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The methyl radical CH3 is stable enough to be observable under laboratory conditions in a dilute gas, although it readily dimerizes to ethane. It is an important intermediary in gas-phase interstellar chemistry. The incorporation of a methyl group, −CH3, into organic compounds can have fundamental biological effects.
History
The CH3 radical was detected in interstellar molecular clouds at wavelengths of about 16 microns using the Infrared Space Observatory (Feuchtgruber et al. 2000).
References and Further Reading
Feuchtgruber H, Helmich FP, van Dishoeck EF, Wright CM (2000) Detection of interstellar CH3. Astrophys J 535:L111–L114
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© 2014 Springer-Verlag Berlin Heidelberg
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Irvine, W.M. (2014). Methyl Radical. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1819-4
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1819-4
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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)- Published:
- 11 April 2019
DOI: https://doi.org/10.1007/978-3-642-27833-4_1819-5
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Methyl Radical- Published:
- 24 April 2015
DOI: https://doi.org/10.1007/978-3-642-27833-4_1819-4