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 (1)

Label Occurrences
NGC 1976 canonical 2

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf H II region
Messier object
emission nebula
alsoKnownAs M42 NERFINISHED
Messier 42 NERFINISHED
Orion Nebula NERFINISHED
angularSize about 65×60 arcminutes
apparentMagnitudeV about 4.0
catalogCode M42 NERFINISHED
NGC 1976 NERFINISHED
Sh 2-281 NERFINISHED
contains brown dwarfs
ionized hydrogen gas
molecular clouds
protoplanetary disks
protostars
young stars
declination −05° 23′
discoveredBy Nicolas-Claude Fabri de Peiresc NERFINISHED
discoveryYear 1610
distanceFromEarth about 1340 light-years
about 410 parsecs
emits strong hydrogen-alpha radiation
excitedBy Theta1 Orionis C NERFINISHED
massive O-type stars
hasAge about 1–3 million years for its youngest stars
hasComponent Trapezium Cluster NERFINISHED
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 NERFINISHED
locatedInConstellation Orion NERFINISHED
near NGC 1982 NERFINISHED
Running Man Nebula NERFINISHED
observedBy Chandra X-ray Observatory NERFINISHED
Hubble Space Telescope NERFINISHED
Spitzer Space Telescope NERFINISHED
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
partOf Orion Molecular Cloud Complex NERFINISHED
regionType stellar nursery
rightAscension 05h 35m
spectralTypeDominantExcitingStar O6

How these facts were elicited

Referenced by (2)

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