Seagull Nebula

E555752

The Seagull Nebula is a large, bird-shaped emission nebula and star-forming region located along the border of the constellations Monoceros and Canis Major.

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Statements (46)

Predicate Object
instanceOf H II region
astronomical object
emission nebula
alsoKnownAs IC 2177 NERFINISHED
Sh 2-292 NERFINISHED
angularSize about 2.5 degrees
apparentMagnitude about 5.9
associatedWith Galactic plane
bestSeenAt dark skies
bestSeenIn winter months
catalog Index Catalogue NERFINISHED
Sharpless catalog NERFINISHED
contains dark nebulae
massive OB stars
open cluster NGC 2335 NERFINISHED
open cluster NGC 2343 NERFINISHED
reflection nebulae
young stellar objects
declination -10° 20′
discoveredBy Isaac Roberts NERFINISHED
discoveryYear 1893
distanceFromEarth 3700 light-years
approximately 1.1 kiloparsecs
dominantEmissionLine H-alpha
galacticLatitude -2.3 degrees
galacticLongitude 224.7 degrees
hasComponent Sh 2-292 NERFINISHED
Sh 2-293 NERFINISHED
Sh 2-294 NERFINISHED
ionizedBy hot young stars
liesOnBorderOf Canis Major NERFINISHED
Monoceros NERFINISHED
locatedIn Orion Arm NERFINISHED
locatedInConstellation Canis Major NERFINISHED
Monoceros NERFINISHED
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
partOf Milky Way NERFINISHED
regionType massive star-forming complex
requires wide-field telescope for full extent
rightAscension 06h 16m
shapeDescribedAs bird-shaped
seagull-shaped
visibleFrom Northern Hemisphere NERFINISHED
Southern Hemisphere NERFINISHED

Referenced by (1)

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

Monoceros contains Seagull Nebula