Hexaphenylbenzene

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Hexaphenylbenzene
Names
Preferred IUPAC name
23,24,25,26-Tetraphenyl-11,21:22,31-terphenyl
Other names
Hexaphenylbenzene
Identifiers
3D model (
JSmol
)
ChemSpider
ECHA InfoCard
 100.012.356 Edit this at Wikidata
UNII
  • InChI=1S/C42H30/c1-7-19-31(20-8-1)37-38(32-21-9-2-10-22-32)40(34-25-13-4-14-26-34)42(36-29-17-6-18-30-36)41(35-27-15-5-16-28-35)39(37)33-23-11-3-12-24-33/h1-30H checkY
    Key: QBHWPVJPWQGYDS-UHFFFAOYSA-N checkY
  • InChI=1/C42H30/c1-7-19-31(20-8-1)37-38(32-21-9-2-10-22-32)40(34-25-13-4-14-26-34)42(36-29-17-6-18-30-36)41(35-27-15-5-16-28-35)39(37)33-23-11-3-12-24-33/h1-30H
    Key: QBHWPVJPWQGYDS-UHFFFAOYAG
  • c1cc(ccc1)c3c(c(c(c(c3c2ccccc2)c4ccccc4)c5ccccc5)c6ccccc6)c7ccccc7
Properties
C42H30
Molar mass 534.702 g·mol−1
Appearance white solid
Melting point 454 to 456 °C (849 to 853 °F; 727 to 729 K)[1]
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
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Hexaphenylbenzene is an

phenyl rings. It is a colorless solid. The compound is the parent member of a wider class of hexaarylbenzenes, which are mainly of theoretical interest.[2]

Preparation

It is prepared by heating

Diels-Alder reaction to give the hexaphenyldienone, which then eliminates carbon monoxide.[1]

Hexaphenylbenzene synthesis

Together with 1,2,3,4-tetraphenylnaphthalene, hexaphenylbenzene forms by the chromium-catalyzed oligomerization of diphenylacetylene.[3] It may also be prepared by the dicobalt octacarbonyl-catalyzed alkyne trimerisation of diphenylacetylene.[2]

Diphenylacetylene cyclotrimerization using dicobalt octacarbonyl

Structure

Perspective view of the crystal structure of hexaphenylbenzene, showing the rotation of the phenyl rings. Hydrogen atoms have been omitted for clarity.[4]

The stable conformation of this molecule has the phenyl rings rotated out of the plane of the central benzene ring. The molecule adopts a propeller-like conformation in which the phenyl rings are rotated about 65°,[4] while in the gas phase, they are perpendicular with some slight oscillations.[5]

References

  1. ^
    doi:10.15227/orgsyn.046.0044
    .
  2. ^
    PMID 27498592.{{cite journal}}: CS1 maint: multiple names: authors list (link
    )
  3. doi:10.1021/ja01532a024.{{cite journal}}: CS1 maint: multiple names: authors list (link
    )
  4. ^
    doi:10.1107/S0567740868004176.[permanent dead link
    ]
  5. doi:10.1021/ja00463a034
    .
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