Right Ascension	05 : 35.6 (h:m)
Declination	-05 : 16 (deg:m)
Distance	1.6 (kly)
Visual Brightness	9.0 (mag)
Apparent Dimension	20x15 (arc min)

Discovered before 1731 by Jean-Jacques Dortous de Mairan.

Messier 43 (M43, NGC 1982) is actually a part of the Great Orion Nebula, M42, which is separated from the main nebula by an impressive, turbulent dark lane.

It was first reported by de Mairan in 1731 as a "brilliance surrounding a star" which he thought was "very similar to the atmosphere of our Sun, if it were dense enough and extensive enough to be visible in telescopes at a similar distance." Charles Messier included in his fine drawing of the Orion Nebula, and assigned it an extra catalog number, M43, on March 4, 1769. Moreover, William Herschel took it into his list with the number H III.1, although normally he careful avoided to assign his numbers to Messier Objects. In his 1811 paper, Herschel states to have observed it as early as March 4, 1774, and cataloged it on November 3, 1783.

The diffuse nebula M43 surrounds the irregular young "nebula variable" NU Orionis (HD 37061, attn: "N" "U" Orionis, not "Nu Orionis", i.e. the variable star 2-letter designation, not the Greek letter) of magnitude 6.5-7.6 and spectral type B IV. It seems that M43 is excited to shine by this star, and contains its own, separate small cluster of stars which have formed in this part of the Orion nebula.

The dark features along its eastern border are well visible in telescopes starting at about 8 inch. The nebula itself is a fine view even in a 4-inch. Alister Ling in his recent review of observing the Orion nebula with filters (Astronomy, December 1995 issue), mentions the Comma shape of this nebula.

Our image was obtained by David Malin with the 3.9-meter Anglo-Australian Telescope. More information on this image is available.

NGC Online data for M43

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Hartmut Frommert
Christine Kronberg
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Last Modification: August 13, 2007