Catalysis by dust grains in the solar nebula.

Details Catalysis by dust grains in the solar nebula. Catalysis by dust grains in the solar nebula.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339..149k&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 149 - 154

Computer Science

Solar Nebula: Chemistry, Solar Nebula: Dust Grains

Scientific paper

In order to determine whether grain-catalyzed reactions played an important role in the chemistry of the solar nebula, the authors applied their time-dependent model of methane formation via Fischer-Tropsch catalysis to pressures from 10-5 to 1 bar and temperatures from 450 to 650K. Results indicate that under certain nebular conditions, conversion of CO to methane could be extremely efficient in the presence of iron-nickel dust grains over timescales very short compared to the lifetime of the solar nebula.

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