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D Centauri
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| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Centaurus[1] |
| Right ascension | 12h 14m 02.697s[2] |
| Declination | −45° 43′ 26.10″[2] |
| Apparent magnitude (V) | +5.31[1] (5.78 + 6.98)[3] |
| Characteristics | |
| Spectral type | K3III[4] (K4IIIab + K2IIIb)[5] |
| U−B color index | +1.82/1.19[5] |
| B−V color index | +1.400±0.003[1]/1.21[5] |
| Astrometry | |
| A | |
| Radial velocity (Rv) | +10.27±0.68[6] km/s |
| Proper motion (μ) | RA: −37.186[6] mas/yr Dec.: 6.606[6] mas/yr |
| Parallax (π) | 5.3350±0.1399 mas[6] |
| Distance | 610 ± 20 ly (187 ± 5 pc) |
| Absolute magnitude (MV) | −0.88[1] |
| B | |
| Proper motion (μ) | RA: −33.604[7] mas/yr Dec.: 5.434[7] mas/yr |
| Parallax (π) | 4.9297±0.0550 mas[7] |
| Distance | 662 ± 7 ly (203 ± 2 pc) |
| Details | |
| A | |
| Radius | 42.8+1.1 −2.13[6] R☉ |
| Luminosity | 434±13[6] L☉ |
| Temperature | 4,026+104 −50[6] K |
| B | |
| Radius | 13.5+1.7 −1.9[7] R☉ |
| Luminosity | 90.5±1.4[7] L☉ |
| Temperature | 4,853+275 −392[7] K |
| Other designations | |
| D Cen, CD−45°7630, GC 16703, HD 106321, HIP 59654, HR 4652, SAO 223297, CCDM J12140-4543[8] | |
| Database references | |
| SIMBAD | data |
D Centauri is a double star in the southern constellation of Centaurus.[8] The system is faintly visible to the naked eye as a point of light with a combined apparent magnitude of +5.31;[1] the two components are of magnitude 5.78 and 6.98, respectively.[3] It is located at a distance of approximately 610 light years from the Sun based on parallax, and is drifting further away with a radial velocity of ~10 km/s.[6]
The dual nature of this star was announced by C. Rumker in 1837. As of 2015, the pair had an angular separation of 2.70″ along a position angle of 242°.[3] This orange-hued double has a combined stellar classification of K3III,[4] matching an aging giant star that has exhausted the supply of hydrogen at its core. In 1984, C. J. Corbally found a class of K4IIIab for the primary and K2IIIb for the fainter secondary.[5]
References
[edit]- ^ a b c d e 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. Vizier catalog entry
- ^ a b c Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122: 3466–3471. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.
- ^ a b Houk, N. (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 2. Dept. of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
- ^ a b c d Corbally, C. J. (1984). "Close visual binaries. I - MK classifications". The Astrophysical Journal Supplement Series. 55: 657. Bibcode:1984ApJS...55..657C. doi:10.1086/190973.
- ^ a b c d e f g h 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 f 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 "D Cen". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-28.
