NGC 6888 - Cygnus

Nebulosa de la Luna Creciente
NGC6888 pertenece a la constelación de Cygnus
NGC 6888 es una nebulosa de emisión llamada la Nebulosa del Creciente o Crescent Nebula.

Es una nebulosa muy interesante enclavada en el largo cuello del Cisne, no es sencilla de de fotografiar por su bajo brillo por unidad de superficie. Con menos 40 minutos de exposición en total no tendremos una fotografía muy clara, aunque eso sí, admite muy bien con fltros tipo UHC o CLS.

En su centro hay una estrella gigante roja de la 7.5 magnitud es una en las últimas etapas de su vida llamada WR-136. Esta estrella expulsó, en su fase de conversión en gigante roja, sus capas exteriores hace cientos de miles o millones de años. En la actualidad produce un viento y una radiación que atrapan la emisión anterior y es son responsables del brillo actual de la nebulosa.

NGC6888 - Nebulosa de la Luna Creciente - en la IA

NGC 6888, also known as the Crescent Nebula, is a stunning emission nebula located in the constellation Cygnus. Here's a breakdown of what makes it so interesting:

Key Features:

  • Shape: It's characterized by its distinct, curved shape, resembling a crescent moon or a bubble. This shape gives it its common name.
  • Type: It's a Wolf-Rayet nebula, formed by the interaction of a fast stellar wind from a massive star with slower moving material ejected earlier in its life.
  • Central Star: The nebula is sculpted by the powerful stellar wind emanating from the Wolf-Rayet star WR 136. This is a hot, luminous star nearing the end of its life.
  • Distance: Located approximately 5,000 light-years away from Earth.
  • Size: It spans roughly 25 light-years in diameter.
  • Composition: The nebula is composed primarily of ionized hydrogen, oxygen, and nitrogen. The different colors you see in images often represent these elements.

Formation and Evolution:

  1. Massive Star Evolution: WR 136 was originally a much larger star (around 40-50 times the mass of the Sun). As massive stars age, they lose mass through powerful stellar winds.
  2. Earlier Mass Loss: Before becoming a Wolf-Rayet star, WR 136 likely went through a red giant or supergiant phase, during which it expelled a large amount of material at a slower pace.
  3. Collision of Winds: The fast stellar wind from the WR star is now colliding with the slower moving material ejected earlier. This collision creates a shockwave that heats and compresses the gas, causing it to glow and form the crescent shape.
  4. Future Supernova: WR 136 is nearing the end of its life and will eventually explode as a supernova. This will dramatically change the nebula's appearance and disperse the gas and dust.

Observing NGC 6888:

  • Location: Found in the constellation Cygnus, near the bright star Sadr (Gamma Cygni).
  • Telescope: It requires a telescope to see well, and even then, it can be challenging due to its faintness. A larger aperture telescope and dark skies are essential for good views.
  • Filters: Narrowband filters, especially those that isolate the light of hydrogen-alpha (Hα) and oxygen-III (OIII), can significantly enhance the contrast and reveal the nebula's intricate details.
  • Astrophotography: A popular target for astrophotography due to its stunning appearance and complex structure. Long exposure times and careful processing are needed to capture its faint details.

In short, NGC 6888 is a beautiful and fascinating example of stellar evolution in action, showcasing the dramatic processes that shape the universe.

Más información sobre NGC 6888 en NASA/IPAC.

Mapa alrededor de NGC 6888


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Wednesday, June 25, 2025 11:32:10 PM
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Otros identificadores de NGC6888:
"LBN 203" ,"LBN 075.51+02.29" ,"NGC 6888" ,"[T70] 32" ,"NAME Crescent Nebula",