Messier 92
E925091
Messier 92 is a bright, ancient globular star cluster located in the constellation Hercules, notable for its high stellar density and visibility even in small telescopes.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Messier 92 canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T11376967 — 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: Messier 92 Context triple: [Hercules, contains, Messier 92]
-
A.
Messier 55
Messier 55 is a large, relatively loose globular star cluster located in the constellation Sagittarius, visible in small telescopes as a faint, diffuse ball of stars.
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B.
Messier 14
Messier 14 is a bright globular star cluster in the constellation Ophiuchus, composed of hundreds of thousands of ancient stars densely packed together.
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C.
Messier 69
Messier 69 is a dense, metal-rich globular star cluster located in the constellation Sagittarius near the center of the Milky Way.
-
D.
Messier 13
Messier 13 is a prominent globular star cluster in the constellation Hercules, renowned as one of the brightest and most studied such clusters in the northern sky.
-
E.
Messier 54
Messier 54 is a dense globular star cluster located in the constellation Sagittarius, notable for being one of the first globular clusters found to belong to a dwarf galaxy outside the Milky Way.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Messier 92 Target entity description: Messier 92 is a bright, ancient globular star cluster located in the constellation Hercules, notable for its high stellar density and visibility even in small telescopes.
-
A.
Messier 55
Messier 55 is a large, relatively loose globular star cluster located in the constellation Sagittarius, visible in small telescopes as a faint, diffuse ball of stars.
-
B.
Messier 14
Messier 14 is a bright globular star cluster in the constellation Ophiuchus, composed of hundreds of thousands of ancient stars densely packed together.
-
C.
Messier 69
Messier 69 is a dense, metal-rich globular star cluster located in the constellation Sagittarius near the center of the Milky Way.
-
D.
Messier 13
Messier 13 is a prominent globular star cluster in the constellation Hercules, renowned as one of the brightest and most studied such clusters in the northern sky.
-
E.
Messier 54
Messier 54 is a dense globular star cluster located in the constellation Sagittarius, notable for being one of the first globular clusters found to belong to a dwarf galaxy outside the Milky Way.
- F. None of above. chosen
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
Messier object
ⓘ
deep-sky object ⓘ globular star cluster ⓘ |
| absoluteMagnitudeV | −8.2 ⓘ |
| age |
about 13 billion years
ⓘ
on the order of the age of the Universe ⓘ |
| alsoKnownAs |
M92
NERFINISHED
ⓘ
NGC 6341 NERFINISHED ⓘ |
| angularSize | 14 arcminutes ⓘ |
| apparentMagnitudeV | 6.3 ⓘ |
| belongsToCatalogue |
Messier Catalogue
NERFINISHED
ⓘ
New General Catalogue NERFINISHED ⓘ |
| cataloguedBy | Charles Messier NERFINISHED ⓘ |
| catalogueEntryDate | 1781 ⓘ |
| concentrationClass | Class IV globular cluster ⓘ |
| contains | RR Lyrae variable stars ⓘ |
| coreRadius | about 1.2 light-years ⓘ |
| declination | +43° 08′ 11″ ⓘ |
| discoveredBy | Johann Elert Bode NERFINISHED ⓘ |
| discoveryDate | 1777 ⓘ |
| distanceFromEarth |
about 26,700 light-years
ⓘ
about 8.2 kiloparsecs ⓘ |
| epoch | J2000 ⓘ |
| galacticLatitude | +34.9° ⓘ |
| galacticLongitude | 68.3° ⓘ |
| halfLightRadius | about 5.5 light-years ⓘ |
| heliocentricRadialVelocity | about −120 km/s ⓘ |
| horizontalBranchMorphology | blue horizontal branch ⓘ |
| locatedIn |
Galactic halo
NERFINISHED
ⓘ
Milky Way ⓘ |
| locatedInConstellation | Hercules NERFINISHED ⓘ |
| mass | about 3×10^5 solar masses ⓘ |
| metallicityClass | very metal-poor ⓘ |
| metallicityFeH | about −2.3 ⓘ |
| notableFeature |
high central stellar density
ⓘ
one of the oldest known globular clusters in the Milky Way ⓘ very low metallicity ⓘ |
| observedIn |
X-ray wavelengths
ⓘ
infrared wavelengths ⓘ optical wavelengths ⓘ |
| orbitalType | highly eccentric orbit around the Milky Way ⓘ |
| rightAscension | 17h 17m 07.3s ⓘ |
| stellarPopulation | Population II NERFINISHED ⓘ |
| surfaceBrightness | high ⓘ |
| tidalRadius | about 54 light-years ⓘ |
| visibility |
marginally visible to the naked eye under very dark skies
ⓘ
visible in small telescopes ⓘ |
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: Messier 92 Description of subject: Messier 92 is a bright, ancient globular star cluster located in the constellation Hercules, notable for its high stellar density and visibility even in small telescopes.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.