A laboratory model for interstellar chemical evolution.
The chemistry in a supersonic plasma source flow was studied as a laboratory model for interstellar chemical evolution. It is important to match the similarity parameters for cosmic and laboratory conditions, which connect the temporal and spatial scales of the two cases. The apparatus simulated the conditions in a molecular cloud with respect to molecular-ionic reaction fraction, temperature, and non-equilibrium kinetics. The plasma flow was found to be cold enough, by the radical expansion, to produce polyatomic molecules. From the simple atomic plasma as reactant, cyanopolyyne and unsaturated hydrocarbons were synthesized in the present experiment. These molecules are also inherent in molecular clouds. The reaction mechanism is discussed.
Ishikawa
Y
Y
Institute of Space and Astronautical Science, Tokyo, Japan.
Kuriki
K
K
D003198:Computer Simulation; D019418:Evolution, Chemical; D005118:Extraterrestrial Environment; D006838:Hydrocarbons / Q000138:chemical synthesis / Q000737:chemistry; D007477:Ions; D008956:Models, Chemical; D017672:Nitrogen Compounds / Q000138:chemical synthesis / Q000737:chemistry; D017601:Oxygen Compounds / Q000138:chemical synthesis / Q000737:chemistry
D006838:Hydrocarbons; D007477:Ions; D017672:Nitrogen Compounds; D017601:Oxygen Compounds