Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Serpens |
Right ascension | 15h 46m 11.25435s[1] |
Declination | +15° 25′ 18.5959″[1] |
Apparent magnitude (V) | +3.65[2] (3.68 + 9.7)[3] |
Characteristics | |
Spectral type | A2 V[4] or A2 IV[5] + K3 V[3] |
U−B color index | +0.09[2] |
B−V color index | +0.073[4] |
Astrometry | |
Radial velocity (Rv) | +0.6±0.3[6] km/s |
Proper motion (μ) | RA: +65.38[1] mas/yr Dec.: −38.61[1] mas/yr |
Parallax (π) | 21.03 ± 0.26 mas[1] |
Distance | 155 ± 2 ly (47.6 ± 0.6 pc) |
Absolute magnitude (MV) | +0.30/+6.59[7] |
Details | |
Mass | 1.94[8] M☉ |
Surface gravity (log g) | 3.27[8] cgs |
Temperature | 8,928±304[8] K |
Rotational velocity (v sin i) | 207±10.4[4] km/s |
Age | 267[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Beta Serpentis, Latinized from β Serpentis, is a binary star[3] 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.[2] Based upon an annual parallax shift of 21.03 mas as seen from Earth,[1] it is located around 155 light years from the Sun. The system is a member of the Ursa Major Moving Group.[7]
vanLeeuwen2007
was invoked but never defined (see the help page).Lutz1977
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Jones2015
was invoked but never defined (see the help page).Gray1987
was invoked but never defined (see the help page).Gontcharov2006
was invoked but never defined (see the help page).King2003
was invoked but never defined (see the help page).David2015
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).