Type Ia supernova explosions
GPTKB entity
Statements (61)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:Supernova
|
gptkbp:affects |
galactic dynamics
|
gptkbp:are_part_of |
stellar evolution
the life cycle of stars |
gptkbp:can_be_used_to |
measure the expansion of the universe
test theories of gravity calibrate distance measurements |
gptkbp:can_cause |
shock waves
|
gptkbp:can_detect |
telescopes
ground-based observatories |
gptkbp:can_involve |
gptkb:Dwarves
|
gptkbp:can_lead_to |
gptkb:supernova_remnants
chemical enrichment of the universe new star formation the formation of neutron stars. galactic chemical enrichment |
gptkbp:can_provide |
insights into dark matter
information about stellar populations |
gptkbp:cause |
thermonuclear explosion
|
gptkbp:emissions_standard |
gamma rays
|
gptkbp:have |
light curves
|
https://www.w3.org/2000/01/rdf-schema#label |
Type Ia supernova explosions
|
gptkbp:influence |
galaxy formation
|
gptkbp:is_associated_with |
Type Ia supernova progenitors
Type Ia supernova light curves |
gptkbp:is_characterized_by |
consistent peak luminosity
|
gptkbp:is_considered |
standard candles
|
gptkbp:is_described_as |
binary star evolution theory
carbon-oxygen white dwarf model thermonuclear runaway process |
gptkbp:is_essential_for |
understanding dark energy
understanding stellar evolution understanding the universe's expansion rate type Ia supernova cosmology |
gptkbp:is_monitored_by |
gptkb:astronomy
|
gptkbp:is_noted_for |
their uniformity in brightness
|
gptkbp:is_observed_in |
space telescopes
distant galaxies various galaxies |
gptkbp:is_recognized_by |
spectral lines
|
gptkbp:is_related_to |
gptkb:Type_II_supernovae
stellar mass loss |
gptkbp:is_studied_for |
their role in nucleosynthesis
their impact on interstellar medium their role in cosmic evolution |
gptkbp:is_studied_in |
gptkb:spectroscopy
astrophysics |
gptkbp:is_targeted_at |
accretion of mass
merger of binary white dwarfs |
gptkbp:is_used_for |
cosmological distance measurement
|
gptkbp:is_used_in |
distance ladder methods
|
gptkbp:key |
gptkb:cosmology
modern cosmology understanding cosmic acceleration |
gptkbp:occur_when |
white dwarf reaches Chandrasekhar limit
|
gptkbp:occurs_in |
binary star systems
|
gptkbp:produces |
gptkb:Iron_Age
|
gptkbp:resulted_in |
brightness increase
|
gptkbp:scientific_classification |
thermonuclear supernovae
|
gptkbp:bfsParent |
gptkb:Type_Ia_supernova_remnants
|
gptkbp:bfsLayer |
7
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