Wikipedia:Today's featured article/requests/Pavo (constellation)

Pavo (constellation)

 * This is the archived discussion of the TFAR nomination for the article below. Subsequent comments should be made on the appropriate discussion page (such as Wikipedia talk:Today's featured article/requests). Please do not modify this page. 

The result was: scheduled for Today's featured article/July 26, 2016 by Brianboulton (talk) 19:15, 11 July 2016 (UTC)



Pavo is a constellation in the southern sky with the Latin name for peacock. It is one of twelve constellations conceived by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. Pavo first appeared on a 35-cm (14 in) diameter celestial globe published in 1598 in Amsterdam by Plancius and Jodocus Hondius and was depicted in Johann Bayer's star atlas Uranometria of 1603. The constellation's brightest member, Alpha Pavonis, is also known as Peacock and appears as a 1.91-magnitude blue-white star, but is actually a spectroscopic binary. Delta Pavonis is a nearby Sun-like star some 19.9 light years distant. Six of the star systems in Pavo have been found to host planets, including HD 181433 with a super-earth, and HD 172555 with evidence of a major interplanetary collision in the past few thousand years. The constellation contains NGC 6752, the third-brightest globular cluster in the sky, and the spiral galaxy NGC 6744, which closely resembles our Milky Way but is twice as large.
 * Most recent similar article(s): June 4, 2016 Circinus
 * Main editors: Casliber
 * Promoted: October 5, 2013
 * Reasons for nomination:
 * Support as nominator. Cas Liber (talk · contribs) 11:06, 7 July 2016 (UTC)