36 Serpentis

36 Serpentis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Serpens
Right ascension 15h 51m 15.59418s
Declination −03° 05 25.7938
Apparent magnitude (V) 5.09 (5.2 + 7.8)
Characteristics
Spectral type A3Vn or A2IV-Vn (A7 + G0)
U−B color index +0.07
B−V color index +0.12
Astrometry
Radial velocity (Rv)−8 km/s
Proper motion (μ) RA: −91.09 mas/yr
Dec.: −28.21 mas/yr
Parallax (π)20.10±0.33 mas
Distance162 ± 3 ly
(49.8 ± 0.8 pc)
Absolute magnitude (MV)1.61
Orbit
Primary36 Ser A
Companion36 Ser B
Period (P)1,073 days
Eccentricity (e)0.7
Semi-amplitude (K1)
(primary)
6 km/s
Orbit
Primary36 Ser AB
Companion36 Ser C
Period (P)50.6±1.5 yr
Semi-major axis (a)0.400±0.006
Eccentricity (e)0.8323±0.0047
Inclination (i)98.08±0.31°
Longitude of the node (Ω)74.00±0.31°
Periastron epoch (T)2002.78±0.17
Argument of periastron (ω)
(secondary)
72.84±0.91°
Details
36 Ser A
Mass1.97 M
Radius2.25 R
Luminosity19.13 L
Surface gravity (log g)3.89 cgs
Temperature8,213 K
Metallicity [Fe/H]−2.00 dex
Rotational velocity (v sin i)229 km/s
Age710 Myr
36 Ser B
Mass≥0.37 and ≤0.50 M
36 Ser C
Mass1.27 M
Radius1.26 R
Temperature6,255 K
Age710 Myr
Other designations
b Ser, 36 Ser, BD−02°4058, FK5 2249, GC 4210, HD 141851, HIP 77660, HR 5895, SAO 140801, WDS J15513-0305
Database references
SIMBADdata

36 Serpentis is a triple star system in the equatorial constellation of Serpens. It has the Bayer designation b Serpentis, while 36 Serpentis is the Flamsteed designation. The system is visible to the naked eye as a dim, white-hued point of light with a combined apparent visual magnitude of 5.09. It is located 162 light years away from the Sun based on parallax, and is moving closer with a radial velocity of −8 km/s.