The Prawn Nebula, or IC 4628, is a colorful and expansive emission nebula located in the southern constellation Scorpius.
The nebula gets its name from its distinctive shape, which resembles a giant shrimp or prawn, and it's a site of active star formation, with numerous hot and young stars embedded within its clouds of gas and dust.
The intense radiation from these stars ionizes the surrounding gas, causing it to glow brightly in a range of vivid colors.
About the Deep Space Collection:
Shot entirely with my rooftop telescope from the urban skies of Buenos Aires, the Deep Space Collection features many objects observable only from the southern hemisphere.
All images in the collection were shot using individual narrowband filters which cut off most of the light and allow only very specific wavelengths to pass (the light emitted from ionized hydrogen, oxygen and sulfur), making it possible to photograph deep space objects even from the highly light polluted skies of the city.
The images from each separate filter are then processed individually, combined and mapped to RGB channels for a final color image.
Two different color mapping palettes were used in this collection: SHO, where sulfur is mapped to red, hydrogen to green and oxygen to blue in what is referred to as "Hubble Palette" processing (as used in the images the famous space telescope) and HOO, where hydrogen is mapped to red, and oxygen to blue and green.
Deep Space Collection # 16. The Prawn
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Deep Space Collection # 16. The Prawn
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The Prawn Nebula, or IC 4628, is a colorful and expansive emission nebula located in the southern constellation Scorpius.
The nebula gets its name from its distinctive shape, which resembles a giant shrimp or prawn, and it's a site of active star formation, with numerous hot and young stars embedded within its clouds of gas and dust.
The intense radiation from these stars ionizes the surrounding gas, causing it to glow brightly in a range of vivid colors.
About the Deep Space Collection:
Shot entirely with my rooftop telescope from the urban skies of Buenos Aires, the Deep Space Collection features many objects observable only from the southern hemisphere.
All images in the collection were shot using individual narrowband filters which cut off most of the light and allow only very specific wavelengths to pass (the light emitted from ionized hydrogen, oxygen and sulfur), making it possible to photograph deep space objects even from the highly light polluted skies of the city.
The images from each separate filter are then processed individually, combined and mapped to RGB channels for a final color image.
Two different color mapping palettes were used in this collection: SHO, where sulfur is mapped to red, hydrogen to green and oxygen to blue in what is referred to as "Hubble Palette" processing (as used in the images the famous space telescope) and HOO, where hydrogen is mapped to red, and oxygen to blue and green.