The distribution of dust in the inner coma of comet IRAS-Araki-Alcock (1983d)

Physics

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Comet Nuclei, Cometary Atmospheres, Cosmic Dust, Iras-Araki-Alcock Comet, Brightness Distribution, Grain Size, High Resolution, Image Analysis, Infrared Imagery, Near Infrared Radiation, Spectral Resolution, Visual Observation, Comets, Iras-Araki-Alcock, Distribution, Dust, Comae, Near-Infrared, Imagery, Scattering, Grains, Emissions, Brightness, Fragmentation, Comet Nuclei, Size, Diameter, Analysis, Earth-Based Observations, Telescope Methods, Mantle

Scientific paper

The behavior and characteristics of the inner coma of the Comet IRAS-Araki-Alcock (IAA) were examined for five nights in May 1983 using a ground-based 2.2 m CCD telescope. A highly variable, asymmetric sunward emission was detected, along with a long filamentary structure. The brightness was highest in the sunward direction, with radial brightnesses diminishing more slowly than predicted with a 1/r model. The slow fall-off is attributed to the emission of conglomerate dust grains which fragment while traveling through the inner coma and increase the effective surface area of the dust. Significant day-to-day variations were observed, and the filamentary features were indicative of a centralized region on a mantled nucleus which rotated. The nucleus is estimated to be no more than 17 km in diameter.

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