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Pleione (28 Tauri) |
 | | A Be star’s emissions come from a surrounding ring of gas that is somehow related to the star’s great rotation speed, Pleione spinning at least as fast as 329 km/s at the equator, 165 times faster than the Sun, giving it a rotation period of under half a day. |
 | | The difference in Be star styles was once thought to be a matter of orientation, but Pleione puts the lie to the theory by switching among all three phases, normal B star, Be star, Be shell star, the changes taking place at intervals of 17 and 34 years. |
 | | Pleione was seen to develop to a shell or envelope twice in the twentieth century: the first in 1938, which reached a peak brightness in 1945, then faded, and a second in 1972. |
| www.daviddarling.info /encyclopedia/P/Pleione.html (408 words) |
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