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The results of the present modeling suggest that the features, which appear in the reflectance spectra of active asteroids, may be induced by the light scattering on aggregate structures in their exospheres and they may serve as a tool for estimating the properties of these structures in terms of the composition and size of grains composing aggregates. Spectral measurements at shorter wavelengths than 0.35 μm can help to estimate more confidently the properties of weakly absorbing, both aggregate and homogeneous, particles in the exospheres of active asteroids.