Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Draco |
Right ascension | 20h 02m 49.07268s[1] |
Declination | +67° 52′ 24.8294″[1] |
Apparent magnitude (V) | 4.52[2] |
Characteristics | |
Spectral type | K3 III[3] |
U−B color index | +1.54[2] |
B−V color index | +1.34[2] |
Astrometry | |
Radial velocity (Rv) | −9.80±0.43[4] km/s |
Proper motion (μ) | RA: +16.44[1] mas/yr Dec.: +47.31[1] mas/yr |
Parallax (π) | 7.61 ± 0.17 mas[1] |
Distance | 429 ± 10 ly (131 ± 3 pc) |
Absolute magnitude (MV) | −0.97[5] |
Details | |
Radius | 28[3] R☉ |
Luminosity | 402[6] L☉ |
Surface gravity (log g) | 1.90[7] cgs |
Temperature | 4370[7] K |
Metallicity [Fe/H] | 0.03[7] dex |
Rotational velocity (v sin i) | 10[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Rho Draconis (ρ Draconis) is a solitary[10] star in the northern circumpolar constellation of Draco. It is faintly visible to the naked eye with an apparent visual magnitude of 4.52.[2] Based upon an annual parallax shift of 7.61 mas as measured from Earth,[1] it is located around 429 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.027 due to interstellar dust.[5]
With a stellar classification of K3 III,[3] Rho Draconis is a normal giant star that is past the first dredge-up phase of its post-main sequence evolution.[7] It has the peculiar spectrum of a CN star, showing abnormal line strengths for cyanogen and calcium.[11] The star has expanded to around 28[3] times the Sun's radius and it is radiating 402[6] times the solar luminosity from its photosphere at an effective temperature of 4,370 K.[7]
vanLeeuwen2007
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was invoked but never defined (see the help page).Mishenina1995
was invoked but never defined (see the help page).Bernacca1970
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was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Mishenina1997
was invoked but never defined (see the help page).