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Lunar Geochemistry from X-Ray Line Flux Ratios Using CLASS on Chandrayaan-2

  • Authors: R. Kumar, Y. Rai, S. Srijan, A. Bansal, Ameya V. Singh, A. Kumar, H. Mhatre, M. Goyal, S. Swain, S. Patidar, Aditya P. Saikia, A. Ahmad, S. Narendranath, Netra S. Pillai, R. Kashyap, V. Bhalerao

R. Kumar et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 4.

Lunar XRF line-intensity ratio maps from CLASS data. Mg/Al and Al/Si best represent the distinction between the major lunar terranes. High Mg/Si values are not restricted to mare, while FeL/Si is higher in mare but not so evidently in the SPAT. Black lines are mare boundaries from LROC data. As mentioned in Section 2.2, Mg/Al and Al/Si maps were created using 96 s data bins, while the Mg/Si and FeL/Si maps used 296 s binning.

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