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Crescent nebula — Emission Nebula in Cygnus

NGC 6888

Emission Nebula Excellent (64/100)
Magnitude 7.4m EmissionNebula Cygnus (Cyg) Visible
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About Crescent nebula

Description

The Crescent Nebula (NGC 6888) is an emission nebula in Cygnus, about 5,000 light-years away. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 colliding with slower material the star ejected when it was a red supergiant.

Observing Tips

A challenging visual target. An OIII filter is almost essential, revealing the crescent-shaped arc in an 8-inch or larger telescope. Located near the center of Cygnus in the rich Milky Way, which provides a spectacular star field. Best in summer.

History

Discovered by William Herschel on September 15, 1792. The nebula is a textbook example of a wind-blown bubble created by a massive star's violent final evolutionary stages before it eventually explodes as a supernova.

Fun Facts

The Wolf-Rayet star WR 136 at the center is losing mass at a staggering rate and will likely explode as a supernova within a few hundred thousand years. The nebula is expanding at about 75 km/s.

Observe

1Properties

Magnitude 7.44
Angular Size 20.0′ × 10.0′
F, vL, vmE, ** att

Position & Identifiers

RA 20h 12m 06.6s
Dec +38° 21' 17.6"
Constellation Cygnus (Cyg)
Catalog NGC 6888

2How easy to spot?

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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Medium+ Medium+ Medium+
150mm Newt. Medium+ Medium+ Medium+
C8 203mm Medium+ Medium+ Medium+
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

With O-III filter

Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy on Seestar S50

3Visibility

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Best season Jun – Aug (peak: Jul)

4 Filter Response Guide

5 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

Crescent nebula · 20.0′×10.0′ · N up, E left

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6 Surface Brightness

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