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M43

De Mairan's Nebula

EmissionNebula Orion Mag 9.0

Dati oggetto

Designazione catalogo
M43
Tipo
EmissionNebula
Costellazione
Orion
Magnitudine
9.0
Ascensione retta
05h 35m 36.0s
Declinazione
-05° 15' 60.0"
Distanza
1,300 anni luce
Dimensione angolare
20.
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Su M43

Descrizione

De Mairan's Nebula is a bright emission/reflection nebula in Orion, physically part of the Great Orion Nebula complex but visually separated from M42 by a dark dust lane. It lies about 1,600 light-years from Earth and spans roughly 7 light-years. The nebula is illuminated by the young B-type star NU Orionis (HD 37061) at its center.

Consigli per l'osservazione

Located immediately north of M42, separated by a dark lane of dust. Visible in the same field of view as M42 in any telescope. It appears as a bright, comma-shaped or round nebula with the central star clearly visible. Often overlooked by observers dazzled by the overwhelming splendor of M42 just below it. A UHC or OIII filter enhances the nebulosity. Best observed from November through March alongside M42.

Storia

Discovered by Jean-Jacques Dortous de Mairan before 1731, hence the name De Mairan's Nebula. Charles Messier cataloged it on March 4, 1769. It was initially described as part of M42 before being recognized as a distinct, though connected, region.

Curiosità

Although M43 appears to be a separate nebula from M42, they are actually parts of the same enormous molecular cloud complex. The dark dust lane separating them is merely a foreground feature. The central star NU Orionis is carving a bubble in the surrounding gas, giving M43 its distinctive round shape — a miniature version of what the Trapezium stars are doing in M42.

Foto della comunità (1)

Credit: Ole Nielsen. License: CC BY-SA 2.5. (Wikimedia Commons)

Credit: Ole Nielsen. License: CC BY-SA 2.5. (Wikimedia Commons)

Skybred Feb 28, 2026