U Sagittarii

E459055

U Sagittarii is a classical Cepheid variable star in the constellation Sagittarius, notable for its periodic brightness variations used to measure cosmic distances.

All labels observed (1)

Label Occurrences
U Sagittarii canonical 4

How this entity was disambiguated

Statements (30)

Predicate Object
instanceOf Cepheid variable ⓘ
classical Cepheid variable star ⓘ
variable star ⓘ
apparentMagnitudeBand visual ⓘ
belongsTo Milky Way ⓘ
celestialCategory star ⓘ
constellation Sagittarius ⓘ
declinationCoordinateSystem ICRS ⓘ
distanceIndicator period–luminosity relation ⓘ
evolutionaryStage post-main-sequence star ⓘ
hasDesignation U Sag ⓘ
U Sgr ⓘ
hasPeriodicBrightnessVariations true ⓘ
hemisphere southern celestial hemisphere ⓘ
isLuminous true ⓘ
isStandardCandle true ⓘ
lightCurveType Cepheid-type ⓘ
locatedIn constellation Sagittarius ⓘ
observedBy ground-based telescopes ⓘ
space-based observatories ⓘ
populationType Population I star ⓘ
pulsationMode fundamental mode ⓘ
rightAscensionCoordinateSystem ICRS ⓘ
spectralType F-type supergiant ⓘ
usedIn studies of period–luminosity relation ⓘ
studies of stellar pulsation ⓘ
uses cosmic distance scale calibration ⓘ
distance measurement in astronomy ⓘ
variabilityMechanism radial pulsation ⓘ
variableType Classical Cepheid ⓘ

How these facts were elicited

Referenced by (4)

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

Messier 25 → containsVariableStar → U Sagittarii ⓘ
M25 → containsVariableStar → U Sagittarii ⓘ
M25 → containsCepheidVariable → U Sagittarii ⓘ