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 (3)

Label Occurrences
Type Ia supernovae canonical 12
SNe Ia 1
Type 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 SNe Ia ⓘ
linked to: Type Ia supernovae

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 (14)

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 → SNe Ia ⓘ
linked to: Type Ia supernovae
Adam G. Riess → researchInterest → Type Ia supernovae ⓘ
M100 → supernovaTypeObserved → Type Ia ⓘ
linked to: Type Ia supernovae
Etherington reciprocity theorem → testedUsing → Type Ia supernovae ⓘ
Gustav A. Tammann → researchInterest → Type Ia supernovae ⓘ
José Maza → researchInterest → Type Ia supernovae ⓘ
subject linked to: Jose Maza
Saurabh Jha → studies → Type Ia supernovae ⓘ
Carl Pennypacker → researchInterest → Type Ia supernovae ⓘ
Peter M. Garnavich → researchInterest → Type Ia supernovae ⓘ
Christopher Stubbs → researchArea → Type Ia supernovae ⓘ
Alex Kim → studies → Type Ia supernovae ⓘ
Robert P. Kirshner → researchInterest → Type Ia supernovae ⓘ