Beta Serpentis

β Serpentis
Location of β Serpentis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Serpens
Right ascension 15h 46m 11.25435s
Declination +15° 25 18.5959
Apparent magnitude (V) +3.65 (3.68 + 9.7)
Characteristics
Spectral type A2 V or A2 IV + K3 V
U−B color index +0.09
B−V color index +0.073
Astrometry
Radial velocity (Rv)+0.6±0.3 km/s
Proper motion (μ) RA: +65.38 mas/yr
Dec.: −38.61 mas/yr
Parallax (π)21.03±0.26 mas
Distance155 ± 2 ly
(47.6 ± 0.6 pc)
Absolute magnitude (MV)+0.30/+6.59
Details
Mass1.828+0.027
−0.03
 M
Radius4.195 (equatorial)
3.07 (polar) R
Luminosity58.17+2.57
−2.25
 L
Surface gravity (log g)3.27 cgs
Temperature6,967 (equatorial)
9,359 (polar) K
Rotational velocity (v sin i)216.6+8.1
−8.7
 km/s
Age610+14
−35
 Myr
Other designations
Zhou, Chow, β Ser, 28 Serpentis, BD+15°2911, HD 141003, HIP 77233, HR 5867, SAO 101725, ADS 9778, CCDM 15461+1525
Database references
SIMBADdata

Beta Serpentis, Latinized from β Serpentis, also named Zhou, is a binary star system in the constellation Serpens, in its head (Serpens Caput). It is visible to the naked eye with a combined apparent visual magnitude of +3.65. Based upon an annual parallax shift of 21.03 mas as seen from Earth, it is located around 155 light years from the Sun. The system is a member of the Ursa Major Moving Group.