Statements (47)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
Star
|
| gptkbp:category |
Late-stage stellar evolution
|
| gptkbp:energyEfficiency |
Sun
|
| gptkbp:examples |
gptkb:Betelgeuse
Antares VY Canis Majoris |
| gptkbp:hasColor |
Red
|
| gptkbp:hasMission |
A few million years
|
| gptkbp:hasRelatedPatent |
M-type
|
| gptkbp:hasSibling |
Very large
|
| gptkbp:hasTechnology |
3000 to 4500 K
|
| https://www.w3.org/2000/01/rdf-schema#label |
Red Supergiant
|
| gptkbp:isA |
Stellar classification
|
| gptkbp:isAccessibleBy |
Yes
Black holes Neutron stars White dwarfs |
| gptkbp:isAssociatedWith |
gptkb:Supernova_remnants
Star formation regions |
| gptkbp:isAttendedBy |
Mass loss due to stellar winds
|
| gptkbp:isCharacterizedBy |
High mass loss rate
|
| gptkbp:isEngagedIn |
Blue supergiants
|
| gptkbp:isExploredIn |
Astrobiology
|
| gptkbp:isFoundIn |
Galaxies
|
| gptkbp:isImportantFor |
Cosmology
|
| gptkbp:isInvolvedIn |
Chemical_enrichment_of_the_galaxy
|
| gptkbp:isKnownFor |
Variable brightness
|
| gptkbp:isLocatedIn |
The Milky Way
|
| gptkbp:isMonitoredBy |
gptkb:Telescopes
|
| gptkbp:isPartOf |
Stellar populations
Stellar evolution The Hertzsprung-Russell diagram Open clusters |
| gptkbp:isRelatedTo |
High-mass stars
Red giants |
| gptkbp:isServedBy |
Infrared_wavelengths
|
| gptkbp:isStudiedIn |
Astrophysics
Nucleosynthesis |
| gptkbp:isSubjectTo |
Astronomical research
|
| gptkbp:isUsedFor |
gptkb:Supernova
|
| gptkbp:isUsedIn |
Main sequence stars
Distance measurement in astronomy The constellation Puppis The_constellation_Carina The_constellation_Orion The_constellation_Scorpius |
| gptkbp:resolution |
1000 to 100000 times that of the Sun
|