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complicated the problem. He located the
                                         moon’s excentric as he had done the sun’s.
                                         He also discovered some of the minor ir-
                                         regularities of the moon’s motion, due, as
                                         Newton’s theory proves, to the disturbing
                                         action of the sun’s attraction.
                                            In the year 134 B.C. Hipparchus observed
                                         a new star. This upset every notion about
                                         the permanence of the fixed stars. He then
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