Mu Serpentis

E460847

Mu Serpentis is a relatively bright A-type main-sequence star located in the tail region of the constellation Serpens.

All labels observed (1)

Label Occurrences
Mu Serpentis canonical 3

How this entity was disambiguated

Statements (35)

Predicate Object
instanceOf A-type star ⓘ
main-sequence star ⓘ
star ⓘ
age hundreds of millions of years (young to mid-age main-sequence) ⓘ
apparentMagnitudeV approximately 3.54 ⓘ
belongsTo Milky Way ⓘ
belongsToAsterism tail of Serpens ⓘ
catalogDesignation HD 141003 ⓘ
HIP 77233 ⓘ
HR 5867 ⓘ
Mu Ser ⓘ
μ Ser ⓘ
colorIndexBminusV approximately 0.00 ⓘ
constellation Serpens ⓘ
declination approximately −03° 25′ ⓘ
distanceFromEarth approximately 170 light-years ⓘ
approximately 52 parsecs ⓘ
effectiveTemperature about 9500 K ⓘ
equatorialCoordinatesEpoch J2000 ⓘ
galacticLatitude near the Galactic plane ⓘ
galacticLongitude in the direction of the Galactic center region ⓘ
galacticPopulation thin disk ⓘ
hasColor white ⓘ
hasCompanion no well-established close stellar companion ⓘ
locatedInArea tail region of the constellation Serpens ⓘ
luminosity about 40 times the luminosity of the Sun ⓘ
mass about 2.5 times the mass of the Sun ⓘ
observedIn optical band ⓘ
parallax about 19 milliarcseconds ⓘ
radius about 2.5 times the radius of the Sun ⓘ
rightAscension approximately 15h 49m ⓘ
rotationalVelocity high projected rotational velocity ⓘ
spectralClass A0V ⓘ
variableStarStatus not known as a prominent variable star ⓘ
visibleIn naked eye ⓘ

How these facts were elicited

Referenced by (3)

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

Serpens Cauda → contains → Mu Serpentis ⓘ
Serpens Caput → contains → Mu Serpentis ⓘ
Serpens → containsStar → Mu Serpentis ⓘ