Large Magellanic Cloud
E20343
The Large Magellanic Cloud is a nearby irregular dwarf galaxy visible from the Southern Hemisphere and notable for its role in studies of galaxy formation, stellar evolution, and the cosmic distance scale.
All labels observed (3)
| Label | Occurrences |
|---|---|
| Large Magellanic Cloud canonical | 29 |
| Large Magellanic Cloud as a nebulous patch (for southern observers) | 1 |
| Milky Way satellite galaxy Large Magellanic Cloud | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T156306 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Large Magellanic Cloud Context triple: [Milky Way, hasSatellite, Large Magellanic Cloud]
-
A.
Triangulum Galaxy
The Triangulum Galaxy is a nearby spiral galaxy in the Local Group, notable as one of the closest large galaxies to the Milky Way and a companion to the Andromeda Galaxy.
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B.
Andromeda Galaxy
The Andromeda Galaxy is the nearest large spiral galaxy to the Milky Way and is on a collision course to eventually merge with it.
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C.
Milky Way
The Milky Way is the barred spiral galaxy that contains our Solar System and hundreds of billions of other stars.
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D.
Milky Way center
The Milky Way center is the dense, energetic core of our galaxy, hosting a supermassive black hole surrounded by stars, gas, and dust.
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E.
Orion Arm
The Orion Arm is a minor spiral arm of the Milky Way galaxy that contains our Solar System and many of the stars visible in the night sky.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Large Magellanic Cloud Target entity description: The Large Magellanic Cloud is a nearby irregular dwarf galaxy visible from the Southern Hemisphere and notable for its role in studies of galaxy formation, stellar evolution, and the cosmic distance scale.
-
A.
Triangulum Galaxy
The Triangulum Galaxy is a nearby spiral galaxy in the Local Group, notable as one of the closest large galaxies to the Milky Way and a companion to the Andromeda Galaxy.
-
B.
Andromeda Galaxy
The Andromeda Galaxy is the nearest large spiral galaxy to the Milky Way and is on a collision course to eventually merge with it.
-
C.
Milky Way
The Milky Way is the barred spiral galaxy that contains our Solar System and hundreds of billions of other stars.
-
D.
Milky Way center
The Milky Way center is the dense, energetic core of our galaxy, hosting a supermassive black hole surrounded by stars, gas, and dust.
-
E.
Orion Arm
The Orion Arm is a minor spiral arm of the Milky Way galaxy that contains our Solar System and many of the stars visible in the night sky.
- F. None of above. chosen
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical object
ⓘ
galaxy ⓘ irregular dwarf galaxy ⓘ satellite galaxy ⓘ |
| abbreviation | LMC ⓘ |
| angularSize | about 10 degrees across on the sky ⓘ |
| apparentMagnitudeV | about 0.9 ⓘ |
| associatedWith | Magellanic Stream ⓘ |
| bestSeenFrom | southern mid-latitudes ⓘ |
| connectedBy |
Magellanic Bridge
ⓘ
surface form:
Magellanic Bridge to the Small Magellanic Cloud
|
| constellation | Dorado ⓘ |
| contains |
30 Doradus
ⓘ
SN 1987A ⓘ Tarantula Nebula ⓘ numerous H II regions ⓘ old globular clusters ⓘ young massive star clusters ⓘ |
| diameter | about 14000 light-years ⓘ |
| discovery | known since antiquity to southern observers ⓘ |
| distanceFromMilkyWay |
about 160000 light-years
ⓘ
about 50 kiloparsecs ⓘ |
| galaxyType |
Magellanic irregular
ⓘ
barred Magellanic spiral ⓘ |
| hasFeature |
Magellanic Bridge
ⓘ
extended gaseous disk ⓘ prominent bar structure ⓘ warped disk ⓘ |
| interactsGravitationallyWith |
Milky Way
ⓘ
Small Magellanic Cloud ⓘ |
| locatedIn | Local Group ⓘ |
| mass | on the order of 10^10 solar masses ⓘ |
| metallicity | lower than Milky Way average ⓘ |
| name | Large Magellanic Cloud self-link ⓘ |
| namedAfter | Ferdinand Magellan ⓘ |
| observedBy |
Gaia observatory
ⓘ
surface form:
Gaia spacecraft
Hubble Space Telescope ⓘ ground-based telescopes worldwide ⓘ |
| orbitalCompanionOf | Small Magellanic Cloud ⓘ |
| orbitalStatus | possibly on first infall into the Milky Way halo ⓘ |
| regionOfSky | southern celestial hemisphere ⓘ |
| satelliteOf | Milky Way ⓘ |
| starFormationRate | relatively high for its size ⓘ |
| stellarMass | on the order of 10^9 solar masses ⓘ |
| usedFor |
Cepheid period–luminosity relation calibration
ⓘ
calibration of the cosmic distance scale ⓘ studies of galaxy formation ⓘ studies of stellar evolution ⓘ |
| visibleFrom | 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.
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.
Subject: Large Magellanic Cloud Description of subject: The Large Magellanic Cloud is a nearby irregular dwarf galaxy visible from the Southern Hemisphere and notable for its role in studies of galaxy formation, stellar evolution, and the cosmic distance scale.
Referenced by (31)
Full triples — surface form annotated when it differs from this entity's canonical label.