NGC 1976

E506956

NGC 1976, better known as the Orion Nebula (M42), is a bright, nearby emission nebula in the constellation Orion and one of the most studied stellar nurseries in the night sky.

All labels observed (2)

Label Occurrences
NGC 1976 canonical 5
NGC 1976 is the Orion Nebula 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf H II region
Messier object
emission nebula
alsoKnownAs M42
Messier 42
Orion Nebula
angularSize about 65×60 arcminutes
apparentMagnitudeV about 4.0
catalogCode M42
NGC 1976
Sh 2-281
contains brown dwarfs
ionized hydrogen gas
molecular clouds
protoplanetary disks
protostars
young stars
declination −05° 23′
discoveredBy Nicolas-Claude Fabri de Peiresc
discoveryYear 1610
distanceFromEarth about 1340 light-years
about 410 parsecs
emits strong hydrogen-alpha radiation
excitedBy Theta1 Orionis C
massive O-type stars
hasAge about 1–3 million years for its youngest stars
hasComponent Trapezium Cluster
hasRole laboratory for studying star formation
is one of the brightest nebulae in the night sky
one of the closest massive star-forming regions to Earth
one of the most studied star-forming regions
visible to the naked eye
locatedIn Milky Way
Orion Arm
locatedInConstellation Orion
near NGC 1982
linked to: NGC 1973

Running Man Nebula
observedBy Chandra X-ray Observatory
Hubble Space Telescope
Spitzer Space Telescope
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
partOf Orion Molecular Cloud Complex
regionType stellar nursery
rightAscension 05h 35m
spectralTypeDominantExcitingStar O6

How these facts were elicited

Referenced by (6)

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

Orion Nebula alsoKnownAs NGC 1976
M42 alsoKnownAs NGC 1976
NGC hasNotableEntry NGC 1976
NGC notableEntryExample NGC 1976 is the Orion Nebula
linked to: NGC 1976
NGC 1976 catalogCode NGC 1976