Delta Tucanae

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Template:Short description

Delta Tucanae A/B
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Tucana
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +4.48[2] (A: 4.52, B: 8.85)[3]
Characteristics
Spectral type B9 Vn + G0 V Fe−2[3]
U−B Template:Engvar A: −0.07, B: −0.02[3]
B−V Template:Engvar A: −0.02, B: +0.51[3]
Astrometry
Proper motion (μ) RA: +68.45[1] mas/yr
Dec.: +10.06[1] mas/yr
Parallax (π)13.00±0.48 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)A: 0.20, B: 4.50[3]
Details
δ Tuc A
Mass2.99[4] Template:Solar mass
Radius2.7[5] Template:Solar radius
Surface gravity (log g)Script error: No such module "val".[4] cgs
TemperatureScript error: No such module "val".[4] K
Rotation2.8535[6] d
Rotational velocity (v sin i)224[7] km/s
Age232[4] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
δ Tuc, CPD−65°4044, HD 212581, HIP 110838, HR 8540, SAO 255222, WDS J22273-6458AB[8]
Database references
SIMBADdata

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Delta Tucanae (δ Tuc, δ Tucanae) is a common proper motion[3] pair located in the southwestern corner of the southern constellation of Tucana.[9] Based upon an annual parallax shift of 13.00 mas as seen from Earth, is approximately 250 light years from the Sun. It is visible to the naked eye with a combined apparent visual magnitude of +4.48.[2] As of 2013, the two components had an angular separation of 7.0 arc seconds along a position angle of 282°.[10]

The brighter primary, component A, is blue-white hued star a visual magnitude of 4.52.[3] It is a B-type main-sequence star with a stellar classification of B9 Vn,[3] where the 'n' suffix indicates "nebulous" absorption lines due to the star's rotation. It is spinning rapidly with a projected rotational velocity of 224 km/s,[7] which is giving the star an oblate shape with an equatorial bulge that is an estimated 12% larger than the polar radius.[11] The star has about three times the mass of the Sun and is around 232 million years old.[4]

The magnitude 8.85[3] companion, component B, is a G-type main-sequence star. It has a classification of G0 V Fe−2,[3] with the suffix indicating an underabundance of iron in the star's photosphere.

References

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Template:Stars of Tucana