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Orbital tilt of the Moon

Why isn’t there an eclipse every month?

The Moon’s orbit is tilted about 5° compared with Earth’s orbit around the Sun. Most months, the Moon passes above or below the alignment needed for an eclipse.

Try the question

Why isn’t there an eclipse every month?

Set the orbit to 0°, then restore its real tilt. Watch the Moon move off the exact Sun–Earth line.

full moonVertical separation is exaggerated so 5.1° can be seen
What changed At 5.1°, the Moon passes above or below the exact line. An eclipse happens only near an orbital crossing.

Watch for: Phase controls left–right alignment; orbital tilt controls the missing up–down dimension.

Open this experiment in the full Moon lab

Earth’s shadow is a real cone past the Moon’s orbit. A 5° tip is enough for the full Moon to miss that cone most months. The drawing of the tip is exaggerated so you can see it.

What to look for

Use the model to compare a tilted orbit with a flat orbit. Watch where the Moon passes Earth’s shadow. Does it enter the shadow on every trip?

Questions answered

Does every full moon make a lunar eclipse? No. The Moon usually passes above or below Earth’s shadow.

Does every new moon make a solar eclipse? No. The Moon’s shadow usually misses Earth. Explore upcoming lunar eclipses.

Get more on this

Where the two paths cross

The flat surface of an orbit is called its plane. The Moon’s orbit crosses Earth’s orbital plane at two places, called nodes. Eclipses can happen when a new or full moon occurs near one of those crossings.

The 5° tilt is different from Earth’s 23.4° axial tilt. One describes an orbit. The other describes how a world spins.

See it live

On the hub: Moon