Tau Tauri

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Tau Tauri
Template:Location mark
Location of τ Tauri (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.27[2]
Characteristics
Spectral type B3V[3] + ? + A0V–A2V[4] + A1V[5]
U−B Template:Engvar -0.57[6]
B−V Template:Engvar -0.14[6]
Astrometry
Radial velocity (Rv)+14.60[7] km/s
Proper motion (μ) RA: -2.89[1] mas/yr
Dec.: -21.86[1] mas/yr
Parallax (π)8.19±0.88 mas[1]
Distanceapprox. Template:Rnd ly
(approx. Template:Rnd pc)
Absolute magnitude (MV)-1.15[2]
Orbit[8]
PrimaryAa
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Eccentricity (e)Script error: No such module "val".
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
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Semi-amplitude (K1)
(primary)
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Details
Aa
Mass6.4[9] Template:Solar mass
Luminosity1,472[10] Template:Solar luminosity
Surface gravity (log g)2.60[11] cgs
Temperature18,700[10] K
Metallicity [Fe/H]-0.51[11] dex
Rotational velocity (v sin i)115[12] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[13]
Database references
SIMBADdata

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Tau Tauri, Latinized from τ Tauri, is a quadruple star system[5] in the constellation Taurus. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.33.[14] The distance to this system is approximately about 400 light years based on parallax.[1] The system is moving further from the Earth with a heliocentric radial velocity of +14.6 km/s,[7] and it is a member of the Taurion OB association, located between Orion and Taurus.[15] It is located 0.7 degree north of the ecliptic, and thus is subject to lunar occultations.[4]

The blue-white hued primary, component Aa, is a B-type main-sequence star with a stellar classification of B3V.[3] It was found to be a close spectroscopic binary in 1903 by American astronomers Edwin B. Frost and Walter S. Adams. The pair have an orbital period of 2.96 days and eccentricity of 0.05.[8] A second companion, white-hued component Ab, has magnitude 6.97 and angular separation 0.2" from the primary in a 58-year orbit.[16][5] This is a probably A-type main-sequence star with a class of A0V–A2V.[4] The more distant component B is a type A1V star with magnitude 7.2 and separation 62.8".[5]

References

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  1. a b c d e f Script error: No such module "Citation/CS1". Vizier catalog entry
  2. a b Script error: No such module "Citation/CS1". Vizier catalog entry
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  5. a b c d Script error: No such module "Citation/CS1". Vizier catalog entry
  6. a b Script error: No such module "Citation/CS1".Vizier catalog entry
  7. a b Script error: No such module "Citation/CS1".
  8. a b Script error: No such module "Citation/CS1".
  9. Script error: No such module "Citation/CS1". Vizier catalog entry
  10. a b Script error: No such module "Citation/CS1". Vizier catalog entry
  11. a b Script error: No such module "Citation/CS1".
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  14. Script error: No such module "Citation/CS1". Vizier catalog entry
  15. Script error: No such module "Citation/CS1".
  16. Script error: No such module "Citation/CS1". Vizier catalog entry

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Template:Stars of Taurus