NGC/IC Project Restoration Effort

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NGC1976

 

Basic Information


Location and Magnitude


Right Ascension: 5:35:17.1
Declination: -5:23:25
Constellation: ORI
Visual Magnitude: 4.0

Historic Information


Discoverer: Peiresc
Year of discovery: 1610
Discovery aperture:

Observational


Summary description: !!! Θ¹ Orionis and the great neb
Sub-type: EN+RN

Corwin's Notes

===== NGC 1976 = M 42. I have adopted the position of the Trapezium as the position of M 42. This helps us avoid the problem of trying to decide on a geometric center for the nebula. See also NGC 1982 = M 43 and IC 429 for other notes about the Orion Nebula and the large, complex region of star formation around it. Finally, the southern part of M 42 may be NGC 1980 (which also see).

Steve's Notes

===== NGC 1976 48" (4/1/11): the Trapezium was first object viewed while the sky was still darkening. The "H" star (discovered by Barnard in 1888 with the Lick 36" was easily visible without reference to a chart, though I apparently missed the G star inside the Trapezium and a fainter companion to H at 1.3" separation. The "E" component was seen for the first time with a vivid orange color! In addition, due north of the A-E pair is a faint double star near the edge of the darker central pocket containing the Trapezium. On the opposite side (SE) of the Trapezium (at the edge of the inner pocket) are a wide pair of stars (~20") oriented E-W with possibly a third extremely difficult star between and a bit further east. Although I didn't take notes or try to sketch the main features of M42, there were several faint pink or red stars peppered over the glow of the nebula! 17.5" (10/12/85): best emission nebula in northern sky, fantastic view under all conditions, bright colored wings sweep to the east and south. The remarkable structure is difficult to describe but includes bays, filaments, knots, nebulous stars and a huge outer loop. Definite colors are visible including pale greens and pinks. Highlighted by the Trapezium which contains six stars and appears to reside in a darker hollow. The bright portion surrounding Theta probably has the highest surface brightness of any HII region in the sky with an "electric" appearance. Dark streaks and a dark wedge = "fish's mouth" intrudes on the NE side. Using an H-Beta filter, the nebulosity significantly dims in general but there is one outer wing or loop on the west side (oriented N-S) which obviously increases in contrast with the filter!