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HD 185269

Coordinates:Sky map19h 37m 11.7408s, +28° 29′ 59.509″
From Wikipedia, the free encyclopedia
Triple star system in the constellation Cygnus
HD 185269
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCygnus[1]
Right ascension19h 37m 11.74116s[2]
Declination+28° 29′ 59.5070″[2]
Apparent magnitude (V)6.67[3]
Characteristics
Evolutionary stagesubgiant[4]
Spectral typeG0IV[3]
B−Vcolor index0.58[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]
Distance169.5 ± 0.2 ly
(51.97 ± 0.05 pc)
Absolute magnitude (MV)3.29[3]
Absolute bolometric
magnitude
 (Mbol)
3.228[3]
Details
Mass1.33[3] M
Radius2.1[2] R
Luminosity4.8[2] L
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
Other designations
BD+28°3412,HIP 96507,SAO 87464[6]
Database references
SIMBADdata
Exoplanet Archivedata

HD 185269 is a stellar triple system[7] approximately 170light-years away in theconstellationCygnus. It is easily visible tobinoculars, but not thenaked eye.

The primary star is a third more massive[3] and nearly five times as luminous than theSun.[2] Thespectrum 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 0.165 M, while the secondary has a mass of 0.154 M.[7]

Planetary system

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The Jupiter-masshot Jupiter was independently discovered orbiting the primary star by two different teams usingdoppler spectroscopy. One group led by Claire Moutou used theELODIE spectrograph at theHaute-Provence Observatory in France whileJohn Asher Johnson and collaborators used theCoudé Auxiliary andC. Donald Shane telescopes atLick 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.

The HD 185269 planetary system[8]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b≥1.010±0.014 MJ0.0770±0.00346.83776±0.000270.229±0.014

See also

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References

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  1. ^Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.
  2. ^abcdefghVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcdefghijklmnMoutou, C.; et al. (2006)."ELODIE metallicity-biased search for transiting Hot Jupiters. III. A hot Jupiter orbiting the star HD 185269".Astronomy and Astrophysics.458 (1):327–329.arXiv:0707.0958.Bibcode:2006A&A...458..327M.doi:10.1051/0004-6361:20066029.
  4. ^abJohnson, John Asher; et al. (2006)."An Eccentric Hot Jupiter Orbiting the Subgiant HD 185269".The Astrophysical Journal.652 (2):1724–1728.arXiv:astro-ph/0608035.Bibcode:2006ApJ...652.1724J.doi:10.1086/508255.
  5. ^Llorente De Andrés, F.; de la Reza, R.; Cruz, P.; Cuenda-Muñoz, D.; Alfaro, E. J.; Chavero, C.; Cifuentes, C. (2024). "The evolution of lithium in FGK dwarf stars. Influence of planets and Galactic migration".Astronomy and Astrophysics.684.arXiv:2402.01315.Bibcode:2024A&A...684A..28L.doi:10.1051/0004-6361/202346744.
  6. ^"HD 185269".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-09-19.
  7. ^abGinski, C.; et al. (2016)."A lucky imaging multiplicity study of exoplanet host stars – II".Monthly Notices of the Royal Astronomical Society.457 (2):2173–2191.arXiv:1601.01524.Bibcode:2016MNRAS.457.2173G.doi:10.1093/mnras/stw049.
  8. ^Luhn, Jacob K.; et al. (2019)."Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts".The Astronomical Journal.157 (4). 149.arXiv:1811.03043.Bibcode:2019AJ....157..149L.doi:10.3847/1538-3881/aaf5d0.S2CID 102486961.

External links

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