47 Boötis

Binary star system in the constellation Boötes From Wikipedia, the free encyclopedia

47 Boötis is a binary star[9] system in the northern constellation of Boötes,[8] located 261 light years away from the Sun.[1] It has the Bayer designation k Boötis; 47 Boötis is the Flamsteed designation.[8] The system is visible to the naked eye as a faint, white-hued star with a combined apparent visual magnitude of 5.58.[2] It is moving closer to the Earth with a heliocentric radial velocity of −13 km/s.[2]

Right ascension15h 05m 25.83464s[1]
Declination+48° 09 03.4943[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
47 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 15h 05m 25.83464s[1]
Declination +48° 09 03.4943[1]
Apparent magnitude (V) 5.581[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A0 Vs[4]
B−V color index −0.005±0.003[5]
Variable type suspected[6]
Astrometry
Radial velocity (Rv)−12.63±0.73[2] km/s
Proper motion (μ) RA: −65.912[1] mas/yr
Dec.: +28.641[1] mas/yr
Parallax (π)12.4980±0.0766 mas[1]
Distance261 ± 2 ly
(80.0 ± 0.5 pc)
Absolute magnitude (MV)0.97[5]
Details
47 Boo A
Mass2.46±0.02[3] M
Radius1.8[7] R
Luminosity45.7+2.2
−2.0
[2] L
Surface gravity (log g)4.32[2] cgs
Temperature10,130[2] K
Rotational velocity (v sin i)54.8±1.6[2] km/s
Other designations
k Boo, 47 Boo, NSV 6934, BD+48°2262, FK5 1395, GC 20308, HD 133962, HIP 73841, HR 5627, SAO 45370, ADS 9500, CCDM 15054+4809[8]
Database references
SIMBADdata
Close

The primary member of the system, designated component A, is an A-type main-sequence star with a stellar classification of A0 Vs.[4] The 's' indicates sharp lines as it has a moderate rotation rate with a projected rotational velocity of 55 km/s.[2] It is a suspected variable star of unknown type.[10] The star has 2.46[3] times the mass of the Sun and is radiating 46[2] times the Sun's luminosity from its photosphere at an effective temperature of 10,130 K.[2]

The companion, component B, is a magnitude 13.3 star located at an angular separation of 6.2 arcseconds away from the primary.[9]

References

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