The nebula’s popular name, “The Medusa Nebula,” is derived from the braided and serpentine filaments of glowing gas observed in its structure. Additionally, this nebula is designated as Abell 21 and is classified as an old planetary nebula, situated at a distance of approximately 1,500 light-years within the Gemini constellation. Similarly to its mythological namesake, the nebula is associated with a dramatic transformation. The planetary nebula phase represents the final stage of evolution for low-mass stars like the Sun, marking their transformation from red giants to hot white dwarf stars and the subsequent shedding of their outer layers. Ultraviolet radiation from the hot star powers the nebular glow. The Medusa’s transforming star is the faint one near the center of the overall bright crescent shape. In this deep telescopic view, fainter filaments clearly extend below and to the left. The estimated diameter of the Medusa Nebula is over four light-years.
Tag Archives: Stars
Stars and Dust in the Pacman Nebula
Stars are capable of creating extensive and complex dust structures from the dense and opaque molecular clouds from which they originate. The tools employed by stars to create their intricate structures are high-energy light and fast stellar winds. The heat generated by the stars causes the dark molecular dust to evaporate and also disperses and causes the ambient hydrogen gas to glow. The image depicts a nascent open cluster of stars, designated IC 1590, encircling the intricate interstellar dust structures within the emission nebula NGC 281. This nebula has been informally dubbed the “Pac-Man Nebula” due to its distinctive overall shape. The dust cloud situated just above the center of the image is classified as a Bok Globule, which may gravitationally collapse and form a star or stars. The Pacman Nebula is situated approximately 10,000 light-years away, within the constellation of Cassiopeia.