description IC 2177 Overview
IC 2177 is a diffuse emission nebula located along the Monoceros-Canis Major border. Discovered in 1898 by Isaac Roberts, it encompasses regions like Sh2-292 and Sh2-296, often referred to as the “Seagull Nebula”. This object is notable for its complex structure and vibrant colors produced by ionized gas. Astronomers and amateur observers interested in observing nebulae and star formation find IC 2177 a visually engaging target.
insights Ranking position
IC 2177 ranks #136 of 564 in the Nebula ranking, behind Tulip Nebula, ahead of Coalsack Nebula.
help IC 2177 FAQ
What is the popular name for the IC 2177 nebula?
IC 2177 is widely known as the Seagull Nebula because its shape resembles a bird with widespread wings. It is a diffuse emission nebula located on the border between the constellations Monoceros and Canis Major.
Who discovered the IC 2177 nebula and when?
The nebula was discovered by the Welsh engineer and astronomer Isaac Roberts in 1898. Roberts was a prominent pioneer in the field of early celestial photography.
What components make up the Seagull Nebula complex?
The overall complex actually encompasses multiple Sharpless catalog objects, including Sh2-292 and Sh2-296. Sh2-292 serves as the glowing head of the celestial seagull.
What kind of telescope is needed to photograph IC 2177?
Because IC 2177 is a very large but faint object, astrophotographers use small aperture, wide-field telescopes or telephoto lenses. Long exposure times and narrowband or nebulium filters are required to bring out its vibrant colors.
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