Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lacerta |
Right ascension | 22h 23m 33.624s[1] |
Declination | +52° 13′ 44.56″[1] |
Apparent magnitude (V) | 4.43[2] |
Characteristics | |
Spectral type | G8 III[3] |
U−B color index | +0.77[4] |
B−V color index | +1.02[4] |
V−R color index | 0.6[2] |
R−I color index | +0.57[4] |
Astrometry | |
Radial velocity (Rv) | −10.4 ± 0.9[2] km/s |
Proper motion (μ) | RA: −13.25±0.13[1] mas/yr Dec.: −186.77±0.13[1] mas/yr |
Parallax (π) | 19.19 ± 0.16 mas[1] |
Distance | 170 ± 1 ly (52.1 ± 0.4 pc) |
Absolute magnitude (MV) | +0.67[5] |
Details[5] | |
Mass | 0.97±0.21[3] M☉ |
Radius | 10.96±0.23[3] R☉ |
Luminosity | 57.7±3.0[3] L☉ |
Surface gravity (log g) | 2.43 cgs |
Temperature | 4803±75[3] K |
Metallicity [Fe/H] | −0.33 dex |
Rotational velocity (v sin i) | < 17[4] km/s |
Age | 6.76±3.59[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Beta Lacertae (Beta Lac, β Lacertae, β Lac) is the fourth-brightest star in the constellation of Lacerta. Based upon an annual parallax shift of 19.19 mas,[1] it is 170 light-years distant from Earth. At that distance, the visual magnitude is diminished by an extinction factor of 0.17 due to interstellar dust.[5]
This is an evolved G-type giant with an apparent visual magnitude of approximately 4.43.[2] It is a red clump[6] star and the primary component of a suspected binary system, with the pair having an angular separation of 0.2 arcsecond.[7]
van Leeuwen2007
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).Baines2018
was invoked but never defined (see the help page).Takeda2008
was invoked but never defined (see the help page).Mishenina2006
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).