| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 14h 22m 37.07301s [1] |
| Declination | −58° 27′ 32.8193″ [1] |
| Apparent magnitude (V) | 4.76 [2] (5.09 + 6.94) [3] |
| Characteristics | |
| Spectral type | G9III + F5V [3] |
| B−V color index | 0.795±0.003 [2]/0.45 [4] |
| Astrometry | |
| Radial velocity (Rv) | +14.6±2.8 [2] km/s |
| Proper motion (μ) |
RA: −43.66±0.90
[1]
mas/
yr Dec.: +17.22±0.76 [1] mas/ yr |
| Parallax (π) | 8.51 ± 1.11 mas [1] |
| Distance | approx. 380
ly (approx. 120 pc) |
| Absolute magnitude (MV) | −0.55 [2] |
| Details | |
| A | |
| Rotational velocity (v sin i) | 5.5 [4] km/s |
| Age | 3.6 [4] Gyr |
| B | |
| Rotational velocity (v sin i) | 6.3 [4] km/s |
| Other designations | |
| 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. [2] 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. [2] The absolute magnitude is −0.55. [2]
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. [6] It is an F-type main-sequence star with a class of F5V. [3]
- ^ a b c d e 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 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. S2CID 119257644.
- ^ a b c d e f g 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 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.
- ^ "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.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 14h 22m 37.07301s [1] |
| Declination | −58° 27′ 32.8193″ [1] |
| Apparent magnitude (V) | 4.76 [2] (5.09 + 6.94) [3] |
| Characteristics | |
| Spectral type | G9III + F5V [3] |
| B−V color index | 0.795±0.003 [2]/0.45 [4] |
| Astrometry | |
| Radial velocity (Rv) | +14.6±2.8 [2] km/s |
| Proper motion (μ) |
RA: −43.66±0.90
[1]
mas/
yr Dec.: +17.22±0.76 [1] mas/ yr |
| Parallax (π) | 8.51 ± 1.11 mas [1] |
| Distance | approx. 380
ly (approx. 120 pc) |
| Absolute magnitude (MV) | −0.55 [2] |
| Details | |
| A | |
| Rotational velocity (v sin i) | 5.5 [4] km/s |
| Age | 3.6 [4] Gyr |
| B | |
| Rotational velocity (v sin i) | 6.3 [4] km/s |
| Other designations | |
| 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. [2] 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. [2] The absolute magnitude is −0.55. [2]
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. [6] It is an F-type main-sequence star with a class of F5V. [3]
- ^ a b c d e 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 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. S2CID 119257644.
- ^ a b c d e f g 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 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.
- ^ "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.
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