IC 2177 - The Seagull Nebula using Sulfer Hydrogen Oxygen Filters
IC 2177, known as the Seagull Nebula, is a large and complex region of emission and reflection nebulosity located roughly 3,800 light-years away, straddling the border between the constellations Monoceros and Canis Major. An interesting fact about this nebula is that it spans over 100 light-years in diameter, making it one of the more expansive nebulae visible in the sky. What makes the Seagull Nebula particularly fascinating is its appearance, which closely resembles the head and wings of a seagull in flight. This visual impression is formed by the bright, arc-like structures that represent the wings and a central bright region that appears as the head.
The nebula is an active site of star formation, lit up by the radiation from young, hot stars within it. The different colors within the nebula are a result of various elements being ionized, primarily hydrogen, which glows red, and traces of other elements that add subtler hues to the mix.
IC 2177 provides a beautiful example of the complex processes and structures that occur within star-forming regions, offering both stunning visuals and valuable insights into the life cycle of stars.
Matte Canvas, Stretched, 1.25"
Materials: cotton and polyester composite (canvas), pine wood (frame)
Soft rubber dots on bottom back corners for support
Back hanging included
Inner frame made with radiata pine sourced from renewable forests
Due to the production process of the canvases, please allow for slight size deviations with a tolerance +/- 1/8" (3.2mm)
