Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Taurus |
Right ascension | 04h 47m 6.7281s[2] |
Declination | 26° 10′ 45.613″[2] |
Apparent magnitude (V) | 9.0–10.6[3] |
Characteristics | |
Evolutionary stage | Post-AGB[4] |
Spectral type | G2eIa-M2Ia[5] |
U−B color index | 0.9-1.8[3] |
B−V color index | 1.5-1.9[3] |
Variable type | RVb[4] |
Astrometry | |
Radial velocity (Rv) | 32[6] km/s |
Proper motion (μ) | RA: 1.557[7] mas/yr Dec.: −4.717[7] mas/yr |
Parallax (π) | 0.6926 ± 0.0605 mas[7] |
Distance | 4,700 ± 400 ly (1,400 ± 100 pc) |
Absolute magnitude (MV) | −3.359[8] |
Orbit[4] | |
Period (P) | 1,198±17 d |
Semi-major axis (a) | 1.5 AU |
Eccentricity (e) | 0.5±0.1 |
Inclination (i) | 71±8° |
Semi-amplitude (K1) (primary) | 14.5±1.6 km/s |
Details | |
A | |
Mass | 0.53[4] M☉ |
Radius | 83.4±12.8[8] R☉ |
Luminosity | 2,800[4] L☉ |
Surface gravity (log g) | 0.6[4] cgs |
Temperature | 4,810±200[4] (4,225-5,080[3]) K |
Metallicity | −0.3±0.2[4] |
B | |
Mass | 0.7±0.1[4] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
RV Tauri (RV Tau) is a star in the constellation Taurus. It is a yellow supergiant and is the prototype of a class of pulsating variables known as RV Tauri variables. It is a post-AGB star and a spectroscopic binary about 4,700 light years away.
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