Crescent Nebula

Crescent Nebula
Emission nebula
The Crescent Nebula, as taken by an amateur astronomer
Observation data: J2000.0 epoch
Right ascension20h 12m 7s[1]
Declination+38° 21.3′[1]
Distance5,000 ly
Apparent magnitude (V)+7.4
Apparent dimensions (V)18′ × 12′
ConstellationCygnus
DesignationsNGC 6888,[1] Sharpless 105, Caldwell 27
See also: Lists of nebulae
Crescent Nebula (Caldwell27) captured by David Rousseau from an urban location in Québec, Canada using Ha and OIII narrowband filters.

The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792.[2] It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000[3] to 400,000[citation needed] years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.

The Crescent Nebula is a rather small object located about 2 degrees Southwest of Sadr. While considered bright by astronomical imaging standards, visually it is relatively faint. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".

  • Crescent Nebula NGC 68888 Imaged by Don Christopher Deaver
    NGC 6888 in Hydrogen and Oxygen Light. HOO Palette. Imaged by Don Christopher Deaver
  • Crescent Nebula in H-alpha and OIII. Imaged with a 715mm focal length telescope. The hydrogen gas is red. The oxygen is blue.
    Crescent Nebula in H-alpha and OIII. Imaged with a 715mm focal length telescope. The hydrogen gas is red. The oxygen is blue.
  • Image of NGC 6888 using H-alpha filter.
    Image of NGC 6888 using H-alpha filter.
  • Picture of NGC 6888 captured in narrowband by amateur astronomer Luca Moretti
    Picture of NGC 6888 captured in narrowband by amateur astronomer Luca Moretti
  • NGC 6888 imaged in 3 nm hydrogen-alpha and oxygen-III narrowband at 2800mm focal length by amateur astronomer Patrick Hsieh.
    NGC 6888 imaged in 3 nm hydrogen-alpha and oxygen-III narrowband at 2800mm focal length by amateur astronomer Patrick Hsieh.
  1. ^ a b c "NGC 6888". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-04-23.
  2. ^ Erdmann, Robert. "NGC 6888". The NGC/IC Project. Archived from the original on 2012-05-20.
  3. ^ "WR 136". jumk.de. Retrieved 25 March 2018.