UGC 426
E459105
UGC 426 is a dwarf elliptical satellite galaxy of the Andromeda Galaxy, more commonly known as Messier 110 (M110).
All labels observed (1)
| Label | Occurrences |
|---|---|
| UGC 426 canonical | 2 |
How this entity was disambiguated
This entity first appeared as the object of triple T4618559 — 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: UGC 426 Context triple: [M110, catalogueDesignation, UGC 426]
-
A.
UGC 64
UGC 64 is a faint dwarf irregular galaxy located in the Local Group, commonly known as Andromeda IV and lying near the Andromeda Galaxy in the constellation Andromeda.
-
B.
UGC 4483
UGC 4483 is a faint dwarf irregular galaxy located in the constellation Camelopardalis and is a member of the nearby M81 Group of galaxies.
-
C.
UGC 9240
UGC 9240 is a dwarf irregular galaxy located in the constellation Ursa Major and is a member of the nearby M81 Group of galaxies.
-
D.
UGC 9992
UGC 9992 is a relatively faint, dwarf galaxy that is a member of the nearby M81 Group in the constellation Ursa Major.
-
E.
UGC 4305
UGC 4305 is a dwarf irregular galaxy located in the nearby M81 Group in the constellation Ursa Major.
- 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: UGC 426 Target entity description: UGC 426 is a dwarf elliptical satellite galaxy of the Andromeda Galaxy, more commonly known as Messier 110 (M110).
-
A.
UGC 64
UGC 64 is a faint dwarf irregular galaxy located in the Local Group, commonly known as Andromeda IV and lying near the Andromeda Galaxy in the constellation Andromeda.
-
B.
UGC 4483
UGC 4483 is a faint dwarf irregular galaxy located in the constellation Camelopardalis and is a member of the nearby M81 Group of galaxies.
-
C.
UGC 9240
UGC 9240 is a dwarf irregular galaxy located in the constellation Ursa Major and is a member of the nearby M81 Group of galaxies.
-
D.
UGC 9992
UGC 9992 is a relatively faint, dwarf galaxy that is a member of the nearby M81 Group in the constellation Ursa Major.
-
E.
UGC 4305
UGC 4305 is a dwarf irregular galaxy located in the nearby M81 Group in the constellation Ursa Major.
- F. None of above. chosen
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical object
ⓘ
dwarf elliptical galaxy ⓘ satellite galaxy ⓘ |
| absoluteMagnitudeV | approximately -16.5 ⓘ |
| alternateName |
M110
ⓘ
Messier 110 NERFINISHED ⓘ NGC 205 NERFINISHED ⓘ |
| angularSize | approximately 21 arcminutes by 11 arcminutes ⓘ |
| apparentMagnitudeV | approximately 8.9 ⓘ |
| bestSeenIn | small telescopes ⓘ |
| catalog |
Messier catalogue
NERFINISHED
ⓘ
NGC NERFINISHED ⓘ PGC NERFINISHED ⓘ UGC NERFINISHED ⓘ |
| contains |
dust lanes
ⓘ
gas ⓘ globular clusters ⓘ |
| declination | +41° 41′ 07″ ⓘ |
| discoveredBy | Giovanni Battista Hodierna NERFINISHED ⓘ |
| discoveryYear | before 1654 ⓘ |
| distanceFromEarth |
approximately 0.83 megaparsecs
ⓘ
approximately 2.7 million light-years ⓘ |
| hasEnvironment | dense tidal field of Andromeda Galaxy ⓘ |
| hasMessierNumber | M110 NERFINISHED ⓘ |
| hasNGCNumber | NGC 205 NERFINISHED ⓘ |
| hasNucleus | central stellar concentration ⓘ |
| hasPGCNumber | PGC 2557 NERFINISHED ⓘ |
| hasStarFormation | low current star formation rate ⓘ |
| hasStellarPopulation |
intermediate-age stars
ⓘ
old stars ⓘ |
| isBrighterThan | most dwarf spheroidal satellites of Andromeda ⓘ |
| isCompanionOf | Andromeda Galaxy NERFINISHED ⓘ |
| isOneOf | brightest dwarf companions of Andromeda Galaxy ⓘ |
| isVisibleFrom | Northern Hemisphere NERFINISHED ⓘ |
| locatedIn | constellation Andromeda NERFINISHED ⓘ |
| mass | on the order of 10^9 solar masses ⓘ |
| memberOf | Local Group NERFINISHED ⓘ |
| morphologicalType | dE5 ⓘ |
| orbitsWithin | Andromeda subgroup of the Local Group NERFINISHED ⓘ |
| radialVelocity | approximately -241 km/s ⓘ |
| recoveredBy | Charles Messier NERFINISHED ⓘ |
| recoveryYear | 1773 ⓘ |
| redshift | approximately -0.000804 ⓘ |
| rightAscension | 00h 40m 22s ⓘ |
| satelliteOf |
Andromeda Galaxy
NERFINISHED
ⓘ
Messier 31 NERFINISHED ⓘ |
| showsEvidenceOf | tidal interaction with Andromeda Galaxy ⓘ |
| surfaceBrightness | low ⓘ |
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: UGC 426 Description of subject: UGC 426 is a dwarf elliptical satellite galaxy of the Andromeda Galaxy, more commonly known as Messier 110 (M110).
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.