Global InformationHD 128311 information
 A near infrared (Y band) light curve for HN Boötes, adapted from Strassmeier et al. (2000)[1] | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Boötes |
| Right ascension | 14h 36m 00.56073s[2] |
| Declination | +09° 44′ 47.4536″[2] |
| Apparent magnitude (V) | 7.48[3] |
| Characteristics | |
| Spectral type | K3V[4] |
| B−V color index | 0.973±0.004[3] |
| Variable type | BY Dra[5] |
| Astrometry | |
| Radial velocity (Rv) | −9.62±0.15[2] km/s |
| Proper motion (μ) | RA: 204.360[2] mas/yr Dec.: −250.390[2] mas/yr |
| Parallax (π) | 61.2111 ± 0.0740 mas[2] |
| Distance | 53.28 ± 0.06 ly (16.34 ± 0.02 pc) |
| Absolute magnitude (MV) | 6.39[3] |
| Details[6] | |
| Mass | 0.82 M☉ |
| Radius | 0.78±0.01[2] R☉ |
| Luminosity | 0.308±0.001[2] L☉ |
| Surface gravity (log g) | 4.58 cgs |
| Temperature | 4,863+46 −15[2] K |
| Metallicity [Fe/H] | 0.08[7] dex 0.12[6] dex |
| Rotational velocity (v sin i) | 5.6 km/s |
| Age | 0.5–1.0 Gyr[8] 6.35[6] Gyr |
| Other designations | |
HN Boo, BD+10° 2710, GC 19679, GJ 3860, HD 128311, HIP 71395, SAO 120554, LTT 14312, GSC 00910-00165[9] | |
| Database references | |
| SIMBAD | data |
| ARICNS | data |
HD 128311 is a variable star in the northern constellation of Boötes. It has the variable star designation HN Boötis, while HD 128311 is the star's designation in the Henry Draper Catalogue. The star is invisible to the naked eye with an apparent visual magnitude that fluctuates around 7.48.[3] It is located at a distance of 53 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −9.6 km/s.[2] Two confirmed extrasolar planets have been detected in orbit around this star.[8]
The stellar classification of HN Boo is K3V,[4] which indicates this is a K-type main sequence star. It is a BY Draconis-type variable, randomly varying in brightness by 0.04 in magnitude over a period of 11.54 days[5] due to star spots and high chromospheric activity. The star exhibits strong emission, which suggests an age of 0.5–1.0 billion years.[8] It has 82% of the mass of the Sun and 78% of the Sun's radius. The metallicity of the star, meaning its abundance of heavier elements, appears slightly higher than in the Sun. It is radiating 31% of the luminosity of the Sun from its photosphere at an effective temperature of 4,863 K.[6]
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