Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)
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LDN 889 & IC1318, Astro-TAPAS
LDN 889 & IC1318
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LDN 889 & IC1318

Getting plate-solving status, please wait...
LDN 889 & IC1318, Astro-TAPAS
LDN 889 & IC1318
Powered byPixInsight

LDN 889 & IC1318

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Description

LDN 889 in Gamma Cygni Nebula (IC1318)

The Gamma Cygni Nebula or IC 1318, is a diffuse emission nebula that can be seen around Sadr (Gamma Cygni), the nebula is at 4,900 light years.

The Gamma Cygni Nebula is considered an emission nebula because it is ionized by the radiation of the nearby stars and it emits visible light as a result. The visible portion of the H II region stretches over an area more than 100 light years across. The nebula is illuminated by an O9-class star which is visually obscured by interstellar material.

The Gamma Cygni Nebula has three distinct parts, designated as IC 1318 A, B and C. The dark cloud about 20 light years thick that divides IC 1318 B and C is a dark nebula known as LDN 889. It is physically related to the emission nebula and the surrounding molecular cloud complex. The dark dust lane is responsible for the nebula’s distinctive shape, resembling that of a butterfly, which is why IC 1318 is sometimes also known as the Butterfly Nebula. The components IC 1318 B and C are not separate parts of the nebula, but a single cloud visually separated by LDN 889.

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LDN 889 & IC1318, Astro-TAPAS

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Entre Encinas y Estrellas (e-EyE)