BD+02 2056
BD+02 2056, also known as WASP-84 is a G-type main-sequence star. Its surface temperature is 5350±31 K, and is slightly enriched in heavy elements compared to the Sun, with a metallicity Fe/H index of 0.05±0.02. It is rich in carbon and depleted of oxygen.[5] BD+02 2056's age is probably older than the Sun at 8.5+4.1
−5.5 billion years.[4] The star appears to have an anomalously small radius, which can be explained by the unusually high helium fraction or by it being very young.[6]
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hydra |
| Right ascension | 08h 44m 25.7033s[1] |
| Declination | +01° 51′ 36.1066″[1] |
| Apparent magnitude (V) | 10.83 |
| Characteristics | |
| Evolutionary stage | main-sequence star |
| Spectral type | G9V[2] |
| Astrometry | |
| Radial velocity (Rv) | −5.1±0.6[3] km/s |
| Proper motion (μ) | RA: −23.344[3] mas/yr Dec.: −31.570[3] mas/yr |
| Parallax (π) | 9.9636 ± 0.0149[3] mas |
| Distance | 327.3 ± 0.5 ly (100.4 ± 0.2 pc) |
| Details[4] | |
| Mass | 0.842+0.037 −0.036 M☉ |
| Radius | 0.748±0.015 R☉ |
| Surface gravity (log g) | 4.63±0.06[5] cgs |
| Temperature | 5350±31[5] K |
| Metallicity [Fe/H] | 0.05±0.02[5] dex |
| Rotation | 14.36±0.35 d |
| Rotational velocity (v sin i) | 4.10±0.30 km/s |
| Age | 8.5+4.1 −5.5 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
A multiplicity survey did not detect any stellar companions to BD+02 2056 as at 2015.[7]
Planetary system
In 2013, one planet, named WASP-84b, was discovered on a tight, circular orbit.[8] The planet cannot have formed in its current location and likely migrated from elsewhere. The planetary orbit is well aligned with the equatorial plane of the star, misalignment being equal to 0.3±1.7°. Planetary equilibrium temperature is 832±13 K.[2]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.694+0.049 −0.047 MJ |
0.0771±0.0011 | 8.5234865±0.000007 | <0.077 | 88.368±0.050° | 0.942±0.022 RJ |
References
- "BD+02 2056". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-25.
- Anderson, D. R.; Triaud, A. H. M. J.; Turner, O. D.; Brown, D. J. A.; Clark, B. J. M.; Smalley, B.; Cameron, A. Collier; Doyle, A. P.; Gillon, M.; Hellier, C.; Lovis, C.; Maxted, P. F. L.; Pollacco, D.; Queloz, D.; Smith, A. M. S. (2015), "THE WELL-ALIGNED ORBIT OF WASP-84b: EVIDENCE FOR DISK MIGRATION OF a HOT JUPITER", The Astrophysical Journal, 800 (1): L9, arXiv:1409.6335, Bibcode:2015ApJ...800L...9A, doi:10.1088/2041-8205/800/1/L9, S2CID 13606807
- Brown, A. G. A.; et al. (Gaia collaboration). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics (in press). arXiv:2012.01533. doi:10.1051/0004-6361/202039657. S2CID 227254300. Gaia EDR3 record for this source at VizieR.
- Bonomo, A. S.; Desidera, S.; Benatti, S.; Borsa, F.; Crespi, S.; Damasso, M.; Lanza, A. F.; Sozzetti, A.; Lodato, G.; Marzari, F.; Boccato, C.; Claudi, R. U.; Cosentino, R.; Covino, E.; Gratton, R.; Maggio, A.; Micela, G.; Molinari, E.; Pagano, I.; Piotto, G.; Poretti, E.; Smareglia, R.; Affer, L.; Biazzo, K.; Bignamini, A.; Esposito, M.; Giacobbe, P.; Hébrard, G.; Malavolta, L.; et al. (2017), "The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets", Astronomy & Astrophysics, A107: 602, arXiv:1704.00373, Bibcode:2017A&A...602A.107B, doi:10.1051/0004-6361/201629882, S2CID 118923163
- Teske, Johanna K.; Thorngren, Daniel; Fortney, Jonathan J.; Hinkel, Natalie; Brewer, John M. (2019), "Do Metal-rich Stars Make Metal-rich Planets? New Insights on Giant Planet Formation from Host Star Abundances", The Astronomical Journal, 158 (6): 239, arXiv:1912.00255, Bibcode:2019AJ....158..239T, doi:10.3847/1538-3881/ab4f79, S2CID 208527082
- Maxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015), "Comparison of gyrochronological and isochronal age estimates for transiting exoplanet host stars", Astronomy & Astrophysics, 577: A90, arXiv:1503.09111, Bibcode:2015A&A...577A..90M, doi:10.1051/0004-6361/201525774, S2CID 53324330
- Wöllert, Maria; Brandner, Wolfgang (2015), "A Lucky Imaging search for stellar sources near 74 transit hosts", Astronomy & Astrophysics, 579: A129, arXiv:1506.05456, Bibcode:2015A&A...579A.129W, doi:10.1051/0004-6361/201526525, S2CID 118903879
- Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Skillen, I.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2014), "Three newly discovered sub-Jupiter-mass planets: WASP-69b and WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary★†", Monthly Notices of the Royal Astronomical Society, 445 (2): 1114–1129, arXiv:1310.5654, doi:10.1093/mnras/stu1737, S2CID 54750890
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