← Understanding Lunar Cycles

Lunar Cycles • A visual guide

Perigee and Apogee

The Moon’s changing distance from Earth

The Moon’s distance changes along its orbit. Perigee names the closest point; apogee names the farthest.

Perigee and apogee on an exaggerated elliptical orbitEarth sits toward the left end of an ellipse. The leftmost Moon marker is perigee, nearer Earth; the rightmost is apogee, farther from Earth.EarthPerigeeApogeeEllipticity exaggerated

Scroll the diagram sideways to explore its labels.

An exaggerated ellipse makes the distance difference visible. Earth is at a focus, away from the center. The two Moon markers show different moments. Shape, sizes, and distances are not to scale. Original LuNAC illustration; conceptual basis: NASA Science — Supermoons.

Two turning points in distance

The Moon’s orbit is slightly elliptical. Perigee and apogee mark its nearest and farthest distances from Earth. Those distances vary from one orbit to another, so neither term represents one permanently fixed distance.

Source: NASA Science — Supermoons

Distance and apparent size

A closer Moon appears a little larger in the sky; a farther Moon appears a little smaller. The Moon itself has not changed size. A full moon near perigee is often called a supermoon, an informal term rather than an official astronomical classification.

Source: NASA Science — Supermoons

A different cycle from phase

The interval from one perigee to the next is called the anomalistic month. The phase cycle is the synodic month. These cycles have different lengths, so perigee does not always coincide with full moon. Distance and phase describe different aspects of the same moving Moon.

Source: Fred Espenak, NASA GSFC — Eclipses and the Moon’s Orbit