This is my image of the IC 4628, also known as the Prawn Nebula, an emission nebula located in the southern constellation Scorpius. It is a region of active star formation and is characterized by its vibrant colors and intricate structures.The Prawn Nebula gets its name from its resemblance to a prawn or shrimp, with its curved shape and elongated body. It spans a large area in the night sky and is located at a distance of approximately 6,000 light-years from Earth.The nebula is primarily composed of ionized hydrogen gas, which emits light in the red part of the spectrum, giving it its characteristic red color. The intense ultraviolet radiation from young, massive stars embedded within the nebula excites the surrounding gas, causing it to glow and create the emission nebula.IC 4628 is associated with a cluster of young stars that formed within the nebula. These young stars are still surrounded by the remnants of the gas and dust clouds from which they were born. Their powerful stellar winds and intense radiation shape the surrounding nebula and sculpt its intricate features.Observing IC 4628 with telescopes or astrophotography equipment reveals a wealth of detail and structure within the nebula. Dark patches and filaments of dust can be seen, interspersed with regions of intense star formation and glowing gas.The Prawn Nebula is a popular target for astrophotographers and astronomers due to its striking appearance and the scientific insights it provides into the process of star formation. By studying regions like IC 4628, astronomers can better understand the mechanisms and conditions that lead to the birth of new stars.Overall, IC 4628, or the Prawn Nebula, is a captivating emission nebula located in the constellation Scorpius, exhibiting intricate structures and vibrant colors, and serving as a window into the fascinating process of stellar birth and evolution