Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Taurus |
Right ascension | 03h 50m 24.9667s [2] |
Declination | 17° 14′ 47.431″ [2] |
Apparent magnitude (V) | 9.40 - 9.71 [3] |
Characteristics | |
Evolutionary stage | K2V + D2 [4] |
Variable type | Algol + RS CVn [3] |
Astrometry | |
Radial velocity (Rv) | 37.4±0.5 [5] km/s |
Proper motion (μ) |
RA: 127.278
[2]
mas/
yr Dec.: −22.321 [2] mas/ yr |
Parallax (π) | 21.0129 ± 0.0158 mas [2] |
Distance | 155.2 ± 0.1
ly (47.59 ± 0.04 pc) |
Orbit [6] | |
Period (P) | 0.52118 days |
Semi-major axis (a) | 0.01496 AU |
Eccentricity (e) | 0 (assumed) |
Inclination (i) | 80.8° |
Details | |
White dwarf | |
Mass | 0.792 [6] M☉ |
Radius | 0.01134 [6] R☉ |
Luminosity | 0.145 [7] L☉ |
Surface gravity (log g) | 8.227 [6] cgs |
Temperature | 34,500 [7] K |
K star | |
Mass | 0.852 [6] M☉ |
Radius | 0.816 [6] R☉ |
Luminosity | 0.41 [8] L☉ |
Surface gravity (log g) | 4.49 [9] cgs |
Temperature | 5,066 [9] K |
Metallicity [Fe/H] | +0.12 [8] dex |
Rotation | 0.5211 days [8] |
Rotational velocity (v sin i) | 89.30 [9] km/s |
Age | 625 [9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
V471 Tauri (short V471 Tau) is an eclipsing variable star in the constellation of Taurus. The star has a visual magnitude of 9 which makes it impossible to see with the naked eye. It is around 155 light-years away from the Solar System.
The V471 Tauri system has at least two members: a white dwarf star of spectral type D2; and a K-type main sequence star (K2 V). There are variations in the timing of the eclipses that were once thought to be due to a third member of the system, proposed to be a brown dwarf, but it may be a pair of smaller brown dwarfs [7] and/or the eclipse variations may be caused by the Applegate mechanism. The system is located in the Hyades star cluster. [6]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Taurus |
Right ascension | 03h 50m 24.9667s [2] |
Declination | 17° 14′ 47.431″ [2] |
Apparent magnitude (V) | 9.40 - 9.71 [3] |
Characteristics | |
Evolutionary stage | K2V + D2 [4] |
Variable type | Algol + RS CVn [3] |
Astrometry | |
Radial velocity (Rv) | 37.4±0.5 [5] km/s |
Proper motion (μ) |
RA: 127.278
[2]
mas/
yr Dec.: −22.321 [2] mas/ yr |
Parallax (π) | 21.0129 ± 0.0158 mas [2] |
Distance | 155.2 ± 0.1
ly (47.59 ± 0.04 pc) |
Orbit [6] | |
Period (P) | 0.52118 days |
Semi-major axis (a) | 0.01496 AU |
Eccentricity (e) | 0 (assumed) |
Inclination (i) | 80.8° |
Details | |
White dwarf | |
Mass | 0.792 [6] M☉ |
Radius | 0.01134 [6] R☉ |
Luminosity | 0.145 [7] L☉ |
Surface gravity (log g) | 8.227 [6] cgs |
Temperature | 34,500 [7] K |
K star | |
Mass | 0.852 [6] M☉ |
Radius | 0.816 [6] R☉ |
Luminosity | 0.41 [8] L☉ |
Surface gravity (log g) | 4.49 [9] cgs |
Temperature | 5,066 [9] K |
Metallicity [Fe/H] | +0.12 [8] dex |
Rotation | 0.5211 days [8] |
Rotational velocity (v sin i) | 89.30 [9] km/s |
Age | 625 [9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
V471 Tauri (short V471 Tau) is an eclipsing variable star in the constellation of Taurus. The star has a visual magnitude of 9 which makes it impossible to see with the naked eye. It is around 155 light-years away from the Solar System.
The V471 Tauri system has at least two members: a white dwarf star of spectral type D2; and a K-type main sequence star (K2 V). There are variations in the timing of the eclipses that were once thought to be due to a third member of the system, proposed to be a brown dwarf, but it may be a pair of smaller brown dwarfs [7] and/or the eclipse variations may be caused by the Applegate mechanism. The system is located in the Hyades star cluster. [6]