Carbon-12
| Carbon-12 | |
|---|---|
| General | |
| Name, symbol | carbon 12 isotope,12C |
| Neutrons | 6 |
| Protons | 6 |
| Nuclide data | |
| Natural abundance | 98.89% |
| Parent isotopes | 12N 12B |
| Isotope mass | 12 u |
| Spin | 0 |
| Excess energy | 0± 0 keV |
| Binding energy | 92,161.753± 0.014 keV |
Carbon-12 is the more abundant of the two stable isotopes of the element carbon, accounting for 98.89% of carbon; it contains 6 protons, 6 neutrons, and 6 electrons.
Carbon-12 is of particular importance as it is used as the standard from which atomic masses of all nuclides are measured: its mass number is by definition 12.
Contents |
History
Prior to 1959 both the IUPAP and IUPAC tended to use oxygen to define the mole, the chemists defining the mole as the number of atoms of oxygen which had mass 16 g, the physicists using a similar definition but with the oxygen-16 isotope only. The two organizations agreed in 1959/60 to define the mole as follows.
The mole is the amount of substance of a system which contains as many elementary entities as there are atoms in 0.012 kilogram of carbon 12; its symbol is "mol."
This was adopted by the CIPM (International Committee for Weights and Measures) in 1967, and in 1971 it was adopted by the 14th CGPM (General Conference on Weights and Measures).
In 1961 the isotope carbon-12 was selected to replace oxygen as the standard relative to which the atomic weights of all the other elements are measured.[1]
In 1980 the CIPM clarified the above definition, defining that the carbon-12 atoms are unbound and in their ground state.
Hoyle state
The Hoyle state is an excited state of carbon-12 with precisely the properties necessary to allow just the right amount of carbon to be created in a stellar environment. The existence of the Hoyle state is essential for the nucleosynthesis of carbon in helium-burning red giant stars. The resonant state was predicted by Fred Hoyle in the 1950s based on the observed abundances of heavy elements in the universe. The resonant state allows carbon to be produced via the triple-alpha process. The existence of the Hoyle state has been confirmed but its precise properties are still being investigated.[2]
Isotopic purification
The isotopes of carbon can be separated in the form of carbon dioxide gas by cascaded chemical exchange reactions with amine carbamate.[3]
See also
References
- ^ "Atomic Weights and the International Committee - A Historical Review". 2004-01-26. http://www.iupac.org/publications/ci/2004/2601/1_holden.html.
- ^ Chernykh, M.; Feldmeier, H.; Neff, T.; Von Neumann-Cosel, P.; Richter, A. (2007). "Structure of the Hoyle State in C12". Physical Review Letters 98 (3): 032501. doi:10.1103/PhysRevLett.98.032501. PMID 17358679. http://www.nscl.msu.edu/~jina/jinaastroclub/papers/Neff.pdf.
- ^ Kenji Takeshita and Masaru Ishidaa (December 2006). "Optimum design of multi-stage isotope separation process by exergy analysis". ECOS 2004 - 17th International Conference on Efficiency, Costs, Optimization, Simulation, and Environmental Impact of Energy on Process Systems 31 (15): 3097-3107. http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6V2S-4KKNN4B-1&_user=10&_rdoc=1&_fmt=&_orig=search&_sort=d&_docanchor=&view=c&_searchStrId=992584935&_rerunOrigin=google&_acct=C000050221&_version=1&_urlVersion=0&_userid=10&md5=0e06e1cde32ec309cbf21937b8171853.
| Lighter: carbon-11 |
Carbon-12 is an isotope of carbon |
Heavier: carbon-13 |
| Decay product of: boron-12, nitrogen-12 |
Decay chain of Carbon-12 |
Decays to: stable |
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