Orion Bar

E460827

Orion Bar is a bright, elongated photodissociation region at the edge of the Orion Nebula, where intense ultraviolet radiation from young massive stars shapes and illuminates dense molecular gas and dust.

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Statements (47)

Predicate Object
instanceOf astrophysical structure
photodissociation region
astronomicalRegionType bright rim
ionization front
photon-dominated region
contains atomic gas
dense molecular gas
interstellar dust
ionized gas
distanceFromEarth approximately 1350 light-years
approximately 414 parsecs
hasDensityGradient true
hasNearbyExcitingStars Theta1 Orionis C NERFINISHED
hasPhysicalProcess heating by photoelectric effect on dust grains
molecular hydrogen excitation
photodissociation of molecules
photoevaporation flows
photoionization
polycyclic aromatic hydrocarbon emission
hasSharpTransitionBetween ionized gas and molecular gas
hasStrongEmissionFrom carbon monoxide
fine-structure lines of ionized atoms
ionized carbon
molecular hydrogen
polycyclic aromatic hydrocarbons
hasTemperatureGradient true
illuminatedBy ultraviolet radiation
isBright true
isEdgeOn true
isElongated true
isShapedBy Theta1 Orionis C NERFINISHED
isTargetOf ALMA observations
Herschel Space Observatory observations
Hubble Space Telescope observations
Spitzer Space Telescope observations
isUsedAs benchmark for interstellar chemistry models
benchmark for photon-dominated region models
template photodissociation region
locatedIn Orion Molecular Cloud Complex NERFINISHED
Orion Nebula NERFINISHED
locatedInConstellation Orion NERFINISHED
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
submillimeter wavelengths
ultraviolet wavelengths
shapedBy ultraviolet radiation

Referenced by (1)

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