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Standard atomic weight Ar°(Ag) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Naturally occurring silver (47Ag) is composed of the two stable isotopes 107Ag and 109Ag in almost equal proportions, with 107Ag being slightly more abundant (51.839% natural abundance). Notably, silver is the only element with all stable istopes having nuclear spins of 1/2. Thus both 107Ag and 109Ag nuclei produce narrow lines in nuclear magnetic resonance spectra. [4]
40 radioisotopes have been characterized with the most stable being 105Ag with a half-life of 41.29 days, 111Ag with a half-life of 7.43 days, and 112Ag with a half-life of 3.13 hours.
All of the remaining radioactive isotopes have half-lives that are less than an hour, and the majority of these have half-lives that are less than 3 minutes. This element has numerous meta states, with the most stable being 108mAg (half-life 439 years), 110mAg (half-life 249.86 days) and 106mAg (half-life 8.28 days).
Isotopes of silver range in atomic weight from 92Ag to 132Ag. The primary decay mode before the most abundant stable isotope, 107Ag, is electron capture and the primary mode after is beta decay. The primary decay products before 107Ag are palladium (element 46) isotopes and the primary products after are cadmium (element 48) isotopes.
The palladium isotope 107Pd decays by beta emission to 107Ag with a half-life of 6.5 million years. Iron meteorites are the only objects with a high enough palladium/silver ratio to yield measurable variations in 107Ag abundance. Radiogenic 107Ag was first discovered in the Santa Clara meteorite in 1978.
The discoverers suggest that the coalescence and differentiation of iron-cored small planets may have occurred 10 million years after a nucleosynthetic event. 107Pd versus 107Ag correlations observed in bodies, which have clearly been melted since the accretion of the Solar System, must reflect the presence of live short-lived nuclides in the early Solar System.
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] [n 7] | Spin and parity [1] [n 8] [n 4] | Natural abundance (mole fraction) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Excitation energy [n 4] | Normal proportion [1] | Range of variation | |||||||||||||||||
92Ag | 47 | 45 | 91.95971(43)# | 1# ms [>400 ns] | β+? | 92Pd | |||||||||||||
p? | 91Pd | ||||||||||||||||||
93Ag | 47 | 46 | 92.95019(43)# | 228(16) ns | β+? | 93Pd | 9/2+# | ||||||||||||
p? | 92Pd | ||||||||||||||||||
β+, p? | 92Rh | ||||||||||||||||||
94Ag | 47 | 47 | 93.94374(43)# | 27(2) ms | β+ (>99.8%) | 94Pd | 0+# | ||||||||||||
β+, p (<0.2%) | 93Rh | ||||||||||||||||||
94m1Ag | 1350(400)# keV | 470(10) ms | β+ (83%) | 94Pd | (7+) | ||||||||||||||
β+, p (17%) | 93Rh | ||||||||||||||||||
94m2Ag | 6500(550)# keV | 400(40) ms | β+ (~68.4%) | 94Pd | (21+) | ||||||||||||||
β+, p (~27%) | 93Rh | ||||||||||||||||||
p (4.1%) | 93Pd | ||||||||||||||||||
2p (0.5%) | 92Rh | ||||||||||||||||||
95Ag | 47 | 48 | 94.93569(43)# | 1.78(6) s | β+ (97.7%) | 95Pd | (9/2+) | ||||||||||||
β+, p (2.3%) | 94Rh | ||||||||||||||||||
95m1Ag | 344.2(3) keV | <0.5 s | IT | 95Ag | (1/2−) | ||||||||||||||
95m2Ag | 2531.3(15) keV | <16 ms | IT | 95Ag | (23/2+) | ||||||||||||||
95m3Ag | 4860.0(15) keV | <40 ms | IT | 95Ag | (37/2+) | ||||||||||||||
96Ag | 47 | 49 | 95.93074(10) | 4.45(3) s | β+ (95.8%) | 96Pd | (8)+ | ||||||||||||
β+, p (4.2%) | 95Rh | ||||||||||||||||||
96m1Ag [n 9] | 0(50)# keV | 6.9(5) s | β+ (85.1%) | 96Pd | (2+) | ||||||||||||||
β+, p (14.9%) | 95Rh | ||||||||||||||||||
96m2Ag | 2461.4(3) keV | 103.2(45) μs | IT | 96Ag | (13−) | ||||||||||||||
96m3Ag | 2686.7(4) keV | 1.561(16) μs | IT | 96Ag | (15+) | ||||||||||||||
96m4Ag | 6951.8(14) keV | 132(17) ns | IT | 96Ag | (19+) | ||||||||||||||
97Ag | 47 | 50 | 96.923881(13) | 25.5(3) s | β+ | 97Pd | (9/2)+ | ||||||||||||
97mAg | 620(40) keV | 100# ms | IT? | 97Ag | 1/2−# | ||||||||||||||
98Ag | 47 | 51 | 97.92156(4) | 47.5(3) s | β+ | 98Pd | (6)+ | ||||||||||||
β+, p (.0012%) | 97Rh | ||||||||||||||||||
98mAg | 107.28(10) keV | 161(7) ns | IT | 98Ag | (4+) | ||||||||||||||
99Ag | 47 | 52 | 98.917646(7) | 2.07(5) min | β+ | 99Pd | (9/2)+ | ||||||||||||
99mAg | 506.2(4) keV | 10.5(5) s | IT | 99Ag | (1/2−) | ||||||||||||||
100Ag | 47 | 53 | 99.916115(5) | 2.01(9) min | β+ | 100Pd | (5)+ | ||||||||||||
100mAg | 15.52(16) keV | 2.24(13) min | IT? | 100Ag | (2)+ | ||||||||||||||
β+? | 100Pd | ||||||||||||||||||
101Ag | 47 | 54 | 100.912684(5) | 11.1(3) min | β+ | 101Pd | 9/2+ | ||||||||||||
101mAg | 274.1(3) keV | 3.10(10) s | IT | 101Ag | (1/2)− | ||||||||||||||
102Ag | 47 | 55 | 101.911705(9) | 12.9(3) min | β+ | 102Pd | 5+ | ||||||||||||
102mAg | 9.40(7) keV | 7.7(5) min | β+ (51%) | 102Pd | 2+ | ||||||||||||||
IT (49%) | 102Ag | ||||||||||||||||||
103Ag | 47 | 56 | 102.908961(4) | 65.7(7) min | β+ | 103Pd | 7/2+ | ||||||||||||
103mAg | 134.45(4) keV | 5.7(3) s | IT | 103Ag | 1/2− | ||||||||||||||
104Ag | 47 | 57 | 103.908624(5) | 69.2(10) min | β+ | 104Pd | 5+ | ||||||||||||
104mAg | 6.90(22) keV | 33.5(20) min | β+ (>99.93%) | 104Pd | 2+ | ||||||||||||||
IT (<0.07%) | 104Ag | ||||||||||||||||||
105Ag | 47 | 58 | 104.906526(5) | 41.29(7) d | β+ | 105Pd | 1/2− | ||||||||||||
105mAg | 25.468(16) keV | 7.23(16) min | IT (99.66%) | 105Ag | 7/2+ | ||||||||||||||
β+ (.34%) | 105Pd | ||||||||||||||||||
106Ag | 47 | 59 | 105.906663(3) | 23.96(4) min | β+ | 106Pd | 1+ | ||||||||||||
β−? | 106Cd | ||||||||||||||||||
106mAg | 89.66(7) keV | 8.28(2) d | β+ | 106Pd | 6+ | ||||||||||||||
IT? | 106Ag | ||||||||||||||||||
107Ag [n 10] | 47 | 60 | 106.9050915(26) | Stable | 1/2− | 0.51839(8) | |||||||||||||
107mAg | 93.125(19) keV | 44.3(2) s | IT | 107Ag | 7/2+ | ||||||||||||||
108Ag [6] | 47 | 61 | 107.9059502(26) | 2.382(11) min | β− (97.15%) | 108Cd | 1+ | ||||||||||||
EC (2.57%) | 108Pd | ||||||||||||||||||
β+ (0.283%) | 108Pd | ||||||||||||||||||
108mAg [6] | 109.466(7) keV | 439(9) y | EC (91.3%) | 108Pd | 6+ | ||||||||||||||
IT (8.96%) | 108Ag | ||||||||||||||||||
109Ag [n 11] | 47 | 62 | 108.9047558(14) | Stable | 1/2− | 0.48161(8) | |||||||||||||
109mAg | 88.0337(10) keV | 39.79(21) s | IT | 109Ag | 7/2+ | ||||||||||||||
110Ag | 47 | 63 | 109.9061107(14) | 24.56(11) s | β− (99.70%) | 110Cd | 1+ | ||||||||||||
EC (0.30%) | 110Pd | ||||||||||||||||||
110m1Ag | 1.112(16) keV | 660(40) ns | IT | 110Ag | 2− | ||||||||||||||
110m2Ag | 117.59(5) keV | 249.863(24) d | β− (98.67%) | 110Cd | 6+ | ||||||||||||||
IT (1.33%) | 110Ag | ||||||||||||||||||
111Ag [n 11] | 47 | 64 | 110.9052968(16) | 7.433(10) d | β− | 111Cd | 1/2− | ||||||||||||
111mAg | 59.82(4) keV | 64.8(8) s | IT (99.3%) | 111Ag | 7/2+ | ||||||||||||||
β− (0.7%) | 111Cd | ||||||||||||||||||
112Ag | 47 | 65 | 111.9070485(26) | 3.130(8) h | β− | 112Cd | 2(−) | ||||||||||||
113Ag | 47 | 66 | 112.906573(18) | 5.37(5) h | β− | 113mCd | 1/2− | ||||||||||||
113mAg | 43.50(10) keV | 68.7(16) s | IT (64%) | 113Ag | 7/2+ | ||||||||||||||
β− (36%) | 113Cd | ||||||||||||||||||
114Ag | 47 | 67 | 113.908823(5) | 4.6(1) s | β− | 114Cd | 1+ | ||||||||||||
114mAg | 198.9(10) keV | 1.50(5) ms | IT | 114Ag | (6+) | ||||||||||||||
115Ag | 47 | 68 | 114.908767(20) | 20.0(5) min | β− | 115mCd | 1/2− | ||||||||||||
115mAg | 41.16(10) keV | 18.0(7) s | β− (79.0%) | 115Cd | 7/2+ | ||||||||||||||
IT (21.0%) | 115Ag | ||||||||||||||||||
116Ag | 47 | 69 | 115.911387(4) | 3.83(8) min | β− | 116Cd | (0−) | ||||||||||||
116m1Ag | 47.90(10) keV | 20(1) s | β− (93%) | 116Cd | (3+) | ||||||||||||||
IT (7%) | 116Ag | ||||||||||||||||||
116m2Ag | 129.80(22) keV | 9.3(3) s | β− (92%) | 116Cd | (6−) | ||||||||||||||
IT (8%) | 116Ag | ||||||||||||||||||
117Ag | 47 | 70 | 116.911774(15) | 73.6(14) s | β− | 117mCd | 1/2−# | ||||||||||||
117mAg | 28.6(2) keV | 5.34(5) s | β− (94.0%) | 117mCd | 7/2+# | ||||||||||||||
IT (6.0%) | 117Ag | ||||||||||||||||||
118Ag | 47 | 71 | 117.9145955(27) | 3.76(15) s | β− | 118Cd | (2−) | ||||||||||||
118m1Ag | 45.79(9) keV | ~0.1 μs | IT | 118Ag | (1,2)− | ||||||||||||||
118m2Ag | 127.63(10) keV | 2.0(2) s | β− (59%) | 118Cd | (5+) | ||||||||||||||
IT (41%) | 118Ag | ||||||||||||||||||
118m3Ag | 279.37(20) keV | ~0.1 μs | IT | 118Ag | (3+) | ||||||||||||||
119Ag | 47 | 72 | 118.915570(16) | 2.1(1) s | β− | 119Cd | (7/2+) | ||||||||||||
119mAg | 33.5(3) keV [7] | 6.0(5) s | β− | 119Cd | (1/2−) | ||||||||||||||
120Ag | 47 | 73 | 119.918785(5) | 1.52(7) s | β− | 120Cd | 4(+) | ||||||||||||
β−, n (<.003%) | 119Cd | ||||||||||||||||||
120m1Ag [n 9] | 0(50)# keV | 940(100) ms | β−? | 120Cd | (0−, 1−) | ||||||||||||||
IT? | 120Ag | ||||||||||||||||||
β−, n? | 119Cd | ||||||||||||||||||
120m2Ag | 203.2(2) keV | 384(22) ms | IT (68%) | 120Sn | 7(−) | ||||||||||||||
β− (32%) | 120Cd | ||||||||||||||||||
β−, n? | 119Cd | ||||||||||||||||||
121Ag | 47 | 74 | 120.920125(13) | 777(10) ms | β− (99.92%) | 121Cd | 7/2+# | ||||||||||||
β−, n (0.080%) | 120Cd | ||||||||||||||||||
122Ag [8] | 47 | 75 | 121.9235420(56) | 550(50) ms | β− | 122Cd | (1−) | ||||||||||||
β−, n? | 121Cd | ||||||||||||||||||
122m1Ag [8] | 303.7(50) keV | 200(50) ms | β− | 122Cd | (9−) | ||||||||||||||
β−, n? | 121Cd | ||||||||||||||||||
IT? | 122Ag | ||||||||||||||||||
122m2Ag | 171(50)# keV | 6.3(1) μs | IT | 122Ag | (1+) | ||||||||||||||
123Ag | 47 | 76 | 122.92532(4) | 294(5) ms | β− (99.44%) | 123Cd | (7/2+) | ||||||||||||
β−, n (0.56%) | 122Cd | ||||||||||||||||||
123m1Ag | 59.5(5) keV | 100# ms | β− | 123Cd | (1/2−) | ||||||||||||||
β−, n? | 122Cd | ||||||||||||||||||
123m2Ag | 1450(14)# keV | 202(20) ns | IT | 123Ag | |||||||||||||||
123m3Ag | 1472.8(8) keV | 393(16) ns | IT | 123Ag | (17/2−) | ||||||||||||||
124Ag | 47 | 77 | 123.92890(27)# | 177.9(26) ms | β− (98.7%) | 124Cd | (2−) | ||||||||||||
β−, n (1.3%) | 123Cd | ||||||||||||||||||
124m1Ag [n 9] | 50(50)# keV | 144(20) ms | β− | 124Cd | 9−# | ||||||||||||||
β−, n? | 123Cd | ||||||||||||||||||
124m2Ag | 155.6(5) keV | 140(50) ns | IT | 124Ag | (1+) | ||||||||||||||
124m3Ag | 231.1(7) keV | 1.48(15) μs | IT | 124Ag | (1−) | ||||||||||||||
125Ag | 47 | 78 | 124.93074(47) | 160(5) ms | β− (88.2%) | 125Cd | (9/2+) | ||||||||||||
β−, n (11.8%) | 124Cd | ||||||||||||||||||
125m1Ag | 97.1(5) keV | 50# ms | β−? | 125Cd | (1/2−) | ||||||||||||||
IT? | 125Ag | ||||||||||||||||||
β−, n? | 124Cd | ||||||||||||||||||
125m2Ag | 1501.2(6) keV | 491(20) ns | IT | 125Ag | (17/2−) | ||||||||||||||
126Ag | 47 | 79 | 125.93481(22)# | 52(10) ms | β− (86.3%) | 126Cd | 3+# | ||||||||||||
β−, n (13.7%) | 125Cd | ||||||||||||||||||
126m1Ag | 100(100)# keV | 108.4(24) ms | β− | 126Cd | 9−# | ||||||||||||||
IT? | 126Ag | ||||||||||||||||||
β−, n? | 125Cd | ||||||||||||||||||
126m2Ag | 254.8(5) keV | 27(6) μs | IT | 126Ag | 1−# | ||||||||||||||
127Ag | 47 | 80 | 126.93704(22)# | 89(2) ms | β− (85.4%) | 127Cd | (9/2+) | ||||||||||||
β−, n (14.6%) | 126Cd | ||||||||||||||||||
127mAg | 1938(17) keV | 67.5(9) ms | β− (91.2%) | 127Cd | (27/2+) | ||||||||||||||
IT (8.8%) | 127Ag | ||||||||||||||||||
128Ag | 47 | 81 | 127.94127(32)# | 60(3) ms | β− (80%) | 128Cd | 3+# | ||||||||||||
β−, n (20%) | 127Cd | ||||||||||||||||||
β−, 2n? | 126Cd | ||||||||||||||||||
129Ag | 47 | 82 | 128.94432(43)# | 49.9(35) ms | β− (>80%) | 129Cd | 9/2+# | ||||||||||||
β−, n (<20%) | 128Cd | ||||||||||||||||||
130Ag | 47 | 83 | 129.95073(46)# | 40.6(45) ms | β− | 130Cd | 1−# | ||||||||||||
β−, n? | 129Cd | ||||||||||||||||||
β−, 2n? | 128Cd | ||||||||||||||||||
131Ag | 47 | 84 | 130.95625(54)# | 35(8) ms | β− (90%) | 131Cd | 9/2+# | ||||||||||||
β−, 2n (10%) | 129Cd | ||||||||||||||||||
β−, n? | 130Cd | ||||||||||||||||||
132Ag | 47 | 85 | 131.96307(54)# | 30(14) ms | β− | 132Cd | 6−# | ||||||||||||
β−, n? | 131Cd | ||||||||||||||||||
β−, 2n? | 130Cd | ||||||||||||||||||
This table header & footer: |
EC: | Electron capture |
IT: | Isomeric transition |
n: | Neutron emission |
p: | Proton emission |
Fluorine (9F) has 19 known isotopes ranging from 13
F
to 31
F
and two isomers. Only fluorine-19 is stable and naturally occurring in more than trace quantities; therefore, fluorine is a monoisotopic and mononuclidic element.
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 3.823 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.
There are 42 isotopes of polonium (84Po). They range in size from 186 to 227 nucleons. They are all radioactive. 210Po with a half-life of 138.376 days has the longest half-life of any naturally-occurring isotope of polonium and is the most common isotope of polonium. It is also the most easily synthesized polonium isotope. 209Po, which does not occur naturally, has the longest half-life of all isotopes of polonium at 124 years. 209Po can be made by using a cyclotron to bombard bismuth with protons, as can 208Po.
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.
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.
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 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 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 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.
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.
Arsenic (33As) has 32 known isotopes and at least 10 isomers. Only one of these isotopes, 75As, is stable; as such, it is considered a monoisotopic element. The longest-lived radioisotope is 73As with a half-life of 80 days.
Germanium (32Ge) has five naturally occurring isotopes, 70Ge, 72Ge, 73Ge, 74Ge, and 76Ge. Of these, 76Ge is very slightly radioactive, decaying by double beta decay with a half-life of 1.78 × 1021 years (130 billion times the age of the universe).
Naturally occurring scandium (21Sc) is composed of one stable isotope, 45Sc. Twenty-five 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.
Aluminium or aluminum (13Al) has 22 known isotopes from 22Al to 43Al and 4 known isomers. Only 27Al (stable isotope) and 26Al (radioactive isotope, t1/2 = 7.2×105 y) occur naturally, however 27Al comprises nearly all natural aluminium. Other than 26Al, all radioisotopes have half-lives under 7 minutes, most under a second. The standard atomic weight is 26.9815385(7). 26Al is produced from argon in the atmosphere by spallation caused by cosmic-ray protons. Aluminium isotopes have found practical application in dating marine sediments, manganese nodules, glacial ice, quartz in rock exposures, and meteorites. The ratio of 26Al to 10Be has been used to study the role of sediment transport, deposition, and storage, as well as burial times, and erosion, on 105 to 106 year time scales. 26Al has also played a significant role in the study of meteorites.
Magnesium (12Mg) naturally occurs in three stable isotopes: 24
Mg, 25
Mg, and 26
Mg. There are 19 radioisotopes that have been discovered, ranging from 18
Mg to 40
Mg. The longest-lived radioisotope is 28
Mg with a half-life of 20.915(9) h. The lighter isotopes mostly decay to isotopes of sodium while the heavier isotopes decay to isotopes of aluminium. The shortest-lived is proton-unbound 18
Mg with a half-life of 4.0(3.4) zeptoseconds.
Einsteinium (99Es) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be discovered was 253Es in 1952. There are 18 known radioisotopes from 240Es to 257Es, and 4 nuclear isomers. The longest-lived isotope is 252Es with a half-life of 471.7 days, or around 1.293 years.
Mendelevium (101Md) is a synthetic element, and thus a standard atomic weight cannot be given. Like all artificial elements, it has no stable isotopes. The first isotope to be synthesized was 256Md in 1955. There are 17 known radioisotopes, ranging in atomic mass from 244Md to 260Md, and 5 isomers. The longest-lived isotope is 258Md with a half-life of 51.3 days, and the longest-lived isomer is 258mMd with a half-life of 57 minutes.