The surface composition of Jupiter Trojans: Visible and near-infrared survey of dynamical families
Asteroid dynamical families are supposed to be formed from the collisional disruption of parent bodies. As a consequence, the investigation of the surface properties of small and large family members may give some hints on the nature of the dynamical group, the internal composition of the parent body, and the role played by space weathering
Dotto, E. et al.
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2006