Pleione Microphylla
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Pleione Microphylla
Pleione may refer to: *Pleione (mythology), a figure in Greek mythology *Pleione (star) PleionePronounced or is a binary star and the seventh-brightest star in the Pleiades star cluster ( Messier 45). It has the variable star designation BU Tauri (BU Tau) and the Flamsteed designation 28 Tauri (28 Tau). The star is ..., a star belonging to the Pleiades star cluster * ''Pleione'' (plant), a genus mainly of ground orchids. Prefer to grow on tree-trunks and in rock crevices {{disambiguation ...
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Pleione (mythology)
Pleione (Ancient Greek: Πληιόνη or Πλειόνη) was an Oceanid nymph in Greek mythology and mother of the Pleiades. Pleione presided over the multiplication of the flocks, fitting, since the meaning of her name is: "to increase in number". Family Pleione was the daughter of Okeanos and Tethys who were the Titan God and Goddess of bodies of water. Pleione was mother to seven daughters, known as the Pleiades. Their names were: Maia, Electra, Taygete, Alcyone, Celaeno, Sterope and Merope. She is often said to be the mother of Calypso with Atlas as well. Among her grandchildren were the god Hermes and the demigod Iasion. Mythology Pleione lived in a southern region of Greece called Arcadia, on a mountain named Mount Kyllini. She married the Titan Atlas and gave birth to the Hyades, Hyas and the Pleiades. She was also the protectress of sailing. In some accounts, when Pleione once was travelling through Boeotia Boeotia ( ), sometimes Latinized as Boiotia ...
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Pleione (star)
PleionePronounced or is a binary star and the seventh-brightest star in the Pleiades star cluster ( Messier 45). It has the variable star designation BU Tauri (BU Tau) and the Flamsteed designation 28 Tauri (28 Tau). The star is located approximately from the Sun, appearing in the constellation of Taurus. Pleione is located close on the sky to the brighter star Atlas, so is difficult for stargazers to distinguish with the naked eye despite being a fifth magnitude star. The brighter star of the Pleione binary pair, component A, is a hot type B star 184 times more luminous than the Sun. It is classified as Be star with certain distinguishing traits: periodic phase changes and a complex circumstellar environment composed of two gaseous disks at different angles to each other. The primary star rotates rapidly, close to its breakup velocity, even faster than Achernar. Although some research on the companion star has been performed, stellar characteristics of the ...
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