R Doradus
 Infrared interferometric image of the star Credit: ESO |
|
| Observation data Epoch J2000 Equinox J2000 |
|
|---|---|
| Constellation | Dorado |
| Right ascension | 04h 36m 45.59127s |
| Declination | −62° 04′ 37.7974″ |
| Apparent magnitude (V) | 4.8–6.6 5.40 |
| Characteristics | |
| Spectral type | M8IIIe |
| Apparent magnitude (J) | −2.6 |
| Apparent magnitude (K) | −4.2 |
| U−B color index | +0.86 |
| B−V color index | +1.58 |
| Variable type | Mira variable |
| Astrometry | |
| Radial velocity (Rv) | +26.1 km/s |
| Proper motion (μ) |
RA: −69.36 mas/yr Dec.: −75.78 mas/yr |
| Parallax (π) | 18.31 ± 0.99mas |
| Distance | 178 ± 10 ly (55 ± 3 pc) |
| Details | |
| Mass | 1.2 M☉ |
| Radius | 370 ± 50 R☉ |
| Luminosity | 6,500 ± 1400 L☉ |
| Temperature | 2,740 ± 190 K |
| Rotation | 340 days |
| Other designations | |
| Database references | |
| SIMBAD | data |
R Doradus (HD 29712 or P Doradus) is the name of a red giant Mira variable star in the far-southern constellation Dorado, although visually it appears more closely associated with the constellation Reticulum. Its distance from Earth is 178 ± 10 light-years (54.6 ± 3.1 parsecs). Having a uniform disk diameter of 0.057 ± 0.005 arcsec, it is currently believed to be the extrasolar star with the largest apparent size as viewed from Earth. The estimated diameter of R Doradus is 515 ± 70 million km (3.46 AU) or 370 ± 50 times the diameter of the Sun. If placed at the centre of the Solar System, the orbit of Mars and most of the main asteroid belt would be contained within the star.
The visible magnitude of R Doradus varies between 4.8 and 6.6, which makes it usually just visible to the naked eye, but in the infrared it is one of the brightest stars in the sky and its bolometric luminosity is 6500 ± 1400 times that of the Sun. With a near-infrared J band magnitude of −2.6, only Betelgeuse at −2.9 is brighter.
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