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 binary 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.

Contents

[edit] Planetary system

In 2001 an extrasolar planet was discovered in orbit around the secondary star.[1]

The HD 178911 system[2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity
b >7.35 ± 0.60 MJ 0.345 ± 0.20 71.511 ± 0.011 0.139 ± 0.014

[edit] See also

[edit] References

  1. ^ Zucker et al.; Naef, D.; Latham, D. W.; Mayor, M.; Mazeh, T.; Beuzit, J. L.; Drukier, G.; Perrier‐bellet, C. et al (2002). "A Planet Candidate in the Stellar Triple System HD 178911". The Astrophysical Journal 568 (1): 363–368. arXiv:astro-ph/0111550. Bibcode 2002ApJ...568..363Z. doi:10.1086/338892. http://www.iop.org/EJ/article/0004-637X/568/1/363/54915.html. 
  2. ^ Butler et al.; Wright, J. T.; Marcy, G. W.; Fischer, D. A.; Vogt, S. S.; Tinney, C. G.; Jones, H. R. A.; Carter, B. D. et al (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode 2006ApJ...646..505B. doi:10.1086/504701. http://www.iop.org/EJ/article/0004-637X/646/1/505/64046.html. 

[edit] External links

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


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