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Compositional characterisation of the Themis family

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Academic year: 2021

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Fig. 1. Top: best fit (red) to the spectra of the Themis family mem- mem-bers (black) using a Rayleigh scattering model
Fig. 2. VNIR spectral slopes versus albedos for 19 Themis family mem- mem-bers. The size of the circles is proportional to the diameter of the objects.
Table 4. Composition of the VNIR best-fit model obtained for each asteroid.
Fig. 3. Reflectance spectra of the minerals used in the modelling proce- proce-dure as calculated from the Mie-Hapke radiative transfer code
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