Rho Boötis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Boötes |
| Right ascension | 14h 31m 49.789s |
| Declination | +30° 22′ 17.17″ |
| Apparent magnitude (V) | 3.59 |
| Characteristics | |
| Spectral type | K4 III |
| U−B color index | +1.44 |
| B−V color index | +1.30 |
| R−I color index | 0.65 |
| Variable type | RS CVn. |
| Astrometry | |
| Radial velocity (Rv) | −13.57±0.19 km/s |
| Proper motion (μ) | RA: –100.531 mas/yr Dec.: +119.870 mas/yr |
| Parallax (π) | 19.8550±0.1587 mas |
| Distance | 164 ± 1 ly (50.4 ± 0.4 pc) |
| Absolute magnitude (MV) | +0.27 |
| Details | |
| Mass | 1.29±0.12 M☉ |
| Radius | 20.58±0.19 R☉ |
| Luminosity | 128.9±6.8 L☉ |
| Surface gravity (log g) | 1.85±0.05 cgs |
| Temperature | 4,285±54 K |
| Metallicity [Fe/H] | −0.19±0.10 dex |
| Rotational velocity (v sin i) | 5.0 km/s |
| Age | 4.31±1.17 Gyr |
| Other designations | |
| ρ Boo, 25 Boötis, BD+31°2628, FK5 534, GC 19597, HD 127665, HIP 71053, HR 5429, SAO 64202, PPM 77975, WDS J14318+3022A | |
| Database references | |
| SIMBAD | data |
Rho Boötis is a single, orange-hued star in the northern constellation of Boötes. Its name is a Bayer designation that is Latinised from ρ Boötis, and abbreviated Rho Boo or ρ Boo. This star is visible to the naked eye with an apparent visual magnitude of 3.59. Based upon parallax measurements, it is located at a distance of approximately 164 light-years (50 parsecs) from Earth. It is moving closer to the Sun with a radial velocity of −13.6 km/s. There is an optical companion, a magnitude 11.5 star, located 34.7 arcseconds away along a position angle of 345° (as of 2013).
This is an evolved K-type giant star, currently on the red-giant branch, with a stellar classification of K4 III and an estimated age of 4 billion years. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. With around 1.23 times the mass of the Sun, it has expanded to 20.6 times the Sun's girth. The star is radiating 129 times the Sun's luminosity from its enlarged photosphere at an effective temperature of about 4,285 K. Rho Boötis is classified as a RS Canum Venaticorum variable. Koen and Eyer examined the Hipparcos data for this star, and found that it varied with a period of 5.214 days, and an amplitude of 0.0027 magnitudes.