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Variation in Lunar Regolith Space Weathering Relative to Latitude and Wavelength

  • Authors: C. Dany Waller, J. T. S. Cahill, K. D. Retherford, B. D. Byron, M. J. Poston, L. O. Magaña, A. R. Hendrix

C. Dany Waller et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 12.

(A) The global total reflectance at 1548 nm wavelength from the Kaguya/MI instrument. (B) Total latitudinal average of 1548 nm reflectance with a standard deviation envelope. (C) Only the mare regions of the global reflectance at 1548 nm wavelength. (D) Maria reflectance latitudinal average with a standard deviation envelope. (E) Only the highland regions of the global reflectance at 1548 nm wavelength. (F) Highlands reflectance latitudinal average with a standard deviation envelope. Horizontal dashed lines mark the ±55° feature in the right column.

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