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Polar motion is the movement of Earth's rotation axis across its surface.

The axis of the Earth's rotation tends, like the axis of a gyroscope, to maintain its orientation with respect to inertial space. However, due to external forces acting upon the Earth, this axis nevertheless exhibits a slow, large-scale motion, known as precession and nutation. Nutation is divided into a predictable part from a "nutation theory," a long series of trigonometric terms depending on time, and derived from motions of the Moon and models of the Earth, plus corrections called the Celestial Pole Offset, which are the measured departures (two-dimensional on the celestial sphere) of the celestial rotation pole from the theory ^[1]. These corrections, of order 0.03 arcseconds, are of no importance to most users, but by monitoring them, a better theory of nutation may be developed in the future.

Contents 1 Earth-fixed reference 2 Causes 3 Notes 4 References

When using, instead of an inertial reference frame, a frame attached to the body of the solid Earth (a so-called Earth-centred, Earth-fixed or ECEF reference frame), the rotation axis also varies slightly. This variation, which is only a few metres measured on the Earth's surface, is called Polar motion.

It consists of two quasi-periodic components and a gradual drift, mostly westward, of the Earth's instantaneous rotational axis or North pole, from a conventionally defined reference axis, the CIO (Conventional International Origin), being the pole's average location over the year 1900.

The two periodic parts are a more or less circular motion called Chandler wobble with a period of about 435 days, and a yearly circular motion. There is also a slow drift which is less well known. These motions are illustrated on International Earth Rotation and Reference Systems Service ^[2].

The mean displacement far exceeds the magnitude of the wobbles. This can lead to errors in software for Earth observing spacecraft, since analysts may read of a 5 meter circular motion and ignore it, while a 20 meter offset exists, fouling the accuracy of the calculated latitude and longitude. The latter are determined based on the International Terrestrial Reference System, which follows the polar motion.

The slow westward drift, about 20 m since 1900, is partly due to motions in the Earth's core and mantle, and partly to the redistribution of water mass as the Greenland ice sheet melts, and to isostatic rebound, i.e. the slow rise of land that was formerly burdened with ice sheets or glaciers^[3]. The drift is roughly along the 80th meridian west.

1. ^ Celestial Pole Offset
2. ^ Polar Motion Map BW, Color
3. ^ Munk, Walter (2002).

• Fisher, Rick (1996). "Earth Rotation and Equatorial Coordinates". Retrieved Jun. 5, 2005.
• Munk, Walter (2002). "Twentieth century sea level: An enigma". Proceedings of the National Academy of Sciences 99, #10. pp. 6550—6555.