HD 114386
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 13h 10m 39.8240s[1] |
| Declination | −35° 03′ 17.215″[1] |
| Apparent magnitude (V) | 8.73[2] |
| Characteristics | |
| Spectral type | K3V[2] |
| B−V color index | 0.982[2] |
| Astrometry | |
| Radial velocity (Rv) | 33.350 ± 0.0004[3] km/s |
| Proper motion (μ) | RA: −137.097[1] mas/yr Dec.: −324.880[1] mas/yr |
| Parallax (π) | 35.7823 ± 0.0515 mas[1] |
| Distance | 91.2 ± 0.1 ly (27.95 ± 0.04 pc) |
| Absolute magnitude (MV) | 6.49[2] |
| Details | |
| Mass | 0.60 ± 0.09[4] M☉ |
| Radius | 0.76 ± 0.02[4] R☉ |
| Luminosity | 0.29[2] L☉ |
| Surface gravity (log g) | 4.45 ± 0.06[4] cgs |
| Temperature | 4836 ± 18[4] K |
| Metallicity [Fe/H] | −0.05[4] dex |
| Rotational velocity (v sin i) | 1.0[2] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 114386 is a 9th magnitude star located approximately 91 light years away in the constellation of Centaurus. It is an orange dwarf, and rather dim compared to our Sun. To see it, one needs a telescope or good binoculars.
In 2004, the Geneva Extrasolar Planet Search Team announced the discovery of an extrasolar planet orbiting the star.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.37 MJ | 1.65 [6] | 445 | 0.12 | — | — |
| c | 1.19 MJ | 1.83 | 1046 | 0.06 | — | — |
See also
References
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
- ^ a b c d e f g Mayor, M.; et al. (2004). "The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE". Astronomy and Astrophysics. 415 (1): 391–402. arXiv:astro-ph/0310316. Bibcode:2004A&A...415..391M. doi:10.1051/0004-6361:20034250.
- ^ Soubiran, C.; Jasniewicz, G.; Chemin, L.; Zurbach, C.; Brouillet, N.; Panuzzo, P.; Sartoretti, P.; Katz, D.; Le Campion, J. -F.; Marchal, O.; Hestroffer, D.; Thévenin, F.; Crifo, F.; Udry, S.; Cropper, M.; Seabroke, G.; Viala, Y.; Benson, K.; Blomme, R.; Jean-Antoine, A.; Huckle, H.; Smith, M.; Baker, S. G.; Damerdji, Y.; Dolding, C.; Frémat, Y.; Gosset, E.; Guerrier, A.; Guy, L. P.; et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars". Astronomy and Astrophysics. 616: A7. arXiv:1804.09370. Bibcode:2018A&A...616A...7S. doi:10.1051/0004-6361/201832795. S2CID 52952408.
- ^ a b c d e Stassun, Keivan G.; Collins, Karen A.; Gaudi, B. Scott (2017). "Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes". The Astronomical Journal. 153 (3): 136. arXiv:1609.04389. Bibcode:2017AJ....153..136S. doi:10.3847/1538-3881/aa5df3. S2CID 119219062.
{{cite journal}}: CS1 maint: unflagged free DOI (link) - ^ "HD 114386". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-06-25.
- ^ [1]
External links
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