Tin (Sn)
post-transition-metalSolid
Masse atomique relative standard
118,71 uConfiguration électronique
[Kr] 5s2 4d10 5p2Point de fusion
231,93 °CPoint d’ébullition
2601,85 °CMasse volumique
7287 kg/m³États d’oxydation
−4, −3, −2, −1, 0, +1, +2, +3, +4Électronégativité (Pauling)
1,96Énergie d’ionisation (1re)
7,343918 eVAnnée de découverte
N/DRayon atomique
145 pmDétails
Tin is a post-transition metal in group 14, known for its low melting point, resistance to ordinary corrosion, and ability to form useful alloys and coatings. It occurs chiefly as cassiterite, a tin dioxide mineral, and has been worked since antiquity, especially in bronze. Chemically it is less reactive than many base metals but readily forms compounds in the +2 and +4 oxidation states, with organotin chemistry being especially important and sometimes hazardous.
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.
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.
Pure tin is a soft, silvery-white metal with a bright metallic luster. It is malleable at room temperature and melts at a relatively low temperature for a metal. Below about 13.2 °C, white tin can slowly transform to brittle gray tin under favorable conditions, a phenomenon known as tin pest.
Tin is used mainly as a protective coating on steel for food cans and other corrosion-resistant sheet products. It is an important constituent of solders, especially lead-free solders based on tin with silver, copper, antimony, or bismuth additions. Tin is also used in bronze, bearing metals, pewter, and some specialty alloys. Indium tin oxide, a mixed oxide material, is widely used as a transparent conducting coating in displays and touch panels.
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.
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] 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] A. Bishayee, D. V. Rao, S. C. Srivastava, L. G. Bouchet, W. E. Bolch, R. W. Howell. J. Nucl. Med.41, 2043 (2000).. 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] 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] B. Ponsard, S. C. Srivastava, L. F. Mausner, F. F. Knapp, M. A. Garland, S. Mirzadeh. Appl. Radiat. Isot.67 1158 (2009)..
Tin commonly forms Sn²⁺ and Sn⁴⁺ compounds. Tin dioxide, SnO₂, is the principal ore mineral and is also used in ceramics, glass polishing, and some conductive or catalytic materials. Tin(II) chloride, SnCl₂, is a reducing agent and a reagent in plating and dyeing processes, while tin(IV) chloride, SnCl₄, is a volatile Lewis acid used in chemical synthesis and surface treatment. Organotin compounds contain Sn–C bonds; some, such as tributyltin oxide, C₂₄H₅₄OSn₂, were formerly used as biocides but are tightly restricted because of toxicity.
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.
Metallic tin has low acute toxicity and is commonly used in food-contact coatings, although excessive intake of soluble tin salts can irritate the gastrointestinal tract. Tin dusts and fumes from melting, soldering, or industrial processing can present inhalation hazards. Organotin compounds vary widely in toxicity; several are potent neurotoxic or endocrine-disrupting substances and require strict control. Radioactive tin isotopes are mainly research or fission-product concerns, not a property of natural tin as a whole.
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.
Tin is present in the crust mostly in resistant oxide minerals, especially cassiterite, and is not highly mobile under many natural surface conditions. Mining and smelting can release tin-bearing particulates and associated metals, depending on the ore and waste management. Inorganic tin compounds usually show limited bioavailability compared with many organotin compounds. Persistent organotin residues in sediments have been a major concern in harbors and shipyard areas where antifouling paints were used.
Tin is produced chiefly by mining cassiterite from hard-rock and alluvial deposits, followed by concentration, smelting, and refining. Supply is geographically concentrated in a limited number of producing regions, and some production comes from small-scale or artisanal mining. Demand is dominated by solder, tinplate, chemicals, and alloy uses. Recycling is important, especially from solder-bearing electronic scrap and tinplate residues, but recovery can be technically diffuse because tin is often present in thin coatings or complex assemblies. Substitution is possible in some coatings and solders, but performance, food-contact requirements, and processing temperatures limit replacements.
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.
Tin is a relatively heavy element made mainly by neutron-capture nucleosynthesis in earlier generations of stars. It is far less abundant cosmically than lighter rock-forming elements, but it is present in meteorites and planetary materials at trace levels. In differentiated planets, tin tends to behave as a lithophile to mildly chalcophile element, concentrating in crustal minerals and some sulfide-associated systems rather than forming abundant native metal.
- Tin has ten stable isotopes, more than any other element.
- The symbol Sn comes from the Latin name stannum.
- The crackling sound of bent tin is called tin cry and comes from crystal deformation.
- Tin pest is promoted by low temperature and can be inhibited by alloying additions.
- Most modern food cans are steel cans with a very thin tin coating, not solid tin.
- Cassiterite is dense, which makes gravity separation useful in ore concentration.
Images
Propriétés
Propriétés physiques
- Rayon atomique (empirique)
- 145 pm Comparer : Rayon atomique (empirique) de tous les éléments →
- Rayon covalent
- 139 pm Comparer : Rayon covalent de tous les éléments →
- Rayon de van der Waals
- 217 pm Comparer : Rayon de van der Waals de tous les éléments →
- Rayon métallique
- 142 pm Comparer : Rayon métallique de tous les éléments →
- Masse volumique
- 7287 kg/m³ Comparer : Masse volumique de tous les éléments →
- Volume molaire
- 0,0163 L/mol
- Phase aux CNTP
- Solide Comparer : Phase aux CNTP de tous les éléments →
- Point de fusion
- 231,93 °C Comparer : Point de fusion de tous les éléments →
- Point d’ébullition
- 2601,85 °C Comparer : Point d’ébullition de tous les éléments →
- Conductivité thermique
- 66,8 W/(m·K) Comparer : Conductivité thermique de tous les éléments →
- Capacité thermique massique
- 0,227 J/(g·K) Comparer : Capacité thermique massique de tous les éléments →
- Capacité thermique molaire
- 26,99 J/(mol·K) Comparer : Capacité thermique molaire de tous les éléments →
- Structure cristalline
- Quadratique Comparer : Structure cristalline de tous les éléments →
Propriétés chimiques
- Électronégativité (Pauling)
- 1,96 Comparer : Électronégativité (Pauling) de tous les éléments →
- Électronégativité (Allen)
- 1,824
- Affinité électronique
- 1,112 eV
- Énergie d’ionisation (1re)
- 7,343918 eV Comparer : Énergie d’ionisation (1re) de tous les éléments →
- Énergie d’ionisation (2e)
- 14,63312 eV Comparer : Énergie d’ionisation (2e) de tous les éléments →
- Énergie d’ionisation (3e)
- 30,506105 eV Comparer : Énergie d’ionisation (3e) de tous les éléments →
- Énergie d’ionisation (4e)
- 40,74014 eV Comparer : Énergie d’ionisation (4e) de tous les éléments →
- Énergie d’ionisation (5e)
- 77,030265 eV Comparer : Énergie d’ionisation (5e) de tous les éléments →
- États d’oxydation
- −4, −3, −2, −1, 0, +1, +2, +3, +4 Comparer : États d’oxydation de tous les éléments →
- Électrons de valence
- 4 Comparer : Électrons de valence de tous les éléments →
- Allotropes
- ["gray", "white"]
- Configuration électronique
- [Kr] 5s2 4d10 5p2
Propriétés thermodynamiques
- Enthalpie de fusion
- 0,07286107 eV Comparer : Enthalpie de fusion de tous les éléments →
- Enthalpie de vaporisation
- 3,067834 eV Comparer : Enthalpie de vaporisation de tous les éléments →
- Enthalpie de sublimation
- 3,131057 eV
- Enthalpie d’atomisation
- 3,131057 eV
- Enthalpie d’atomisation
- 3,121729 eV
Propriétés nucléaires
- Protons
- 50 Comparer : Protons de tous les éléments →
- Neutrons
- 70 Comparer : Neutrons de tous les éléments →
- Isotopes connus
- 42 Comparer : Isotopes connus de tous les éléments →
- Isotopes stables
- 9 Comparer : Isotopes stables de tous les éléments →
- Isotope le plus stable
- Sn-120
Abondance
- Abondance (croûte terrestre)
- 2,3 mg/kg Comparer : Abondance (croûte terrestre) de tous les éléments →
- Abondance (océan)
- 4 × 10−6 mg/L Comparer : Abondance (océan) de tous les éléments →
Structure cristalline
- Paramètre de maille a
- 582 pm
Structure électronique
- Électrons par couche
- 2, 8, 18, 18, 4 Comparer : Électrons par couche de tous les éléments →
Identifiants
- Numéro CAS
- 7440-31-5 Comparer : Numéro CAS de tous les éléments →
- Symbole de terme
- 3P0
- InChI
- InChI=1S/Sn
- Clé InChI
- ATJFFYVFTNAWJD-UHFFFAOYSA-N
Configuration électronique Mesuré
Sn: 4d¹⁰ 5s² 5p²[Kr] 4d¹⁰ 5s² 5p²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p²Modèle atomique
Les isotopes diffèrent par leur nombre de neutrons, leur masse et leur stabilité — pas par la configuration électronique de l’atome neutre.
Modèle atomique schématique, non à l’échelle.
Empreinte atomique
Spectre d’émission / d’absorption
Distribution isotopique
| Nombre de masse | Masse atomique (u) | Abondance naturelle | Demi-vie |
|---|---|---|---|
| 112 Stable | 111,90482387 ± 0,00000061 | 0,9700% | Stable |
| 114 Stable | 113,9027827 ± 0,000001 | 0,6600% | Stable |
| 115 Stable | 114,903344699 ± 0,000000016 | 0,3400% | Stable |
| 116 Stable | 115,9017428 ± 0,0000001 | 14,5400% | Stable |
| 117 Stable | 116,90295398 ± 0,00000052 | 7,6800% | Stable |
| 118 Stable | 117,90160657 ± 0,00000054 | 24,2200% | Stable |
| 119 Stable | 118,90331117 ± 0,00000078 | 8,5900% | Stable |
| 120 Stable | 119,90220163 ± 0,00000097 | 32,5800% | Stable |
Phase / État
Explication: 206,9 °C en dessous du point de fusion (231,93 °C)
Schématique, non à l’échelle
Points de transition de phase
Énergies de transition
Énergie nécessaire pour faire fondre 1 mol au point de fusion
Énergie nécessaire pour vaporiser 1 mol au point d’ébullition
Énergie nécessaire pour sublimer 1 mol au point de sublimation
Masse volumique
Dans les conditions standard
Dans les conditions standard
Spectres atomiques
Affichage de 10 sur 50. Tri par charge ionique croissante.
Raies répertoriées ?
| Ion | Charge | Nombre total de raies | Probabilités de transition | Désignations des niveaux |
|---|---|---|---|---|
| Sn I | 0 | 227 | 55 | 226 |
| Sn II | +1 | 215 | 141 | 215 |
| Sn III | +2 | 259 | 0 | 259 |
| Sn IV | +3 | 18 | 0 | 0 |
| Sn V | +4 | 13 | 0 | 0 |
Niveaux répertoriés ?
| Ion | Charge | Niveaux |
|---|---|---|
| Sn I | 0 | 228 |
| Sn II | +1 | 77 |
| Sn III | +2 | 86 |
| Sn IV | +3 | 24 |
| Sn V | +4 | 26 |
| Sn VI | +5 | 37 |
| Sn VII | +6 | 2 |
| Sn VIII | +7 | 2 |
| Sn IX | +8 | 2 |
| Sn X | +9 | 2 |
Données de structure cristalline indisponibles
Structure cristalline: tetragonal
Rayons ioniques
| Charge | Coordinence | Spin | Rayon |
|---|---|---|---|
| +4 | 4 | N/D | 55.00000000000001 pm |
| +4 | 5 | N/D | 62 pm |
| +4 | 6 | N/D | 69 pm |
| +4 | 7 | N/D | 75 pm |
| +4 | 8 | N/D | 81 pm |
Composés
Isotopes (9)
| Nombre de masse | Masse atomique (u) | Abondance naturelle | Demi-vie | Mode de désintégration | |
|---|---|---|---|---|---|
| 112 Stable | 111,90482387 ± 0,00000061 | 0,9700% ± 0,0100% | Stable | stable | |
| 114 Stable | 113,9027827 ± 0,000001 | 0,6600% ± 0,0100% | Stable | stable | |
| 115 Stable | 114,903344699 ± 0,000000016 | 0,3400% ± 0,0100% | Stable | stable | |
| 116 Stable | 115,9017428 ± 0,0000001 | 14,5400% ± 0,0900% | Stable | stable | |
| 117 Stable | 116,90295398 ± 0,00000052 | 7,6800% ± 0,0700% | Stable | stable | |
| 118 Stable | 117,90160657 ± 0,00000054 | 24,2200% ± 0,0900% | Stable | stable | |
| 119 Stable | 118,90331117 ± 0,00000078 | 8,5900% ± 0,0400% | Stable | stable | |
| 120 Stable | 119,90220163 ± 0,00000097 | 32,5800% ± 0,0900% | Stable | stable | |
| 122 Stable | 121,9034438 ± 0,0000026 | 4,6300% ± 0,0300% | Stable | stable |
Raies spectrales
Affichage de 50 sur 96. Seules les raies spectrales dont l’intensité a été mesurée sont affichées par défaut.
| Longueur d’onde (nm) | Intensité | Degré d’ionisation | Type | Transition | Précision | Source | |
|---|---|---|---|---|---|---|---|
| 556.19094 nm | 2700 | Sn II | emission | 5s2.6p 2P* → 5s2.6d 2D | Mesurée | NIST | |
| 579.88578 nm | 2700 | Sn II | emission | 5s2.5d 2D → 5s2.4f 2F* | Mesurée | NIST | |
| 558.88153 nm | 2600 | Sn II | emission | 5s2.5d 2D → 5s2.4f 2F* | Mesurée | NIST | |
| 645.35421 nm | 2500 | Sn II | emission | 5s2.6s 2S → 5s2.6p 2P* | Mesurée | NIST | |
| 452.47334 nm | 2200 | Sn I | emission | 5s2.5p2 1S → 5s2.5p.6s 1P* | Mesurée | NIST | |
| 533.23391 nm | 1600 | Sn II | emission | 5s2.6p 2P* → 5s2.6d 2D | Mesurée | NIST | |
| 607.97742 nm | 1400 | Sn II | emission | 5s2.4f 2F* → 5s2.6g 2G | Mesurée | NIST | |
| 684.41863 nm | 1300 | Sn II | emission | 5s2.6s 2S → 5s2.6p 2P* | Mesurée | NIST | |
| 719.07778 nm | 1100 | Sn II | emission | 5s2.6p 2P* → 5s2.7s 2S | Mesurée | NIST | |
| 666.11 nm | 1000 | Sn II | emission | 5s2.6d 2D → 5s2.6f 2F* | Mesurée | NIST | |
| 676.08103 nm | 840 | Sn II | emission | 5s2.6p 2P* → 5s2.7s 2S | Mesurée | NIST | |
| 656.851 nm | 830 | Sn II | emission | 5s2.9d 2D → 5s.5p.(3P*).5d 4P* | Mesurée | NIST | |
| 642.908 nm | 760 | Sn II | emission | 5s2.8s 2S → 5s.5p.(3P*).6s 2P* | Mesurée | NIST | |
| 723.005 nm | 670 | Sn II | emission | 5s2.7p 2P* → 5s2.8d 2D | Mesurée | NIST | |
| 690.47 nm | 538 | Sn III | emission | 4d10.5s.6d 3D → 4d10.5s.5f 3F* | Mesurée | NIST | |
| 731.417 nm | 500 | Sn II | emission | 5s2.7d 2D → 5s.5p.(3P*).6s 2P* | Mesurée | NIST | |
| 579.69075 nm | 490 | Sn II | emission | 5s2.5d 2D → 5s2.4f 2F* | Mesurée | NIST | |
| 707.93 nm | 485 | Sn III | emission | 4d10.5s.6d 3D → 4d10.5s.5f 3F* | Mesurée | NIST | |
| 738.71637 nm | 480 | Sn II | emission | 5s.5p2 2D → 5s2.6p 2P* | Mesurée | NIST | |
| 529.083 nm | 448 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 384.13749 nm | 440 | Sn II | emission | 5s2.6p 2P* → 5s2.8s 2S | Mesurée | NIST | |
| 536.929 nm | 421 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 601.34 nm | 419 | Sn III | emission | 4d10.5s.6s 1S → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 624.113 nm | 380 | Sn II | emission | 5s2.6d 2D → 5s2.9p 2P* | Mesurée | NIST | |
| 740.827 nm | 380 | Sn II | emission | 5s2.7p 2P* → 5s2.8d 2D | Mesurée | NIST | |
| 719.9 nm | 373 | Sn III | emission | 4d10.5s.7p 3P* → 4d10.5s.7d 1D | Mesurée | NIST | |
| 507.26 nm | 360 | Sn II | emission | 5s2.4f 2F* → 5s2.7g 2G | Mesurée | NIST | |
| 429.433 nm | 340 | Sn II | emission | 5s2.4f 2F* → 5s2.9g 2G | Mesurée | NIST | |
| 433.013 nm | 309 | Sn III | emission | 4d10.5s.6s 3S → 4d10.5s.6p 1P* | Mesurée | NIST | |
| 502.038 nm | 302 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 534.881 nm | 271 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 563.16738 nm | 270 | Sn I | emission | 5s2.5p2 1S → 5s2.5p.6s 3P* | Mesurée | NIST | |
| 467.046 nm | 241 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 1P* | Mesurée | NIST | |
| 396.169 nm | 231 | Sn III | emission | 4d10.5s.6p 3P* → 4d10.5s.7s 3S | Mesurée | NIST | |
| 522.464 nm | 225 | Sn III | emission | 4d10.5s.6s 1S → 4d10.5s.6p 1P* | Mesurée | NIST | |
| 411.13 nm | 180 | Sn II | emission | 5s2.4f 2F* → 5s2.10g 2G | Mesurée | NIST | |
| 390.698 nm | 170 | Sn III | emission | 4d10.5s.5d 1D → 4d10.4f.5s 1F* | Mesurée | NIST | |
| 471.558 nm | 164 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 1P* | Mesurée | NIST | |
| 494.42561 nm | 150 | Sn II | emission | 5s2.5d 2D → 5s2.7p 2P* | Mesurée | NIST | |
| 510.022 nm | 145 | Sn III | emission | 4d10.5s.5d 3D → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 458.025 nm | 140 | Sn II | emission | 5s2.4f 2F* → 5s2.8g 2G | Mesurée | NIST | |
| 614.96038 nm | 140 | Sn I | emission | 5s2.5p.6s 3P* → 5s2.5p.7p 3D | Mesurée | NIST | |
| 492.435 nm | 131 | Sn III | emission | 4d10.5s.6s 3S → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 457.432 nm | 120 | Sn II | emission | 5s2.4f 2F* → 5s2.10d 2D | Mesurée | NIST | |
| 487.7209 nm | 100 | Sn II | emission | 5s2.5d 2D → 5s2.7p 2P* | Mesurée | NIST | |
| 606.91169 nm | 95 | Sn I | emission | 5s2.5p.6s 3P* → 5s2.5p.7p 3P | Mesurée | NIST | |
| 457.553 nm | 91 | Sn II | emission | 5s2.4f 2F* → 5s2.10d 2D | Mesurée | NIST | |
| 461.82363 nm | 90 | Sn II | emission | 5s.5p2 4P → 5s2.6p 2P* | Mesurée | NIST | |
| 485.827 nm | 89 | Sn III | emission | 4d10.5s.6s 3S → 4d10.5s.6p 3P* | Mesurée | NIST | |
| 491.78 nm | 83 | Sn II | emission | 5s2.7p 2P* → 5s2.11d 2D | Mesurée | NIST |
Propriétés étendues
Rayons covalents (données étendues)
- Rayon covalent (Pyykkö)
- 140 pm
- Rayon covalent (Pyykkö, liaison double)
- 130 pm
- Rayon covalent (Pyykkö, liaison triple)
- 132 pm
- Rayon covalent (Bragg)
- 140 pm
Rayons de van der Waals
- Bondi
- 217 pm
- Batsanov
- 225 pm
- Alvarez
- 242 pm
- UFF
- 439,2 pm
- MM3
- 259 pm
- Dreiding
- 447 pm
Rayons atomiques et métalliques
- Rayon atomique (Rahm)
- 248 pm
- Rayon métallique (C12)
- 163 pm
Échelles de numérotation
- Mendeleev
- 90
- Pettifor
- 83
- Glawe
- 83
Échelles d’électronégativité
- Ghosh
- 0
- Miedema
- 4
- Gunnarsson–Lundqvist
- 5
- Robles–Bartolotti
- 4
Polarisabilité et dispersion
- Polarisabilité dipolaire
- 53 a.u.
- Polarisabilité dipolaire (incertitude)
- 6 a.u.
- C₆
- 659 Ha·Bohr6
- C₆ (Gould–Bučko)
- 715 Ha·Bohr6
Paramètres de Miedema
- Volume molaire de Miedema
- 16,3 cm3/mol
- Densité électronique de Miedema
- 2
Risque d’approvisionnement et économie
- Concentration de la production
- 46
- Risque relatif d’approvisionnement
- 7
- Répartition des réserves
- 31
- Stabilité politique (principal producteur)
- 24
- Stabilité politique (principal détenteur de réserves)
- 24
Transitions de phase et allotropes
| Température de transition | 286,35 K |
| Point d’ébullition | 2859,15 K |
| Point de fusion | 505,08 K |
| Point d’ébullition | 2859,15 K |
Catégories d’états d’oxydation
Données de référence avancées
Constantes d’écran (11)
| n | Orbitale | σ |
|---|---|---|
| 1 | s | 1,008 |
| 2 | p | 4,1146 |
| 2 | s | 13,1406 |
| 3 | d | 14,2583 |
| 3 | p | 17,6468 |
| 3 | s | 17,5802 |
| 4 | d | 32,03 |
| 4 | p | 28,7348 |
| 4 | s | 27,342 |
| 5 | p | 40,898 |
Détail des rayons cristallins (5)
| Charge | CN | Spin | rcrystal (pm) | Origine |
|---|---|---|---|---|
| 4 | IV | 69 | from r^3 vs V plots, | |
| 4 | V | 76 | calculated, | |
| 4 | VI | 83 | from r^3 vs V plots, | |
| 4 | VII | 89 | ||
| 4 | VIII | 95 | calculated, |
Modes de désintégration des isotopes (54)
| Isotope | Mode | Intensité |
|---|---|---|
| 99 | B+ | 100% |
| 99 | B+p | 5% |
| 100 | B+ | 100% |
| 100 | B+p | 17% |
| 101 | B+ | 100% |
| 101 | B+p | 21% |
| 102 | B+ | 100% |
| 103 | B+ | 100% |
| 103 | B+p | 1,2% |
| 104 | B+ | 100% |
Facteurs de diffusion des rayons X (510)
| Énergie (eV) | f₁ | f₂ |
|---|---|---|
| 10 | — | 3,97344 |
| 10,1617 | — | 3,94095 |
| 10,3261 | — | 3,90871 |
| 10,4931 | — | 3,87675 |
| 10,6628 | — | 3,84504 |
| 10,8353 | — | 3,81359 |
| 11,0106 | — | 3,7824 |
| 11,1886 | — | 3,75146 |
| 11,3696 | — | 3,72078 |
| 11,5535 | — | 3,64688 |
Données complémentaires
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
2.3 milligrams per kilogram
Références (1)
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
4×10-6 milligrams per liter
Références (1)
Sources
Sources of this element.
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.
Références (1)
Références
(9)
Data deposited in or computed by PubChem
The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.
Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.
The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.
Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/
The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.
The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database
This section provides all form of data related to element Tin.
The element property data was retrieved from publications.