Delta Antliae

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Template:Short description

δ Antliae
Template:Location mark
Location of δ Antliae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Antlia
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +5.55[2] (5.58/9.65)[3]
Characteristics
Spectral type B9.5 V + F9 Ve[3]
U−B Template:Engvar −0.18[2]
B−V Template:Engvar −0.04[2]
Astrometry
Radial velocity (Rv)+14[4] km/s
Proper motion (μ) RA: −29.598 mas/yr[1]
Dec.: +1.704 mas/yr[1]
Parallax (π)7.0076±0.2204 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)–0.37[5]
Details
δ Ant A
Mass3.35±0.15[5] Template:Solar mass
Luminosity200[5] Template:Solar luminosity
Temperature11,117[5] K
Rotational velocity (v sin i)27[6] km/s
Age214[5] Myr
δ Ant B
Mass1.22–1.31[7] Template:Solar mass
Luminosity2.58[7] Template:Solar luminosity
Temperature5,948[7] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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Delta Antliae is a binary star[5] system in the southern constellation of Antlia. Its Bayer designation is Latinized from δ Antliae, and is abbreviated Del Ant or δ Ant, respectively. The combined apparent visual magnitude of the system is +5.57,[2] allowing it to be viewed from the suburbs with the naked eye. Based on the parallax shift of this system, it is located at a distance of approximately 470 light-years from Earth.[1] The system is reduced in magnitude by 0.03 due to extinction caused by intervening gas and dust.[3]

The primary component of the system has a stellar classification of B9.5 V, indicating that it is a B-type main sequence star. This star has an estimated 3.4[5] times the mass of the Sun. It is radiating around 200[5] times as much luminosity as the Sun from its photosphere at an effective temperature of 11,117 K.[5] At this heat, it shines with the characteristic blue-white hue of a B-type star.[9] The companion is an F-type main sequence star with a classification of F9 Ve, where the 'e' indicates that there are emission lines in the spectrum.

This is a young system with age estimates of 120[10] and 214[5] million years, with the secondary still in the post T Tauri stage.[7] The two stars are separated by 11 arcseconds,[3] corresponding to a physical separation of about Script error: No such module "val"..[10]

References

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Template:Stars of Antlia