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.

All labels observed (1)

Label Occurrences
Orion Bar canonical 2

How this entity was disambiguated

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 ⓘ
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 ⓘ
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 ⓘ
Orion Nebula ⓘ
locatedInConstellation Orion ⓘ
observedIn infrared wavelengths ⓘ
optical wavelengths ⓘ
radio wavelengths ⓘ
submillimeter wavelengths ⓘ
ultraviolet wavelengths ⓘ
shapedBy ultraviolet radiation ⓘ

How these facts were elicited

Referenced by (2)

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