Online Encyclopedia

PERSEUS

Online Encyclopedia
Originally appearing in Volume V21, Page 187 of the 1911 Encyclopedia Britannica.
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PERSEUS  , in

astronomy, a constellation of the
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northern hemisphere, called after the Greek legendary hero, it is mentioned by
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Eudoxus (4th century B.c.) and
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Aratus (3rd century B.C.); ' Author of a
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history of
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Antioch; he is quoted by John Malalas, Chronographia, pp . 37-38, ed .
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Bonn (1831) . Nothing further is known of him (see C . W . Muller, Fragmenta historicorum graecorum, W . 467) . Ptolemy and Tycho Brahe catalogued 29 stars, Hevelius 46 . The most important member of this constellation is 13 Persei or
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Algol (q.v.), a famous variable
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star . 6 Persei is a triple star, composed of one 4th magnitude star and two of the loth magnitude; p Persei is an irregular variable, with a range in magnitude of 3.4 to 4'1 . Nova Persei is a " new " star discovered in 1887 and subsequently recognized on Harvard plates by Mrs Fleming in 1895; another new star was discovered by Anderson on the 21st of
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February 1901, which, after increasing in magnitude, gradually became fainter and ultimately disappeared . There is a nebula surrounding Nova Persei (1901) which was photo-graphed at Yerkes
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observatory in September 1901; a pair of star clusters, appearing as a bright patch in the Milky Way; and the meteoric swarm named the Perseids, which appear in August and have their radiant in Perseus .

End of Article: PERSEUS
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PERSEUS OF MACEDONIA (b. c. 212 B.C.)

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