What can meteorites tell us about comets?

Computer Science

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Catalysis, Chondrites, Comets, Interstellar Chemistry, Solar Corona, Anhydrides, Carbon Dioxide, Hydrogen Peroxide, Photochemical Reactions, Silicates

Scientific paper

Cometary and meteoritic matter, though originally interstellar, was reprocessed to varying degrees in the early solar system. The history of cometary matter can be inferred from various clues; specifically, the following questions are considered in this paper: (1) Anhydrous, Fe2+-bearing silicates: when and where did they form? (2) Hydrated silicates: if present, were they made by gaseous or liquid H2O? (3) Sources of organic compounds: ion-molecule reactions, photochemistry, grain catalysis. (4) Sources of CO2 and of organic polymer. (5) Interstellar molecules and grains in comets.

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