Southern Ring Nebula

E60084

The Southern Ring Nebula is a bright, roughly 2,000-light-year-distant planetary nebula in the constellation Vela, formed from the outer layers of a dying sun-like star and notable for its intricate, colorful gas shells.

AI illustration

How this image was made

AI-generated illustration of Southern Ring Nebula

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of the Southern Ring Nebula (The Southern Ring Nebula is a bright, roughly 2,000-light-year-distant planetary nebula in the constellation Vela, formed from the outer layers of a dying sun-like star and notable for its intricate, colorful gas shells.)

All labels observed (1)

Label Occurrences
Southern Ring Nebula canonical 6

How this entity was disambiguated

Statements (53)

Predicate Object
instanceOf emission nebula ⓘ
planetary nebula ⓘ
angularSize ~1.7 × 1.4 arcminutes ⓘ
apparentMagnitudeV 9.87 ⓘ
apparentShape elliptical ring ⓘ
approximateDistance about 2,000 light-years ⓘ
bestViewingSeason late southern summer and autumn ⓘ
catalogNumber C 74 ⓘ
NGC 3132 ⓘ
centralBinaryComponent sun-like companion star ⓘ
white dwarf remnant ⓘ
centralStarMass about 0.6 solar masses ⓘ
centralStarType white dwarf ⓘ
colorAppearance bluish-green interior with reddish outer regions in optical images ⓘ
constellation Vela ⓘ
contains central binary star system ⓘ
declination −40° 26′ 11″ ⓘ
discoveredBy John Herschel ⓘ
discoveryYear 1835 ⓘ
distanceFromEarth 2000 light-years ⓘ
dominantEmissionLines hydrogen ⓘ
nitrogen ⓘ
oxygen ⓘ
evolutionaryPhase late stage of low- to intermediate-mass star evolution ⓘ
featuredIn first full-color images released by James Webb Space Telescope in July 2022 ⓘ
formationMechanism ejected outer layers of a dying star ⓘ
galacticRegion Milky Way disk ⓘ
linked to: Galactic thin disk
gasComposition heavier elements such as carbon, nitrogen, and oxygen ⓘ
helium ⓘ
hydrogen-rich gas ⓘ
JWSTInstrumentUsed MIRI ⓘ
NIRCam ⓘ
locatedIn Milky Way ⓘ
notableFeature bright inner ring structure ⓘ
complex, asymmetric morphology ⓘ
fainter extended halo ⓘ
intricate shells of ionized gas ⓘ
multiple nested gas shells ⓘ
observedBy Hubble Space Telescope ⓘ
James Webb Space Telescope ⓘ
ground-based telescopes ⓘ
observedIn infrared wavelengths ⓘ
optical wavelengths ⓘ
ultraviolet wavelengths ⓘ
otherName Caldwell 74 ⓘ
Eight-Burst Nebula ⓘ
NGC 3132 ⓘ
progenitorStarType Sun-like star ⓘ
rightAscension 10h 07m 01s ⓘ
shapingMechanism interaction of stellar winds and binary companion ⓘ
spectralTypeOfCompanion roughly solar-type star ⓘ
structure inner bright ring and outer diffuse envelope ⓘ
visibility best observed from Southern Hemisphere ⓘ

How these facts were elicited

Referenced by (6)

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

NGC 3132 → hasAlternativeName → Southern Ring Nebula ⓘ
Eight-Burst Nebula → hasAlternativeName → Southern Ring Nebula ⓘ
Caldwell 74 → hasAlternativeName → Southern Ring Nebula ⓘ
Caldwell 74 → hasCommonName → Southern Ring Nebula ⓘ
C 74 → hasAlternativeName → Southern Ring Nebula ⓘ