HD 212301

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Template:Short description

HD 212301
Observation data
Epoch J2000      Equinox J2000
Constellation Octans
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 7.76[2]
Characteristics
Spectral type F8V[3] + M3V[4]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val".[1] mas/yr
Dec.: Script error: No such module "val".[1] mas/yr
Parallax (π)18.4109±0.0290 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)4.06[2]
Details
A
Mass1.20[5] Template:Solar mass
RadiusScript error: No such module "val".[1] Template:Solar radius
LuminosityScript error: No such module "val".[1] Template:Solar luminosity
Surface gravity (log g)4.35[5] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]Script error: No such module "val".[2] dex
Rotational velocity (v sin i)5.44[6] km/s
AgeScript error: No such module "val".[2] Gyr
B
MassScript error: No such module "val".[4] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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HD 212301 is a binary star[4] system in the south circumpolar constellation of Octans. This star is also called HIP 110852.[7] With an apparent visual magnitude of 7.76,[2] it is too faint to be visible to the naked eye. The system is located at a distance of 177 light years from the Sun based on parallax,[1] and is drifting further away with a radial velocity of +4.7 km/s.[2] It has an absolute magnitude of 4.06.[2]

The primary, component A, is an F-type main-sequence star with a stellar classification of F8V.[3] It has 20%[5] greater mass than the Sun and a 23%[1] larger radius. Its age is about the same as the Sun and it is spinning with a projected rotational velocity of 5.4 km/s.[6] It is a metal-rich star with 50% more metals than the Sun has.[6] The star is radiating 1.9[1] times the luminosity of the Sun from its photosphere at an effective temperature of 6,169 K.[1]

A secondary companion was announced in 2009. This faint star is located at an angular separation of Script error: No such module "val". to the northwest of the primary, corresponding to a projected separation of Script error: No such module "val".. This is a red dwarf with an estimated class of M3V and a mass equal to around 35% of the mass of the Sun. The pair share a common proper motion.[4]

A hot jupiter candidate exoplanet was discovered orbiting the primary, based on radial velocity observations taken in 2003 and 2005.[6]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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  7. a b Template:Cite simbad

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External links

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Template:Sky Template:Stars of Octans