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Theory of tides : ウィキペディア英語版
Theory of tides

The theory of tides is the application of continuum mechanics to interpret and predict the tidal deformations of planetary and satellite bodies and their atmospheres and oceans (especially Earth's Ocean) under the gravitational loading of another astronomical body or bodies (especially the Moon).
== Kepler ==

In 1609 Johannes Kepler correctly suggested that the gravitation of the Moon causes the tides,〔Johannes Kepler, ''Astronomia nova …'' (1609), p. 5 of the Introductio in hoc opus〕 basing his argument upon ancient observations and correlations. It was originally mentioned in Ptolemy's ''Tetrabiblos'' as having derived from ancient observation.

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