HD 149143
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ophiuchus |
| Right ascension | 16h 32m 51.051s[1] |
| Declination | +02° 05′ 05.38″[1] |
| Apparent magnitude (V) | 7.89[2] |
| Characteristics | |
| Spectral type | G0 IV[2] or G3V[3] |
| B−V color index | 0.680[2] |
| Astrometry | |
| Radial velocity (Rv) | 12.104±0.0054[4] km/s |
| Proper motion (μ) | RA: −9.240 mas/yr[5] Dec.: −86.678 mas/yr[5] |
| Parallax (π) | 13.6279 ± 0.0247 mas[5] |
| Distance | 239.3 ± 0.4 ly (73.4 ± 0.1 pc) |
| Absolute magnitude (MV) | 3.87[2] |
| Details | |
| Mass | 1.1±0.1[2] M☉ |
| Radius | 1.302+0.083 −0.041[6] R☉ |
| Luminosity | 2.278±0.008[6] L☉ |
| Surface gravity (log g) | 4.10[2] cgs |
| Temperature | 6,213[6] K |
| Metallicity [Fe/H] | 0.20±0.05[2] dex |
| Rotational velocity (v sin i) | 3.9[2] km/s |
| Age | 7.6±1.2[2] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | 149143 data |
| Exoplanet Archive | data |
HD 149143, also called Rosalíadecastro, is a star with a close orbiting exoplanet in the Ophiuchus constellation. Its apparent visual magnitude is 7.89[2] (a binocular object) and the absolute magnitude is 3.87.[8] The system is located at a distance of 239 light years from the Sun based on parallax measurements, and it is drifting further away with a radial velocity of 12 km/s.[4]
On December 17, 2019, as part of the IAU's NameExoWorlds project, the star HD 149143 was given the name Rosalíadecastro in honour of the Spanish poet Rosalía de Castro, who was a significant figure of Galician culture and prominent Spanish writer, whose work often referenced the night and celestial objects. The exoplanet companion was named Riosar in honour of the Sar River in Spain that was present in much of the literary work of the Spanish author Rosalía de Castro.[9][10]
This is a slightly evolved star with a stellar classification of G0 that is overluminous for a high-metallicity G-type dwarf.[8] It has 1.1[2] times the mass of the Sun and 1.3[6] times the Sun's radius. The star has an estimated age of around 7.6 billion years and is spinning with a projected rotational velocity of 3.9 km/s.[2] It is radiating 2.3 times the luminosity of the Sun from its photosphere at an effective temperature of 6,213 K.[6]
Planetary system
[edit]HD 149143 b, the planet that orbits HD 149143, was discovered by the N2K Consortium during their search for short-period gas giant planets around metal-rich stars.[2] The planet was independently discovered by the Elodie metallicity-biased search for transiting Hot Jupiters.[8]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b (Riosar) | ≥1.33±0.15 MJ | 0.053±0.0029 | 4.07182±0.00001 | 0.0167±0.004 | — | 1.05 RJ |
See also
[edit]
References
[edit]- ^ a b 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 c d e f g h i j k l m Fischer, Debra A.; et al. (2006). "The N2K Consortium. III. Short-Period Planets Orbiting HD 149143 and HD 109749". The Astrophysical Journal. 637 (2): 1094–1101. Bibcode:2006ApJ...637.1094F. doi:10.1086/498557.
- ^ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey. 5. Bibcode:1999MSS...C05....0H.
- ^ a b Soubiran, C.; 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 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. Gaia DR2 record for this source at VizieR.
- ^ a b c d e Johns, Daniel; et al. (November 2018). "Revised Exoplanet Radii and Habitability Using Gaia Data Release 2". The Astrophysical Journal Supplement Series. 239 (1): 14. arXiv:1808.04533. Bibcode:2018ApJS..239...14J. doi:10.3847/1538-4365/aae5fb. 14.
- ^ "HD 149143". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-12-25.
- ^ a b c da Silva, R.; et al. (2006). "Elodie metallicity-biased search for transiting Hot Jupiters I. Two Hot Jupiters orbiting the slightly evolved stars HD118203 and HD149143". Astronomy and Astrophysics. 446 (2): 717–722. arXiv:astro-ph/0510048. Bibcode:2006A&A...446..717D. doi:10.1051/0004-6361:20054116. S2CID 18907493.
- ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
- ^ "IAU Catalog of Star Names". Retrieved 5 March 2020.
- ^ Ment, Kristo; et al. (2018). "Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810". The Astronomical Journal. 156 (5). 213. arXiv:1809.01228. Bibcode:2018AJ....156..213M. doi:10.3847/1538-3881/aae1f5. S2CID 119243619.
