6 Lacertae

6 Lacertae
Observation data
Epoch J2000      Equinox J2000
Constellation Lacerta
Right ascension 22h 30m 29.26005s
Declination +43° 07 24.1565
Apparent magnitude (V) 4.52
Characteristics
Spectral type B2 IV
B−V color index −0.086±0.018
Astrometry
Radial velocity (Rv)−8.7±0.9 km/s
Proper motion (μ) RA: −4.800 mas/yr
Dec.: −2.598 mas/yr
Parallax (π)1.7577±0.2697 mas
Distanceapprox. 1,900 ly
(approx. 570 pc)
Absolute magnitude (MV)−2.62
Orbit
Period (P)880 days
Eccentricity (e)0.30
Periastron epoch (T)2,416,300 JD
Argument of periastron (ω)
(secondary)
190°
Semi-amplitude (K1)
(primary)
9 km/s
Details
Mass12.5±0.6 M
Radius6.9 R
Luminosity (bolometric)34,590 L
Surface gravity (log g)3.56 cgs
Temperature21,150 K
Metallicity [Fe/H]−0.04 dex
Rotational velocity (v sin i)70 km/s
Age15.7±0.1 Myr
Other designations
6 Lac, BD+42°4420, FK5 3800, HD 213420, HIP 111104, HR 8579, SAO 52079
Database references
SIMBADdata

6 Lacertae is a binary star system in the northern constellation of Lacerta, located around 1,900 light years from the Sun. It is visible to the naked eye as a dim, blue-white hued star with a combined apparent visual magnitude of 4.52. The system is moving closer to the Earth with a heliocentric radial velocity of −9 km/s, and is a suspected member of the Lac OB1 association.

This system forms a single-lined spectroscopic binary with an orbital period of 880 days and an eccentricity of 0.3. The visible component has a stellar classification of B2 IV, matching a B-type subgiant star. It is about 16 million years old with a relatively high projected rotational velocity of 70 km/s. The star has 12.5 times the mass of the Sun and about 7 times the Sun's radius. It is radiating a net 34,590 times the Sun's luminosity from its photosphere at an effective temperature of 21,150 K.