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C 6

Carbon (C)

nonmetal
Período: 2 Grupo: 14 Bloco: p

Solid

Peso atômico padrão

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

Configuração eletrônica

[He] 2s2 2p2

Ponto de fusão

3549,85 °C

Ponto de ebulição

3824,85 °C

Densidade

2267 kg/m³

Estados de oxidação

−4, −3, −2, −1, 0, +1, +2, +3, +4

Eletronegatividade (Pauling)

2,55

Energia de ionização (1ª)

11,260288 eV

Ano da descoberta

1797

Raio atômico

70 pm

Detalhes

Origem do nome Latin: carbo, (charcoal).
Descobridores 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.

Imagens

Propriedades

Química

Eletronegatividade (Pauling)
2,55 Comparar Eletronegatividade (Pauling) de todos os elementos →
Eletronegatividade (Allen)
2,544
Afinidade eletrônica
1,2621 eV
Energia de ionização (1ª)
11,260288 eV Comparar Energia de ionização (1ª) de todos os elementos →
Energia de ionização (2ª)
24,383227 eV Comparar Energia de ionização (2ª) de todos os elementos →
Energia de ionização (3ª)
47,887945 eV Comparar Energia de ionização (3ª) de todos os elementos →
Energia de ionização (4ª)
64,493742 eV Comparar Energia de ionização (4ª) de todos os elementos →
Energia de ionização (5ª)
392,09191 eV Comparar Energia de ionização (5ª) de todos os elementos →
Estados de oxidação
−4, −3, −2, −1, 0, +1, +2, +3, +4 Comparar Estados de oxidação de todos os elementos →
Elétrons de valência
4 Comparar Elétrons de valência de todos os elementos →
Alótropos
["graphite"]
Configuração eletrônica
[He] 2s2 2p2

Termodinâmica

Ponto triplo (temperatura)
4489 °C
Ponto triplo (pressão)
1,03e+7 Pa
Calor de vaporização
7,410478 eV Comparar Calor de vaporização de todos os elementos →
Calor de sublimação
7,42789 eV
Calor de atomização
7,42789 eV
Entalpia de atomização
7,42986 eV

Abundância

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

Estrutura cristalina

Constante de rede a
357 pm

Estrutura eletrônica

Elétrons por camada
2, 4 Comparar Elétrons por camada de todos os elementos →

Identificadores

Número CAS
7440-44-0 Comparar Número CAS de todos os elementos →
Símbolo de termo
3P0
InChI
InChI=1S/C
Chave InChI
OKTJSMMVPCPJKN-UHFFFAOYSA-N

Configuração eletrônica Medido

Carga do íon
Prótons 6
Elétrons 6
Carga Neutro
Configuração C: 2s² 2p²
Configuração eletrônica
Medido
[He] 2s² 2p²
1s² 2s² 2p²
Diagrama de orbitais
1s
2/2
2s
2/2
2p
2/6 2↑
Total de elétrons: 6 Desemparelhados: 2 ?

Modelo atômico

Prótons 6
Nêutrons 6
Elétrons 6
Número de massa 12
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

1298,9300%131,0700%Número de massaAbundância natural (%)
Número de massaMassa atômica (u)Abundância naturalMeia-vida
12 Estável1298,9300%Estável
13 Estável13,00335483507 ± 0,000000000231,0700%Estável
Medido

Fase / Estado

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

Motivo: 3799,8 °C abaixo do ponto de sublimação (3824,85 °C)

Ponto de sublimação 3824,85 °C
0 K Temperatura atual: 25 °C 6000 K
Linha do tempo das fases

Esquemático, sem escala

Sólido
Gás
Sublimação
25°C
Sólido
Líquido
Gás
Atual

Pontos de transição de fase

Ponto de sublimação Literatura
3824,85 °C
Fase atual Calculado
Sólido

Energias de transição

Calor de vaporização Literatura
7,410478 eV

Energia necessária para vaporizar 1 mol no ponto de ebulição

Calor de sublimação Literatura
7,42789 eV

Energia necessária para sublimar 1 mol no ponto de sublimação

Densidade

Densidade de referência Literatura
2267 kg/m³

Em condições padrão

Densidade atual Calculado
2267 kg/m³

Em condições padrão

Avançado

Ponto triplo Literatura
4489 °C

Espectros atômicos

Mostrando 10 de 11. Ordenado por carga do íon (ordem crescente).

Dados de linhas disponíveis ?

ÍonCargaTotal de linhasProbabilidades de transiçãoDesignações dos níveis
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
Dados de linhas disponíveis no NIST →

Dados de níveis disponíveis ?

ÍonCargaNíveis
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
Dados de níveis disponíveis no NIST →
6 C 12.0106

Carbon — Visualizador de orbitais atômicos

[He]2s22p2
Níveis de energia 2 4
Estados de oxidação -4, -3, -2, -1, 0, +1, +2, +3, +4
HOMO 2p n=2 · l=1 · m=-1
Carbon — Prévia do visualizador de orbitais atômicos
O Three.js é carregado apenas quando solicitado
6 C 12.0106

Carbon — Visualizador de estruturas cristalinas

Face-Centered Cubic · Pearson cF8
Experimental
Pearson cF8
Nº de coord. 4
Empacotamento 34.000%
Carbon — Prévia do visualizador de estruturas cristalinas
O Three.js é carregado apenas quando solicitado

Raios iônicos

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

Compostos

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 de massaMassa atômica (u)Abundância naturalMeia-vidaModo de decaimento
12 Estável1298,9300% ± 0,0800%Estável
stable
13 Estável13,00335483507 ± 0,000000000231,0700% ± 0,0800%Estável
stable
12 Estável
Massa atômica (u) 12
Abundância natural 98,9300% ± 0,0800%
Meia-vida Estável
Modo de decaimento
stable
13 Estável
Massa atômica (u) 13,00335483507 ± 0,00000000023
Abundância natural 1,0700% ± 0,0800%
Meia-vida Estável
Modo de decaimento
stable

Linhas espectrais

Mostrando 50 de 993. Por padrão, são mostradas apenas as linhas espectrais com intensidade medida.

Comprimento de onda (nm)IntensidadeEstágio de ionizaçãoTipoTransiçãoExatidãoFonte
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

Propriedades ampliadas

Raios covalentes (dados ampliados)

Raio covalente (Pyykkö)
75 pm
Raio covalente (Pyykkö, ligação dupla)
67 pm
Raio covalente (Pyykkö, ligação tripla)
60 pm
Raio covalente (Bragg)
77 pm

Raios 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

Raios atômicos e metálicos

Raio atômico (Rahm)
190 pm
Raio metálico (C12)
86 pm

Escalas de numeração

Mendeleev
87
Pettifor
95
Glawe
87

Escalas de eletronegatividade

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

Polarizabilidade e dispersão

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

Parâmetros de Miedema

Volume molar de Miedema
3,26 cm3/mol
Densidade eletrônica de Miedema
6

Risco de abastecimento e economia

Concentração da produção
46
Risco relativo de abastecimento
5
Distribuição das reservas
28
Estabilidade política (maior produtor)
24
Estabilidade política (detentor das maiores reservas)
57

Transições de fase e alótropos

graphite Sublimação
Ponto de ebulição4098,15 K
Ponto triplo (temperatura)4762,15 K
Ponto triplo (pressão)10300 kPa

Categorias de estados de oxidação

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

Dados de referência avançados

Constantes de blindagem (3)
nOrbitalσ
1s0,3273
2p2,8642
2s2,7834
Detalhes dos raios cristalinos (3)
CargaCNSpinrcrystal (pm)Origem
4III6
4IV29Pauling's (1960) crystal radius,
4VI30Ahrens (1952) ionic radius,
Modos de decaimento dos isótopos (27)
IsótopoModoIntensidade
82p100%
9B+100%
9B+p7,5%
9B+A38,4%
10B+100%
11B+100%
14B-100%
15B-100%
16B-100%
16B-n99%
Fatores de espalhamento de raios X (502)
Energia (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

Dados adicionais

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)..

Referências (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).
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Referências

(9)
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 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
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 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
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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