Lunar precession

Precession is the change in direction of an axis of rotation with respect to a reference plane. The orbit of the Moon has two important such precessional motions.

The first precession is movement of the plane of the lunar orbit. The period of the lunar nodal precession is defined as the time it takes the ascending node to move through 360 degrees relative to the vernal equinox. It is about 18.6 years and the direction of motion is westward, ie. in the same direction as the Earth's orbit around the sun. This is the reason that a draconic month or nodal period ( the period of time that the Moon takes to return to the same node in its orbit ) is shorter than the sidereal month. After one nodal precession period, the number of draconic months exceeds the number of sidereal months by exactly one. This period is about 6,793 days (18.60 years).

As a result of this nodal precession, the time for the Sun to return to the same lunar node, the eclipse year, is about 18.6377 days shorter than a sidereal year. The number of solar orbits ( years ) during one lunar nodal precession period equals the period of orbit ( one year ) divided by this difference, minus one. 365.25/18.6377 - 1