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.

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All labels observed (1)

Label Occurrences
NGC 281 (Pacman Nebula) canonical 1

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 IC 1848 (Soul Nebula)
surface form: Sharpless 184
hasStarFormationMode triggered star formation
ionizingSource massive O-type stars in IC 1590
isIncludedInCatalogue H II regions
surface form: Sharpless catalog of 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

Referenced by (1)

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

Perseus Arm contains NGC 281 (Pacman Nebula)