Ring Nebula

E461994

The Ring Nebula is a famous planetary nebula in the constellation Lyra, known for its bright, ring-shaped shell of ionized gas surrounding a hot central white dwarf.

All labels observed (1)

Label Occurrences
Ring Nebula canonical 3

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf astronomical object
deep-sky object
emission nebula
planetary nebula
age on the order of several thousand years
alsoKnownAs M57
Messier 57
NGC 6720
angularSize about 1.4 × 1.0 arcminutes
apparentMagnitudeV 8.8
bestSeenIn summer sky of the Northern Hemisphere
catalog Messier catalogue
New General Catalogue
centralStarApparentMagnitude about 15.8
centralStarEffectiveTemperature about 100,000 K
declination +33° 01′ 45″
discoveredBy Antoine Darquier de Pellepoix
discoveryYear 1779
distanceFromEarth about 2,300 light-years
about 700 parsecs
dominantEmissionLines H-alpha
He II
[O III]
hasCentralStar white dwarf
hasHalo faint outer halo of gas
hasMorphology elliptical planetary nebula
imagedBy Hubble Space Telescope
James Webb Space Telescope
ionizationSource ultraviolet radiation from central white dwarf
locatedIn Galactic halo
Milky Way
locatedInConstellation Lyra
messierNumber M57
nearbyObject Sheliak (Beta Lyrae)
linked to: β Lyrae

Sulafat (Gamma Lyrae)
nebulaExpansionVelocity about 20–30 km/s
ngcNumber NGC 6720
observableWith small telescope
observedIn infrared wavelengths
optical wavelengths
ultraviolet wavelengths
origin ejected outer layers of a dying star
partOf Lyra constellation region near Vega
physicalDiameter about 1 light-year
progenitorStarMass about 1.2 solar masses
rightAscension 18h 53m 35.1s
shape ring-like shell
spectralTypeOfCentralStar DAO white dwarf
structure ionized gas shell

How these facts were elicited

Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Messier 57 alsoKnownAs Ring Nebula