HD 164922 b

HD 164922 b is an exoplanet, of the main sequence star HD 164922 orbits every 1155 days. Due to its high mass is assumed that it is a gas planet.

Discovery

As the majority of exoplanets was also discovered that using the radial velocity method. The planet was from Paul Butler et al. discovered in 2006.

Circulation and mass

The planet orbits its star at a distance of approximately 2.11 astronomical units and has a mass of about 114.4 Earth masses and 0.36 Jupiter masses.