Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  



























Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Properties  



1.1  Electromagnetic properties  







2 Reactions  





3 History  





4 See also  





5 References  














Diatomic carbon






تۆرکجه

Čeština
Español
فارسی
Français
Bahasa Indonesia

Русский
Српски / srpski
Srpskohrvatski / српскохрватски
Українська
Tiếng Vit

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 


















From Wikipedia, the free encyclopedia
 


Diatomic carbon
Names
IUPAC name

Diatomic carbon

Systematic IUPAC name

Ethenediylidene (substitutive)
Dicarbon(CC) (additive)

Identifiers

CAS Number

3D model (JSmol)

ChEBI
ChemSpider

Gmelin Reference

196

PubChem CID

CompTox Dashboard (EPA)

  • InChI=1S/C2/c1-2 checkY

    Key: LBVWYGNGGJURHQ-UHFFFAOYSA-N checkY

  • [C]=[C]

Properties

Chemical formula

C2
Molar mass 24.022 g·mol−1

Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).

Infobox references

Diatomic carbon (systematically named dicarbon and 2,2λ2-ethene), is a green, gaseous inorganic chemical with the chemical formula C=C (also written [C2] or C2). It is kinetically unstable at ambient temperature and pressure, being removed through autopolymerisation. It occurs in carbon vapor, for example in electric arcs; in comets, stellar atmospheres, and the interstellar medium; and in blue hydrocarbon flames.[1] Diatomic carbon is the second simplest of the allotropes of carbon (after atomic carbon), and is an intermediate participator in the genesis of fullerenes.

Properties[edit]

C2 is a component of carbon vapor. One paper estimates that carbon vapor is around 28% diatomic,[2] but theoretically this depends on the temperature and pressure.

Electromagnetic properties[edit]

The electrons in diatomic carbon are distributed among the molecular orbitals according to the Aufbau principle to produce unique quantum states, with corresponding energy levels. The state with the lowest energy level, or ground state, is a singlet state (1Σ+
g
), which is systematically named ethene-1,2-diylidene or dicarbon(0•). There are several excited singlet and triplet states that are relatively close in energy to the ground state, which form significant proportions of a sample of dicarbon under ambient conditions. When most of these excited states undergo photochemical relaxation, they emit in the infrared region of the electromagnetic spectrum. However, one state in particular emits in the green region. That state is a triplet state (3Πg), which is systematically named ethene-μ,μ-diyl-μ-ylidene or dicarbon(2•). In addition, there is an excited state somewhat further in energy from the ground state, which only form a significant proportion of a sample of dicarbon under mid-ultraviolet irradiation. Upon relaxation, this excited state fluoresces in the violet region and phosphoresces in the blue region. This state is also a singlet state (1Πg), which is also named ethene-μ,μ-diyl-μ-ylidene or dicarbon(2•).

State Excitation
enthalpy
(kJ mol−1)
Relaxation
transition
Relaxation
wavelength
Relaxation EM-region
X1Σ+
g
0
a3Π
u
8.5 a3Π
u
X1Σ+
g
14.0 μm Long-wavelength infrared
b3Σ
g
77.0 b3Σ
g
a3Π
u
1.7 μm Short-wavelength infrared
A1Π
u
100.4 A1Π
u
X1Σ+
g

A1Π
u
b3Σ
g
1.2 μm
5.1 μm
Near infrared
Mid-wavelength infrared
B1Σ+
g
? B1Σ+
g
A1Π
u

B1Σ+
g
a3Π
u
?
?
?
?
c3Σ+
u
159.3 c3Σ+
u
b3Σ
g

c3Σ+
u
X1Σ+
g

c3Σ+
u
B1Σ+
g
1.5 μm
751.0 nm
?
Short-wavelength infrared
Near infrared
?
d3Π
g
239.5 d3Π
g
a3Π
u

d3Π
g
c3Σ+
u

d3Π
g
A1Π
u
518.0 nm
1.5 μm
860.0 nm
Green
Short-wavelength infrared
Near infrared
C1Π
g
409.9 C1Π
g
A1Π
u

C1Π
g
a3Π
u

C1Π
g
c3Σ+
u
386.6 nm
298.0 nm
477.4 nm
Violet
Mid-ultraviolet
Blue

Molecular orbital theory shows that there are two sets of paired electrons in a degenerate pi bonding set of orbitals. This gives a bond order of 2, meaning that there should exist a double bond between the two carbon atoms in a C2 molecule.[3] One analysis suggested instead that a quadruple bond exists,[4] an interpretation that was disputed.[5] CASSCF calculations indicate that the quadruple bond based on molecular orbital theory is also reasonable.[3] Bond dissociation energies (BDE) of B2, C2, and N2 show increasing BDE, indicating single, double, and triple bonds, respectively.

In certain forms of crystalline carbon, such as diamond and graphite, a saddle point or "hump" occurs at the bond site in the charge density. The triplet state of C2 does follow this trend. However, the singlet state of C2 acts more like siliconorgermanium; that is, the charge density has a maximum at the bond site.[6]

Reactions[edit]

Diatomic carbon will react with acetone and acetaldehyde to produce acetylene by two different pathways.[2]

History[edit]

C/2014 Q2 (Lovejoy) glows green due to diatomic carbon.
C/2022 E3 (ZTF) also looks green.

The light of gas-rich comets mainly originates from the emission of diatomic carbon. An example is C/2014 Q2 (Lovejoy), where there are several lines of C2 light, mostly in the visible spectrum[10] , forming the Swan bands.[11] C/2022 E3 (ZTF), visible in early 2023, also exhibits green color due to the presence of diatomic carbon.[12]

See also[edit]

References[edit]

  1. ^ Hoffmann, Roald (1995). "Marginalia: C2 In All Its Guises" (PDF). American Scientist. 83 (4): 309–311. Bibcode:1995AmSci..83..309H. JSTOR 29775475. Archived from the original (PDF) on 2023-03-21. Retrieved 2017-07-22.
  • ^ a b c d Skell, Philip S.; Plonka, James H. (1970). "Chemistry of the singlet and triplet C2 molecules. Mechanism of acetylene formation from reaction with acetone and acetaldehyde". Journal of the American Chemical Society. 92 (19): 5620–5624. doi:10.1021/ja00722a014.
  • ^ a b Zhong, Ronglin; Zhang, Min; Xu, Hongliang; Su, Zhongmin (2016). "Latent harmony in dicarbon between VB and MO theories through orthogonal hybridization of 3σg and 2σu". Chemical Science. 7 (2): 1028–1032. doi:10.1039/c5sc03437j. PMC 5954846. PMID 29896370.
  • ^ Shaik, Sason; Danovich, David; Wu, Wei; Su, Peifeng; Rzepa, Henry S.; Hiberty, Philippe C. (2012). "Quadruple bonding in C2 and analogous eight-valence electron species". Nature Chemistry. 4 (3): 195–200. Bibcode:2012NatCh...4..195S. doi:10.1038/nchem.1263. PMID 22354433.
  • ^ Grunenberg, Jörg (2012). "Quantum chemistry: Quadruply bonded carbon". Nature Chemistry. 4 (3): 154–155. Bibcode:2012NatCh...4..154G. doi:10.1038/nchem.1274. PMID 22354425.
  • ^ Chelikowsky, James R.; Troullier, N.; Wu, K.; Saad, Y. (1994). "Higher-order finite-difference pseudopotential method: An application to diatomic molecules". Physical Review B. 50 (16): 11356–11364. Bibcode:1994PhRvB..5011355C. doi:10.1103/PhysRevB.50.11355. PMID 9975266.
  • ^ Skell, P. S.; Fagone, F. A.; Klabunde, K. J. (1972). "Reaction of Diatomic Carbon with Alkanes and Ethers/ Trapping of Alkylcarbenes by Vinylidene". Journal of the American Chemical Society. 94 (22): 7862–7866. doi:10.1021/ja00777a032.
  • ^ Miyamoto, Kazunori; Narita, Shodai; Masumoto, Yui; Hashishin, Takahiro; Osawa, Taisei; Kimura, Mutsumi; Ochiai, Masahito; Uchiyama, Masanobu (2020-05-01). "Room-temperature chemical synthesis of C 2". Nature Communications. 11 (1): 2134. Bibcode:2020NatCo..11.2134M. doi:10.1038/s41467-020-16025-x. ISSN 2041-1723. PMC 7195449. PMID 32358541.
  • ^ Rzepa, Henry S. (2021-02-23). "A thermodynamic assessment of the reported room-temperature chemical synthesis of C 2". Nature Communications. 12 (1): 1241. Bibcode:2021NatCo..12.1241R. doi:10.1038/s41467-021-21433-8. ISSN 2041-1723. PMC 7902603. PMID 33623013.
  • ^ Venkataramani, Kumar; Ghetiya, Satyesh; Ganesh, Shashikiran; et, al. (2016). "Optical spectroscopy of comet C/2014 Q2 (Lovejoy) from the Mount Abu Infrared Observatory". Monthly Notices of the Royal Astronomical Society. 463 (2): 2137–2144. arXiv:1607.06682. Bibcode:2016MNRAS.463.2137V. doi:10.1093/mnras/stw1820.
  • ^ Mikuz, Herman; Dintinjana, Bojan (1994). "CCD Photometry of Comets". International Comet Quarterly. Retrieved October 26, 2006.
  • ^ Georgiou, Aristos (2023-01-10). "What makes the green comet green?". Newsweek. Archived from the original on 2023-01-25. Retrieved 2023-01-25.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Diatomic_carbon&oldid=1214392984"

    Categories: 
    Astrochemistry
    Allotropes of carbon
    Homonuclear diatomic molecules
    Hidden categories: 
    Articles without InChI source
    Articles without KEGG source
    Articles without UNII source
    Articles with changed CASNo identifier
    Articles containing unverified chemical infoboxes
    Articles with short description
    Short description matches Wikidata
     



    This page was last edited on 18 March 2024, at 17:54 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki