HD 171301

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Template:Short description

HD 171301
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 5.47[1] + 12.7[3]
Characteristics
Spectral type B8IV[4] or B8V[5]
U−B Template:Engvar −0.463[1]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[6] km/s
Proper motion (μ) RA: 13.229[2] mas/yr
Dec.: 11.581[2] mas/yr
Parallax (π)9.3894±0.1103 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.27[1]
Details
A
MassScript error: No such module "val".[7] Template:Solar mass
RadiusScript error: No such module "val".[8] Template:Solar radius
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]Script error: No such module "val".[9] dex
Rotational velocity (v sin i)Script error: No such module "val".[5] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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HD 171301 is a suspected binary star[11] system in the northern constellation of Lyra. It has not been well-studied.[5] The brighter member of the pair, designated component A,[3] has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of 5.47.[1] The system is located at a distance of approximately 347 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −10 km/s.[6]

The stellar classification of HD 171301 is B8IV,[4] matching a late B-type star that may be a subgiant that is evolving off the main sequence. HD 171301 appears to be a type of chemically peculiar mercury-manganese star.[5] It has an estimated mass three[7] times that of the Sun and 2.7 times the Sun's radius.[8] The star is spinning with a projected rotational velocity of 36 km/s.[5] It is radiating 124[7] times the luminosity of the Sun from its photosphere at an effective temperature of 11,695 K.[7]

Its companion, component B, is a 13th magnitude star of an unknown spectral type.[12] It was first reported by S. W. Burnham in 1891. As of 1998, it was located at an angular separation of Script error: No such module "val". from the brighter star along a position angle of 157°.[3]

References

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  2. a b c d e Template:Cite DR2
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  5. a b c d e Script error: No such module "Citation/CS1".
  6. a b Script error: No such module "Citation/CS1".
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  8. a b Script error: No such module "Citation/CS1".
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External links

Template:Stars of Lyra