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Tánganran

Lát'ọwọ́ Wikipedia, ìwé ìmọ̀ ọ̀fẹ́
Chemical element with atomic number 50Àdàkọ:SHORTDESC:Chemical element with atomic number 50
Tin, 50Sn
Tin
Ìhànsójúsilvery lustrous gray
Ìwúwo átọ̀mù Ar, std(Sn)118.710(7)[1]
Tin ní orítábìlì àyè
HydrogenHelium
LithiumBerylliumBoronCarbonNitrogenOxygenFluorineNeon
SodiumMagnesiumAluminiumSiliconPhosphorusSulfurChlorineArgon
PotassiumCalciumScandiumTitaniumVanadiumChromiumManganeseIronCobaltNickelCopperZincGalliumGermaniumArsenicSeleniumBromineKrypton
RubidiumStrontiumYttriumZirconiumNiobiumMolybdenumTechnetiumRutheniumRhodiumPalladiumSilverCadmiumIndiumTinAntimonyTelluriumIodineXenon
CaesiumBariumLanthanumCeriumPraseodymiumNeodymiumPromethiumSamariumEuropiumGadoliniumTerbiumDysprosiumHolmiumErbiumThuliumYtterbiumLutetiumHafniumTantalumTungstenRheniumOsmiumIridiumPlatinumGoldMercury (element)ThalliumLeadBismuthPoloniumAstatineRadon
FranciumRadiumActiniumThoriumProtactiniumUraniumNeptuniumPlutoniumAmericiumCuriumBerkeliumCaliforniumEinsteiniumFermiumMendeleviumNobeliumLawrenciumRutherfordiumDubniumSeaborgiumBohriumHassiumMeitneriumDarmstadtiumRoentgeniumCoperniciumNihoniumFleroviumMoscoviumLivermoriumTennessineOganesson
Ge
↑
Sn
↓
Pb
indium ←tin →antimony
Nọ́mbà átọ̀mù(Z)50
Ẹgbẹ́group 14 (carbon group)
Àyèàyè 5
Àdìpọ̀Àdìpọ̀-p
Ẹ̀ka ẹ́límẹ́ntì Post-transition metal
Ìtò ẹ̀lẹ́ktrọ́nù[Kr] 4d10 5s2 5p2
Iye ẹ̀lẹ́ktrọ́nù lórí ìpele kọ̀ọ̀kan2, 8, 18, 18, 4
Àwọn ohun ìní ara
Ìfarahànat STPsolid
Ìgbà ìyọ́505.08 K ​(231.93 °C, ​449.47 °F)
Ígbà ìhó2875 K ​(2602 °C, ​4716 °F)
Kíki (near r.t.)(white) 7.365 g/cm3
(gray) 5.769 g/cm3
when liquid (at m.p.)6.99 g/cm3
Heat of fusion(white) 7.03 kJ/mol
Heat of(white) 296.1 kJ/mol
Molar heat capacity(white) 27.112 J/(mol·K)
 pressure
P (Pa)1101001 k10 k100 k
at T (K)149716571855210724382893
Atomic properties
Oxidation states−4, −3, −2, −1, 0,[2] +1,[3]+2, +3,[4]+4Àdàkọ:Infobox element/symbol-to-oxidation-state/comment
ElectronegativityPauling scale: 1.96
Atomic radiusempirical: 140 pm
Covalent radius139±4 pm
Van der Waals radius217 pm
Color lines in a spectral range
Color lines in a spectral range
Spectral lines of tin
Other properties
Natural occurrenceprimordial
Crystal structure ​Tetragonal (white),diamond cubic (gray)
Thermal expansion22.0 µm/(m·K) (at 25 °C)
Thermal conductivity66.8 W/(m·K)
Electrical resistivity115 n Ω·m (at 0 °C)
Magnetic ordering(gray)diamagnetic[5], (white)paramagnetic
Young's modulus50 GPa
Shear modulus18 GPa
Bulk modulus58 GPa
Poisson ratio0.36
Mohs hardness1.5
Brinell hardness51 MPa
CAS Number7440-31-5
Mainisotopes of tin
Iso­topeAbun­danceHalf-life(t1/2)Decay modePro­duct
112Sn0.97%112Sn isstable with 62neutrons
114Sn0.66%114Sn isstable with 64neutrons
115Sn0.34%115Sn isstable with 65neutrons
116Sn14.54%116Sn isstable with 66neutrons
117Sn7.68%117Sn isstable with 67neutrons
118Sn24.22%118Sn isstable with 68neutrons
119Sn8.59%119Sn isstable with 69neutrons
120Sn32.58%120Sn isstable with 70neutrons
122Sn4.63%122Sn isstable with 72neutrons
124Sn5.79%124Sn isstable with 74neutrons
126Sntrace2.3×105yβ−0.380126Sb
Àdàkọ:Category-inline
| references

Tin jeIpilese elegbogi pelu ami-idamoSn (Látìnì:Stannum) atinomba atomu 50.

Àyọkà yìí tàbí apá rẹ̀ únfẹ́ àtúnṣe sí.

Ẹ lefẹ̀ jù báyìí lọ tàbí kí ẹṣàtúnṣe rẹ̀ lọ́nà tí yíò mu kúnrẹ́rẹ́. Ẹ ran Wikipedia lọ́wọ́ látifẹ̀ẹ́ jù báyìí lọ.

Itokasi

[àtúnṣe |àtúnṣe àmìọ̀rọ̀]
  1. ↑Meija, Juris; Coplen, Tyler B.; Berglund, Michael; Brand, Willi A.; De Bièvre, Paul; Gröning, Manfred; Holden, Norman E.; Irrgeher, Johanna et al. (2016). "Atomic weights of the elements 2013 (IUPAC Technical Report)". Pure and Applied Chemistry 88 (3): 265–91. doi:10.1515/pac-2015-0305. 
  2. ↑"New Type of Zero-Valent Tin Compound".Chemistry Europe. 27 August 2016. 
  3. ↑"HSn".NIST Chemistry WebBook. National Institute of Standards and Technology. Retrieved23 January 2013. 
  4. ↑"SnH3".NIST Chemistry WebBook. National Institure of Standards and Technology. Retrieved23 January 2013. 
  5. ↑Magnetic susceptibility of the elements and inorganic compounds, in Handbook of Chemistry and Physics 81st edition, CRC press.
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