Isotopes of antimony
From Infogalactic: the planetary knowledge core
Antimony (Sb) occurs in two stable isotopes, 121Sb and 123Sb. There are 35 artificial radioactive isotopes, the longest-lived of which are 125Sb, with a half-life of 2.75856 years; 124Sb, with a half-life of 60.2 days; and 126Sb, with a half-life of 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 a half-life of 5.76 days.
Relative atomic mass: 121.760(1).
Contents
Table
nuclide symbol |
Z(p) | N(n) | isotopic mass (u) |
half-life | decay mode(s)[1][n 1] |
daughter isotope(s)[n 2] |
nuclear spin |
representative isotopic composition (mole fraction) |
range of natural variation (mole fraction) |
---|---|---|---|---|---|---|---|---|---|
excitation energy | |||||||||
103Sb | 51 | 52 | 102.93969(32)# | 100# ms [>1.5 µs] | β+ | 103Sn | 5/2+# | ||
104Sb | 51 | 53 | 103.93647(39)# | 0.47(13) s [0.44(+15−11) s] |
β+ (86%) | 104Sn | |||
p (7%) | 103Sn | ||||||||
β+, p (7%) | 103In | ||||||||
α (<1%) | 100In | ||||||||
105Sb | 51 | 54 | 104.93149(11) | 1.12(16) s | β+ (99%) | 105Sn | (5/2+) | ||
p (1%) | 104Sn | ||||||||
β+, p (<1%) | 104In | ||||||||
106Sb | 51 | 55 | 105.92879(34)# | 0.6(2) s | β+ | 106Sn | (4+) | ||
106mSb | 1000(500)# keV | 220(20) ns | |||||||
107Sb | 51 | 56 | 106.92415(32)# | 4.0(2) s | β+ | 107Sn | 5/2+# | ||
108Sb | 51 | 57 | 107.92216(22)# | 7.4(3) s | β+ | 108Sn | (4+) | ||
β+, p (rare) | 107In | ||||||||
109Sb | 51 | 58 | 108.918132(20) | 17.3(5) s | β+ | 109Sn | 5/2+# | ||
110Sb | 51 | 59 | 109.91675(22)# | 23.0(4) s | β+ | 110Sn | (4+) | ||
111Sb | 51 | 60 | 110.91316(3) | 75(1) s | β+ | 111Sn | (5/2+) | ||
112Sb | 51 | 61 | 111.912398(19) | 51.4(10) s | β+ | 112Sn | 3+ | ||
113Sb | 51 | 62 | 112.909372(19) | 6.67(7) min | β+ | 113Sn | 5/2+ | ||
114Sb | 51 | 63 | 113.90927(3) | 3.49(3) min | β+ | 114Sn | (3+) | ||
114mSb | 495.5(7) keV | 219(12) µs | (8−) | ||||||
115Sb | 51 | 64 | 114.906598(17) | 32.1(3) min | β+ | 115Sn | 5/2+ | ||
116Sb | 51 | 65 | 115.906794(6) | 15.8(8) min | β+ | 116Sn | 3+ | ||
116m1Sb | 93.99(5) keV | 194(4) ns | 1+ | ||||||
116m2Sb | 380(40) keV | 60.3(6) min | β+ | 116Sn | 8− | ||||
117Sb | 51 | 66 | 116.904836(10) | 2.80(1) h | β+ | 117Sn | 5/2+ | ||
118Sb | 51 | 67 | 117.905529(4) | 3.6(1) min | β+ | 118Sn | 1+ | ||
118m1Sb | 50.814(21) keV | 20.6(6) µs | (3)+ | ||||||
118m2Sb | 250(6) keV | 5.00(2) h | β+ | 118Sn | 8− | ||||
119Sb | 51 | 68 | 118.903942(9) | 38.19(22) h | EC | 119Sn | 5/2+ | ||
119m1Sb | 2553.6(3) keV | 130(3) ns | (19/2−) | ||||||
119m2Sb | 2852(7) keV | 850(90) ms | IT | 119Sb | 27/2+# | ||||
120Sb | 51 | 69 | 119.905072(8) | 15.89(4) min | β+ | 120Sn | 1+ | ||
120m1Sb | 0(100)# keV | 5.76(2) d | β+ | 120Sn | 8− | ||||
120m2Sb | 78.16(5) keV | 246(2) ns | (3+) | ||||||
120m3Sb | 2328.3(6) keV | 400(8) ns | (6) | ||||||
121Sb[n 3] | 51 | 70 | 120.9038157(24) | Stable[n 4] | 5/2+ | 0.5721(5) | |||
122Sb | 51 | 71 | 121.9051737(24) | 2.7238(2) d | β− (97.59%) | 122Te | 2− | ||
β+ (2.41%) | 122Sn | ||||||||
122m1Sb | 61.4131(5) keV | 1.86(8) µs | 3+ | ||||||
122m2Sb | 137.4726(8) keV | 0.53(3) ms | (5)+ | ||||||
122m3Sb | 163.5591(17) keV | 4.191(3) min | IT | 122Sb | (8)− | ||||
123Sb[n 3] | 51 | 72 | 122.9042140(22) | Stable[n 4] | 7/2+ | 0.4279(5) | |||
124Sb | 51 | 73 | 123.9059357(22) | 60.20(3) d | β− | 124Te | 3− | ||
124m1Sb | 10.8627(8) keV | 93(5) s | IT (75%) | 124Sb | 5+ | ||||
β− (25%) | 124Te | ||||||||
124m2Sb | 36.8440(14) keV | 20.2(2) min | (8)− | ||||||
124m3Sb | 40.8038(7) keV | 3.2(3) µs | (3+,4+) | ||||||
125Sb | 51 | 74 | 124.9052538(28) | 2.75856(25) y | β− | 125mTe | 7/2+ | ||
126Sb | 51 | 75 | 125.90725(3) | 12.35(6) d | β− | 126Te | (8−) | ||
126m1Sb | 17.7(3) keV | 19.15(8) min | β− (86%) | 126Te | (5+) | ||||
IT (14%) | 126Sb | ||||||||
126m2Sb | 40.4(3) keV | ~11 s | IT | 126m1Sb | (3−) | ||||
126m3Sb | 104.6(3) keV | 553(5) ns | (3+) | ||||||
127Sb | 51 | 76 | 126.906924(6) | 3.85(5) d | β− | 127mTe | 7/2+ | ||
128Sb | 51 | 77 | 127.909169(27) | 9.01(4) h | β− | 128Te | 8− | ||
128mSb | 10(7) keV | 10.4(2) min | β− (96.4%) | 128Te | 5+ | ||||
IT (3.6%) | 128Sb | ||||||||
129Sb | 51 | 78 | 128.909148(23) | 4.40(1) h | β− | 129mTe | 7/2+ | ||
129m1Sb | 1851.05(10) keV | 17.7(1) min | β− (85%) | 129Te | (19/2−) | ||||
IT (15%) | 129Sb | ||||||||
129m2Sb | 1860.90(10) keV | >2 µs | (15/2−) | ||||||
129m3Sb | 2138.9(5) keV | 1.1(1) µs | (23/2+) | ||||||
130Sb | 51 | 79 | 129.911656(18) | 39.5(8) min | β− | 130Te | (8−)# | ||
130mSb | 4.80(20) keV | 6.3(2) min | β− | 130Te | (4,5)+ | ||||
131Sb | 51 | 80 | 130.911982(22) | 23.03(4) min | β− | 131mTe | (7/2+) | ||
132Sb | 51 | 81 | 131.914467(15) | 2.79(5) min | β− | 132Te | (4+) | ||
132m1Sb | 200(30) keV | 4.15(5) min | β− | 132Te | (8−) | ||||
132m2Sb | 254.5(3) keV | 102(4) ns | (6−) | ||||||
133Sb | 51 | 82 | 132.915252(27) | 2.5(1) min | β− | 133mTe | (7/2+) | ||
134Sb | 51 | 83 | 133.92038(5) | 0.78(6) s | β− | 134Te | (0-) | ||
134mSb | 80(110) keV | 10.07(5) s | β− (99.9%) | 134Te | (7−) | ||||
β−, n (.091%) | 133Te | ||||||||
135Sb | 51 | 84 | 134.92517(11) | 1.68(2) s | β− (82.4%) | 135Te | (7/2+) | ||
β−, n (17.6%) | 134Te | ||||||||
136Sb | 51 | 85 | 135.93035(32)# | 0.923(14) s | β− (83%) | 136Te | 1−# | ||
β−, n (17%) | 135Te | ||||||||
136mSb | 173(3) keV | 570(50) ns | 6−# | ||||||
137Sb | 51 | 86 | 136.93531(43)# | 450(50) ms | β− | 137Te | 7/2+# | ||
β−, n | 136Te | ||||||||
138Sb | 51 | 87 | 137.94079(32)# | 500# ms [>300 ns] | β− | 138Te | 2−# | ||
β−, n | 137Te | ||||||||
139Sb | 51 | 88 | 138.94598(54)# | 300# ms [>300 ns] | β− | 139Te | 7/2+# |
- ↑ Abbreviations:
EC: Electron capture
IT: Isomeric transition - ↑ Bold for stable isotopes, bold italics for nearly-stable isotopes (half-life longer than the age of the universe)
- ↑ 3.0 3.1 Fission product
- ↑ 4.0 4.1 Theoretically capable of spontaneous fission
Notes
- Geologically exceptional samples are known in which the isotopic composition lies outside the reported range. The uncertainty in the atomic mass may exceed the stated value for such specimens.
- Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
- Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC, which use expanded uncertainties.
See also
References
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- Isotope masses from:
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- Isotopic compositions and standard atomic masses from:
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- Lua error in package.lua at line 80: module 'strict' not found.
- Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
Isotopes of tin | Isotopes of antimony | Isotopes of tellurium |
Table of nuclides |
Isotopes of the chemical elements | |||||||||||||||||
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1 H |
2 He |
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3 Li |
4 Be |
5 B |
6 C |
7 N |
8 O |
9 F |
10 Ne |
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11 Na |
12 Mg |
13 Al |
14 Si |
15 P |
16 S |
17 Cl |
18 Ar |
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19 K |
20 Ca |
21 Sc |
22 Ti |
23 V |
24 Cr |
25 Mn |
26 Fe |
27 Co |
28 Ni |
29 Cu |
30 Zn |
31 Ga |
32 Ge |
33 As |
34 Se |
35 Br |
36 Kr |
37 Rb |
38 Sr |
39 Y |
40 Zr |
41 Nb |
42 Mo |
43 Tc |
44 Ru |
45 Rh |
46 Pd |
47 Ag |
48 Cd |
49 In |
50 Sn |
51 Sb |
52 Te |
53 I |
54 Xe |
55 Cs |
56 Ba |
72 Hf |
73 Ta |
74 W |
75 Re |
76 Os |
77 Ir |
78 Pt |
79 Au |
80 Hg |
81 Tl |
82 Pb |
83 Bi |
84 Po |
85 At |
86 Rn |
|
87 Fr |
88 Ra |
104 Rf |
105 Db |
106 Sg |
107 Bh |
108 Hs |
109 Mt |
110 Ds |
111 Rg |
112 Cn |
113 Uut |
114 Fl |
115 Uup |
116 Lv |
117 Uus |
118 Uuo |
|
57 La |
58 Ce |
59 Pr |
60 Nd |
61 Pm |
62 Sm |
63 Eu |
64 Gd |
65 Tb |
66 Dy |
67 Ho |
68 Er |
69 Tm |
70 Yb |
71 Lu |
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89 Ac |
90 Th |
91 Pa |
92 U |
93 Np |
94 Pu |
95 Am |
96 Cm |
97 Bk |
98 Cf |
99 Es |
100 Fm |
101 Md |
102 No |
103 Lr |
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