NGC 1499

E509186

NGC 1499, also known as the California Nebula, is a large emission nebula in the constellation Perseus notable for its shape resembling the U.S. state of California.

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Statements (45)

Predicate Object
instanceOf H II region
emission nebula
alsoKnownAs California Nebula NERFINISHED
angularSize about 2.5 degrees
apparentMagnitudeV 5.0
associatedWithStar ξ Persei NERFINISHED
bestSeenFromHemisphere Northern Hemisphere NERFINISHED
bestSeenInSeason northern winter
catalog New General Catalogue NERFINISHED
catalogNumber NGC 1499 NERFINISHED
commonFor astrophotography
contains interstellar dust
interstellar gas
declination +36° 25′
discoveredBy Edward Emerson Barnard NERFINISHED
discoveryYear 1884
distanceFromEarth about 1000 light-years
about 300 parsecs
emissionLine hydrogen-alpha
galacticLatitude about -15 degrees
galacticLongitude about 160 degrees
hasColor reddish
influences star formation in surrounding molecular clouds
ionizationSource ultraviolet radiation from Xi Persei
ionizingStar Xi Persei NERFINISHED
locatedIn Milky Way
Orion Arm NERFINISHED
locatedInConstellation Perseus NERFINISHED
locatedInSkyRegion near Xi Persei
namedAfter California NERFINISHED
nebulaType emission
observedBy amateur astronomers
professional astronomers
observedInWavelength H-alpha
optical
partOf Perseus molecular cloud complex NERFINISHED
local spiral structure of the Milky Way
requiresFilterForBestView H-beta filter
UHC filter NERFINISHED
rightAscension 04h 03m
shapeResembles U.S. state of California NERFINISHED
spectralTypeOfIonizingStar O7.5III (Xi Persei) NERFINISHED
surfaceBrightness low
visibleInBinoculars yes
visibleToNakedEye under very dark skies

Referenced by (2)

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

NGC 1499 (California Nebula) catalogCode NGC 1499
subject surface form: NGC 1499