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C 6

Carbon (C)

nonmetal
Periodo: 2 Grupo: 14 Bloque: p

Solid

Peso atómico estándar

12,011 u [12,0096, 12,0116]

Configuración electrónica

[He] 2s2 2p2

Punto de fusión

3549,85 °C

Punto de ebullición

3824,85 °C

Densidad

2267 kg/m³

Estados de oxidación

−4, −3, −2, −1, 0, +1, +2, +3, +4

Electronegatividad (Pauling)

2,55

Energía de ionización (1.ª)

11,260288 eV

Año de descubrimiento

1797

Radio atómico

70 pm

Detalles

Origen del nombre Latin: carbo, (charcoal).
Descubridores Known to the ancients

Carbon is a nonmetal in group 14 and the defining element of organic chemistry. Its small atoms form strong covalent bonds with carbon and many other elements, allowing chains, rings, networks, and multiple bonds of great diversity. It occurs naturally as graphite, diamond, amorphous carbon-rich materials, carbonate minerals, fossil carbon, dissolved carbon species, and as a central element in living matter.

Carbon is a member of group 14 of the periodic table. It has three allotropic forms of it, diamonds, graphite and fullerite. Carbon-14 is commonly used in radioactive dating. Carbon occurs in all organic life and is the basis of organic chemistry. Carbon has the interesting chemical property of being able to bond with itself, and a wide variety of other elements.

The name derives from the Latin carbo for "charcoal". It was known in prehistoric times in the form of charcoal and soot. In 1797, the English chemist Smithson Tennant proved that diamond is pure carbon.

Carbon, the sixth most abundant element in the universe, has been known since ancient times. Carbon is most commonly obtained from coal deposits, although it usually must be processed into a form suitable for commercial use. Three naturally occurring allotropes of carbon are known to exist: amorphous, graphite and diamond.

From the Latin word carbo: charcoal. Carbon, an element of prehistoric discovery, is very widely distributed in nature. It is found in abundance in the sun, stars, comets, and atmospheres of most planets. Carbon in the form of microscopic diamonds is found in some meteorites.

Natural diamonds are found in kimberlite of ancient volcanic "pipes," found in South Africa, Arkansas, and elsewhere. Diamonds are now also being recovered from the ocean floor off the Cape of Good Hope. About 30% of all industrial diamonds used in the U.S. are now made synthetically.

The energy of the sun and stars can be attributed at least in part to the well-known carbon-nitrogen cycle.

Imágenes

Propiedades

Químicas

Electronegatividad (Pauling)
2,55 Comparar Electronegatividad (Pauling) de todos los elementos →
Electronegatividad (Allen)
2,544
Afinidad electrónica
1,2621 eV
Energía de ionización (1.ª)
11,260288 eV Comparar Energía de ionización (1.ª) de todos los elementos →
Energía de ionización (2.ª)
24,383227 eV Comparar Energía de ionización (2.ª) de todos los elementos →
Energía de ionización (3.ª)
47,887945 eV Comparar Energía de ionización (3.ª) de todos los elementos →
Energía de ionización (4.ª)
64,493742 eV Comparar Energía de ionización (4.ª) de todos los elementos →
Energía de ionización (5.ª)
392,09191 eV Comparar Energía de ionización (5.ª) de todos los elementos →
Estados de oxidación
−4, −3, −2, −1, 0, +1, +2, +3, +4 Comparar Estados de oxidación de todos los elementos →
Electrones de valencia
4 Comparar Electrones de valencia de todos los elementos →
Alótropos
["graphite"]
Configuración electrónica
[He] 2s2 2p2

Termodinámicas

Punto triple (temperatura)
4489 °C
Punto triple (presión)
1,03e+7 Pa
Calor de vaporización
7,410478 eV Comparar Calor de vaporización de todos los elementos →
Calor de sublimación
7,42789 eV
Calor de atomización
7,42789 eV
Entalpía de atomización
7,42986 eV

Nucleares

Protones
6 Comparar Protones de todos los elementos →
Neutrones
6 Comparar Neutrones de todos los elementos →
Isótopos conocidos
16 Comparar Isótopos conocidos de todos los elementos →
Isótopos estables
2 Comparar Isótopos estables de todos los elementos →
Isótopo más estable
C-12
Año de descubrimiento
1797

Estructura cristalina

Constante de red a
357 pm

Estructura electrónica

Electrones por capa
2, 4 Comparar Electrones por capa de todos los elementos →

Identificadores

Número CAS
7440-44-0 Comparar Número CAS de todos los elementos →
Símbolo del término
3P0
InChI
InChI=1S/C
Clave InChI
OKTJSMMVPCPJKN-UHFFFAOYSA-N

Configuración electrónica Medido

Carga del ion
Protones 6
Electrones 6
Carga Neutro
Configuración C: 2s² 2p²
Configuración electrónica
Medido
[He] 2s² 2p²
1s² 2s² 2p²
Diagrama de orbitales
1s
2/2
2s
2/2
2p
2/6 2↑
Total de electrones: 6 Desapareados: 2 ?

Modelo atómico

Protones 6
Neutrones 6
Electrones 6
Número másico 12
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

1298,9300%131,0700%Número másicoAbundancia natural (%)
Número másicoMasa atómica (u)Abundancia naturalPeriodo de semidesintegración
12 Estable1298,9300%Estable
13 Estable13,00335483507 ± 0,000000000231,0700%Estable
Medido

Fase / Estado

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

Motivo: 3799,8 °C por debajo del punto de sublimación (3824,85 °C)

Punto de sublimación 3824,85 °C
0 K Temperatura actual: 25 °C 6000 K
Secuencia de fases

Esquemático, no a escala

Sólido
Gas
Sublimación
25°C
Sólido
Líquido
Gas
Actual

Puntos de transición de fase

Punto de sublimación Bibliografía
3824,85 °C
Fase actual Calculado
Sólido

Energías de transición

Calor de vaporización Bibliografía
7,410478 eV

Energía necesaria para vaporizar 1 mol en el punto de ebullición

Calor de sublimación Bibliografía
7,42789 eV

Energía necesaria para sublimar 1 mol en el punto de sublimación

Densidad

Densidad de referencia Bibliografía
2267 kg/m³

En condiciones estándar

Densidad actual Calculado
2267 kg/m³

En condiciones estándar

Avanzado

Punto triple Bibliografía
4489 °C

Espectros atómicos

Se muestran 10 de 11. Ordenado por carga del ion (ascendente).

Líneas disponibles ?

IonCargaTotal de líneasProbabilidades de transiciónDesignaciones de los niveles
C I 0210216162102
12C I Isótopo089089
13C I Isótopo089089
12C II Isótopo+11870187
14C II Isótopo+11870187
C II +1160514331605
13C II Isótopo+11870187
C III +2882878878
C IV +3259224255
C V +4149146147
Líneas disponibles en el NIST →

Niveles disponibles ?

IonCargaNiveles
C I 0435
12C I Isótopo033
13C I Isótopo033
12C II Isótopo+136
14C II Isótopo+136
C II +1415
13C II Isótopo+136
C III +2201
C IV +3107
C V +4156
Niveles disponibles en el NIST →
6 C 12.0106

Carbon — Visualizador de orbitales atómicos

[He]2s22p2
Niveles de energía 2 4
Estados de oxidación -4, -3, -2, -1, 0, +1, +2, +3, +4
HOMO 2p n=2 · l=1 · m=-1
Carbon — Vista previa del visualizador de orbitales atómicos
Three.js solo se carga cuando se solicita
6 C 12.0106

Carbon — Visualizador de estructuras cristalinas

Face-Centered Cubic · Pearson cF8
Experimental
Pearson cF8
N.º de coord. 4
Empaquetamiento 34.000%
Carbon — Vista previa del visualizador de estructuras cristalinas
Three.js solo se carga cuando se solicita

Radios iónicos

CargaCoordinaciónEspínRadio
+44N/D15 pm
+46N/D16 pm

Compuestos

C
12,011 u

Isótopos (2)

Carbon has seven isotopes. In 1961 the International Union of Pure and Applied Chemistry adopted the isotope carbon-12 as the basis for atomic weights. Carbon-14, an isotope with a half-life of 5715 years, has been widely used to date such materials as wood, archaeological specimens, etc.

Número másicoMasa atómica (u)Abundancia naturalPeriodo de semidesintegraciónModo de desintegración
12 Estable1298,9300% ± 0,0800%Estable
stable
13 Estable13,00335483507 ± 0,000000000231,0700% ± 0,0800%Estable
stable
12 Estable
Masa atómica (u) 12
Abundancia natural 98,9300% ± 0,0800%
Periodo de semidesintegración Estable
Modo de desintegración
stable
13 Estable
Masa atómica (u) 13,00335483507 ± 0,00000000023
Abundancia natural 1,0700% ± 0,0800%
Periodo de semidesintegración Estable
Modo de desintegración
stable

Líneas espectrales

Se muestran 50 de 993. De forma predeterminada, solo se muestran las líneas espectrales con intensidad medida.

Longitud de onda (nm)IntensidadEstado de ionizaciónTipoTransiciónExactitudFuente
505.214927 nm160000C Iemission2s2.2p.3s 1P* → 2s2.2p.4p 1DMedidaNIST
538.033014 nm120000C Iemission2s2.2p.3s 1P* → 2s2.2p.4p 1PMedidaNIST
711.31656 nm110000C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3F*MedidaNIST
493.202524 nm73000C Iemission2s2.2p.3s 1P* → 2s2.2p.4p 1SMedidaNIST
477.173374 nm69000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3PMedidaNIST
711.697758 nm45000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MedidaNIST
658.76211 nm40000C Iemission2s2.2p.3p 1P → 2s2.2p.4d 1P*MedidaNIST
579.311495 nm38000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMedidaNIST
711.96559 nm37000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MedidaNIST
580.059993 nm35000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMedidaNIST
600.1123 nm35000C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MedidaNIST
477.589266 nm34000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3PMedidaNIST
437.13814 nm33000C Iemission2s2.2p.3s 1P* → 2s2.2p.5p 1PMedidaNIST
711.145795 nm32000C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3F*MedidaNIST
682.814076 nm27000C Iemission2s2.2p.3p 1P → 2s2.2p.4d 1D*MedidaNIST
504.149039 nm25000C Iemission2s.2p3 3D* → 2s2.2p.(2P*<1/2>).4f 2[5/2]MedidaNIST
477.002376 nm24000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3PMedidaNIST
600.6012 nm23000C Iemission2s2.2p.3p 3D → 2s2.2p.5d 3D*MedidaNIST
665.55294 nm20000C Iemission2s2.2p.3p 1P → 2s2.2p.5s 1P*MedidaNIST
710.011312 nm19000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MedidaNIST
566.894 nm18000C Iemission2s2.2p.3p 1P → 2s2.2p.5d 1P*MedidaNIST
596.933151 nm18000C Iemission2s.2p3 3D* → 2s2.2p.4p 3DMedidaNIST
708.782188 nm18000C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3D*MedidaNIST
402.94119 nm16000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3PMedidaNIST
601.64487 nm16000C Iemission2s2.2p.3p 3D → 2s2.2p.5d 3F*MedidaNIST
473.426281 nm15000C Iemission2s.2p3 3D* → 2s2.2p.5p 3PMedidaNIST
481.737213 nm15000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3SMedidaNIST
579.446608 nm15000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMedidaNIST
748.344451 nm15000C Iemission2s2.2p.3p 3S → 2s2.2p.4d 3P*MedidaNIST
406.52425 nm14000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3DMedidaNIST
580.52017 nm14000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMedidaNIST
601.4833 nm14000C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MedidaNIST
710.89263 nm14000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MedidaNIST
400.9928 nm13000C Iemission2s2.2p.3s 1P* → 2s2.2p.6p 1PMedidaNIST
422.83269 nm13000C Iemission2s2.2p.3s 1P* → 2s2.2p.5p 1SMedidaNIST
447.85821 nm13000C Iemission2s.2p3 3D* → 2s2.2p.(2P*<1/2>).5f 2[5/2]MedidaNIST
504.012903 nm12000C Iemission2s.2p3 3D* → 2s2.2p.(2P*<1/2>).4f 2[7/2]MedidaNIST
601.0669 nm12000C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MedidaNIST
406.4264 nm11000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3DMedidaNIST
639.7965 nm11000C Iemission2s2.2p.3p 3S → 2s2.2p.6s 3P*MedidaNIST
666.3043 nm11000C Iemission2s2.2p.3p 3P → 2s2.2p.5d 3D*MedidaNIST
667.1849 nm11000C Iemission2s2.2p.3p 3P → 2s2.2p.6s 3P*MedidaNIST
403.180216 nm10000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3PMedidaNIST
482.679468 nm10000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3SMedidaNIST
598.903753 nm10000C Iemission2s.2p3 3D* → 2s2.2p.4p 3DMedidaNIST
707.649944 nm9900C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3D*MedidaNIST
402.284321 nm9700C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3PMedidaNIST
555.1578 nm9600C Iemission2s2.2p.3p 3D → 2s2.2p.7s 3P*MedidaNIST
600.7173 nm9600C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MedidaNIST
502.492938 nm9400C Iemission2s.2p3 3D* → 2s2.2p.(2P*<3/2>).4f 2[7/2]MedidaNIST

Propiedades ampliadas

Radios covalentes (ampliados)

Radio covalente (Pyykkö)
75 pm
Radio covalente (Pyykkö, enlace doble)
67 pm
Radio covalente (Pyykkö, enlace triple)
60 pm
Radio covalente (Bragg)
77 pm

Radios de van der Waals

Bondi
170 pm
Batsanov
170 pm
Alvarez
177 pm
UFF
385,1 pm
MM3
204 pm
Dreiding
389,83 pm
Rowland–Taylor
177 pm

Radios atómicos y metálicos

Radio atómico (Rahm)
190 pm
Radio metálico (C12)
86 pm

Escalas de numeración

Mendeleev
87
Pettifor
95
Glawe
87

Escalas de electronegatividad

Ghosh
0
Miedema
6
Gunnarsson–Lundqvist
7
Robles–Bartolotti
6

Polarizabilidad y dispersión

Polarizabilidad dipolar
11,3 a.u.
Polarizabilidad dipolar (incert.)
0,2 a.u.
C₆
46,6 Ha·Bohr6
C₆ (Gould–Bučko)
47,9 Ha·Bohr6

Parámetros de Miedema

Volumen molar de Miedema
3,26 cm3/mol
Densidad electrónica de Miedema
6

Riesgo de suministro y economía

Concentración de la producción
46
Riesgo relativo de suministro
5
Distribución de las reservas
28
Estabilidad política (principal productor)
24
Estabilidad política (país con mayores reservas)
57

Transiciones de fase y alótropos

graphite Sublimación
Punto de ebullición4098,15 K
Punto triple (temperatura)4762,15 K
Punto triple (presión)10300 kPa

Categorías de estados de oxidación

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

Datos de referencia avanzados

Constantes de apantallamiento (3)
nOrbitalσ
1s0,3273
2p2,8642
2s2,7834
Detalle de los radios cristalinos (3)
CargaCNEspínrcrystal (pm)Origen
4III6
4IV29Pauling's (1960) crystal radius,
4VI30Ahrens (1952) ionic radius,
Modos de desintegración de los isótopos (27)
IsótopoModoIntensidad
82p100%
9B+100%
9B+p7,5%
9B+A38,4%
10B+100%
11B+100%
14B-100%
15B-100%
16B-100%
16B-n99%
Factores de dispersión de rayos X (502)
Energía (eV)f₁f₂
10—0,80688
10,1617—0,85152
10,3261—0,89863
10,4931—0,94834
10,6628—1,0008
10,8353—1,05755
11,0106—1,12167
11,1886—1,18968
11,3696—1,26181
11,5535—1,33832

Datos adicionales

Isotopes in Forensic Science and Anthropology

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

Variations in the isotope-amount ratio n(13C)/n(12C) of biological products can be observed using isotope-ratio mass spectrometry (IRMS) to detect adulteration (the addition of inferior ingredients) in honey and other food products.

The isotope-amount ratio n(13C)/n(12C) can fluctuate between carbon sources, for example C3 plants (found in temperate climates and which use atmospheric carbon dioxide to make a 3-carbon molecule during photosynthesis — examples include rice, potatoes, tomatoes, and sugar beets), C4 plants (found in hot climates and which use atmospheric carbon dioxide to make a 4-carbon molecule during photosynthesis — examples include corn and sugar cane), animal carbon, atmospheric CO2, etc. This commonly makes it possible to detect whether these different carbon sources have been mixed by using isotope or mass balance to distinguish, for example, between beet sugar and cane sugar. Complications in source identification can arise with plants that open stomata at night to collect carbon dioxide to use a third mechanism to fix atmospheric carbon dioxide (CAM or crassulacean acid metabolism). The isotope-amount ratio n(13C)/n(12C) of CAM plants overlaps that of C3 or C4 plants — examples include pineapples and jade plants. The following adulterations are commonly detected using stable carbon isotope IRMS:

–Variations in the isotope-amount ratio n(13C)/n(12C) of honey are used to detect the addition (and potential adulteration) of high fructose corn syrup, corn, or sugar cane [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)..

–Variations in the isotope-amount ratio n(13C)/n(12C) of fruit juice have been used to detect the addition of a sugar [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)..

–Variations in the isotope-amount ratio n(13C)/n(12C) of natural vanilla extract have been used to detect the addition of artificial vanillin or p-hydroxybenzaldehyde [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)..

–Variations in the isotope-amount ratio n(13C)/n(12C) of beer are used to detect C4 carbon, which would indicate that a beer company may have added ingredients that are not traditionally used in brewing beer. Therefore, this ratio is used to detect the misrepresentation of a product as being pure [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)., [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002)..

Stable carbon IRMS has been used to determine if the botanical origin of an alcoholic spirit has been mislabeled and if chaptalization (the process of adding sugar to increase the alcoholic content) of wine has occurred [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)., [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002).. 14C scintillation counting has been used to determine the age of wine and alcoholic spirits [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)., [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002).. Variations in the isotope-amount ratio n(13C)/n(12C) of urine has been used to determine if steroids in urine are natural or of synthetic origin. These measurements enable anti-doping laboratories to perfect their methods for detecting steroid doping in athletes [69] B. D. Ahrens, A. W. Butch. Drug Test Anal.5, 534 (2013)., [70] E. Bulska, D. Gorczyca, I. Zalewska, A. Pokrywka, D. Kwiatkowska. J. Pharm. Biomed. Anal.106, 159 (2015)., [71] A. Casilli, T. Piper, F. A. de Oliveira, M. Costa Padilha, H. Marcelo Pereira, M. Thevis, F. R. de Aquino Neto. Drug Test Anal.8, 1204 (2016).. Variations in the isotope-amount ratio n(13C)/n(12C) of marijuana can provide information to determine if the plants were grown “inside” a building or greenhouse or were “open grown” (Fig. IUPAC.6.4). Plant carbon isotopic compositions are controlled by atmospheric CO2 and the supply and demand of CO2 in photosynthesis (the process used by plants to convert light energy from the sun into chemical energy). “Open grown” plants are grown in an area that is well ventilated and receives natural CO2. In contrast, plants grown “inside” receive supplemented CO2 and the photosynthesis process is more confined. Additionally, CO2 from a tank of compressed gas used to augment atmospheric CO2 to increase the growth of marijuana plants is commonly highly depleted in 13C as a refinery by-product. These differences change the carbon isotope ratios of the plants and the ratios vary enough to enable the determination of the growing and cultivation process of marijuana [72] E. K. Shibuya, J. E. Souza Sarkis, O. N. Neto, M. Z. Moreira, R. L. Victoria. Forensic Sci. Int.160, 35 (2006)., [73] J. B. West, J. M. Hurley, J. R. Ehleringer. J Forensic Sci.54, 84 (2009)..

Referencias (9)
  • [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002).
  • [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002).
  • [69] B. D. Ahrens, A. W. Butch. Drug Test Anal.5, 534 (2013).
  • [70] E. Bulska, D. Gorczyca, I. Zalewska, A. Pokrywka, D. Kwiatkowska. J. Pharm. Biomed. Anal.106, 159 (2015).
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Referencias

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

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)
Carbon

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
Carbon

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
Carbon

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
Carbon

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
Carbon

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

9 PubChem Elements
Carbon

The element property data was retrieved from publications.

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