Isotopes of tin

Tin (Sn) is the element with the greatest number of stable isotopes (ten), which is probably related to the fact that 50 is a "magic number" of protons. 29 additional unstable isotopes are known, including the "doubly magic" tin-100 (100Sn) (discovered in 1994)[1] and tin-132 (132Sn). The longest-lived radioisotope is 126Sn with a half-life of 230,000 years. All other radioisotopes have half-lives less than a year.

Contents

Tin-121m

Medium-lived
fission products
Prop:
Unit:
t½
a
Yield
%
Q *
keV
βγ
*
155Eu 4.76 .0803 252 βγ
85Kr 10.76 .2180 687 βγ
113mCd 14.1 .0008 316 β
90Sr 28.9 4.505 2826 β
137Cs 30.23 6.337 1176 βγ
121mSn 43.9 .00005 390 βγ
151Sm 90 .5314 77 β

Tin-121m is a radioisotope and nuclear isomer of tin with a halflife of 43.9 years. In a normal thermal reactor, it has a very low fission product yield; thus, this isotope is not a significant contributor to nuclear waste.

Fast fission or fission of some heavier actinides will produce 121mSn at higher yields.

Tin-126

Long-lived
fission products
Prop:
Unit:
t½
Ma
Yield
%
Q *
KeV
βγ
*
99Tc 0.211 6.1385 294 β
126Sn 0.230 0.1084 4050 βγ
79Se 0.327 0.0447 151 β
93Zr 1.53 5.4575 91 βγ
135Cs 2.3  6.9110 269 β
107Pd 6.5  1.2499 33 β
129I 15.7  0.8410 194 βγ
Chain yield, % per fission[2]
Thermal Fast 14 MeV
232Th not fissile .0593±.0087 1.08 ± .17
233U .233 ± .032 .325 ± .075 1.79 ± .24
235U .0594±.0052 .098 ± .020 1.62 ± .49
238U not fissile .093 ± .020 1.38 ± .25
239Pu .314 ± .049 .209 ± .044  ?
241Pu .362 ± .089 .157 ± .031  ?

Tin-126 is a radioisotope of tin and one of only 7 long-lived fission products. While tin-126's halflife of 230,000 years translates to a low specific activity that limits its radioactive hazard, its short-lived decay product, antimony-126, emits high-energy gamma radiation, making external exposure to tin-126 a potential concern.

126Sn is in the middle of the mass range for fission products. Thermal reactors, which make up almost all current nuclear power plants, produce it at a very low yield (such as 0.0236% or 0.06%), since slow neutrons almost always fission 235U or 239Pu into unequal halves. Fast fission in a fast reactor or nuclear weapon, or fission of some heavy minor actinides like californium, will produce it at higher yields.

Actinides Half-life Fission products
244Cm 241Pu f 250Cf 243Cmf 10–30 y 137Cs 90Sr 85Kr
232 f 238Pu f is for
fissile
69–90 y 151Sm nc➔
4n 249Cf  f 242Amf 141–351 No fission product
has half-life 102
to 2×105 years
241Am 251Cf  f 431–898
240Pu 229Th 246Cm 243Am 5–7 ky
4n 245Cmf 250Cm 239Pu f 8–24 ky
233U    f 230Th 231Pa 32–160
4n+1 234U 4n+3 211–290 99Tc 126Sn 79Se
248Cm 242Pu 340–373 Long-lived fission products
237Np 4n+2 1–2 My 93Zr 135Cs nc➔
236U 4n+1 247Cmf 6–23 My 107Pd 129I
244Pu 80 My >7% >5% >1% >.1%
232Th 238U 235U    f 0.7–12 Gy fission product yield


Table

nuclide
symbol
Z(p) N(n)  
isotopic mass (u)
 
half-life decay
mode(s)[3][n 1]
daughter
isotope(s)[n 2]
nuclear
spin
representative
isotopic
composition
(mole fraction)
range of natural
variation
(mole fraction)
excitation energy
99Sn[n 3] 50 49 98.94933(64)# 5# ms 9/2+#
100Sn[n 4] 50 50 99.93904(76) 1.1(4) s
[0.94(+54-27) s]
β+ (83%) 100In 0+
β+, p (17%) 99Cd
101Sn 50 51 100.93606(32)# 3(1) s β+ 101In 5/2+#
β+, p (rare) 100Cd
102Sn 50 52 101.93030(14) 4.5(7) s β+ 102In 0+
β+, p (rare) 101Cd
102mSn 2017(2) keV 720(220) ns (6+)
103Sn 50 53 102.92810(32)# 7.0(6) s β+ 103In 5/2+#
β+, p (rare) 102Cd
104Sn 50 54 103.92314(11) 20.8(5) s β+ 104In 0+
105Sn 50 55 104.92135(9) 34(1) s β+ 105In (5/2+)
β+, p (rare) 105Cd
106Sn 50 56 105.91688(5) 115(5) s β+ 106In 0+
107Sn 50 57 106.91564(9) 2.90(5) min β+ 107In (5/2+)
108Sn 50 58 107.911925(21) 10.30(8) min β+ 108In 0+
109Sn 50 59 108.911283(11) 18.0(2) min β+ 109In 5/2(+)
110Sn 50 60 109.907843(15) 4.11(10) h EC 110In 0+
111Sn 50 61 110.907734(7) 35.3(6) min β+ 111In 7/2+
111mSn 254.72(8) keV 12.5(10) µs 1/2+
112Sn 50 62 111.904818(5) Observationally Stable[n 5] 0+ 0.0097(1)
113Sn 50 63 112.905171(4) 115.09(3) d β+ 113In 1/2+
113mSn 77.386(19) keV 21.4(4) min IT (91.1%) 113Sn 7/2+
β+ (8.9%) 113In
114Sn 50 64 113.902779(3) Observationally Stable[n 6] 0+ 0.0066(1)
114mSn 3087.37(7) keV 733(14) ns 7-
115Sn 50 65 114.903342(3) Observationally Stable[n 6] 1/2+ 0.0034(1)
115m1Sn 612.81(4) keV 3.26(8) µs 7/2+
115m2Sn 713.64(12) keV 159(1) µs 11/2-
116Sn 50 66 115.901741(3) Observationally Stable[n 6] 0+ 0.1454(9)
117Sn 50 67 116.902952(3) Observationally Stable[n 6] 1/2+ 0.0768(7)
117m1Sn 314.58(4) keV 13.76(4) d IT 117Sn 11/2-
117m2Sn 2406.4(4) keV 1.75(7) µs (19/2+)
118Sn 50 68 117.901603(3) Observationally Stable[n 6] 0+ 0.2422(9)
119Sn 50 69 118.903308(3) Observationally Stable[n 6] 1/2+ 0.0859(4)
119m1Sn 89.531(13) keV 293.1(7) d IT 119Sn 11/2-
119m2Sn 2127.0(10) keV 9.6(12) µs (19/2+)
120Sn 50 70 119.9021947(27) Observationally Stable[n 6] 0+ 0.3258(9)
120m1Sn 2481.63(6) keV 11.8(5) µs (7-)
120m2Sn 2902.22(22) keV 6.26(11) µs (10+)#
121Sn[n 7] 50 71 120.9042355(27) 27.03(4) h β- 121Sb 3/2+
121m1Sn 6.30(6) keV 43.9(5) a IT (77.6%) 121Sn 11/2-
β- (22.4%) 121Sb
121m2Sn 1998.8(9) keV 5.3(5) µs (19/2+)#
121m3Sn 2834.6(18) keV 0.167(25) µs (27/2-)
122Sn[n 7] 50 72 121.9034390(29) Observationally Stable[n 8] 0+ 0.0463(3)
123Sn[n 7] 50 73 122.9057208(29) 129.2(4) d β- 123Sb 11/2-
123m1Sn 24.6(4) keV 40.06(1) min β- 123Sb 3/2+
123m2Sn 1945.0(10) keV 7.4(26) µs (19/2+)
123m3Sn 2153.0(12) keV 6 µs (23/2+)
123m4Sn 2713.0(14) keV 34 µs (27/2-)
124Sn[n 7] 50 74 123.9052739(15) Observationally Stable[n 9] 0+ 0.0579(5)
124m1Sn 2204.622(23) keV 0.27(6) µs 5-
124m2Sn 2325.01(4) keV 3.1(5) µs 7-
124m3Sn 2656.6(5) keV 45(5) µs (10+)#
125Sn[n 7] 50 75 124.9077841(16) 9.64(3) d β- 125Sb 11/2-
125mSn 27.50(14) keV 9.52(5) min 3/2+
126Sn[n 10] 50 76 125.907653(11) 2.30(14)×105 a β- (66.5%) 126m2Sb 0+
β- (33.5%) 126m1Sb
126m1Sn 2218.99(8) keV 6.6(14) µs 7-
126m2Sn 2564.5(5) keV 7.7(5) µs (10+)#
127Sn 50 77 126.910360(26) 2.10(4) h β- 127Sb (11/2-)
127mSn 4.7(3) keV 4.13(3) min β- 127Sb (3/2+)
128Sn 50 78 127.910537(29) 59.07(14) min β- 128Sb 0+
128mSn 2091.50(11) keV 6.5(5) s IT 128Sn (7-)
129Sn 50 79 128.91348(3) 2.23(4) min β- 129Sb (3/2+)#
129mSn 35.2(3) keV 6.9(1) min β- (99.99%) 129Sb (11/2-)#
IT (.002%) 129Sn
130Sn 50 80 129.913967(11) 3.72(7) min β- 130Sb 0+
130m1Sn 1946.88(10) keV 1.7(1) min β- 130Sb (7-)#
130m2Sn 2434.79(12) keV 1.61(15) µs (10+)
131Sn 50 81 130.917000(23) 56.0(5) s β- 131Sb (3/2+)
131m1Sn 80(30)# keV 58.4(5) s β- (99.99%) 131Sb (11/2-)
IT (.0004%) 131Sn
131m2Sn 4846.7(9) keV 300(20) ns (19/2- to 23/2-)
132Sn 50 82 131.917816(15) 39.7(8) s β- 132Sb 0+
133Sn 50 83 132.92383(4) 1.45(3) s β- (99.97%) 133Sb (7/2-)#
β-, n (.0294%) 132Sb
134Sn 50 84 133.92829(11) 1.050(11) s β- (83%) 134Sb 0+
β-, n (17%) 133Sb
135Sn 50 85 134.93473(43)# 530(20) ms β- 135Sb (7/2-)
β-, n 134Sb
136Sn 50 86 135.93934(54)# 0.25(3) s β- 136Sb 0+
β-, n 135Sb
137Sn 50 87 136.94599(64)# 190(60) ms β- 137Sb 5/2-#
  1. ^ Abbreviations:
    EC: Electron capture
    IT: Isomeric transition
  2. ^ Bold for stable isotopes
  3. ^ Heaviest known nuclide with more protons than neutrons
  4. ^ Heaviest known nuclide with equal numbers of protons and neutrons
  5. ^ Believed to decay by β+β+ to 112Cd
  6. ^ a b c d e f g Theoretically capable of spontaneous fission
  7. ^ a b c d e Fission product
  8. ^ Believed to undergo β-β- decay to 122Te
  9. ^ Believed to undergo β-β- decay to 124Te with a half-life over 100×1015 years
  10. ^ Long-lived fission product

Notes

References

  1. ^ Identification and decay spectroscopy of 100Sn at the GSI projectile fragment separator FRS, K. Sümmerer et al., Nucl. Phys. A616, 341 (1997).
  2. ^ http://www-nds.iaea.org/sgnucdat/c1.htm Chain Fission Yields, IAEA
  3. ^ http://www.nucleonica.net/unc.aspx
Isotopes of indium Isotopes of tin Isotopes of antimony
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