HD 185269

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HD 185269
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cygnus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 6.67[3]
Characteristics
Evolutionary stage subgiant[4]
Spectral type G0IV[3]
B−V Template:Engvar 0.58[3]
Astrometry
Proper motion (μ) RA: −31.563[2] mas/yr
Dec.: −81.082[2] mas/yr
Parallax (π)19.2423±0.0182 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.29[3]
Absolute bolometric
magnitude
 (Mbol)
3.228[3]
Details
Mass1.33[3] Template:Solar mass
Radius2.1[2] Template:Solar radius
Luminosity4.8[2] Template:Solar luminosity
Surface gravity (log g)4.05[3] cgs
Temperature5,983[3] K
Metallicity [Fe/H]0.10[3] dex
Rotation29.5[5] days
Rotational velocity (v sin i)5.5[3] km/s
Age4.0[3] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Database references
SIMBADdata
Exoplanet Archivedata

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HD 185269 is a stellar triple system[6] approximately 170 light-years away in the constellation Cygnus. It is easily visible to binoculars, but not the naked eye.

The primary star is a third more massive[3] and nearly five times as luminous than the Sun.[2] The spectrum of the star is G0IV.[3] About 4.5 arcseconds away are the two other stars, which are much less massive than the Sun. The primary has a mass of Template:Solar mass, while the secondary has a mass of Template:Solar mass.[6]

Planetary system

The Jupiter-mass hot Jupiter was independently discovered orbiting the primary star by two different teams using doppler spectroscopy. One group led by Claire Moutou used the ELODIE spectrograph at the Haute-Provence Observatory in France while John Asher Johnson and collaborators used the Coudé Auxiliary and C. Donald Shane telescopes at Lick Observatory in California.[3][4] The planet takes 6.8 days to orbit at 0.077 AU from the primary star in an eccentric orbit.

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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External links

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