10 Boötis

Star in the constellation Boötes From Wikipedia, the free encyclopedia

10 Boötis is a suspected astrometric binary[8] star system in the northern constellation of Boötes,[7] located around 528 light years away from the Sun. It is visible to the naked eye under suitable viewing conditions as a dim, white-hued star with an apparent visual magnitude of 5.76.[2] Its magnitude is diminished by an extinction of 0.17 due to interstellar dust.[9] This system is moving away from the Earth with a heliocentric radial velocity of +6 km/s.[5]

Right ascension13h 58m 38.92101s[1]
Declination+21° 41 46.3302[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
10 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 13h 58m 38.92101s[1]
Declination +21° 41 46.3302[1]
Apparent magnitude (V) 5.76[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A0 Vs[4]
B−V color index −0.002±0.004[2]
Astrometry
Radial velocity (Rv)+6.1±2.9[5] km/s
Proper motion (μ) RA: −3.641[1] mas/yr
Dec.: −42.535[1] mas/yr
Parallax (π)6.1741±0.1059 mas
Distance528 ± 9 ly
(162 ± 3 pc)
Absolute magnitude (MV)−0.01[2]
Details
Mass2.87±0.14[3] M
Radius2.7[6] R
Luminosity113+32
−25
[3] L
Temperature9441±108[3] K
Rotational velocity (v sin i)75[3] km/s
Age337[2] Myr
Other designations
10 Boo, BD+22°2650, HD 121996, HIP 68276, HR 5255, SAO 83103[7]
Database references
SIMBADdata
Close

The visible component is an ordinary A-type main-sequence star with a stellar classification of A0 Vs,[4] where the 's' notation indicates "sharp" absorption lines. It is 337[2] million years old with a moderate rotation rate, showing a projected rotational velocity of 75 km/s.[3] The star has 2.87[3] times the mass of the Sun and about 2.7[6] times the Sun's radius. It is radiating 113[3] times the Sun's luminosity from its photosphere at an effective temperature of 9,441 K.[3]

References

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