Sigma1 Tauri

Sigma1 Tauri
Location of σ1 Tauri (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Taurus
Right ascension 04h 39m 09.22247s
Declination +15° 47′ 59.5345″
Apparent magnitude (V) 5.07
Characteristics
Spectral type A4m
U−B color index 0.190
B−V color index 0.146
Astrometry
Radial velocity (Rv)+26.1±10.0 km/s
Proper motion (μ) RA: +41.91 mas/yr
Dec.: −66.88 mas/yr
Parallax (π)22.18±0.93 mas
Distance147 ± 6 ly
(45 ± 2 pc)
Absolute magnitude (MV)1.73
Orbit
Primaryσ1 Tau A
Nameσ1 Tau B
Period (P)38.951 d
Eccentricity (e)0.15
Longitude of the node (Ω)82°
Periastron epoch (T)2443094.319 JD
Semi-amplitude (K1)
(primary)
7.9 km/s
Details
Mass1.94 M
Luminosity14.7 L
Surface gravity (log g)4.08 cgs
Temperature8,470 K
Rotational velocity (v sin i)56.5±7.1 km/s
Other designations
91 Tauri, BD+15°665, HD 29479, HIP 21673, HR 1478, SAO 94051, WDS J04393+1555B
Database references
SIMBADdata

Sigma1 Tauri1 Tauri) is the Bayer designation for a white-hued star in the zodiac constellation of Taurus. It has an apparent visual magnitude of +5.07, which indicates it is visible to the naked eye. Based upon parallax measurements, σ1 Tauri is about 147 light-years from the Sun.

σ1 Tauri is a single-lined spectroscopic binary star system with an orbital period of 38.951 days and an eccentricity of 0.15. The visible component is an Am star with a stellar classification of A4m, indicating it is chemically peculiar A-type star. It is spinning with a projected rotational velocity of 56.5 km/s. The star has 1.9 times the mass of the Sun and is radiating 14.7 times the Sun's luminosity from its photosphere at an effective temperature of 8,470 K. Although it lies in the general direction of the Hyades cluster, based on parallax measurements it has been excluded from the list of candidate members.