Orion Nebula Cluster

E514712

The Orion Nebula Cluster is a dense, young star cluster embedded within the Orion Nebula, notable as one of the nearest and most studied regions of active star formation.

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Statements (50)

Predicate Object
instanceOf embedded cluster
open star cluster
young stellar cluster
age about 1 million years
ageRange less than 3 million years
alsoKnownAs ONC NERFINISHED
Trapezium Cluster NERFINISHED
centralStarsDesignation Theta1 Orionis NERFINISHED
containsApproximateNumberOfStars about 2000
between 2000 and 4000
containsObject B-type stars
Herbig–Haro objects NERFINISHED
T Tauri stars NERFINISHED
Trapezium stars NERFINISHED
brown dwarfs
dust
ionized gas
massive O-type stars
molecular gas
protoplanetary disks
distanceFromEarth about 1350 light-years
about 414 parsecs
hasAngularSize about 20 arcminutes
hasCoreRegion Trapezium NERFINISHED
hasInitialMassFunction well-studied initial mass function
hasMass several thousand solar masses
hasProperty contains many pre-main-sequence stars
mass-segregated
rich in circumstellar disks
strong nebular emission
hasStellarDensity high central stellar density
ionizedBy Theta1 Orionis C NERFINISHED
isEmbeddedIn H II region
giant molecular cloud
isOneOf best-studied young clusters
nearest massive star-forming regions to Earth
isRegionOf active star formation
locatedIn Orion Molecular Cloud Complex NERFINISHED
Orion Nebula NERFINISHED
locatedInConstellation Orion NERFINISHED
observedBy Chandra X-ray Observatory NERFINISHED
Hubble Space Telescope NERFINISHED
Spitzer Space Telescope NERFINISHED
Very Large Telescope NERFINISHED
observedInWavelength X-ray
infrared
optical
partOf Orion A molecular cloud NERFINISHED
usedAs benchmark for pre-main-sequence evolution models
laboratory for star formation studies

Referenced by (1)

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

Orion Nebula hostTo Orion Nebula Cluster