Iota Tauri

Double star in the constellation Taurus From Wikipedia, the free encyclopedia

Iota Tauri, Latinized from ι Tauri, is a white-hued star in the zodiac constellation Taurus and an outlying member of the Hyades star cluster.[9] It is visible to the naked eye with an apparent visual magnitude of 4.62,[2] and is located at an estimated distance of about 173 light years based upon parallax measurements.[1] The star is moving away from the Sun with a radial velocity of +38 km/s.[5]

Right ascension05h 03m 05.74725s[1]
Declination+21° 35 23.8627[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
ι Tauri
Location of ι Tauri (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 05h 03m 05.74725s[1]
Declination +21° 35 23.8627[1]
Apparent magnitude (V) 4.62[2]
Characteristics
Spectral type A7 V[3]
U−B color index +0.15[4]
B−V color index +0.16[4]
Astrometry
Radial velocity (Rv)+38.30[5] km/s
Proper motion (μ) RA: +68.88[1] mas/yr
Dec.: -41.06[1] mas/yr
Parallax (π)18.88±0.30 mas[1]
Distance173 ± 3 ly
(53.0 ± 0.8 pc)
Absolute magnitude (MV)1.00[2]
Details
Mass2.22[6] M
Radius2.6[7] R
Luminosity36[6] L
Surface gravity (log g)3.97[8] cgs
Temperature8,054[6] K
Metallicity [Fe/H]+0.15[2] dex
Rotational velocity (v sin i)131[6] km/s
Age717[8] Myr
Other designations
ι Tau, 102 Tauri, BD+21°751, FK5 184, GC 6158, HD 32301, HIP 23497, HR 1620, SAO 76920, WDS J05031+2135AB, GSC 01293-02747
Database references
SIMBADdata
Close

This has been reported as a double star with two components at separation 0.1", both of type A7V and magnitude 5.4.[10][11] The combined spectrum matches a stellar classification of A7 V,[3] which would normally indicate an A-type main-sequence star that is generating energy through hydrogen fusion at its core. It has an estimated age of 717[8] million years.

References

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