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S 16

Sulfur (S)

nonmetal
Periode: 3 Gruppe: 16 Block: p

Solid

Standardatomgewicht

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

Elektronenkonfiguration

[Ne] 3s2 3p4

Schmelzpunkt

115,21 °C

Siedepunkt

444,6 °C

Dichte

2067 kg/m³

Oxidationszustände

−2, −1, 0, +1, +2, +3, +4, +5, +6

Elektronegativität (Pauling)

2,58

Ionisierungsenergie (1.)

10,360017 eV

Entdeckungsjahr

1777

Atomradius

100 pm

Details

Namensherkunft Latin: sulphur (brimstone).
Entdecker 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.

Bilder

Eigenschaften

Physikalisch

Atomradius (empirisch)
100 pm Vergleiche Atomradius (empirisch) aller Elemente →
Kovalenzradius
105 pm Vergleiche Kovalenzradius aller Elemente →
Van-der-Waals-Radius
180 pm Vergleiche Van-der-Waals-Radius aller Elemente →
Metallradius
104 pm Vergleiche Metallradius aller Elemente →
Dichte
2067 kg/m³ Vergleiche Dichte aller Elemente →
Molares Volumen
0,0155 L/mol
Aggregatzustand bei Standardbedingungen
Fest Vergleiche Aggregatzustand bei Standardbedingungen aller Elemente →
Schmelzpunkt
115,21 °C Vergleiche Schmelzpunkt aller Elemente →
Siedepunkt
444,6 °C Vergleiche Siedepunkt aller Elemente →
Wärmeleitfähigkeit
0,27 W/(m·K) Vergleiche Wärmeleitfähigkeit aller Elemente →
Spezifische Wärmekapazität
0,708 J/(g·K) Vergleiche Spezifische Wärmekapazität aller Elemente →
Molare Wärmekapazität
22,7 J/(mol·K) Vergleiche Molare Wärmekapazität aller Elemente →
Kristallstruktur
Orthorhombisch Vergleiche Kristallstruktur aller Elemente →

Chemisch

Elektronegativität (Pauling)
2,58 Vergleiche Elektronegativität (Pauling) aller Elemente →
Elektronegativität (Allen)
2,589
Elektronenaffinität
2,0771 eV
Ionisierungsenergie (1.)
10,360017 eV Vergleiche Ionisierungsenergie (1.) aller Elemente →
Ionisierungsenergie (2.)
23,33796 eV Vergleiche Ionisierungsenergie (2.) aller Elemente →
Ionisierungsenergie (3.)
34,86012 eV Vergleiche Ionisierungsenergie (3.) aller Elemente →
Ionisierungsenergie (4.)
47,222163 eV Vergleiche Ionisierungsenergie (4.) aller Elemente →
Ionisierungsenergie (5.)
72,59475 eV Vergleiche Ionisierungsenergie (5.) aller Elemente →
Oxidationszustände
−2, −1, 0, +1, +2, +3, +4, +5, +6 Vergleiche Oxidationszustände aller Elemente →
Valenzelektronen
6 Vergleiche Valenzelektronen aller Elemente →
Allotrope
["monoclinic", "rhombic"]
Elektronenkonfiguration
[Ne] 3s2 3p4

Thermodynamisch

Kritischer Punkt (Temperatur)
1041 °C
Kritischer Punkt (Druck)
2,07e+7 Pa
Schmelzwärme
0,01793025 eV Vergleiche Schmelzwärme aller Elemente →
Verdampfungswärme
0,46639374 eV Vergleiche Verdampfungswärme aller Elemente →
Sublimationswärme
2,870913 eV
Atomisierungswärme
2,870913 eV
Atomisierungsenthalpie
2,872675 eV

Nuklear

Protonen
16 Vergleiche Protonen aller Elemente →
Neutronen
16 Vergleiche Neutronen aller Elemente →
Bekannte Isotope
24 Vergleiche Bekannte Isotope aller Elemente →
Stabile Isotope
4 Vergleiche Stabile Isotope aller Elemente →
Stabilstes Isotop
S-32
Entdeckungsjahr
1777

Häufigkeit

Häufigkeit (Erdkruste)
350 mg/kg Vergleiche Häufigkeit (Erdkruste) aller Elemente →
Häufigkeit (Ozean)
905 mg/L Vergleiche Häufigkeit (Ozean) aller Elemente →

Kristallstruktur

Gitterkonstante a
1047 pm

Elektronische Struktur

Elektronen pro Schale
2, 8, 6 Vergleiche Elektronen pro Schale aller Elemente →

Identifikatoren

CAS-Nummer
7704-34-9 Vergleiche CAS-Nummer aller Elemente →
Termsymbol
3P2
InChI
InChI=1S/S
InChI-Key
NINIDFKCEFEMDL-UHFFFAOYSA-N

Elektronenkonfiguration Gemessen

Ionenladung
Protonen 16
Elektronen 16
Ladung Neutral
Konfiguration S: 3s² 3p⁴
Elektronenkonfiguration
Gemessen
[Ne] 3s² 3p⁴
1s² 2s² 2p⁶ 3s² 3p⁴
Orbitaldiagramm
1s
2/2
2s
2/2
2p
6/6
3s
2/2
3p
4/6 2↑
Gesamtelektronen: 16 Ungepaart: 2 ?

Atommodell

Protonen 16
Neutronen 16
Elektronen 16
Massenzahl 32
Stabilität Stabil

Isotope ändern die Neutronenzahl, Masse und Stabilität — nicht die Elektronenkonfiguration eines neutralen Atoms.

Schematisches Atommodell, nicht maßstabsgetreu.

Atomarer Fingerabdruck

Emissions- / Absorptionsspektrum

25 / 50 (50 50 mit Intensität)
Gemessen
Emission Sichtbar: 380–750 nm

Isotopenverteilung

3294,9900%344,2500%330,7500%360,0100%MassenzahlNatürliche Häufigkeit (%)
MassenzahlAtommasse (u)Natürliche HäufigkeitHalbwertszeit
32 Stabil31,9720711744 ± 0,000000001494,9900%Stabil
33 Stabil32,9714589098 ± 0,00000000150,7500%Stabil
34 Stabil33,967867004 ± 0,0000000474,2500%Stabil
36 Stabil35,96708071 ± 0,00000020,0100%Stabil
Gemessen

Phase / Zustand

1 atm / 101.325 kPa
Fest 25 °C (298,15 K)

Grund: 90,2 °C unter Schmelzpunkt (115,21 °C)

Schmelzpunkt 115,21 °C
Siedepunkt 444,6 °C
Unter Schmelzpunkt um 90,2 °C
0 K Aktuelle Temperatur: 25 °C 6000 K
Phasenzeitlinie

Schematisch, nicht maßstabsgetreu

Fest
Flüssig
Gas
Schmelzen
Sieden
25°C
Fest
Flüssig
Gas
Aktuell

Phasenübergangspunkte

Schmelzpunkt Literatur
115,21 °C
Siedepunkt Literatur
444,6 °C
Aktuelle Phase Berechnet
Fest

Übergangsenergien

Schmelzwärme Literatur
0,01793025 eV

Energie benötigt, um 1 mol am Schmelzpunkt zu schmelzen

Verdampfungswärme Literatur
0,46639374 eV

Energie benötigt, um 1 mol am Siedepunkt zu verdampfen

Sublimationswärme Literatur
2,870913 eV

Energie benötigt, um 1 mol am Sublimationspunkt zu sublimieren

Dichte

Referenzdichte Literatur
2067 kg/m³

Bei Standardbedingungen

Aktuelle Dichte Berechnet
2067 kg/m³

Bei Standardbedingungen

Erweitert

Kritischer Punkt Literatur
1041 °C

Atomspektren

10 von 16 angezeigt. Sortiert nach Ionenladung (aufsteigend).

Liniendaten ?

IonLadungGesamtlinienÜbergangswahrscheinlichkeitenNiveau-Bezeichnungen
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
NIST Liniendaten →

Niveaudaten ?

IonLadungNiveaus
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
NIST Niveaudaten →
16 S 32.067499999999995

Sulfur — Atomorbital-Visualisierer

[Ne]3s23p4
Energieniveaus 2 8 6
Oxidationszustände -2, -1, 0, +1, +2, +3, +4, +5, +6
HOMO 3p n=3 · l=1 · m=-1
Sulfur — Atomorbital-Visualisierer Vorschau
Three.js lädt nur auf Anfrage
16 S 32.067499999999995

Sulfur — Kristallstruktur-Visualisierer

Orthorhombic · Pearson N/A
Experimentell
Pearson N/A
Sulfur — Kristallstruktur-Visualisierer Vorschau
Three.js lädt nur auf Anfrage

Ionenradien

LadungKoordinationSpinRadius
-26N/A184 pm
+46N/A37 pm
+64N/A12 pm
+66N/A28.999999999999996 pm

Verbindungen

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

Isotope (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.

MassenzahlAtommasse (u)Natürliche HäufigkeitHalbwertszeitZerfallsart
32 Stabil31,9720711744 ± 0,000000001494,9900% ± 0,2600%Stabil
stable
33 Stabil32,9714589098 ± 0,00000000150,7500% ± 0,0200%Stabil
stable
34 Stabil33,967867004 ± 0,0000000474,2500% ± 0,2400%Stabil
stable
36 Stabil35,96708071 ± 0,00000020,0100% ± 0,0100%Stabil
stable
32 Stabil
Atommasse (u) 31,9720711744 ± 0,0000000014
Natürliche Häufigkeit 94,9900% ± 0,2600%
Halbwertszeit Stabil
Zerfallsart
stable
33 Stabil
Atommasse (u) 32,9714589098 ± 0,0000000015
Natürliche Häufigkeit 0,7500% ± 0,0200%
Halbwertszeit Stabil
Zerfallsart
stable
34 Stabil
Atommasse (u) 33,967867004 ± 0,000000047
Natürliche Häufigkeit 4,2500% ± 0,2400%
Halbwertszeit Stabil
Zerfallsart
stable
36 Stabil
Atommasse (u) 35,96708071 ± 0,0000002
Natürliche Häufigkeit 0,0100% ± 0,0100%
Halbwertszeit Stabil
Zerfallsart
stable

Spektrallinien

50 von 556 angezeigt. Standardmäßig werden nur Spektrallinien mit gemessener Intensität angezeigt.

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

Erweiterte Eigenschaften

Kovalente Radien (Erweitert)

Kovalenzradius (Pyykkö)
103 pm
Kovalenzradius (Pyykkö, doppelt)
94 pm
Kovalenzradius (Pyykkö, dreifach)
95 pm
Kovalenzradius (Bragg)
102 pm

Van-der-Waals-Radien

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

Atom- & Metallische Radien

Atomradius (Rahm)
214 pm
Metallradius (C12)
127 pm

Nummerierungsskalen

Mendeleev
100
Pettifor
94
Glawe
96

Elektronegativitätsskalen

Ghosh
0
Gunnarsson–Lundqvist
6
Robles–Bartolotti
5

Polarisierbarkeit & Dispersion

Dipolpolarisierbarkeit
19,4 a.u.
Dipolpolarisierbarkeit (Uns.)
0,1 a.u.
C₆
134 Ha·Bohr6
C₆ (Gould–Bučko)
140 Ha·Bohr6

Chemische Affinität

Protonenaffinität
664,3 kJ/mol
Gasbasizität
640,2 kJ/mol

Lieferrisiko & Wirtschaftlichkeit

Produktionskonzentration
17
Relatives Lieferrisiko
4
Politische Stabilität (Top-Produzent)
24

Phasenübergänge & Allotrope

rhombic
Übergangstemperatur368,35 K
Siedepunkt717,76 K
Kritischer Punkt (Temperatur)1314,15 K
Kritischer Punkt (Druck)20,7 MPa
monoclinic
Schmelzpunkt388,36 K
Siedepunkt717,76 K
Kritischer Punkt (Temperatur)1314,15 K

Oxidationszustands-Kategorien

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

Erweiterte Referenzdaten

Abschirmkonstanten (5)
nOrbitalσ
1s0,4591
2p4,023
2s5,3712
3p10,5181
3s9,6331
Kristallradien-Details (4)
LadungCNSpinrcrystal (pm)Herkunft
-2VI170Pauling's (1960) crystal radius,
4VI51Ahrens (1952) ionic radius,
6IV26
6VI43calculated,
Isotopenzerfallsarten (38)
IsotopModusIntensität
262p—
27B+100%
27B+p61%
272p3%
28B+100%
28B+p20,7%
29B+100%
29B+p46,4%
30B+100%
31B+100%
Röntgenstreufaktoren (504)
Energie (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

Zusätzliche Daten

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.

Referenzen (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.

Referenzen (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)..

Referenzen (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

Referenzen

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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.

Lizenzhinweis: 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/

Lizenzhinweis: 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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