Star Clusters
by members of the Wells & Mendip Astronomers
Star clusters come in two types: Open clusters (a clump of new born stars slowly drifting apart) and globular clusters (an ancient structure of old stars, perhaps the remnant of a dwarf galaxy absorbed by the Milky Way). Globular clusters are large enough to be observable also in nearby galaxies such as in the Andromeda Galaxy
Contributors:
Hugh Allen (200mm Meade LX90 telescope, Meade DSI II colour camera. Spectra: Alpy 600 spectroscope and Atik 314L camera)
Richard Hook (100mm Skywatcher Esprit telescope, Nikon D3200 camera)
Ian Humphreys (Televue NP101mm and 405mm Orion Optics telescopes, Canon 1100D and Atik 11000 Mono (LRGB filters) cameras
Pete Richardson (William Optics ZS80mm APO telescope, QSI683WSG camera)
Fred and Ed Vanner (Sky-Watcher Skymax 150 Pro or Esprit 80ED Pro telescope, ZWO ASI183MC or MM camera)
Send contributions to: [email protected]
Hugh Allen (200mm Meade LX90 telescope, Meade DSI II colour camera. Spectra: Alpy 600 spectroscope and Atik 314L camera)
Richard Hook (100mm Skywatcher Esprit telescope, Nikon D3200 camera)
Ian Humphreys (Televue NP101mm and 405mm Orion Optics telescopes, Canon 1100D and Atik 11000 Mono (LRGB filters) cameras
Pete Richardson (William Optics ZS80mm APO telescope, QSI683WSG camera)
Fred and Ed Vanner (Sky-Watcher Skymax 150 Pro or Esprit 80ED Pro telescope, ZWO ASI183MC or MM camera)
Send contributions to: [email protected]
M6 The Butterfly Cluster (open cluster, distance 1590 ly) |
|
M7 Open cluster (distance 980 ly) |
|
M9 Globular cluster (distance 25800 ly) |
|
M10 Globular cluster (distance 14300 ly) |
|
M12 Globular cluster (distance 15700 ly) |
|
M14 Globlar cluster (distance 30300 ly) |
|
M18
Open cluster (distance 4230 ly)
M19 Globular cluster (distance 28700 ly) |
|
M21 Open cluster (distance 3930 ly) |
|
M22 Globular cluster (distance 10600 ly) |
|
M23 Open cluster (distance 2050 ly) |
|
M24 Sagittarius Star Cloud (distance approx. 10000 ly) |
|
M25 Open cluster (distance 2000 ly) |
|
M26 Open cluster (distance 5160 ly) |
|
M28 Globular cluster (distance 17900 ly) |
|
M29 Open cluster (distance 3740 ly) |
|
M30 Globular cluster (distance 27100 ly) |
|
M34 Open cluster (distance 1500 ly) |
|
M39 Open cluster (distance 1010 ly) |
|
M40 Double star (optical double star, distance A = 1140ly and B = 460 ly |
|
M41 Open cluster (distance 2300 ly) |
|
M44 Beehive Cluster (open cluster, distance 577 ly) |
|
M47 Open cluster (distance 1600 ly) |
|
M52 Open cluster (distance 4600 ly) |
|
M54 Globular cluster (distance 87400 ly) |
|
M55 Globular cluster (distance 17600 ly) |
|
M56 Globular cluster (distance 32900 ly) |
|
M62 Globular cluster (distance 22200 ly) |
|
M67 Open cluster (distance approx. 2750 ly) |
|
M68 Globular cluster (distance 33000 ly) |
|
M69 Globular cluster (distance 28700 ly) |
|
M70 Globular cluster (distance 29400 ly) |
|
M72 Globular cluster (distance 55000 ly) |
|
M73 Sparse asterism (distance to individual stars 820 - 3300 ly) |
|
M75 Globular cluster (distance 67500 ly) |
|
M79 Globular cluster (distance 42000 ly) |
|
M80 Globular cluster (distance 32600 ly) |
|
M92 Globular cluster (distance 26700 ly) |
|
M93 Open cluster (distance 3380 ly) |
|
M107 Globular cluster (distance 20900 ly) |
|
NGC 869 and 884 Perseus Double Cluster (open clusters) |
|
Would you like to become a member?
If you are interested in becoming a member of Wells and Mendip Astronomers, please contact us using the email icon below.