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.

All labels observed (1)

Label Occurrences
Seagull Nebula canonical 2

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf H II region
astronomical object
emission nebula
alsoKnownAs IC 2177
Sh 2-292
angularSize about 2.5 degrees
apparentMagnitude about 5.9
associatedWith Galactic plane
bestSeenAt dark skies
bestSeenIn winter months
catalog Index Catalogue
Sharpless catalog
linked to: Sharpless catalogue
contains dark nebulae
massive OB stars
open cluster NGC 2335
open cluster NGC 2343
linked to: NGC 2343

reflection nebulae
young stellar objects
declination -10° 20′
discoveredBy Isaac Roberts
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
Sh 2-293
Sh 2-294
ionizedBy hot young stars
liesOnBorderOf Canis Major
Monoceros
locatedIn Orion Arm
locatedInConstellation Canis Major
Monoceros
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
partOf Milky Way
regionType massive star-forming complex
requires wide-field telescope for full extent
rightAscension 06h 16m
shapeDescribedAs bird-shaped
seagull-shaped
visibleFrom Northern Hemisphere
Southern Hemisphere

How these facts were elicited

Referenced by (2)

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

Monoceros contains Seagull Nebula
IC 2177 alsoKnownAs Seagull Nebula