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Gliese 86 b

Coordinates:Sky map02h 10m 14s, −50° 50′ 00″
From Wikipedia, the free encyclopedia
Jovian planet orbiting Gliese 86 A
Gliese 86 b
The exoplanet Gliese 86 Ab (min mass ~4 MJ) rendered by Celestia
Discovery
Discovered byMayoret al.[1]
Discovery siteFrance
Discovery date24 November 1998[2]
Doppler spectroscopy
Orbital characteristics
0.1177+0.0015
−0.0012
 AU
[3]
Eccentricity0.0478±0.0024[3]
15.76491 ± 0.00039[4]d
2451903.36 ± 0.59[4]
269 ± 16[4]
Semi-amplitude376.7 ± 2.9[4]
StarGliese 86
Physical characteristics
Mass4.266+0.11
−0.087
 MJ
[3]

Gliese 86 b, sometimes referred to asGliese 86 A b[3] (so as to distinguish the planet from companion star "B") and/or shortened toGl 86 b, is anextrasolar planet approximately 35light-years away in theconstellation ofEridanus. The planet was discovered orbiting aK-type main-sequence star (Gliese 86 A) byFrench scientists in November 1998.[2] The planet orbits very close to the star, completing an orbit in 15.78days.

Preliminaryastrometric measurements made with theHipparcos space probe suggested the planet has an orbitalinclination of 164.0° and amass 15 times that ofJupiter, which would make the object abrown dwarf.[5] However, further analysis suggests the Hipparcos measurements are not precise enough to reliably determine astrometric orbits of substellar companions, thus the orbital inclination andtrue mass of the candidate planet remain unknown.[6]

See also

[edit]

References

[edit]
  1. ^Michel Mayor,Didier Queloz,Udryet al.
  2. ^ab"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.
  3. ^abcdZeng, Yunlin; Brandt, Timothy D.; Li, Gongjie; Dupuy, Trent J.; Li, Yiting; Mirek Brandt, G.; 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 245123923.
  4. ^abcdButler, R.; et al. (2007)."Planets Table".Catalog of Nearby Exoplanets.Archived from the original on 2019-03-05. Retrieved2007-08-02.
  5. ^Han; Black, David C.; Gatewood, George (2001)."Preliminary astrometric masses for proposed extrasolar planetary companions".The Astrophysical Journal Letters.548 (1):L57–L60.Bibcode:2001ApJ...548L..57H.doi:10.1086/318927.
  6. ^Pourbaix, D.; Arenou, F. (2001). "Screening the Hipparcos-based astrometric orbits of sub-stellar objects".Astronomy and Astrophysics.372 (3):935–944.arXiv:astro-ph/0104412.Bibcode:2001A&A...372..935P.doi:10.1051/0004-6361:20010597.S2CID 378792.

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