Gamma Serpentis

Gamma Serpentis
Observation data
Epoch J2000      Equinox J2000
Constellation Serpens
Right ascension 15h 56m 27.18266s
Declination +15° 39 41.8096
Apparent magnitude (V) 3.85
Characteristics
Spectral type F6 V
U−B color index −0.03
B−V color index +0.48
Variable type Suspected
Astrometry
Radial velocity (Rv)6.51±0.13 km/s
Proper motion (μ) RA: +311.183 mas/yr
Dec.: −1,282.767 mas/yr
Parallax (π)89.5647±0.1835 mas
Distance36.42 ± 0.07 ly
(11.17 ± 0.02 pc)
Absolute magnitude (MV)3.60
Details
Mass1.21±0.06 M
Radius1.461±0.007 R
Luminosity3.019±0.021 L
Surface gravity (log g)4.16±0.01 cgs
Temperature6,296±16 K
Metallicity [Fe/H]−0.18±0.01 dex
Rotational velocity (v sin i)10.2 km/s
Age3.6+0.9
−0.2
 Gyr
Other designations
Ainalhai, 41 Serpentis, BD+16°2849, FK5 591, GCTP 3604.00, HD 142860, HIP 78072, HR 5933, LHS 408, SAO 101826
Database references
SIMBADdata

Gamma Serpentis (γ Serpentis, γ Ser) is a star in the equatorial constellation Serpens, in the part of the constellation that represents the serpent's head (Serpens Caput). It has an apparent visual magnitude +3.85, which means it is visible to the naked eye. Based upon parallax measurements by the Gaia spacecraft, this star is approximately 36.4 light years from Earth.