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Gliese 86

Coordinates:Sky map02h 10m 14s, −50° 50′ 00″
From Wikipedia, the free encyclopedia
Binary star system in the constellation Eridanus
Gliese 86
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationEridanus
Gliese 86 A
Right ascension02h 10m 25.9191s[1]
Declination−50° 49′ 25.4672″[1]
Apparent magnitude (V)6.17[2]
Gliese 86 B
Right ascension02h 10m 26s
Declination−50° 49′ 25″
Characteristics
Spectral typeK1V[3] + DQ6[4][5]
U−Bcolor index0.45
B−Vcolor index0.812[6]
V−Rcolor index0.45
R−Icolor index0.40
Astrometry
Radial velocity (Rv)56.7[7] km/s
Proper motion (μ)RA: 2,124.853±0.075[1]mas/yr
Dec.: 638.092±0.063[1]mas/yr
Parallax (π)92.7042±0.0454 mas[1]
Distance35.18 ± 0.02 ly
(10.787 ± 0.005 pc)
Absolute magnitude (MV)5.95[8]
Orbit[4]
PrimaryGliese 86 A
CompanionGliese 86 B
Period (P)≈100yr
Semi-major axis (a)23.7 au
Eccentricity (e)0.429
Inclination (i)126.44°
Longitude of the node (Ω)234.2°
Details[9]
Gliese 86 A
Mass0.83±0.05 M
Radius0.79±0.03 R
Surface gravity (log g)4.56±0.10 cgs
Temperature5180±80 K
Metallicity [Fe/H]−0.27±0.07 dex
Rotational velocity (v sin i)2.0±1.0 km/s
Age10±1 Gyr
Gliese 86 B
Mass0.5425[4] M
Temperature8180±120[5] K
Other designations
Gliese 86A:CD−51°532,HD 13445,HIP 10138,HR 637,SAO 232658,WDS J02104-5049A[10]
Gliese 86B:GJ 86 B,HD 13445B,WDS J02104-5049B,WD 0208-510[11]
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata

Gliese 86 (13 G. Eridani, HD 13445) is aK-type main-sequence star approximately 35light-years away in theconstellation ofEridanus. It has been confirmed that awhite dwarf orbits the primary star. In 1998 theEuropean Southern Observatory announced that anextrasolar planet was orbiting the star.[12]

Stellar components

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The primary companion (Gliese 86 A) is a K-type main-sequencestar ofspectral type K1V. The characteristics in comparison to theSun are 83% the mass, 79% the radius, and 50% the luminosity. The star has a close-orbiting massiveJovian planet.

Gliese 86 B is awhite dwarf located around 21 AU from the primary star, making the Gliese 86 system one of the tightest binaries known to host an extrasolar planet.[13] It was discovered in 2001 and initially suspected to be abrown dwarf,[14] but high contrast observations in 2005 suggested that the object is probably a white dwarf, as its spectrum does not exhibit molecular absorption features which are typical of brown dwarfs.[15] Assuming the white dwarf has a mass about half that of the Sun and that the linear trend observed in radial velocity measurements is due to Gliese 86 B, a plausible orbit for this star around Gliese 86 A has asemimajor axis of 18.42 AU and aneccentricity of 0.3974.[16] When both stars were on the main sequence, the separation between the two stars was closer, at around 9 AU.[4] More precise measurements for the white dwarf give it a mass of 55% the mass of the Sun[4] and a temperature of around 8200 K.[9]

Planetary system

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The planet Gliese 86 b was discovered by the Swiss 1.2 mLeonhard Euler Telescope operated by theGeneva Observatory.[17] Such an object was formed from aprotoplanetary disk that was truncated at 2 AU from the parent star.[4]

The radial velocity measurements of Gliese 86 show a linear trend once the motion due to this planet are taken out. This may be associated with the orbital motion of the white dwarf companion.

The Gliese 86 planetary system[18]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b≥6.588±0.018 MJ0.114340±0.00000115.76480±0.000040.048±0.002

See also

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References

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  1. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^C. Cincunegui; P. J. D. Mauas (2004)."Library of flux-calibrated echelle spectra of southern late-type dwarfs with different activity levels".Astronomy and Astrophysics.414 (2):699–706.Bibcode:2004A&A...414..699C.doi:10.1051/0004-6361:20031671.hdl:11336/21158.Archived from the original on 2019-06-22. Retrieved2012-06-12.
  3. ^Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample",The Astronomical Journal,132 (1):161–170,arXiv:astro-ph/0603770,Bibcode:2006AJ....132..161G,doi:10.1086/504637.
  4. ^abcdefZeng, Yunlin; Brandt, Timothy D.; Li, Gongjie; Dupuy, Trent J.; Li, Yiting; Brandt, G. Mirek; Farihi, Jay; Horner, Jonathan; Wittenmyer, Robert A.; Butler, R. Paul.; Tinney, Christopher G.; Carter, Bradley D.; Wright, Duncan J.; Jones, Hugh R. A.; o'Toole, Simon J. (2022)."The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at ≈2 au".The Astronomical Journal.164 (5): 188.arXiv:2112.06394.Bibcode:2022AJ....164..188Z.doi:10.3847/1538-3881/ac8ff7.S2CID 252872318.
  5. ^ab"Open Exoplanet Catalogue, Gliese 86". Archived fromthe original on 2020-07-14. Retrieved2020-07-13.
  6. ^van Leeuwen, F. (2007)."Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.Archived from the original on 2019-03-28. Retrieved2018-02-12.Vizier catalog entryArchived 2018-10-01 at theWayback Machine
  7. ^Ramírez, I.; et al. (February 2013), "Oxygen abundances in nearby FGK stars and the galactic chemical evolution of the local disk and halo",The Astrophysical Journal,764 (1): 78,arXiv:1301.1582,Bibcode:2013ApJ...764...78R,doi:10.1088/0004-637X/764/1/78.
  8. ^Holmberg, J.; et al. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics",Astronomy and Astrophysics,501 (3):941–947,arXiv:0811.3982,Bibcode:2009A&A...501..941H,doi:10.1051/0004-6361/200811191.
  9. ^abFuhrmann, K.; et al. (2014)."On the Age of Gliese 86".The Astrophysical Journal.785 (1). 68.Bibcode:2014ApJ...785...68F.doi:10.1088/0004-637X/785/1/68.
  10. ^"HD 13445".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-08-14.
  11. ^"HD 13445B".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-08-14.
  12. ^"Extrasolar Planet in Double Star System Discovered from La Silla" (Press release). Garching, Germany: European Southern Observatory. November 24, 1998.Archived from the original on May 21, 2020. RetrievedDecember 29, 2012.
  13. ^Raghavan, Deepak; et al. (2006)."Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems".The Astrophysical Journal.646 (1):523–542.arXiv:astro-ph/0603836.Bibcode:2006ApJ...646..523R.doi:10.1086/504823.
  14. ^Els, S. G.; et al. (2001)."A second substellar companion in the Gliese 86 system. A brown dwarf in an extrasolar planetary system".Astronomy and Astrophysics.370 (1):L1 –L4.Bibcode:2001A&A...370L...1E.doi:10.1051/0004-6361:20010298.Archived from the original on 2019-06-26. Retrieved2009-12-19.
  15. ^Mugrauer, M.; Neuhäuser, R. (2005)."Gl86B: a white dwarf orbits an exoplanet host star".Monthly Notices of the Royal Astronomical Society: Letters.361 (1):L15 –L19.arXiv:astro-ph/0506311.Bibcode:2005MNRAS.361L..15M.doi:10.1111/j.1745-3933.2005.00055.x.S2CID 16904466.
  16. ^Lagrange, A.-M.; et al. (2006)."New constrains on Gliese 86 B. VLT near infrared coronographic imaging survey of planetary hosts".Astronomy and Astrophysics.459 (3):955–963.Bibcode:2006A&A...459..955L.doi:10.1051/0004-6361:20054710.
  17. ^"Southern Sky extrasolar Planet search Programme".Archived from the original on 2020-07-15. Retrieved2009-02-18.
  18. ^Wittenmyer, Robert A.; et al. (2020)."Cool Jupiters greatly outnumber their toasty siblings: occurrence rates from the Anglo-Australian Planet Search".Monthly Notices of the Royal Astronomical Society.492 (1):377–383.arXiv:1912.01821.Bibcode:2020MNRAS.492..377W.doi:10.1093/mnras/stz3436.S2CID 208617606.

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