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Fig. 3 | Progress in Earth and Planetary Science

Fig. 3

From: Asteroid Ryugu before the Hayabusa2 encounter

Fig. 3

The reduced V magnitude of Ryugu as a function of phase angle predicted by the Lommel-Seeliger model is shown compared with the ground-based measurements of Ishiguro et al. (2014) and references therein. Shown are the minimum (red dots), maximum (blue dashes), and nominal (black solid line) models. Our minimum and maximum models do not include the Mathilde data; however, our nominal model does. Reflectance rLS is in units of sr−1. Figure from Le Corre et al. (2018)

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