Cepheid variables

E581535

Cepheid variables are pulsating stars whose regular brightness variations make them crucial standard candles for measuring cosmic distances and mapping galactic structure.

All labels observed (6)

Label Occurrences
Cepheid variable stars 2
Cepheid variables canonical 2
Cepheids 1

How this entity was disambiguated

Statements (51)

Predicate Object
instanceOf class of variable stars ⓘ
standard candles ⓘ
distinguishedBy correlation between pulsation period and intrinsic luminosity ⓘ
regular, predictable light curves ⓘ
exhibits periodic brightness variations ⓘ
radial pulsations ⓘ
hasAlternativeName Cepheid variable stars ⓘ
Cepheids ⓘ
linked to: Cepheid variables
hasCauseOfPulsation kappa mechanism ⓘ
opacity changes in partial ionization zones ⓘ
hasCauseOfVariability pulsation of stellar envelope ⓘ
hasDiscovery period–luminosity relation discovered by Henrietta Swan Leavitt ⓘ
hasKeyProperty period–color relation ⓘ
period–luminosity relation ⓘ
period–radius relation ⓘ
hasLightCurveShape sawtooth-like in many cases ⓘ
hasLuminosityClass I (supergiant) ⓘ
hasPhaseRelation maximum brightness occurs near minimum radius ⓘ
hasSpectralTypeRange F-type supergiants ⓘ
G-type supergiants ⓘ
hasSubClass Anomalous Cepheids ⓘ
Classical Cepheids ⓘ
linked to: Cepheid variables

Type II Cepheids ⓘ
linked to: Cepheid variables
hasTypicalAbsoluteMagnitudeRange about −2 to −6 in V band ⓘ
hasTypicalAgeRange tens to hundreds of millions of years (Classical Cepheids) ⓘ
hasTypicalAmplitudeRange about 0.1 to 2 magnitudes in visible light ⓘ
hasTypicalMassRange about 3 to 15 solar masses (Classical Cepheids) ⓘ
hasTypicalPeriodRange 1 to 100 days ⓘ
hasTypicalTemperatureVariation several hundred to a few thousand Kelvin over a cycle ⓘ
importantFor establishing the first rung of the cosmic distance ladder ⓘ
modeledBy stellar pulsation theory ⓘ
namedAfter Delta Cephei ⓘ
linked to: δ Cephei
observedIn Large Magellanic Cloud ⓘ
Milky Way ⓘ
Small Magellanic Cloud ⓘ
many nearby galaxies ⓘ
periodLuminosityRelationPublishedIn 1912 ⓘ
requiresForAccurateUse corrections for interstellar extinction ⓘ
metallicity corrections ⓘ
traces older stellar populations (Type II Cepheids) ⓘ
young stellar populations (Classical Cepheids) ⓘ
typicallyFoundIn irregular galaxies ⓘ
spiral galaxies ⓘ
usedAs primary distance indicators ⓘ
usedFor calibrating Type Ia supernova luminosities ⓘ
calibrating the extragalactic distance scale ⓘ
determining the Hubble constant ⓘ
mapping galactic structure ⓘ
measuring distances to nearby galaxies ⓘ
measuring distances within the Milky Way ⓘ
tracing spiral arms in disk galaxies ⓘ

How these facts were elicited

Referenced by (8)

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

Galactic thin disk → isTracedBy → Cepheid variables ⓘ
Leavitt law → appliesTo → Type I Cepheid ⓘ
linked to: Cepheid variables
Cepheid variables → hasAlternativeName → Cepheids ⓘ
linked to: Cepheid variables
Cepheid variables → hasSubClass → Classical Cepheids ⓘ
linked to: Cepheid variables
Cepheid variables → hasSubClass → Type II Cepheids ⓘ
linked to: Cepheid variables
VISTA Variables in the Via Lactea → detects → Cepheid variables ⓘ
Shapley–Curtis debate → usedEvidence → Cepheid variable stars ⓘ
linked to: Cepheid variables
Recalibration of the Hubble constant → usesMethod → Cepheid variable stars ⓘ
linked to: Cepheid variables