Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Draco |
Right ascension | 11h 31m 24.22075s[1] |
Declination | +69° 19′ 51.8696″[1] |
Apparent magnitude (V) | +3.85[2] |
Characteristics | |
Evolutionary stage | asymptotic giant branch[3] |
Spectral type | M0III-IIIa Ca1[4] |
U−B color index | +1.97[2] |
B−V color index | +1.62[2] |
Variable type | slow irregular[5] |
Astrometry | |
Radial velocity (Rv) | +6.58±0.30[6] km/s |
Proper motion (μ) | RA: −40.97[1] mas/yr Dec.: −19.19[1] mas/yr |
Parallax (π) | 9.79 ± 0.15 mas[1] |
Distance | 333 ± 5 ly (102 ± 2 pc) |
Absolute magnitude (MV) | −1.14±0.033[7] |
Details[8] | |
Mass | 1.53±0.12 M☉ |
Radius | 69.99+1.06 −1.10 R☉ |
Luminosity | 884±52 L☉ |
Surface gravity (log g) | 1.10±0.05[9] cgs |
Temperature | 3,761±47 K |
Metallicity [Fe/H] | 0.00 dex |
Age | 2.33±0.48 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Lambda Draconis (λ Draconis, abbreviated Lam Dra, λ Dra), also named Giausar (/ˈdʒɔːzɑːr/ JAW-zar),[11][12] is a solitary,[13] orange-red[14] star in the northern circumpolar constellation of Draco. It is visible to the naked eye with an apparent visual magnitude of +3.85.[2] Based upon an annual parallax shift of 9.79 mas as seen from the Earth,[1] the star is located around 333 light years from the Sun.
This is an evolved red giant star on the asymptotic giant branch[3] with a stellar classification of M0III-IIIa Ca1.[4] It is a suspected slow irregular variable with a periodicity of roughly 1,100 days.[5] It has an estimated 1.53 times the mass of the Sun and a measured radius of 70 times the radius of the Sun. It is radiating 884 times the solar luminosity from its photosphere at an effective temperature of 3,761 K.[8]
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