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Name / Constellation

NGC 6811

Other: Cr 402; Mel 222


Coordinates AR:19h 37m 17s- Dec: -+46° 23′ 18″
Optics Takahashi FSQ 106N APO Fluorite F5 - 60/220 guiding refractor
Camera-Mount SBIG STF8300M - Orion StarShot Guider - 10Micron GM2000 QCI Mount
Filters Baader LRGB
  • Lum
  • Red
  • Green
  • Blue
  • 12 x 300 sec - 1 hour
  • 6 x 300 sec - 30 min
  • 6 x 300sec - 30 min
  • 6 x 300 sec - 30 min
Location / Date Promiod (Valle D'Aosta-Italy) "TLP" Remote Observatory - 02/03 oct 2019
Seeing About 3.2 @ 2.1 arcosec/pixel unbinned
Note Bad seeing
Acquisition MaxIm DL - CCD Autopilot 5
Processing Adobe Photoshop CS6 -

NGC 6811 is an open cluster in the constellation of Cygnus, near the constellation of Lyra. It has an angular size half that of the full Moon and includes about 1000 stars of roughly similar magnitude. It has also been called "The Hole in the Cluster" because of its dark center.NGC 6811 lies far away from the galactic plane, a feature it shares with many other old open clusters.It is 1107 ± 90 parsecsdistant, 14–20 light years across, and has a total luminosity of 2100 suns. Approximately 1.00 ± 0.17 billion years old, it probably contained some 6000 stars at birth, but gravitational interactions and stellar evolution have since reduced the number to 1000. The spectral types of most of its stars range from mid-F to early-K, with surface temperatures relatively similar to the Sun's; the rest include A2-types, several O-types, and more than 100 B-types. Sixteen stars have been observed to vary in brightness, twelve of which are Delta Scuti variables. Its Trumpler classification is III 1r—it is "a rich cluster with equally bright stars with no noticeable central concentration". The stars do, however, have an unusual (if not concentrated) distribution, with an apparent coronasurrounding the core, leaving the impression of a hole.NGC 6811 was first observed by John Herschel in 1829 and was added to his General Catalogue of Nebulae and Clusters in 1864. The cluster has been the subject of study by the Kepler mission, with the aim of characterizing its stars' rotation rate, age, and distance to help the hunt for exoplanets.

NGC 6811 is best observed from Earth in the Northern Hemisphere in summer. In these conditions it lies close to the zenith during the night, northeast of Delta Cygni. It is considered an aesthetically pleasant object for amateur astronomers, even if the brightest members are just 10th magnitude objects. It appears as a hazy patch in 10x binoculars, but it is best seen at around 70x with a moderate-aperture telescope. It has been described by amateur astronomers as a "smoke ring of stars" or "a jeweled mask a woman might wear at a masquerade ball".