Fig. 7

Comparison between the September 2007 (Vilas 2008) visible spectrum of Ryugu in the top panel and the visible spectrum of (101955) Bennu from Clark et al. (2011) in the bottom panel, with the mean spectra of the C-type (red) and B-type (blue) asteroids in the Erigone family. The standard deviation of the mean (±1σ) is shown with vertical lines.
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