Laplace's Tidal Equations

Laplace’s Tidal Equations describe the movement of ocean waters caused by gravitational forces, primarily from the moon and sun. They are a set of mathematical formulas that account for how these forces create tides, considering factors like the Earth's rotation, the shape of ocean basins, and gravity. Essentially, they model how water is pulled toward celestial bodies, resulting in rising and falling sea levels in different locations. These equations help scientists predict tides, understand ocean circulation, and study how water responds to gravitational forces on a planetary scale.