D Centauri
From Wikipedia, the free encyclopedia
 |
This article does not cite any references or sources. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed. (December 2009) |
For d Centauri, see HD 117440.
| Observation data Epoch J2000.0 Equinox J2000.0 |
|
|---|---|
| Constellation | Centaurus |
| Right ascension | 12h14m02.6s |
| Declination | −45°43′26″ |
| Apparent magnitude (V) | +5.31 |
| Characteristics | |
| Spectral type | K3III |
| U−B color index | +1.59 |
| B−V color index | +1.43 |
| Variable type | none |
| Astrometry | |
| Radial velocity (Rv) | +7 km/s |
| Proper motion (μ) | RA: −35.19 mas/yr Dec.: 4.41 mas/yr |
| Parallax (π) | 5.76 ± 0.83 mas |
| Distance | 566 ly (174 pc) |
| Absolute magnitude (MV) | −0.88 |
| Other designations | |
| Database references | |
| SIMBAD | data |
D Centauri (D Cen) is a double star in the constellation Centaurus. The system has a combined apparent magnitude of +5.31 and is approximately 566 light years from Earth.
The system is classified as an orange K-type giant. The brighter component has an apparent magnitude of +5.31, while the apparent magnitude of the optical companion is +6.8. The two stars are separated by 2.9 arcseconds.
|
|||||||||||
 |
This binary or multiple star system–related article is a stub. You can help Wikipedia by expanding it. |
