Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 04h 27m 17.4508s [1] |
Declination | +22° 59′ 46.778″ [1] |
Apparent magnitude (V) | 5.514 [2] |
Characteristics | |
Evolutionary stage | main sequence [1] |
Spectral type | B7V [3] |
U−B color index | −0.48 [4] |
B−V color index | −0.10 [4] |
Astrometry | |
Radial velocity (Rv) | 32.2±1.1 [5] km/s |
Proper motion (μ) |
RA: −1.409
[1]
mas/
yr Dec.: −13.722 [1] mas/ yr |
Parallax (π) | 7.9390 ± 0.398 mas [1] |
Distance | 410 ± 20
ly (126 ± 6 pc) |
Absolute magnitude (MV) | +0.21 [6] |
Details | |
Mass | 3.47 [1] M☉ |
Radius | 2.8 [1] R☉ |
Luminosity | 185 [1] L☉ |
Surface gravity (log g) | 3.97 [1] cgs |
Temperature | 12,689 [1] K |
Rotational velocity (v sin i) | 115 [7] km/s |
Age | 38 [8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
72 Tauri (abbreviated 72 Tau) is a possible binary star in the zodiac constellation of Taurus. It is faintly visible to the naked eye with an apparent visual magnitude of +5.5, although only 0.29° from the brighter υ Tauri. Based upon an annual parallax shift of 7.9 mas seen from Earth, it is around 410 light years from the Sun.
72 Tauri is a B-type main sequence star with a stellar classification of B7V. [3] With a mass of 3.48 M☉ and an estimated age of 38 million years, [8] it is 2.8 times the size of the Sun and 185 times its luminosity. [1]
Occasionally this star system is given the Bayer designation υ2 Tauri with υ Tauri, which is separated from it by 0.29° in the sky. [4] υ Tauri is a foreground star, the two are unrelated, [11] and although 72 Tauri lies near the Hyades open cluster, it is much further away. [1]
72 Tauri lies near the ecliptic and can be occulted by the moon. Observations of an occultation in 1985 showed that it was a binary star with the two components separated by 0.1 ″. [12] There has been no confirmation of this finding and other sources list the star as single. [13]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 04h 27m 17.4508s [1] |
Declination | +22° 59′ 46.778″ [1] |
Apparent magnitude (V) | 5.514 [2] |
Characteristics | |
Evolutionary stage | main sequence [1] |
Spectral type | B7V [3] |
U−B color index | −0.48 [4] |
B−V color index | −0.10 [4] |
Astrometry | |
Radial velocity (Rv) | 32.2±1.1 [5] km/s |
Proper motion (μ) |
RA: −1.409
[1]
mas/
yr Dec.: −13.722 [1] mas/ yr |
Parallax (π) | 7.9390 ± 0.398 mas [1] |
Distance | 410 ± 20
ly (126 ± 6 pc) |
Absolute magnitude (MV) | +0.21 [6] |
Details | |
Mass | 3.47 [1] M☉ |
Radius | 2.8 [1] R☉ |
Luminosity | 185 [1] L☉ |
Surface gravity (log g) | 3.97 [1] cgs |
Temperature | 12,689 [1] K |
Rotational velocity (v sin i) | 115 [7] km/s |
Age | 38 [8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
72 Tauri (abbreviated 72 Tau) is a possible binary star in the zodiac constellation of Taurus. It is faintly visible to the naked eye with an apparent visual magnitude of +5.5, although only 0.29° from the brighter υ Tauri. Based upon an annual parallax shift of 7.9 mas seen from Earth, it is around 410 light years from the Sun.
72 Tauri is a B-type main sequence star with a stellar classification of B7V. [3] With a mass of 3.48 M☉ and an estimated age of 38 million years, [8] it is 2.8 times the size of the Sun and 185 times its luminosity. [1]
Occasionally this star system is given the Bayer designation υ2 Tauri with υ Tauri, which is separated from it by 0.29° in the sky. [4] υ Tauri is a foreground star, the two are unrelated, [11] and although 72 Tauri lies near the Hyades open cluster, it is much further away. [1]
72 Tauri lies near the ecliptic and can be occulted by the moon. Observations of an occultation in 1985 showed that it was a binary star with the two components separated by 0.1 ″. [12] There has been no confirmation of this finding and other sources list the star as single. [13]