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Methyl radical

From Wikipedia, the free encyclopedia
Methyl radical
Names
IUPAC name
Methyl[1]
Identifiers
3D model (JSmol)
1696831
ChEBI
ChemSpider
57
MeSHMethyl+radical
UNII
  • InChI=1S/CH3/h1H3 checkY
    Key: WCYWZMWISLQXQU-UHFFFAOYSA-N checkY
  • [CH3]
Properties
CH3
Molar mass15.035 g·mol−1
Except where otherwise noted, data are given for materials in theirstandard state (at 25 °C [77 °F], 100 kPa).
Chemical compound

Methyl radical is anorganic compound with thechemical formulaCH
3
(also written as[CH
3
]
). It is a metastable colourless gas, which is mainly producedin situ as a precursor to other hydrocarbons in the petroleum cracking industry. It can act as either a strongoxidant or a strongreductant, and is quite corrosive to metals.

Chemical properties

[edit]

Its first ionization potential (yielding themethenium ion,CH+
3
) is9.837±0.005 eV.[2]

Redox behaviour

[edit]

The carbon centre in methyl can bond with electron-donating molecules by reacting:

CH
3
+ RRCH
3

Because of the capture of the nucleophile (R), methyl has oxidising character. Methyl is a strong oxidant with organic chemicals. However, it is equally a strong reductant with chemicals such as water. It does not form aqueous solutions, as it reduces water to producemethanol and elemental hydrogen:

CH
3
+ 2 H
2
O
→ 2 CH
3
OH
+H
2

Structure

[edit]

Themolecular geometry of the methyl radical istrigonal planar (bond angles are 120°), although the energy cost of distortion to apyramidal geometry is small. All other electron-neutral, non-conjugated alkyl radicals are pyramidalized to some extent, though with very small inversion barriers. For instance, thet-butyl radical has a bond angle of 118° with a 0.7 kcal/mol (2.9 kJ/mol) barrier topyramidal inversion. On the other hand, substitution of hydrogen atoms by more electronegative substituents leads to radicals with a strongly pyramidal geometry (112°), such as thetrifluoromethyl radical,CF
3
, with a much more substantial inversion barrier of around 25 kcal/mol (100 kJ/mol).[3]

Chemical reactions

[edit]

Methyl undergoes the typical chemical reactions of a radical. Below approximately 1,100 °C (1,400 K), it rapidly dimerises to formethane. Upon treatment with an alcohol, it converts tomethane and either an alkoxy or hydroxyalkyl. Reduction of methyl gives methane. When heated above, at most, 1,400 °C (1,700 K), methyl decomposes to producemethylidyne and elemental hydrogen, or to producemethylene and atomic hydrogen:

CH
3
→ CH +H
2
CH
3
CH
2
+ H

Methyl is very corrosive to metals, forming methylated metal compounds:

M +n CH
3
→ M(CH3)n

Production

[edit]

Biosynthesis

[edit]

Someradical SAM enzymes generate methyl radicals by reduction of S-adenosylmethionine.[4]

Acetone photolysis

[edit]

It can be produced by the ultraviolet photodissociation ofacetone vapour at 193 nm:[5]

C
3
H
6
O
→ CO + 2 CH
3

Halomethane photolysis

[edit]

It is also produced by the ultraviolet dissociation ofhalomethanes:

CH
3
X
→ X +CH
3

Methane oxidation

[edit]
Further information:Atmospheric methane § Removal processes

It can also be produced by the reaction ofmethane with thehydroxyl radical:

OH + CH4CH
3
+ H2O

This process begins the major removal mechanism of methane from the atmosphere. The reaction occurs in thetroposphere orstratosphere. In addition to being the largest known sink for atmospheric methane, this reaction is one of the most important sources of water vapor in the upper atmosphere.

This reaction in thetroposphere gives a methane lifetime of 9.6 years. Two more minor sinks are soil sinks (160 year lifetime) and stratospheric loss by reaction withOH,Cl andO1D in the stratosphere (120 year lifetime), giving a net lifetime of 8.4 years.[6]

Azomethane pyrolysis

[edit]

Methyl radicals can also be obtained bypyrolysis ofazomethane, CH3N=NCH3, in a low-pressure system.

In the interstellar medium

[edit]

Methyl was discovered ininterstellar medium in 2000 by a team led by Helmut Feuchtgruber who detected it using theInfrared Space Observatory. It was first detected in molecular clouds toward the centre of the Milky Way.[7]

References

[edit]
  1. ^International Union of Pure and Applied Chemistry (2014).Nomenclature of Organic Chemistry: IUPAC Recommendations and Preferred Names 2013.The Royal Society of Chemistry. p. 1051.doi:10.1039/9781849733069.ISBN 978-0-85404-182-4.
  2. ^Golob, L.; Jonathan, N.; Morris, A.; Okuda, M.; Ross, K.J. (1972). "The first ionization potential of the methyl radical as determined by photoelectron spectroscopy".Journal of Electron Spectroscopy and Related Phenomena.1 (5):506–508.Bibcode:1972JESRP...1..506G.doi:10.1016/0368-2048(72)80022-7.
  3. ^Anslyn E.V. and Dougherty D.A.,Modern Physical Organic Chemistry (University Science Books, 2006), p.57
  4. ^Ribbe, M. W.; Hu, Y.; Hodgson, K. O.; Hedman, B. (2014)."Biosynthesis of Nitrogenase Metalloclusters".Chemical Reviews.114 (8):4063–4080.doi:10.1021/cr400463x.PMC 3999185.PMID 24328215.
  5. ^Hall, G. E.; Vanden Bout, D.; Sears, Trevor J. (1991)."Photodissociation of acetone at 193 nm: Rotational- and vibrational-state distributions of methyl fragments by diode laser absorption/gain spectroscopy".The Journal of Chemical Physics.94 (6).AIP Publishing: 4182.Bibcode:1991JChPh..94.4182H.doi:10.1063/1.460741.
  6. ^"Trace Gases: Current Observations, Trends, and Budgets".Climate Change 2001, IPCC Third Assessment Report. IPCC/United Nations Environment Programme.
  7. ^"ISO detects a new molecule in interstellar space".Science & Technology.European Space Agency. Retrieved17 June 2013.
Molecules
Diatomic








Triatomic
Four
atoms
Five
atoms
Six
atoms
Seven
atoms
Eight
atoms
Nine
atoms
Ten
atoms
or more
Deuterated
molecules
Unconfirmed
Related
Alkali metal
(Group 1) hydrides
Alkaline (Group 2)
earth hydrides
Monohydrides
Dihydrides
Group 13
hydrides
Boranes
Alanes
Gallanes
Indiganes
Thallanes
Nihonanes(predicted)
  • NhH
  • NhH3
  • Nh2H6
  • NhH5
Group 14 hydrides
Hydrocarbons
Silanes
Silenes
Silynes
Germanes
Stannanes
Plumbanes
Flerovanes(predicted)
  • FlH
  • FlH2
  • FlH4
Pnictogen
(Group 15) hydrides
Azanes
Azenes
Phosphanes
Phosphenes
Arsanes
Stibanes
Bismuthanes
Moscovanes
Hydrogen
chalcogenides
(Group 16 hydrides)
Polyoxidanes
Polysulfanes
Selanes
Tellanes
Polanes
Livermoranes
Hydrogen halides
(Group 17 hydrides)
  • HF
  • HCl
  • HBr
  • HI
  • HAt
  • HTs(predicted)
  • Transition
    metal hydrides
    Lanthanide
    hydrides
    Actinide
    hydrides
    Exotic matter hydrides
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