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gptkbp:instance_of
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gptkb:star
|
|
gptkbp:available_colors
|
red and orange
|
|
gptkbp:can_be_found_in
|
gptkb:the_Milky_Way_Galaxy
globular clusters
open clusters
|
|
gptkbp:can_be_part_of_a_binary_system_with
|
another star
|
|
gptkbp:can_create
|
planetary nebulae
|
|
gptkbp:can_eventually_lead_to
|
supernova or white dwarf formation
|
|
gptkbp:can_fuse
|
helium into carbon
|
|
gptkbp:can_have_a_complex_internal_structure_with
|
multiple layers
|
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gptkbp:can_have_a_mass_loss_rate_of
|
10^-7 to 10^-5 solar masses per year
|
|
gptkbp:can_have_a_surface_temperature_of
|
around 2,200 to 4,000 K
|
|
gptkbp:can_have_a_variable_brightness_due_to
|
pulsation modes
|
|
gptkbp:can_vary_in_size_from
|
10 to 100 times the radius of the Sun
|
|
gptkbp:created
|
gptkb:Red_Supergiant
|
|
gptkbp:exhibits
|
pulsations
|
|
gptkbp:has_a_core_that_is_primarily
|
helium
|
|
gptkbp:has_a_focus_on
|
stellar evolution research
|
|
gptkbp:has_luminosity
|
up to 1,000 times that of the Sun
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Red Giant
|
|
gptkbp:is_a_common_phase_for_stars_like
|
gptkb:Betelgeuse
|
|
gptkbp:is_a_key_phase_in_understanding
|
stellar nucleosynthesis
|
|
gptkbp:is_a_phase_that_can_last_for
|
a few million years
|
|
gptkbp:is_a_phase_that_can_lead_to
|
the creation of new stars from ejected material
the formation of red giant branches
|
|
gptkbp:is_a_phase_that_follows
|
the hydrogen burning phase
|
|
gptkbp:is_a_significant_phase_in_the_life_of
|
stars like the Sun
|
|
gptkbp:is_associated_with
|
the loss of mass
|
|
gptkbp:is_characterized_by
|
expansion and cooling
a significant increase in radius
|
|
gptkbp:is_essential_for
|
galactic chemical evolution
|
|
gptkbp:is_observed_in
|
gptkb:the_Andromeda_Galaxy
various galaxies
|
|
gptkbp:is_often_associated_with
|
the late stages of stellar evolution
|
|
gptkbp:is_often_depicted_as
|
astronomical illustrations
|
|
gptkbp:is_often_referenced_in
|
stellar classification.
|
|
gptkbp:is_often_seen_in
|
supergiants
the Hertzsprung-Russell diagram
the later stages of stellar evolution
|
|
gptkbp:is_often_studied_using
|
gptkb:spectroscopy
|
|
gptkbp:is_often_the_end_stage_for
|
low to intermediate mass stars
|
|
gptkbp:is_part_of
|
stellar lifecycle
|
|
gptkbp:is_popular_for
|
heavy element production
|
|
gptkbp:is_studied_in
|
astrophysics
stellar models
|
|
gptkbp:is_surrounded_by
|
a shell of gas and dust
|
|
gptkbp:occurs_in
|
main sequence phase
|
|
gptkbp:scientific_classification
|
different subtypes
|
|
gptkbp:type_of
|
stellar evolution stage
|
|
gptkbp:bfsParent
|
gptkb:Dwarves
|
|
gptkbp:bfsLayer
|
4
|