Mu Serpentis
E460847
Mu Serpentis is a relatively bright A-type main-sequence star located in the tail region of the constellation Serpens.
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 NERFINISHED ⓘ |
| belongsToAsterism | tail of Serpens ⓘ |
| catalogDesignation |
HD 141003
NERFINISHED
ⓘ
HIP 77233 NERFINISHED ⓘ HR 5867 NERFINISHED ⓘ Mu Ser NERFINISHED ⓘ μ Ser NERFINISHED ⓘ |
| colorIndexBminusV | approximately 0.00 ⓘ |
| constellation | Serpens NERFINISHED ⓘ |
| 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 ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.