Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  Foxhead Cluster  ·  NGC 6819
NGC 6819, the Foxhead Cluster, BrettWaller
NGC 6819, the Foxhead Cluster
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NGC 6819, the Foxhead Cluster

NGC 6819, the Foxhead Cluster, BrettWaller
NGC 6819, the Foxhead Cluster
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NGC 6819, the Foxhead Cluster

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Description

NGC 6819 is a highly concentrated and rich open cluster of faint stars that contrasts with the surrounding field of Milky Way stars. Deep images reveal a hundred stars of magntitude 11.5 to 15 within a 5' area. Discovered by Caroline Herschel on 12 May 1784, she described it as "halfway between delta Cyg & eta & theta Lyrae making an isosceles triangle downwards when in that situation". With an integrated visual magnitude of 7.3, it contains approximately 150 stars within a diameter 9.5', the brightest member being magnitude 11.49. It often appears in lists of challenging objects for visual observers.

NGC 6819 is Trumpler Type I 1 r open cluster, also catalogued as Melotte 233, Collinder 403, and Lund 900. It visually resembles a globular cluster, and Lund mistakenly listed it as such. It lies at a distance of 7,200 light years, and its age is estimated as 2.5 billion years, thus the reddish color of it's older red-giant members. The surrounding, bright bluish stars are unrelated and in the foreground of the Milky Way.

If you are wondering, as I was, about why this cluster has the moniker "Fox Head', many visual observers see a distinct "V" in the brightest stars of the cluster, and since a fox has a triangular head, the name caught on.

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NGC 6819, the Foxhead Cluster, BrettWaller