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HD 125628
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus[1] |
| Right ascension | 14h 22m 37.07301s[2] |
| Declination | −58° 27′ 32.8193″[2] |
| Apparent magnitude (V) | 4.76[1] (5.09 + 6.94)[3] |
| Characteristics | |
| A | |
| Evolutionary stage | giant[4] |
| Spectral type | G9III[3] |
| B−V color index | +0.795±0.003[1] |
| B | |
| Evolutionary stage | main sequence[5] |
| Spectral type | F5V[3] |
| B−V color index | +0.45[4] |
| Astrometry | |
| A | |
| Radial velocity (Rv) | +14.6±2.8[1] km/s |
| B | |
| Proper motion (μ) | RA: −39.763 mas/yr[5] Dec.: +24.058 mas/yr[5] |
| Parallax (π) | 13.0246±0.0192 mas[5] |
| Distance | 250.4 ± 0.4 ly (76.8 ± 0.1 pc) |
| Details | |
| A | |
| Mass | 2.9[6] M☉ |
| Radius | 12.3[6] R☉ |
| Surface gravity (log g) | 2.73[6] cgs |
| Temperature | 5,370[6] K |
| Rotational velocity (v sin i) | 5.5[4] km/s |
| Age | 3.6[4] Gyr |
| B | |
| Mass | 1.4[7] M☉ |
| Radius | 2.1[7] R☉ |
| Luminosity | 7.5[7] L☉ |
| Surface gravity (log g) | 3.95[7] cgs |
| Temperature | 6,642[7] K |
| Rotational velocity (v sin i) | 6.3[4] km/s |
| Age | 2.7[4] Gyr |
| Other designations | |
| CPD−57°6619, HD 125628, HIP 70264, HR 5371, SAO 241673[8] | |
| Database references | |
| SIMBAD | data |
HD 125628 is a binary star[3] system in the constellation Centaurus. It is faintly visible to the naked eye with a combined apparent visual magnitude of 4.76.[1] The distance to this system is approximately 380 light years based on parallax. It is drifting further away from the Sun with a radial velocity of +15 km/s.[1] The absolute magnitude is −0.55.[1]
The primary component of this system, component A, is an aging giant star with a stellar classification of G9III[3] and a visual magnitude of 5.09.[3] The secondary companion, designated component B, is a magnitude 6.94[3] star located at an angular separation of 9.10″ from the primary, along a position angle of 157°, as of 2016.[9] It is an F-type main-sequence star with a class of F5V.[3]
References
[edit]- ^ a b c d e f g 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 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. S2CID 18759600.
- ^ a b c d e f g h Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
- ^ a b c d e f Desidera, S.; et al. (August 2006). "Spectroscopic characterization of a sample of southern visual binaries". Astronomy and Astrophysics. 454 (2): 553–558. Bibcode:2006A&A...454..553D. doi:10.1051/0004-6361:20064895.
- ^ a b c 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 Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555. arXiv:astro-ph/9911002. Bibcode:1999A&A...352..555A.
- ^ a b c d e Stassun, Keivan G.; et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467.
- ^ "HD 125628". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-27.
- ^ Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.
