Similar to Fig. 4, but for phases during which the moon casts a shadow on the planet. The left ordinate now shows the angle φ_ms, which specifies the lunar position. Again, this angle was transformed to a time in hours, as shown on the right ordinate, where a time of 0 corresponds to the time when the planet, moon, and star are perfectly aligned. A single run of the shadow of the moon across the planetary surface corresponds to a passage through the color maps perpendicular to the abscissa.