50
Sn
Tin
Atomic Mass 118.710
Electron Configuration [Kr]5s24d105p2
Oxidation States +4, +2
Year Discovered Ancient

Identifiers

Element Name Tin
Element Symbol Sn
InChI InChI=1S/Sn
InChIKey ATJFFYVFTNAWJD-UHFFFAOYSA-N

Properties

Atomic Weight

118.710(7)

118.710

118.7

118.710(7)

Electron Configuration

[Kr]5s24d105p2

Atomic Radius

Van der Waals Atomic Radius : 217 pm (Van der Waals)

Empirical Atomic Radius : 145pm (Empirical)

Covalent Atomic Radius : 139(4) pm (Covalent)

Oxidation States

+4, +2

4, 3,2, 1, -1, -2, -3, -4 ​(an amphoteric oxide)

Ground Level

3P0

Ionization Energy

7.344 eV

7.343918 ± 0.000012 eV

Electronegativity

Pauling Scale Electronegativity : 1.96(Pauling Scale)

Allen Scale Electronegativity : 1.824(Allen Scale)

Electron Affinity

1.2eV

1.03eV

Atomic Spectra

Lines Holdings

Levels Holdings

Physical Description

Solid

Element Classification

Metal

Element Period Number

5

Element Group Number

14

Density

7.287 grams per cubic centimeter

Melting Point

505.08 K (231.93°C or 449.47°F)

231.93°C

Boiling Point

2875 K (2602°C or 4715°F)

2602°C

Estimated Crustal Abundance

2.3 milligrams per kilogram

Estimated Oceanic Abundance

4×10-6 milligrams per liter

History

The name derives from the Anglo-Saxon tin of unknown origin. The symbol Sn is derived from Latin stannum for alloys containing lead. The element was known in prehistoric times.

Archaeological evidence suggests that people have been using tin for at least 5500 years. Tin is primarily obtained from the mineral cassiterite (SnO2) and is extracted by roasting cassiterite in a furnace with carbon. Tin makes up only about 0.001% of the earth's crust and is chiefly mined in Malaysia. Two allotropes of tin occur near room temperature. The first form of tin is called gray tin and is stable at temperatures below 13.2°C (55.76°F). There are few, if any, uses for gray tin. At temperatures above 13.2°C, gray tin slowly turns into tin's second form, white tin. White tin is the normal form of the metal and has many uses. Unfortunately, white tin will turn into gray tin if its temperature falls below 13.2°C. This change can be prevented if small amounts of antimony or bismuth are added to white tin.

The Latin word for tin is stannum. Known to the ancients.

Historical Atomic Weights

Year Atomic Weight (uncertainty) [u] Reference
1983 118.710(7) https://doi.org/10.1351/pac198456060653
1969 118.69(3) https://doi.org/10.1351/pac197021010091
1961 118.69 https://doi.org/10.1021/ja00881a001
1925 118.70 https://doi.org/10.1039/CT9252700913
1916 118.7 https://doi.org/10.1021/ja02176a001
1903 119.0 https://doi.org/10.1021/ja02003a001
1902 118.5 https://doi.org/10.1007/BF01370337

Historical Isotopic Abundances

Year Isotope Abundance (uncertainty) Reference
1997 112Sn 0.0097(1) https://doi.org/10.1351/pac199870010217
1997 114Sn 0.0066(1) https://doi.org/10.1351/pac199870010217
1997 115Sn 0.0034(1) https://doi.org/10.1351/pac199870010217
1997 116Sn 0.1454(9) https://doi.org/10.1351/pac199870010217
1997 117Sn 0.0768(7) https://doi.org/10.1351/pac199870010217
1997 118Sn 0.2422(9) https://doi.org/10.1351/pac199870010217
1997 119Sn 0.0859(4) https://doi.org/10.1351/pac199870010217
1997 120Sn 0.3258(9) https://doi.org/10.1351/pac199870010217
1997 122Sn 0.0463(3) https://doi.org/10.1351/pac199870010217
1997 124Sn 0.0579(5) https://doi.org/10.1351/pac199870010217
1989 112Sn 0.0097(1) https://doi.org/10.1351/pac199163070991
1989 114Sn 0.0065(1) https://doi.org/10.1351/pac199163070991
1989 115Sn 0.0034(1) https://doi.org/10.1351/pac199163070991
1989 116Sn 0.1453(1) https://doi.org/10.1351/pac199163070991
1989 117Sn 0.0768(7) https://doi.org/10.1351/pac199163070991
1989 118Sn 0.2423(11) https://doi.org/10.1351/pac199163070991
1989 119Sn 0.0859(4) https://doi.org/10.1351/pac199163070991
1989 120Sn 0.3259(10) https://doi.org/10.1351/pac199163070991
1989 122Sn 0.0463(3) https://doi.org/10.1351/pac199163070991
1989 124Sn 0.0579(5) https://doi.org/10.1351/pac199163070991
1983 112Sn 0.0097(1) https://doi.org/10.1351/pac198456060675
1983 114Sn 0.0065(1) https://doi.org/10.1351/pac198456060675
1983 115Sn 0.0036(1) https://doi.org/10.1351/pac198456060675
1983 116Sn 0.1453(11) https://doi.org/10.1351/pac198456060675
1983 117Sn 0.0768(7) https://doi.org/10.1351/pac198456060675
1983 118Sn 0.2422(11) https://doi.org/10.1351/pac198456060675
1983 119Sn 0.0858(4) https://doi.org/10.1351/pac198456060675
1983 120Sn 0.3259(10) https://doi.org/10.1351/pac198456060675
1983 122Sn 0.0463(3) https://doi.org/10.1351/pac198456060675
1983 124Sn 0.0579(5) https://doi.org/10.1351/pac198456060675
1979 112Sn 0.010(2) https://doi.org/10.1351/pac198052102349
1979 114Sn 0.007(2) https://doi.org/10.1351/pac198052102349
1979 115Sn 0.004(2) https://doi.org/10.1351/pac198052102349
1979 116Sn 0.147(3) https://doi.org/10.1351/pac198052102349
1979 117Sn 0.077(2) https://doi.org/10.1351/pac198052102349
1979 118Sn 0.243(4) https://doi.org/10.1351/pac198052102349
1979 119Sn 0.086(2) https://doi.org/10.1351/pac198052102349
1979 120Sn 0.324(4) https://doi.org/10.1351/pac198052102349
1979 122Sn 0.046(2) https://doi.org/10.1351/pac198052102349
1979 124Sn 0.056(2) https://doi.org/10.1351/pac198052102349
1975 112Sn 0.01 https://doi.org/10.1351/pac197647010075
1975 114Sn 0.007 https://doi.org/10.1351/pac197647010075
1975 115Sn 0.004 https://doi.org/10.1351/pac197647010075
1975 116Sn 0.147 https://doi.org/10.1351/pac197647010075
1975 117Sn 0.077 https://doi.org/10.1351/pac197647010075
1975 118Sn 0.243 https://doi.org/10.1351/pac197647010075
1975 119Sn 0.086 https://doi.org/10.1351/pac197647010075
1975 120Sn 0.324 https://doi.org/10.1351/pac197647010075
1975 122Sn 0.046 https://doi.org/10.1351/pac197647010075
1975 124Sn 0.056 https://doi.org/10.1351/pac197647010075

Description

Ordinary tin is composed of nine stable isotopes; 18 unstable isotopes are also known. Ordinary tin is a silver-white metal, is malleable, somewhat ductile, and has a highly crystalline structure. Due to the breaking of these crystals, a "tin cry" is heard when a bar is bent.

Users

Tin resists corrosion and is used as a protective coating on other metals. Tin cans are probably the most familiar example of this application. A tin can is actually made from steel. A thin layer of tin is applied to the inside and outside of the can to keep the steel from rusting. Once widely used, tin cans have largely been replaced with plastic and aluminum containers.

Tin is used in the Pilkington process to produce window glass. In the Pilkington process, molten glass is poured onto a pool of molten tin. The glass floats on the surface of the tin and cools, forming solid glass with flat, parallel surfaces. Most of the window glass produced today is made this way.

Tin is used to form many useful alloys. Bronze is an alloy of tin and copper. Tin and lead are alloyed to make pewter and solder. An alloy of tin and niobium is used to make superconductive wire. Type metal, fusible metal, bell metal and Babbitt metal are other examples of tin alloys.

Tin salts can be sprayed onto glass to make electrically conductive coatings. These can then be used to make panel lighting and frost-free windshields. Stannous fluoride (SnF2) is used in some types of toothpaste.

Sources

Tin is found chiefly in cassiterite (SnO2). Most of the world's supply comes from Malaya, Bolivia, Indonesia, Zaire, Thailand, and Nigeria. The U.S. produces almost none, although occurrences have been found in Alaska and California. Tin is obtained by reducing the ore with coal in a reverberatory furnace.

Compounds

The element has two allotropic forms at normal pressure. On warming, gray, or alpha tin, with a cubic structure, changes at 13.2°C into white, or beta tin, the ordinary form of the metal. White tin has a tetragonal structure. When tin is cooled below 13.2°C, it changes slowly from white to gray. This change is affected by impurities such as aluminum and zinc, and can be prevented by small additions of antimony or bismuth. This change from the alpha to beta form is called the tin pest. There are few if any uses for gray tin. Tin takes a high polish and is used to coat other metals to prevent corrosion or other chemical action. Such tin plate over steel is used in the so-called tin can for preserving food.

Alloys of tin are very important. Soft solder, type metal, fusible metal, pewter, bronze, bell metal, Babbitt metal, White metal, die casting alloy, and phosphor bronze are some of the important alloys using tin.

Tin resists distilled sea and soft tap water, but is attacked by strong acids, alkalis, and acid salts. Oxygen in solution accelerates the attack. When heated in air, tin forms Sn2, which is feebly acid, forming stannate salts with basic oxides. The most important salt is the chloride, which is used as a reducing agent and as a mordant in calico printing. Tin salts sprayed onto glass are used to produce electrically conductive coatings. These have been used for panel lighting and for frost-free windshields. Most window glass is now made by floating molten glass on molten tin (float glass) to produce a flat surface (Pilkington process).

Also interesting is a crystalline tin-niobium alloy that is superconductive at very low temperatures. This promises to be important in the construction of superconductive magnets that generate enormous field strengths but use practically no power. Such magnets, made of tin-niobium wire, weigh only a few pounds and produce magnetic fields that, when started with a small battery, are comparable to that of a 100 ton electromagnet operated continuously with a large power supply.

See more information at the Tin compound page.

Element Forms

CID Name Formula SMILES Molecular Weight
5352426 tin Sn [Sn] 118.71
4077523 tin(4+) Sn+4 [Sn+4] 118.71
104883 tin(2+) Sn+2 [Sn+2] 118.71
6335514 tin-113 Sn [113Sn] 112.90518
6335914 tin-126 Sn [126Sn] 125.9077
6337030 tin-117 Sn [117Sn] 116.902954
6337622 tin-119 Sn [119Sn] 118.903311
6337663 tin-110 Sn [110Sn] 109.9078
6337049 tin-121 Sn [121Sn] 120.90424
6337050 tin-123 Sn [123Sn] 122.90573
6337561 tin-118 Sn [118Sn] 117.901607
6337564 tin-114 Sn [114Sn] 113.9027801
6337575 tin-112 Sn [112Sn] 111.904825
6337579 tin-127 Sn [127Sn] 126.91039
6337587 tin-111 Sn [111Sn] 110.90774
6337596 tin-128 Sn [128Sn] 127.9105
25087153 tin-115 Sn [115Sn] 114.9033447
25195421 tin-120 Sn [120Sn] 119.902203
6336618 tin-125 Sn [125Sn] 124.90779
25195420 tin-116 Sn [116Sn] 115.901743
121233902 tin-122 Sn [122Sn] 121.90345
46898734 tin-117(4+) Sn+4 [117Sn+4] 116.902954
51352785 tin-125(4+) Sn+4 [125Sn+4] 124.90779
131708376 tin-124 Sn [124Sn] 123.90528

Handling And Storage

The small amount of tin found in canned foods is quite harmless. The agreed limit of tin content in U.S. foods is 300 mg/kg. The trialkyl and triaryl tin compounds are used as biocides and must be handled carefully.

Isotopes

Stable Isotope Count 8

Isotopes in Earth/Planetary Science

Molecules, atoms, and ions of the stable isotopes of tin possess slightly different physical and chemical properties, and they commonly will be fractionated during physical, chemical, and biological processes, giving rise to variations in isotopic abundances and in atomic weights. There are measureable variations in the isotopic abundances of tin in natural terrestrial materials (Fig. IUPAC.50.1) [366].

Fig. IUPAC.50.1: Variation of the isotope amount ratio n(¹²⁴Sn)/n(¹²⁰Sn) of selected cassiterite samples from China (modified after [366]).

[366] E. Yamazaki, S. Nakai, T. Yokoyama, S. Ishihara, H. Tang. Geochem. J.47, 21 (2013).

Isotopes in Medicine

117mSn (with a half-life of 14 days) DTPA is routinely used for diagnostic bone imaging and for the treatment of bone pain caused by the spread of cancer to bones. The m in the superscript of 117mSn indicates a metastable state of the isotope. By using 117mSn DTPA, marrow toxicity can be reduced, and the therapeutic efficacy of using radionuclides is maintained [367]. 117mSn is a promising radionuclide for therapeutic applications because the radionuclide decays in a way that causes less damage to healthy tissues and bone marrow than other available treatments. These properties of 117mSn make it useful for the treatment of inflammatory synovial disease (i.e. rheumatoid arthritis) [368].

[367] A. Bishayee, D. V. Rao, S. C. Srivastava, L. G. Bouchet, W. E. Bolch, R. W. Howell. J. Nucl. Med.41, 2043 (2000).
[368] S. C. Srivastava. Braz. Arch. Biol. Technol.50, 49 (2007).

Isotopes Used as a Source of Radioactive Isotope(s)

112Sn is used to produce the radioisotope 113Sn (with a half-life of 115 days) via the reaction 112Sn (n, γ) 113Sn. This is used for n(113Sn)/n(113mIn) generators for the elution (extracting one material from another) of 113mIn (with a half-life of 1.66 h) as chloride for blood pool imaging. The m the superscript of 113mIn indicates a metastable state of the isotope. 117mSn is a medical radioisotope that can be produced using 116Sn and 117Sn [369].

[369] B. Ponsard, S. C. Srivastava, L. F. Mausner, F. F. Knapp, M. A. Garland, S. Mirzadeh. Appl. Radiat. Isot.67 1158 (2009).

Isotope Mass and Abundance

Isotope Atomic Mass (uncertainty) [u] Abundance (uncertainty)
112Sn 111.904 825(2) 0.0097(1) 0.0097(1)
114Sn 113.902 7801(2) 0.0066(1) 0.0066(1)
115Sn 114.903 3447(1) 0.0034(1) 0.0034(1)
116Sn 115.901 7428(6) 0.1454(9) 0.1454(9)
117Sn 116.902 954(3) 0.0768(7) 0.0768(7)
118Sn 117.901 607(3) 0.2422(9) 0.2422(9)
119Sn 118.903 311(5) 0.0859(4) 0.0859(4)
120Sn 119.902 202(6) 0.3258(9) 0.3258(9)
122Sn 121.903 44(2) 0.0463(3) 0.0463(3)
124Sn 123.905 277(7) 0.0579(5) 0.0579(5)

Atomic Mass, Half Life, and Decay

Nuclide Atomic Mass and Uncertainty [u] Half Life and Uncertainty Discovery Year Decay Modes, Intensities and Uncertainties [%]
99Sn 98.948495 ± 0.000625 [Estimated] 24 ms ± 4 2011 β+=100%; β+p=5±0.3%
100Sn 99.938648944 ± 0.000257661 1.18 s ± 0.08 1994 β+=100%; β+p<17%
100Snm 99.938648944 ± 0.000257661 100 ns [Estimated] p ?
101Sn 100.935259252 ± 0.000322068 2.22 s ± 0.05 1994 β+=100%; β+p=21.0±0.7%
102Sn 101.930289525 ± 0.000107466 3.8 s ± 0.2 1994 β+=100%
102Snm 101.930289525 ± 0.000107466 367 ns ± 8 1996 IT=100%
103Sn 102.927973 ± 0.000108 [Estimated] 7.0 s ± 0.2 1981 β+=100%; β+p=1.2±0.1%
104Sn 103.923105195 ± 0.000006167 20.8 s ± 0.5 1985 β+=100%
105Sn 104.921268421 ± 0.000004263 32.7 s ± 0.5 1981 β+=100%; β+p=0.011±0.4%
106Sn 105.916957394 ± 0.000005465 1.92 m ± 0.08 1975 β+=100%
107Sn 106.915713649 ± 0.0000057 2.90 m ± 0.05 1976 β+=100%
108Sn 107.911894290 ± 0.000005778 10.30 m ± 0.08 1968 β+=100%
109Sn 108.911292857 ± 0.000008533 18.1 m ± 0.2 1966 β+=100%
110Sn 109.907844835 ± 0.00001479 4.154 h ± 0.004 1965 ε=100%
111Sn 110.907741143 ± 0.000005728 35.3 m ± 0.6 1949 β+=100%
111Snm 110.907741143 ± 0.000005728 12.5 us ± 1.0 1972 IT=100%
112Sn 111.904824894 ± 0.000000315 Stable 1927 IS=0.97±0.1%; 2β+ ?
113Sn 112.905175857 ± 0.00000169 115.08 d ± 0.04 1939 β+=100%
113Snm 112.905175857 ± 0.00000169 21.4 m ± 0.4 1961 IT=91.1±2.3%; β+=8.9±2.3%
114Sn 113.902780130 ± 0.000000031 Stable 1927 IS=0.66±0.1%
114Snm 113.902780130 ± 0.000000031 733 ns ± 14 1980 IT=100%
115Sn 114.903344695 ± 0.000000016 Stable 1927 IS=0.34±0.1%
115Snm 114.903344695 ± 0.000000016 3.26 us ± 0.08 1967 IT=100%
115Snn 114.903344695 ± 0.000000016 159 us ± 1 1958 IT=100%
116Sn 115.901742825 ± 0.000000103 Stable 1922 IS=14.54±0.9%
116Snm 115.901742825 ± 0.000000103 348 ns ± 19 1964 IT=100%
116Snn 115.901742825 ± 0.000000103 833 ns ± 30 1978 IT=100%
117Sn 116.902954036 ± 0.000000518 Stable 1923 IS=7.68±0.7%
117Snm 116.902954036 ± 0.000000518 13.939 d ± 0.024 1950 IT=100%
117Snn 116.902954036 ± 0.000000518 1.75 us ± 0.07 1979 IT=100%
118Sn 117.901606630 ± 0.000000536 Stable 1924 IS=24.22±0.9%
118Snm 117.901606630 ± 0.000000536 230 ns ± 10 1961 IT=100%
118Snn 117.901606630 ± 0.000000536 2.52 us ± 0.06 1973 IT=100%
119Sn 118.903311266 ± 0.000000778 Stable 1925 IS=8.59±0.4%
119Snm 118.903311266 ± 0.000000778 293.1 d ± 0.7 1950 IT=100%
119Snn 118.903311266 ± 0.000000778 9.6 us ± 1.2 1992 IT=100%
119Snp 118.903311266 ± 0.000000778 96 ns ± 9 2016 IT=100%
120Sn 119.902202557 ± 0.000000987 Stable 1926 IS=32.58±0.9%
120Snm 119.902202557 ± 0.000000987 11.8 us ± 0.5 1960 IT=100%
120Snn 119.902202557 ± 0.000000987 6.26 us ± 0.11 1987 IT=100%
121Sn 120.904243488 ± 0.00000105 27.03 h ± 0.04 1948 β-=100%
121Snm 120.904243488 ± 0.00000105 43.9 y ± 0.5 1962 IT=77.6±2%; β-=22.4±2%
121Snn 120.904243488 ± 0.00000105 5.3 us ± 0.5 1995 IT=100%
121Snp 120.904243488 ± 0.00000105 520 ns ± 50 2012 IT=100%
121Snq 120.904243488 ± 0.00000105 167 ns ± 25 1995 IT=100%
122Sn 121.903445494 ± 0.000002627 Stable 1928 IS=4.63±0.3%; 2β- ?
122Snm 121.903445494 ± 0.000002627 7.5 us ± 0.9 1979 IT=100%
122Snn 121.903445494 ± 0.000002627 62 us ± 3 1992 IT=100%
122Snp 121.903445494 ± 0.000002627 139 ns ± 9 2012 IT=100%
123Sn 122.905727065 ± 0.000002661 129.2 d ± 0.4 1948 β-=100%
123Snm 122.905727065 ± 0.000002661 40.06 m ± 0.01 1948 β-=100%
123Snn 122.905727065 ± 0.000002661 7.4 us ± 2.6 1992 IT=100%
123Snp 122.905727065 ± 0.000002661 6 us 1994 IT=100%
123Snq 122.905727065 ± 0.000002661 34 us 1994 IT=100%
124Sn 123.905279619 ± 0.00000141 Stable >100Py 1922 IS=5.79±0.5%; 2β- ?
124Snm 123.905279619 ± 0.00000141 270 ns ± 60 1979 IT=100%
124Snn 123.905279619 ± 0.00000141 3.1 us ± 0.5 1979 IT=100%
124Snp 123.905279619 ± 0.00000141 51 us ± 3 1992 IT=100%
124Snq 123.905279619 ± 0.00000141 260 ns ± 25 2012 IT=100%
125Sn 124.907789370 ± 0.000001426 9.634 d ± 0.015 1939 β-=100%
125Snm 124.907789370 ± 0.000001426 9.77 m ± 0.25 1939 β-=100%
125Snn 124.907789370 ± 0.000001426 6.2 us ± 0.2 2000 IT=100%
125Snp 124.907789370 ± 0.000001426 650 ns ± 60 2008 IT=100%
125Snq 124.907789370 ± 0.000001426 230 ns ± 17 2000 IT=100%
126Sn 125.907658958 ± 0.000011473 230 ky ± 14 1962 β-=100%
126Snm 125.907658958 ± 0.000011473 6.1 us ± 0.7 1979 IT=100%
126Snn 125.907658958 ± 0.000011473 7.6 us ± 0.3 2000 IT=100%
126Snp 125.907658958 ± 0.000011473 114 ns ± 2 2012 IT=100%
127Sn 126.910391726 ± 0.000009904 2.10 h ± 0.04 1951 β-=100%
127Snm 126.910391726 ± 0.000009904 4.13 m ± 0.03 1962 β-=100%
127Snn 126.910391726 ± 0.000009904 4.52 us ± 0.15 2000 IT=100%
127Snp 126.910391726 ± 0.000009904 1.26 us ± 0.15 2004 IT=100%
127Snq 126.910391726 ± 0.000009904 250 ns ± 30 2008 IT=100%
128Sn 127.910507828 ± 0.000018982 59.07 m ± 0.14 1956 β-=100%
128Snm 127.910507828 ± 0.000018982 6.5 s ± 0.5 1979 IT=100%
128Snn 127.910507828 ± 0.000018982 2.91 us ± 0.14 1981 IT=100%
128Snp 127.910507828 ± 0.000018982 220 ns ± 30 2011 IT=100%
129Sn 128.913482440 ± 0.00001854 2.23 m ± 0.04 1962 β-=100%
129Snm 128.913482440 ± 0.00001854 6.9 m ± 0.1 1962 β-=100%
129Snn 128.913482440 ± 0.00001854 3.49 us ± 0.11 2000 IT=100%
129Snp 128.913482440 ± 0.00001854 2.22 us ± 0.13 2000 IT=100%
129Snq 128.913482440 ± 0.00001854 221 ns ± 18 2008 IT=100%
130Sn 129.913974531 ± 0.00000201 3.72 m ± 0.07 1972 β-=100%
130Snm 129.913974531 ± 0.00000201 1.7 m ± 0.1 1974 β-=100%
130Snn 129.913974531 ± 0.00000201 1.501 us ± 0.017 1981 IT=100%
131Sn 130.917053067 ± 0.000003887 56.0 s ± 0.5 1963 β-=100%
131Snm 130.917053067 ± 0.000003887 58.4 s ± 0.5 1977 β-=100%; IT ?
131Snn 130.917053067 ± 0.000003887 316 ns ± 5 2001 IT=100%
132Sn 131.917823898 ± 0.000002121 39.7 s ± 0.8 1963 β-=100%
132Snm 131.917823898 ± 0.000002121 2.080 us ± 0.016 1986 IT=100%
133Sn 132.923913753 ± 0.000002043 1.37 s ± 0.07 1973 β-=100%; β-n=0.0294±2.4%
134Sn 133.928680430 ± 0.0000034 0.93 s ± 0.08 1974 β-=100%; β-n=17±1.3%
134Snm 133.928680430 ± 0.0000034 87 ns ± 8 2000 IT=100%
135Sn 134.934908603 ± 0.0000033 515 ms ± 5 1994 β-=100%; β-n=21±0.3%; β-2n ?
136Sn 135.939699 ± 0.000215 [Estimated] 355 ms ± 18 1994 β-=100%; β-n=28±0.3%; β-2n ?
137Sn 136.946162 ± 0.000322 [Estimated] 249 ms ± 15 1994 β-=100%; β-n=48±0.6%; β-2n ?
138Sn 137.951143 ± 0.000429 [Estimated] 148 ms ± 9 2010 β-=100%; β-n=36±1.2%; β-2n ?
138Snm 137.951143 ± 0.000429 [Estimated] 210 ns ± 45 2014 IT=100%
139Sn 138.957799 ± 0.000429 [Estimated] 120 ms ± 38 2015 β-=100%; β-n ?; β-2n ?
140Sn 139.962973 ± 0.000322 [Estimated] 50 ms >550ns [Estimated] 2018 β- ?; β-n ?; β-2n ?

Information Sources

  1. 1.  PubChem
  2. 2.  Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
  3. 3.  IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
  4. 4.  Jefferson Lab, U.S. Department of Energy
    LICENSE
    Please see citation and linking information https https://www.jlab.org/privacy-and-security-notice
  5. 5.  Los Alamos National Laboratory, U.S. Department of Energy
  6. 6.  NIST Physical Measurement Laboratory
  7. 7.  IUPAC Periodic Table of the Elements and Isotopes (IPTEI)
    LICENSE
    Copyright (c) 2020 International Union of Pure and Applied Chemistry. The International Union of Pure and Applied Chemistry (IUPAC) contribution within Pubchem is provided under a CC-BY-NC-ND 4.0 license, unless otherwise stated.
    https://creativecommons.org/licenses/by-nc-nd/4.0/
  8. 8.  PubChem Elements
    Tin

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