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NGC6820 is an emission nebula in the constellation Vulpecula with a big, trunk-like dust pillar pointing towards the open cluster NGC6823. This open cluster has a distance of aboout 6000 light years and contains very hot, active stars. The radiation of those stars forms the globules and dust pillars that can be found throughout the complete emission nebula complex. Sometimes, the naming of this complex is a bit screwed up: The emission nebula is NGC6820, the central open cluster is NGC6823. Some sites state, that NGC6820 is only a small reflection nebula in the emission nebula complex. As the surface brightness of this nebula is quite low, a photographic approach to this faint object requires a very high transmission of the sky, especially a very low mist or haze.
Datum/Date: 06.08.2015 & 07.08.2015 /August 6th and 7th, 2015 Optik / Scope: 7,5” Maksutov Newtonian Astrograph f/5.3 with 2” 1:10 Crayford focusser Sensor/CCD: QHY10 CCD-Camera (APS-C) @ -20°C, Gain=30, Offset=118 Autoguiding: ALccd5 off-axis guiding Belichtung/Exposure: 24x1500sec, total integration time= 10h 00min Workflow: Regim, PixInsight, Photoshop CS6
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Juniper Hill Observatory
Köfering, Bavaria 12° 12’ E 48°56’ N 344m N.N.
NGC 6820 (Sh2-86)
Lichter sollen am Himmelsgewölbe sein, um Tag und Nacht zu scheiden!