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Seagull Nebula, Darius Kopriva
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Seagull Nebula

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Seagull Nebula, Darius Kopriva
Powered byPixInsight

Seagull Nebula

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Description

The Seagull Nebula, also known as IC 2177, is a captivating emission nebula located in the constellation Monoceros. Its name derives from the striking resemblance it bears to a seagull in flight, with the shape of its wings and head clearly visible. The nebula is situated approximately 3,700 light-years away from Earth.

This celestial object spans an area of about 100 light-years and is composed of a mix of gas and dust illuminated by the radiation emitted by young, hot stars. The intense radiation from these stars ionizes the surrounding hydrogen gas.

The Seagull Nebula is also home to a collection of dark nebulae, which appear as dense patches blocking the light from background stars. These dark nebulae create a stark contrast against the colorful backdrop of the emission nebula, adding to its allure.

Located near the "body" of the seagull shape is a prominent star cluster known as NGC 2335. This cluster consists of numerous young, massive stars that have recently formed from the surrounding gas and dust. The energetic radiation and stellar winds from these stars shape and sculpt the surrounding nebula, creating intricate structures and filamentary patterns.

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Seagull Nebula, Darius Kopriva

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Southern Hemisphere Astro