Image Details
Caption: Figure 11.
(A) The global total reflectance at 1248 nm wavelength from the Kaguya/MI instrument. (B) Total latitudinal average of 1248 nm reflectance with a standard deviation envelope. (C) Only the mare regions of the global reflectance at 1248 nm wavelength. (D) Maria reflectance latitudinal average with a standard deviation envelope. (E) Only the highland regions of the global reflectance at 1248 nm wavelength. (F) Highlands reflectance latitudinal average with a standard deviation envelope. Horizontal dashed lines mark the ±55° feature in the right column.
© 2026. The Author(s). Published by the American Astronomical Society.