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The Lunar Opposition Effect: Dual-mechanism Partitioning and Shallow-regolith Constraints from GaoFen-4 Photometry

  • Authors: Siyuan Li, 思源 李, Tianyi Xu, 天弈 徐, Yunzhao Wu, 昀昭 吴, Yanhe Yin, 延鹤 殷, Yi Xiu, 义 修, Songyi Xiao, 松毅 肖

Siyuan Li et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Terrain classification and CE-3 benchmark region. (a) Spatial distribution of the classified mare (blue) and highland (orange) units on the lunar disk using the GF-4 observation on 2018 July 25. (b) Histogram of B4 Lommel–Seeliger reduced reflectance (﹩{r}_{\mathrm{LS}}﹩) for all pixels and for the classified mare and highland subsets. (c) Geologic context of the CE-3 ROI. The geologic base map is modified from the United States Geological Survey (USGS) Unified Geologic Map of the Moon (C. M. Fortezzo et al. 2020).

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