Lambda Draconis

λ Draconis
Location of λ Draconis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Draco
Right ascension 11h 31m 24.22075s
Declination +69° 19 51.8696
Apparent magnitude (V) +3.85
Characteristics
Evolutionary stage asymptotic giant branch
Spectral type M0III-IIIa Ca1
U−B color index +1.97
B−V color index +1.62
Variable type slow irregular
Astrometry
Radial velocity (Rv)+6.58±0.30 km/s
Proper motion (μ) RA: −40.97 mas/yr
Dec.: −19.19 mas/yr
Parallax (π)9.79±0.15 mas
Distance333 ± 5 ly
(102 ± 2 pc)
Absolute magnitude (MV)−1.14±0.033
Details
Mass1.53±0.12 M
Radius69.99+1.06
−1.10
 R
Luminosity884±52 L
Surface gravity (log g)1.10±0.05 cgs
Temperature3,761±47 K
Metallicity [Fe/H]0.00 dex
Age2.33±0.48 Gyr
Other designations
λ Dra, 1 Draconis, BD−70°665, FK5 433, HD 100029, HIP 56211, HR 4434, SAO 15532
Database references
SIMBADdata

Lambda Draconis (λ Draconis, abbreviated Lam Dra, λ Dra), also named Giausar (/ˈɔːzɑːr/ JAW-zar), is a solitary, orange-red star in the northern circumpolar constellation of Draco. It is visible to the naked eye with an apparent visual magnitude of +3.85. Based upon an annual parallax shift of 9.79 mas as seen from the Earth, the star is located around 333 light years from the Sun.

This is an evolved red giant star on the asymptotic giant branch with a stellar classification of M0III-IIIa Ca1. It is a suspected slow irregular variable with a periodicity of roughly 1,100 days. 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.