Comet dust as a mixture of aggregates and solid particles: model consistent with ground-based and space-mission results

The most Successful model of cornet dust presents comet particles as aggregates Of submicron grains. It qualitatively explains the spectral and angular change in the comet brig h the ss and polarization and is consistent with the thermal infrared data and composition of the Cornet dust obtained in situ for comet 1P/Halley. However. it experiences some difficulties ill providing a quantitative fit to the observational data. Here we present it model that considers Cornet dust as a mixture of aggregates and compact particles, The model is based oil the Giotto and Stardust Mission findings that both aggregates (made mainly of organics, silicates, and carbon) and solid Silicate particles are present in the comet dust. We simulate aggregates as Ballistic Cluster-Cluster Aggregates (BCCA) and compact particles as polydisperse spheroids with some distribution of the aspect ratio. The particles follow it power-law size distribution with the power -3 that is close to the one obtained for comet dust ill situ, at Studies of the Stardust returned samples, and the results Of ground-based observations of cornets. The model provides a good fit to the angular polarization Curve. It also reproduces the positive spectral gradient of polarization. Led color of the dust, and low albedo. It also has the ratio of compact to fluffy particles close to the one found in Situ for comet 1P/Halley and the mass ratio of silicate to carbonaceous Materials equal to unity that is in accordance with the elemental abundances of Halley's dust found by Giotto mission.