Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Draco |
Right ascension | 12h 55m 28.550015s[2] |
Declination | +65° 26′ 18.5079″[2] |
Apparent magnitude (V) | 5.225[3] |
Characteristics | |
Spectral type | F1VmA7(n)[4] |
B−V color index | 0.303±0.005[5] |
Variable type | Gamma Doradus[6] |
Astrometry | |
Radial velocity (Rv) | +9.0[7] km/s |
Proper motion (μ) | RA: −4.235[2] mas/yr Dec.: −30.174[2] mas/yr |
Parallax (π) | 34.0276 ± 0.0922 mas[2] |
Distance | 95.9 ± 0.3 ly (29.39 ± 0.08 pc) |
Absolute magnitude (MV) | 2.90[5] |
Details | |
Mass | 1.56[8] M☉ |
Radius | 1.50[8] R☉ |
Luminosity | 5.75[5] L☉ |
Surface gravity (log g) | 4.01[4] cgs |
Temperature | 7,129[4] K |
Metallicity [Fe/H] | −0.14[4] dex |
Rotational velocity (v sin i) | 119.6[9] km/s |
Age | 250±200[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
8 Draconis, formally named Taiyi /ˌtaɪˈjiː/,[11] is a single[12] star in the northern circumpolar constellation of Draco. Based upon an annual parallax shift of 34.14 mas as seen from the Earth,[13] the star is located approximately 96 light-years from the Sun. It is moving further away with a heliocentric radial velocity of +9 km/s,[7] having come within 40.6 ly some 2.6 million years ago.[5]
This is an F-type main-sequence star with a stellar classification of F1VmA7(n).[4] It is a Gamma Doradus variable star with a brightness variation of about one tenth of a magnitude.[6] 8 Dra has a relatively high rate of rotation, showing a projected rotational velocity of 120 km/s.[9] The star has 1.56 times the mass of the Sun and 1.50 times the Sun's radius.[8] It is radiating 5.75[5] times the Sun's luminosity from its photosphere at an effective temperature of 7,129 K.[4] An infrared excess has been detected at wavelengths of 24 and 70μm, which suggests the presence of a circumstellar disk orbiting the star.[8]
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