BM Scorpii
E1390386
UNEXPLORED
BM Scorpii is a luminous red supergiant star in the constellation Scorpius that serves as the visually dominant member of the Butterfly Cluster (Messier 6).
All labels observed (1)
| Label | Occurrences |
|---|---|
| BM Scorpii canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T19686274 — 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.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: BM Scorpii Context triple: [Butterfly Cluster, brightestStar, BM Scorpii]
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A.
β Lyrae
β Lyrae is a well-known eclipsing binary star system in the constellation Lyra, notable for its continuously varying brightness caused by mass transfer between its closely orbiting stellar components.
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B.
GQ Lupi
GQ Lupi is a young T Tauri star in the constellation Lupus, notable for hosting a directly imaged substellar companion.
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C.
WZ Scuti
WZ Scuti is a variable star located in the constellation Scutum, known for its changes in brightness over time.
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D.
Sigma Sagittarii
Sigma Sagittarii is a bright blue-white giant star in the constellation Sagittarius, marking one of the prominent points of the Teapot asterism.
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E.
Gamma Microscopii
Gamma Microscopii is a yellow giant star in the southern constellation Microscopium, notable as its most luminous visible member.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: BM Scorpii Target entity description: BM Scorpii is a luminous red supergiant star in the constellation Scorpius that serves as the visually dominant member of the Butterfly Cluster (Messier 6).
-
A.
β Lyrae
β Lyrae is a well-known eclipsing binary star system in the constellation Lyra, notable for its continuously varying brightness caused by mass transfer between its closely orbiting stellar components.
-
B.
GQ Lupi
GQ Lupi is a young T Tauri star in the constellation Lupus, notable for hosting a directly imaged substellar companion.
-
C.
WZ Scuti
WZ Scuti is a variable star located in the constellation Scutum, known for its changes in brightness over time.
-
D.
Sigma Sagittarii
Sigma Sagittarii is a bright blue-white giant star in the constellation Sagittarius, marking one of the prominent points of the Teapot asterism.
-
E.
Gamma Microscopii
Gamma Microscopii is a yellow giant star in the southern constellation Microscopium, notable as its most luminous visible member.
- F. None of above. chosen
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.