Image Details

Choose export citation format:

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 2.

Equator-anchored cosine fit results for maria reflectance vs. wavelength. (a) Coefficient of determination (R2) indicating goodness of fit to the SZA-motivated model ﹩R(| \,\rm{lat}\,| )={R}_{\,\rm{eq}\,}+A(\cos | \,\rm{lat}\,| -1)﹩. (b) Normalized amplitude A/Req representing the fractional reflectance change from the equator to higher latitudes. NUV–NIR wavelengths (321–1548 nm) show A < 0 (increasing reflectance with increasing latitude), while Lyα (121.6 nm) shows A > 0 (decreasing reflectance with increasing latitude), both consistent with enhanced weathering at equatorial latitudes.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse