Solid C triple bond N bearing material on outer solar system bodies

Computer Science

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Asteroids, Cyano Compounds, Interstellar Matter, Solar System, Spectral Reflectance, Iapetus, Solid Phases, Uranus Rings

Scientific paper

Recent telescopic observations have led to the identification of cyanogroup-containing molecules in the dark surface solids of several D-class asteroids, cometary dusts, and the rings of Uranus, as well as the low-albedo atmosphere of Iapetus. The occurrence of the 2.2-micron overtone of C triple-bond N's stretching fundamental mode in all four classes of small solar system bodies is presently suggested to serve as a diagnostic of both exposure duration and degree of modification of surface materials.

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