Psi Tauri

Star in the constellation Taurus From Wikipedia, the free encyclopedia

Psi Tauri, which is Latinized from ψ Tauri, is a solitary[9] star in the zodiac constellation of Taurus. It has a yellow-white hue and is visible to the naked eye with an apparent visual magnitude of +5.22.[2] The distance to this system, as determined using an annual parallax shift of 36.2 mas as seen from the Earth,[10] is 91 light years. It is drifting further away with a radial velocity of +9 km/s.

Right ascension04h 07m 00.45695s[1]
Declination+29° 00 04.7093[1]
Quick facts Constellation, Right ascension ...
Psi Tauri
Location of ψ Tauri (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Taurus
Right ascension 04h 07m 00.45695s[1]
Declination +29° 00 04.7093[1]
Apparent magnitude (V) +5.22[2]
Characteristics
Evolutionary stage main sequence[1]
Spectral type F1 V[3]
U−B color index −0.01[2]
B−V color index +0.34[2]
Astrometry
Radial velocity (Rv)+9.15±0.42[4] km/s
Proper motion (μ) RA: −91.661[1] mas/yr
Dec.: +8.096[1] mas/yr
Parallax (π)35.9320±0.1055 mas[1]
Distance90.8 ± 0.3 ly
(27.83 ± 0.08 pc)
Absolute magnitude (MV)3.01[5]
Details
Mass1.59[5] M
Radius1.4[1] R
Luminosity5.2[1] L
Surface gravity (log g)4.36±0.14[5] cgs
Temperature6,856[1] K
Metallicity [Fe/H]−0.20[6] dex
Rotational velocity (v sin i)45.4±2.3[7] km/s
Age1.435[5] Gyr
Other designations
ψ Tau, 42 Tau, BD+28°619, FK5 2295, HD 25867, HIP 19205, HR 1269, SAO 76461[8]
Database references
SIMBADdata
Close

This object is an F-type main sequence star with a stellar classification of F1 V,[3] which indicates it is undergoing core hydrogen fusion. It is about 1.4 billion years old and is spinning with a projected rotational velocity of 45 km/s.[7] The star has 1.6 times the mass of the Sun[5] and 1.4 times its radius.[1] It is radiating 4.8 times the Sun's luminosity from its photosphere at an effective temperature of 7,088 K.[5]

References

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