IC418

E540379

IC 418 is a small, bright planetary nebula in the constellation Lepus, often called the Spirograph Nebula for its intricate, filamentary appearance.

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Observed surface forms (1)

Surface form Occurrences
IC 418 0

Statements (44)

Predicate Object
instanceOf emission nebula
planetary nebula
alternativeName Spirograph Nebula NERFINISHED
angularDiameter ~12 arcseconds
apparentMagnitudeV ~9.6
bestSeenIn small to medium amateur telescopes
catalog Index Catalogue NERFINISHED
catalogNumber IC 418 NERFINISHED
centralStarEffectiveTemperature ~39,000 K
centralStarType hot white dwarf
declination -12° 42′ (approx)
discoveredBy Williamina Fleming NERFINISHED
discoveryYear 1891
distanceFromEarth ~1.1 kiloparsecs
~3600 light-years
dominantEmissionLines H-alpha
[N II]
[O III]
evolutionaryStage late stage of low- to intermediate-mass star
excitationClass high-excitation nebula
expandingGas ionized gas shell
formationMechanism ejected outer layers of dying star
hasCentralStarMagnitude ~10.2
hasColor reddish and greenish hues in images
hasStructure fainter outer halo
inner bright shell
imageNicknameOrigin Spirograph-like pattern in HST images
ionizationSource ultraviolet radiation from central star
locatedInConstellation Lepus NERFINISHED
locatedInGalaxy Milky Way NERFINISHED
morphologicalType elliptical planetary nebula
notableFor high surface brightness
intricate filamentary structure
ring-like inner shell
observedBy Hubble Space Telescope NERFINISHED
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
rightAscension 05h 27m (approx)
shapeDescription nearly circular on the sky
spectralFeatures recombination lines of hydrogen and helium
strong forbidden lines
surfaceBrightness high
visibleFromHemisphere Southern Hemisphere NERFINISHED

Referenced by (1)

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