NGC 281 (Pacman Nebula)

E109442

NGC 281, commonly known as the Pacman Nebula, is an emission nebula and active star-forming region in the constellation Cassiopeia, notable for its distinctive shape and embedded young star cluster IC 1590.

All labels observed (1)

Label Occurrences
NGC 281 (Pacman Nebula) canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf H II region ⓘ
emission nebula ⓘ
nebula ⓘ
star-forming region ⓘ
alsoKnownAs Pacman Nebula ⓘ
angularSize ~35 arcminutes ⓘ
apparentMagnitudeV 7.4 ⓘ
associatedWith radio source W1 ⓘ
bestSeenInMonth October ⓘ
bestSeenInSeason northern autumn ⓘ
catalog New General Catalogue ⓘ
contains Bok globules ⓘ
dark dust lanes ⓘ
molecular clouds ⓘ
pre-main-sequence stars ⓘ
young stellar objects ⓘ
declination +56° 37′ ⓘ
discoveredBy Edward Emerson Barnard ⓘ
discoveryYear 1883 ⓘ
distanceFromEarth ~2.9 kiloparsecs ⓘ
~9500 light-years ⓘ
excitedBy ultraviolet radiation from massive stars ⓘ
galacticLatitude −6.31° ⓘ
galacticLongitude 123.07° ⓘ
hasDominantEmissionLine H-alpha ⓘ
[O III] ⓘ
hasEmbeddedStarCluster IC 1590 ⓘ
hasMorphologicalType emission nebula with dark lanes ⓘ
hasNebulaType diffuse nebula ⓘ
hasOpenCluster IC 1590 ⓘ
hasRegionDesignation Sharpless 184 ⓘ
hasStarFormationMode triggered star formation ⓘ
ionizingSource massive O-type stars in IC 1590 ⓘ
isIncludedInCatalogue Sharpless catalog of H II regions ⓘ
linked to: H II regions
isInNorthernSky true ⓘ
isTargetOf infrared surveys ⓘ
radio observations of molecular gas ⓘ
star formation studies ⓘ
locatedInConstellation Cassiopeia ⓘ
notableFor active star formation ⓘ
distinctive Pacman-like shape ⓘ
observedInWavelength infrared ⓘ
optical ⓘ
radio ⓘ
partOf Perseus Spiral Arm ⓘ
rightAscension 00h 52m ⓘ
visibleWith small amateur telescopes under dark skies ⓘ

How these facts were elicited

Referenced by (1)

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

Perseus Arm → contains → NGC 281 (Pacman Nebula) ⓘ