Kappa Orionis

E572550

Kappa Orionis, traditionally known as Saiph, is a bright blue supergiant star marking one of the knees of the constellation Orion.

Jump to: Surface forms Statements Referenced by

Observed surface forms (1)

Surface form Occurrences
κ Orionis 1

Statements (48)

Predicate Object
instanceOf star
supergiant star
absoluteMagnitudeV −6.0
age on the order of a few million years
apparentMagnitudeV 2.06
bayerDesignation κ Orionis NERFINISHED
belongsTo Milky Way galaxy NERFINISHED
catalogDesignation BD−09 1235 NERFINISHED
GC 7284 NERFINISHED
SAO 132542 NERFINISHED
colorIndexB−V −0.21
colorIndexU−B −0.97
componentOf Orion constellation asterism NERFINISHED
constellation Orion NERFINISHED
declination −09° 40′ 11″
distanceFromEarth about 200 parsecs
about 650 light-years
dominantFusionProcess helium and heavier element fusion in core or shell
effectiveTemperature about 26,500 K
equatorialCoordinateSystem ICRS NERFINISHED
evolutionaryStage post-main-sequence
flamsteedDesignation 53 Orionis NERFINISHED
futureEvolution core-collapse supernova candidate
galacticLatitude −25.3°
galacticLongitude 214.5°
hasStellarWind strong
hdNumber HD 38771 NERFINISHED
hemisphereVisibility both northern and southern hemispheres
hipparcosNumber HIP 27366 NERFINISHED
hrNumber HR 2004
locatedIn Orion Arm of the Milky Way NERFINISHED
luminosity about 57,000 times the Sun
luminosityClass Ia
marks right knee of Orion
mass about 15 times the Sun
metallicity slightly sub-solar
opticalColor blue-white
parallax 4.38 mas
properMotionDec +1.99 mas/yr
properMotionRA +1.55 mas/yr
radialVelocity +21 km/s
radius about 22 times the Sun
rightAscension 05h 47m 45.4s
spectralType B0.5Ia
surfaceGravity low compared to main-sequence B stars
traditionalName Saiph NERFINISHED
variableStarStatus suspected variable
visibleToNakedEye true

Referenced by (2)

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

Saiph BayerDesignation Kappa Orionis
this entity surface form: κ Orionis
Saiph otherName Kappa Orionis