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Vega

[vey-guh; Spanish be-gah] /ˈveɪ gə; Spanish ˈbɛ gɑ/
noun
1.
Lope de
[law-pe th e] /ˈlɔ pɛ ðɛ/ (Show IPA),
(Lope Félix de Vega Carpio) 1562–1635, Spanish dramatist and poet.
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Based on the Random House Dictionary, © Random House, Inc. 2014.
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British Dictionary definitions for lope vega

Vega1

/ˈviːɡə/
noun
1.
the brightest star in the constellation Lyra and one of the most conspicuous in the N hemisphere. It is part of an optical double star having a faint companion. Distance: 25.3 light years; spectral type: A0V
Word Origin
C17: from Medieval Latin, from Arabic (al nasr) al wāqi, literally: the falling (vulture), that is, the constellation Lyra

Vega2

/ˈveɪɡə; Spanish ˈbeɣa/
noun
1.
Collins English Dictionary - Complete & Unabridged 2012 Digital Edition
© William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins
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Word Origin and History for lope vega

Vega

n.

1638, bright northern star, the alpha of Lyra, from Arabic (Al Nasr) al Waqi translated variously as "the eagle of the desert" or "the falling vulture."

Online Etymology Dictionary, © 2010 Douglas Harper
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lope vega in Science
Vega
  (vē'gə, vā'gə)   
A star in the constellation Lyra and one of the five brightest stars in the night sky. It is a white main-sequence star in the Hertzsprung-Russell diagram, with an apparent magnitude of 0.04. Vega, along with Altair and Deneb, form the Summer Triangle asterism. Scientific name: Alpha Lyra.
The American Heritage® Science Dictionary
Copyright © 2002. Published by Houghton Mifflin. All rights reserved.
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Encyclopedia Article for lope vega

Vega

brightest star in the northern constellation Lyra and fifth brightest in the night sky, with a visual magnitude of 0.03. It is also one of the Sun's closer neighbours, at a distance of about 25 light-years. Vega's spectral type is A (white) and its luminosity class V (main sequence). It will become the northern polestar by about AD 14,000 because of the precession of the equinoxes.

Learn more about Vega with a free trial on Britannica.com
Encyclopedia Britannica, 2008. Encyclopedia Britannica Online.
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