R Scuti
E483243
R Scuti is a luminous, pulsating yellow supergiant star in the constellation Scutum, known as one of the brightest and most studied RV Tauri variable stars.
All labels observed (1)
| Label | Occurrences |
|---|---|
| R Scuti canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T4943664 — 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: R Scuti Context triple: [Scutum, contains, R Scuti]
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A.
UY Scuti
UY Scuti is a 2021 studio album by Nigerian rapper and singer Olamide that blends Afrobeats, hip-hop, and pop influences.
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B.
UY Scuti
UY Scuti is an extremely large red supergiant star, among the biggest known in the Milky Way, located in the constellation Scutum.
-
C.
Beta Scuti
Beta Scuti is a prominent giant star in the constellation Scutum, notable as one of its brightest members.
-
D.
B Cassiopeiae
B Cassiopeiae is the historic supernova observed in 1572 in the constellation Cassiopeia, famously studied by Tycho Brahe and crucial to early modern astronomy.
-
E.
Betelgeuse
Betelgeuse is a massive red supergiant star in the constellation Orion, notable for its brightness and status as a likely future supernova.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: R Scuti Target entity description: R Scuti is a luminous, pulsating yellow supergiant star in the constellation Scutum, known as one of the brightest and most studied RV Tauri variable stars.
-
A.
UY Scuti
UY Scuti is an extremely large red supergiant star, among the biggest known in the Milky Way, located in the constellation Scutum.
-
B.
UY Scuti
UY Scuti is a 2021 studio album by Nigerian rapper and singer Olamide that blends Afrobeats, hip-hop, and pop influences.
-
C.
Beta Scuti
Beta Scuti is a prominent giant star in the constellation Scutum, notable as one of its brightest members.
-
D.
B Cassiopeiae
B Cassiopeiae is the historic supernova observed in 1572 in the constellation Cassiopeia, famously studied by Tycho Brahe and crucial to early modern astronomy.
-
E.
Betelgeuse
Betelgeuse is a massive red supergiant star in the constellation Orion, notable for its brightness and status as a likely future supernova.
- F. None of above. chosen
Statements (49)
| Predicate | Object |
|---|---|
| instanceOf |
RV Tauri variable star
ⓘ
pulsating variable star ⓘ star ⓘ yellow supergiant ⓘ |
| apparentMagnitudeV |
4.5
ⓘ
8.9 ⓘ |
| belongsToConstellation | Scutum NERFINISHED ⓘ |
| brightnessVariationType | semiregular deep and shallow minima ⓘ |
| catalogIdentifier |
AAVSO 1829-05
NERFINISHED
ⓘ
BD−05° 4729 NERFINISHED ⓘ HD 173819 NERFINISHED ⓘ HIP 92175 NERFINISHED ⓘ HR 7065 NERFINISHED ⓘ SAO 142996 NERFINISHED ⓘ |
| colorIndex | yellow to orange ⓘ |
| constellation | Scutum NERFINISHED ⓘ |
| declination | −05° 42′ (approximate) ⓘ |
| discoverer | Edward Pigott NERFINISHED ⓘ |
| discoveryYear | 1795 ⓘ |
| distanceFromEarth_ly | approximately 1400 ⓘ |
| distanceFromEarth_pc | approximately 430 ⓘ |
| evolutionaryStage |
post-AGB object
ⓘ
post-asymptotic giant branch star ⓘ |
| galacticComponent | thick disk or halo population ⓘ |
| hasCircumstellarMaterial | yes ⓘ |
| hemisphere | celestial equator region ⓘ |
| lightCurveCharacteristic |
alternating deep and shallow minima
ⓘ
irregular cycle lengths ⓘ |
| locationInGalaxy | Milky Way NERFINISHED ⓘ |
| luminosityComparedToSun | several thousand times solar luminosity ⓘ |
| massLoss | experiences stellar wind and mass loss ⓘ |
| meanPulsationPeriod_days | about 70 ⓘ |
| metallicity | low metallicity compared to Sun ⓘ |
| notableFor |
extensively observed by amateur and professional astronomers
ⓘ
one of the brightest RV Tauri stars in the sky ⓘ prototype-like RV Tauri variability ⓘ |
| observability |
requires binoculars or small telescope at minimum
ⓘ
visible to naked eye at maximum ⓘ |
| periodRange_days | about 60 to 150 ⓘ |
| population | Population II star ⓘ |
| pulsationMechanism | radial pulsations ⓘ |
| rightAscension | 18h 47m (approximate) ⓘ |
| spectralClassRange | G–K supergiant ⓘ |
| spectralType |
G0Ib
ⓘ
K2Ib ⓘ |
| usedFor |
calibration of RV Tauri period–luminosity relations
ⓘ
studies of late stellar evolution ⓘ |
| variableStarDesignation | R Sct NERFINISHED ⓘ |
| variableStarType | RV Tauri NERFINISHED ⓘ |
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: R Scuti Description of subject: R Scuti is a luminous, pulsating yellow supergiant star in the constellation Scutum, known as one of the brightest and most studied RV Tauri variable stars.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.