Messier 57

E457105

Messier 57, also known as the Ring Nebula, is a famous planetary nebula in the constellation Lyra formed from the expelled outer layers of a dying star.

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Statements (49)

Predicate Object
instanceOf Messier object
deep-sky object
emission nebula
planetary nebula
alsoKnownAs M57 NERFINISHED
NGC 6720 NERFINISHED
Ring Nebula NERFINISHED
angularSize about 1.4 × 1.0 arcminutes
apparentMagnitudeV 8.8
bestSeenIn medium telescopes
small telescopes
catalogNumber M57 NERFINISHED
NGC 6720 NERFINISHED
centralStar white dwarf
centralStarApparentMagnitude about 15.8
centralStarEffectiveTemperature about 120,000 K
declination +33° 01′ 45″
discoveredBy Antoine Darquier de Pellepoix NERFINISHED
Charles Messier NERFINISHED
discoveryYear 1779
distanceFromEarth about 2,300 light-years
about 700 parsecs
dominantEmissionLine [O III]
dominantEmissionLineWavelength 500.7 nm
estimatedAge about 7,000 years
galacticLatitude 13.99°
galacticLongitude 63.17°
hasFeature bright inner ring
fainter outer halo
filamentary structures
locatedIn Galactic halo region near the plane
Milky Way
locatedInConstellation Lyra NERFINISHED
morphology elliptical planetary nebula
nearTo bright star Vega NERFINISHED
constellation Cygnus border
nebulaExpansionVelocity about 20–30 km/s
observedIn infrared wavelengths
optical wavelengths
ultraviolet wavelengths
origin expelled outer layers of a dying star
partOf Messier catalogue NERFINISHED
New General Catalogue NERFINISHED
progenitorStarMass about 1.2 solar masses
rightAscension 18h 53m 35s
shape ring-like
spectralType emission-line nebula
visibleFrom Northern Hemisphere NERFINISHED
visibleSeason northern summer

Referenced by (2)

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

Charles Messier cataloged Messier 57
Messier catalogue contains Messier 57