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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 3.

(A) The global total reflectance at 121.6 nm (Lyα) wavelength from the LRO/LAMP instrument. (B) Total latitudinal average of 121.6 nm reflectance with a standard deviation envelope. (C) Only the mare regions of the global reflectance at 121.6 nm wavelength. (D) Maria reflectance latitudinal average with a standard deviation envelope. (E) Only the highland regions of the global reflectance at 121.6 nm wavelength. (F) Highlands reflectance latitudinal average with a standard deviation envelope. Horizontal dashed lines mark ±55° latitude.

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