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.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Southern Ring Nebula canonical | 6 |
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 |
Galactic thin disk
ⓘ
surface form:
Milky Way 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
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
Instruction
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Input
Subject: Southern Ring Nebula Description of subject: 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.
Referenced by (6)
Full triples — surface form annotated when it differs from this entity's canonical label.