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

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

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icar...94..345c&link_type=abstract

Icarus (ISSN 0019-1035), vol. 94, Dec. 1991, p. 345-353. Research supported by NASA.

Computer Science

67

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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