NGC 1499 (California Nebula)

E113786

NGC 1499, commonly known as the California Nebula, is a large, faint emission nebula in the constellation Perseus whose shape resembles the outline of the U.S. state of California.

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All labels observed (1)

Label Occurrences
NGC 1499 (California Nebula) canonical 1

Statements (47)

Predicate Object
instanceOf H II region
diffuse nebula
emission nebula
alsoKnownAs California Nebula
angularSize about 145 arcminutes × 40 arcminutes
apparentMagnitudeV 5.0
associatedStar ξ Persei
surface form: Xi Persei
bestSeenIn long-exposure astrophotography
bestSeenWith binoculars under dark skies
wide-field telescope
catalog New General Catalogue
catalogCode NGC 1499
contains interstellar dust
interstellar gas
containsEmission [N II] lines
[S II] lines
hydrogen recombination lines
declination +36° 25′
discoveredBy Edward Emerson Barnard
discoveryYear 1884
distanceFromEarth about 1000 light-years
about 300 parsecs
dominantColor red
dominantEmissionLine H-alpha
environment star-forming region
excitedBy ultraviolet radiation from Xi Persei
galacticLatitude about -8°
galacticLongitude about 160°
hasFeature elongated north–south structure
filamentary edges
ionizingSource ξ Persei
surface form: Xi Persei
locatedIn Milky Way
Orion Arm
locatedInConstellation Perseus
namedAfter California, United States
surface form: California
observedInWavelength infrared
optical
radio
partOf Perseus molecular cloud complex
local interstellar medium of Perseus arm
requires dark skies for naked-eye visibility
rightAscension 04h 03m
shapeResembles outline of the U.S. state of California
spectralTypeOfExcitingStar ξ Persei
surface form: O7.5III (Xi Persei)
typeOfNebula photoionized nebula
visibleFromHemisphere Northern Hemisphere
visibleIn small telescopes as faint glow

Referenced by (1)

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

Perseus Arm contains NGC 1499 (California Nebula)