Type Ia supernovae

E374518

Type Ia supernovae are a class of stellar explosions with nearly uniform intrinsic brightness, making them powerful standard candles for measuring cosmic distances and probing the expansion history of the universe.

All labels observed (2)

Label Occurrences
Type Ia supernovae canonical 3
SNe Ia 1

How this entity was disambiguated

Statements (52)

Predicate Object
instanceOf astronomical phenomenon
standard candle
supernova type
associatedNobelPrize 2011 Nobel Prize in Physics
cosmologicalUse constraining dark energy
constructing the cosmic distance ladder
measuring cosmological parameters
measuring extragalactic distances
measuring the Hubble constant
probing the expansion history of the universe
discoveryContribution evidence for accelerating expansion of the universe
evidence for dark energy
distanceIndicatorRole primary distance indicators for cosmology
distanceRange observable to redshifts greater than 1
energySource fusion of carbon and oxygen
radioactive decay of cobalt-56
radioactive decay of nickel-56
explosionMechanism thermonuclear runaway
hasAlternativeName Type Ia supernovae
surface form: SNe Ia

Type I-a supernovae
hasSubclass 1991T-like Type Ia supernovae
1991bg-like Type Ia supernovae
normal Type Ia supernovae
overluminous Type Ia supernovae
underluminous Type Ia supernovae
hostEnvironment elliptical galaxies
lenticular galaxies
old stellar populations
spiral galaxies
young stellar populations
intrinsicBrightness nearly uniform
lightCurveFeature correlation between decline rate and peak luminosity
secondary maximum in near-infrared bands
observationalBand near-infrared wavelengths
optical wavelengths
openQuestion details of explosion mechanism
exact nature of progenitor systems
progenitorScenario double-degenerate scenario
single-degenerate scenario
progenitorSystem binary star system
spectralFeature lack of helium lines
lack of hydrogen lines
strong silicon II absorption line near 6150 Å
standardizationMethod Phillips relation
typicalEjectedMass on the order of one solar mass
typicalExplosionEnergy about 10^51 ergs
typicalHostStellarPopulationAge often several billion years
typicalNickelMass about 0.4–0.8 solar masses of nickel-56
typicalPeakAbsoluteMagnitude about −19.3 in B band
typicalProgenitor carbon–oxygen white dwarf
typicalRiseTime about 17–20 days to B-band maximum
usedAs standardizable candles

How these facts were elicited

Referenced by (4)

Full triples — surface form annotated when it differs from this entity's canonical label.

Dark Energy Survey cosmologicalProbe Type Ia supernovae
High-z Supernova Search Team uses Type Ia supernovae
Type Ia supernovae hasAlternativeName Type Ia supernovae
this entity surface form: SNe Ia
Adam G. Riess researchInterest Type Ia supernovae