The origin of the polycyclic aromatic hydrocarbons in meteorites

@article{Wing2005TheOO,
  title={The origin of the polycyclic aromatic hydrocarbons in meteorites},
  author={Michael R. Wing and Jeffrey L. Bada},
  journal={Origins of life and evolution of the biosphere},
  year={2005},
  volume={21},
  pages={375-383}
}
  • M. R. Wing, J. Bada
  • Published 2005
  • Chemistry
  • Origins of life and evolution of the biosphere
Polycyclic aromatic hydrocarbons (PAHs) in C1 and C2 Carbonaceous Chondrites appear to be the product of a high-temperature synthesis. This observation counters a prevailing view that PAHs in meteorites are a thermal alternation product of preexisting aliphatic compounds, which in turn required the presence of low-temperature mineral phases such as magnetite and hydrated phyllosilicates for their formation. Such a process would necessarily lead to a more low-temperature assemblage of PAHs, as… Expand

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