Mira

E591819

Mira is a famous red giant variable star in the constellation Cetus, known for its dramatic changes in brightness over time.

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Statements (48)

Predicate Object
instanceOf Mira variable
long-period variable star
pulsating variable star
red giant star
star
alsoKnownAs Omicron Ceti NERFINISHED
ο Ceti NERFINISHED
apparentMagnitudeRange about 2.0 to 10.1
catalogDesignation HD 14386 NERFINISHED
HIP 10732 NERFINISHED
HR 681 NERFINISHED
color red
constellation Cetus NERFINISHED
coreComposition carbon-oxygen core
declination −02° 59′
discoveredAsVariableBy David Fabricius NERFINISHED
discoveryOfVariabilityYear 1596
distanceFromEarth about 300 light-years
about 92 parsecs
effectiveTemperature about 3000 K
evolutionaryStage asymptotic giant branch star
futureEvolution will become a white dwarf
hasCompanion Mira B NERFINISHED
hasFeature comet-like tail
extended gaseous envelope
heliocentricRadialVelocity about 63 km/s
isPrototypeOf Mira variables NERFINISHED
locatedIn Milky Way
Orion Arm NERFINISHED
luminosity about 8000 times solar luminosity
mass about 1.2 solar masses
massLoss strong stellar wind
MiraBInstanceOf white dwarf star
namedBy Johannes Hevelius NERFINISHED
nameLanguage Latin
nameMeaning wonderful
observedInUltravioletBy GALEX NERFINISHED
properMotion high
radius about 300 solar radii
rightAscension 02h 19m
spectralType M7IIIe
systemType binary star system
tailLength about 13 light-years
variabilityCause radial pulsations
variabilityPeriod about 332 days
variableType Mira-type variable
visibleToNakedEyeAtMaximum true
visibleToNakedEyeAtMinimum false

Referenced by (3)

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