HD 202206

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Template:Short description

HD 202206
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Capricornus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) Script error: No such module "val".[3]
Characteristics
Spectral type G6V[4] + M8V[3]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: −39.079[2] mas/yr
Dec.: −119.999[2] mas/yr
Parallax (π)21.7264±0.0651 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+4.80[1]
Orbit[3]
Period (P)256.33 days
Semi-major axis (a)Script error: No such module "val".
Eccentricity (e)Script error: No such module "val".
Inclination (i)Script error: No such module "val".°
Longitude of the node (Ω)Script error: No such module "val".°
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Semi-amplitude (K1)
(primary)
Script error: No such module "val". km/s
Details
A
MassScript error: No such module "val".[3] Template:Solar mass
RadiusScript error: No such module "val".[2] Template:Solar radius
LuminosityScript error: No such module "val".[2] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[3] cgs
TemperatureScript error: No such module "val".[2] K
Metallicity [Fe/H]Script error: No such module "val".[1] dex
Rotational velocity (v sin i)Script error: No such module "val".[3] km/s
AgeScript error: No such module "val".[3] Gyr
B
MassScript error: No such module "val".[3] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[6]
Database references
SIMBADdata

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HD 202206 is a binary star system in the southern constellation of Capricornus. With an apparent visual magnitude of +8.1,[3] it is too faint to be visible to the naked eye. It is located at a distance of 150 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +14.7 km/s.[5]

The primary component is a G-type main-sequence star with a stellar classification of G6V,[4] indicating it is generating energy through core hydrogen fusion. It is an estimated three[3] billion years old and is spinning with a projected rotational velocity of 2.3 km/s.[3] It is a metal-rich star – what astronomers term the abundance of elements of higher atomic number than helium – which may explain the star's unusually high luminosity for its class.[7] The star has a slightly greater mass and radius compared to the Sun.[3]


Companions

In 2000, analysis of radial velocity measurements of the star revealed the existence of a brown dwarf companion[8] with at least 17 times the mass of Jupiter around the star in an eccentric orbit with a period of around 256 days.[7] Even after the brown dwarf was accounted for, the star still showed a drift in the radial velocity measurements, suggesting another companion in a longer-period orbit. In 2004 after further observations, the parameters of a proposed companion was announced.[9]

Further observation of this system revised this picture in 2017, showing that the system instead consisted of a pair of co-orbiting stars being viewed nearly face-on, with the pair being orbited in turn by a Super-Jupiter designated HD 202206 c. The secondary stellar companion, now designated component B rather than 'b', is a red dwarf star with 8.9% of the mass of the Sun.[3]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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References

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  1. a b c d Template:Cite XHIP
  2. a b c d e f g h Template:Cite Gaia DR2
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  4. a b Script error: No such module "citation/CS1".
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External links

Template:Sky

Template:Stars of Capricornus