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50 Persei
50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.50. Located around distant, it is a White main-sequence star of spectral type F7V, a star that is currently fusing its core hydrogen. The star is an RS Canum Venaticorum variable,〔 meaning that it is a close binary star whose components have star-spots, which cause variations in brightness. ==References==
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