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M57 - Planetary Nebula, Lyra
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Calibrate monitor
 

  The famous ring nebula M57 is often regarded as the prototype of a planetary nebula, and a showpiece in the northern hemisphere summer sky. Recent research has confirmed that it is, most probably, actually a ring (torus) of bright light-emitting material surrounding its central star, and not a spherical (or ellipsoidal) shell, thus coinciding with an early assumption by John Herschel. Viewed from this equatorial plane, it would thus more resemble the Dumbbell Nebula M27 or the Little Dumbbell Nebula M76 than its appearance we know from here: We happen to view it from near one pole.
  Location J65 Celbridge Observatory
  Date/Time (UTC) 30 May 2006, 00:30
  Optics 200mm SCT, F6.3 reducer
  Filters None
  Imager Meade DSI-C
  Mount Astro-physics 1200GTO
  Exposure details 19 images * 120 seconds
  Software MaximDL, Photoshop 7
© David McDonald 2012 Updated 10 June 2012