HD 13931
Appearance
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 16m 47.3790s[1] |
Declination | +43° 46′ 22.788″[1] |
Apparent magnitude (V) | 7.597 |
Characteristics | |
Spectral type | G0V[2] |
Apparent magnitude (B) | 8.237 |
Apparent magnitude (R) | 7.2 |
Apparent magnitude (I) | 6.9 |
Apparent magnitude (J) | 6.452 |
Apparent magnitude (H) | 6.234 |
Apparent magnitude (K) | 6.139 |
B−V color index | 0.640 |
V−R color index | 0.4 |
R−I color index | 0.3 |
Variable type | none |
Astrometry | |
Radial velocity (Rv) | +33.7 km/s |
Proper motion (μ) | RA: 99.03 ± 0.66[3] mas/yr Dec.: –183.19 ± 0.49[3] mas/yr |
Parallax (π) | 21.39 ± 0.24 mas[1] |
Distance | 152 ± 2 ly (46.8 ± 0.5 pc) |
Details | |
Mass | 1.04 ± 0.01[4] M☉ |
Radius | 1.18 ± 0.02[4] R☉ |
Luminosity | 1.49 ± 0.01[4] L☉ |
Surface gravity (log g) | 4.3 ± 0.03[4] cgs |
Temperature | 5868 ± 24[4] K |
Metallicity | +0.03 |
Rotation | ~26 days |
Age | 6.8 ± 0.6[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 13931 is an 8th magnitude G-type star located approximately 144 light years away[3] in the constellation Andromeda. This star is larger, hotter, brighter, and more massive than our Sun. Also its metal content is about 8% greater than the Sun. In 2009, a very long-period gas giant planet was found in orbit around the star.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥1.88 ± 0.15 MJ | 5.15 ± 0.29 | 4218 ± 388 | 0.02 ± 0.05 | — | — |
See also
References
- ^ a b c Gaia Collaboration; Brown, A. G. A.; Vallenari, A.; Prusti, T.; De Bruijne, J. H. J.; Mignard, F.; Drimmel, R.; Babusiaux, C.; Bailer-Jones, C. A. L.; Bastian, U.; Biermann, M.; Evans, D. W.; Eyer, L.; Jansen, F.; Jordi, C.; Katz, D.; Klioner, S. A.; Lammers, U.; Lindegren, L.; Luri, X.; O'Mullane, W.; Panem, C.; Pourbaix, D.; Randich, S.; Sartoretti, P.; Siddiqui, H. I.; Soubiran, C.; Valette, V.; Van Leeuwen, F.; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy & Astrophysics. 595: A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512.
- ^ Grenier, S.; Baylac, M.-O.; Rolland, L.; Burnage, R.; Arenou, F.; Briot, D.; Delmas, F.; Duflot, M.; Genty, V.; Gómez, A. E.; Halbwachs, J.-L.; Marouard, M.; Oblak, E.; Sellier, A. (1999). "Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS". Astronomy and Astrophysics Supplement. 137 (3): 451. Bibcode:1999A&AS..137..451G. doi:10.1051/aas:1999489.
- ^ a b c van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- ^ a b c d e f Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951.
- ^ Howard, Andrew W.; et al. (2010). "The California Planet Survey. I. Four New Giant Exoplanets". The Astrophysical Journal. 721 (2): 1467–1481. arXiv:1003.3488. Bibcode:2010ApJ...721.1467H. doi:10.1088/0004-637X/721/2/1467.