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Libration

What is libration?

Libration is the Moon’s apparent wobble as we watch it from Earth. It lets us see a little around the edges, so over time we can view about 59% of its surface.

Try the question

How can a locked Moon appear to wobble?

Move through the slightly elliptical orbit. Compare the steady spin angle with the changing orbital speed.

Apparent face from EarthSlightly elliptical orbit
What changed The steady spin and changing orbital speed differ by 6.3°. We peek around the eastern limb.

Watch for: Near perigee the Moon moves faster but its spin does not speed up to match.

Open this experiment in the full Moon lab

A locked Moon on an ellipse seems to nod: the spin is steady, the orbital speed is not, so we look slightly around the east or west limb.

A peek, not a roll

If the orbit were a perfect circle and we sat at the centre, tidal locking would show us exactly half. The orbit is a little stretched, and we are a little off to the side on a turning Earth. Those geometric cheats are libration.

Get more on this

Three small cheats

Longitudinal: the Moon speeds up near perigee while its spin stays even. Latitudinal: the Moon’s equator is tipped a few degrees, so we see a little past the poles. Diurnal: we watch from the sides of a spinning Earth, not from its centre.

See it live

On the hub: Sun–Earth–Moon simulator · Moon