HD 178911

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HD 178911
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
Right ascension 19h 09m 04.3838s
Declination +34° 36′ 01.625″
Apparent magnitude (V) 6.74
Distance 160 ly
(49.0 pc)
Spectral type G1V
Other designations
BD+34° 3439, HIP 94076, HR 7272, LTT 15608, SAO 67879
Database references
SIMBAD data
Extrasolar Planets
Encyclopaedia
data

HD 178911 is a triple star system in the constellation Lyra. The secondary star (designated as HD 178911 B) has an apparent magnitude of 6.74 and a spectral type of G1V, which is very similar to our Sun at a distance of 160 light years. The age of the star is slightly older and have significantly higher metallicity than our Sun.

Stellar system

The HD 178911 system consists of HD 178911A and HD 178911B in a 1300 day orbit with HD 178911B being a more distant common proper motion companion and HD 178911A is in fact a tight binary pair consisting of HD 178911Aa and Ab.[1] An additional companion HD 178911C is a chance optical alignment and is not part of the system.[2]

Planetary system

In 2001 an extrasolar planet was discovered in orbit around HD 178911B.[3][4]

The HD 178911 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >7.35 ± 0.60 MJ 0.345 ± 0.20 71.511 ± 0.011 0.139 ± 0.014

See also

References

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External links

Coordinates: Sky map 19h 09m 04.3838s, +34° 36′ 01.625″


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