  | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Gemini[1] |
| Right ascension | 07h 31m 48.40451s[2] |
| Declination | +17° 05′ 09.7647″[2] |
| Apparent magnitude (V) | +5.45[1] |
| Characteristics | |
| Evolutionary stage | red clump[3][4] |
| Spectral type | K2III[5] |
| B−V color index | 1.126±0.006[1] |
| Astrometry | |
| Radial velocity (Rv) | −33.35±0.15[2] km/s |
| Proper motion (μ) | RA: +39.385 mas/yr[2] Dec.: −75.752 mas/yr[2] |
| Parallax (π) | 11.3298±0.0764 mas[2] |
| Distance | 288 ± 2 ly (88.3 ± 0.6 pc) |
| Absolute magnitude (MV) | 0.52[1] |
| Orbit[6] | |
| 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[7] | |
| 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[8] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HD 59686 is a binary star[9] 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.[1] 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.[2]
This is a single-lined spectroscopic binary system with an orbital period of 32.0 years and a high eccentricity of 0.73.[6] The visible component is an aging giant star with a stellar classification of K2III.[5] It is most likely fusing helium in its core in a position on the H-R diagram called the red clump.[3] The stellar radius is very large: 11.2 times that of the Sun.[7] 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.[7]
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.[7]
Planetary system
[edit]The giant star HD 59686 A has one known planet, the gas giant HD 59686 Ab; it was discovered by Doppler spectroscopy and first announced in 2003,[10] but the discovery was not formally published until 2016. HD 59686, along with Nu Octantis, is one of the closest binary star systems known to host a planet orbiting a single star.[6]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥6.92+0.18 −0.24 MJ |
1.0860+0.0006 −0.0007 |
299.36+0.26 −0.31 |
0.05+0.03 −0.02 |
— | — |
References
[edit]- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
- ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b Stock, Stephan; Reffert, Sabine; Quirrenbach, Andreas (2018). "Precise radial velocities of giant stars. X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search". Astronomy and Astrophysics. 616: A33. arXiv:1805.04094. Bibcode:2018A&A...616A..33S. doi:10.1051/0004-6361/201833111.
- ^ Soubiran, C.; Bienaymé, O.; Mishenina, T. V.; Kovtyukh, V. V. (2008). "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants". Astronomy and Astrophysics. 480 (1): 91. arXiv:0712.1370. Bibcode:2008A&A...480...91S. doi:10.1051/0004-6361:20078788.
- ^ a b Adams, Walter S.; Joy, Alfred H.; Humason, Milton L.; Brayton, Ada Margaret (1935), "The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars", Astrophysical Journal, 81: 187, Bibcode:1935ApJ....81..187A, doi:10.1086/143628.
- ^ a b c d Ortiz, Mauricio; et al. (October 2016), "Precise radial velocities of giant stars. IX. HD 59686 Ab: a massive circumstellar planet orbiting a giant star in a 13.6 au eccentric binary system", Astronomy & Astrophysics, 595: 14, arXiv:1608.00963, Bibcode:2016A&A...595A..55O, doi:10.1051/0004-6361/201628791, S2CID 26289447, A55.
- ^ a b c d Jofré, E.; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets", Astronomy and Astrophysics, 574: A50, arXiv:1410.6422, Bibcode:2015A&A...574A..50J, doi:10.1051/0004-6361/201424474, S2CID 53666931.
- ^ "HD 59686". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-01-06.
- ^ Trifonov, Trifon; et al. (April 2018), "Dynamical Analysis of the Circumprimary Planet in the Eccentric Binary System HD 59686", The Astronomical Journal, 155 (4): 14, arXiv:1803.01434, Bibcode:2018AJ....155..174T, doi:10.3847/1538-3881/aab439, S2CID 119487750, 174.
- ^ Mitchell, D.; et al. (2003), "Four Substellar Companions Found Around Nearby K Giant Stars", Bulletin of the American Astronomical Society, 35: 1234, Bibcode:2003AAS...203.1703M.
External links
[edit]- "HD 59686". Extrasolar Planets Encyclopaedia. Archived from the original on July 2, 2007.
