The theory of tides is the application of continuum mechanics to interpret and predict the tidal deformations of planetary and satellite bodies and their atmospheres and oceans, under the gravitational loading of another astronomical body or bodies. It commonly refers to the fluid dynamic motions for the Earth's oceans.
Tidal physics
Tidal forcing
The forces discussed here apply to body (Earth tides), oceanic and atmospheric tides. Atmospheric tides on Earth, however, tend to be dominated by forcing due to solar heating.
On the planet (or satellite) experiencing tidal motion consider a point at latitude and longitude at distance from the center of mass, then point can written in cartesian coordinates as where
:
Let be the declination and be the right ascension of the deforming body, the Moon for example, then the vector direction is
:
and be the orbital distance between the center of masses and the mass of the body. Then the force on the point is
:
where For a circular orbit the angular momentum centripetal acceleration balances gravity at the planetary center of mass
:
where is the distance between the center of mass for the orbit and planet and is the planetary mass.Consider the point in the reference fixed without rotation, but translating at a fixed translation with respect to the center of mass of the planet. The body's centripetal force acts on the point so that the total force is
:
Substituting for center of mass acceleration, and reordering
:In ocean tidal forcing, the radial force is not significant, the next step is to rewrite the coefficient. Let then
:
where is the inner product determining the angle "z" of the deforming body or Moon from the zenith. This means that
:
if ε is small. If particle is on the surface of the planet then the local gravity is andset .
:
which is a small fraction of . Note also that force is attractive toward the Moon when the