The study of the physics of cometary nuclei

Details The study of the physics of cometary nuclei The study of the physics of cometary nuclei

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983sao..reptq....w&link_type=abstract

Semiannual Progress Report, 1 Oct. 1982 - 31 Mar. 1983 Smithsonian Astrophysical Observatory, Cambridge, MA.

Other

Comet Nuclei, Gas Jets, Gas-Solid Interfaces, Halos, Meteoroid Dust Clouds, Periodic Variations, Spin-Orbit Interactions, Angular Momentum, Halley'S Comet, Histories, Ice, Solar Heating, Solar System, Spectroscopy, Sun, Time Lag, Vaporizing

Scientific paper

On the basis of the icy conglometate model of cometary nuclei various observations demonstrate the spotted nature of many or most nuclei, i.e., regions of unusual activity, either high or low. Rotation periods, spin axes and even precession of the axes have been determined. Narrow dust jets near the nuclei of some bright comets require that small sources be embedded in larger active areas. Certain evidence suggests that very dusty areas and very dusty comets may be less active, respectively, than surrounding areas or other comets.

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