Fig. 6From: Compositional variations along the route of Chang’e-3 Yutu rover revealed by the lunar penetrating radarThe TiO2 (a), FeO (b), and their combined (c) contents at the CE-3 landing site (white stars). The data are derived from the Multispectral Imager data, and the maps are revised from Zhao et al. (2014). The white dashed line is the boundary between the Imbrian- (north) and Eratosthenian-aged mare units (down). North is up in all the panelsBack to article page