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Standard atomic weight Ar°(Nd) | ||||||||||||||||||||||||||||||||||||||||||||||
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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 11 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).
The primary decay modes for isotopes lighter than the most abundant stable isotope (also the only theoretically stable isotope), 142Nd, are electron capture and positron decay, and the primary mode for heavier radioisotopes is beta decay. The primary decay products for lighter radioisotopes are praseodymium isotopes and the primary products for heavier ones are promethium isotopes.
Neodymium is one of the more common fission products that results from the splitting of uranium-233, uranium-235, plutonium-239 and plutonium-241. The distribution of resulting neodymium isotopes is distinctly different than those found in crustal rock formation on Earth. One of the methods used to verify that the Oklo Fossil Reactors in Gabon had produced a natural nuclear fission reactor some two billion years before present was to compare the relative abundances of neodymium isotopes found at the reactor site with those found elsewhere on Earth. [4] [5] [6]
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 [n 5] | Normal proportion [1] | Range of variation | |||||||||||||||||
125Nd | 60 | 65 | 124.94840(43)# | 0.65(15) s | β+ | 125Pr | (5/2)(+#) | ||||||||||||
β+, p (?%) | 124Ce | ||||||||||||||||||
126Nd | 60 | 66 | 125.94269(32)# | 1# s [>200 ns] | 0+ | ||||||||||||||
127Nd | 60 | 67 | 126.93998(32)# | 1.8(4) s | β+ | 127Pr | 5/2+# | ||||||||||||
β+, p (?%) | 126Ce | ||||||||||||||||||
128Nd | 60 | 68 | 127.93502(22)# | 5# s | 0+ | ||||||||||||||
129Nd | 60 | 69 | 128.93304(22)# | 6.8(6) s | β+ | 129Pr | 7/2− [8] | ||||||||||||
β+, p (?%) | 128Ce | ||||||||||||||||||
129m1Nd | 17 keV [8] | 2.6(4) s | β+ | 129Pr | 1/2+ [8] | ||||||||||||||
β+, p (?%) | 128Ce | ||||||||||||||||||
129m2Nd [8] | 39 keV | 2.6(4) s | β+ | 129Pr | 3/2+ | ||||||||||||||
β+, p (?%) | 128Ce | ||||||||||||||||||
129m3Nd [8] | 108 keV | IT (?%) | 129m2Nd | 5/2+ | |||||||||||||||
IT (?%) | 129Nd | ||||||||||||||||||
129m4Nd [8] | 1893 keV | IT | 129Nd | (17/2+) | |||||||||||||||
129m5Nd [8] | 2109 keV | IT | 129Nd | (19/2+) | |||||||||||||||
129m6Nd [8] | 2284 keV | 0.48(4) μs | IT | 129Nd | (21/2+) | ||||||||||||||
130Nd | 60 | 70 | 129.928506(30) | 21(3) s | β+ | 130Pr | 0+ | ||||||||||||
131Nd | 60 | 71 | 130.927248(30) | 25.4(9) s | β+ | 131Pr | (5/2+) | ||||||||||||
β+, p (?%) | 130Ce | ||||||||||||||||||
132Nd | 60 | 72 | 131.923321(26) | 1.56(10) min | β+ | 132Pr | 0+ | ||||||||||||
133Nd | 60 | 73 | 132.922348(50) | 70(10) s | β+ | 133Pr | (7/2+) | ||||||||||||
133m1Nd | 127.97(12) keV | ~70 s | β+ (?%) | 133Pr | (1/2)+ | ||||||||||||||
IT (?%) | 133Nd | ||||||||||||||||||
133m2Nd | 176.10(10) keV | 301(18) ns | IT | 133Nd | (9/2–) | ||||||||||||||
134Nd | 60 | 74 | 133.918790(13) | 8.5(15) min | β+ | 134Pr | 0+ | ||||||||||||
134mNd | 2293.0(4) keV | 389(17) μs | IT | 134Nd | 8– | ||||||||||||||
135Nd | 60 | 75 | 134.918181(21) | 12.4(6) min | β+ | 135Pr | 9/2– | ||||||||||||
135mNd | 64.95(24) keV | 5.5(5) min | β+ | 135Pr | (1/2+) | ||||||||||||||
136Nd | 60 | 76 | 135.914976(13) | 50.65(33) min | β+ | 136Pr | 0+ | ||||||||||||
137Nd | 60 | 77 | 136.914563(13) | 38.5(15) min | β+ | 137Pr | 1/2+ | ||||||||||||
137mNd | 519.43(20) keV | 1.60(15) s | IT | 137Nd | 11/2– | ||||||||||||||
138Nd | 60 | 78 | 137.911951(12) | 5.04(9) h | β+ | 138Pr | 0+ | ||||||||||||
138mNd | 3174.5(4) keV | 370(5) ns | IT | 138Nd | 10+ | ||||||||||||||
139Nd | 60 | 79 | 138.911951(30) | 29.7(5) min | β+ | 139Pr | 3/2+ | ||||||||||||
139m1Nd | 231.16(5) keV | 5.50(20) h | β+ (87.0%) | 139Pr | 11/2– | ||||||||||||||
IT (13.0%) | 139Nd | ||||||||||||||||||
139m2Nd | 2616.9(6) keV | 276.8(18) ns | IT | 139Nd | 23/2 | ||||||||||||||
140Nd | 60 | 80 | 139.9095461(35) | 3.37(2) d | EC | 140Pr | 0+ | ||||||||||||
140m1Nd | 2221.65(9) keV | 600(50) μs | IT | 140Nd | 7– | ||||||||||||||
140m2Nd | 7435.1(4) keV | 1.22(6) μs | IT | 140Nd | 20+ | ||||||||||||||
141Nd | 60 | 81 | 140.9096167(34) | 2.49(3) h | EC (97.28%) | 141Pr | 3/2+ | ||||||||||||
β+ (2.72%) | 141Pr | ||||||||||||||||||
141mNd | 756.51(5) keV | 62.0(8) s | IT (99.97%) | 141Nd | 11/2– | ||||||||||||||
β+ (0.032%) | 141Pr | ||||||||||||||||||
142Nd | 60 | 82 | 141.9077288(13) | Stable | 0+ | 0.27153(40) | |||||||||||||
143Nd [n 9] | 60 | 83 | 142.9098198(13) | Observationally Stable [n 10] | 7/2− | 0.12173(26) | |||||||||||||
144Nd [n 9] [n 11] | 60 | 84 | 143.9100928(13) | 2.29(16)×1015 y | α | 140Ce | 0+ | 0.23798(19) | |||||||||||
145Nd [n 9] | 60 | 85 | 144.9125792(14) | Observationally Stable [n 12] | 7/2− | 0.08293(12) | |||||||||||||
146Nd [n 9] | 60 | 86 | 145.9131225(14) | Observationally Stable [n 13] | 0+ | 0.17189(32) | |||||||||||||
147Nd [n 9] | 60 | 87 | 146.9161060(14) | 10.98(1) d | β− | 147Pm | 5/2− | ||||||||||||
148Nd [n 9] | 60 | 88 | 147.9168990(22) | Observationally Stable [n 14] | 0+ | 0.05756(21) | |||||||||||||
149Nd [n 9] | 60 | 89 | 148.9201546(22) | 1.728(1) h | β− | 149Pm | 5/2− | ||||||||||||
150Nd [n 9] [n 11] | 60 | 90 | 149.9209013(12) | 9.3(7)×1018 y | β−β− | 150Sm | 0+ | 0.05638(28) | |||||||||||
151Nd | 60 | 91 | 150.9238394(12) | 12.44(7) min | β− | 151Pm | 3/2+ | ||||||||||||
152Nd | 60 | 92 | 151.924691(26) | 11.4(2) min | β− | 152Pm | 0+ | ||||||||||||
153Nd | 60 | 93 | 152.9277179(29) | 31.6(10) s | β− | 153Pm | (3/2)− | ||||||||||||
153mNd | 191.71(16) keV | 1.10(4) μs | IT | 153Nd | (5/2)+ | ||||||||||||||
154Nd | 60 | 94 | 153.9295974(11) | 25.9(2) s | β− | 154Pm | 0+ | ||||||||||||
154mNd | 1297.9(4) keV | 3.2(3) μs | IT | 154Nd | (4−) | ||||||||||||||
155Nd | 60 | 95 | 154.9331356(98) | 8.9(2) s | β− | 155Pm | (3/2−) | ||||||||||||
156Nd | 60 | 96 | 155.9353704(14) | 5.06(13) s | β− | 156Pm | 0+ | ||||||||||||
156mNd | 1431.3(4) keV | 365(145) ns | IT | 156Nd | 5− | ||||||||||||||
157Nd | 60 | 97 | 156.9393511(23) | 1.17(4) s [12] | β− | 157Pm | 5/2−# | ||||||||||||
158Nd | 60 | 98 | 157.9422056(14) | 810(30) ms | β− | 158Pm | 0+ | ||||||||||||
158mNd | 1648.1(14) keV | 339(20) ns | IT | 158Nd | (6−) | ||||||||||||||
159Nd | 60 | 99 | 158.946619(32) | 500(30) ms | β− | 159Pm | 7/2+# | ||||||||||||
160Nd | 60 | 100 | 159.949839(50) | 439(37) ms | β− | 160Pm | 0+ | ||||||||||||
160mNd | 1107.9(9) keV | 1.63(21) μs | IT | 160Nd | (4−) | ||||||||||||||
161Nd | 60 | 101 | 160.95466(43)# | 215(76) ms | β− | 161Pm | 1/2−# | ||||||||||||
162Nd | 60 | 102 | 161.95812(43)# | 310(200) ms | β− | 162Pm | 0+ | ||||||||||||
163Nd | 60 | 103 | 162.96341(54)# | 80# ms [>550 ns] | 5/2−# | ||||||||||||||
This table header & footer: |
EC: | Electron capture |
IT: | Isomeric transition |
p: | Proton emission |
Protactinium (91Pa) has no stable isotopes. The four naturally occurring isotopes allow a standard atomic weight to be given.
There are 39 known isotopes of radon (86Rn), from 193Rn to 231Rn; all are radioactive. The most stable isotope is 222Rn with a half-life of 3.8235 days, which decays into 218
Po
. Six isotopes of radon, 217, 218, 219, 220, 221, 222Rn, occur in trace quantities in nature as decay products of, respectively, 217At, 218At, 223Ra, 224Ra, 225Ra, and 226Ra. 217Rn and 221Rn are produced in rare branches in the decay chain of trace quantities of 237Np; 222Rn is an intermediate step in the decay chain of 238U; 219Rn is an intermediate step in the decay chain of 235U; and 220Rn occurs in the decay chain of 232Th.
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.
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.
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 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 3.8×1016 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 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 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.
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 europium (63Eu) is composed of two isotopes, 151Eu and 153Eu, with 153Eu being the most abundant (52.2% natural abundance). While 153Eu is observationally stable (theoretically can undergo alpha decay with half-life over 5.5×1017 years), 151Eu was found in 2007 to be unstable and undergo alpha decay. The half-life is measured to be (4.62 ± 0.95(stat.) ± 0.68(syst.)) × 1018 years which corresponds to 1 alpha decay per two minutes in every kilogram of natural europium. Besides the natural radioisotope 151Eu, 36 artificial radioisotopes have been characterized, with the most stable being 150Eu with a half-life of 36.9 years, 152Eu with a half-life of 13.516 years, 154Eu with a half-life of 8.593 years, and 155Eu with a half-life of 4.7612 years. The majority of the remaining radioactive isotopes, which range from 130Eu to 170Eu, have half-lives that are less than 12.2 seconds. This element also has 18 metastable isomers, with the most stable being 150mEu (t1/2 12.8 hours), 152m1Eu (t1/2 9.3116 hours) and 152m5Eu (t1/2 96 minutes).
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.
Promethium (61Pm) is an artificial element, except in trace quantities as a product of spontaneous fission of 238U and 235U and alpha decay of 151Eu, and thus a standard atomic weight cannot be given. Like all artificial elements, it has no stable isotopes. It was first synthesized in 1945.
Naturally occurring praseodymium (59Pr) is composed of one stable isotope, 141Pr. Thirty-eight radioisotopes have been characterized with the most stable being 143Pr, with a half-life of 13.57 days and 142Pr, with a half-life of 19.12 hours. All of the remaining radioactive isotopes have half-lives that are less than six hours and the majority of these have half-lives that are less than 33 seconds. This element also has 15 meta states with the most stable being 138mPr, 142mPr and 134mPr.
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 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).
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 zirconium (40Zr) is composed of four stable isotopes (of which one may in the future be found radioactive), and one very long-lived radioisotope (96Zr), a primordial nuclide that decays via double beta decay with an observed half-life of 2.0×1019 years; it can also undergo single beta decay, which is not yet observed, but the theoretically predicted value of t1/2 is 2.4×1020 years. The second most stable radioisotope is 93Zr, which has a half-life of 1.53 million years. Thirty other radioisotopes have been observed. All have half-lives less than a day except for 95Zr (64.02 days), 88Zr (83.4 days), and 89Zr (78.41 hours). The primary decay mode is electron capture for isotopes lighter than 92Zr, and the primary mode for heavier isotopes is beta decay.
Naturally occurring chromium (24Cr) is composed of four stable isotopes; 50Cr, 52Cr, 53Cr, and 54Cr with 52Cr being the most abundant (83.789% natural abundance). 50Cr is suspected of decaying by β+β+ to 50Ti with a half-life of (more than) 1.8×1017 years. Twenty-two radioisotopes, all of which are entirely synthetic, have been characterized, the most stable being 51Cr with a half-life of 27.7 days. All of the remaining radioactive isotopes have half-lives that are less than 24 hours and the majority of these have half-lives that are less than 1 minute. This element also has two meta states, 45mCr, the more stable one, and 59mCr, the least stable isotope or isomer.
Naturally occurring scandium (21Sc) is composed of one stable isotope, 45Sc. Twenty-seven radioisotopes have been characterized, with the most stable being 46Sc with a half-life of 83.8 days, 47Sc with a half-life of 3.35 days, and 48Sc with a half-life of 43.7 hours and 44Sc with a half-life of 3.97 hours. All the remaining isotopes have half-lives that are less than four hours, and the majority of these have half-lives that are less than two minutes, the least stable being proton unbound 39Sc with a half-life shorter than 300 nanoseconds. This element also has 13 meta states with the most stable being 44m2Sc.