Gliese 86

Binary star system in the constellation Eridanus From Wikipedia, the free encyclopedia

Gliese 86 (13 G. Eridani, HD 13445) is a K-type main-sequence star 35 light-years away in the constellation of Eridanus. It has been confirmed that a white dwarf orbits the primary star. In 1998 the European Southern Observatory announced that an extrasolar planet was also orbiting the star.[18]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Apparent magnitude (V) ...
Gliese 86
Location of Gliese 86 (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Eridanus[1]
Gliese 86 A
Right ascension 02h 10m 25.9182s[2]
Declination −50° 49 25.465[2]
Apparent magnitude (V) 6.17[3]
Gliese 86 B
Right ascension 02h 10m 26.1144s[4]
Declination −50° 49 26.334[4]
Apparent magnitude (V) 14.0[5]
Characteristics
A
Evolutionary stage main sequence[2]
Spectral type K1V[6]
U−B color index 0.44[7]
B−V color index 0.82[7]
B
Evolutionary stage white dwarf[8]
Spectral type DQ6[9][10]
Astrometry
A
Radial velocity (Rv)+55.22±0.15[2] km/s
Proper motion (μ) RA: +2,125.416 mas/yr[2]
Dec.: +637.975 mas/yr[2]
Parallax (π)92.9251±0.0461 mas[2]
Distance35.10 ± 0.02 ly
(10.761 ± 0.005 pc)
Absolute magnitude (MV)5.95[11]
Orbit[9]
PrimaryGliese 86 A
NameGliese 86 B
Period (P)≈100 yr
Semi-major axis (a)23.7 au
Eccentricity (e)0.429
Inclination (i)126.44°
Longitude of the node (Ω)234.2°
Details
Gliese 86 A
Mass0.83±0.05[12] M
Radius0.79±0.03[12] R
Luminosity0.41[13] L
Surface gravity (log g)4.56±0.10[12] cgs
Temperature5,180±80[12] K
Metallicity [Fe/H]−0.27±0.07[12] dex
Rotation30.0 days[14]
Rotational velocity (v sin i)2.0±1.0[12] km/s
Age10±1[12] Gyr
Gliese 86 B
Mass0.5425[9] M
Surface gravity (log g)8.00[15] cgs
Temperature5,000±500[8] K
Other designations
GJ 86, WDS J02104-5049
Gliese 86A: CD−51°532, HD 13445, HIP 10138, HR 637, SAO 232658[16]
Gliese 86B: WD 0208-510[17]
Database references
SIMBADdata
B
Exoplanet Archivedata
ARICNSdata
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Stellar components

The primary companion (Gliese 86 A) is a K-type main-sequence star of spectral type K1V. The characteristics in comparison to the Sun are 83% the mass, 79% the radius, and 50% the luminosity. The star has a close-orbiting massive Jovian planet.

Gliese 86 B is a white 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.[19] It was discovered in 2001 and initially suspected to be a brown dwarf,[20] 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.[8] 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 a semimajor axis of 18.42 AU and an eccentricity of 0.3974.[21] When both stars were on the main sequence, the separation between the two stars was closer, at around 9 AU.[9] More precise measurements for the white dwarf give it a mass of 55% the mass of the Sun[9] and a temperature of around 8200 K.[12]

Planetary system

The planet Gliese 86 b was discovered by the Swiss 1.2 m Leonhard Euler Telescope operated by the Geneva Observatory.[22] Such an object was formed from a protoplanetary disk that was truncated at 2 AU from the parent star.[9]

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.

More information Companion (in order from star), Mass ...
The Gliese 86 A planetary system[23]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥6.588±0.018 MJ 0.114340±0.000001 15.76480±0.00004 0.048±0.002
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See also

References

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