HD 59686
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Gemini |
| Right ascension | 07h 31m 48.40451s |
| Declination | +17° 05′ 09.7647″ |
| Apparent magnitude (V) | +5.45 |
| Characteristics | |
| Evolutionary stage | red clump |
| Spectral type | K2III |
| B−V color index | 1.126±0.006 |
| Astrometry | |
| Radial velocity (Rv) | −33.35±0.15 km/s |
| Proper motion (μ) | RA: +39.385 mas/yr Dec.: −75.752 mas/yr |
| Parallax (π) | 11.3298±0.0764 mas |
| Distance | 288 ± 2 ly (88.3 ± 0.6 pc) |
| Absolute magnitude (MV) | 0.52 |
| Orbit | |
| Period (P) | 11,680+234 −173 d |
| Semi-major axis (a) | 13.56+0.18 −0.14 AU |
| Eccentricity (e) | 0.729+0.004 −0.003 |
| Argument of periastron (ω) (secondary) | 149.4±0.2° |
| Semi-amplitude (K1) (primary) | 4.014+0.010 −0.008 km/s |
| Details | |
| A | |
| Mass | 1.43±0.23 M☉ |
| Radius | 11.22±0.70 R☉ |
| Luminosity | 57.5+14.9 −11.8 L☉ |
| Surface gravity (log g) | 2.63±0.09 cgs |
| Temperature | 4,670±34 K |
| Metallicity [Fe/H] | 0.01±0.03 dex |
| Rotational velocity (v sin i) | 1.03±0.23 km/s |
| Age | 2.73±1.11 Gyr |
| B | |
| Mass | ≥0.53 M☉ |
| Other designations | |
| BD+17°1596, GC 10073, HD 59686, HIP 36616, HR 2877, SAO 96985, GSC 01364-01582 | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HD 59686 is a binary star system in the northern constellation of Gemini. It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.45. The distance to this system is approximately 288 light-years based on parallax, but it is drifting closer with a radial velocity of −33 km/s.
This is a single-lined spectroscopic binary system with an orbital period of 32.0 years and a high eccentricity of 0.73. The visible component is an aging giant star with a stellar classification of K2III. It is most likely fusing helium in its core in a position on the H-R diagram called the red clump. The stellar radius is very large: 11.2 times that of the Sun. The star is around 2.7 billion years old with 1.4 times the mass of the Sun. It is radiating 58 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,670 K.
The secondary component has a minimum mass 53% that of the Sun, which indicates it must be a star rather than a brown dwarf or a planet.