Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 04h 24m 05.75985s [1] |
Declination | +17° 26′ 38.8583″ [1] |
Apparent magnitude (V) | +4.80 [2] |
Characteristics | |
Spectral type | A2 Vs [3] |
U−B color index | +0.12 [2] |
B−V color index | +0.15 [2] |
Astrometry | |
Radial velocity (Rv) | +37.1 [4] km/s |
Proper motion (μ) |
RA: +108.16
[1]
mas/
yr Dec.: −34.66 [1] mas/ yr |
Parallax (π) | 20.21 ± 0.40 mas [1] |
Distance | 161 ± 3
ly (49.5 ± 1.0 pc) |
Absolute magnitude (MV) | +1.62 [5] |
Details | |
Mass | 1.79 [6] M☉ |
Radius | 1.8 [7] R☉ |
Luminosity | 27 [8] L☉ |
Surface gravity (log g) | 4.15 [4] cgs |
Temperature | 7,997 [4] K |
Metallicity [Fe/H] | +0.14 [4] dex |
Rotational velocity (v sin i) | 42 [4] km/s |
Age | 449 [6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Delta2 Tauri (δ2 Tauri) is a solitary, [10] white-hued star in the zodiac constellation of Taurus. Based upon an annual parallax shift of 20.21 mas as seen from Earth, [1] it is located roughly 161 light years distant from the Sun. It is separated from δ1 Tauri by 0.3° on the sky [11] and is faintly visible to the naked eye with an apparent visual magnitude of +4.80. [2] The star is considered a member of the Hyades cluster. [12]
At the estimated age of 449 million years, [6] this is an A-type main-sequence star with a stellar classification of A2 Vs, [3] where the 's' suffix indicates narrow (sharp) absorption lines. It has 1.8 [6] times the mass of the Sun and about 1.8 [7] times the Sun's radius. The star is radiating 27 [8] times the Sun's luminosity from its photosphere at an effective temperature of 7,997 K. [4]
δ2 Tauri is a source of X-ray emission with a luminosity of 101.1×1020 W. Since A-type stars are not normally a source of X-rays, this emission may be coming from an unknown companion or from a line of sight source. [13]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 04h 24m 05.75985s [1] |
Declination | +17° 26′ 38.8583″ [1] |
Apparent magnitude (V) | +4.80 [2] |
Characteristics | |
Spectral type | A2 Vs [3] |
U−B color index | +0.12 [2] |
B−V color index | +0.15 [2] |
Astrometry | |
Radial velocity (Rv) | +37.1 [4] km/s |
Proper motion (μ) |
RA: +108.16
[1]
mas/
yr Dec.: −34.66 [1] mas/ yr |
Parallax (π) | 20.21 ± 0.40 mas [1] |
Distance | 161 ± 3
ly (49.5 ± 1.0 pc) |
Absolute magnitude (MV) | +1.62 [5] |
Details | |
Mass | 1.79 [6] M☉ |
Radius | 1.8 [7] R☉ |
Luminosity | 27 [8] L☉ |
Surface gravity (log g) | 4.15 [4] cgs |
Temperature | 7,997 [4] K |
Metallicity [Fe/H] | +0.14 [4] dex |
Rotational velocity (v sin i) | 42 [4] km/s |
Age | 449 [6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Delta2 Tauri (δ2 Tauri) is a solitary, [10] white-hued star in the zodiac constellation of Taurus. Based upon an annual parallax shift of 20.21 mas as seen from Earth, [1] it is located roughly 161 light years distant from the Sun. It is separated from δ1 Tauri by 0.3° on the sky [11] and is faintly visible to the naked eye with an apparent visual magnitude of +4.80. [2] The star is considered a member of the Hyades cluster. [12]
At the estimated age of 449 million years, [6] this is an A-type main-sequence star with a stellar classification of A2 Vs, [3] where the 's' suffix indicates narrow (sharp) absorption lines. It has 1.8 [6] times the mass of the Sun and about 1.8 [7] times the Sun's radius. The star is radiating 27 [8] times the Sun's luminosity from its photosphere at an effective temperature of 7,997 K. [4]
δ2 Tauri is a source of X-ray emission with a luminosity of 101.1×1020 W. Since A-type stars are not normally a source of X-rays, this emission may be coming from an unknown companion or from a line of sight source. [13]