Plans for ring-moon imaging after Daphnis on January 16 include Epimetheus and Mimas on January 30; Epimetheus and the propeller Santos-Dumont on February 21; Pan on March 7; the propeller Earhart on March 22; and Atlas on April 12. Not all of these attempts will result in images, though. The ring-moons have tiny masses and are tugged around in their orbits by all the larger moons as well as the rings themselves. It is wretchedly difficult to plan observations months in advance in which the moons will reliably appear where they are supposed to. That's why you get frustrating photos like this one of Pandora, with its weird smooth crescent falling off the edge of the frame.

On April 22, Cassini changes its orbit periapsis, bringing the ring-moon observation opportuities to an end, and ushering in the final phase of the mission.