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This is an interesting planetary nebula in telescopes large and small. Named for it's resemblance to M27, the famous "Dumbbell nebula" in Cygnus, this planetary is nonetheless considerably smaller and fainter. On the other hand it is much larger than the vast majority of planetaries and it's fairly faint integrated magnitude of 12.2 is misleading (it appears considerably brighter than this would suggest).
In a 6-inch scope this planetary appears as an elongated, rectangular hazy spot. A slight pinching at the middle can be glimpsed with averted vision. As is the case for all but the brightest of it's class, larger aperture is required to see more detail. In my 18" the two lobes are easily visible as separate entities. There are hints of structure -- a sort of blobishness -- to the dark area between the two lobes. The outer ends of the lobes have filaments arcing outward from each corner. A star is embedded at one of these corners where the filament starts. An OIII filter helps increase the contrast a bit. In photographs the filaments make complete arcs, joining
the filament from the opposing lobe. User's of large instruments should
attempt to trace these filaments all of the way across.
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