Resolved spectrophotometric properties of the Ceres surface from Dawn Framing Camera images

•We evaluate photometric models for the surface of Ceres as seen in Dawn images.•We present global maps of the normal albedo, phase curve steepness, and color.•The blue color of fresh terrain may be due to dehydrated phyllosilicates.•The bright spot in Occator crater has an unusually steep phase function.•We find no evidence for haze in Occator.