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S 16

Sulfur (S)

nonmetal
Periodo: 3 Grupo: 16 Bloque: p

Solid

Peso atómico estándar

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

Configuración electrónica

[Ne] 3s2 3p4

Punto de fusión

115,21 °C

Punto de ebullición

444,6 °C

Densidad

2067 kg/m³

Estados de oxidación

−2, −1, 0, +1, +2, +3, +4, +5, +6

Electronegatividad (Pauling)

2,58

Energía de ionización (1.ª)

10,360017 eV

Año de descubrimiento

1777

Radio atómico

100 pm

Detalles

Origen del nombre Latin: sulphur (brimstone).
Descubridores 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.

Imágenes

Propiedades

Químicas

Electronegatividad (Pauling)
2,58 Comparar Electronegatividad (Pauling) de todos los elementos →
Electronegatividad (Allen)
2,589
Afinidad electrónica
2,0771 eV
Energía de ionización (1.ª)
10,360017 eV Comparar Energía de ionización (1.ª) de todos los elementos →
Energía de ionización (2.ª)
23,33796 eV Comparar Energía de ionización (2.ª) de todos los elementos →
Energía de ionización (3.ª)
34,86012 eV Comparar Energía de ionización (3.ª) de todos los elementos →
Energía de ionización (4.ª)
47,222163 eV Comparar Energía de ionización (4.ª) de todos los elementos →
Energía de ionización (5.ª)
72,59475 eV Comparar Energía de ionización (5.ª) de todos los elementos →
Estados de oxidación
−2, −1, 0, +1, +2, +3, +4, +5, +6 Comparar Estados de oxidación de todos los elementos →
Electrones de valencia
6 Comparar Electrones de valencia de todos los elementos →
Alótropos
["monoclinic", "rhombic"]
Configuración electrónica
[Ne] 3s2 3p4

Termodinámicas

Punto crítico (temperatura)
1041 °C
Punto crítico (presión)
2,07e+7 Pa
Calor de fusión
0,01793025 eV Comparar Calor de fusión de todos los elementos →
Calor de vaporización
0,46639374 eV Comparar Calor de vaporización de todos los elementos →
Calor de sublimación
2,870913 eV
Calor de atomización
2,870913 eV
Entalpía de atomización
2,872675 eV

Nucleares

Protones
16 Comparar Protones de todos los elementos →
Neutrones
16 Comparar Neutrones de todos los elementos →
Isótopos conocidos
24 Comparar Isótopos conocidos de todos los elementos →
Isótopos estables
4 Comparar Isótopos estables de todos los elementos →
Isótopo más estable
S-32
Año de descubrimiento
1777

Abundancia

Abundancia (corteza terrestre)
350 mg/kg Comparar Abundancia (corteza terrestre) de todos los elementos →
Abundancia (océano)
905 mg/L Comparar Abundancia (océano) de todos los elementos →

Estructura cristalina

Constante de red a
1047 pm

Estructura electrónica

Electrones por capa
2, 8, 6 Comparar Electrones por capa de todos los elementos →

Identificadores

Número CAS
7704-34-9 Comparar Número CAS de todos los elementos →
Símbolo del término
3P2
InChI
InChI=1S/S
Clave InChI
NINIDFKCEFEMDL-UHFFFAOYSA-N

Configuración electrónica Medido

Carga del ion
Protones 16
Electrones 16
Carga Neutro
Configuración S: 3s² 3p⁴
Configuración electrónica
Medido
[Ne] 3s² 3p⁴
1s² 2s² 2p⁶ 3s² 3p⁴
Diagrama de orbitales
1s
2/2
2s
2/2
2p
6/6
3s
2/2
3p
4/6 2↑
Total de electrones: 16 Desapareados: 2 ?

Modelo atómico

Protones 16
Neutrones 16
Electrones 16
Número másico 32
Estabilidad Estable

Los isótopos cambian el número de neutrones, la masa y la estabilidad, pero no la configuración electrónica de un átomo neutro.

Modelo atómico esquemático, no a escala.

Huella atómica

Espectro de emisión / absorción

25 / 50 (50 50 con intensidad)
Medido
Emisión Visible: 380–750 nm

Distribución isotópica

3294,9900%344,2500%330,7500%360,0100%Número másicoAbundancia natural (%)
Número másicoMasa atómica (u)Abundancia naturalPeriodo de semidesintegración
32 Estable31,9720711744 ± 0,000000001494,9900%Estable
33 Estable32,9714589098 ± 0,00000000150,7500%Estable
34 Estable33,967867004 ± 0,0000000474,2500%Estable
36 Estable35,96708071 ± 0,00000020,0100%Estable
Medido

Fase / Estado

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

Motivo: 90,2 °C por debajo del punto de fusión (115,21 °C)

Punto de fusión 115,21 °C
Punto de ebullición 444,6 °C
Por debajo del punto de fusión en 90,2 °C
0 K Temperatura actual: 25 °C 6000 K
Secuencia de fases

Esquemático, no a escala

Sólido
Líquido
Gas
Fusión
Ebullición
25°C
Sólido
Líquido
Gas
Actual

Puntos de transición de fase

Punto de fusión Bibliografía
115,21 °C
Punto de ebullición Bibliografía
444,6 °C
Fase actual Calculado
Sólido

Energías de transición

Calor de fusión Bibliografía
0,01793025 eV

Energía necesaria para fundir 1 mol en el punto de fusión

Calor de vaporización Bibliografía
0,46639374 eV

Energía necesaria para vaporizar 1 mol en el punto de ebullición

Calor de sublimación Bibliografía
2,870913 eV

Energía necesaria para sublimar 1 mol en el punto de sublimación

Densidad

Densidad de referencia Bibliografía
2067 kg/m³

En condiciones estándar

Densidad actual Calculado
2067 kg/m³

En condiciones estándar

Avanzado

Punto crítico Bibliografía
1041 °C

Espectros atómicos

Se muestran 10 de 16. Ordenado por carga del ion (ascendente).

Líneas disponibles ?

IonCargaTotal de líneasProbabilidades de transiciónDesignaciones de los niveles
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
Líneas disponibles en el NIST →

Niveles disponibles ?

IonCargaNiveles
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
Niveles disponibles en el NIST →
16 S 32.067499999999995

Sulfur — Visualizador de orbitales atómicos

[Ne]3s23p4
Niveles de energía 2 8 6
Estados de oxidación -2, -1, 0, +1, +2, +3, +4, +5, +6
HOMO 3p n=3 · l=1 · m=-1
Sulfur — Vista previa del visualizador de orbitales atómicos
Three.js solo se carga cuando se solicita
16 S 32.067499999999995

Sulfur — Visualizador de estructuras cristalinas

Orthorhombic · Pearson N/A
Experimental
Pearson N/A
Sulfur — Vista previa del visualizador de estructuras cristalinas
Three.js solo se carga cuando se solicita

Radios iónicos

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

Compuestos

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 másicoMasa atómica (u)Abundancia naturalPeriodo de semidesintegraciónModo de desintegración
32 Estable31,9720711744 ± 0,000000001494,9900% ± 0,2600%Estable
stable
33 Estable32,9714589098 ± 0,00000000150,7500% ± 0,0200%Estable
stable
34 Estable33,967867004 ± 0,0000000474,2500% ± 0,2400%Estable
stable
36 Estable35,96708071 ± 0,00000020,0100% ± 0,0100%Estable
stable
32 Estable
Masa atómica (u) 31,9720711744 ± 0,0000000014
Abundancia natural 94,9900% ± 0,2600%
Periodo de semidesintegración Estable
Modo de desintegración
stable
33 Estable
Masa atómica (u) 32,9714589098 ± 0,0000000015
Abundancia natural 0,7500% ± 0,0200%
Periodo de semidesintegración Estable
Modo de desintegración
stable
34 Estable
Masa atómica (u) 33,967867004 ± 0,000000047
Abundancia natural 4,2500% ± 0,2400%
Periodo de semidesintegración Estable
Modo de desintegración
stable
36 Estable
Masa atómica (u) 35,96708071 ± 0,0000002
Abundancia natural 0,0100% ± 0,0100%
Periodo de semidesintegración Estable
Modo de desintegración
stable

Líneas espectrales

Se muestran 50 de 556. De forma predeterminada, solo se muestran las líneas espectrales con intensidad medida.

Longitud de onda (nm)IntensidadEstado de ionizaciónTipoTransiciónExactitudFuente
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

Propiedades ampliadas

Radios covalentes (ampliados)

Radio covalente (Pyykkö)
103 pm
Radio covalente (Pyykkö, enlace doble)
94 pm
Radio covalente (Pyykkö, enlace triple)
95 pm
Radio covalente (Bragg)
102 pm

Radios 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

Radios atómicos y metálicos

Radio atómico (Rahm)
214 pm
Radio metálico (C12)
127 pm

Escalas de numeración

Mendeleev
100
Pettifor
94
Glawe
96

Escalas de electronegatividad

Ghosh
0
Gunnarsson–Lundqvist
6
Robles–Bartolotti
5

Polarizabilidad y dispersión

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

Afinidad química

Afinidad protónica
664,3 kJ/mol
Basicidad en fase gaseosa
640,2 kJ/mol

Riesgo de suministro y economía

Concentración de la producción
17
Riesgo relativo de suministro
4
Estabilidad política (principal productor)
24

Transiciones de fase y alótropos

rhombic
Temperatura de transición368,35 K
Punto de ebullición717,76 K
Punto crítico (temperatura)1314,15 K
Punto crítico (presión)20,7 MPa
monoclinic
Punto de fusión388,36 K
Punto de ebullición717,76 K
Punto crítico (temperatura)1314,15 K

Categorías de estados de oxidación

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

Datos de referencia avanzados

Constantes de apantallamiento (5)
nOrbitalσ
1s0,4591
2p4,023
2s5,3712
3p10,5181
3s9,6331
Detalle de los radios cristalinos (4)
CargaCNEspínrcrystal (pm)Origen
-2VI170Pauling's (1960) crystal radius,
4VI51Ahrens (1952) ionic radius,
6IV26
6VI43calculated,
Modos de desintegración de los isótopos (38)
IsótopoModoIntensidad
262p—
27B+100%
27B+p61%
272p3%
28B+100%
28B+p20,7%
29B+100%
29B+p46,4%
30B+100%
31B+100%
Factores de dispersión de rayos X (504)
Energía (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

Datos adicionales

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.

Referencias (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.

Referencias (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)..

Referencias (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

Referencias

(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 la licencia: 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 la licencia: 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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