K. Mimura et al., HYDROCARBON GASES AND AROMATIC-HYDROCARBONS PRODUCED BY IMPACT SHOCK FROM FROZEN BENZENE - COSMOCHEMICAL SIGNIFICANCE, Earth and planetary science letters, 133(3-4), 1995, pp. 265-269
Shock waves trigger reactions in solid benzene at 77 K to produce hydr
ogen, light alkanes from C-1 to C-3, light alkenes from C-2 to C-3, ac
etylene, aromatic hydrocarbons with high-molecular weights ranging fro
m 102 (phenylacetylene) to 306 (quaterphenyl), and unknown carbonaceou
s materials. These products are similar to those yielded by rapidly qu
enched pyrolysis. Shock synthesis favours the formation of compounds w
ith metapositions in these structural isomers. The reaction mechanism
producing aromatic hydrocarbons with low molecular weights is vague at
present, but it cannot be a simple radical reaction. Most of shock-de
rived products are detected in carbonaceous chondrites. These results
suggest that many sorts of hydrocarbons in solar materials such as met
eorites have been produced by frequent and violent shocks throughout t
he history of the solar system. In particular, this process may be res
ponsible for the formation of extraterrestrial unsaturated hydrocarbon
gases.