01

Sunlight creates every phase

Half of the Moon is always illuminated by the Sun. As the Moon orbits Earth, our viewing angle changes and we see a different fraction of that sunlit half.

Earth's shadow does not cause the ordinary phases. Earth's shadow reaches the Moon only during a lunar eclipse, when the Sun, Earth and Moon align near full moon.

02

The eight named phases

The eight named phases
PhaseWhat you seeTypical viewing
New moonMoon near the SunUsually not visible
Waxing crescentGrowing thin crescentWestern sky after sunset
First quarterHalf-lit discAfternoon and evening
Waxing gibbousMore than half litAfternoon into night
Full moonFully lit near sideRises near sunset
Waning gibbousShrinking lit areaLate evening and morning
Last quarterHalf-lit discAfter midnight and morning
Waning crescentShrinking thin crescentEastern sky before sunrise
03

Waxing, waning and the terminator

Waxing means the illuminated portion is growing from night to night. Waning means it is shrinking. The dividing line between lunar day and night is called the terminator.

Low-angle sunlight near the terminator casts long shadows across craters and mountains, making quarter and crescent phases especially rewarding through binoculars or a telescope.

04

Why there is not an eclipse every month

The Moon's orbit is tilted by about five degrees relative to Earth's orbit around the Sun. At most new and full moons, the three bodies are not aligned closely enough for an eclipse.

A solar eclipse requires a new moon near an orbital node. A lunar eclipse requires a full moon near a node. These alignments occur during eclipse seasons spaced roughly six months apart.

SOURCES

Sources and methodology

Dates, paths and safety guidance use the references below. Local timings are rounded calculations for the stated reference points; recalculate your exact observing location.