Statements (45)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:Ruchbah
|
| gptkbp:average_temperature |
< 3,500 K
|
| gptkbp:can_create |
gptkb:theorem
|
| gptkbp:color |
gptkb:theorem
|
| gptkbp:exhibits |
variable brightness
pulsations |
| gptkbp:has_luminosity |
up to 10,000 times that of the Sun
|
| gptkbp:has_spectral_type |
gptkb:M
|
| https://www.w3.org/2000/01/rdf-schema#label |
M-type giant star
|
| gptkbp:is_associated_with |
stellar winds
carbon stars red dwarf stars |
| gptkbp:is_atype_of |
gptkb:star
|
| gptkbp:is_characterized_by |
cool surface temperature
strong molecular bands in spectrum |
| gptkbp:is_essential_for |
understanding stellar nucleosynthesis
|
| gptkbp:is_found_in |
gptkb:the_Milky_Way_galaxy
star clusters |
| gptkbp:is_known_for |
high metallicity
its red color produce heavy elements |
| gptkbp:is_observed_in |
infrared wavelengths
various galaxies |
| gptkbp:is_often_compared_to |
K-type giant stars
|
| gptkbp:is_often_depicted_as |
the late stages of stellar evolution
|
| gptkbp:is_often_used_in |
the universe
G-type stars |
| gptkbp:is_part_of |
stellar populations
the Hertzsprung-Russell diagram the Milky Way's stellar population. the stellar lifecycle the cosmic chemical evolution |
| gptkbp:is_studied_in |
astrophysics
mass loss rates |
| gptkbp:is_used_in |
stellar evolution studies
|
| gptkbp:is_used_to |
calibrate distance scales
|
| gptkbp:lifespan |
up to several billion years
|
| gptkbp:lighting |
main-sequence stars
|
| gptkbp:located_in |
the lower right of the Hertzsprung-Russell diagram
|
| gptkbp:mass |
0.8 to 8 solar masses
|
| gptkbp:origin |
gptkb:nebula
|
| gptkbp:scientific_classification |
supergiant or giant
|
| gptkbp:size |
main-sequence stars
|