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1693, compared this value with his own mea-
                                         surements, and so discovered the acceler-
                                         ation of the moon’s mean motion.  This
                                         was conclusively established, but could not
                                         be explained by the Newtonian theory for
                                         quite a long time.] He determined the plane
                                         of the moon’s orbit and its inclination to the
                                         ecliptic. The motion of this plane round the
                                         pole of the ecliptic once in eighteen years
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