IC418

E540379

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

All labels observed (1)

Label Occurrences
IC418 canonical 1

How this entity was disambiguated

Statements (44)

Predicate Object
instanceOf emission nebula ⓘ
planetary nebula ⓘ
alternativeName Spirograph Nebula ⓘ
angularDiameter ~12 arcseconds ⓘ
apparentMagnitudeV ~9.6 ⓘ
bestSeenIn small to medium amateur telescopes ⓘ
catalog Index Catalogue ⓘ
catalogNumber IC 418 ⓘ
centralStarEffectiveTemperature ~39,000 K ⓘ
centralStarType hot white dwarf ⓘ
declination -12° 42′ (approx) ⓘ
discoveredBy Williamina Fleming ⓘ
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 ⓘ
locatedInGalaxy Milky Way ⓘ
morphologicalType elliptical planetary nebula ⓘ
notableFor high surface brightness ⓘ
intricate filamentary structure ⓘ
ring-like inner shell ⓘ
observedBy Hubble Space Telescope ⓘ
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 ⓘ

How these facts were elicited

Referenced by (1)

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