Delta2 Tauri

Star in the constellation Taurus From Wikipedia, the free encyclopedia

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]

Right ascension04h 24m 05.75985s[1]
Declination+17° 26 38.8583[1]
Quick facts Constellation, Right ascension ...
Delta2 Tauri

Location of δ2 Tauri in the Hyades, indicated by its Flamsteed designation 64
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
Evolutionary stage main sequence
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]
Distance161 ± 3 ly
(49.5 ± 1.0 pc)
Absolute magnitude (MV)+1.62[5]
Details
Mass1.79[6] M
Radius1.8[7] R
Luminosity27[8] L
Surface gravity (log g)4.15[4] cgs
Temperature7,997[4] K
Metallicity [Fe/H]+0.14[4] dex
Rotational velocity (v sin i)42[4] km/s
Age449[6] Myr
Other designations
δ2 Tau, 64 Tauri, BD+17°714, HD 27819, HIP 20542, HR 1380, SAO 93907[9]
Database references
SIMBADdata
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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]

References

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