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    The astronomical origin of tides for sailors.
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    In astronomy, precession refers to slow changes in an astronomical body's rotational or orbital parameters. An important example is the steady change in the orientation of the axis of rotation of the Earth, known as the precession of the equinoxes. The term "precession" used in astronomy generally describes the observable precession of the equinox, whereas the term "precession" as used in physics, generally describes a mechanical process.
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