Astronomy
The Moon’s hidden edges
Increase orbital eccentricity and follow the difference between uniform rotation and nonuniform orbital motion. Surface markers reveal the rocking.

The model and its limits
Keplerian orbit with uniform synchronous spin; latitude libration is a prescribed axial tilt. Physical libration and solar perturbations are omitted.
Equations used in the module
Equations E - e sin E = M; tan(ν/2) = √((1+e)/(1-e)) tan(E/2); libration = ν - M


