| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Corvus |
| Right ascension | 12h 19m 37.8707s |
| Declination | −19° 15′ 21.862″ |
| Apparent magnitude (V) | 6.7 to 14.4 |
| Characteristics | |
| Evolutionary stage | AGB |
| Spectral type | M4.5e-M9e |
| U−B color index | +0.16 |
| B−V color index | +1.53 |
| Variable type | Mira |
| Astrometry | |
| Radial velocity (Rv) | −22.00 km/s |
| Proper motion (μ) | RA: −4.247 mas/yr Dec.: −8.663 mas/yr |
| Parallax (π) | 1.2136±0.0718 mas |
| Distance | 2,700 ± 200 ly (820 ± 50 pc) |
| Details | |
| Mass | 3.4 M☉ |
| Surface gravity (log g) | 1.59 cgs |
| Temperature | 3,857 K |
| Metallicity [Fe/H] | −0.38 dex |
| Other designations | |
| R Cvr, BD−18°3367, HD 107199, HIP 60106, SAO 157211 | |
| Database references | |
| SIMBAD | data |
R Corvi (R Crv) is a Mira variable star in the constellation Corvus, which ranges from a magnitude of 6.7 to 14.4 with a period of approximately 317 days. In the sky it appears close to Gamma Corvi and can be seen in the same binocular field. Extrapolating its luminosity from its period of 317 days yields a distance of 810 parsecs.
Franciszek Karliński discovered that the star's brightness varies, in 1867.
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