(oscillating motion of orbiting bodies relative to each other)
Libration is relative oscillating motion between
two orbiting bodies. A common use of the term is
in describing the Moon's rocking motion
as viewed from Earth. It is also used for
similar situations with other orbiting bodies
and disks (e.g., circumstellar disks) and other
situations where there is such an oscillation.
The moon, as viewed from a point on Earth shows
four kinds of libration:
- Libration in longitude - the Moon's apparent slight oscillation from side to side due to the moon rotating so as to keep single face toward the Earth, but due to the orbit's eccentricity, sometimes during the month, the rotation is slightly ahead or behind this position.
- Libration in latitude - the Moon's axis is slightly different than the axis of its orbit around Earth, so sometimes during the month its north or south pole is slightly visible.
- Diurnal libration - as the Earth rotates, a person on the Earth sees a very slight difference in the Moon's face as the day progresses, i.e., the moon gives a slightly different face to persons looking at it from different longitudes.
- Physical libration or forced libration - this is an actual motion of the moon and is small: the Moon's mass's slight asymmetry, with gravity, determine which part faces the Earth, and the moon can swing back and forth like a pendulum through that direction, with very little dampening. Generally it happens north-to-south, which is the case for the moon.
A study of Enceladus's physical libration has
been given as evidence of a disconnection between
its surface and much of its mass, implying a global
ocean under its ice.
Lagrangian points, are also known as
libration points. I imagine this is because some of the
points are stable, and an object can sit in a small
orbit around the point.
corotation resonance (CR)