HD 102195 b

HD 102195 b is an exoplanet, of the main sequence star HD 102195 orbits every 4.121 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 of Jian Ge et al. discovered in 2006.

Circulation and mass

The planet orbits its star at a distance of about 0.0491 astronomical units and has a mass of about 156.4 Earth masses and 0.492 Jupiter masses.