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Mare Crisium is one of the most prominent multi-ring basins on the nearside of the Moon. In this study, the regolith thermophysical features of Mare Crisium are studied with the CELMS data from CE-2 satellite. Several important results are as follows. Firstly, the current geological interpretation only by optical data is not enough, and a new geological perspective is provided. Secondly, the analysis of the low <i>T<sub>B</sub></i> anomaly combined with the (FeO+TiO<sub>2</sub>) abundance anddoi:10.5194/isprs-archives-xlii-3-1279-2018 fatcat:q4lcb2j2bvaa3jxx26chooxvdm