Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 04h 26m 36.37093s [1] |
Declination | +14° 42′ 49.6126″ [1] |
Apparent magnitude (V) | +4.69 [2] |
Characteristics | |
Spectral type | G7 IIIa Fe-1 [3] |
U−B color index | +0.72 [2] |
B−V color index | +0.98 [2] |
Astrometry | |
Radial velocity (Rv) | +31.4±0.3 [4] km/s |
Proper motion (μ) |
RA: −9.52
[1]
mas/
yr Dec.: −31.44 [1] mas/ yr |
Parallax (π) | 7.83 ± 0.22 mas [1] |
Distance | 420 ± 10
ly (128 ± 4 pc) |
Absolute magnitude (MV) | −1.27 [5] |
Details | |
Mass | 3.94 [5] M☉ |
Radius | 21 [6] R☉ |
Luminosity | 229 [7] L☉ |
Surface gravity (log g) | 2.54 [5] cgs |
Temperature | 5,086 [7] K |
Metallicity [Fe/H] | −0.08 [5] dex |
Age | 17 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Pi Tauri (π Tauri) is a solitary, [9] yellow-hued star in the zodiac constellation of Taurus. With an apparent visual magnitude of +4.69, [2] it is bright enough to be visible to the naked eye. Although it appears to lie among the stars of the Hyades cluster, it is not itself a member, being three times farther from Earth than the cluster. The distance to this star, as determined using an annual parallax shift of 7.83 mas as seen from the Earth, [1] is around 420 light years. At that range, the visual magnitude of the star is diminished by an extinction factor of 0.24 due to interstellar dust. [5]
This is an evolved G-type giant star with a stellar classification of G7 IIIa Fe-1, [3] where the suffix notation indicates an underabundance of iron in the spectrum. The measured angular diameter is 1.55±0.06 mas. [10] At the estimated distance of Pi Tauri, this yields a physical size of about 21 times the radius of the Sun. [6] It possesses nearly four [5] times the mass of the Sun and is radiating 229 times the Sun's luminosity at an effective temperature of 5,086 K. [7]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 04h 26m 36.37093s [1] |
Declination | +14° 42′ 49.6126″ [1] |
Apparent magnitude (V) | +4.69 [2] |
Characteristics | |
Spectral type | G7 IIIa Fe-1 [3] |
U−B color index | +0.72 [2] |
B−V color index | +0.98 [2] |
Astrometry | |
Radial velocity (Rv) | +31.4±0.3 [4] km/s |
Proper motion (μ) |
RA: −9.52
[1]
mas/
yr Dec.: −31.44 [1] mas/ yr |
Parallax (π) | 7.83 ± 0.22 mas [1] |
Distance | 420 ± 10
ly (128 ± 4 pc) |
Absolute magnitude (MV) | −1.27 [5] |
Details | |
Mass | 3.94 [5] M☉ |
Radius | 21 [6] R☉ |
Luminosity | 229 [7] L☉ |
Surface gravity (log g) | 2.54 [5] cgs |
Temperature | 5,086 [7] K |
Metallicity [Fe/H] | −0.08 [5] dex |
Age | 17 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Pi Tauri (π Tauri) is a solitary, [9] yellow-hued star in the zodiac constellation of Taurus. With an apparent visual magnitude of +4.69, [2] it is bright enough to be visible to the naked eye. Although it appears to lie among the stars of the Hyades cluster, it is not itself a member, being three times farther from Earth than the cluster. The distance to this star, as determined using an annual parallax shift of 7.83 mas as seen from the Earth, [1] is around 420 light years. At that range, the visual magnitude of the star is diminished by an extinction factor of 0.24 due to interstellar dust. [5]
This is an evolved G-type giant star with a stellar classification of G7 IIIa Fe-1, [3] where the suffix notation indicates an underabundance of iron in the spectrum. The measured angular diameter is 1.55±0.06 mas. [10] At the estimated distance of Pi Tauri, this yields a physical size of about 21 times the radius of the Sun. [6] It possesses nearly four [5] times the mass of the Sun and is radiating 229 times the Sun's luminosity at an effective temperature of 5,086 K. [7]