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NGC 1931 is a tiny little cluster of stars embedded in nebulosity found about a degree to the west of the open cluster M36. At the heart of the NGC 1931 cluster lies a tiny version of the famous Trapezium in M42; four stars that make a rough trapezoid. This is a small object, so be sure to try as much magnification as the conditions will bear on it. In smaller scopes or at low powers it will appear as a fuzzy star. More magnification will reveal a fairly bright, round fuzzy knot of nebulosity. OIII and H-Beta filters have little effect on the nebula. Brian Skiff gathered some
information regarding the trapezium stars, which I have reproduced below.
The multiple star system that forms the "little trapezium" is ADS 4112
(BD+34 1074).
The A, B, and C stars are easy to see but the E component is a little more difficult. At least an 8-inch scope will be required to see it. The D component is even more difficult, requiring a very large aperture. When I observed NGC 1931 in my 18-inch f/4.5 I immediately noticed the nebula as a bright knot at 97x. I was surprised at how bright it appeared. The best view came at 430x, where the little trapezium became very obvious.
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