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S 16

Sulfur (S)

nonmetal
Período: 3 Grupo: 16 Bloco: p

Solid

Peso atômico padrão

32,06 u [32,059, 32,076]

Configuração eletrônica

[Ne] 3s2 3p4

Ponto de fusão

115,21 °C

Ponto de ebulição

444,6 °C

Densidade

2067 kg/m³

Estados de oxidação

−2, −1, 0, +1, +2, +3, +4, +5, +6

Eletronegatividade (Pauling)

2,58

Energia de ionização (1ª)

10,360017 eV

Ano da descoberta

1777

Raio atômico

100 pm

Detalhes

Origem do nome Latin: sulphur (brimstone).
Descobridores Known to the ancients.

Sulfur is a reactive nonmetal in group 16, occurring naturally as elemental sulfur and in sulfide and sulfate minerals. It forms many allotropes and a large range of compounds, especially with oxygen, hydrogen, metals, and organic groups. Its chemistry is central to fertilizers, petroleum refining, vulcanized rubber, and biological molecules such as amino acids and cofactors.

Sulfur is pale yellow, odorless, brittle solid, which is insoluble in water but soluble in carbon disulfide. In every state, whether gas, liquid or solid, elemental sulfur occurs in more than one allotropic form or modification; these present a confusing multitude of forms whose relations are not yet fully understood.

In 1975, University of Pennsylvania scientists reported synthesis of polymeric sulfur nitride, which has the properties of a metal, although it contains no metal atoms. The material has unusual optical and electrical properties.

High-purity sulfur is commercially available in purities of 99.999+%.

Amorphous or "plastic" sulfur is obtained by fast cooling of the crystalline form. X-ray studies indicate that amorphous sulfur may have a helical structure with eight atoms per spiral. Crystalline sulfur seems to be made of rings, each containing eight sulfur atoms, which fit together to give a normal X-ray pattern.

The name derives from the Latin sulphurium and the Sanskrit sulveri. Sulfur was known as brenne stone for "combustible stone" from which brim-stone is derived. It was known from prehistoric times and thought to contain hydrogen and oxygen. In 1809, the French chemists Louis-Joseph Gay-Lussac and Louis-Jacques Thenard proved the elemental nature of sulfur.

Sulfur, the tenth most abundant element in the universe, has been known since ancient times. Sometime around 1777, Antoine Lavoisier convinced the rest of the scientific community that sulfur was an element. Sulfur is a component of many common minerals, such as galena (PbS), gypsum (CaSO4·2(H2O), pyrite (FeS2), sphalerite (ZnS or FeS), cinnabar (HgS), stibnite (Sb2S3), epsomite (MgSO4·7(H2O)), celestite (SrSO4) and barite (BaSO4). Nearly 25% of the sulfur produced today is recovered from petroleum refining operations and as a byproduct of extracting other materials from sulfur containing ores. The majority of the sulfur produced today is obtained from underground deposits, usually found in conjunction with salt deposits, with a process known as the Frasch process. Sulfur is a pale yellow, odorless and brittle material. It displays three allotropic forms: orthorhombic, monoclinic and amorphous. The orthorhombic form is the most stable form of sulfur. Monoclinic sulfur exists between the temperatures of 96°C and 119°C and reverts back to the orthorhombic form when cooled. Amorphous sulfur is formed when molten sulfur is quickly cooled. Amorphous sulfur is soft and elastic and eventually reverts back to the orthorhombic form.

Known to the ancients; referred to in Genesis as brimstone.

Imagens

Propriedades

Química

Eletronegatividade (Pauling)
2,58 Comparar Eletronegatividade (Pauling) de todos os elementos →
Eletronegatividade (Allen)
2,589
Afinidade eletrônica
2,0771 eV
Energia de ionização (1ª)
10,360017 eV Comparar Energia de ionização (1ª) de todos os elementos →
Energia de ionização (2ª)
23,33796 eV Comparar Energia de ionização (2ª) de todos os elementos →
Energia de ionização (3ª)
34,86012 eV Comparar Energia de ionização (3ª) de todos os elementos →
Energia de ionização (4ª)
47,222163 eV Comparar Energia de ionização (4ª) de todos os elementos →
Energia de ionização (5ª)
72,59475 eV Comparar Energia de ionização (5ª) de todos os elementos →
Estados de oxidação
−2, −1, 0, +1, +2, +3, +4, +5, +6 Comparar Estados de oxidação de todos os elementos →
Elétrons de valência
6 Comparar Elétrons de valência de todos os elementos →
Alótropos
["monoclinic", "rhombic"]
Configuração eletrônica
[Ne] 3s2 3p4

Termodinâmica

Ponto crítico (temperatura)
1041 °C
Ponto crítico (pressão)
2,07e+7 Pa
Calor de fusão
0,01793025 eV Comparar Calor de fusão de todos os elementos →
Calor de vaporização
0,46639374 eV Comparar Calor de vaporização de todos os elementos →
Calor de sublimação
2,870913 eV
Calor de atomização
2,870913 eV
Entalpia de atomização
2,872675 eV

Abundância

Abundância (crosta terrestre)
350 mg/kg Comparar Abundância (crosta terrestre) de todos os elementos →
Abundância (oceano)
905 mg/L Comparar Abundância (oceano) de todos os elementos →

Estrutura cristalina

Constante de rede a
1047 pm

Estrutura eletrônica

Elétrons por camada
2, 8, 6 Comparar Elétrons por camada de todos os elementos →

Identificadores

Número CAS
7704-34-9 Comparar Número CAS de todos os elementos →
Símbolo de termo
3P2
InChI
InChI=1S/S
Chave InChI
NINIDFKCEFEMDL-UHFFFAOYSA-N

Configuração eletrônica Medido

Carga do íon
Prótons 16
Elétrons 16
Carga Neutro
Configuração S: 3s² 3p⁴
Configuração eletrônica
Medido
[Ne] 3s² 3p⁴
1s² 2s² 2p⁶ 3s² 3p⁴
Diagrama de orbitais
1s
2/2
2s
2/2
2p
6/6
3s
2/2
3p
4/6 2↑
Total de elétrons: 16 Desemparelhados: 2 ?

Modelo atômico

Prótons 16
Nêutrons 16
Elétrons 16
Número de massa 32
Estabilidade Estável

Os isótopos alteram o número de nêutrons, a massa e a estabilidade — não a configuração eletrônica de um átomo neutro.

Modelo atômico esquemático, sem escala.

Assinatura atômica

Espectro de emissão / absorção

25 / 50 (50 50 com intensidade)
Medido
Emissão Visível: 380–750 nm

Distribuição isotópica

3294,9900%344,2500%330,7500%360,0100%Número de massaAbundância natural (%)
Número de massaMassa atômica (u)Abundância naturalMeia-vida
32 Estável31,9720711744 ± 0,000000001494,9900%Estável
33 Estável32,9714589098 ± 0,00000000150,7500%Estável
34 Estável33,967867004 ± 0,0000000474,2500%Estável
36 Estável35,96708071 ± 0,00000020,0100%Estável
Medido

Fase / Estado

1 atm / 101,325 kPa
Sólido 25 °C (298,15 K)

Motivo: 90,2 °C abaixo do ponto de fusão (115,21 °C)

Ponto de fusão 115,21 °C
Ponto de ebulição 444,6 °C
Abaixo do ponto de fusão em 90,2 °C
0 K Temperatura atual: 25 °C 6000 K
Linha do tempo das fases

Esquemático, sem escala

Sólido
Líquido
Gás
Fusão
Ebulição
25°C
Sólido
Líquido
Gás
Atual

Pontos de transição de fase

Ponto de fusão Literatura
115,21 °C
Ponto de ebulição Literatura
444,6 °C
Fase atual Calculado
Sólido

Energias de transição

Calor de fusão Literatura
0,01793025 eV

Energia necessária para fundir 1 mol no ponto de fusão

Calor de vaporização Literatura
0,46639374 eV

Energia necessária para vaporizar 1 mol no ponto de ebulição

Calor de sublimação Literatura
2,870913 eV

Energia necessária para sublimar 1 mol no ponto de sublimação

Densidade

Densidade de referência Literatura
2067 kg/m³

Em condições padrão

Densidade atual Calculado
2067 kg/m³

Em condições padrão

Avançado

Ponto crítico Literatura
1041 °C

Espectros atômicos

Mostrando 10 de 16. Ordenado por carga do íon (ordem crescente).

Dados de linhas disponíveis ?

ÍonCargaTotal de linhasProbabilidades de transiçãoDesignações dos níveis
S I 0143710521429
S II +113497531349
S III +2329273329
S IV +311999991199
S V +4866699866
S VI +5457393457
S VII +6259253255
S VIII +7254253254
S IX +8175175175
S X +9270268270
Dados de linhas disponíveis no NIST →

Dados de níveis disponíveis ?

ÍonCargaNíveis
S I 0382
S II +1247
S III +259
S IV +3142
S V +4150
S VI +588
S VII +657
S VIII +754
S IX +845
S X +944
Dados de níveis disponíveis no NIST →
16 S 32.067499999999995

Sulfur — Visualizador de orbitais atômicos

[Ne]3s23p4
Níveis de energia 2 8 6
Estados de oxidação -2, -1, 0, +1, +2, +3, +4, +5, +6
HOMO 3p n=3 · l=1 · m=-1
Sulfur — Prévia do visualizador de orbitais atômicos
O Three.js é carregado apenas quando solicitado
16 S 32.067499999999995

Sulfur — Visualizador de estruturas cristalinas

Orthorhombic · Pearson N/A
Experimental
Pearson N/A
Sulfur — Prévia do visualizador de estruturas cristalinas
O Three.js é carregado apenas quando solicitado

Raios iônicos

CargaCoordenaçãoSpinRaio
-26N/D184 pm
+46N/D37 pm
+64N/D12 pm
+66N/D28.999999999999996 pm

Compostos

S
32,070 u
S-2
32,070 u
S-
32,070 u
S-2
33,968 u
S
33,968 u
S
32,971 u
S
31,972 u
S-2
34,969 u

Isótopos (4)

Eleven isotopes of sulfur exist. None of the four isotopes that are found in nature are radioactive. A finely divided form of sulfur, known as flowers of sulfur, is obtained by sublimation.

Número de massaMassa atômica (u)Abundância naturalMeia-vidaModo de decaimento
32 Estável31,9720711744 ± 0,000000001494,9900% ± 0,2600%Estável
stable
33 Estável32,9714589098 ± 0,00000000150,7500% ± 0,0200%Estável
stable
34 Estável33,967867004 ± 0,0000000474,2500% ± 0,2400%Estável
stable
36 Estável35,96708071 ± 0,00000020,0100% ± 0,0100%Estável
stable
32 Estável
Massa atômica (u) 31,9720711744 ± 0,0000000014
Abundância natural 94,9900% ± 0,2600%
Meia-vida Estável
Modo de decaimento
stable
33 Estável
Massa atômica (u) 32,9714589098 ± 0,0000000015
Abundância natural 0,7500% ± 0,0200%
Meia-vida Estável
Modo de decaimento
stable
34 Estável
Massa atômica (u) 33,967867004 ± 0,000000047
Abundância natural 4,2500% ± 0,2400%
Meia-vida Estável
Modo de decaimento
stable
36 Estável
Massa atômica (u) 35,96708071 ± 0,0000002
Abundância natural 0,0100% ± 0,0100%
Meia-vida Estável
Modo de decaimento
stable

Linhas espectrais

Mostrando 50 de 556. Por padrão, são mostradas apenas as linhas espectrais com intensidade medida.

Comprimento de onda (nm)IntensidadeEstágio de ionizaçãoTipoTransiçãoExatidãoFonte
545.3853 nm42000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4D*MedidaNIST
543.2797 nm30000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4D*MedidaNIST
416.2665 nm25000S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).4d 4FMedidaNIST
532.0715 nm24000S IIemission3s2.3p2.(1D).4s 2D → 3s2.3p2.(1D).4p 2F*MedidaNIST
415.3066 nm20000S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).4d 4FMedidaNIST
503.2435 nm20000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4P*MedidaNIST
542.8658 nm20000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4D*MedidaNIST
547.3617 nm20000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4D*MedidaNIST
550.9702 nm20000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4D*MedidaNIST
560.6158 nm20000S IIemission3s2.3p2.(3P).3d 4F → 3s2.3p2.(3P).4p 4D*MedidaNIST
563.998 nm20000S IIemission3s2.3p2.(3P).4s 2P → 3s2.3p2.(3P).4p 2D*MedidaNIST
414.5059 nm16000S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).4d 4FMedidaNIST
429.44 nm16000S IIemission3s2.3p2.(3P).4p 4P* → 3s2.3p2.(3P).4d 4DMedidaNIST
481.5553 nm16000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4S*MedidaNIST
534.5715 nm16000S IIemission3s2.3p2.(1D).4s 2D → 3s2.3p2.(1D).4p 2F*MedidaNIST
393.326 nm13000S IIemission3s2.3p2.(3P).4p 2D* → 3s2.3p2.(3P).4d 2FMedidaNIST
402.875 nm13000S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).4d 4DMedidaNIST
414.2259 nm13000S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).4d 4FMedidaNIST
417.4266 nm13000S IIemission3s2.3p2.(1D).4p 2F* → 3s2.3p2.(1D).4d 2GMedidaNIST
426.7762 nm13000S IIemission3s2.3p2.(3P).4p 4P* → 3s2.3p2.(3P).4d 4DMedidaNIST
452.4942 nm13000S IIemission3s2.3p2.(1D).4s 2D → 3s2.3p2.(1D).4p 2P*MedidaNIST
500.9564 nm13000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4P*MedidaNIST
501.4044 nm13000S IIemission3s2.3p2.(3P).4s 2P → 3s2.3p2.(3P).4p 2P*MedidaNIST
521.2614 nm13000S IIemission3s2.3p2.(1D).4s 2D → 3s2.3p2.(1D).4p 2D*MedidaNIST
630.5479 nm13000S IIemission3s2.3p2.(3P).3d 4D → 3s2.3p2.(3P).4p 4P*MedidaNIST
556.4958 nm12000S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4D*MedidaNIST
564.0336 nm12000S IIemission3s2.3p2.(3P).3d 4F → 3s2.3p2.(3P).4p 4D*MedidaNIST
564.6998 nm12000S IIemission3s2.3p2.(3P).4s 2P → 3s2.3p2.(3P).4p 2D*MedidaNIST
565.9998 nm12000S IIemission3s2.3p2.(3P).3d 4F → 3s2.3p2.(3P).4p 4D*MedidaNIST
628.6951 nm12000S IIemission3s2.3p2.(3P).3d 2F → 3s2.3p2.(3P).4p 2D*MedidaNIST
392.3449 nm10000S IIemission3s2.3p2.(3P).4p 2D* → 3s2.3p2.(3P).4d 2FMedidaNIST
446.358 nm10000S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).5s 4PMedidaNIST
639.7363 nm10000S IIemission3s2.3p2.(3P).3d 4D → 3s2.3p2.(3P).4p 4P*MedidaNIST
471.6272 nm9900S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4S*MedidaNIST
499.1968 nm9800S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4P*MedidaNIST
502.72 nm9800S IIemission3s2.3p2.(3P).3d 2P → 3s2.3p2.(3P).4p 2S*MedidaNIST
520.1025 nm9800S IIemission3s2.3p2.(1D).4s 2D → 3s2.3p2.(1D).4p 2D*MedidaNIST
566.4773 nm9700S IIemission3s2.3p2.(3P).3d 4F → 3s2.3p2.(3P).4p 4D*MedidaNIST
631.2666 nm7900S IIemission3s2.3p2.(3P).3d 2F → 3s2.3p2.(3P).4p 2D*MedidaNIST
399.3499 nm7800S IIemission3s2.3p2.(3P).3d 2F → 3s2.3p2.(1D).4p 2F*MedidaNIST
403.2767 nm7800S IIemission3s2.3p2.(3P).4p 4S* → 3s2.3p2.(3P).4d 4PMedidaNIST
417.4001 nm7700S IIemission3s2.3p2.(1D).4p 2F* → 3s2.3p2.(1D).4d 2GMedidaNIST
446.443 nm7700S IIemission3s2.3p2.(1D).3d 2F → 3s2.3p2.(3P<2>).4f 2[5]*MedidaNIST
448.3428 nm7700S IIemission3s2.3p2.(3P).4p 4D* → 3s2.3p2.(3P).5s 4PMedidaNIST
465.6762 nm7700S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4S*MedidaNIST
491.7197 nm7600S IIemission3s2.3p2.(3P).4s 2P → 3s2.3p2.(3P).4p 2P*MedidaNIST
492.5347 nm7600S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4P*MedidaNIST
510.3332 nm7600S IIemission3s2.3p2.(3P).4s 4P → 3s2.3p2.(3P).4p 4P*MedidaNIST
581.9238 nm7500S IIemission3s2.3p2.(3P).4s 2P → 3s2.3p2.(3P).4p 2D*MedidaNIST
639.8015 nm7500S IIemission3s2.3p2.(3P).3d 4D → 3s2.3p2.(3P).4p 4P*MedidaNIST

Propriedades ampliadas

Raios covalentes (dados ampliados)

Raio covalente (Pyykkö)
103 pm
Raio covalente (Pyykkö, ligação dupla)
94 pm
Raio covalente (Pyykkö, ligação tripla)
95 pm
Raio covalente (Bragg)
102 pm

Raios de van der Waals

Bondi
180 pm
Batsanov
180 pm
Alvarez
189 pm
UFF
403,5 pm
MM3
215 pm
Dreiding
403 pm
Rowland–Taylor
181 pm

Raios atômicos e metálicos

Raio atômico (Rahm)
214 pm
Raio metálico (C12)
127 pm

Escalas de numeração

Mendeleev
100
Pettifor
94
Glawe
96

Escalas de eletronegatividade

Ghosh
0
Gunnarsson–Lundqvist
6
Robles–Bartolotti
5

Polarizabilidade e dispersão

Polarizabilidade dipolar
19,4 a.u.
Polarizabilidade dipolar (incerteza)
0,1 a.u.
C₆
134 Ha·Bohr6
C₆ (Gould–Bučko)
140 Ha·Bohr6

Afinidade química

Afinidade protônica
664,3 kJ/mol
Basicidade em fase gasosa
640,2 kJ/mol

Risco de abastecimento e economia

Concentração da produção
17
Risco relativo de abastecimento
4
Estabilidade política (maior produtor)
24

Transições de fase e alótropos

rhombic
Temperatura de transição368,35 K
Ponto de ebulição717,76 K
Ponto crítico (temperatura)1314,15 K
Ponto crítico (pressão)20,7 MPa
monoclinic
Ponto de fusão388,36 K
Ponto de ebulição717,76 K
Ponto crítico (temperatura)1314,15 K

Categorias de estados de oxidação

+2 main
0 extended
+1 extended
+3 extended
+5 extended
+4 main
+6 main
−1 extended
−2 main

Dados de referência avançados

Constantes de blindagem (5)
nOrbitalσ
1s0,4591
2p4,023
2s5,3712
3p10,5181
3s9,6331
Detalhes dos raios cristalinos (4)
CargaCNSpinrcrystal (pm)Origem
-2VI170Pauling's (1960) crystal radius,
4VI51Ahrens (1952) ionic radius,
6IV26
6VI43calculated,
Modos de decaimento dos isótopos (38)
IsótopoModoIntensidade
262p—
27B+100%
27B+p61%
272p3%
28B+100%
28B+p20,7%
29B+100%
29B+p46,4%
30B+100%
31B+100%
Fatores de espalhamento de raios X (504)
Energia (eV)f₁f₂
10—4,05213
10,1617—4,23511
10,3261—4,42637
10,4931—4,62625
10,6628—4,83517
10,8353—5,05351
11,0106—5,28172
11,1886—5,52024
11,3696—5,79892
11,5535—6,15554

Dados adicionais

Sources

Sources of this element.

Sulfur is found in meteorites. R.W. Wood suggests that the dark area near the crater Aristarchus is a sulfur deposit.

Sulfur occurs native in the vicinity of volcanos and hot springs. It is widely distributed in nature as iron pyrites, galena, sphalerite, cinnabar, stibnite, gypsum, epsom salts, celestite, barite, etc.

Referências (1)

Production

Production of this element (from raw materials or other compounds containing the element).

Sulfur is commercially recovered from wells sunk into the salt domes along the Gulf Coast of the U.S. Using the Frasch process heated water is forced into the wells to melt the sulfur, which is then brought to the surface.

Sulfur also occurs in natural gas and petroleum crudes and must be removed from these products. Formerly this was done chemically, which wasted the sulfur; new processes now permit recovery. Large amounts of sulfur are being recovered from Alberta gas fields.

Referências (1)

Isotopes in Forensic Science and Anthropology

Information on the use of this element's isotopes in forensic science and anthropology.

The isotope-amount ratio n(34S)/n(32S) can be used to authenticate the dietary source of cattle. First, stable isotopes are measured to infer the dietary source of the cattle. Once the source of the diet is found, the isotopic compositions can be traced in certain muscle groups of the cattle and can be used to determine if the diet of the animal has been changed or if the feed is consistent with what the animal has been claimed to have been fed [145] B. Bahar, A. P. Moloney, F. J. Monahan, S. M. Harrison, A. Zazzo, C. M. Scrimgeour, I. S. Begley, O. Schmidt. J. Anim. Sci.87, 905 (2009)..

Referências (2)
  • [145] B. Bahar, A. P. Moloney, F. J. Monahan, S. M. Harrison, A. Zazzo, C. M. Scrimgeour, I. S. Begley, O. Schmidt. J. Anim. Sci.87, 905 (2009).
  • [4] IUPAC Periodic Table of the Elements and Isotopes (IPTEI) https://doi.org/10.1515/pac-2015-0703

Referências

(9)
2 Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
S

The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.

3 IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
Sulfur

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.

4 IUPAC Periodic Table of the Elements and Isotopes (IPTEI)

The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.

Nota sobre a licença: 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.
5 Jefferson Lab, U.S. Department of Energy
Sulfur

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/

Nota sobre a licença: Please see citation and linking information: https://education.jlab.org/faq/index.html
6 Los Alamos National Laboratory, U.S. Department of Energy
Sulfur

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.

7 NIST Physical Measurement Laboratory
Sulfur

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

8 PubChem Elements
Sulfur

This section provides all form of data related to element Sulfur.

9 PubChem Elements
Sulfur

The element property data was retrieved from publications.

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