Remote comets and related bodies - VJHK colorimetry and surface materials

Astronomy and Astrophysics – Astronomy

Scientific paper

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Asteroids, Astronomical Photometry, Colorimetry, Comets, Planetary Surfaces, Solar System, Comet Nuclei, Diagrams, Infrared Astronomy, Natural Satellites, Spectral Reflectance, Spectrophotometry

Scientific paper

VJHK colors for a number of asteroids and eight comets at various solar distances and levels of activity were obtained, and the observations are interpreted in terms of a two-component mixing model in which outer solar system interplanetary bodies are viewed as mixtures of ice and dark carbonaceous-type (RD and C) dirt. It is inferred that the observed comets have comae, and perhaps surfaces, of dirty ice or ice dirt grains colored by an RD-dirt component. This inference is supported by systematics of an 'alpha index' based on VJHK colors and empirically correlated with albedo and ice/dirt ratio. Among comets the alpha index correlates with solar distance in a way that suggests comets emit dirty ice grains which are stable at large solar distance but from which the ice component sublimes and leaves dirt grains at small solar distance.

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