Cometary implications of recent laboratory experiments on the photochemistry of the C2H and C3H2 radicals

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Carbon Compounds, Cometary Atmospheres, Comets, Energy Distribution, Photochemical Reactions, Photodissociation, Photolysis, Radicals, Absorption Cross Sections, Absorption Spectra, Atomic Energy Levels, Emission Spectra, Quantum Chemistry

Scientific paper

Recent laboratory results on the photodissociation of the C2H and C3H2 radicals are described. These studies show that the C2 and C3 radicals are produced by the 193 nm photolysis of the C2H and C3H2 radicals, respectively. The quantum state distributions that were determined for the C2 radicals put certain constraints on the initial conditions for any models of the observed C2 cometary spectra. Experimental observations of C2 formed by the 212.8 nm photolysis of C2H are used to calculate a range of photochemical lifetimes for the C2H radical.

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