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us. This should give rise either to intermit-
                                         tence in the star’s light or else to variabil-
                                         ity. It was by supposing the existence of a
                                         dark companion to Algol that its discoverer,
                                         Goodricke of York,[16] in 1783, explained
                                                                         ˆ
                                         variable stars of this type. Algol (I Per-
                                         sei) completes the period of variable bright-
                                         ness in 68.8 hours. It loses three-fifths of its
                                         light, and regains it in twelve hours. In 1889
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