HD 178911 Bb
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HD 178911 Bb is a planet discovered in 2001 by Zucker who used the
radial velocity The radial velocity or line-of-sight velocity, also known as radial speed or range rate, of a target with respect to an observer is the temporal rate of change, rate of change of the distance or Slant range, range between the two points. It is e ...
method. The minimum mass of this giant planet is 7.35 times that of
Jupiter Jupiter is the fifth planet from the Sun and the List of Solar System objects by size, largest in the Solar System. It is a gas giant with a mass more than two and a half times that of all the other planets in the Solar System combined, but ...
that orbits close to the star. The period of the planet is 71.5 days and the semi-
amplitude The amplitude of a periodic variable is a measure of its change in a single period (such as time or spatial period). The amplitude of a non-periodic signal is its magnitude compared with a reference value. There are various definitions of amplit ...
is 346.9 m/s.


References


External links

* Exoplanets discovered in 2001 Giant planets Lyra Exoplanets detected by radial velocity {{extrasolar-planet-stub de:HD 178911 B b