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Table 2 Lommel-Seeliger functions that predict [I/ℱ] (i, e, α) (reflectance) of Ryugu at 550 nm. ALS is Lommel-Seeliger Albedo and f(α) = \( {e}^{\beta \alpha +\gamma {\alpha}^2+\delta {\alpha}^3} \). Table from Le Corre et al. (2018)

From: Asteroid Ryugu before the Hayabusa2 encounter

 

A LS

β

γ

δ

Nominal

0.027

− 4.14 × 10−2

3.22 × 10−4

19.16 × 10−7

Maximum

0.030

− 3.99 × 10−2

3.27 × 10−4

22.15 × 10−7

Minimum

0.024

− 4.46 × 10−2

3.77 × 10−4

21.33 × 10−7