When a planet revolves around a star in an elliptical orbit, moving the star's mass from one focus to another alters the orbital dynamics. The direction of the planet's revolution remains unchanged, but the angular velocity will be affected based on the planet's position in its orbit. If the star is moved while the planet is at periapsis, the planet's trajectory will adjust accordingly. Conversely, if the star is relocated while the planet is at apoapsis, the dynamics will also shift. The change in angular velocity occurs over a period of time rather than instantaneously.