 97 | 162.92873722(74) | Stable [n 14] | 5/2− | 0.24896(42) | |||||||||||||
164Dy [n 15] | 66 | 98 | 163.92918082(75) | Stable | 0+ | 0.28260(54) | |||||||||||||
165Dy | 66 | 99 | 164.93170940(75) | 2.332(4) h | β− | 165Ho | 7/2+ | ||||||||||||
165mDy | 108.1552(13) keV | 1.257(6) min | IT (97.76%) | 165Dy | 1/2− | ||||||||||||||
β− (2.24%) | 165Ho | ||||||||||||||||||
166Dy | 66 | 100 | 165.93281281(86) | 81.6(1) h | β− | 166Ho | 0+ | ||||||||||||
167Dy | 66 | 101 | 166.9356824(43) | 6.20(8) min | β− | 167Ho | (1/2−) | ||||||||||||
168Dy | 66 | 102 | 167.93713(15) | 8.7(3) min | β− | 168Ho | 0+ | ||||||||||||
168mDy | 1378.2(6) keV | 0.57(7) μs | IT | 168Dy | (4−) | ||||||||||||||
169Dy | 66 | 103 | 168.94032(32) | 39(8) s | β− | 169Ho | (5/2)− | ||||||||||||
169mDy | 166.1(5) keV | 1.26(17) μs | IT | 169Dy | (1/2−) | ||||||||||||||
170Dy | 66 | 104 | 169.94234(22)# | 54.9(80) s | β− | 170Ho | 0+ | ||||||||||||
170mDy | 1643.8(3) keV | 0.99(4) μs | IT | 170Dy | (6+) | ||||||||||||||
171Dy | 66 | 105 | 170.94631(22)# | 4.07(40) s | β− | 171Ho | 7/2−# | ||||||||||||
172Dy | 66 | 106 | 171.94873(32)# | 3.4(2) s | β− | 172Ho | 0+ | ||||||||||||
172mDy | 1278(1) keV | 710(50) ms | IT (81%) | 172Dy | (8−) | ||||||||||||||
β− (19%) | 172Ho | ||||||||||||||||||
173Dy | 66 | 107 | 172.95304(43)# | 1.43(20) s | β− | 173Ho | 9/2+# | ||||||||||||
β−, n? | 172Ho | ||||||||||||||||||
174Dy | 66 | 108 | 173.95585(54)# | 1# s [>300 ns] | β−? | 174Ho | 0+ | ||||||||||||
β−, n? | 173Ho | ||||||||||||||||||
175Dy | 66 | 109 | 174.96057(54)# | 390# ms [>550 ns] | β−? | 175Ho | 1/2-# | ||||||||||||
β−, n? | 174Ho | ||||||||||||||||||
176Dy | 66 | 110 | 175.96392(54)# | 440# ms [>550 ns] | β−? | 176Ho | 0+ | ||||||||||||
β−, n? | 175Ho | ||||||||||||||||||
This table header & footer: |
EC: | Electron capture |
IT: | Isomeric transition |
p: | Proton emission |
The radioactive isotope 165Dy, with a half-life of 2.334 hours, has radiopharmaceutical uses in radiation synovectomy of the knee. It had been previously performed with colloidal-sized particles containing longer-lived isotopes such as 198Au and 90Y. The major problem with the usage of those isotopes was radiation leakage out of the knee. 165Dy, with its shorter half-life and thus shorter period of potential radiation leakage, is more suitable for the procedure. [8]
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.
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.
Osmium (76Os) has seven naturally occurring isotopes, five of which are stable: 187Os, 188Os, 189Os, 190Os, and (most abundant) 192Os. The other natural isotopes, 184Os, and 186Os, have extremely long half-life (1.12×1013 years and 2×1015 years, respectively) and for practical purposes can be considered to be stable as well. 187Os is the daughter of 187Re (half-life 4.12×1010 years) and is most often measured in an 187Os/188Os ratio. This ratio, as well as the 187Re/188Os ratio, have been used extensively in dating terrestrial as well as meteoric rocks. It has also been used to measure the intensity of continental weathering over geologic time and to fix minimum ages for stabilization of the mantle roots of continental cratons. However, the most notable application of Os in dating has been in conjunction with iridium, to analyze the layer of shocked quartz along the Cretaceous–Paleogene boundary that marks the extinction of the dinosaurs 66 million years ago.
Naturally occurring tungsten (74W) consists of five isotopes. Four are considered stable (182W, 183W, 184W, and 186W) and one is slightly radioactive, 180W, with an extremely long half-life of 1.8 ± 0.2 exayears (1018 years). On average, two alpha decays of 180W occur per gram of natural tungsten per year, so for most practical purposes, 180W can be considered stable. Theoretically, all five can decay into isotopes of element 72 (hafnium) by alpha emission, but only 180W has been observed to do so. The other naturally occurring isotopes have not been observed to decay (they are observationally stable), and lower bounds for their half-lives have been established:
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 ytterbium (70Yb) is composed of seven stable isotopes: 168Yb, 170Yb–174Yb, and 176Yb, with 174Yb being the most abundant. 30 radioisotopes have been characterized, with the most stable being 169Yb with a half-life of 32.014 days, 175Yb with a half-life of 4.185 days, and 166Yb with a half-life of 56.7 hours. All of the remaining radioactive isotopes have half-lives that are less than 2 hours, and the majority of these have half-lives that are less than 20 minutes. This element also has 18 meta states, with the most stable being 169mYb.
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 five stable isotopes, 142Nd, 143Nd, 145Nd, 146Nd and 148Nd, with 142Nd being the most abundant (27.2% natural abundance), and two long-lived radioisotopes, 144Nd and 150Nd. In all, 35 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 9.3×1018 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 15 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 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).
Antimony (51Sb) occurs in two stable isotopes, 121Sb and 123Sb. There are 37 artificial radioactive isotopes, the longest-lived of which are 125Sb, with a half-life of 2.75856 years; 124Sb, with half-life 60.2 days; and 126Sb, with half-life 12.35 days. All other isotopes have half-lives less than 4 days, most less than an hour. There are also many isomers, the longest-lived of which is 120m1Sb with half-life 5.76 days.
Natural palladium (46Pd) is composed of six stable isotopes, 102Pd, 104Pd, 105Pd, 106Pd, 108Pd, and 110Pd, although 102Pd and 110Pd are theoretically unstable. The most stable radioisotopes are 107Pd with a half-life of 6.5 million years, 103Pd with a half-life of 17 days, and 100Pd with a half-life of 3.63 days. Twenty-three other radioisotopes have been characterized with atomic weights ranging from 90.949 u (91Pd) to 128.96 u (129Pd). Most of these have half-lives that are less than 30 minutes except 101Pd, 109Pd, and 112Pd.
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.
The alkaline earth metal strontium (38Sr) has four stable, naturally occurring isotopes: 84Sr (0.56%), 86Sr (9.86%), 87Sr (7.0%) and 88Sr (82.58%). Its standard atomic weight is 87.62(1).
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.
Naturally occurring titanium (22Ti) is composed of five stable isotopes; 46Ti, 47Ti, 48Ti, 49Ti and 50Ti with 48Ti being the most abundant. Twenty-one radioisotopes have been characterized, with the most stable being 44Ti with a half-life of 60 years, 45Ti with a half-life of 184.8 minutes, 51Ti with a half-life of 5.76 minutes, and 52Ti with a half-life of 1.7 minutes. All of the remaining radioactive isotopes have half-lives that are less than 33 seconds, and the majority of these have half-lives that are less than half a second.