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HD 206610

From Wikipedia, the free encyclopedia
Star in the Aquarius constellation
HD 206610 / Bosona

SDSS image of HD 206610
Observation data
Epoch J2000      Equinox J2000
ConstellationAquarius[1]
Right ascension21h 43m 24.900s[2]
Declination−07° 24′ 29.71″[2]
Apparent magnitude (V)8.34[1]
Characteristics
Evolutionary stagesubgiant[3]
Spectral typeK0III[4]
B−Vcolor index1.009±0.019[1]
Astrometry
Radial velocity (Rv)−18.62±0.12[2] km/s
Proper motion (μ)RA: 2.184±0.027mas/yr[2]
Dec.: 1.781±0.024mas/yr[2]
Parallax (π)6.7637±0.0270 mas[2]
Distance482 ± 2 ly
(147.8 ± 0.6 pc)
Absolute magnitude (MV)1.99[1]
Details
Mass1.51±0.05[5] M
Radius6.0±0.2[5] R
Luminosity18±1[5] L
Surface gravity (log g)3.22±0.02[6] cgs
Temperature4,819±9[6] K
Metallicity[Fe/H]0.09±0.05[6] dex
Rotational velocity (v sin i)1.77±0.40[6] km/s
Age3.0±0.3[5] Gyr
Other designations
BD−08°5719,Gaia DR2 2667434008056899712,HD 206610,HIP 107251,SAO 145619,TIC 333314269,TYC 5221-00210-1,2MASS J21432490-0724296,WISE J214324.89-072429.7[7]
Database references
SIMBADdata

HD 206610, also known asBosona, is astar with an orbitingexoplanet in theconstellation ofAquarius. Based onparallax measurements, it is located at a distance of approximately 482 light years from theSun.[2] Theabsolute magnitude of this star is 1.99,[1] but at that distance it is too faint to view with the naked eye, having anapparent visual magnitude of 8.34.[1] The system is drifting closer with aradial velocity of −18.6 km/s.[2]

This is an agingK-typesubgiant star[3] with astellar classification of K0III.[4] Having exhausted the supply of hydrogen at itscore, the star is cooling and expanding along thered giant branch. At the age of about three billion years, it has 1.5 times the Sun's mass and has grown to six times the radius of the Sun.[5] It has a similar iron abundance to the Sun and is spinning with aprojected rotational velocity of 1.77 km/s.[6] The star is radiating 18[5] times the luminosity of the Sun from its enlargedphotosphere at aneffective temperature of 4,819 K.[6]

The star HD 206610 and its exoplanet HD 206610 b are named Bosona andNaron respectively. The names were selected in theNameExoWorlds campaigns byBosnia and Herzegovina during the 100th anniversary of theIAU. Bosona is the historic name forBosnia,Horion Bosona, described inDe Administrando Imperio byPorphyrogenitus in 10th century, and its namesake the riverBosna's ancient name Bosona (Bosina, Basina, Basante). Naron is one of the names given to theNeretva river in Herzegovina originating with theRomans (Naro, Narona, Narenta, Nerenta), while in local tradition the name is said to go back even earlier with theCelts who called it Nera Etwa, which means the Flowing Divinity.[8][9][10]

Planetary system

[edit]

HD 206610 has one known exoplanet,HD 206610 b named Naron, discovered in 2010 using theradial velocity method.[3]

The HD 206610 planetary system[11]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b / Naron≥2.036±0.065 MJ1.74±0.33673.2±3.30.100±0.042

References

[edit]
  1. ^abcdefAnderson, 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.S2CID 119257644.
  2. ^abcdefgVallenari, 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. ^abcJohnson, John Asher; et al. (2010)."Retired A Stars and Their Companions. IV. Seven Jovian Exoplanets from Keck Observatory".Publications of the Astronomical Society of the Pacific.122 (892):701–711.arXiv:1003.3445.Bibcode:2010PASP..122..701J.doi:10.1086/653809.
  4. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  5. ^abcdefBonfanti, A.; et al. (2016). "Age consistency between exoplanet hosts and field stars".Astronomy & Astrophysics.585: 14.arXiv:1511.01744.Bibcode:2016A&A...585A...5B.doi:10.1051/0004-6361/201527297.S2CID 53971692. A5.
  6. ^abcdefJofré, E.; et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets".Astronomy & Astrophysics.574: A50.arXiv:1410.6422.Bibcode:2015A&A...574A..50J.doi:10.1051/0004-6361/201424474.S2CID 53666931.
  7. ^"HD 206610".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2024-01-03.
  8. ^"IAU 100 #NameExoWorlds: Bosna i Hercegovina imenovala zvijezdu i egzoplanetu u sazviježđu Vodolije".Astronomsko društvo Orion (in Serbo-Croatian). Sarajevo. 17 December 2019. Retrieved26 February 2023.
  9. ^"International Astronomical Union".www.iau.org. Archived fromthe original on 2022-12-05. Retrieved2020-01-02.
  10. ^"Approved names".NameExoworlds. Retrieved2020-01-02.
  11. ^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.

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