Talk:NGC 6752

A fact from NGC 6752 appeared on Wikipedia's Main Page in the Did you know column on 27 August 2013 (check views). The text of the entry was as follows:

Did you know... that NGC 6752, containing 100,000 stars, is the third brightest globular cluster in the sky?

A record of the entry may be seen at Wikipedia:Recent additions/2013/August. The nomination discussion and review may be seen at Template:Did you know nominations/NGC 6752.

Wikipedia

Third brightest globular?

Is this really the third-brightest globular? Have you checked what Wikipedia says about M22? Did the folks at APoD? 88.108.53.110 (talk) 20:25, 22 August 2013 (UTC)[reply]

The wikipedia page says M22 is one of the brightest. Actually there is some discrepancies depending on how one looks at it, so will add a few lines. Cas Liber (talk · contribs) 20:50, 22 August 2013 (UTC)[reply]

File:NGC 6752 Hubble WikiSky.jpg to appear as POTD

Hello! This is a note to let the editors of this article know that File:NGC 6752 Hubble WikiSky.jpg will be appearing as picture of the day on July 2, 2015. You can view and edit the POTD blurb at Template:POTD/2015-07-02. If this article needs any attention or maintenance, it would be preferable if that could be done before its appearance on the Main Page. Thanks! — Chris Woodrich (talk) 23:59, 10 June 2015 (UTC)[reply]

Picture of the day

NGC 6752 is a globular cluster of intermediate density in the constellation Pavo. First identified in 1826 by James Dunlop, the cluster lies around 13,000 light years distant. It is visible to the naked eye in good viewing conditions.Photograph: NASA/STScI

Archive – More featured pictures...

External links modified (January 2018)

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