HD 178911

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HD 178911
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Lyra
Right ascension 19h 09m 04.3838s
Declination +34º 36' 01.6250″
Apparent magnitude (V) 6.74
Absolute magnitude (V) 3.29
Distance 160 ly
(49.0 pc)
Spectral type G1V
Other designations
BD+34 3439, HIP 94076, HR 7272, SAO 67879

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.

As it is typical for few metal-rich Sun-like stars, it has at least one planet in orbit around this secondary star.

[edit] HD 178911 Bb

HD 178911 Bb
Extrasolar planet List of extrasolar planets
Orbital elements
Semimajor axis (a) 0.345 AU
Eccentricity (e) 0.139±0.14
Orbital period (P) 71.511±0.011 d
Angular distance (θ) 7.04 mas
Longitude of
periastron
(ω) 172.3±5°
Time of periastron (T0) 2,451,378.23±83 JD
Semi-amplitude (K) 346.9±4.2 m/s
Physical characteristics
Mass (m) >7.35 MJ
Discovery information
Discovery date April 4, 2001
Discoverer(s) Zucker et al.
Detection method Radial velocity
Discovery status Published

HD 178911 Bb is a planet discovered in 2001 by Zucker who used radial velocity method. The minimum mass of this giant planet is 7.35 times that of Jupiter that orbits close to the star. The period of the planet is 71.5 days and the semi-amplitude is 346.9 m/s.

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