Leavitt law

E571548

The Leavitt law is the period–luminosity relation for Cepheid variable stars that enables astronomers to measure cosmic distances and determine the scale of the universe.

All labels observed (2)

Label Occurrences
Leavitt law canonical 1
Leavitt’s law 1

How this entity was disambiguated

Statements (45)

Predicate Object
instanceOf astronomical relation ⓘ
distance indicator ⓘ
period–luminosity relation ⓘ
accuracyImprovedBy corrections for reddening and extinction ⓘ
observations in infrared bands ⓘ
appliesTo Cepheid variable star ⓘ
Classical Cepheid variable ⓘ
Type I Cepheid ⓘ
linked to: Cepheid variables
assumes Cepheids in the same galaxy are at nearly the same distance ⓘ
calibratedUsing Gaia mission parallaxes ⓘ
Hubble Space Telescope observations ⓘ
trigonometric parallax of nearby Cepheids ⓘ
category Observational cosmology ⓘ
linked to: Physical Cosmology

Stellar astronomy ⓘ
describesRelationBetween intrinsic luminosity of Cepheid variables ⓘ
pulsation period of Cepheid variables ⓘ
enables calibration of the cosmic distance ladder ⓘ
determination of extragalactic distances ⓘ
measurement of cosmic distances ⓘ
hasAlternativeName period–luminosity relation ⓘ
hasDiscoverer Henrietta Swan Leavitt ⓘ
hasKeyParameter slope of the period–luminosity relation ⓘ
zero point of the period–luminosity relation ⓘ
hasLimitation metallicity dependence of the relation ⓘ
scatter due to interstellar extinction ⓘ
hasVariant infrared period–luminosity relation ⓘ
period–luminosity–color relation ⓘ
historicalSignificance provided first reliable method to measure distances to external galaxies ⓘ
implies longer-period Cepheids are more luminous ⓘ
influencedWorkOf Edwin Hubble ⓘ
isPartOf cosmic distance ladder ⓘ
mathematicallyExpressedAs linear relation between absolute magnitude and logarithm of period ⓘ
namedAfter Henrietta Swan Leavitt ⓘ
playsRoleIn determination of the Hubble constant ⓘ
testing cosmological models ⓘ
relatedTo Hubble–Lemaître law ⓘ
standard candle concept ⓘ
requiresCalibrationBy independent distance measurements ⓘ
subjectOf cosmological distance scale studies ⓘ
usedFor calibrating Type Ia supernova distances ⓘ
determining the scale of the universe ⓘ
measuring distances to nearby galaxies ⓘ
measuring distances within the Milky Way ⓘ
wasDiscoveredIn early 20th century ⓘ
wasFirstFormulatedFromObservationsOf Cepheid variables in the Small Magellanic Cloud ⓘ

How these facts were elicited

Referenced by (2)

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