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 ⓘ